Sample records for ice volume variability

  1. Variability of the volume and thickness of sea ice in the Bay of Bothnia

    NASA Astrophysics Data System (ADS)

    Ronkainen, Iina; Lehtiranta, Jonni; Lensu, Mikko; Rinne, Eero; Hordoir, Robinson; Haapala, Jari

    2017-04-01

    Variability of the volume and thickness of sea ice in the Bay of Bothnia In our study, we want to quantify the variability of sea ice volume and thickness in the Bay of Bothnia and to introduce the drivers of the observed variability. There has been similar studies, but only for fast ice. We use various different data sets: in-situ ice thickness data, remote sensing data, model data and ice charts. In-situ data is from the regular monitoring stations in the coastal fast ice zone and from field campaigns. The remote sensing data is helicopter-borne and ship-borne electromagnetic data. The models we use are HELMI and NEMO-Nordic. We analyze the different data sets and compare them to each other to solve the inter-annual variability and to discuss the ratio of level and deformed ice.

  2. Satellite Observations of Antarctic Sea Ice Thickness and Volume

    NASA Technical Reports Server (NTRS)

    Kurtz, Nathan; Markus, Thorsten

    2012-01-01

    We utilize satellite laser altimetry data from ICESat combined with passive microwave measurements to analyze basin-wide changes in Antarctic sea ice thickness and volume over a 5 year period from 2003-2008. Sea ice thickness exhibits a small negative trend while area increases in the summer and fall balanced losses in thickness leading to small overall volume changes. Using a five year time-series, we show that only small ice thickness changes of less than -0.03 m/yr and volume changes of -266 cu km/yr and 160 cu km/yr occurred for the spring and summer periods, respectively. The calculated thickness and volume trends are small compared to the observational time period and interannual variability which masks the determination of long-term trend or cyclical variability in the sea ice cover. These results are in stark contrast to the much greater observed losses in Arctic sea ice volume and illustrate the different hemispheric changes of the polar sea ice covers in recent years.

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

    NASA Astrophysics Data System (ADS)

    Heimbach, P.; Bugnion, V.

    2009-04-01

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

  4. The Response of Ice Sheets to Climate Variability

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

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

  5. A glimpse beneath Antarctic sea ice: observation of platelet-layer thickness and ice-volume fraction with multifrequency EM

    NASA Astrophysics Data System (ADS)

    Hoppmann, Mario; Hunkeler, Priska A.; Hendricks, Stefan; Kalscheuer, Thomas; Gerdes, Rüdiger

    2016-04-01

    In Antarctica, ice crystals (platelets) form and grow in supercooled waters below ice shelves. These platelets rise, accumulate beneath nearby sea ice, and subsequently form a several meter thick, porous sub-ice platelet layer. This special ice type is a unique habitat, influences sea-ice mass and energy balance, and its volume can be interpreted as an indicator of the health of an ice shelf. Although progress has been made in determining and understanding its spatio-temporal variability based on point measurements, an investigation of this phenomenon on a larger scale remains a challenge due to logistical constraints and a lack of suitable methodology. In the present study, we applied a lateral constrained Marquardt-Levenberg inversion to a unique multi-frequency electromagnetic (EM) induction sounding dataset obtained on the ice-shelf influenced fast-ice regime of Atka Bay, eastern Weddell Sea. We adapted the inversion algorithm to incorporate a sensor specific signal bias, and confirmed the reliability of the algorithm by performing a sensitivity study using synthetic data. We inverted the field data for sea-ice and platelet-layer thickness and electrical conductivity, and calculated ice-volume fractions within the platelet layer using Archie's Law. The thickness results agreed well with drillhole validation datasets within the uncertainty range, and the ice-volume fraction yielded results comparable to other studies. Both parameters together enable an estimation of the total ice volume within the platelet layer, which was found to be comparable to the volume of landfast sea ice in this region, and corresponded to more than a quarter of the annual basal melt volume of the nearby Ekström Ice Shelf. Our findings show that multi-frequency EM induction sounding is a suitable approach to efficiently map sea-ice and platelet-layer properties, with important implications for research into ocean/ice-shelf/sea-ice interactions. However, a successful application of this

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

    USGS Publications Warehouse

    Trabant, Dennis C.

    1999-01-01

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

  7. Bayesian prediction of future ice sheet volume using local approximation Markov chain Monte Carlo methods

    NASA Astrophysics Data System (ADS)

    Davis, A. D.; Heimbach, P.; Marzouk, Y.

    2017-12-01

    We develop a Bayesian inverse modeling framework for predicting future ice sheet volume with associated formal uncertainty estimates. Marine ice sheets are drained by fast-flowing ice streams, which we simulate using a flowline model. Flowline models depend on geometric parameters (e.g., basal topography), parameterized physical processes (e.g., calving laws and basal sliding), and climate parameters (e.g., surface mass balance), most of which are unknown or uncertain. Given observations of ice surface velocity and thickness, we define a Bayesian posterior distribution over static parameters, such as basal topography. We also define a parameterized distribution over variable parameters, such as future surface mass balance, which we assume are not informed by the data. Hyperparameters are used to represent climate change scenarios, and sampling their distributions mimics internal variation. For example, a warming climate corresponds to increasing mean surface mass balance but an individual sample may have periods of increasing or decreasing surface mass balance. We characterize the predictive distribution of ice volume by evaluating the flowline model given samples from the posterior distribution and the distribution over variable parameters. Finally, we determine the effect of climate change on future ice sheet volume by investigating how changing the hyperparameters affects the predictive distribution. We use state-of-the-art Bayesian computation to address computational feasibility. Characterizing the posterior distribution (using Markov chain Monte Carlo), sampling the full range of variable parameters and evaluating the predictive model is prohibitively expensive. Furthermore, the required resolution of the inferred basal topography may be very high, which is often challenging for sampling methods. Instead, we leverage regularity in the predictive distribution to build a computationally cheaper surrogate over the low dimensional quantity of interest (future ice

  8. Arctic Sea Ice Basal Melt Onset Variability and Associated Ocean Surface Heating

    NASA Astrophysics Data System (ADS)

    Merrick, R. A.; Hutchings, J. K.

    2015-12-01

    The interannual and regional variability in Arctic sea ice melt has previously been characterized only in terms of surface melting. A focus on the variability in the onset of basal melt is additionally required to understand Arctic melt patterns. Monitoring basal melt provides a glimpse into the importance of ocean heating to sea ice melt. This warming is predominantly through seawater exposure due to lead opening and the associated solar warming at the ocean's surface. We present the temporal variability in basal melt onset observed by ice mass balance buoys throughout the Arctic Ocean since 2003, providing a different perspective than the satellite microwave data used to measure the onset of surface melt. We found that melt onset varies greatly, even for buoys deployed within 100km of each other. Therefore large volumes of data are necessary to accurately estimate the variability of basal melt onset. Once the variability of basal melt onset has been identified, we can investigate how this range has been changing as a response to atmospheric and oceanic warming, changes in ice morphology as well as the intensification of the ice albedo feedback.

  9. A glimpse beneath Antarctic sea ice: observation of platelet-layer thickness and ice-volume fraction with multi-frequency EM

    NASA Astrophysics Data System (ADS)

    Hendricks, S.; Hoppmann, M.; Hunkeler, P. A.; Kalscheuer, T.; Gerdes, R.

    2015-12-01

    In Antarctica, ice crystals (platelets) form and grow in supercooled waters below ice shelves. These platelets rise and accumulate beneath nearby sea ice to form a several meter thick sub-ice platelet layer. This special ice type is a unique habitat, influences sea-ice mass and energy balance, and its volume can be interpreted as an indicator for ice - ocean interactions. Although progress has been made in determining and understanding its spatio-temporal variability based on point measurements, an investigation of this phenomenon on a larger scale remains a challenge due to logistical constraints and a lack of suitable methodology. In the present study, we applied a lateral constrained Marquardt-Levenberg inversion to a unique multi-frequency electromagnetic (EM) induction sounding dataset obtained on the ice-shelf influenced fast-ice regime of Atka Bay, eastern Weddell Sea. We adapted the inversion algorithm to incorporate a sensor specific signal bias, and confirmed the reliability of the algorithm by performing a sensitivity study using synthetic data. We inverted the field data for sea-ice and sub-ice platelet-layer thickness and electrical conductivity, and calculated ice-volume fractions from platelet-layer conductivities using Archie's Law. The thickness results agreed well with drill-hole validation datasets within the uncertainty range, and the ice-volume fraction also yielded plausible results. Our findings imply that multi-frequency EM induction sounding is a suitable approach to efficiently map sea-ice and platelet-layer properties. However, we emphasize that the successful application of this technique requires a break with traditional EM sensor calibration strategies due to the need of absolute calibration with respect to a physical forward model.

  10. Variability of Fram Strait Ice Flux and North Atlantic Oscillation

    NASA Technical Reports Server (NTRS)

    Kwok, Ron

    1999-01-01

    An important term in the mass balance of the Arctic Ocean sea ice is the ice export. We estimated the winter sea ice export through the Fram Strait using ice motion from satellite passive microwave data and ice thickness data from moored upward looking sonars. The average winter area flux over the 18-year record (1978-1996) is 670,000 square km, approximately 7% of the area of the Arctic Ocean. The winter area flux ranges from a minimum of 450,000 sq. km in 1984 to a maximum of 906,000 sq km in 1995. The daily, monthly and interannual variabilities of the ice area flux are high. There is an upward trend in the ice area flux over the 18-year record. The average winter volume flux over the winters of October 1990 through May 1995 is 1745 cubic km ranging from a low of 1375 cubic km in 1990 to a high of 2791 cubic km in 1994. The sea-level pressure gradient across the Fram Strait explains more than 80% of the variance in the ice flux over the 18-year record. We use the coefficients from the regression of the time-series of area flux versus pressure gradient across the Fram Strait and ice thickness data to estimate the summer area and volume flux. The average 12-month area flux and volume flux are 919,000 sq km and 2366 cubic km. We find a significant correlation (R =0.86) between the area flux and positive phases of the North Atlantic Oscillation (NAO) index over the months of December through March. Correlation between our six years of volume flux estimates and the NAO index gives R =0.56. During the high NAO years, a more intense Icelandic low increases the gradient in the sea-level pressure by almost 1 mbar across the Fram Strait thus increasing the atmospheric forcing on ice transport. Correlation is reduced during the negative NAO years because of decreased dominance of this large-scale atmospheric pattern on the sea-level pressure gradient across the Fram Strait. Additional information is contained in the original.

  11. Replicating the Ice-Volume Signal of the Early Pleistocene with a Complex Earth System Model

    NASA Astrophysics Data System (ADS)

    Tabor, C. R.; Poulsen, C. J.; Pollard, D.

    2013-12-01

    Milankovitch theory proposes high-latitude summer insolation intensity paces the ice ages by controlling perennial snow cover amounts (Milankovitch, 1941). According to theory, the ~21 kyr cycle of precession should dominate the ice-volume records since it has the greatest influence on high-latitude summer insolation. Modeling experiments frequently support Milankovitch theory by attributing the majority of Northern Hemisphere high-latitude summer snowmelt to changes in the cycle of precession (e.g. Jackson and Broccoli, 2003). However, ice-volume proxy records, especially those of the Early Pleistocene (2.6-0.8 Ma), display variability with a period of ~41 kyr (Raymo and Lisiecki, 2005), indicative of insolation forcing from obliquity, which has a much smaller influence on summer insolation intensity than precession. Several hypotheses attempt to explain the discrepancies between Milkankovitch theory and the proxy records by invoking phenomena such as insolation gradients (Raymo and Nisancioglu, 2003), hemispheric offset (Raymo et al., 2006; Lee and Poulsen, 2009), and integrated summer energy (Huybers, 2006); however, all of these hypotheses contain caveats (Ruddiman, 2006) and have yet to be supported by modeling studies that use a complex GCM. To explore potential solutions to this '41 kyr problem,' we use an Earth system model composed of the GENESIS GCM and Land Surface model, the BIOME4 vegetation model, and the Pennsylvania State ice-sheet model. Using an asynchronous coupling technique, we run four idealized transient combinations of obliquity and precession, representing the orbital extremes of the Pleistocene (Berger and Loutre, 1991). Each experiment is run through several complete orbital cycles with a dynamic ice domain spanning North America and Greenland, and fixed preindustrial greenhouse-gas concentrations. For all orbital configurations, model results produce greater ice-volume spectral power at the frequency of obliquity despite significantly

  12. Ice-Sheet Dynamics and Millennial-Scale Climate Variability in the North Atlantic across the Middle Pleistocene Transition (Invited)

    NASA Astrophysics Data System (ADS)

    Hodell, D. A.; Nicholl, J.

    2013-12-01

    During the Middle Pleistocene Transition (MPT), the climate system evolved from a more linear response to insolation forcing in the '41-kyr world' to one that was decidedly non-linear in the '100-kyr world'. Smaller ice sheets in the early Pleistocene gave way to larger ice sheets in the late Pleistocene with an accompanying change in ice sheet dynamics. We studied Sites U1308 (49° 52.7'N, 24° 14.3'W; 3871 m) and U1304 (53° 3.4'N, 33° 31.8'W; 3024 m) in the North Atlantic to determine how ice sheet dynamics and millennial-scale climate variability evolved as glacial boundary conditions changed across the MPT. The frequency of ice-rafted detritus (IRD) in the North Atlantic was greater during glacial stages prior to 650 ka (MIS 16), reflecting more frequent crossing of an ice volume threshold when the climate system spent more time in the 'intermediate ice volume' window, resulting in persistent millennial scale variability. The rarity of Heinrich Events containing detrital carbonate and more frequent occurrence of IRD events prior to 650 ka may indicate the presence of 'low-slung, slippery ice sheets' that flowed more readily than their post-MPT counterparts (Bailey et al., 2010). Ice volume surpassed a critical threshold across the MPT that permitted ice sheets to survive boreal summer insolation maxima, thereby increasing ice volume and thickness, lengthening glacial cycles, and activating the dynamical processes responsible for Laurentide Ice Sheet instability in the region of Hudson Strait (i.e., Heinrich events). The excess ice volume during post-MPT glacial maxima provided a large, unstable reservoir of freshwater to be released to the North Atlantic during glacial terminations with the potential to perturb Atlantic Meridional Overtunring Circulation. We speculate that orbital- and millennial-scale variability co-evolved across the MPT and the interaction of processes on orbital and suborbital time scales gave rise to the changing patterns of glacial

  13. Predicting uncertainty in future marine ice sheet volume using Bayesian statistical methods

    NASA Astrophysics Data System (ADS)

    Davis, A. D.

    2015-12-01

    The marine ice instability can trigger rapid retreat of marine ice streams. Recent observations suggest that marine ice systems in West Antarctica have begun retreating. However, unknown ice dynamics, computationally intensive mathematical models, and uncertain parameters in these models make predicting retreat rate and ice volume difficult. In this work, we fuse current observational data with ice stream/shelf models to develop probabilistic predictions of future grounded ice sheet volume. Given observational data (e.g., thickness, surface elevation, and velocity) and a forward model that relates uncertain parameters (e.g., basal friction and basal topography) to these observations, we use a Bayesian framework to define a posterior distribution over the parameters. A stochastic predictive model then propagates uncertainties in these parameters to uncertainty in a particular quantity of interest (QoI)---here, the volume of grounded ice at a specified future time. While the Bayesian approach can in principle characterize the posterior predictive distribution of the QoI, the computational cost of both the forward and predictive models makes this effort prohibitively expensive. To tackle this challenge, we introduce a new Markov chain Monte Carlo method that constructs convergent approximations of the QoI target density in an online fashion, yielding accurate characterizations of future ice sheet volume at significantly reduced computational cost.Our second goal is to attribute uncertainty in these Bayesian predictions to uncertainties in particular parameters. Doing so can help target data collection, for the purpose of constraining the parameters that contribute most strongly to uncertainty in the future volume of grounded ice. For instance, smaller uncertainties in parameters to which the QoI is highly sensitive may account for more variability in the prediction than larger uncertainties in parameters to which the QoI is less sensitive. We use global sensitivity

  14. Variability and Trends in Sea Ice Extent and Ice Production in the Ross Sea

    NASA Technical Reports Server (NTRS)

    Comiso, Josefino; Kwok, Ronald; Martin, Seelye; Gordon, Arnold L.

    2011-01-01

    Salt release during sea ice formation in the Ross Sea coastal regions is regarded as a primary forcing for the regional generation of Antarctic Bottom Water. Passive microwave data from November 1978 through 2008 are used to examine the detailed seasonal and interannual characteristics of the sea ice cover of the Ross Sea and the adjacent Bellingshausen and Amundsen seas. For this period the sea ice extent in the Ross Sea shows the greatest increase of all the Antarctic seas. Variability in the ice cover in these regions is linked to changes in the Southern Annular Mode and secondarily to the Antarctic Circumpolar Wave. Over the Ross Sea shelf, analysis of sea ice drift data from 1992 to 2008 yields a positive rate of increase in the net ice export of about 30,000 sq km/yr. For a characteristic ice thickness of 0.6 m, this yields a volume transport of about 20 cu km/yr, which is almost identical, within error bars, to our estimate of the trend in ice production. The increase in brine rejection in the Ross Shelf Polynya associated with the estimated increase with the ice production, however, is not consistent with the reported Ross Sea salinity decrease. The locally generated sea ice enhancement of Ross Sea salinity may be offset by an increase of relatively low salinity of the water advected into the region from the Amundsen Sea, a consequence of increased precipitation and regional glacial ice melt.

  15. Ice thickness measurements and volume estimates for glaciers in Norway

    NASA Astrophysics Data System (ADS)

    Andreassen, Liss M.; Huss, Matthias; Melvold, Kjetil; Elvehøy, Hallgeir; Winsvold, Solveig H.

    2014-05-01

    Whereas glacier areas in many mountain regions around the world now are well surveyed using optical satellite sensors and available in digital inventories, measurements of ice thickness are sparse in comparison and a global dataset does not exist. Since the 1980s ice thickness measurements have been carried out by ground penetrating radar on many glaciers in Norway, often as part of contract work for hydropower companies with the aim to calculate hydrological divides of ice caps. Measurements have been conducted on numerous glaciers, covering the largest ice caps as well as a few smaller mountain glaciers. However, so far no ice volume estimate for Norway has been derived from these measurements. Here, we give an overview of ice thickness measurements in Norway, and use a distributed model to interpolate and extrapolate the data to provide an ice volume estimate of all glaciers in Norway. We also compare the results to various volume-area/thickness-scaling approaches using values from the literature as well as scaling constants we obtained from ice thickness measurements in Norway. Glacier outlines from a Landsat-derived inventory from 1999-2006 together with a national digital elevation model were used as input data for the ice volume calculations. The inventory covers all glaciers in mainland Norway and consists of 2534 glaciers (3143 glacier units) covering an area of 2692 km2 ± 81 km2. To calculate the ice thickness distribution of glaciers in Norway we used a distributed model which estimates surface mass balance distribution, calculates the volumetric balance flux and converts it into thickness using the flow law for ice. We calibrated this model with ice thickness data for Norway, mainly by adjusting the mass balance gradient. Model results generally agree well with the measured values, however, larger deviations were found for some glaciers. The total ice volume of Norway was estimated to be 275 km3 ± 30 km3. From the ice thickness data set we selected

  16. A regional-scale estimation of ice wedge ice volumes in the Canadian High Arctic

    NASA Astrophysics Data System (ADS)

    Templeton, M.; Pollard, W. H.; Grand'Maison, C. B.

    2016-12-01

    Ice 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 ice wedge melt out has become an immediate issue, receiving much attention in the permafrost literature. In this study we estimate the volume of ice wedge ice 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 ice wedge polygons from satellite imagery using ArcGIS. The average width and depth of these ice 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 ice wedge volume have been tested, including trough width being representative of ice wedge width, and ice wedge ice content (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 ice 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 ice wedges where it could be argued that they are a key driver of thermokarst terrain. The ubiquitous nature of ice wedges across arctic terrain highlights the importance and the need to improve our understanding of ice wedge dynamics, as subsidence from ice wedge melt-out could lead to large scale landscape change.

  17. Influence of temperature fluctuations on equilibrium
    ice sheet volume

    NASA Astrophysics Data System (ADS)

    Bøgeholm Mikkelsen, Troels; Grinsted, Aslak; Ditlevsen, Peter

    2018-01-01

    Forecasting the future sea level relies on accurate modeling of the response of the Greenland and Antarctic ice sheets to changing temperatures. The surface mass balance (SMB) of the Greenland Ice Sheet (GrIS) has a nonlinear response to warming. Cold and warm anomalies of equal size do not cancel out and it is therefore important to consider the effect of interannual fluctuations in temperature. We find that the steady-state volume of an ice sheet is biased toward larger size if interannual temperature fluctuations are not taken into account in numerical modeling of the ice sheet. We illustrate this in a simple ice sheet model and find that the equilibrium ice volume is approximately 1 m SLE (meters sea level equivalent) smaller when the simple model is forced with fluctuating temperatures as opposed to a stable climate. It is therefore important to consider the effect of interannual temperature fluctuations when designing long experiments such as paleo-spin-ups. We show how the magnitude of the potential bias can be quantified statistically. For recent simulations of the Greenland Ice Sheet, we estimate the bias to be 30 Gt yr-1 (24-59 Gt yr-1, 95 % credibility) for a warming of 3 °C above preindustrial values, or 13 % (10-25, 95 % credibility) of the present-day rate of ice loss. Models of the Greenland Ice Sheet show a collapse threshold beyond which the ice sheet becomes unsustainable. The proximity of the threshold will be underestimated if temperature fluctuations are not taken into account. We estimate the bias to be 0.12 °C (0.10-0.18 °C, 95 % credibility) for a recent estimate of the threshold. In light of our findings it is important to gauge the extent to which this increased variability will influence the mass balance of the ice sheets.

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

    PubMed

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

    2016-02-18

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

  19. Arctic sea ice trends, variability and implications for seasonal ice forecasting

    PubMed Central

    Serreze, Mark C.; Stroeve, Julienne

    2015-01-01

    September Arctic sea ice extent over the period of satellite observations has a strong downward trend, accompanied by pronounced interannual variability with a detrended 1 year lag autocorrelation of essentially zero. We argue that through a combination of thinning and associated processes related to a warming climate (a stronger albedo feedback, a longer melt season, the lack of especially cold winters) the downward trend itself is steepening. The lack of autocorrelation manifests both the inherent large variability in summer atmospheric circulation patterns and that oceanic heat loss in winter acts as a negative (stabilizing) feedback, albeit insufficient to counter the steepening trend. These findings have implications for seasonal ice forecasting. In particular, while advances in observing sea ice thickness and assimilating thickness into coupled forecast systems have improved forecast skill, there remains an inherent limit to predictability owing to the largely chaotic nature of atmospheric variability. PMID:26032315

  20. Variability of Antarctic Sea Ice 1979-1998

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay; Comiso, Josefino C.; Parkinson, Claire L.; Cavalieri, Donald J.; Gloersen, Per; Koblinsky, Chester J. (Technical Monitor)

    2001-01-01

    The principal characteristics of the variability of Antarctic sea ice cover as previously described from satellite passive-microwave observations are also evident in a systematically-calibrated and analyzed data set for 20.2 years (1979-1998). The total Antarctic sea ice extent (concentration > 15 %) increased by 13,440 +/- 4180 sq km/year (+1.18 +/- 0.37%/decade). The area of sea ice within the extent boundary increased by 16,960 +/- 3,840 sq km/year (+1.96 +/- 0.44%/decade). Regionally, the trends in extent are positive in the Weddell Sea (1.5 +/- 0.9%/decade), Pacific Ocean (2.4 +/- 1.4%/decade), and Ross (6.9 +/- 1.1 %/decade) sectors, slightly negative in the Indian Ocean (-1.5 +/- 1.8%/decade, and strongly negative in the Bellingshausen-Amundsen Seas sector (-9.5 +/- 1.5%/decade). For the entire ice pack, small ice increases occur in all seasons with the largest increase during autumn. On a regional basis, the trends differ season to season. During summer and fall, the trends are positive or near zero in all sectors except the Bellingshausen-Amundsen Seas sector. During winter and spring, the trends are negative or near zero in all sectors except the Ross Sea, which has positive trends in all seasons. Components of interannual variability with periods of about 3 to 5 years are regionally large, but tend to counterbalance each other in the total ice pack. The interannual variability of the annual mean sea-ice extent is only 1.6% overall, compared to 5% to 9% in each of five regional sectors. Analysis of the relation between regional sea ice extents and spatially-averaged surface temperatures over the ice pack gives an overall sensitivity between winter ice cover and temperature of -0.7% change in sea ice extent per K. For summer, some regional ice extents vary positively with temperature and others negatively. The observed increase in Antarctic sea ice cover is counter to the observed decreases in the Arctic. It is also qualitatively consistent with the

  1. Controls on Arctic sea ice from first-year and multi-year ice survival rates

    NASA Astrophysics Data System (ADS)

    Armour, K.; Bitz, C. M.; Hunke, E. C.; Thompson, L.

    2009-12-01

    The recent decrease in Arctic sea ice cover has transpired with a significant loss of multi-year (MY) ice. The transition to an Arctic that is populated by thinner first-year (FY) sea ice has important implications for future trends in area and volume. We develop a reduced model for Arctic sea ice with which we investigate how the survivability of FY and MY ice control various aspects of the sea-ice system. We demonstrate that Arctic sea-ice area and volume behave approximately as first-order autoregressive processes, which allows for a simple interpretation of September sea-ice in which its mean state, variability, and sensitivity to climate forcing can be described naturally in terms of the average survival rates of FY and MY ice. This model, used in concert with a sea-ice simulation that traces FY and MY ice areas to estimate the survival rates, reveals that small trends in the ice survival rates explain the decline in total Arctic ice area, and the relatively larger loss of MY ice area, over the period 1979-2006. Additionally, our model allows for a calculation of the persistence time scales of September area and volume anomalies. A relatively short memory time scale for ice area (~ 1 year) implies that Arctic ice area is nearly in equilibrium with long-term climate forcing at all times, and therefore observed trends in area are a clear indication of a changing climate. A longer memory time scale for ice volume (~ 5 years) suggests that volume can be out of equilibrium with climate forcing for long periods of time, and therefore trends in ice volume are difficult to distinguish from its natural variability. With our reduced model, we demonstrate the connection between memory time scale and sensitivity to climate forcing, and discuss the implications that a changing memory time scale has on the trajectory of ice area and volume in a warming climate. Our findings indicate that it is unlikely that a “tipping point” in September ice area and volume will be

  2. Arctic sea ice trends, variability and implications for seasonal ice forecasting.

    PubMed

    Serreze, Mark C; Stroeve, Julienne

    2015-07-13

    September Arctic sea ice extent over the period of satellite observations has a strong downward trend, accompanied by pronounced interannual variability with a detrended 1 year lag autocorrelation of essentially zero. We argue that through a combination of thinning and associated processes related to a warming climate (a stronger albedo feedback, a longer melt season, the lack of especially cold winters) the downward trend itself is steepening. The lack of autocorrelation manifests both the inherent large variability in summer atmospheric circulation patterns and that oceanic heat loss in winter acts as a negative (stabilizing) feedback, albeit insufficient to counter the steepening trend. These findings have implications for seasonal ice forecasting. In particular, while advances in observing sea ice thickness and assimilating thickness into coupled forecast systems have improved forecast skill, there remains an inherent limit to predictability owing to the largely chaotic nature of atmospheric variability. © 2015 The Author(s) Published by the Royal Society. All rights reserved.

  3. Variability of Arctic Sea Ice as Determined from Satellite Observations

    NASA Technical Reports Server (NTRS)

    Parkinson, Claire L.

    1999-01-01

    The compiled, quality-controlled satellite multichannel passive-microwave record of polar sea ice now spans over 18 years, from November 1978 through December 1996, and is revealing considerable information about the Arctic sea ice cover and its variability. The information includes data on ice concentrations (percent areal coverages of ice), ice extents, ice melt, ice velocities, the seasonal cycle of the ice, the interannual variability of the ice, the frequency of ice coverage, and the length of the sea ice season. The data reveal marked regional and interannual variabilities, as well as some statistically significant trends. For the north polar ice cover as a whole, maximum ice extents varied over a range of 14,700,000 - 15,900,000 sq km, while individual regions experienced much greater percent variations, for instance, with the Greenland Sea having a range of 740,000 - 1,110,000 sq km in its yearly maximum ice coverage. In spite of the large variations from year to year and region to region, overall the Arctic ice extents showed a statistically significant, 2.80% / decade negative trend over the 18.2-year period. Ice season lengths, which vary from only a few weeks near the ice margins to the full year in the large region of perennial ice coverage, also experienced interannual variability, along with spatially coherent overall trends. Linear least squares trends show the sea ice season to have lengthened in much of the Bering Sea, Baffin Bay, the Davis Strait, and the Labrador Sea, but to have shortened over a much larger area, including the Sea of Okhotsk, the Greenland Sea, the Barents Sea, and the southeastern Arctic.

  4. Trends in Arctic Sea Ice Volume 2010-2013 from CryoSat-2

    NASA Astrophysics Data System (ADS)

    Tilling, R.; Ridout, A.; Wingham, D.; Shepherd, A.; Haas, C.; Farrell, S. L.; Schweiger, A. J.; Zhang, J.; Giles, K.; Laxon, S.

    2013-12-01

    Satellite records show a decline in Arctic sea ice extent over the past three decades with a record minimum in September 2012, and results from the Pan-Arctic Ice-Ocean Modelling and Assimilation System (PIOMAS) suggest that this has been accompanied by a reduction in volume. We use three years of measurements recorded by the European Space Agency CryoSat-2 (CS-2) mission, validated with in situ data, to generate estimates of seasonal variations and inter-annual trends in Arctic sea ice volume between 2010 and 2013. The CS-2 estimates of sea ice thickness agree with in situ estimates derived from upward looking sonar measurements of ice draught and airborne measurements of ice thickness and freeboard to within 0.1 metres. Prior to the record minimum in summer 2012, autumn and winter Arctic sea ice volume had fallen by ~1300 km3 relative to the previous year. Using the full 3-year period of CS-2 observations, we estimate that winter Arctic sea ice volume has decreased by ~700 km3/yr since 2010, approximately twice the average rate since 1980 as predicted by the PIOMAS.

  5. Mapping and Assessing Variability in the Antarctic Marginal Ice Zone, the Pack Ice and Coastal Polynyas

    NASA Astrophysics Data System (ADS)

    Stroeve, Julienne; Jenouvrier, Stephanie

    2016-04-01

    Sea ice variability within the marginal ice zone (MIZ) and polynyas plays an important role for phytoplankton productivity and krill abundance. Therefore mapping their spatial extent, seasonal and interannual variability is essential for understanding how current and future changes in these biological active regions may impact the Antarctic marine ecosystem. Knowledge of the distribution of different ice types to the total Antarctic sea ice cover may also help to shed light on the factors contributing towards recent expansion of the Antarctic ice cover in some regions and contraction in others. The long-term passive microwave satellite data record provides the longest and most consistent data record for assessing different ice types. However, estimates of the amount of MIZ, consolidated pack ice and polynyas depends strongly on what sea ice algorithm is used. This study uses two popular passive microwave sea ice algorithms, the NASA Team and Bootstrap to evaluate the distribution and variability in the MIZ, the consolidated pack ice and coastal polynyas. Results reveal the NASA Team algorithm has on average twice the MIZ and half the consolidated pack ice area as the Bootstrap algorithm. Polynya area is also larger in the NASA Team algorithm, and the timing of maximum polynya area may differ by as much as 5 months between algorithms. These differences lead to different relationships between sea ice characteristics and biological processes, as illustrated here with the breeding success of an Antarctic seabird.

  6. Validation of sea ice models using an uncertainty-based distance metric for multiple model variables: NEW METRIC FOR SEA ICE MODEL VALIDATION

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

    Urrego-Blanco, Jorge R.; Hunke, Elizabeth C.; Urban, Nathan M.

    Here, we implement a variance-based distance metric (D n) to objectively assess skill of sea ice models when multiple output variables or uncertainties in both model predictions and observations need to be considered. The metric compares observations and model data pairs on common spatial and temporal grids improving upon highly aggregated metrics (e.g., total sea ice extent or volume) by capturing the spatial character of model skill. The D n metric is a gamma-distributed statistic that is more general than the χ 2 statistic commonly used to assess model fit, which requires the assumption that the model is unbiased andmore » can only incorporate observational error in the analysis. The D n statistic does not assume that the model is unbiased, and allows the incorporation of multiple observational data sets for the same variable and simultaneously for different variables, along with different types of variances that can characterize uncertainties in both observations and the model. This approach represents a step to establish a systematic framework for probabilistic validation of sea ice models. The methodology is also useful for model tuning by using the D n metric as a cost function and incorporating model parametric uncertainty as part of a scheme to optimize model functionality. We apply this approach to evaluate different configurations of the standalone Los Alamos sea ice model (CICE) encompassing the parametric uncertainty in the model, and to find new sets of model configurations that produce better agreement than previous configurations between model and observational estimates of sea ice concentration and thickness.« less

  7. Validation of sea ice models using an uncertainty-based distance metric for multiple model variables: NEW METRIC FOR SEA ICE MODEL VALIDATION

    DOE PAGES

    Urrego-Blanco, Jorge R.; Hunke, Elizabeth C.; Urban, Nathan M.; ...

    2017-04-01

    Here, we implement a variance-based distance metric (D n) to objectively assess skill of sea ice models when multiple output variables or uncertainties in both model predictions and observations need to be considered. The metric compares observations and model data pairs on common spatial and temporal grids improving upon highly aggregated metrics (e.g., total sea ice extent or volume) by capturing the spatial character of model skill. The D n metric is a gamma-distributed statistic that is more general than the χ 2 statistic commonly used to assess model fit, which requires the assumption that the model is unbiased andmore » can only incorporate observational error in the analysis. The D n statistic does not assume that the model is unbiased, and allows the incorporation of multiple observational data sets for the same variable and simultaneously for different variables, along with different types of variances that can characterize uncertainties in both observations and the model. This approach represents a step to establish a systematic framework for probabilistic validation of sea ice models. The methodology is also useful for model tuning by using the D n metric as a cost function and incorporating model parametric uncertainty as part of a scheme to optimize model functionality. We apply this approach to evaluate different configurations of the standalone Los Alamos sea ice model (CICE) encompassing the parametric uncertainty in the model, and to find new sets of model configurations that produce better agreement than previous configurations between model and observational estimates of sea ice concentration and thickness.« less

  8. Rapid coupling between ice volume and polar temperature over the past 150,000 years.

    PubMed

    Grant, K M; Rohling, E J; Bar-Matthews, M; Ayalon, A; Medina-Elizalde, M; Ramsey, C Bronk; Satow, C; Roberts, A P

    2012-11-29

    Current global warming necessitates a detailed understanding of the relationships between climate and global ice volume. Highly resolved and continuous sea-level records are essential for quantifying ice-volume changes. However, an unbiased study of the timing of past ice-volume changes, relative to polar climate change, has so far been impossible because available sea-level records either were dated by using orbital tuning or ice-core timescales, or were discontinuous in time. Here we present an independent dating of a continuous, high-resolution sea-level record in millennial-scale detail throughout the past 150,000 years. We find that the timing of ice-volume fluctuations agrees well with that of variations in Antarctic climate and especially Greenland climate. Amplitudes of ice-volume fluctuations more closely match Antarctic (rather than Greenland) climate changes. Polar climate and ice-volume changes, and their rates of change, are found to covary within centennial response times. Finally, rates of sea-level rise reached at least 1.2 m per century during all major episodes of ice-volume reduction.

  9. Variability of Arctic Sea Ice as Viewed from Space

    NASA Technical Reports Server (NTRS)

    Parkinson, Claire L.

    1998-01-01

    Over the past 20 years, satellite passive-microwave radiometry has provided a marvelous means for obtaining information about the variability of the Arctic sea ice cover and particularly about sea ice concentrations (% areal coverages) and from them ice extents and the lengths of the sea ice season. This ability derives from the sharp contrast between the microwave emissions of sea ice versus liquid water and allows routine monitoring of the vast Arctic sea ice cover, which typically varies in extent from a minimum of about 8,000,000 sq km in September to a maximum of about 15,000,000 sq km in March, the latter value being over 1.5 times the area of either the United States or Canada. The vast Arctic ice cover has many impacts, including hindering heat, mass, and y momentum exchanges between the oceans and the atmosphere, reducing the amount of solar radiation absorbed at the Earth's surface, affecting freshwater transports and ocean circulation, and serving as a vital surface for many species of polar animals. These direct impacts also lead to indirect impacts, including effects on local and perhaps global atmospheric temperatures, effects that are being examined in general circulation modeling studies, where preliminary results indicate that changes on the order of a few percent sea ice concentration can lead to temperature changes of 1 K or greater even in local areas outside of the sea ice region. Satellite passive-microwave data for November 1978 through December 1996 reveal marked regional and interannual variabilities in both the ice extents and the lengths of the sea ice season, as well as some statistically significant trends. For the north polar ice cover as a whole, maximum ice extents varied over a range of 14,700,000 - 15,900,000 km(2), while individual regions showed much greater percentage variations, e.g., with the Greenland Sea experiencing a range of 740,000 - 1,1110,000 km(2) in its yearly maximum ice coverage. Although variations from year to

  10. The frequency response of a coupled ice sheet-ice shelf-ocean system to climate forcing variability

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

    Changes at the West Antarctic ice-ocean boundary in recent decades has triggered significant increases in the regions contribution to global sea-level rise, coincident with large scale, and in some cases potentially unstable, grounding line retreat. Much of the induced change is thought to be driven by fluctuations in the oceanic heat available at the ice-ocean boundary, transported on-shelf via warm Circumpolar Deep Water (CDW). However, the processes in which ocean heat drives ice-sheet loss remains poorly understood, with observational studies routinely hindered by the extreme environment notorious to the Antarctic region. In this study we apply a novel synchronous coupled ice-ocean model, developed within the MITgcm, and are thus able to provide detailed insight into the impacts of short time scale (interannual to decadal) climate variability and feedbacks within the ice-ocean system. Feedbacks and response are assessed in an idealised ice-sheet/ocean-cavity configuration in which the far field ocean condition is adjusted to emulate periodic climate variability patterns. We reveal a non-linear response of the ice-sheet to periodic variations in thermocline depth. These non-linearities illustrate the heightened sensitivity of fast flowing ice-shelves to periodic perturbations in heat fluxes occurring at interannual and decadal time scales. The results thus highlight how small perturbations in variable climate forcing, like that of ENSO, may trigger large changes in ice-sheet response.

  11. High interannual variability of sea ice thickness in the Arctic region.

    PubMed

    Laxon, Seymour; Peacock, Neil; Smith, Doug

    2003-10-30

    Possible future changes in Arctic sea ice cover and thickness, and consequent changes in the ice-albedo feedback, represent one of the largest uncertainties in the prediction of future temperature rise. Knowledge of the natural variability of sea ice thickness is therefore critical for its representation in global climate models. Numerical simulations suggest that Arctic ice thickness varies primarily on decadal timescales owing to changes in wind and ocean stresses on the ice, but observations have been unable to provide a synoptic view of sea ice thickness, which is required to validate the model results. Here we use an eight-year time-series of Arctic ice thickness, derived from satellite altimeter measurements of ice freeboard, to determine the mean thickness field and its variability from 65 degrees N to 81.5 degrees N. Our data reveal a high-frequency interannual variability in mean Arctic ice thickness that is dominated by changes in the amount of summer melt, rather than by changes in circulation. Our results suggest that a continued increase in melt season length would lead to further thinning of Arctic sea ice.

  12. Processes driving sea ice variability in the Bering Sea in an eddying ocean/sea ice model: Mean seasonal cycle

    NASA Astrophysics Data System (ADS)

    Li, Linghan; McClean, Julie L.; Miller, Arthur J.; Eisenman, Ian; Hendershott, Myrl C.; Papadopoulos, Caroline A.

    2014-12-01

    The seasonal cycle of sea ice variability in the Bering Sea, together with the thermodynamic and dynamic processes that control it, are examined in a fine resolution (1/10°) global coupled ocean/sea-ice model configured in the Community Earth System Model (CESM) framework. The ocean/sea-ice model consists of the Los Alamos National Laboratory Parallel Ocean Program (POP) and the Los Alamos Sea Ice Model (CICE). The model was forced with time-varying reanalysis atmospheric forcing for the time period 1970-1989. This study focuses on the time period 1980-1989. The simulated seasonal-mean fields of sea ice concentration strongly resemble satellite-derived observations, as quantified by root-mean-square errors and pattern correlation coefficients. The sea ice energy budget reveals that the seasonal thermodynamic ice volume changes are dominated by the surface energy flux between the atmosphere and the ice in the northern region and by heat flux from the ocean to the ice along the southern ice edge, especially on the western side. The sea ice force balance analysis shows that sea ice motion is largely associated with wind stress. The force due to divergence of the internal ice stress tensor is large near the land boundaries in the north, and it is small in the central and southern ice-covered region. During winter, which dominates the annual mean, it is found that the simulated sea ice was mainly formed in the northern Bering Sea, with the maximum ice growth rate occurring along the coast due to cold air from northerly winds and ice motion away from the coast. South of St Lawrence Island, winds drive the model sea ice southwestward from the north to the southwestern part of the ice-covered region. Along the ice edge in the western Bering Sea, model sea ice is melted by warm ocean water, which is carried by the simulated Bering Slope Current flowing to the northwest, resulting in the S-shaped asymmetric ice edge. In spring and fall, similar thermodynamic and dynamic

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

    NASA Astrophysics Data System (ADS)

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

    2012-04-01

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

  14. Multiple Off-Ice Performance Variables Predict On-Ice Skating Performance in Male and Female Division III Ice Hockey Players.

    PubMed

    Janot, Jeffrey M; Beltz, Nicholas M; Dalleck, Lance D

    2015-09-01

    The purpose of this study was to determine if off-ice performance variables could predict on-ice skating performance in Division III collegiate hockey players. Both men (n = 15) and women (n = 11) hockey players (age = 20.5 ± 1.4 years) participated in the study. The skating tests were agility cornering S-turn, 6.10 m acceleration, 44.80 m speed, modified repeat skate, and 15.20 m full speed. Off-ice variables assessed were years of playing experience, height, weight and percent body fat and off-ice performance variables included vertical jump (VJ), 40-yd dash (36.58m), 1-RM squat, pro-agility, Wingate peak power and peak power percentage drop (% drop), and 1.5 mile (2.4km) run. Results indicated that 40-yd dash (36.58m), VJ, 1.5 mile (2.4km) run, and % drop were significant predictors of skating performance for repeat skate (slowest, fastest, and average time) and 44.80 m speed time, respectively. Four predictive equations were derived from multiple regression analyses: 1) slowest repeat skate time = 2.362 + (1.68 x 40-yd dash time) + (0.005 x 1.5 mile run), 2) fastest repeat skate time = 9.762 - (0.089 x VJ) - (0.998 x 40-yd dash time), 3) average repeat skate time = 7.770 + (1.041 x 40-yd dash time) - (0.63 x VJ) + (0.003 x 1.5 mile time), and 4) 47.85 m speed test = 7.707 - (0.050 x VJ) - (0.01 x % drop). It was concluded that selected off-ice tests could be used to predict on-ice performance regarding speed and recovery ability in Division III male and female hockey players. Key pointsThe 40-yd dash (36.58m) and vertical jump tests are significant predictors of on-ice skating performance specific to speed.In addition to 40-yd dash and vertical jump, the 1.5 mile (2.4km) run for time and percent power drop from the Wingate anaerobic power test were also significant predictors of skating performance that incorporates the aspect of recovery from skating activity.Due to the specificity of selected off-ice variables as predictors of on-ice performance, coaches can

  15. Multiple Off-Ice Performance Variables Predict On-Ice Skating Performance in Male and Female Division III Ice Hockey Players

    PubMed Central

    Janot, Jeffrey M.; Beltz, Nicholas M.; Dalleck, Lance D.

    2015-01-01

    The purpose of this study was to determine if off-ice performance variables could predict on-ice skating performance in Division III collegiate hockey players. Both men (n = 15) and women (n = 11) hockey players (age = 20.5 ± 1.4 years) participated in the study. The skating tests were agility cornering S-turn, 6.10 m acceleration, 44.80 m speed, modified repeat skate, and 15.20 m full speed. Off-ice variables assessed were years of playing experience, height, weight and percent body fat and off-ice performance variables included vertical jump (VJ), 40-yd dash (36.58m), 1-RM squat, pro-agility, Wingate peak power and peak power percentage drop (% drop), and 1.5 mile (2.4km) run. Results indicated that 40-yd dash (36.58m), VJ, 1.5 mile (2.4km) run, and % drop were significant predictors of skating performance for repeat skate (slowest, fastest, and average time) and 44.80 m speed time, respectively. Four predictive equations were derived from multiple regression analyses: 1) slowest repeat skate time = 2.362 + (1.68 x 40-yd dash time) + (0.005 x 1.5 mile run), 2) fastest repeat skate time = 9.762 - (0.089 x VJ) - (0.998 x 40-yd dash time), 3) average repeat skate time = 7.770 + (1.041 x 40-yd dash time) - (0.63 x VJ) + (0.003 x 1.5 mile time), and 4) 47.85 m speed test = 7.707 - (0.050 x VJ) - (0.01 x % drop). It was concluded that selected off-ice tests could be used to predict on-ice performance regarding speed and recovery ability in Division III male and female hockey players. Key points The 40-yd dash (36.58m) and vertical jump tests are significant predictors of on-ice skating performance specific to speed. In addition to 40-yd dash and vertical jump, the 1.5 mile (2.4km) run for time and percent power drop from the Wingate anaerobic power test were also significant predictors of skating performance that incorporates the aspect of recovery from skating activity. Due to the specificity of selected off-ice variables as predictors of on-ice performance, coaches

  16. Interannual variability of monthly Southern Ocean sea ice distributions

    NASA Technical Reports Server (NTRS)

    Parkinson, Claire L.

    1992-01-01

    The interannual variability of the Southern-Ocean sea-ice distributions was mapped and analyzed using data from Nimbus-5 ESMR and Nimbus-7 SMMR, collected from 1973 to 1987. The set of 12 monthly maps obtained reveals many details on spatial variability that are unobtainable from time series of ice extents. These maps can be used as baseline maps for comparisons against future Southern Ocean sea ice distributions. The maps are supplemented by more detailed maps of the frequency of ice coverage, presented in this paper for one month within each of the four seasons, and by the breakdown of these results to the periods covered individually by each of the two passive-microwave imagers.

  17. Estimating the impact of internal climate variability on ice sheet model simulations

    NASA Astrophysics Data System (ADS)

    Tsai, C. Y.; Forest, C. E.; Pollard, D.

    2016-12-01

    Rising sea level threatens human societies and coastal habitats and melting ice sheets are a major contributor to sea level rise (SLR). Thus, understanding uncertainty of both forcing and variability within the climate system is essential for assessing long-term risk of SLR given their impact on ice sheet evolution. The predictability of polar climate is limited by uncertainties from the given forcing, the climate model response to this forcing, and the internal variability from feedbacks within the fully coupled climate system. Among those sources of uncertainty, the impact of internal climate variability on ice sheet changes has not yet been robustly assessed. Here we investigate how internal variability affects ice sheet projections using climate fields from two Community Earth System Model (CESM) large-ensemble (LE) experiments to force a three-dimensional ice sheet model. Each ensemble member in an LE experiment undergoes the same external forcings but with unique initial conditions. We find that for both LEs, 2m air temperature variability over Greenland ice sheet (GrIS) can lead to significantly different ice sheet responses. Our results show that the internal variability from two fully coupled CESM LEs can cause about 25 35 mm differences of GrIS's contribution to SLR in 2100 compared to present day (about 20% of the total change), and 100m differences of SLR in 2300. Moreover, only using ensemble-mean climate fields as the forcing in ice sheet model can significantly underestimate the melt of GrIS. As the Arctic region becomes warmer, the role of internal variability is critical given the complex nonlinear interactions between surface temperature and ice sheet. Our results demonstrate that internal variability from coupled atmosphere-ocean general circulation model can affect ice sheet simulations and the resulting sea-level projections. This study highlights an urgent need to reassess associated uncertainties of projecting ice sheet loss over the next few

  18. Effects of ice shelf basal melt variability on evolution of Thwaites Glacier

    NASA Astrophysics Data System (ADS)

    Hoffman, M. J.; Fyke, J. G.; Price, S. F.; Asay-Davis, X.; Perego, M.

    2017-12-01

    Theory, modeling, and observations indicate that marine ice sheets on a retrograde bed, including Thwaites Glacier, Antarctica, are only conditionally stable. Previous modeling studies have shown that rapid, unstable retreat can occur when steady ice-shelf basal melting causes the grounding line to retreat past restraining bedrock bumps. Here we explore the initiation and evolution of unstable retreat of Thwaites Glacier when the ice-shelf basal melt forcing includes temporal variability mimicking realistic climate variability. We use the three-dimensional, higher-order Model for Prediction Across Scales-Land Ice (MPASLI) model forced with an ice shelf basal melt parameterization derived from previous coupled ice sheet/ocean simulations. We add sinusoidal temporal variability to the melt parameterization that represents shoaling and deepening of Circumpolar Deep Water. We perform an ensemble of 250 year duration simulations with different values for the amplitude, period, and phase of the variability. Preliminary results suggest that, overall, variability leads to slower grounding line retreat and less mass loss than steady simulations. Short period (2 yr) variability leads to similar results as steady forcing, whereas decadal variability can result in up to one-third less mass loss. Differences in phase lead to a large range in mass loss/grounding line retreat, but it is always less than the steady forcing. The timing of ungrounding from each restraining bedrock bump, which is strongly affected by the melt variability, is the rate limiting factor, and variability-driven delays in ungrounding at each bump accumulate. Grounding line retreat in the regions between bedrock bumps is relatively unaffected by ice shelf melt variability. While the results are sensitive to the form of the melt parameterization and its variability, we conclude that decadal period ice shelf melt variability could potentially delay marine ice sheet instability by up to many decades. However

  19. Seasonal and Interannual Variability of the Arctic Sea Ice: A Comparison between AO-FVCOM and Observations

    NASA Astrophysics Data System (ADS)

    Zhang, Y.; Chen, C.; Beardsley, R. C.; Gao, G.; Qi, J.; Lin, H.

    2016-02-01

    A high-resolution (up to 2 km), unstructured-grid, fully ice-sea coupled Arctic Ocean Finite-Volume Community Ocean Model (AO-FVCOM) was used to simulate the Arctic sea ice over the period 1978-2014. Good agreements were found between simulated and observed sea ice extent, concentration, drift velocity and thickness, indicating that the AO-FVCOM captured not only the seasonal and interannual variability but also the spatial distribution of the sea ice in the Arctic in the past 37 years. Compared with other six Arctic Ocean models (ECCO2, GSFC, INMOM, ORCA, NAME and UW), the AO-FVCOM-simulated ice thickness showed a higher correlation coefficient and a smaller difference with observations. An effort was also made to examine the physical processes attributing to the model-produced bias in the sea ice simulation. The error in the direction of the ice drift velocity was sensitive to the wind turning angle; smaller when the wind was stronger, but larger when the wind was weaker. This error could lead to the bias in the near-surface current in the fully or partially ice-covered zone where the ice-sea interfacial stress was a major driving force.

  20. Inception and variability of the Antarctic ice sheet across the Eocene-Oligocene transition

    NASA Astrophysics Data System (ADS)

    Stocchi, Paolo; Galeotti, Simone; Ladant, Jan-Baptiste; DeConto, Robert; Vermeersen, Bert; Rugenstein, Maria

    2014-05-01

    Climate cooling throughout middle to late Eocene (~48 - 34 Million years ago, Ma) triggered the transition from hot-house to ice-house conditions. Based on deep-sea marine δ18O values, a continental-scale Antarctic Ice Sheet (AIS) rapidly developed across the Eocene-Oligocene transition (EOT) in two ~200 kyr-spaced phases between 34.0 - 33.5 Ma. Regardless of the geographical configuration of southern ocean gateways, geochemical data and ice-sheet modelling show that AIS glaciation initiated as atmospheric CO2 fell below ~2.5 times pre-industrial values. AIS likely reached or even exceeded present-day dimensions. Quantifying the magnitude and timing of AIS volume variations by means of δ18O records is hampered by the fact that the latter reflect a coupled signal of temperature and ice-sheet volume. Besides, bathymetric variations based on marine geologic sections are affected by large uncertainties and, most importantly, reflect the local response of relative sea level (rsl) to ice volume fluctuations rather than the global eustatic signal. AIS proximal and Northern Hemisphere (NH) marine settings show an opposite trend of rsl change across the EOT. In fact, consistently with central values based on δ18O records, an 60 ± 20m rsl drop is estimated from NH low-latitude shallow marine sequences. Conversely, sedimentary facies from shallow shelfal areas in the proximity of the AIS witness an 50 - 150m rsl rise across the EOT. Accounting for ice-load-induced crustal and geoidal deformations and for the mutual gravitational attraction between the growing AIS and the ocean water is a necessary requirement to reconcile near- and far-field rsl sites, regardless of tectonics and of any other possible local contamination. In this work we investigate the AIS inception and variability across the EOT by combining the observed rsl changes with predictions based on numerical modeling of Glacial Isostatic Adjustment (GIA). We solve the gravitationally self-consistent Sea Level

  1. Characterizing Arctic Sea Ice Topography Using High-Resolution IceBridge Data

    NASA Technical Reports Server (NTRS)

    Petty, Alek; Tsamados, Michel; Kurtz, Nathan; Farrell, Sinead; Newman, Thomas; Harbeck, Jeremy; Feltham, Daniel; Richter-Menge, Jackie

    2016-01-01

    We present an analysis of Arctic sea ice topography using high resolution, three-dimensional, surface elevation data from the Airborne Topographic Mapper, flown as part of NASA's Operation IceBridge mission. Surface features in the sea ice cover are detected using a newly developed surface feature picking algorithm. We derive information regarding the height, volume and geometry of surface features from 2009-2014 within the Beaufort/Chukchi and Central Arctic regions. The results are delineated by ice type to estimate the topographic variability across first-year and multi-year ice regimes.

  2. Delayed build-up of Arctic ice sheets during 400,000-year minima in insolation variability.

    PubMed

    Hao, Qingzhen; Wang, Luo; Oldfield, Frank; Peng, Shuzhen; Qin, Li; Song, Yang; Xu, Bing; Qiao, Yansong; Bloemendal, Jan; Guo, Zhengtang

    2012-10-18

    Knowledge of the past variability of climate at high northern latitudes during astronomical analogues of the present interglacial may help to inform our understanding of future climate change. Unfortunately, long-term continuous records of ice-sheet variability in the Northern Hemisphere only are scarce because records of benthic (18)O content represent an integrated signal of changes in ice volume in both polar regions. However, variations in Northern Hemisphere ice sheets influence the Siberian High (an atmospheric pressure system), so variations in the East Asian winter monsoon (EAWM)--as recorded in the aeolian dust deposits on the Chinese Loess Plateau--can serve as a useful proxy of Arctic climate variability before the ice-core record begins. Here we present an EAWM proxy record using grain-size variations in two parallel loess sections representative of sequences across the whole of the Chinese Loess Plateau over the past 900,000 years. The results show that during periods of low eccentricity and precessional variability at approximately 400,000-year intervals, the grain-size-inferred intensity of the EAWM remains weak for up to 20,000 years after the end of the interglacial episode of high summer monsoon activity and strong pedogenesis. In contrast, there is a rapid increase in the EAWM after the end of most other interglacials. We conclude that, for both the 400,000-year interglacials, the weak EAWM winds maintain a mild, non-glacial climate at high northern latitudes for much longer than expected from the conventional loess and marine oxygen isotope records. During these times, the less-severe summer insolation minima at 65° N (ref. 4) would have suppressed ice and snow accumulation, leading to a weak Siberian High and, consequently, weak EAWM winds.

  3. Arctic Sea Ice: Trends, Stability and Variability

    NASA Astrophysics Data System (ADS)

    Moon, Woosok

    A stochastic Arctic sea-ice model is derived and analyzed in detail to interpret the recent decay and associated variability of Arctic sea-ice under changes in greenhouse gas forcing widely referred to as global warming. The approach begins from a deterministic model of the heat flux balance through the air/sea/ice system, which uses observed monthly-averaged heat fluxes to drive a time evolution of sea-ice thickness. This model reproduces the observed seasonal cycle of the ice cover and it is to this that stochastic noise---representing high frequency variability---is introduced. The model takes the form of a single periodic non-autonomous stochastic ordinary differential equation. Following an introductory chapter, the two that follow focus principally on the properties of the deterministic model in order to identify the main properties governing the stability of the ice cover. In chapter 2 the underlying time-dependent solutions to the deterministic model are analyzed for their stability. It is found that the response time-scale of the system to perturbations is dominated by the destabilizing sea-ice albedo feedback, which is operative in the summer, and the stabilizing long wave radiative cooling of the ice surface, which is operative in the winter. This basic competition is found throughout the thesis to define the governing dynamics of the system. In particular, as greenhouse gas forcing increases, the sea-ice albedo feedback becomes more effective at destabilizing the system. Thus, any projections of the future state of Arctic sea-ice will depend sensitively on the treatment of the ice-albedo feedback. This in turn implies that the treatment a fractional ice cover as the ice areal extent changes rapidly, must be handled with the utmost care. In chapter 3, the idea of a two-season model, with just winter and summer, is revisited. By breaking the seasonal cycle up in this manner one can simplify the interpretation of the basic dynamics. Whereas in the fully

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

    USGS Publications Warehouse

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

    1997-01-01

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

  5. 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

  6. Variable volume combustor

    DOEpatents

    Ostebee, Heath Michael; Ziminsky, Willy Steve; Johnson, Thomas Edward; Keener, Christopher Paul

    2017-01-17

    The present application provides a variable volume combustor for use with a gas turbine engine. The variable volume combustor may include a liner, a number of micro-mixer fuel nozzles positioned within the liner, and a linear actuator so as to maneuver the micro-mixer fuel nozzles axially along the liner.

  7. Modeling the imprint of Milankovitch cycles on early Pleistocene ice volume

    NASA Astrophysics Data System (ADS)

    Roychowdhury, R.; DeConto, R.; Pollard, D.

    2017-12-01

    Global climate during Quaternary and Late Pliocene (present-3.1 Ma) is characterized by alternating glacial and interglacial conditions. Several proposed theories associate these cycles with variations in the Earth's orbital configuration. In this study, we attempt to address the anomalously strong obliquity forcing in the Late Pliocene/Early Pleistocene ice volume records (41 kyr world), which stands in sharp contrast to the primary cyclicity of insolation, which is at precessional periods (23 kyr). Model results from GCM simulations show that at low eccentricities (e<0.015), the effect of precession is minimal, and the integrated insolation metrics (such as summer metric, PDD, etc.) vary in-phase between the two hemispheres. At higher eccentricities (e>0.015), precessional response is important, and the insolation metrics vary out-of-phase between the two hemispheres. Using simulations from a GCM-driven ice sheet model, we simulate time continuous ice volume changes from Northern and Southern Hemispheres. Under eccentricities lower than 0.015, ice sheets in both hemispheres respond only to obliquity cycle, and grow and melt together (in-phase). If the ice sheet is simulated with eccentricity higher than 0.015, both hemispheres become more sensitive to precessional variation, and vary out-of-phase with each other, which is consistent with proxy observations from the late Pleistocene glaciations. We use the simulated ice volumes from 2.0 to 1.0 ma to empirically calculate global benthic δ18O variations based on the assumption that relationships between collapse and growth of ice-sheets and sea level is linear and symmetric and that the isotopic signature of the individual ice-sheets has not changed with time. Our modeled global benthic δ18O values are broadly consistent with the paleoclimate proxy records such as the LR04 stack.

  8. Variability in Arctic sea ice topography and atmospheric form drag: Combining IceBridge laser altimetry with ASCAT radar backscatter.

    NASA Astrophysics Data System (ADS)

    Petty, A.; Tsamados, M.; Kurtz, N. T.

    2016-12-01

    Here we present atmospheric form drag estimates over Arctic sea ice using high resolution, three-dimensional surface elevation data from NASA's Operation IceBridge Airborne Topographic Mapper (ATM), and surface roughness estimates from the Advanced Scatterometer (ASCAT). Surface features of the ice pack (e.g. pressure ridges) are detected using IceBridge ATM elevation data and a novel surface feature-picking algorithm. We use simple form drag parameterizations to convert the observed height and spacing of surface features into an effective atmospheric form drag coefficient. The results demonstrate strong regional variability in the atmospheric form drag coefficient, linked to variability in both the height and spacing of surface features. This includes form drag estimates around 2-3 times higher over the multiyear ice north of Greenland, compared to the first-year ice of the Beaufort/Chukchi seas. We compare results from both scanning and linear profiling to ensure our results are consistent with previous studies investigating form drag over Arctic sea ice. A strong correlation between ASCAT surface roughness estimates (using radar backscatter) and the IceBridge form drag results enable us to extrapolate the IceBridge data collected over the western-Arctic across the entire Arctic Ocean. While our focus is on spring, due to the timing of the primary IceBridge campaigns since 2009, we also take advantage of the autumn data collected by IceBridge in 2015 to investigate seasonality in Arctic ice topography and the resulting form drag coefficient. Our results offer the first large-scale assessment of atmospheric form drag over Arctic sea ice due to variable ice topography (i.e. within the Arctic pack ice). The analysis is being extended to the Antarctic IceBridge sea ice data, and the results are being used to calibrate a sophisticated form drag parameterization scheme included in the sea ice model CICE, to improve the representation of form drag over Arctic and

  9. Interannual Variability of Snow and Ice and Impact on the Carbon Cycle

    NASA Technical Reports Server (NTRS)

    Yung, Yuk L.

    2004-01-01

    The goal of this research is to assess the impact of the interannual variability in snow/ice using global satellite data sets acquired in the last two decades. This variability will be used as input to simulate the CO2 interannual variability at high latitudes using a biospheric model. The progress in the past few years is summarized as follows: 1) Albedo decrease related to spring snow retreat; 2) Observed effects of interannual summertime sea ice variations on the polar reflectance; 3) The Northern Annular Mode response to Arctic sea ice loss and the sensitivity of troposphere-stratosphere interaction; 4) The effect of Arctic warming and sea ice loss on the growing season in northern terrestrial ecosystem.

  10. Seasonal and interannual variability of the Arctic sea ice: A comparison between AO-FVCOM and observations

    NASA Astrophysics Data System (ADS)

    Zhang, Yu; Chen, Changsheng; Beardsley, Robert C.; Gao, Guoping; Qi, Jianhua; Lin, Huichan

    2016-11-01

    A high-resolution (up to 2 km), unstructured-grid, fully ice-sea coupled Arctic Ocean Finite-Volume Community Ocean Model (AO-FVCOM) was used to simulate the sea ice in the Arctic over the period 1978-2014. The spatial-varying horizontal model resolution was designed to better resolve both topographic and baroclinic dynamics scales over the Arctic slope and narrow straits. The model-simulated sea ice was in good agreement with available observed sea ice extent, concentration, drift velocity and thickness, not only in seasonal and interannual variability but also in spatial distribution. Compared with six other Arctic Ocean models (ECCO2, GSFC, INMOM, ORCA, NAME, and UW), the AO-FVCOM-simulated ice thickness showed a higher mean correlation coefficient of ˜0.63 and a smaller residual with observations. Model-produced ice drift speed and direction errors varied with wind speed: the speed and direction errors increased and decreased as the wind speed increased, respectively. Efforts were made to examine the influences of parameterizations of air-ice external and ice-water interfacial stresses on the model-produced bias. The ice drift direction was more sensitive to air-ice drag coefficients and turning angles than the ice drift speed. Increasing or decreasing either 10% in water-ice drag coefficient or 10° in water-ice turning angle did not show a significant influence on the ice drift velocity simulation results although the sea ice drift speed was more sensitive to these two parameters than the sea ice drift direction. Using the COARE 4.0-derived parameterization of air-water drag coefficient for wind stress did not significantly influence the ice drift velocity simulation.

  11. Sea ice convergence along the Arctic coasts of Greenland and the Canadian Arctic Archipelago: Variability and extremes (1992-2014)

    NASA Astrophysics Data System (ADS)

    Kwok, Ron

    2015-09-01

    After the summer of 2013, a convergence-induced tail in the thickness distribution of the ice cover is found along the Arctic coasts of Greenland and Canadian Arctic Archipelago. Prompted by this, a normalized ice convergence index (ICI) is introduced to examine the variability and extremes in convergence in a 23 year record (1992-2014) of monthly ice drift. Large-scale composites of circulation patterns, characteristic of regional convergence and divergence, are examined. Indeed, the ICI shows the June 2013 convergence event to be an extreme (i.e., ICI > 2). Furthermore, there is a cluster of 9 months over a 17 month period with positive ICIs (i.e., >1) following the record summer minimum ice extent (SMIE) in 2012; the imprint of ice dynamics from this cluster of positive ICIs likely contributed to higher SMIEs in 2013 and 2014. The impact of convergence on SMIE is discussed, and the increase in Arctic ice volume in 2013 is underscored.

  12. Sea Ice and Hydrographic Variability in the Northwest North Atlantic

    NASA Astrophysics Data System (ADS)

    Fenty, I. G.; Heimbach, P.; Wunsch, C. I.

    2010-12-01

    Sea ice anomalies in the Northwest North Atlantic's Labrador Sea are of climatic interest because of known and hypothesized feedbacks with hydrographic anomalies, deep convection/mode water formation, and Northern Hemisphere atmospheric patterns. As greenhouse gas concentrations increase, hydrographic anomalies formed in the Arctic Ocean associated with warming will propagate into the Labrador Sea via the Fram Strait/West Greenland Current and the Canadian Archipelago/Baffin Island Current. Therefore, understanding the dynamical response of sea ice in the basin to hydrographic anomalies is essential for the prediction and interpretation of future high-latitude climate change. Historically, efforts to quantify the link between the observed sea ice and hydrographic variability in the region has been limited due to in situ observation paucity and technical challenges associated with synthesizing ocean and sea ice observations with numerical models. To elaborate the relationship between sea ice and ocean variability, we create three one-year (1992-1993, 1996-1997, 2003-2004) three-dimensional time-varying reconstructions of the ocean and sea ice state in Labrador Sea and Baffin Bay. The reconstructions are syntheses of a regional coupled 32 km ocean-sea ice model with a suite of contemporary in situ and satellite hydrographic and ice data using the adjoint method. The model and data are made consistent, in a least-squares sense, by iteratively adjusting several model control variables (e.g., ocean initial and lateral boundary conditions and the atmospheric state) to minimize an uncertainty-weighted model-data misfit cost function. The reconstructions reveal that the ice pack attains a state of quasi-equilibrium in mid-March (the annual sea ice maximum) in which the total ice-covered area reaches a steady state -ice production and dynamical divergence along the coasts balances dynamical convergence and melt along the pack’s seaward edge. Sea ice advected to the

  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. Strong and highly variable push of ocean waves on Southern Ocean sea ice.

    PubMed

    Stopa, Justin E; Sutherland, Peter; Ardhuin, Fabrice

    2018-06-05

    Sea ice in the Southern Ocean has expanded over most of the past 20 y, but the decline in sea ice since 2016 has taken experts by surprise. This recent evolution highlights the poor performance of numerical models for predicting extent and thickness, which is due to our poor understanding of ice dynamics. Ocean waves are known to play an important role in ice break-up and formation. In addition, as ocean waves decay, they cause a stress that pushes the ice in the direction of wave propagation. This wave stress could not previously be quantified due to insufficient observations at large scales. Sentinel-1 synthetic aperture radars (SARs) provide high-resolution imagery from which wave height is measured year round encompassing Antarctica since 2014. Our estimates give an average wave stress that is comparable to the average wind stress acting over 50 km of sea ice. We further reveal highly variable half-decay distances ranging from 400 m to 700 km, and wave stresses from 0.01 to 1 Pa. We expect that this variability is related to ice properties and possibly different floe sizes and ice thicknesses. A strong feedback of waves on sea ice, via break-up and rafting, may be the cause of highly variable sea-ice properties.

  15. Impacts of the Variability of Ice Types on the Decline of the Arctic Perennial Sea Ice Cover

    NASA Technical Reports Server (NTRS)

    Comiso, Josefino C.

    2005-01-01

    The observed rapid decline in the Arctic perennial ice cover is one of the most remarkable signal of change in the Arctic region. Updated data now show an even higher rate of decline of 9.8% per decade than the previous report of 8.9% per decade mainly because of abnormally low values in the last 4 years. To gain insights into this decline, the variability of the second year ice, which is the relatively thin component of the perennial ice cover, and other ice types is studied. The perennial ice cover in the 1990s was observed to be highly variable which might have led to higher production of second year ice and may in part explain the observed ice thinning during the period and triggered further decline. The passive microwave signature of second year ice is also studied and results show that while the signature is different from that of the older multiyear ice, it is surprisingly more similar to that of first year ice. This in part explains why previous estimates of the area of multiyear ice during the winter period are considerably lower than the area of the perennial ice cover during the preceding summer. Four distinct clusters representing radiometrically different types have been identified using multi-channel cluster analysis of passive microwave data. Data from two of these clusters, postulated to come from second year and older multiyear ice regions are also shown to have average thicknesses of 2.4 and 4.1 m, respectively, indicating that the passive microwave data may contain some ice thickness information that can be utilized for mass balance studies. The yearly anomaly maps indicate high gains of first year ice cover in the Arctic during the last decade which means higher production of second year ice and fraction of this type in the declining perennial ice cover. While not the only cause, the rapid decline in the perennial ice cover is in part caused by the increasing fractional component of the thinner second year ice cover that is very vulnerable to

  16. Ice Ih anomalies: Thermal contraction, anomalous volume isotope effect, and pressure-induced amorphization.

    PubMed

    Salim, Michael A; Willow, Soohaeng Yoo; Hirata, So

    2016-05-28

    Ice Ih displays several anomalous thermodynamic properties such as thermal contraction at low temperatures, an anomalous volume isotope effect (VIE) rendering the volume of D2O ice greater than that of H2O ice, and a pressure-induced transition to the high-density amorphous (HDA) phase. Furthermore, the anomalous VIE increases with temperature, despite its quantum-mechanical origin. Here, embedded-fragment ab initio second-order many-body perturbation (MP2) theory in the quasiharmonic approximation (QHA) is applied to the Gibbs energy of an infinite, proton-disordered crystal of ice Ih at wide ranges of temperatures and pressures. The quantum effect of nuclei moving in anharmonic potentials is taken into account from first principles without any empirical or nonsystematic approximation to either the electronic or vibrational Hamiltonian. MP2 predicts quantitatively correctly the thermal contraction at low temperatures, which is confirmed to originate from the volume-contracting hydrogen-bond bending modes (acoustic phonons). It qualitatively reproduces (but underestimates) the thermal expansion at higher temperatures, caused by the volume-expanding hydrogen-bond stretching (and to a lesser extent librational) modes. The anomalous VIE is found to be the result of subtle cancellations among closely competing isotope effects on volume from all modes. Consequently, even ab initio MP2 with the aug-cc-pVDZ and aug-cc-pVTZ basis sets has difficulty reproducing this anomaly, yielding qualitatively varied predictions of the sign of the VIE depending on such computational details as the choice of the embedding field. However, the temperature growth of the anomalous VIE is reproduced robustly and is ascribed to the librational modes. These solid-state MP2 calculations, as well as MP2 Born-Oppenheimer molecular dynamics, find a volume collapse and a loss of symmetry and long-range order in ice Ih upon pressure loading of 2.35 GPa or higher. Concomitantly, rapid softening of

  17. Ice Ih anomalies: Thermal contraction, anomalous volume isotope effect, and pressure-induced amorphization

    NASA Astrophysics Data System (ADS)

    Salim, Michael A.; Willow, Soohaeng Yoo; Hirata, So

    2016-05-01

    Ice Ih displays several anomalous thermodynamic properties such as thermal contraction at low temperatures, an anomalous volume isotope effect (VIE) rendering the volume of D2O ice greater than that of H2O ice, and a pressure-induced transition to the high-density amorphous (HDA) phase. Furthermore, the anomalous VIE increases with temperature, despite its quantum-mechanical origin. Here, embedded-fragment ab initio second-order many-body perturbation (MP2) theory in the quasiharmonic approximation (QHA) is applied to the Gibbs energy of an infinite, proton-disordered crystal of ice Ih at wide ranges of temperatures and pressures. The quantum effect of nuclei moving in anharmonic potentials is taken into account from first principles without any empirical or nonsystematic approximation to either the electronic or vibrational Hamiltonian. MP2 predicts quantitatively correctly the thermal contraction at low temperatures, which is confirmed to originate from the volume-contracting hydrogen-bond bending modes (acoustic phonons). It qualitatively reproduces (but underestimates) the thermal expansion at higher temperatures, caused by the volume-expanding hydrogen-bond stretching (and to a lesser extent librational) modes. The anomalous VIE is found to be the result of subtle cancellations among closely competing isotope effects on volume from all modes. Consequently, even ab initio MP2 with the aug-cc-pVDZ and aug-cc-pVTZ basis sets has difficulty reproducing this anomaly, yielding qualitatively varied predictions of the sign of the VIE depending on such computational details as the choice of the embedding field. However, the temperature growth of the anomalous VIE is reproduced robustly and is ascribed to the librational modes. These solid-state MP2 calculations, as well as MP2 Born-Oppenheimer molecular dynamics, find a volume collapse and a loss of symmetry and long-range order in ice Ih upon pressure loading of 2.35 GPa or higher. Concomitantly, rapid softening of

  18. Arctic sea ice variability in the context of recent atmospheric circulation trends

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

    Deser, C.; Walsh, J.E.; Timlin, M.S.

    Sea ice is a sensitive component of the climate system, influenced by conditions in both the atmosphere and ocean. Variations in sea ice may in turn modulate climate by altering the surface albedo; the exchange of heat, moisture, and momentum between the atmosphere and ocean; and the upper ocean stratification in areas of deep water formation. The surface albedo effect is considered to be one of the dominant factors in the poleward amplification of global warming due to increased greenhouse gas concentrations simulated in many climate models. Forty years (1958--97) of reanalysis products and corresponding sea ice concentration data aremore » used to document Arctic sea ice variability and its association with surface air temperature (SAT) and sea level pressure (SLP) throughout the Northern Hemisphere extratropics. The dominant mode of winter (January-March) sea ice variability exhibits out-of-phase fluctuations between the western and eastern North Atlantic, together with a weaker dipole in the North Pacific. The time series of this mode has a high winter-to-winter autocorrelation (0.69) and is dominated by decadal-scale variations and a longer-term trend of diminishing ice cover east of Greenland and increasing ice cover west of Greenland. Associated with the dominant pattern of winter sea ice variability are large-scale changes in SAT and SLP that closely resemble the North Atlantic oscillation. The associated SAT and surface sensible and latent heat flux anomalies are largest over the portions of the marginal sea ice zone in which the trends of ice coverage have been greatest, although the well-documented warming of the northern continental regions is also apparent. the temporal and spatial relationships between the SLP and ice anomaly fields are consistent with the notion that atmospheric circulation anomalies force the sea ice variations. However, there appears to be a local response of the atmospheric circulation to the changing sea ice variations. However

  19. Future Interannual Variability of Arctic Sea Ice Area and its Implications for Marine Navigation

    NASA Astrophysics Data System (ADS)

    Vavrus, S. J.; Mioduszewski, J.; Holland, M. M.; Wang, M.; Landrum, L.

    2016-12-01

    As both a symbol and driver of ongoing climate change, the diminishing Arctic sea ice pack has been widely studied in a variety of contexts. Most research, however, has focused on time-mean changes in sea ice, rather than on short-term variations that also have important physical and societal consequences. In this study we test the hypothesis that interannual Arctic sea ice variability will increase in the future by utilizing a set of 40 independent simulations from the Community Earth System Model's Large Ensemble for the 1920-2100 period. The model projects that ice variability will indeed grow substantially in all months but with a strong seasonal dependence in magnitude and timing. The variability increases most during late autumn (November-December) and least during spring. This increase proceeds in a time-transgressive manner over the course of the year, peaking soonest (2020s) in late-summer months and latest (2090s) during late spring. The variability in every month is inversely correlated with the average melt rate, resulting in an eventual decline in both terms as the ice pack becomes seasonal by late century. These projected changes in sea ice variations will likely have significant consequences for marine navigation, which we assess with the empirical Ice Numeral (IN) metric. A function of ice concentration and thickness, the IN quantifies the difficulty in traversing a transect of sea ice-covered ocean as a function of vessel strength. Our results show that although increasingly open Arctic seas will mean generally more favorable conditions for navigation, the concurrent rise in the variability of ice cover poses a competing risk. In particular, future intervals featuring the most rapid declines in ice area that coincide with the highest interannual ice variations will offer more inviting shipping opportunities tempered by less predictable navigational conditions.

  20. Controls on Arctic sea ice from first-year and multi-year survival rates

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

    Hunke, Jes

    2009-01-01

    The recent decrease in Arctic sea ice cover has transpired with a significant loss of multi year ice. The transition to an Arctic that is populated by thinner first year sea ice has important implications for future trends in area and volume. Here we develop a reduced model for Arctic sea ice with which we investigate how the survivability of first year and multi year ice control the mean state, variability, and trends in ice area and volume.

  1. Rapid grounding line migration induced by internal variability of a marine-terminating ice stream

    NASA Astrophysics Data System (ADS)

    Robel, A.; Schoof, C.; Tziperman, E.

    2013-12-01

    Numerous studies have found significant variability in the velocity of ice streams to be a prominent feature of geomorphologic records in the Siple Coast (Catania et al. 2012) and other regions in West Antarctica (Dowdeswell et al. 2008). Observations indicate that grounding line position is strongly influenced by ice stream variability, producing rapid grounding line migration in the recent past (Catania et al. 2006) and the modern (Joughin & Tulaczyk 2002). We analyze the interaction of grounding line mass flux and position in a marine-terminating ice stream using a stretch-coordinate flowline model. This model is based on that described in Schoof (2007), with a mesh refined near the grounding line to ensure accurate resolution of the mechanical transition zone. Here we have added lateral shear stress (Dupont & Alley 2005) and an undrained plastic bed (Tulaczyk et al. 2000). The parameter dependence of ice stream variability seen in this model compares favorably to both simpler (Robel et al. 2013) and more complex (van der Wel et al. 2013) models, though with some key differences. We find that thermally-induced internal ice stream variability can cause very rapid grounding line migration even in the absence of retrograde bed slopes or external forcing. Activation waves propagate along the ice stream length and trigger periods of rapid grounding line migration. We compare the behavior of the grounding line due to internal ice stream variability to changes triggered externally at the grounding line such as the rapid disintegration of buttressing ice shelves. Implications for Heinrich events and the Marine Ice Sheet Instability are discussed.

  2. Greenland Ice Sheet flow response to runoff variability

    NASA Astrophysics Data System (ADS)

    Stevens, Laura A.; Behn, Mark D.; Das, Sarah B.; Joughin, Ian; Noël, Brice P. Y.; Broeke, Michiel R.; Herring, Thomas

    2016-11-01

    We use observations of ice sheet surface motion from a Global Positioning System network operating from 2006 to 2014 around North Lake in west Greenland to investigate the dynamical response of the Greenland Ice Sheet's ablation area to interannual variability in surface melting. We find no statistically significant relationship between runoff season characteristics and ice flow velocities within a given year or season. Over the 7 year time series, annual velocities at North Lake decrease at an average rate of -0.9 ± 1.1 m yr-2, consistent with the negative trend in annual velocities observed in neighboring regions over recent decades. We find that net runoff integrated over several preceding years has a negative correlation with annual velocities, similar to findings from the two other available decadal records of ice velocity in western Greenland. However, we argue that this correlation is not necessarily evidence for a direct hydrologic mechanism acting on the timescale of multiple years but could be a statistical construct. Finally, we stress that neither the decadal slowdown trend nor the negative correlation between velocity and integrated runoff is predicted by current ice-sheet models, underscoring that these models do not yet capture all the relevant feedbacks between runoff and ice dynamics needed to predict long-term trends in ice sheet flow.

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

    NASA Astrophysics Data System (ADS)

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

    2016-08-01

    Sea ice variability within the marginal ice zone (MIZ) and polynyas plays an important role for phytoplankton productivity and krill abundance. Therefore, mapping their spatial extent as well as seasonal and interannual variability is essential for understanding how current and future changes in these biologically active regions may impact the Antarctic marine ecosystem. Knowledge of the distribution of MIZ, consolidated pack ice and coastal polynyas in the total Antarctic sea ice cover may also help to shed light on the factors contributing towards recent expansion of the Antarctic ice cover in some regions and contraction in others. The long-term passive microwave satellite data record provides the longest and most consistent record for assessing the proportion of the sea ice cover that is covered by each of these ice categories. However, estimates of the amount of MIZ, consolidated pack ice and polynyas depend strongly on which sea ice algorithm is used. This study uses two popular passive microwave sea ice algorithms, the NASA Team and Bootstrap, and applies the same thresholds to the sea ice concentrations to evaluate the distribution and variability in the MIZ, the consolidated pack ice and coastal polynyas. Results reveal that the seasonal cycle in the MIZ and pack ice is generally similar between both algorithms, yet the NASA Team algorithm has on average twice the MIZ and half the consolidated pack ice area as the Bootstrap algorithm. Trends also differ, with the Bootstrap algorithm suggesting statistically significant trends towards increased pack ice area and no statistically significant trends in the MIZ. The NASA Team algorithm on the other hand indicates statistically significant positive trends in the MIZ during spring. Potential coastal polynya area and amount of broken ice within the consolidated ice pack are also larger in the NASA Team algorithm. The timing of maximum polynya area may differ by as much as 5 months between algorithms. These

  4. Ice Ih anomalies: Thermal contraction, anomalous volume isotope effect, and pressure-induced amorphization

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

    Salim, Michael A.; Willow, Soohaeng Yoo; Hirata, So, E-mail: sohirata@illinois.edu

    Ice Ih displays several anomalous thermodynamic properties such as thermal contraction at low temperatures, an anomalous volume isotope effect (VIE) rendering the volume of D{sub 2}O ice greater than that of H{sub 2}O ice, and a pressure-induced transition to the high-density amorphous (HDA) phase. Furthermore, the anomalous VIE increases with temperature, despite its quantum-mechanical origin. Here, embedded-fragment ab initio second-order many-body perturbation (MP2) theory in the quasiharmonic approximation (QHA) is applied to the Gibbs energy of an infinite, proton-disordered crystal of ice Ih at wide ranges of temperatures and pressures. The quantum effect of nuclei moving in anharmonic potentials ismore » taken into account from first principles without any empirical or nonsystematic approximation to either the electronic or vibrational Hamiltonian. MP2 predicts quantitatively correctly the thermal contraction at low temperatures, which is confirmed to originate from the volume-contracting hydrogen-bond bending modes (acoustic phonons). It qualitatively reproduces (but underestimates) the thermal expansion at higher temperatures, caused by the volume-expanding hydrogen-bond stretching (and to a lesser extent librational) modes. The anomalous VIE is found to be the result of subtle cancellations among closely competing isotope effects on volume from all modes. Consequently, even ab initio MP2 with the aug-cc-pVDZ and aug-cc-pVTZ basis sets has difficulty reproducing this anomaly, yielding qualitatively varied predictions of the sign of the VIE depending on such computational details as the choice of the embedding field. However, the temperature growth of the anomalous VIE is reproduced robustly and is ascribed to the librational modes. These solid-state MP2 calculations, as well as MP2 Born–Oppenheimer molecular dynamics, find a volume collapse and a loss of symmetry and long-range order in ice Ih upon pressure loading of 2.35 GPa or higher. Concomitantly

  5. Volume Ice Radiolysis in the Outer Solar System

    NASA Technical Reports Server (NTRS)

    Cooper, John F.; Cooper, Paul D.

    2006-01-01

    The primary energy flux of charged particle components of the heliospheric and magnetospheric environments of the solar system is primarily carried by highly penetrating energetic particles. Although laboratory experiments on production of organics and oxidants typically only address effects on very thin surface layers, energy deposition occurs on surfaces of icy bodies of the outer solar system to meters in depth. Time scales for significant radiolytic deposition vary from thousands of years at millimeter depths on Europa to billions of years in the meters-deep regolith of Kuiper Belt Objects. Radioisotope decay (e.g., K-40) also contributes to volume radiolysis as the only energy source at much greater depths. Radiolytic oxygen is a potential resource for life within Europa and a partial source of oxygen for Saturn's magnetosphere and Titan's upper atmosphere. Interactions of very high energy cosmic rays with ices at Titan's surface may provide one of the few sources of oxidants in that highly reducing environment. The red colors of low-inclination classical Kuiper Belt Objects at 40-50 AU, and Centaur objects originating from this same population, may arise from volume radiolysis of deep ice layers below more refractory radiation crusts eroded away by surface sputtering and micrometeoroid impacts. A variety of techniques are potentially available to measure volume radiolysis products and have been proposed for study as part of the new Space Physics of Life initiative at NASA Goddard Space Flight Center. The technique of Electron Paramagnetic Resonance (EPR) has been used in medical studies to measure oxidant production in irradiated human tissue for cancer treatment. Other potential techniques include optical absorption spectroscopy and standard wet chemical analysis. These and other potential techniques are briefly reviewed for applicability to problems in solar system ice radiolysis and astrobiology.

  6. Arctic ice shelves and ice islands: Origin, growth and disintegration, physical characteristics, structural-stratigraphic variability, and dynamics

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

    Jeffries, M.O.

    1992-08-01

    Ice shelves are thick, floating ice masses most often associated with Antarctica where they are seaward extensions of the grounded Antarctic ice sheet and sources of many icebergs. However, there are also ice shelves in the Arctic, primarily located along the north coast of Ellesmere Island in the Canadian High Arctic. The only ice shelves in North America and the most extensive in the north polar region, the Ellesmere ice shelves originate from glaciers and from sea ice and are the source of ice islands, the tabular icebergs of the Arctic Ocean. The present state of knowledge and understanding ofmore » these ice features is summarized in this paper. It includes historical background to the discovery and early study of ice shelves and ice islands, including the use of ice islands as floating laboratories for polar geophysical research. Growth mechanisms and age, the former extent and the twentieth century disintegration of the Ellesmere ice shelves, and the processes and mechanisms of ice island calving are summarized. Surface features, thickness, thermal regime, and the size, shape, and numbers of ice islands are discussed. The structural-stratigraphic variability of ice islands and ice shelves and the complex nature of their growth and development are described. Large-scale and small-scale dynamics of ice 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

  7. Determination of Arctic sea ice variability modes on interannual timescales via nonhierarchical clustering

    NASA Astrophysics Data System (ADS)

    Fučkar, Neven-Stjepan; Guemas, Virginie; Massonnet, François; Doblas-Reyes, Francisco

    2015-04-01

    Over the modern observational era, the northern hemisphere sea ice concentration, age and thickness have experienced a sharp long-term decline superimposed with strong internal variability. Hence, there is a crucial need to identify robust patterns of Arctic sea ice variability on interannual timescales and disentangle them from the long-term trend in noisy datasets. The principal component analysis (PCA) is a versatile and broadly used method for the study of climate variability. However, the PCA has several limiting aspects because it assumes that all modes of variability have symmetry between positive and negative phases, and suppresses nonlinearities by using a linear covariance matrix. Clustering methods offer an alternative set of dimension reduction tools that are more robust and capable of taking into account possible nonlinear characteristics of a climate field. Cluster analysis aggregates data into groups or clusters based on their distance, to simultaneously minimize the distance between data points in a given cluster and maximize the distance between the centers of the clusters. We extract modes of Arctic interannual sea-ice variability with nonhierarchical K-means cluster analysis and investigate the mechanisms leading to these modes. Our focus is on the sea ice thickness (SIT) as the base variable for clustering because SIT holds most of the climate memory for variability and predictability on interannual timescales. We primarily use global reconstructions of sea ice fields with a state-of-the-art ocean-sea-ice model, but we also verify the robustness of determined clusters in other Arctic sea ice datasets. Applied cluster analysis over the 1958-2013 period shows that the optimal number of detrended SIT clusters is K=3. Determined SIT cluster patterns and their time series of occurrence are rather similar between different seasons and months. Two opposite thermodynamic modes are characterized with prevailing negative or positive SIT anomalies over the

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

    NASA Astrophysics Data System (ADS)

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

    2009-01-01

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

  9. Dynamic Antarctic ice sheet during the early to mid-Miocene

    PubMed Central

    DeConto, Robert M.; Pollard, David; Levy, Richard H.

    2016-01-01

    Geological data indicate that there were major variations in Antarctic ice sheet volume and extent during the early to mid-Miocene. Simulating such large-scale changes is problematic because of a strong hysteresis effect, which results in stability once the ice sheets have reached continental size. A relatively narrow range of atmospheric CO2 concentrations indicated by proxy records exacerbates this problem. Here, we are able to simulate large-scale variability of the early to mid-Miocene Antarctic ice sheet because of three developments in our modeling approach. (i) We use a climate–ice sheet coupling method utilizing a high-resolution atmospheric component to account for ice sheet–climate feedbacks. (ii) The ice sheet model includes recently proposed mechanisms for retreat into deep subglacial basins caused by ice-cliff failure and ice-shelf hydrofracture. (iii) We account for changes in the oxygen isotopic composition of the ice sheet by using isotope-enabled climate and ice sheet models. We compare our modeling results with ice-proximal records emerging from a sedimentological drill core from the Ross Sea (Andrill-2A) that is presented in a companion article. The variability in Antarctic ice volume that we simulate is equivalent to a seawater oxygen isotope signal of 0.52–0.66‰, or a sea level equivalent change of 30–36 m, for a range of atmospheric CO2 between 280 and 500 ppm and a changing astronomical configuration. This result represents a substantial advance in resolving the long-standing model data conflict of Miocene Antarctic ice sheet and sea level variability. PMID:26903645

  10. Forward Modeling of Oxygen Isotope Variability in Tropical Andean Ice Cores

    NASA Astrophysics Data System (ADS)

    Vuille, M. F.; Hurley, J. V.; Hardy, D. R.

    2016-12-01

    Ice core records from the tropical Andes serve as important archives of past tropical Pacific SST variability and changes in monsoon intensity upstream over the Amazon basin. Yet the interpretation of the oxygen isotopic signal in these ice cores remains controversial. Based on 10 years of continuous on-site glaciologic, meteorologic and isotopic measurements at the summit of the world's largest tropical ice cap, Quelccaya, in southern Peru, we developed a process-based physical forward model (proxy system model), capable of simulating intraseasonal, seasonal and interannual variability in delta-18O as observed in snow pits and short cores. Our results highlight the importance of taking into account post-depositional effects (sublimation and isotopic enrichment) to properly simulate the seasonal cycle. Intraseasonal variability is underestimated in our model unless the effects of cold air incursions, triggering significant monsoonal snowfall and more negative delta-18O values, are included. A number of sensitivity test highlight the influence of changing boundary conditions on the final snow isotopic profile. Such tests also show that our model provides much more realistic data than applying direct model output of precipitation delta-18O from isotope-enabled climate models (SWING ensemble). The forward model was calibrated with and run under present-day conditions, but it can also be driven with past climate forcings to reconstruct paleo-monsoon variability and investigate the influence of changes in radiative forcings (solar, volcanic) on delta-18O variability in Andean snow. The model is transferable and may be used to render a paleoclimatic context at other ice core locations.

  11. Aircraft Icing Handbook. Volume 2

    DTIC Science & Technology

    1991-03-01

    an airfoil surface. icenhobig - A surface property exhibiting a reduced adhesion to ice; literally, "ice-hating." light icing - The rate of...power, and are a light weight system of reasonable cost. K. ill I-I1 1.I.2 Pneumatic Impulse Ice Protection A Pneumatic Impulse Ice Protection System...should be about 5 to 6 seconds. During moderate icing a 60 second cycle is suggested, while for light icing, longer accretion times of 3 to 4 minutes

  12. Understanding Cirrus Ice Crystal Number Variability for Different Heterogeneous Ice Nucleation Spectra

    NASA Technical Reports Server (NTRS)

    Sullivan, Sylvia C.; Betancourt, Ricardo Morales; Barahona, Donifan; Nenes, Athanasios

    2016-01-01

    Along with minimizing parameter uncertainty, understanding the cause of temporal and spatial variability of the nucleated ice crystal number, Ni, is key to improving the representation of cirrus clouds in climate models. To this end, sensitivities of Ni to input variables like aerosol number and diameter provide valuable information about nucleation regime and efficiency for a given model formulation. Here we use the adjoint model of the adjoint of a cirrus formation parameterization (Barahona and Nenes, 2009b) to understand Ni variability for various ice-nucleating particle (INP) spectra. Inputs are generated with the Community Atmosphere Model version 5, and simulations are done with a theoretically derived spectrum, an empirical lab-based spectrum and two field-based empirical spectra that differ in the nucleation threshold for black carbon particles and in the active site density for dust. The magnitude and sign of Ni sensitivity to insoluble aerosol number can be directly linked to nucleation regime and efficiency of various INP. The lab-based spectrum calculates much higher INP efficiencies than field-based ones, which reveals a disparity in aerosol surface properties. Ni sensitivity to temperature tends to be low, due to the compensating effects of temperature on INP spectrum parameters; this low temperature sensitivity regime has been experimentally reported before but never deconstructed as done here.

  13. Understanding cirrus ice crystal number variability for different heterogeneous ice nucleation spectra

    DOE PAGES

    Sullivan, Sylvia C.; Morales Betancourt, Ricardo; Barahona, Donifan; ...

    2016-03-03

    Along with minimizing parameter uncertainty, understanding the cause of temporal and spatial variability of the nucleated ice crystal number, N i, is key to improving the representation of cirrus clouds in climate models. To this end, sensitivities of N i to input variables like aerosol number and diameter provide valuable information about nucleation regime and efficiency for a given model formulation. Here we use the adjoint model of the adjoint of a cirrus formation parameterization (Barahona and Nenes, 2009b) to understand N i variability for various ice-nucleating particle (INP) spectra. Inputs are generated with the Community Atmosphere Model version 5, andmore » simulations are done with a theoretically derived spectrum, an empirical lab-based spectrum and two field-based empirical spectra that differ in the nucleation threshold for black carbon particles and in the active site density for dust. The magnitude and sign of N i sensitivity to insoluble aerosol number can be directly linked to nucleation regime and efficiency of various INP. The lab-based spectrum calculates much higher INP efficiencies than field-based ones, which reveals a disparity in aerosol surface properties. In conclusion, N i sensitivity to temperature tends to be low, due to the compensating effects of temperature on INP spectrum parameters; this low temperature sensitivity regime has been experimentally reported before but never deconstructed as done here.« less

  14. The Arctic's sea ice cover: trends, variability, predictability, and comparisons to the Antarctic.

    PubMed

    Serreze, Mark C; Meier, Walter N

    2018-05-28

    As assessed over the period of satellite observations, October 1978 to present, there are downward linear trends in Arctic sea ice extent for all months, largest at the end of the melt season in September. The ice cover is also thinning. Downward trends in extent and thickness have been accompanied by pronounced interannual and multiyear variability, forced by both the atmosphere and ocean. As the ice thins, its response to atmospheric and oceanic forcing may be changing. In support of a busier Arctic, there is a growing need to predict ice conditions on a variety of time and space scales. A major challenge to providing seasonal scale predictions is the 7-10 days limit of numerical weather prediction. While a seasonally ice-free Arctic Ocean is likely well within this century, there is much uncertainty in the timing. This reflects differences in climate model structure, the unknown evolution of anthropogenic forcing, and natural climate variability. In sharp contrast to the Arctic, Antarctic sea ice extent, while highly variable, has increased slightly over the period of satellite observations. The reasons for this different behavior remain to be resolved, but responses to changing atmospheric circulation patterns appear to play a strong role. © 2018 New York Academy of Sciences.

  15. Arctic sea ice variability during the last deglaciation: a biomarker approach

    NASA Astrophysics Data System (ADS)

    Müller, J.; Stein, R. H.

    2014-12-01

    The last transition from full glacial to current interglacial conditions was accompanied by distinct short-term climate fluctuations caused by changes in the global ocean circulation system. Most palaeoceanographic studies focus on the documentation of the behaviour of the Atlantic Meridional Overturning Circulation (AMOC) during the last deglaciation in response to freshwater forcing events. In this respect, the role of Arctic sea ice remained relatively unconsidered - primarily because of the difficulty of its reconstruction. Here we present new proxy data on late glacial (including the Last Glacial Maximum; LGM) and deglacial sea ice variability in the Arctic Ocean and its main gateway - the Fram Strait - and how these changes in sea ice coverage contributed to AMOC perturbations observed during Heinrich Event 1 and the Younger Dryas. Recurrent short-term advances and retreats of sea ice in Fram Strait, prior and during the LGM, are in line with a variable (or intermittent) North Atlantic heat flow along the eastern corridor of the Nordic Seas. Possibly in direct response to the initial freshwater discharge from melting continental ice-sheets, a permanent sea ice cover established only at about 19 ka BP (i.e. post-LGM) and lasted until 17.6 ka BP, when an abrupt break-up of this thick ice cover and a sudden discharge of huge amounts of sea ice and icebergs through Fram Strait coincided with the weakening of the AMOC during Heinrich Event 1. Similarly, another sea ice maximum at about 12.8 ka BP is associated with the slowdown of the AMOC during the Younger Dryas. The new data sets clearly highlight the important role of Arctic sea ice for the re-organisation of the oceanographic setting in the North Atlantic during the last deglaciation. Further studies and sensitivity experiments to identify crucial driving (and feedback) mechanisms within the High Latitude ice-ocean-atmosphere system will contribute the understanding of rapid climate changes.

  16. Improved parameterization of marine ice dynamics and flow instabilities for simulation of the Austfonna ice cap using a large-scale ice sheet model

    NASA Astrophysics Data System (ADS)

    Dunse, T.; Greve, R.; Schuler, T.; Hagen, J. M.; Navarro, F.; Vasilenko, E.; Reijmer, C.

    2009-12-01

    The Austfonna ice cap covers an area of 8120 km2 and is by far the largest glacier on Svalbard. Almost 30% of the entire area is grounded below sea-level, while the figure is as large as 57% for the known surge-type basins in particular. Marine ice dynamics, as well as flow instabilities presumably control flow regime, form and evolution of Austfonna. These issues are our focus in numerical simulations of the ice cap. We employ the thermodynamic, large-scale ice sheet model SICOPOLIS (http://sicopolis.greveweb.net/) which is based on the shallow-ice approximation. We present improved parameterizations of (a) the marine extent and calving and (b) processes that may initiate flow instabilities such as switches from cold to temperate basal conditions, surface steepening and hence, increases in driving stress, enhanced sliding or deformation of unconsolidated marine sediments and diminishing ice thicknesses towards flotation thickness. Space-borne interferometric snapshots of Austfonna revealed a velocity structure of a slow moving polar ice cap (< 10m/a) interrupted by distinct fast flow units with velocities in excess of 100m/a. However, observations of flow variability are scarce. In spring 2008, we established a series of stakes along the centrelines of two fast-flowing units. Repeated DGPS and continuous GPS measurements of the stake positions give insight in the temporal flow variability of these units and provide constrains to the modeled surface velocity field. Austfonna’s thermal structure is described as polythermal. However, direct measurements of the temperature distribution is available only from one single borehole at the summit area. The vertical temperature profile shows that the bulk of the 567m thick ice column is cold, only underlain by a thin temperate basal layer of approximately 20m. To acquire a spatially extended picture of the thermal structure (and bed topography), we used low-frequency (20 MHz) GPR profiling across the ice cap and the

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

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

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

  18. Observations of Recent Arctic Sea Ice Volume Loss and Its Impact on Ocean-Atmosphere Energy Exchange and Ice Production

    NASA Technical Reports Server (NTRS)

    Kurtz, N. T.; Markus, T.; Farrell, S. L.; Worthen, D. L.; Boisvert, L. N.

    2011-01-01

    Using recently developed techniques we estimate snow and sea ice thickness distributions for the Arctic basin through the combination of freeboard data from the Ice, Cloud, and land Elevation Satellite (ICESat) and a snow depth model. These data are used with meteorological data and a thermodynamic sea ice model to calculate ocean-atmosphere heat exchange and ice volume production during the 2003-2008 fall and winter seasons. The calculated heat fluxes and ice growth rates are in agreement with previous observations over multiyear ice. In this study, we calculate heat fluxes and ice growth rates for the full distribution of ice thicknesses covering the Arctic basin and determine the impact of ice thickness change on the calculated values. Thinning of the sea ice is observed which greatly increases the 2005-2007 fall period ocean-atmosphere heat fluxes compared to those observed in 2003. Although there was also a decline in sea ice thickness for the winter periods, the winter time heat flux was found to be less impacted by the observed changes in ice thickness. A large increase in the net Arctic ocean-atmosphere heat output is also observed in the fall periods due to changes in the areal coverage of sea ice. The anomalously low sea ice coverage in 2007 led to a net ocean-atmosphere heat output approximately 3 times greater than was observed in previous years and suggests that sea ice losses are now playing a role in increasing surface air temperatures in the Arctic.

  19. A combined surface/volume scattering retracking algorithm for ice sheet satellite altimetry

    NASA Technical Reports Server (NTRS)

    Davis, Curt H.

    1992-01-01

    An algorithm that is based upon a combined surface-volume scattering model is developed. It can be used to retrack individual altimeter waveforms over ice sheets. An iterative least-squares procedure is used to fit the combined model to the return waveforms. The retracking algorithm comprises two distinct sections. The first generates initial model parameter estimates from a filtered altimeter waveform. The second uses the initial estimates, the theoretical model, and the waveform data to generate corrected parameter estimates. This retracking algorithm can be used to assess the accuracy of elevations produced from current retracking algorithms when subsurface volume scattering is present. This is extremely important so that repeated altimeter elevation measurements can be used to accurately detect changes in the mass balance of the ice sheets. By analyzing the distribution of the model parameters over large portions of the ice sheet, regional and seasonal variations in the near-surface properties of the snowpack can be quantified.

  20. Interannual Variability in Amundsen Sea Ice-Shelf Height Change Linked to ENSO

    NASA Astrophysics Data System (ADS)

    Paolo, F. S.; Fricker, H. A.; Padman, L.

    2015-12-01

    Atmospheric and sea-ice conditions around Antarctica, particularly in the Amundsen and Bellingshausen seas, respond to climate dynamics in the tropical Pacific Ocean on interannual time scales including the El Nino-Southern Oscillation (ENSO). It has been hypothesized that the mass balance of the Antarctic Ice Sheet, including its floating ice shelves, also responds to this climate signal; however, this has not yet been unambiguously demonstrated. We apply multivariate singular spectrum analysis (MSSA) to our 18-year (1994-2012) time series of ice-shelf height in the Amundsen Sea (AS) region. This advanced spectral method distinguishes between regular deterministic behavior ("cycles") at sub-decadal time scale and irregular behavior ("noise") at shorter time scales. Although the long-term trends of AS ice-shelf height changes are much larger than the range of interannual variability, the short-term rate of change dh/dt can vary about the trend by more than 50%. The mode of interannual variability in the AS ice-shelf height is strongly correlated with the low-frequency mode of ENSO (periodicity of ~4.5 years) as represented by the Southern Oscillation Index. The ice-shelf height in the AS is expected to respond to changes in precipitation and inflows of warm subsurface Circumpolar Deep Water (CDW) into the ocean cavities under the ice shelves, altering basal melt rates. Since both of these processes affecting ice-shelf mass balance respond to changes in wind fields for different ENSO states, we expect some correlation between them. We will describe the spatial structure of AS ice-shelf height response to ENSO, and attempt to distinguish the precipitation signal from basal mass balance due to changing CDW inflows.

  1. RICE ice core: Black Carbon reflects climate variability at Roosevelt Island, West Antarctica

    NASA Astrophysics Data System (ADS)

    Ellis, Aja; Edwards, Ross; Bertler, Nancy; Winton, Holly; Goodwin, Ian; Neff, Peter; Tuohy, Andrea; Proemse, Bernadette; Hogan, Chad; Feiteng, Wang

    2015-04-01

    The Roosevelt Island Climate Evolution (RICE) project successfully drilled a deep ice core from Roosevelt Island during the 2011/2012 and 2012/2013 seasons. Located in the Ross Ice Shelf in West Antarctica, the site is an ideal location for investigating climate variability and the past stability of the Ross Ice Shelf. Black carbon (BC) aerosols are emitted by both biomass burning and fossil fuels, and BC particles emitted in the southern hemisphere are transported in the atmosphere and preserved in Antarctic ice. The past record of BC is expected to be sensitive to climate variability, as it is modulated by both emissions and transport. To investigate BC variability over the past 200 years, we developed a BC record from two overlapping ice cores (~1850-2012) and a high-resolution snow pit spanning 2010-2012 (cal. yr). Consistent results are found between the snow pit profiles and ice core records. Distinct decadal trends are found with respect to BC particle size, and the record indicates a steady rise in BC particle size over the last 100 years. Differences in emission sources and conditions may be a possible explanation for changes in BC size. These records also show a significant increase in BC concentration over the past decade with concentrations rising over 1.5 ppb (1.5*10^-9 ng/g), suggesting a fundamental shift in BC deposition to the site.

  2. Variability and Trends in the Arctic Sea Ice Cover: Results from Different Techniques

    NASA Technical Reports Server (NTRS)

    Comiso, Josefino C.; Meier, Walter N.; Gersten, Robert

    2017-01-01

    Variability and trend studies of sea ice in the Arctic have been conducted using products derived from the same raw passive microwave data but by different groups using different algorithms. This study provides consistency assessment of four of the leading products, namely, Goddard Bootstrap (SB2), Goddard NASA Team (NT1), EUMETSAT Ocean and Sea Ice Satellite Application Facility (OSI-SAF 1.2), and Hadley HadISST 2.2 data in evaluating variability and trends in the Arctic sea ice cover. All four provide generally similar ice patterns but significant disagreements in ice concentration distributions especially in the marginal ice zone and adjacent regions in winter and meltponded areas in summer. The discrepancies are primarily due to different ways the four techniques account for occurrences of new ice and meltponding. However, results show that the different products generally provide consistent and similar representation of the state of the Arctic sea ice cover. Hadley and NT1 data usually provide the highest and lowest monthly ice extents, respectively. The Hadley data also show the lowest trends in ice extent and ice area at negative 3.88 percent decade and negative 4.37 percent decade, respectively, compared to an average of negative 4.36 percent decade and negative 4.57 percent decade for all four. Trend maps also show similar spatial distribution for all four with the largest negative trends occurring at the Kara/Barents Sea and Beaufort Sea regions, where sea ice has been retreating the fastest. The good agreement of the trends especially with updated data provides strong confidence in the quantification of the rate of decline in the Arctic sea ice cover.

  3. Strong sensitivity of Pine Island ice-shelf melting to climatic variability.

    PubMed

    Dutrieux, Pierre; De Rydt, Jan; Jenkins, Adrian; Holland, Paul R; Ha, Ho Kyung; Lee, Sang Hoon; Steig, Eric J; Ding, Qinghua; Abrahamsen, E Povl; Schröder, Michael

    2014-01-10

    Pine Island Glacier has thinned and accelerated over recent decades, significantly contributing to global sea-level rise. Increased oceanic melting of its ice shelf is thought to have triggered those changes. Observations and numerical modeling reveal large fluctuations in the ocean heat available in the adjacent bay and enhanced sensitivity of ice-shelf melting to water temperatures at intermediate depth, as a seabed ridge blocks the deepest and warmest waters from reaching the thickest ice. Oceanic melting decreased by 50% between January 2010 and 2012, with ocean conditions in 2012 partly attributable to atmospheric forcing associated with a strong La Niña event. Both atmospheric variability and local ice shelf and seabed geometry play fundamental roles in determining the response of the Antarctic Ice Sheet to climate.

  4. Reconciliation of Antarctic marine and terrestrial geologic records: climate and ice-sheet variability in the mid-Miocene

    NASA Astrophysics Data System (ADS)

    Halberstadt, A. R. W.; DeConto, R.; Gasson, E.; Kowalewski, D. E.; Levy, R. H.; Naish, T.; Chorley, H.

    2017-12-01

    summer orbit, and an ice sheet 53% of its modern volume). Model results will be compared with emerging terrestrial data from the Friis Hills in the MDVs, to test the hypothesis that climate in the MDVs remained relatively cold and insensitive to a highly variable West Antarctic Ice Sheet and marine conditions in the proximal Ross Sea.

  5. Interannual variability of high ice cloud properties over the tropics

    NASA Astrophysics Data System (ADS)

    Tamura, S.; Iwabuchi, H.

    2015-12-01

    The El Niño/Southern Oscillation (ENSO) affects atmospheric conditions and cloud physical properties such as cloud fraction (CF) and cloud top height (CTH). However, an impact of the ENSO on physical properties in high-ice cloud is not well known. Therefore, this study attempts to reveal relationship between variability of ice cloud physical properties and ENSO. Ice clouds are inferred with the multiband IR method in this study. Ice clouds are categorized in terms of cloud optical thickness (COT) as thin (0.1< COT <0.3), opaque (0.3< COT <3.6), thick (3.6< COT <11), and deep convective (DC) (11< COT) clouds, and relationship between ENSO and interannual variability of cloud physical properties is investigated for each category during the period from January 2003 to December 2014. The deseasonalized anomalies of CF and CTH in all categories correlate well with Niño3.4 index, with positive anomaly over the eastern Pacific and negative anomaly over the western Pacific during El Niño condition. However, the global distribution of these correlation coefficients is different by cloud categories. For example, CF of DC correlates well with Niño3.4 index over the convergence zone, while, that of thin cloud shows high correlation extending to high latitude from convergence zone, suggesting a connection with cloud formation. The global distributions of average rate of change differ by cloud category, because the different associate with ENSO and gradual trend toward La Niña condition had occurred over the analysis period. In this conference, detailed results and relationship between variability of cloud physical properties and atmospheric conditions will be shown.

  6. Change and variability in East antarctic sea ice seasonality, 1979/80-2009/10.

    PubMed

    Massom, Robert; Reid, Philip; Stammerjohn, Sharon; Raymond, Ben; Fraser, Alexander; Ushio, Shuki

    2013-01-01

    Recent analyses have shown that significant changes have occurred in patterns of sea ice seasonality in West Antarctica since 1979, with wide-ranging climatic, biological and biogeochemical consequences. Here, we provide the first detailed report on long-term change and variability in annual timings of sea ice advance, retreat and resultant ice season duration in East Antarctica. These were calculated from satellite-derived ice concentration data for the period 1979/80 to 2009/10. The pattern of change in sea ice seasonality off East Antarctica comprises mixed signals on regional to local scales, with pockets of strongly positive and negative trends occurring in near juxtaposition in certain regions e.g., Prydz Bay. This pattern strongly reflects change and variability in different elements of the marine "icescape", including fast ice, polynyas and the marginal ice zone. A trend towards shorter sea-ice duration (of 1 to 3 days per annum) occurs in fairly isolated pockets in the outer pack from∼95-110°E, and in various near-coastal areas that include an area of particularly strong and persistent change near Australia's Davis Station and between the Amery and West Ice Shelves. These areas are largely associated with coastal polynyas that are important as sites of enhanced sea ice production/melt. Areas of positive trend in ice season duration are more extensive, and include an extensive zone from 160-170°E (i.e., the western Ross Sea sector) and the near-coastal zone between 40-100°E. The East Antarctic pattern is considerably more complex than the well-documented trends in West Antarctica e.g., in the Antarctic Peninsula-Bellingshausen Sea and western Ross Sea sectors.

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

    NASA Astrophysics Data System (ADS)

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

    2016-04-01

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

  8. Variability in sea ice cover and climate elicit sex specific responses in an Antarctic predator

    PubMed Central

    Labrousse, Sara; Sallée, Jean-Baptiste; Fraser, Alexander D.; Massom, Rob A.; Reid, Phillip; Hobbs, William; Guinet, Christophe; Harcourt, Robert; McMahon, Clive; Authier, Matthieu; Bailleul, Frédéric; Hindell, Mark A.; Charrassin, Jean-Benoit

    2017-01-01

    Contrasting regional changes in Southern Ocean sea ice have occurred over the last 30 years with distinct regional effects on ecosystem structure and function. Quantifying how Antarctic predators respond to such changes provides the context for predicting how climate variability/change will affect these assemblages into the future. Over an 11-year time-series, we examine how inter-annual variability in sea ice concentration and advance affect the foraging behaviour of a top Antarctic predator, the southern elephant seal. Females foraged longer in pack ice in years with greatest sea ice concentration and earliest sea ice advance, while males foraged longer in polynyas in years of lowest sea ice concentration. There was a positive relationship between near-surface meridional wind anomalies and female foraging effort, but not for males. This study reveals the complexities of foraging responses to climate forcing by a poleward migratory predator through varying sea ice property and dynamic anomalies. PMID:28233791

  9. Variability in sea ice cover and climate elicit sex specific responses in an Antarctic predator.

    PubMed

    Labrousse, Sara; Sallée, Jean-Baptiste; Fraser, Alexander D; Massom, Rob A; Reid, Phillip; Hobbs, William; Guinet, Christophe; Harcourt, Robert; McMahon, Clive; Authier, Matthieu; Bailleul, Frédéric; Hindell, Mark A; Charrassin, Jean-Benoit

    2017-02-24

    Contrasting regional changes in Southern Ocean sea ice have occurred over the last 30 years with distinct regional effects on ecosystem structure and function. Quantifying how Antarctic predators respond to such changes provides the context for predicting how climate variability/change will affect these assemblages into the future. Over an 11-year time-series, we examine how inter-annual variability in sea ice concentration and advance affect the foraging behaviour of a top Antarctic predator, the southern elephant seal. Females foraged longer in pack ice in years with greatest sea ice concentration and earliest sea ice advance, while males foraged longer in polynyas in years of lowest sea ice concentration. There was a positive relationship between near-surface meridional wind anomalies and female foraging effort, but not for males. This study reveals the complexities of foraging responses to climate forcing by a poleward migratory predator through varying sea ice property and dynamic anomalies.

  10. Extreme events, trends, and variability in Northern Hemisphere lake-ice phenology (1855-2005)

    USGS Publications Warehouse

    Benson, Barbara J.; Magnuson, John J.; Jensen, Olaf P.; Card, Virginia M.; Hodgkins, Glenn; Korhonen, Johanna; Livingstone, David M.; Stewart, Kenton M.; Weyhenmeyer, Gesa A.; Granin, Nick G.

    2012-01-01

    Often extreme events, more than changes in mean conditions, have the greatest impact on the environment and human well-being. Here we examine changes in the occurrence of extremes in the timing of the annual formation and disappearance of lake ice in the Northern Hemisphere. Both changes in the mean condition and in variability around the mean condition can alter the probability of extreme events. Using long-term ice phenology data covering two periods 1855–6 to 2004–5 and 1905–6 to 2004–5 for a total of 75 lakes, we examined patterns in long-term trends and variability in the context of understanding the occurrence of extreme events. We also examined patterns in trends for a 30-year subset (1975–6 to 2004–5) of the 100-year data set. Trends for ice variables in the recent 30-year period were steeper than those in the 100- and 150-year periods, and trends in the 150-year period were steeper than in the 100-year period. Ranges of rates of change (days per decade) among time periods based on linear regression were 0.3−1.6 later for freeze, 0.5−1.9 earlier for breakup, and 0.7−4.3 shorter for duration. Mostly, standard deviation did not change, or it decreased in the 150-year and 100-year periods. During the recent 50-year period, standard deviation calculated in 10-year windows increased for all ice measures. For the 150-year and 100-year periods changes in the mean ice dates rather than changes in variability most strongly influenced the significant increases in the frequency of extreme lake ice events associated with warmer conditions and decreases in the frequency of extreme events associated with cooler conditions.

  11. Molecular Markers in the Quelccaya Ice Cap, Peru Describe 20th Century Biomass Burning Variability

    NASA Astrophysics Data System (ADS)

    Makou, M. C.; Thompson, L. G.; Eglinton, T. I.; Montluçon, D. B.

    2007-12-01

    Organic geochemical analytical methods were applied to Andean ice core samples, resulting in a multi- molecular biomass burning record spanning 1915 to 2001 AD. The Quelccaya Ice Cap in Peru is situated on the eastern flank of the Andes at 14°S and is well situated to receive aeolian inputs of organic matter derived from Amazonian forest fire events. Compounds of interest, which occur in trace quantities in ice, were recovered by stir bar sorptive extraction and analyzed by gas chromatography/time-of-flight mass spectrometry coupled with thermal desorption. These methods permitted identification and quantitation of numerous biomarkers in sample volumes of as little as 10 ml. At least one wet and dry season sample was analyzed for every year. Observed biomarkers that may be derived from vegetation fires include several polycyclic aromatic hydrocarbons (PAHs), atraric acid, 2-ethylhexyl p-methoxycinnamate, and a range of other aromatic compounds. Abrupt changes in compound abundances were superimposed on decadal variability. Systematic offsets between wet and dry season abundances were not observed, suggesting that the biomass burning signal is not biased by seasonal depositional effects, such as dust delivery. Inputs likely reflect a combination of sources from anthropogenic burning of the Amazon rainforest as well as natural fires related to aridity, and include both high and low elevation vegetation. These compounds and techniques can be applied to older ice in this and other core locations as an independent estimate of aridity.

  12. Aircraft Icing Handbook. Volume 3

    DTIC Science & Technology

    1991-03-01

    Measurement," Harvard-Mt. Washington Icing Research Report, 1976-1947,L U. S. Air Materiel Command, Tech. Rept. No. 5676, 82. Findeisen , W...34Meteorological-Physical Limitations of Icing on the Atmosphere," NACA TM 885, 1939. 83. Findeisen , W., "Meteorological Commentary on D (air) 1209, Icing...November 1972, pp. 2603-2616. 58. Findeisen , W., "The Thermometric Ice Warning Indicator," (Translation) Project No. M992-B, University of Michigan

  13. Neogene ice volume and ocean temperatures: Insights from infaunal foraminiferal Mg/Ca paleothermometry

    NASA Astrophysics Data System (ADS)

    Lear, Caroline H.; Coxall, Helen K.; Foster, Gavin L.; Lunt, Daniel J.; Mawbey, Elaine M.; Rosenthal, Yair; Sosdian, Sindia M.; Thomas, Ellen; Wilson, Paul A.

    2015-11-01

    Antarctic continental-scale glaciation is generally assumed to have initiated at the Eocene-Oligocene Transition, yet its subsequent evolution is poorly constrained. We reconstruct changes in bottom water temperature and global ice volume from 0 to 17 Ma using δ18O in conjunction with Mg/Ca records of the infaunal benthic foraminifer, O. umbonatus from Ocean Drilling Program (ODP) Site 806 (equatorial Pacific; ~2500 m). Considering uncertainties in core top calibrations and sensitivity to seawater Mg/Ca (Mg/Ca)sw, we produce a range of Mg/Ca-temperature-Mg/Casw calibrations. Our favored exponential temperature calibration is Mg/Ca = 0.66 ± 0.08 × Mg/Casw0.27±0.06 × e(0.114±0.02 × BWT) and our favored linear temperature calibration is Mg/Ca = (1.21 ± 0.04 + 0.12 ± 0.004 × BWT (bottom water temperature)) × (Mg/Casw-0.003±0.02) (stated errors are 2 s.e.). The equations are obtained by comparing O. umbonatus Mg/Ca for a Paleocene-Eocene section from Ocean Drilling Program (ODP) Site 690 (Weddell Sea) to δ18O temperatures, calculated assuming ice-free conditions during this peak warmth period of the Cenozoic. This procedure suggests negligible effect of Mg/Casw on the Mg distribution coefficient (DMg). Application of the new equations to the Site 806 record leads to the suggestion that global ice volume was greater than today after the Middle Miocene Climate Transition (~14 Ma). ODP Site 806 bottom waters cooled and freshened as the Pacific zonal sea surface temperature gradient increased, and climate cooled through the Pliocene, prior to the Plio-Pleistocene glaciation of the Northern Hemisphere. The records indicate a decoupling of deep water temperatures and global ice volume, demonstrating the importance of thresholds in the evolution of the Antarctic ice sheet.

  14. Plume Activity and Tidal Deformation on Enceladus Influenced by Faults and Variable Ice Shell Thickness

    PubMed Central

    Souček, Ondřej; Hron, Jaroslav; Čadek, Ondřej

    2017-01-01

    Abstract We investigated the effect of variations in ice shell thickness and of the tiger stripe fractures crossing Enceladus' south polar terrain on the moon's tidal deformation by performing finite element calculations in three-dimensional geometry. The combination of thinning in the polar region and the presence of faults has a synergistic effect that leads to an increase of both the displacement and stress in the south polar terrain by an order of magnitude compared to that of the traditional model with a uniform shell thickness and without faults. Assuming a simplified conductive heat transfer and neglecting the heat sources below the ice shell, we computed the global heat budget of the ice shell. For the inelastic properties of the shell described by a Maxwell viscoelastic model, we show that unrealistically low average viscosity of the order of 1013 Pa s is necessary for preserving the volume of the ocean, suggesting the important role of the heat sources in the deep interior. Similarly, low viscosity is required to predict the observed delay of the plume activity, which hints at other delaying mechanisms than just the viscoelasticity of the ice shell. The presence of faults results in large spatial and temporal heterogeneity of geysering activity compared to the traditional models without faults. Our model contributes to understanding the physical mechanisms that control the fault activity, and it provides potentially useful information for future missions that will sample the plume for evidence of life. Key Words: Enceladus—Tidal deformation—Faults—Variable ice shell thickness—Tidal heating—Plume activity and timing. Astrobiology 17, 941–954. PMID:28816521

  15. Regional variability in sea ice melt in a changing Arctic

    PubMed Central

    Perovich, Donald K.; Richter-Menge, Jacqueline A.

    2015-01-01

    In recent years, the Arctic sea ice cover has undergone a precipitous decline in summer extent. The sea ice mass balance integrates heat and provides insight on atmospheric and oceanic forcing. The amount of surface melt and bottom melt that occurs during the summer melt season was measured at 41 sites over the time period 1957 to 2014. There are large regional and temporal variations in both surface and bottom melting. Combined surface and bottom melt ranged from 16 to 294 cm, with a mean of 101 cm. The mean ice equivalent surface melt was 48 cm and the mean bottom melt was 53 cm. On average, surface melting decreases moving northward from the Beaufort Sea towards the North Pole; however interannual differences in atmospheric forcing can overwhelm the influence of latitude. Substantial increases in bottom melting are a major contributor to ice losses in the Beaufort Sea, due to decreases in ice concentration. In the central Arctic, surface and bottom melting demonstrate interannual variability, but show no strong temporal trends from 2000 to 2014. This suggests that under current conditions, summer melting in the central Arctic is not large enough to completely remove the sea ice cover. PMID:26032323

  16. Regional variability in sea ice melt in a changing Arctic.

    PubMed

    Perovich, Donald K; Richter-Menge, Jacqueline A

    2015-07-13

    In recent years, the Arctic sea ice cover has undergone a precipitous decline in summer extent. The sea ice mass balance integrates heat and provides insight on atmospheric and oceanic forcing. The amount of surface melt and bottom melt that occurs during the summer melt season was measured at 41 sites over the time period 1957 to 2014. There are large regional and temporal variations in both surface and bottom melting. Combined surface and bottom melt ranged from 16 to 294 cm, with a mean of 101 cm. The mean ice equivalent surface melt was 48 cm and the mean bottom melt was 53 cm. On average, surface melting decreases moving northward from the Beaufort Sea towards the North Pole; however interannual differences in atmospheric forcing can overwhelm the influence of latitude. Substantial increases in bottom melting are a major contributor to ice losses in the Beaufort Sea, due to decreases in ice concentration. In the central Arctic, surface and bottom melting demonstrate interannual variability, but show no strong temporal trends from 2000 to 2014. This suggests that under current conditions, summer melting in the central Arctic is not large enough to completely remove the sea ice cover. © 2015 The Author(s) Published by the Royal Society. All rights reserved.

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

    PubMed

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

    2015-04-24

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

  18. Mechanisms of interannual- to decadal-scale winter Labrador Sea ice variability

    NASA Astrophysics Data System (ADS)

    Close, S.; Herbaut, C.; Houssais, M.-N.; Blaizot, A.-C.

    2017-12-01

    The variability of the winter sea ice cover of the Labrador Sea region and its links to atmospheric and oceanic forcing are investigated using observational data, a coupled ocean-sea ice model and a fully-coupled model simulation drawn from the CMIP5 archive. A consistent series of mechanisms associated with high sea ice cover are found amongst the various data sets. The highest values of sea ice area occur when the northern Labrador Sea is ice covered. This region is found to be primarily thermodynamically forced, contrasting with the dominance of mechanical forcing along the eastern coast of Baffin Island and Labrador, and the growth of sea ice is associated with anomalously fresh local ocean surface conditions. Positive fresh water anomalies are found to propagate to the region from a source area off the southeast Greenland coast with a 1 month transit time. These anomalies are associated with sea ice melt, driven by the enhanced offshore transport of sea ice in the source region, and its subsequent westward transport in the Irminger Current system. By combining sea ice transport through the Denmark Strait in the preceding autumn with the Greenland Blocking Index and the Atlantic Multidecadal Oscillation Index, strong correlation with the Labrador Sea ice area of the following winter is obtained. This relationship represents a dependence on the availability of sea ice to be melted in the source region, the necessary atmospheric forcing to transport this offshore, and a further multidecadal-scale link with the large-scale sea surface temperature conditions.

  19. Spatial and Temporal Variability of Surface Energy Fluxes During Autumn Ice Advance: Observations and Model Validation

    NASA Astrophysics Data System (ADS)

    Persson, O. P. G.; Blomquist, B.; Grachev, A. A.; Guest, P. S.; Stammerjohn, S. E.; Solomon, A.; Cox, C. J.; Capotondi, A.; Fairall, C. W.; Intrieri, J. M.

    2016-12-01

    From Oct 4 to Nov 5, 2015, the Office of Naval Research - sponsored Sea State cruise in the Beaufort Sea with the new National Science Foundation R/V Sikuliaq obtained extensive in-situ and remote sensing observations of the lower troposphere, the advancing sea ice, wave state, and upper ocean conditions. In addition, a coupled atmosphere, sea ice, upper-ocean model, based on the RASM model, was run at NOAA/PSD in a hindcast mode for this same time period, providing a 10-day simulation of the atmosphere/ice/ocean evolution. Surface energy fluxes quantitatively represent the air-ice, air-ocean, and ice-ocean interaction processes, determining the cooling (warming) rate of the upper ocean and the growth (melting) rate of sea ice. These fluxes also impact the stratification of the lower troposphere and the upper ocean. In this presentation, both direct and indirect measurements of the energy fluxes during Sea State will be used to explore the spatial and temporal variability of these fluxes and the impacts of this variability on the upper ocean, ice, and lower atmosphere during the autumn ice advance. Analyses have suggested that these fluxes are impacted by atmospheric synoptic evolution, proximity to existing ice, ice-relative wind direction, ice thickness and snow depth. In turn, these fluxes impact upper-ocean heat loss and timing of ice formation, as well as stability in the lower troposphere and upper ocean, and hence heat transport to the free troposphere and ocean mixed-layer. Therefore, the atmospheric structure over the advancing first-year ice differs from that over the nearby open water. Finally, these observational analyses will be used to provide a preliminary validation of the spatial and temporal variability of the surface energy fluxes and the associated lower-tropospheric and upper-ocean structures in the simulations.

  20. Interannual Variability of Water Ice Clouds at Gale Crater

    NASA Astrophysics Data System (ADS)

    Martinez, G.; Giuranna, M.; McConnochie, T. H.; Tamppari, L.; Smith, M. D.; Vicente-Retortillo, Á.; Renno, N. O.; Kloos, J. L.; Moores, J. E.; Guzewich, S.

    2017-12-01

    The Aphelion Cloud Belt (ACB) is a water ice cloud band that encircles the planet longitudinally at latitudes ranging from about 10°S to 30°N during the northern spring and summer (aphelion season). The ACB has been studied extensively using satellite observations over the last two decades [1], showing little interannual variability from MY 24 to 34. The Mars Science Laboratory (MSL) mission has completed more than 1750 sols of measurements at Gale crater (4.5°S), from Ls 155° in MY 31 to Ls 33° in MY 34. Interestingly, MSL results from various instruments indicate that the ACB produces significant interannual variability at Gale crater during the aphelion season. In particular, near-noon retrievals of water ice opacity by the ChemCam instrument indicate an increase in water ice opacity up to 50% from MY 32 to 33 [2], further supported by analysis of UV [3] and ground temperature [4] data taken by the Rover Environmental Monitoring Station during MY 32 and 33. A weaker ( 5%) increase in water ice opacity in MY 33 relative to MY 32 was also observed from images taken during afternoon hours by the rover's Navigation Cameras [5]. We are analyzing simultaneous and noncontemporary satellite observations at the location of Gale made by the Planetary Fourier Spectrometer [6], Mars Climate Sounder, Thermal Emission Imaging System and Thermal Emission Spectrometer to shed light on the nature of the interannual variability of the ACB at Gale, and to locally understand the relation between the ACB and the water cycle. References:[1] Smith, M.D. (2008), Spacecraft observations of the martian atmosphere, Annu. Rev. Earth Planet. Sci. 36. [2] McConnochie, T. H., et al. (2017), Retrieval of Water Vapor Column Abundance and Aerosol Properties from ChemCam Passive Sky Spectroscopy, Icarus (submitted). [3] Vicente-Retortillo, Á., et al. (2017), Determination of dust aerosol particle size at Gale Crater using REMS UVS and Mastcam measurements, GRL, 44. [4] Vasavada, A.R. et al

  1. An Ice Core Perspective on Aleutian Low Variability over the Common Era

    NASA Astrophysics Data System (ADS)

    Osterberg, E. C.; Winski, D.; Kreutz, K. J.; Wake, C. P.; Ferris, D. G.; Campbell, S.; Introne, D.

    2016-12-01

    The Aleutian Low (ALow) is the dominant feature of atmospheric circulation in the North Pacific, strongly influencing wintertime temperature, precipitation and wind patterns in Alaska and the Yukon Territory, as well as further downstream in North America via atmospheric teleconnections. Changes in ALow strength are known to impact marine ecosystems by contributing to the multi-decadal sea-surface temperature mode in the North Pacific known as the Pacific Decadal Oscillation (PDO). Meteorological records show that in addition to distinct PDO-like variability, the ALow has intensified over the 20th century. However, ALow variability prior to the instrumental period remains unclear due to generally poor correlations among published ALow and PDO reconstructions, including the Mt. Logan ice core ALow record. An improved understanding of past ALow variability is critical for evaluating natural ALow forcing mechanisms, placing the 20th century intensification in context, and improving ALow projections under increased anthropogenic forcing. Here we combine ALow-sensitive time series from the new Denali ice core and the Mt. Logan ice core to develop a high-resolution (1-3 year) multi-ice-core record of ALow variability over the past 1500 years. The Denali ice core was collected from the summit plateau (3900 m) of Mt. Hunter in 2013, and was sampled using the Dartmouth continuous melter system with discrete sampling for major ion (IC), trace element (ICP-MS), and stable isotope ratios (Picarro), as well as continuous flow analyses for dust size and concentration (Klotz Abakus). We focus here on the sea-salt sodium time series, and calibrate our record over the 20th century with reanalysis wind speed and pressure data. The Denali sodium record of ALow strength strongly resembles the Mt. Logan ALow record, with both showing a recent intensification of the ALow that started in the late 1600s and continues into the 20th century. Both records reveal that the ALow was stronger

  2. A combined approach of remote sensing and airborne electromagnetics to determine the volume of polynya sea ice in the Laptev Sea

    NASA Astrophysics Data System (ADS)

    Rabenstein, L.; Krumpen, T.; Hendricks, S.; Koeberle, C.; Haas, C.; Hoelemann, J. A.

    2013-06-01

    A combined interpretation of synthetic aperture radar (SAR) satellite images and helicopter electromagnetic (HEM) sea-ice thickness data has provided an estimate of sea-ice volume formed in Laptev Sea polynyas during the winter of 2007/08. The evolution of the surveyed sea-ice areas, which were formed between late December 2007 and middle April 2008, was tracked using a series of SAR images with a sampling interval of 2-3 days. Approximately 160 km of HEM data recorded in April 2008 provided sea-ice thicknesses along profiles that transected sea ice varying in age from 1 to 116 days. For the volume estimates, thickness information along the HEM profiles was extrapolated to zones of the same age. The error of areal mean thickness information was estimated to be between 0.2 m for younger ice and up to 1.55 m for older ice, with the primary error source being the spatially limited HEM coverage. Our results have demonstrated that the modal thicknesses and mean thicknesses of level ice correlated with the sea-ice age, but that varying dynamic and thermodynamic sea-ice growth conditions resulted in a rather heterogeneous sea-ice thickness distribution on scales of tens of kilometers. Taking all uncertainties into account, total sea-ice area and volume produced within the entire surveyed area were 52 650 km2 and 93.6 ± 26.6 km3. The surveyed polynya contributed 2.0 ± 0.5% of the sea-ice produced throughout the Arctic during the 2007/08 winter. The SAR-HEM volume estimate compares well with the 112 km3 ice production calculated with a~high-resolution ocean sea-ice model. Measured modal and mean-level ice thicknesses correlate with calculated freezing-degree-day thicknesses with a factor of 0.87-0.89, which was too low to justify the assumption of homogeneous thermodynamic growth conditions in the area, or indicates a strong dynamic thickening of level ice by rafting of even thicker ice.

  3. A combined approach of remote sensing and airborne electromagnetics to determine the volume of polynya sea ice in the Laptev Sea

    NASA Astrophysics Data System (ADS)

    Rabenstein, L.; Krumpen, T.; Hendricks, S.; Koeberle, C.; Haas, C.; Hoelemann, J. A.

    2013-02-01

    A combined interpretation of synthetic aperture radar (SAR) satellite images and helicopter electromagnetic (HEM) sea-ice thickness data has provided an estimate of sea-ice volume formed in Laptev Sea polynyas during the winter of 2007/08. The evolution of the surveyed sea-ice areas, which were formed between late December 2007 and middle April 2008, was tracked using a series of SAR images with a sampling interval of 2-3 days. Approximately 160 km of HEM data recorded in April 2008 provided sea-ice thicknesses along profiles that transected sea-ice varying in age from 1-116 days. For the volume estimates, thickness information along the HEM profiles was extrapolated to zones of the same age. The error of areal mean thickness information was estimated to be between 0.2 m for younger ice and up to 1.55 m for older ice, with the primary error source being the spatially limited HEM coverage. Our results have demonstrated that the modal thicknesses and mean thicknesses of level ice correlated with the sea-ice age, but that varying dynamic and thermodynamic sea-ice growth conditions resulted in a rather heterogeneous sea-ice thickness distribution on scales of tens of kilometers. Taking all uncertainties into account, total sea-ice area and volume produced within the entire surveyed area were 52 650 km2 and 93.6 ± 26.6 km3. The surveyed polynya contributed 2.0 ± 0.5% of the sea-ice produced throughout the Arctic during the 2007/08 winter. The SAR-HEM volume estimate compares well with the 112 km3 ice production calculated with a high resolution ocean sea-ice model. Measured modal and mean-level ice thicknesses correlate with calculated freezing-degree-day thicknesses with a factor of 0.87-0.89, which was too low to justify the assumption of homogeneous thermodynamic growth conditions in the area, or indicates a strong dynamic thickening of level ice by rafting of even thicker ice.

  4. Snow and Ice Control Materials for Texas Roads; VOLUME 1: Literature and Best Practices Review; VOLUME 2: Field Trials and Laboratory Study

    DOT National Transportation Integrated Search

    2017-03-01

    This report provides findings from a four-year research study of snow and ice control materials for winter weather roadway maintenance applications in Texas. The report is presented in two volumes. Volume 1 is a literature review and best practices r...

  5. Variability and trends in the Arctic Sea ice cover: Results from different techniques

    NASA Astrophysics Data System (ADS)

    Comiso, Josefino C.; Meier, Walter N.; Gersten, Robert

    2017-08-01

    Variability and trend studies of sea ice in the Arctic have been conducted using products derived from the same raw passive microwave data but by different groups using different algorithms. This study provides consistency assessment of four of the leading products, namely, Goddard Bootstrap (SB2), Goddard NASA Team (NT1), EUMETSAT Ocean and Sea Ice Satellite Application Facility (OSI-SAF 1.2), and Hadley HadISST 2.2 data in evaluating variability and trends in the Arctic sea ice cover. All four provide generally similar ice patterns but significant disagreements in ice concentration distributions especially in the marginal ice zone and adjacent regions in winter and meltponded areas in summer. The discrepancies are primarily due to different ways the four techniques account for occurrences of new ice and meltponding. However, results show that the different products generally provide consistent and similar representation of the state of the Arctic sea ice cover. Hadley and NT1 data usually provide the highest and lowest monthly ice extents, respectively. The Hadley data also show the lowest trends in ice extent and ice area at -3.88%/decade and -4.37%/decade, respectively, compared to an average of -4.36%/decade and -4.57%/decade for all four. Trend maps also show similar spatial distribution for all four with the largest negative trends occurring at the Kara/Barents Sea and Beaufort Sea regions, where sea ice has been retreating the fastest. The good agreement of the trends especially with updated data provides strong confidence in the quantification of the rate of decline in the Arctic sea ice cover.Plain Language SummaryThe declining Arctic sea <span class="hlt">ice</span> cover, especially in the summer, has been the center of attention in recent years. Reports on the sea <span class="hlt">ice</span> cover have been provided by different institutions using basically the same set of satellite data but different techniques for estimating key parameters such as <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C41B0695B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C41B0695B"><span>Greenland <span class="hlt">ice</span> sheet albedo <span class="hlt">variability</span> and feedback: 2000-2015</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Box, J. E.; van As, D.; Fausto, R. S.; Mottram, R.; Langen, P. P.; Steffen, K.</p> <p>2015-12-01</p> <p>Absorbed solar irradiance represents the dominant source of surface melt energy for Greenland <span class="hlt">ice</span>. Surface melting has increased as part of a positive feedback amplifier due to surface darkening. The 16 most recent summers of observations from the NASA MODIS sensor indicate a darkening exceeding 6% in July when most melting occurs. Without the darkening, the increase in surface melting would be roughly half as large. A minority of the albedo decline signal may be from sensor degradation. So, in this study, MOD10A1 and MCD43 albedo products from MODIS are evaluated for sensor degradation and anisotropic reflectance errors. Errors are minimized through calibration to GC-Net and PROMICE Greenland snow and <span class="hlt">ice</span> ground control data. The seasonal and spatial <span class="hlt">variability</span> in Greenland snow and <span class="hlt">ice</span> albedo over a 16 year period is presented, including quantifying changing absorbed solar irradiance and melt enhancement due to albedo feedback using the DMI HIRHAM5 5 km model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRD..123..473M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRD..123..473M"><span>Isolating the Liquid Cloud Response to Recent Arctic Sea <span class="hlt">Ice</span> <span class="hlt">Variability</span> Using Spaceborne Lidar Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morrison, A. L.; Kay, J. E.; Chepfer, H.; Guzman, R.; Yettella, V.</p> <p>2018-01-01</p> <p>While the radiative influence of clouds on Arctic sea <span class="hlt">ice</span> is known, the influence of sea <span class="hlt">ice</span> cover on Arctic clouds is challenging to detect, separate from atmospheric circulation, and attribute to human activities. Providing observational constraints on the two-way relationship between sea <span class="hlt">ice</span> cover and Arctic clouds is important for predicting the rate of future sea <span class="hlt">ice</span> loss. Here we use 8 years of CALIPSO (Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations) spaceborne lidar observations from 2008 to 2015 to analyze Arctic cloud profiles over sea <span class="hlt">ice</span> and over open water. Using a novel surface mask to restrict our analysis to where sea <span class="hlt">ice</span> concentration varies, we isolate the influence of sea <span class="hlt">ice</span> cover on Arctic Ocean clouds. The study focuses on clouds containing liquid water because liquid-containing clouds are the most important cloud type for radiative fluxes and therefore for sea <span class="hlt">ice</span> melt and growth. Summer is the only season with no observed cloud response to sea <span class="hlt">ice</span> cover <span class="hlt">variability</span>: liquid cloud profiles are nearly identical over sea <span class="hlt">ice</span> and over open water. These results suggest that shortwave summer cloud feedbacks do not slow long-term summer sea <span class="hlt">ice</span> loss. In contrast, more liquid clouds are observed over open water than over sea <span class="hlt">ice</span> in the winter, spring, and fall in the 8 year mean and in each individual year. Observed fall sea <span class="hlt">ice</span> loss cannot be explained by natural <span class="hlt">variability</span> alone, which suggests that observed increases in fall Arctic cloud cover over newly open water are linked to human activities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910011228','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910011228"><span>West Antarctic <span class="hlt">Ice</span> Sheet Initiative. <span class="hlt">Volume</span> 1: Science and Implementation Plan</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bindschadler, Robert A. (Editor)</p> <p>1990-01-01</p> <p>The Science and Implementation Plan of the West Antarctic <span class="hlt">Ice</span> Sheet Initiative (WAIS) is described. The goal of this initiative is the prediction of the future behavior of this <span class="hlt">ice</span> sheet and an assessment of its potential to collapse, rapidly raising global sea level. The multidisciplinary nature of WAIS reflects the complexity of the polar <span class="hlt">ice</span> sheet environment. The project builds upon past and current polar studies in many fields and meshes with future programs of both the U.S. and other countries. Important tasks in each discipline are described and a coordinated schedule by which the majority of these tasks can be accomplished in 5 years is presented. The companion report (<span class="hlt">Volume</span> 2) contains seven discipline review papers on the state of knowledge of Antarctica and opinions on how that knowledge must be increased to attain the WAIS goal.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.1690J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.1690J"><span>Antarctic Climate <span class="hlt">Variability</span>: Covariance of Ozone and Sea <span class="hlt">Ice</span> in Atmosphere - Ocean Coupled Model Simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jrrar, Amna; Abraham, N. Luke; Pyle, John A.; Holland, David</p> <p>2014-05-01</p> <p>Changes in sea <span class="hlt">ice</span> significantly modulate climate change because of its high reflective and insulating nature. While Arctic Sea <span class="hlt">Ice</span> Extent (SIE) shows a negative trend. Antarctic SIE shows a weak but positive trend, estimated at 0.127 x 106 km2 per decade. The trend results from large regional cancellations, more <span class="hlt">ice</span> in the Weddell and the Ross seas, and less <span class="hlt">ice</span> in the Amundsen - Bellingshausen seas. A number of studies had demonstrated that stratospheric ozone depletion has had a major impact on the atmospheric circulation, causing a positive trend in the Southern Annular Mode (SAM), which has been linked to the observed positive trend in autumn sea <span class="hlt">ice</span> in the Ross Sea. However, other modelling studies show that models forced with prescribed ozone hole simulate decreased sea <span class="hlt">ice</span> in all regions comparative to a control run. A recent study has also shown that stratospheric ozone recovery will mitigate Antarctic sea <span class="hlt">ice</span> loss. To verify this assumed relationship, it is important first to investigate the covariance between ozone's natural (dynamical) <span class="hlt">variability</span> and Antarctic sea <span class="hlt">ice</span> distribution in pre-industrial climate, to estimate the trend due to natural <span class="hlt">variability</span>. We investigate the relationship between anomalous Antarctic ozone years and the subsequent changes in Antarctic sea <span class="hlt">ice</span> distribution in a multidecadal control simulation using the AO-UMUKCA model. The model has a horizontal resolution of 3.75 X 2.5 degrees in longitude and latitude; and 60 hybrid height levels in the vertical, from the surface up to a height of 84 km. The ocean component is the NEMO ocean model on the ORCA2 tripolar grid, and the sea <span class="hlt">ice</span> model is CICE. We evaluate the model's performance in terms of sea <span class="hlt">ice</span> distribution, and we calculate sea <span class="hlt">ice</span> extent trends for composites of anomalously low versus anomalously high SH polar ozone column. We apply EOF analysis to the seasonal anomalies of sea <span class="hlt">ice</span> concentration, MSLP, and Z 500, and identify the leading climate modes controlling the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51E2122W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51E2122W"><span>The role of synoptic weather <span class="hlt">variability</span> in Greenland <span class="hlt">ice</span> sheet dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walker, J. M.; Radic, V.</p> <p>2017-12-01</p> <p>Much of the large uncertainty in predictions of future global sea level rise is due to our limited understanding of Greenland <span class="hlt">ice</span> sheet (GrIS) motion and its interactions with climate. Over the next century, climate models predict that the GrIS will experience not only gradual warming, but also changes in atmospheric circulation, hydrology, and weather, including a northward shift of the North Atlantic storm track, with greater frequency and intensity of rain storms over the GrIS. Recent studies of GrIS dynamics have focused on the effects of increased seasonal mean meltwater on <span class="hlt">ice</span> velocities, finding only a modest impact due to compensation by subglacial drainage systems, but subglacial hydraulic theory indicates that <span class="hlt">variability</span> on shorter timescales is also relevant: short-term surges in meltwater or rainfall can overload drainage systems at rates faster than they can adjust, leading to water pressure spikes and <span class="hlt">ice</span> acceleration. If the magnitude or frequency of these transient <span class="hlt">ice</span> accelerations increase substantially as synoptic weather patterns change over the next century, there could be a significant cumulative impact on seasonal mean <span class="hlt">ice</span> velocities. However, this issue has not been addressed in the literature and represents a major source of uncertainty. In this study, we investigate the role of synoptic weather <span class="hlt">variability</span> in GrIS dynamics, with the ultimate goal of evaluating the relationships between extreme weather events and <span class="hlt">ice</span> sheet flow in different seasons and regions of the GrIS. As a first step, we apply the machine learning technique of self-organizing maps to atmospheric reanalysis data to categorize the predominant synoptic weather systems over the GrIS domain, evaluating atmospheric moisture transport and rainfall to assess the impacts of each weather system on GrIS surface hydrology. The preliminary results presented here will be used in conjunction with <span class="hlt">ice</span> velocity satellite measurements in future work, to identify any correlations</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27230650','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27230650"><span>Unveiling the pan-genome of the SXT/R391 family of <span class="hlt">ICEs</span>: molecular characterisation of new <span class="hlt">variable</span> regions of SXT/R391-like <span class="hlt">ICEs</span> detected in Pseudoalteromonas sp. and Vibrio scophthalmi.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rodríguez-Blanco, Arturo; Lemos, Manuel L; Osorio, Carlos R</p> <p>2016-08-01</p> <p>Integrating conjugative elements (<span class="hlt">ICEs</span>) of the SXT/R391 family have been identified in fish-isolated bacterial strains collected from marine aquaculture environments of the northwestern Iberian Peninsula. Here we analysed the <span class="hlt">variable</span> regions of two <span class="hlt">ICEs</span>, one preliminarily characterised in a previous study (ICEVscSpa3) and one newly identified (ICEPspSpa1). Bacterial strains harboring these <span class="hlt">ICEs</span> were phylogenetically assigned to Vibrio scophthalmi and Pseudoalteromonas sp., thus constituting the first evidence of SXT/R391-like <span class="hlt">ICEs</span> in the genus Pseudoalteromonas to date. <span class="hlt">Variable</span> DNA regions, which confer element-specific properties to <span class="hlt">ICEs</span> of this family, were characterised. Interestingly, the two <span class="hlt">ICEs</span> contained 29 genes not found in <span class="hlt">variable</span> DNA insertions of previously described <span class="hlt">ICEs</span>. Most notably, <span class="hlt">variable</span> gene content for ICEVscSpa3 showed similarity to genes potentially involved in housekeeping functions of replication, nucleotide metabolism and transcription. For these genes, closest homologues were found clustered in the genome of Pseudomonas psychrotolerans L19, suggesting a transfer as a block to ICEVscSpa3. Genes encoding antibiotic resistance, restriction modification systems and toxin/antitoxin systems were absent from hotspots of ICEVscSpa3. In contrast, the <span class="hlt">variable</span> gene content of ICEPspSpa1 included genes involved in restriction/modification functions in two different hotspots and genes related to <span class="hlt">ICE</span> maintenance. The present study unveils a relatively large number of novel genes in SXT/R391-<span class="hlt">ICEs</span>, and demonstrates the major role of <span class="hlt">ICE</span> elements as contributors to horizontal gene transfer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.5647K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.5647K"><span>Arctic energy budget in relation to sea-<span class="hlt">ice</span> <span class="hlt">variability</span> on monthly to annual time scales</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krikken, Folmer; Hazeleger, Wilco</p> <p>2015-04-01</p> <p>The strong decrease in Arctic sea-<span class="hlt">ice</span> in recent years has triggered a strong interest in Arctic sea-<span class="hlt">ice</span> predictions on seasonal to decadal time scales. Hence, it is key to understand physical processes that provide enhanced predictability beyond persistence of sea <span class="hlt">ice</span> anomalies. The authors report on an analysis of natural <span class="hlt">variability</span> of Arctic sea-<span class="hlt">ice</span> from an energy budget perspective, using 15 CMIP5 climate models, and comparing these results to atmospheric and oceanic reanalyses data. We quantify the persistence of sea <span class="hlt">ice</span> anomalies and the cross-correlation with the surface and top energy budget components. The Arctic energy balance components primarily indicate the important role of the seasonal sea-<span class="hlt">ice</span> albedo feedback, in which sea-<span class="hlt">ice</span> anomalies in the melt season reemerge in the growth season. This is a robust anomaly reemergence mechanism among all 15 climate models. The role of ocean lies mainly in storing heat content anomalies in spring, and releasing them in autumn. Ocean heat flux variations only play a minor role. The role of clouds is further investigated. We demonstrate that there is no direct atmospheric response of clouds to spring sea-<span class="hlt">ice</span> anomalies, but a delayed response is evident in autumn. Hence, there is no cloud-<span class="hlt">ice</span> feedback in late spring and summer, but there is a cloud-<span class="hlt">ice</span> feedback in autumn, which strengthens the <span class="hlt">ice</span>-albedo feedback. Anomalies in insolation are positively correlated with sea-<span class="hlt">ice</span> <span class="hlt">variability</span>. This is primarily a result of reduced multiple-reflection of insolation due to an albedo decrease. This effect counteracts the sea-<span class="hlt">ice</span> albedo effect up to 50%. ERA-Interim and ORAS4 confirm the main findings from the climate models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21C1134H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21C1134H"><span>3D <span class="hlt">Volume</span> and Morphology of Perennial Cave <span class="hlt">Ice</span> and Related Geomorphological Models at Scăriloara <span class="hlt">Ice</span> Cave, Romania, from Structure from Motion, Ground Penetrating Radar and Total Station Surveys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hubbard, J.; Onac, B. P.; Kruse, S.; Forray, F. L.</p> <p>2017-12-01</p> <p>Research at Scăriloara <span class="hlt">Ice</span> Cave has proceeded for over 150 years, primarily driven by the presence and paleoclimatic importance of the large perennial <span class="hlt">ice</span> block and various <span class="hlt">ice</span> speleothems located within its galleries. Previous observations of the <span class="hlt">ice</span> block led to rudimentary <span class="hlt">volume</span> estimates of 70,000 to 120,000 cubic meters (m3), prospectively placing it as one of the world's largest cave <span class="hlt">ice</span> deposits. The cave morphology and the surface of the <span class="hlt">ice</span> block are now recreated in a total station survey-validated 3D model, produced using Structure from Motion (SfM) software. With the total station survey and the novel use of ArcGIS tools, the SfM validation process is drastically simplified to produce a scaled, georeferenced, and photo-texturized 3D model of the cave environment with a root-mean-square error (RMSE) of 0.24 m. Furthermore, ground penetrating radar data was collected and spatially oriented with the total station survey to recreate the <span class="hlt">ice</span> block basal surface and was combined with the SfM model to create a model of the <span class="hlt">ice</span> block itself. The resulting <span class="hlt">ice</span> block model has a <span class="hlt">volume</span> of over 118,000 m3 with an uncertainty of 9.5%, with additional <span class="hlt">volumes</span> left un-surveyed. The varying elevation of the <span class="hlt">ice</span> block basal surface model reflect specific features of the cave roof, such as areas of enlargement, shafts, and potential joints, which offer further validation and inform theories on cave and <span class="hlt">ice</span> genesis. Specifically, a large depression area was identified as a potential area of initial <span class="hlt">ice</span> growth. Finally, an <span class="hlt">ice</span> thickness map was produced that will aid in the designing of future <span class="hlt">ice</span> coring projects. This methodology presents a powerful means to observe and accurately characterize and measure cave and cave <span class="hlt">ice</span> morphologies with ease and affordability. Results further establish the significance of Scăriloara's <span class="hlt">ice</span> block to paleoclimate research, provide insights into cave and <span class="hlt">ice</span> block genesis, and aid future study design.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25313072','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25313072"><span>Sea level and global <span class="hlt">ice</span> <span class="hlt">volumes</span> from the Last Glacial Maximum to the Holocene.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lambeck, Kurt; Rouby, Hélène; Purcell, Anthony; Sun, Yiying; Sambridge, Malcolm</p> <p>2014-10-28</p> <p>The major cause of sea-level change during <span class="hlt">ice</span> ages is the exchange of water between <span class="hlt">ice</span> and ocean and the planet's dynamic response to the changing surface load. Inversion of ∼1,000 observations for the past 35,000 y from localities far from former <span class="hlt">ice</span> margins has provided new constraints on the fluctuation of <span class="hlt">ice</span> <span class="hlt">volume</span> in this interval. Key results are: (i) a rapid final fall in global sea level of ∼40 m in <2,000 y at the onset of the glacial maximum ∼30,000 y before present (30 ka BP); (ii) a slow fall to -134 m from 29 to 21 ka BP with a maximum grounded <span class="hlt">ice</span> <span class="hlt">volume</span> of ∼52 × 10(6) km(3) greater than today; (iii) after an initial short duration rapid rise and a short interval of near-constant sea level, the main phase of deglaciation occurred from ∼16.5 ka BP to ∼8.2 ka BP at an average rate of rise of 12 m⋅ka(-1) punctuated by periods of greater, particularly at 14.5-14.0 ka BP at ≥40 mm⋅y(-1) (MWP-1A), and lesser, from 12.5 to 11.5 ka BP (Younger Dryas), rates; (iv) no evidence for a global MWP-1B event at ∼11.3 ka BP; and (v) a progressive decrease in the rate of rise from 8.2 ka to ∼2.5 ka BP, after which ocean <span class="hlt">volumes</span> remained nearly constant until the renewed sea-level rise at 100-150 y ago, with no evidence of oscillations exceeding ∼15-20 cm in time intervals ≥200 y from 6 to 0.15 ka BP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4217469','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4217469"><span>Sea level and global <span class="hlt">ice</span> <span class="hlt">volumes</span> from the Last Glacial Maximum to the Holocene</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lambeck, Kurt; Rouby, Hélène; Purcell, Anthony; Sun, Yiying; Sambridge, Malcolm</p> <p>2014-01-01</p> <p>The major cause of sea-level change during <span class="hlt">ice</span> ages is the exchange of water between <span class="hlt">ice</span> and ocean and the planet’s dynamic response to the changing surface load. Inversion of ∼1,000 observations for the past 35,000 y from localities far from former <span class="hlt">ice</span> margins has provided new constraints on the fluctuation of <span class="hlt">ice</span> <span class="hlt">volume</span> in this interval. Key results are: (i) a rapid final fall in global sea level of ∼40 m in <2,000 y at the onset of the glacial maximum ∼30,000 y before present (30 ka BP); (ii) a slow fall to −134 m from 29 to 21 ka BP with a maximum grounded <span class="hlt">ice</span> <span class="hlt">volume</span> of ∼52 × 106 km3 greater than today; (iii) after an initial short duration rapid rise and a short interval of near-constant sea level, the main phase of deglaciation occurred from ∼16.5 ka BP to ∼8.2 ka BP at an average rate of rise of 12 m⋅ka−1 punctuated by periods of greater, particularly at 14.5–14.0 ka BP at ≥40 mm⋅y−1 (MWP-1A), and lesser, from 12.5 to 11.5 ka BP (Younger Dryas), rates; (iv) no evidence for a global MWP-1B event at ∼11.3 ka BP; and (v) a progressive decrease in the rate of rise from 8.2 ka to ∼2.5 ka BP, after which ocean <span class="hlt">volumes</span> remained nearly constant until the renewed sea-level rise at 100–150 y ago, with no evidence of oscillations exceeding ∼15–20 cm in time intervals ≥200 y from 6 to 0.15 ka BP. PMID:25313072</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3660359','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3660359"><span>Change and <span class="hlt">Variability</span> in East Antarctic Sea <span class="hlt">Ice</span> Seasonality, 1979/80–2009/10</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Massom, Robert; Reid, Philip; Stammerjohn, Sharon; Raymond, Ben; Fraser, Alexander; Ushio, Shuki</p> <p>2013-01-01</p> <p>Recent analyses have shown that significant changes have occurred in patterns of sea <span class="hlt">ice</span> seasonality in West Antarctica since 1979, with wide-ranging climatic, biological and biogeochemical consequences. Here, we provide the first detailed report on long-term change and <span class="hlt">variability</span> in annual timings of sea <span class="hlt">ice</span> advance, retreat and resultant <span class="hlt">ice</span> season duration in East Antarctica. These were calculated from satellite-derived <span class="hlt">ice</span> concentration data for the period 1979/80 to 2009/10. The pattern of change in sea <span class="hlt">ice</span> seasonality off East Antarctica comprises mixed signals on regional to local scales, with pockets of strongly positive and negative trends occurring in near juxtaposition in certain regions e.g., Prydz Bay. This pattern strongly reflects change and <span class="hlt">variability</span> in different elements of the marine “icescape”, including fast <span class="hlt">ice</span>, polynyas and the marginal <span class="hlt">ice</span> zone. A trend towards shorter sea-<span class="hlt">ice</span> duration (of 1 to 3 days per annum) occurs in fairly isolated pockets in the outer pack from∼95–110°E, and in various near-coastal areas that include an area of particularly strong and persistent change near Australia's Davis Station and between the Amery and West <span class="hlt">Ice</span> Shelves. These areas are largely associated with coastal polynyas that are important as sites of enhanced sea <span class="hlt">ice</span> production/melt. Areas of positive trend in <span class="hlt">ice</span> season duration are more extensive, and include an extensive zone from 160–170°E (i.e., the western Ross Sea sector) and the near-coastal zone between 40–100°E. The East Antarctic pattern is considerably more complex than the well-documented trends in West Antarctica e.g., in the Antarctic Peninsula-Bellingshausen Sea and western Ross Sea sectors. PMID:23705008</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120013478','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120013478"><span><span class="hlt">Variability</span> and Anomalous Trends in the Global Sea <span class="hlt">Ice</span> Cover</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comiso, Josefino C.</p> <p>2012-01-01</p> <p>The advent of satellite data came fortuitously at a time when the global sea <span class="hlt">ice</span> cover has been changing rapidly and new techniques are needed to accurately assess the true state and characteristics of the global sea <span class="hlt">ice</span> cover. The extent of the sea <span class="hlt">ice</span> in the Northern Hemisphere has been declining by about -4% per decade for the period 1979 to 2011 but for the period from 1996 to 2010, the rate of decline became even more negative at -8% per decade, indicating an acceleration in the decline. More intriguing is the drastically declining perennial sea <span class="hlt">ice</span> area, which is the <span class="hlt">ice</span> that survives the summer melt and observed to be retreating at the rate of -14% per decade during the 1979 to 2012 period. Although a slight recovery occurred in the last three years from an abrupt decline in 2007, the perennial <span class="hlt">ice</span> extent was almost as low as in 2007 in 2011. The multiyear <span class="hlt">ice</span>, which is the thick component of the perennial <span class="hlt">ice</span> and regarded as the mainstay of the Arctic sea <span class="hlt">ice</span> cover is declining at an even higher rate of -19% per decade. The more rapid decline of the extent of this thicker <span class="hlt">ice</span> type means that the <span class="hlt">volume</span> of the <span class="hlt">ice</span> is also declining making the survival of the Arctic <span class="hlt">ice</span> in summer highly questionable. The slight recovery in 2008, 2009 and 2010 for the perennial <span class="hlt">ice</span> in summer was likely associated with an apparent cycle in the time series with a period of about 8 years. Results of analysis of concurrent MODIS and AMSR-E data in summer also provide some evidence of more extensive summer melt and meltponding in 2007 and 2011 than in other years. Meanwhile, the Antarctic sea <span class="hlt">ice</span> cover, as observed by the same set of satellite data, is showing an unexpected and counter intuitive increase of about 1 % per decade over the same period. Although a strong decline in <span class="hlt">ice</span> extent is apparent in the Bellingshausen/ Amundsen Seas region, such decline is more than compensated by increases in the extent of the sea <span class="hlt">ice</span> cover in the Ross Sea region. The results of analysis of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..179...87E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..179...87E"><span><span class="hlt">Ice</span> streams of the Late Wisconsin Cordilleran <span class="hlt">Ice</span> Sheet in western North America</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eyles, Nick; Arbelaez Moreno, Lina; Sookhan, Shane</p> <p>2018-01-01</p> <p>The Late Wisconsin Cordilleran <span class="hlt">Ice</span> Sheet (CIS) of western North America is thought to have reached its maximum extent (∼2.5 × 106 km2) as late at c. 14.5 ka. Most (80%) of the <span class="hlt">ice</span> sheet's bed consists of high mountains but its 'core zone' sited on plateaux of the Intermontane Belt of British Columbia and coterminous parts of the USA, shows broad swaths of subglacially-streamlined rock and sediment. Broad scale mapping from new digital imagery data identifies three subglacial bed types: 1) 'hard beds' of <span class="hlt">variably</span> streamlined bedrock; 2) drumlinized 'soft beds' of deformation till reworked from antecedent sediment, and 3) 'mixed beds' of <span class="hlt">variably</span>-streamlined bedrock protruding through drumlinized sediment. Drumlins on soft beds appear to be erosional features cut into till and antecedent sediments, and identify the catchment areas of paleo <span class="hlt">ice</span> streams expressed downglacier as flow sets of megascale glacial lineations (MSGLs). 'Grooved' and 'cloned' drumlins appear to record the transition from drumlins to MSGLs. The location of paleo <span class="hlt">ice</span> streams reflects topographic funneling of <span class="hlt">ice</span> from plateau surfaces through outlet valleys and a soft bed that sustained fast flow; rock-cut MSGLs are also present locally on the floors of outlet valleys. CIS disintegrated in <1000 years shortly after c. 13.0 ka releasing very large <span class="hlt">volumes</span> of meltwater and sediment to the Pacific coast. Abrupt deglaciation may reflect unsustainable calving of marine-based <span class="hlt">ice</span> streams along the glacio-isostatically depressed coast; large deep 'fiord lakes' in the <span class="hlt">ice</span> sheet's interior may have played an analogous role. Mapping of the broad scale distribution of bed types across the Cordilleran <span class="hlt">Ice</span> Sheet provides key information for paleoglaciological modelling and also for understanding the beds of modern <span class="hlt">ice</span> masses such as the Greenland <span class="hlt">Ice</span> Sheet which is of a comparable topographic setting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012E%26PSL.341..243F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012E%26PSL.341..243F"><span>The evolution of pCO2, <span class="hlt">ice</span> <span class="hlt">volume</span> and climate during the middle Miocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Foster, Gavin L.; Lear, Caroline H.; Rae, James W. B.</p> <p>2012-08-01</p> <p>The middle Miocene Climatic Optimum (17-15 Ma; MCO) is a period of global warmth and relatively high CO2 and is thought to be associated with a significant retreat of the Antarctic <span class="hlt">Ice</span> Sheet (AIS). We present here a new planktic foraminiferal δ11B record from 16.6 to 11.8 Ma from two deep ocean sites currently in equilibrium with the atmosphere with respect to CO2. These new data demonstrate that the evolution of global climate during the middle Miocene (as reflected by changes in the cyrosphere) was well correlated to variations in the concentration of atmospheric CO2. What is more, within our sampling resolution (∼1 sample per 300 kyr) there is no evidence of hysteresis in the response of <span class="hlt">ice</span> <span class="hlt">volume</span> to CO2 forcing during the middle Miocene, contrary to what is understood about the Antarctic <span class="hlt">Ice</span> Sheet from <span class="hlt">ice</span> sheet modelling studies. In agreement with previous data, we show that absolute levels of CO2 during the MCO were relatively modest (350-400 ppm) and levels either side of the MCO are similar or lower than the pre-industrial (200-260 ppm). These new data imply the presence of either a very dynamic AIS at relatively low CO2 during the middle Miocene or the advance and retreat of significant northern hemisphere <span class="hlt">ice</span>. Recent drilling on the Antarctic margin and shore based studies indicate significant retreat and advance beyond the modern limits of the AIS did occur during the middle Miocene, but the complete loss of the AIS was unlikely. Consequently, it seems that <span class="hlt">ice</span> <span class="hlt">volume</span> and climate variations during the middle Miocene probably involved a more dynamic AIS than the modern but also some component of land-based <span class="hlt">ice</span> in the northern hemisphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5810994','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5810994"><span>Vestibular schwannomas: Accuracy of tumor <span class="hlt">volume</span> estimated by <span class="hlt">ice</span> cream cone formula using thin-sliced MR images</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ho, Hsing-Hao; Li, Ya-Hui; Lee, Jih-Chin; Wang, Chih-Wei; Yu, Yi-Lin; Hueng, Dueng-Yuan; Hsu, Hsian-He</p> <p>2018-01-01</p> <p>Purpose We estimated the <span class="hlt">volume</span> of vestibular schwannomas by an <span class="hlt">ice</span> cream cone formula using thin-sliced magnetic resonance images (MRI) and compared the estimation accuracy among different estimating formulas and between different models. Methods The study was approved by a local institutional review board. A total of 100 patients with vestibular schwannomas examined by MRI between January 2011 and November 2015 were enrolled retrospectively. Informed consent was waived. <span class="hlt">Volumes</span> of vestibular schwannomas were estimated by cuboidal, ellipsoidal, and spherical formulas based on a one-component model, and cuboidal, ellipsoidal, Linskey’s, and <span class="hlt">ice</span> cream cone formulas based on a two-component model. The estimated <span class="hlt">volumes</span> were compared to the <span class="hlt">volumes</span> measured by planimetry. Intraobserver reproducibility and interobserver agreement was tested. Estimation error, including absolute percentage error (APE) and percentage error (PE), was calculated. Statistical analysis included intraclass correlation coefficient (ICC), linear regression analysis, one-way analysis of variance, and paired t-tests with P < 0.05 considered statistically significant. Results Overall tumor size was 4.80 ± 6.8 mL (mean ±standard deviation). All ICCs were no less than 0.992, suggestive of high intraobserver reproducibility and high interobserver agreement. Cuboidal formulas significantly overestimated the tumor <span class="hlt">volume</span> by a factor of 1.9 to 2.4 (P ≤ 0.001). The one-component ellipsoidal and spherical formulas overestimated the tumor <span class="hlt">volume</span> with an APE of 20.3% and 29.2%, respectively. The two-component <span class="hlt">ice</span> cream cone method, and ellipsoidal and Linskey’s formulas significantly reduced the APE to 11.0%, 10.1%, and 12.5%, respectively (all P < 0.001). Conclusion The <span class="hlt">ice</span> cream cone method and other two-component formulas including the ellipsoidal and Linskey’s formulas allow for estimation of vestibular schwannoma <span class="hlt">volume</span> more accurately than all one-component formulas. PMID:29438424</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('https://www.ncbi.nlm.nih.gov/pubmed/29438424','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29438424"><span>Vestibular schwannomas: Accuracy of tumor <span class="hlt">volume</span> estimated by <span class="hlt">ice</span> cream cone formula using thin-sliced MR images.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ho, Hsing-Hao; Li, Ya-Hui; Lee, Jih-Chin; Wang, Chih-Wei; Yu, Yi-Lin; Hueng, Dueng-Yuan; Ma, Hsin-I; Hsu, Hsian-He; Juan, Chun-Jung</p> <p>2018-01-01</p> <p>We estimated the <span class="hlt">volume</span> of vestibular schwannomas by an <span class="hlt">ice</span> cream cone formula using thin-sliced magnetic resonance images (MRI) and compared the estimation accuracy among different estimating formulas and between different models. The study was approved by a local institutional review board. A total of 100 patients with vestibular schwannomas examined by MRI between January 2011 and November 2015 were enrolled retrospectively. Informed consent was waived. <span class="hlt">Volumes</span> of vestibular schwannomas were estimated by cuboidal, ellipsoidal, and spherical formulas based on a one-component model, and cuboidal, ellipsoidal, Linskey's, and <span class="hlt">ice</span> cream cone formulas based on a two-component model. The estimated <span class="hlt">volumes</span> were compared to the <span class="hlt">volumes</span> measured by planimetry. Intraobserver reproducibility and interobserver agreement was tested. Estimation error, including absolute percentage error (APE) and percentage error (PE), was calculated. Statistical analysis included intraclass correlation coefficient (ICC), linear regression analysis, one-way analysis of variance, and paired t-tests with P < 0.05 considered statistically significant. Overall tumor size was 4.80 ± 6.8 mL (mean ±standard deviation). All ICCs were no less than 0.992, suggestive of high intraobserver reproducibility and high interobserver agreement. Cuboidal formulas significantly overestimated the tumor <span class="hlt">volume</span> by a factor of 1.9 to 2.4 (P ≤ 0.001). The one-component ellipsoidal and spherical formulas overestimated the tumor <span class="hlt">volume</span> with an APE of 20.3% and 29.2%, respectively. The two-component <span class="hlt">ice</span> cream cone method, and ellipsoidal and Linskey's formulas significantly reduced the APE to 11.0%, 10.1%, and 12.5%, respectively (all P < 0.001). The <span class="hlt">ice</span> cream cone method and other two-component formulas including the ellipsoidal and Linskey's formulas allow for estimation of vestibular schwannoma <span class="hlt">volume</span> more accurately than all one-component formulas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=personality+AND+characteristics+AND+athlete+AND+research+AND+paper&id=ED141340','ERIC'); return false;" href="https://eric.ed.gov/?q=personality+AND+characteristics+AND+athlete+AND+research+AND+paper&id=ED141340"><span>The Relationship of Various Psychosocial <span class="hlt">Variables</span> on the Positioning of College <span class="hlt">Ice</span> Hockey Players.</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>Krotee, March L.; La Point, James D.</p> <p></p> <p>This paper presents the results of research conducted to investigate the relationship of various psychosocial <span class="hlt">variables</span> on the positioning of college <span class="hlt">ice</span> hockey players. The California Personality Inventory (CPI) was administered to the NCAA Championship <span class="hlt">ice</span> hockey team at the University of Minnesota, and a separate subjective psychosocial rating…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5461504','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5461504"><span>Multicentennial record of Labrador Sea primary productivity and sea-<span class="hlt">ice</span> <span class="hlt">variability</span> archived in coralline algal barium</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chan, P.; Halfar, J.; Adey, W.; Hetzinger, S.; Zack, T.; Moore, G.W.K.; Wortmann, U. G.; Williams, B.; Hou, A.</p> <p>2017-01-01</p> <p>Accelerated warming and melting of Arctic sea-<span class="hlt">ice</span> has been associated with significant increases in phytoplankton productivity in recent years. Here, utilizing a multiproxy approach, we reconstruct an annually resolved record of Labrador Sea productivity related to sea-<span class="hlt">ice</span> <span class="hlt">variability</span> in Labrador, Canada that extends well into the Little <span class="hlt">Ice</span> Age (LIA; 1646 AD). Barium-to-calcium ratios (Ba/Ca) and carbon isotopes (δ13C) measured in long-lived coralline algae demonstrate significant correlations to both observational and proxy records of sea-<span class="hlt">ice</span> <span class="hlt">variability</span>, and show persistent patterns of co-<span class="hlt">variability</span> broadly consistent with the timing and phasing of the Atlantic Multidecadal Oscillation (AMO). Results indicate reduced productivity in the Subarctic Northwest Atlantic associated with AMO cool phases during the LIA, followed by a step-wise increase from 1910 to present levels—unprecedented in the last 363 years. Increasing phytoplankton productivity is expected to fundamentally alter marine ecosystems as warming and freshening is projected to intensify over the coming century. PMID:28569839</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024935','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024935"><span>Historical trend in river <span class="hlt">ice</span> thickness and coherence in hydroclimatological trends in Maine</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Huntington, T.G.; Hodgkins, G.A.; Dudley, R.W.</p> <p>2003-01-01</p> <p>We analyzed long-term records of <span class="hlt">ice</span> thickness on the Piscataquis River in central Maine and air temperature in Maine to determine whether there were temporal trends that were associated with climate warming. The trend in <span class="hlt">ice</span> thickness was compared and correlated with regional time series of winter air temperature, heating degree days (HDD), date of river <span class="hlt">ice</span>-out, seasonal center-of-<span class="hlt">volume</span> date (SCVD) (date on which half of the stream runoff <span class="hlt">volume</span> during the period 1 Jan. to 31 May has occurred), water temperature, and lake <span class="hlt">ice</span>-out date. All of these <span class="hlt">variables</span> except lake <span class="hlt">ice</span>-out date showed significant temporal trends during the 20th century. Average <span class="hlt">ice</span> thickness around 28 February decreased by about 23 cm from 1912 to 2001. Over the period 1900 to 1999, winter air temperature increased by 1.7??C and HDD decreased by about 7.5%. Final <span class="hlt">ice</span>-out date on the Piscataquis River occurred earlier (advanced), by 0.21 days yr-1 over the period 1931 to 2002, and the SCVD advanced by 0.11 days yr-1 over the period 1903 to 2001. <span class="hlt">Ice</span> thickness was significantly correlated (P-value < 0.01) with winter air temperature, HDD, river <span class="hlt">ice</span>-out, and SCVD. These systematic temporal trends in multiple hydrologic indicator <span class="hlt">variables</span> indicate a coherent response to climate forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A41N..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A41N..04H"><span>Observed and simulated changes in Antarctic sea <span class="hlt">ice</span> and sea level pressure: anthropogenic or natural <span class="hlt">variability</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>Hobbs, W. R.</p> <p>2013-12-01</p> <p>Statistically-significant changes in Antarctic sea <span class="hlt">ice</span> cover and the overlying atmosphere have been observed over the last 30 years, but there is an open question of whether these changes are due to multi-decadal natural <span class="hlt">variability</span> or an anthropogenically-forced response. A number of recent papers have shown that the slight increase in total sea <span class="hlt">ice</span> cover is within the bounds of internal <span class="hlt">variability</span> exhibited by coupled climate models in the CMIP5 suite. Modelled changes for the same time period generally show a decrease, but again with a magnitude that is within internal <span class="hlt">variability</span>. However, in contrast to the Arctic, sea <span class="hlt">ice</span> tends in the Antarctic are spatially highly heterogeneous, and consideration of the total <span class="hlt">ice</span> cover may mask important regional signals. In this work, a robust ';fingerprinting' approach is used to show that the observed spatial pattern of sea <span class="hlt">ice</span> trends is in fact outside simulated natural <span class="hlt">variability</span> in west Antarctic, and furthermore that the CMIP5 models consistently show decreased <span class="hlt">ice</span> cover in the Ross and Weddell Seas, sectors which in fact have an observed increase in cover. As a first step towards understanding the disagreement between models and observations, modelled sea level pressure trends are analysed using and optimal fingerprinting approach, to identify whether atmospheric deficiencies in the models can explain the model-observation discrepancy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.C22A..03S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.C22A..03S"><span>Southern Alaska Glaciers: Spatial and Temporal Variations in <span class="hlt">Ice</span> <span class="hlt">Volume</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sauber, J.; Molnia, B. F.; Luthcke, S.; Rowlands, D.; Harding, D.; Carabajal, C.; Hurtado, J. M.; Spada, G.</p> <p>2004-12-01</p> <p> footprint returns to estimate glacier <span class="hlt">ice</span> elevations and surface characteristics. To obtain the optimal ICESat results, we are reprocessing the ICESat data from Alaska to provide a well-calibrated regional ICESat solution. We anticipate that our ICESat results combined with earlier data will provide new constraints on the temporal and spatial variations in <span class="hlt">ice</span> <span class="hlt">volume</span> of individual Alaskan mountain ranges. These results allow us to address how recent melting of the southern Alaska glaciers contribute to short-term sea-level rise. Our results will also enable us to quantify crustal stress changes due to <span class="hlt">ice</span> mass fluctuations and to assess the influence of <span class="hlt">ice</span> mass changes on the seismically active southern Alaskan plate boundary zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120010371','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120010371"><span><span class="hlt">Variability</span> of Basal Melt Beneath the Pine Island Glacier <span class="hlt">Ice</span> Shelf, West Antarctica</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bindschadler, Robert; Vaughan, David G.; Vornberger, Patricia</p> <p>2011-01-01</p> <p>Observations from satellite and airborne platforms are combined with model calculations to infer the nature and efficiency of basal melting of the Pine Island Glacier <span class="hlt">ice</span> shelf, West Antarctica, by ocean waters. Satellite imagery shows surface features that suggest <span class="hlt">ice</span>-shelf-wide changes to the ocean s influence on the <span class="hlt">ice</span> shelf as the grounding line retreated. Longitudinal profiles of <span class="hlt">ice</span> surface and bottom elevations are analyzed to reveal a spatially dependent pattern of basal melt with an annual melt flux of 40.5 Gt/a. One profile captures a persistent set of surface waves that correlates with quasi-annual variations of atmospheric forcing of Amundsen Sea circulation patterns, establishing a direct connection between atmospheric <span class="hlt">variability</span> and sub-<span class="hlt">ice</span>-shelf melting. <span class="hlt">Ice</span> surface troughs are hydrostatically compensated by <span class="hlt">ice</span>-bottom voids up to 150m deep. Voids form dynamically at the grounding line, triggered by enhanced melting when warmer-than-average water arrives. Subsequent enlargement of the voids is thermally inefficient (4% or less) compared with an overall melting efficiency beneath the <span class="hlt">ice</span> shelf of 22%. Residual warm water is believed to cause three persistent polynyas at the <span class="hlt">ice</span>-shelf front seen in Landsat imagery. Landsat thermal imagery confirms the occurrence of warm water at the same locations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015TCD.....9.1077S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015TCD.....9.1077S"><span>Arctic sea <span class="hlt">ice</span> area in CMIP3 and CMIP5 climate model ensembles - <span class="hlt">variability</span> and change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Semenov, V. A.; Martin, T.; Behrens, L. K.; Latif, M.</p> <p>2015-02-01</p> <p>The shrinking Arctic sea <span class="hlt">ice</span> cover observed during the last decades is probably the clearest manifestation of ongoing climate change. While climate models in general reproduce the sea <span class="hlt">ice</span> retreat in the Arctic during the 20th century and simulate further sea <span class="hlt">ice</span> area loss during the 21st century in response to anthropogenic forcing, the models suffer from large biases and the model results exhibit considerable spread. The last generation of climate models from World Climate Research Programme Coupled Model Intercomparison Project Phase 5 (CMIP5), when compared to the previous CMIP3 model ensemble and considering the whole Arctic, were found to be more consistent with the observed changes in sea <span class="hlt">ice</span> extent during the recent decades. Some CMIP5 models project strongly accelerated (non-linear) sea <span class="hlt">ice</span> loss during the first half of the 21st century. Here, complementary to previous studies, we compare results from CMIP3 and CMIP5 with respect to regional Arctic sea <span class="hlt">ice</span> change. We focus on September and March sea <span class="hlt">ice</span>. Sea <span class="hlt">ice</span> area (SIA) <span class="hlt">variability</span>, sea <span class="hlt">ice</span> concentration (SIC) <span class="hlt">variability</span>, and characteristics of the SIA seasonal cycle and interannual <span class="hlt">variability</span> have been analysed for the whole Arctic, termed Entire Arctic, Central Arctic and Barents Sea. Further, the sensitivity of SIA changes to changes in Northern Hemisphere (NH) averaged temperature is investigated and several important dynamical links between SIA and natural climate <span class="hlt">variability</span> involving the Atlantic Meridional Overturning Circulation (AMOC), North Atlantic Oscillation (NAO) and sea level pressure gradient (SLPG) in the western Barents Sea opening serving as an index of oceanic inflow to the Barents Sea are studied. The CMIP3 and CMIP5 models not only simulate a coherent decline of the Arctic SIA but also depict consistent changes in the SIA seasonal cycle and in the aforementioned dynamical links. The spatial patterns of SIC <span class="hlt">variability</span> improve in the CMIP5 ensemble, particularly in summer. Both</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995EOSTr..76..265C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995EOSTr..76..265C"><span><span class="hlt">Ice</span> sheets play important role in climate change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clark, Peter U.; MacAyeal, Douglas R.; Andrews, John T.; Bartlein, Patrick J.</p> <p></p> <p><span class="hlt">Ice</span> sheets once were viewed as passive elements in the climate system enslaved to orbitally generated variations in solar radiation. Today, modeling results and new geologic records suggest that <span class="hlt">ice</span> sheets actively participated in late-Pleistocene climate change, amplifying or driving significant <span class="hlt">variability</span> at millennial as well as orbital timescales. Although large changes in global <span class="hlt">ice</span> <span class="hlt">volume</span> were ultimately caused by orbital variations (the Milankovitch hypothesis), once in existence, the former <span class="hlt">ice</span> sheets behaved dynamically and strongly influenced regional and perhaps even global climate by altering atmospheric and oceanic circulation and temperature.Experiments with General Circulation Models (GCMs) yielded the first inklings of <span class="hlt">ice</span> sheets' climatic significance. Manabe and Broccoli [1985], for example, found that the topographic and albedo effects of <span class="hlt">ice</span> sheets alone explain much of the Northern Hemisphere cooling identified in paleoclimatic records of the last glacial maximum (˜21 ka).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C21B0683C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21B0683C"><span>Patterns of <span class="hlt">variability</span> in steady- and non steady-state Ross <span class="hlt">Ice</span> Shelf flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Campbell, A. J.; Hulbe, C. L.; Scambos, T. A.; Klinger, M. J.; Lee, C. K.</p> <p>2016-12-01</p> <p><span class="hlt">Ice</span> shelves are gateways through which climate change can be transmitted from the ocean or atmosphere to a grounded <span class="hlt">ice</span> sheet. It is thus important to separate patterns of <span class="hlt">ice</span> shelf change driven internally (from the <span class="hlt">ice</span> sheet) and patterns driven externally (by the ocean or atmosphere) so that modern observations can be viewed in an appropriate context. Here, we focus on the Ross <span class="hlt">Ice</span> Shelf (RIS), a major component of the West Antarctic <span class="hlt">Ice</span> Sheet system and a feature known to experience <span class="hlt">variable</span> <span class="hlt">ice</span> flux from tributary <span class="hlt">ice</span> streams and glaciers, for example, <span class="hlt">ice</span> stream stagnation and glacier surges. We perturb a model of the Ross <span class="hlt">Ice</span> Shelf with periodic influx variations, <span class="hlt">ice</span> rise and <span class="hlt">ice</span> plain grounding events, and iceberg calving in order to generate transients in the <span class="hlt">ice</span> shelf flow and thickness. Characteristic patterns associated with those perturbations are identified using empirical orthogonal functions (EOFs). The leading EOFs reveal shelf-wide pattern of response to local perturbations that can be interpreted in terms of coupled mass and momentum balance. For example, speed changes on Byrd Glacier cause both thinning and thickening in a broad region that extends to Roosevelt Island. We calculate decay times at various locations for various perturbations and find that mutli-decadal to century time scales are typical. Unique identification of responses to particular forcings may thus be difficlult to achieve and flow divergence cannot be assumed to be constant when interpreting observed changes in <span class="hlt">ice</span> thickness. In reality, perturbations to the <span class="hlt">ice</span> shelf do not occur individually, rather the <span class="hlt">ice</span> shelf contains a history of boundary perturbations. To explore the degree individual perturbations are seperable from their ensemble, EOFs from individual events are combined in pairs and compared against experiments with the same periodic perturbations pairs. Residuals between these EOFs reveal the degree interaction between between disctinct perturbations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Natur.554..351J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Natur.554..351J"><span>Southern Hemisphere climate <span class="hlt">variability</span> forced by Northern Hemisphere <span class="hlt">ice</span>-sheet topography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jones, T. R.; Roberts, W. H. G.; Steig, E. J.; Cuffey, K. M.; Markle, B. R.; White, J. W. C.</p> <p>2018-02-01</p> <p>The presence of large Northern Hemisphere <span class="hlt">ice</span> sheets and reduced greenhouse gas concentrations during the Last Glacial Maximum fundamentally altered global ocean-atmosphere climate dynamics. Model simulations and palaeoclimate records suggest that glacial boundary conditions affected the El Niño-Southern Oscillation, a dominant source of short-term global climate <span class="hlt">variability</span>. Yet little is known about changes in short-term climate <span class="hlt">variability</span> at mid- to high latitudes. Here we use a high-resolution water isotope record from West Antarctica to demonstrate that interannual to decadal climate <span class="hlt">variability</span> at high southern latitudes was almost twice as large at the Last Glacial Maximum as during the ensuing Holocene epoch (the past 11,700 years). Climate model simulations indicate that this increased <span class="hlt">variability</span> reflects an increase in the teleconnection strength between the tropical Pacific and West Antarctica, owing to a shift in the mean location of tropical convection. This shift, in turn, can be attributed to the influence of topography and albedo of the North American <span class="hlt">ice</span> sheets on atmospheric circulation. As the planet deglaciated, the largest and most abrupt decline in teleconnection strength occurred between approximately 16,000 years and 15,000 years ago, followed by a slower decline into the early Holocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.5307W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.5307W"><span>Concentration and <span class="hlt">variability</span> of <span class="hlt">ice</span> nuclei in the subtropical maritime boundary layer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Welti, André; Müller, Konrad; Fleming, Zoë L.; Stratmann, Frank</p> <p>2018-04-01</p> <p>Measurements of the concentration and <span class="hlt">variability</span> of <span class="hlt">ice</span> nucleating particles in the subtropical maritime boundary layer are reported. Filter samples collected in Cabo Verde over the period 2009-2013 are analyzed with a drop freezing experiment with sensitivity to detect the few rare <span class="hlt">ice</span> nuclei active at low supercooling. The data set is augmented with continuous flow diffusion chamber measurements at temperatures below -24 °C from a 2-month field campaign in Cabo Verde in 2016. The data set is used to address the following questions: what are typical concentrations of <span class="hlt">ice</span> nucleating particles active at a certain temperature? What affects their concentration and where are their sources? Concentration of <span class="hlt">ice</span> nucleating particles is found to increase exponentially by 7 orders of magnitude from -5 to -38 °C. Sample-to-sample variation in the steepness of the increase indicates that particles of different origin, with different <span class="hlt">ice</span> nucleation properties (size, composition), contribute to the <span class="hlt">ice</span> nuclei concentration at different temperatures. The concentration of <span class="hlt">ice</span> nuclei active at a specific temperature varies over a range of up to 4 orders of magnitude. The frequency with which a certain <span class="hlt">ice</span> nuclei concentration is measured within this range is found to follow a lognormal distribution, which can be explained by random dilution during transport. To investigate the geographic origin of <span class="hlt">ice</span> nuclei, source attribution of air masses from dispersion modeling is used to classify the data into seven typical conditions. While no source could be attributed to the <span class="hlt">ice</span> nuclei active at temperatures higher than -12 °C, concentrations at lower temperatures tend to be elevated in air masses originating from the Sahara.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120008192','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120008192"><span><span class="hlt">Variability</span> of Surface Temperature and Melt on the Greenland <span class="hlt">Ice</span> Sheet, 2000-2011</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hall, Dorothy K.; Comiso, Josefino, C.; Shuman, Christopher A.; Koenig, Lora S.; DiGirolamo, Nicolo E.</p> <p>2012-01-01</p> <p>Enhanced melting along with surface-temperature increases measured using infrared satellite data, have been documented for the Greenland <span class="hlt">Ice</span> Sheet. Recently we developed a climate-quality data record of <span class="hlt">ice</span>-surface temperature (IST) of the Greenland <span class="hlt">Ice</span> Sheet using the Moderate-Resolution Imaging Spectroradiometer (MODIS) 1ST product -- http://modis-snow-<span class="hlt">ice</span>.gsfc.nasa.gov. Using daily and mean monthly MODIS 1ST maps from the data record we show maximum extent of melt for the <span class="hlt">ice</span> sheet and its six major drainage basins for a 12-year period extending from March of 2000 through December of 2011. The duration of the melt season on the <span class="hlt">ice</span> sheet varies in different drainage basins with some basins melting progressively earlier over the study period. Some (but not all) of the basins also show a progressively-longer duration of melt. The short time of the study period (approximately 12 years) precludes an evaluation of statistically-significant trends. However the dataset provides valuable information on natural <span class="hlt">variability</span> of IST, and on the ability of the MODIS instrument to capture changes in IST and melt conditions indifferent drainage basins of the <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA619700','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA619700"><span>Control Strategy: Wind Energy Powered <span class="hlt">Variable</span> Chiller with Thermal <span class="hlt">Ice</span> Storage</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-12-01</p> <p>New York, 2013. [8] A. Togelou et al., “Wind power forecasting in the absence of historical data,” IEEE trans. on sustainable energy, vol. 3, no...WIND ENERGY POWERED <span class="hlt">VARIABLE</span> CHILLER WITH THERMAL <span class="hlt">ICE</span> STORAGE by Rex A. Boonyobhas December 2014 Thesis Advisor: Anthony J. Gannon Co...AND DATES COVERED December 20 14 Master ’s Thesis 4. TITLE AND SUBTITLE 5. FUNDING NUMBERS CONTROL STRATEGY: WIND ENERGY POWERED <span class="hlt">VARIABLE</span> CHILLER</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21G1187P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21G1187P"><span>Spatial and Temporal Means and <span class="hlt">Variability</span> of Arctic Sea <span class="hlt">Ice</span> Climate Indicators from Satellite Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peng, G.; Meier, W.; Bliss, A. C.; Steele, M.; Dickinson, S.</p> <p>2017-12-01</p> <p>Arctic sea <span class="hlt">ice</span> has been undergoing rapid and accelerated loss since satellite-based measurements became available in late 1970s, especially the summer <span class="hlt">ice</span> coverage. For the Arctic as a whole, the long-term trend for the annual sea <span class="hlt">ice</span> extent (SIE) minimum is about -13.5±2.93 % per decade change relative to the 1979-2015 climate average, while the trends of the annual SIE minimum for the local regions can range from 0 to up to -42 % per decade. This presentation aims to examine and baseline spatial and temporal means and <span class="hlt">variability</span> of Arctic sea <span class="hlt">ice</span> climate indicators, such as the annual SIE minimum and maximum, snow/<span class="hlt">ice</span> melt onset, etc., from a consistent, inter-calibrated, long-term time series of remote sensing sea <span class="hlt">ice</span> data for understanding regional vulnerability and monitoring <span class="hlt">ice</span> state for climate adaptation and risk mitigation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A33E3229I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A33E3229I"><span>A Linkage of Recent Arctic Summer Sea <span class="hlt">Ice</span> and Snowfall <span class="hlt">Variability</span> of Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iwamoto, K.; Honda, M.; Ukita, J.</p> <p>2014-12-01</p> <p>In spite of its mid-latitude location, Japan has a markedly high amount of snowfall, which owes much to the presence of cold air-break from Siberia and thus depends on the strength of the Siberian high and the Aleutian low. With this background this study examines the relationship between interannual <span class="hlt">variability</span> and spatial patterns of snowfall in Japan with large-scale atmospheric and sea <span class="hlt">ice</span> variations. The lag regression map of the winter snowfall in Japan on the time series of the Arctic SIE from the preceding summer shows a seesaw pattern in the snowfall, suggesting an Arctic teleconnection to regional weather. From the EOF analyses conducted on the snowfall distribution in Japan, we identify two modes with physical significance. The NH SIC and SLP regressed on PC1 show a sea <span class="hlt">ice</span> reduction in the Barents and Kara Seas and anomalous strength of the Siberia high as discussed in Honda et al. (2009) and other studies, which support the above notion that the snowfall <span class="hlt">variability</span> of Japan is influenced by Arctic sea <span class="hlt">ice</span> conditions. Another mode is related to the AO/NAO and the hemispheric scale double sea-<span class="hlt">ice</span> seesaw centered over the sub-Arctic region: one between the Labrador and Nordic Seas in the Atlantic and the other between the Okhotsk and Bering Seas from the Pacific as discussed in Ukita et al. (2007). Together, observations point to a significant role of the sea-<span class="hlt">ice</span> in determining mid-latitude regional climate and weather patterns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035675','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035675"><span>Sensitivity of Pliocene <span class="hlt">ice</span> sheets to orbital forcing</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dolan, A.M.; Haywood, A.M.; Hill, D.J.; Dowsett, H.J.; Hunter, S.J.; Lunt, D.J.; Pickering, S.J.</p> <p>2011-01-01</p> <p>The stability of the Earth's major <span class="hlt">ice</span> sheets is a critical uncertainty in predictions of future climate and sea level change. One method of investigating the behaviour of the Greenland and the Antarctic <span class="hlt">ice</span> sheets in a warmer-than-modern climate is to look back at past warm periods of Earth history, for example the Pliocene. This paper presents climate and <span class="hlt">ice</span> sheet modelling results for the mid-Pliocene warm period (mPWP; 3.3 to 3.0 million years ago), which has been identified as a key interval for understanding warmer-than-modern climates (Jansen et al., 2007). Using boundary conditions supplied by the United States Geological Survey PRISM Group (Pliocene Research, Interpretation and Synoptic Mapping), the Hadley Centre coupled ocean–atmosphere climate model (HadCM3) and the British Antarctic Survey <span class="hlt">Ice</span> Sheet Model (BASISM), we show large reductions in the Greenland and East Antarctic <span class="hlt">Ice</span> Sheets (GrIS and EAIS) compared to modern in standard mPWP experiments. We also present the first results illustrating the <span class="hlt">variability</span> of the <span class="hlt">ice</span> sheets due to realistic orbital forcing during the mid-Pliocene. While GrIS <span class="hlt">volumes</span> are lower than modern under even the most extreme (cold) mid-Pliocene orbit (losing at least 35% of its <span class="hlt">ice</span> mass), the EAIS can both grow and shrink, losing up to 20% or gaining up to 10% of its present-day <span class="hlt">volume</span>. The changes in <span class="hlt">ice</span> sheet <span class="hlt">volume</span> incurred by altering orbital forcing alone means that global sea level can vary by more than 25 m during the mid-Pliocene. However, we have also shown that the response of the <span class="hlt">ice</span> sheets to mPWP orbital hemispheric forcing can be in anti-phase, whereby the greatest reductions in EAIS <span class="hlt">volume</span> are concurrent with the smallest reductions of the GrIS. If this anti-phase relationship is in operation throughout the mPWP, then the total eustatic sea level response would be dampened compared to the <span class="hlt">ice</span> sheet fluctuations that are theoretically possible. This suggests that maximum eustatic sea level rise does not</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OcDyn..68..347S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OcDyn..68..347S"><span>High-frequency and meso-scale winter sea-<span class="hlt">ice</span> <span class="hlt">variability</span> in the Southern Ocean in a high-resolution global 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>Stössel, Achim; von Storch, Jin-Song; Notz, Dirk; Haak, Helmuth; Gerdes, Rüdiger</p> <p>2018-03-01</p> <p>This study is on high-frequency temporal <span class="hlt">variability</span> (HFV) and meso-scale spatial <span class="hlt">variability</span> (MSV) of winter sea-<span class="hlt">ice</span> drift in the Southern Ocean simulated with a global high-resolution (0.1°) sea <span class="hlt">ice</span>-ocean model. Hourly model output is used to distinguish MSV characteristics via patterns of mean kinetic energy (MKE) and turbulent kinetic energy (TKE) of <span class="hlt">ice</span> drift, surface currents, and wind stress, and HFV characteristics via time series of raw <span class="hlt">variables</span> and correlations. We find that (1) along the <span class="hlt">ice</span> edge, the MSV of <span class="hlt">ice</span> drift coincides with that of surface currents, in particular such due to ocean eddies; (2) along the coast, the MKE of <span class="hlt">ice</span> drift is substantially larger than its TKE and coincides with the MKE of wind stress; (3) in the interior of the <span class="hlt">ice</span> pack, the TKE of <span class="hlt">ice</span> drift is larger than its MKE, mostly following the TKE pattern of wind stress; (4) the HFV of <span class="hlt">ice</span> drift is dominated by weather events, and, in the absence of tidal currents, locally and to a much smaller degree by inertial oscillations; (5) along the <span class="hlt">ice</span> edge, the curl of the <span class="hlt">ice</span> drift is highly correlated with that of surface currents, mostly reflecting the impact of ocean eddies. Where ocean eddies occur and the <span class="hlt">ice</span> is relatively thin, <span class="hlt">ice</span> velocity is characterized by enhanced relative vorticity, largely matching that of surface currents. Along the <span class="hlt">ice</span> edge, ocean eddies produce distinct <span class="hlt">ice</span> filaments, the realism of which is largely confirmed by high-resolution satellite passive-microwave data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1366510','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1366510"><span><span class="hlt">Variable</span> <span class="hlt">volume</span> combustor with a conical liner support</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>Johnson, Thomas Edward; McConnaughhay, Johnie Franklin; Keener, Chrisophter Paul</p> <p></p> <p>The present application provides a <span class="hlt">variable</span> <span class="hlt">volume</span> combustor for use with a gas turbine engine. The <span class="hlt">variable</span> <span class="hlt">volume</span> combustor may include a liner, a number of micro-mixer fuel nozzles positioned within the liner, and a conical liner support supporting the liner.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP31B2281L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP31B2281L"><span>Insight to Marine Isotope Stage 13 using Late Pleistocene relaxation models of <span class="hlt">ice</span> <span class="hlt">volume</span> and carbon cycle change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lisiecki, L. E.; Herrero, C.; García-Olivares, A.</p> <p>2016-12-01</p> <p>The Marine Isotope Stage (MIS) 13 interglacial is unusual in that warm Northern Hemisphere conditions were accompanied by relatively cool Southern Hemisphere conditions and because it was preceded by a mild glaciation (MIS 14) with less <span class="hlt">ice</span> <span class="hlt">volume</span> and higher CO2 levels than the two preceding glacial maxima. Here we investigate Late Pleistocene glacial cycles, and MIS 13 in particular, using two relaxation models from García-Olivares & Herrero [2013] that describe the relationships between global <span class="hlt">ice</span> <span class="hlt">volume</span> (V), atmospheric CO2 (C) and the extent of the Antarctic <span class="hlt">ice</span> shelves (A). The two models differ in parameterizing deep ocean stratification as either a function of V and A (model 3τ) or as a function of C and A (model LS). Note that global <span class="hlt">ice</span> <span class="hlt">volume</span>, V, is most closely related to Northern hemisphere climate, whereas C and A are most closely related to Antarctic climate. Here we present the results of using a sea level stack [Spratt & Lisiecki, 2016] as the <span class="hlt">ice</span> <span class="hlt">volume</span> tuning target instead of benthic δ18O. We find that tuning to the sea level stack dramatically improves the simulation of MIS 13 in the 3τ model. With the sea level stack, 3τ correctly reproduces the weak amplitudes of MIS 13 and 14 and a double peak in CO2 during MIS 13, whereas the LS model does not reproduce these features using either tuning target. The first peak in CO2 follows a minor <span class="hlt">ice</span> <span class="hlt">volume</span> decrease at 530 kyr but significantly precedes a second, larger sea level rise at 500 kyr. The later sea level rise coincides with a second benthic δ18O decrease and likely triggered the second CO2 peak. This two-step transition to peak interglacial conditions might be caused by deep ocean stratification and Antarctic <span class="hlt">ice</span> cover acting out of phase: weakened stratification produced an initial pulse of CO2 from the deep ocean, but because Antarctic warming was unusually weak, the Antarctic <span class="hlt">ice</span> shelf remained relatively wide and less CO2 than usual was released from the deep ocean. Because 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_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('https://www.ncbi.nlm.nih.gov/pubmed/29515117','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29515117"><span><span class="hlt">Ice-volume</span>-forced erosion of the Chinese Loess Plateau global Quaternary stratotype site.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stevens, T; Buylaert, J-P; Thiel, C; Újvári, G; Yi, S; Murray, A S; Frechen, M; Lu, H</p> <p>2018-03-07</p> <p>The International Commission on Stratigraphy (ICS) utilises benchmark chronostratigraphies to divide geologic time. The reliability of these records is fundamental to understand past global change. Here we use the most detailed luminescence dating age model yet published to show that the ICS chronology for the Quaternary terrestrial type section at Jingbian, desert marginal Chinese Loess Plateau, is inaccurate. There are large hiatuses and depositional changes expressed across a dynamic gully landform at the site, which demonstrates rapid environmental shifts at the East Asian desert margin. We propose a new independent age model and reconstruct monsoon climate and desert expansion/contraction for the last ~250 ka. Our record demonstrates the dominant influence of <span class="hlt">ice</span> <span class="hlt">volume</span> on desert expansion, dust dynamics and sediment preservation, and further shows that East Asian Summer Monsoon (EASM) variation closely matches that of <span class="hlt">ice</span> <span class="hlt">volume</span>, but lags insolation by ~5 ka. These observations show that the EASM at the monsoon margin does not respond directly to precessional forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PNAS..114.3867L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PNAS..114.3867L"><span>Evolution of the early Antarctic <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>Liebrand, Diederik; de Bakker, Anouk T. M.; Beddow, Helen M.; Wilson, Paul A.; Bohaty, Steven M.; Ruessink, Gerben; Pälike, Heiko; Batenburg, Sietske J.; Hilgen, Frederik J.; Hodell, David A.; Huck, Claire E.; Kroon, Dick; Raffi, Isabella; Saes, Mischa J. M.; van Dijk, Arnold E.; Lourens, Lucas J.</p> <p>2017-04-01</p> <p>Understanding the stability of the early Antarctic <span class="hlt">ice</span> cap in the geological past is of societal interest because present-day atmospheric CO2 concentrations have reached values comparable to those estimated for the Oligocene and the Early Miocene epochs. Here we analyze a new high-resolution deep-sea oxygen isotope (δ18O) record from the South Atlantic Ocean spanning an interval between 30.1 My and 17.1 My ago. The record displays major oscillations in deep-sea temperature and Antarctic <span class="hlt">ice</span> <span class="hlt">volume</span> in response to the ˜110-ky eccentricity modulation of precession. Conservative minimum <span class="hlt">ice</span> <span class="hlt">volume</span> estimates show that waxing and waning of at least ˜85 to 110% of the <span class="hlt">volume</span> of the present East Antarctic <span class="hlt">Ice</span> Sheet is required to explain many of the ˜110-ky cycles. Antarctic <span class="hlt">ice</span> sheets were typically largest during repeated glacial cycles of the mid-Oligocene (˜28.0 My to ˜26.3 My ago) and across the Oligocene-Miocene Transition (˜23.0 My ago). However, the high-amplitude glacial-interglacial cycles of the mid-Oligocene are highly symmetrical, indicating a more direct response to eccentricity modulation of precession than their Early Miocene counterparts, which are distinctly asymmetrical—indicative of prolonged <span class="hlt">ice</span> buildup and delayed, but rapid, glacial terminations. We hypothesize that the long-term transition to a warmer climate state with sawtooth-shaped glacial cycles in the Early Miocene was brought about by subsidence and glacial erosion in West Antarctica during the Late Oligocene and/or a change in the <span class="hlt">variability</span> of atmospheric CO2 levels on astronomical time scales that is not yet captured in existing proxy reconstructions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5393229','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5393229"><span>Evolution of the early Antarctic <span class="hlt">ice</span> ages</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>de Bakker, Anouk T. M.; Beddow, Helen M.; Wilson, Paul A.; Bohaty, Steven M.; Pälike, Heiko; Batenburg, Sietske J.; Hilgen, Frederik J.; Hodell, David A.; Huck, Claire E.; Kroon, Dick; Raffi, Isabella; Saes, Mischa J. M.; van Dijk, Arnold E.; Lourens, Lucas J.</p> <p>2017-01-01</p> <p>Understanding the stability of the early Antarctic <span class="hlt">ice</span> cap in the geological past is of societal interest because present-day atmospheric CO2 concentrations have reached values comparable to those estimated for the Oligocene and the Early Miocene epochs. Here we analyze a new high-resolution deep-sea oxygen isotope (δ18O) record from the South Atlantic Ocean spanning an interval between 30.1 My and 17.1 My ago. The record displays major oscillations in deep-sea temperature and Antarctic <span class="hlt">ice</span> <span class="hlt">volume</span> in response to the ∼110-ky eccentricity modulation of precession. Conservative minimum <span class="hlt">ice</span> <span class="hlt">volume</span> estimates show that waxing and waning of at least ∼85 to 110% of the <span class="hlt">volume</span> of the present East Antarctic <span class="hlt">Ice</span> Sheet is required to explain many of the ∼110-ky cycles. Antarctic <span class="hlt">ice</span> sheets were typically largest during repeated glacial cycles of the mid-Oligocene (∼28.0 My to ∼26.3 My ago) and across the Oligocene−Miocene Transition (∼23.0 My ago). However, the high-amplitude glacial−interglacial cycles of the mid-Oligocene are highly symmetrical, indicating a more direct response to eccentricity modulation of precession than their Early Miocene counterparts, which are distinctly asymmetrical—indicative of prolonged <span class="hlt">ice</span> buildup and delayed, but rapid, glacial terminations. We hypothesize that the long-term transition to a warmer climate state with sawtooth-shaped glacial cycles in the Early Miocene was brought about by subsidence and glacial erosion in West Antarctica during the Late Oligocene and/or a change in the <span class="hlt">variability</span> of atmospheric CO2 levels on astronomical time scales that is not yet captured in existing proxy reconstructions. PMID:28348211</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009CG.....35.2145V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009CG.....35.2145V"><span>SteamTables: An approach of multiple <span class="hlt">variable</span> sets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Verma, Mahendra P.</p> <p>2009-10-01</p> <p>Using the IAPWS-95 formulation, an ActiveX component SteamTablesIIE in Visual Basic 6.0 is developed to calculate thermodynamic properties of pure water as a function of two independent intensive <span class="hlt">variables</span>: (1) temperature ( T) or pressure ( P) and (2) T, P, <span class="hlt">volume</span> ( V), internal energy ( U), enthalpy ( H), entropy ( S) or Gibbs free energy ( G). The second <span class="hlt">variable</span> cannot be the same as <span class="hlt">variable</span> 1. Additionally, it calculates the properties along the separation boundaries (i.e., sublimation, saturation, critical isochor, <span class="hlt">ice</span> I melting, <span class="hlt">ice</span> III to <span class="hlt">ice</span> IIV melting and minimum <span class="hlt">volume</span> curves) considering the input parameter as T or P for the <span class="hlt">variable</span> 1. SteamTablesIIE is an extension of the ActiveX component SteamTables implemented earlier considering T (190 to 2000 K) and P (3.23×10 -8 to 10000 MPa) as independent <span class="hlt">variables</span>. It takes into account the following 27 intensive properties: temperature ( T), pressure ( P), fraction, state, <span class="hlt">volume</span> ( V), density ( Den), compressibility factor ( Z0), internal energy ( U), enthalpy ( H), Gibbs free energy ( G), Helmholtz free energy ( A), entropy ( S), heat capacity at constant pressure ( C p), heat capacity at constant <span class="hlt">volume</span> ( C v), coefficient of thermal expansion ( CTE), isothermal compressibility ( Z iso), speed of sound ( VelS), partial derivative of P with T at constant V ( dPdT), partial derivative of T with V at constant P ( dTdV), partial derivative of V with P at constant T ( dVdP), Joule-Thomson coefficient ( JTC), isothermal throttling coefficient ( IJTC), viscosity ( Vis), thermal conductivity ( ThrmCond), surface tension ( SurfTen), Prandtl number ( PrdNum) and dielectric constant ( DielCons).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912539S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912539S"><span>Analysis on <span class="hlt">variability</span> and trend in Antarctic sea <span class="hlt">ice</span> albedo between 1983 and 2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seo, Minji; Kim, Hyun-cheol; Choi, Sungwon; Lee, Kyeong-sang; Han, Kyung-soo</p> <p>2017-04-01</p> <p>Sea <span class="hlt">ice</span> is key parameter in order to understand the cryosphere climate change. Several studies indicate the different trend of sea <span class="hlt">ice</span> between Antarctica and Arctic. Albedo is important factor for understanding the energy budget and factors for observing of environment changes of Cryosphere such as South Pole, due to it mainly covered by <span class="hlt">ice</span> and snow with high albedo value. In this study, we analyzed <span class="hlt">variability</span> and trend of long-term sea <span class="hlt">ice</span> albedo data to understand the changes of sea <span class="hlt">ice</span> over Antarctica. In addiction, sea <span class="hlt">ice</span> albedo researched the relationship with Antarctic oscillation in order to determine the atmospheric influence. We used the sea <span class="hlt">ice</span> albedo data at The Satellite Application Facility on Climate Monitoring and Antarctic Oscillation data at NOAA Climate Prediction Center (CPC). We analyzed the annual trend in albedo using linear regression to understand the spatial and temporal tendency. Antarctic sea <span class="hlt">ice</span> albedo has two spatial trend. Weddle sea / Ross sea sections represent a positive trend (0.26% ˜ 0.04% yr-1) and Bellingshausen Amundsen sea represents a negative trend (- 0.14 ˜ -0.25%yr-1). Moreover, we performed the correlation analysis between albedo and Antarctic oscillation. As a results, negative area indicate correlation coefficient of - 0.3639 and positive area indicates correlation coefficient of - 0.0741. Theses results sea <span class="hlt">ice</span> albedo has regional trend according to ocean. Decreasing sea <span class="hlt">ice</span> trend has negative relationship with Antarctic oscillation, its represent a possibility that sea <span class="hlt">ice</span> influence atmospheric factor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11..773L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11..773L"><span>Regional Greenland accumulation <span class="hlt">variability</span> from Operation <span class="hlt">Ice</span>Bridge airborne accumulation radar</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, Gabriel; Osterberg, Erich; Hawley, Robert; Whitmore, Brian; Marshall, Hans Peter; Box, Jason</p> <p>2017-03-01</p> <p>The mass balance of the Greenland <span class="hlt">Ice</span> Sheet (GrIS) in a warming climate is of critical interest to scientists and the general public in the context of future sea-level rise. An improved understanding of temporal and spatial <span class="hlt">variability</span> of snow accumulation will reduce uncertainties in GrIS mass balance models and improve projections of Greenland's contribution to sea-level rise, currently estimated at 0.089 ± 0.03 m by 2100. Here we analyze 25 NASA Operation <span class="hlt">Ice</span>Bridge accumulation radar flights totaling > 17 700 km from 2013 to 2014 to determine snow accumulation in the GrIS dry snow and percolation zones over the past 100-300 years. <span class="hlt">Ice</span>Bridge accumulation rates are calculated and used to validate accumulation rates from three regional climate models. Averaged over all 25 flights, the RMS difference between the models and <span class="hlt">Ice</span>Bridge accumulation is between 0.023 ± 0.019 and 0.043 ± 0.029 m w.e. a-1, although each model shows significantly larger differences from <span class="hlt">Ice</span>Bridge accumulation on a regional basis. In the southeast region, for example, the Modèle Atmosphérique Régional (MARv3.5.2) overestimates by an average of 20.89 ± 6.75 % across the drainage basin. Our results indicate that these regional differences between model and <span class="hlt">Ice</span>Bridge accumulation are large enough to significantly alter GrIS surface mass balance estimates. Empirical orthogonal function analysis suggests that the first two principal components account for 33 and 19 % of the variance, and correlate with the Atlantic Multidecadal Oscillation (AMO) and wintertime North Atlantic Oscillation (NAO), respectively. Regions that disagree strongest with climate models are those in which we have the fewest <span class="hlt">Ice</span>Bridge data points, requiring additional in situ measurements to verify model uncertainties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP42B..06N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP42B..06N"><span>The Role Of Orbital Forcing On Polar <span class="hlt">Ice</span> <span class="hlt">Volume</span> And Global Sea-Level During The Late Pliocene (3.3-.2.6 Ma)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Naish, T.; Grant, G.; Dunbar, G. B.; Patterson, M. O.; Kominz, M. A.; Stocchi, P.</p> <p>2017-12-01</p> <p>Challenges remain concerning the potentially intractable problem of constraining the absolute magnitude of Pliocene eustatic sea-level change, and the role of orbital forcing on the frequency of <span class="hlt">ice</span> <span class="hlt">volume</span>/sea-level change is widely debated. Here, we present three new high-resolution geological archives for the MPWP: (i) <span class="hlt">ice</span>-berg rafted debris (IBRD) mass accumulation rates from deep ocean sediment core (IODP U1361) off the Wilkes Margin of Antarctica recording fluctuations in the East Antarctic <span class="hlt">ice</span> sheet; (ii) a continuous shallow-marine record of sea-level change from the Wanganui Basin, New Zealand; and (iii) a record sea-level-controlled terrigenous sedimentation (IODP 1124) to the deep ocean on Hikurangi margin of New Zealand. All three records are dominated by precession-paced cyclicity ( 20ka) in-phase with high-latitude southern hemisphere insolation between 3.3M-2.9Ma, and provide insights into orbital-forcing of <span class="hlt">ice</span> <span class="hlt">volume</span> and sea-level independent of the benthic oxygen isotope records. Moreover, we have back-stripped the Wanganui record to reveal glacial-interglacial sea-level changes of 20±10m amplitude. We conclude that during this interval, precession-paced Antarctic <span class="hlt">ice</span> <span class="hlt">volume</span> changes largely drove global glacial-interglacial sea-level fluctuations, in the absence of a significant northern hemisphere <span class="hlt">ice</span> <span class="hlt">volume</span> contribution. Prior to 3.3Ma, proxy data from IODP U1361 and ANDRILL 1-A records extending back to 5Ma, show that the Antarctic margin experienced warmer ocean temperatures, a lack of perennial sea-<span class="hlt">ice</span>, and fluctuations in <span class="hlt">ice</span> extent paced by obliquity. The emergence of precession at 3.3Ma coincident with the M2 glaciation in the benthic d18O record, also coincides with continent-wide cooling, <span class="hlt">ice</span> expansion and the development of extensive seasonal sea-<span class="hlt">ice</span> around Antarctica. We argue that a melt threshold response to orbital forcing was crossed, whereby Antarctic <span class="hlt">ice</span> sheet melt was restricted to peak austral summer insolation (precession</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP11E..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP11E..02G"><span>Simulating a Dynamic Antarctic <span class="hlt">Ice</span> Sheet in the Early to Middle Miocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gasson, E.; DeConto, R.; Pollard, D.; Levy, R. H.</p> <p>2015-12-01</p> <p>There are a variety of sources of geological data that suggest major variations in the <span class="hlt">volume</span> and extent of the Antarctic <span class="hlt">ice</span> sheet during the early to middle Miocene. Simulating such <span class="hlt">variability</span> using coupled climate-<span class="hlt">ice</span> sheet models is problematic due to a strong hysteresis effect caused by height-mass balance feedback and albedo feedback. This results in limited retreat of the <span class="hlt">ice</span> sheet once it has reached the continental size, as likely occurred prior to the Miocene. Proxy records suggest a relatively narrow range of atmospheric CO2 during the early to middle Miocene, which exacerbates this problem. We use a new climate forcing which accounts for <span class="hlt">ice</span> sheet-climate feedbacks through an asynchronous GCM-RCM coupling, which is able to better resolve the narrow Antarctic ablation zone in warm climate simulations. When combined with recently suggested mechanisms for retreat into subglacial basins due to <span class="hlt">ice</span> shelf hydrofracture and <span class="hlt">ice</span> cliff failure, we are able to simulate large-scale <span class="hlt">variability</span> of the Antarctic <span class="hlt">ice</span> sheet in the Miocene. This <span class="hlt">variability</span> is equivalent to a seawater oxygen isotope signal of ~0.5 ‰, or a sea level equivalent change of ~35 m, for a range of atmospheric CO2 between 280 - 500 ppm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.U22A..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.U22A..01S"><span>Climate <span class="hlt">Variability</span>, Melt-Flow Acceleration, and <span class="hlt">Ice</span> Quakes at the Western Slope 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>Steffen, K.; Zwally, J. H.; Rial, J. A.; Behar, A.; Huff, R.</p> <p>2006-12-01</p> <p>The Greenland <span class="hlt">ice</span> sheet experienced surface melt increase over the past 15 years with record melt years in 1987, 1991, 1998, 2002 and 2005. For the western part of the <span class="hlt">ice</span> sheet the melt area increased by 30 percent (1979-2005). Monthly mean air temperatures increased in spring and fall by 0.23 deg. C per year since 1990, extending the length of melt and total ablation. Winter air temperatures increased by as much as 0.5 deg. C per year during the past 15 years. The equilibrium line altitude ranged between 400 and 1530 m above sea level at 70 deg. north along the western slope of the <span class="hlt">ice</span> sheet for the past 15 years, equaling a horizontal distance of 100 km. The ELA has been below the Swiss Camp (1100 m elevation) in the nineties, and since 1997 moved above the Swiss Camp height. An increase in ELA leads to an increase in melt water run-off which has been verified by regional model studies (high-resolution re-analysis). Interannual <span class="hlt">variability</span> of snow accumulation varies from 0.3 to 2.0 m, whereas snow and <span class="hlt">ice</span> ablation ranges from 0 to 1.5 m water equivalent at Swiss Camp during 1990-2005. A GPS network (10 stations) monitors <span class="hlt">ice</span> velocity, acceleration, and surface height change at high temporal resolution throughout the year. The network covers a range of 500 and 1500 m above sea level, close to the Ilulissat Icefjord World Heritage region. The <span class="hlt">ice</span> sheet continued to accelerate during the height of the melt season with short-term velocity increases up to 100 percent, and vertical uplift rates of 0.5 m. There seems to be a good correlation between the change in <span class="hlt">ice</span> velocity and total surface melt, suggesting that melt water penetrates to great depth through moulins and cracks, lubricating the bottom of the <span class="hlt">ice</span> sheet. A new bore-hole video movie will be shown from a 110 m deep moulin close to Swiss Camp. A PASSCAL array of 10 portable, 3-component seismic stations deployed around Swiss Camp from May to August 2006 detected numerous microearthquakes within the <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900061679&hterms=CO2+H2O&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DCO2%2BH2O','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900061679&hterms=CO2+H2O&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DCO2%2BH2O"><span>The <span class="hlt">volume</span>- and surface-binding energies of <span class="hlt">ice</span> systems containing CO, CO2, and H2O</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sandford, Scott A.; Allamandola, Louis J.</p> <p>1990-01-01</p> <p>Laboratory-measured, temperature-dependent sticking efficiencies are presently used to derive the surface-binding energies of CO and CO2 on H2O-rich <span class="hlt">ices</span>, with a view to determining the condensation and vaporization properties of these systems as well as to the measured energies' implications for both cometary behavior and the evolution of interstellar <span class="hlt">ices</span>. The molecular <span class="hlt">volume</span> and the surface binding energies are not found to be necessarily related on the basis of simple nearest-neighbor scaling in surface and bulk sites; this may be due to the physical constraints associated with matrix structure-associated physical constraints, which sometimes dominate the <span class="hlt">volume</span>-binding energies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19937284','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19937284"><span>Reduced pressure <span class="hlt">ice</span> fog technique for controlled <span class="hlt">ice</span> nucleation during freeze-drying.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Patel, Sajal M; Bhugra, Chandan; Pikal, Michael J</p> <p>2009-01-01</p> <p>A method to achieve controlled <span class="hlt">ice</span> nucleation during the freeze-drying process using an <span class="hlt">ice</span> fog technique was demonstrated in an earlier report. However, the time required for nucleation was about 5 min, even though only one shelf was used, which resulted in Ostwald ripening (annealing) in some of the vials that nucleated earlier than the others. As a result, the <span class="hlt">ice</span> structure was not optimally uniform in all the vials. The objective of the present study is to introduce a simple variation of the <span class="hlt">ice</span> fog method whereby a reduced pressure in the chamber is utilized to allow more rapid and uniform freezing which is also potentially easier to scale up. Experiments were conducted on a lab scale freeze dryer with sucrose as model compound at different concentration, product load, and fill <span class="hlt">volume</span>. Product resistance during primary drying was measured using manometric temperature measurement. Specific surface area of the freeze-dried cake was also determined. No difference was observed either in average product resistance or specific surface area for the different experimental conditions studied, indicating that with use of the reduced pressure <span class="hlt">ice</span> fog technique, the solutions nucleated at very nearly the same temperature (-10 degrees C). The striking feature of the "Reduced Pressure <span class="hlt">Ice</span> Fog Technique" is the rapid <span class="hlt">ice</span> nucleation (less than a minute) under conditions where the earlier procedure required about 5 min; hence, effects of <span class="hlt">variable</span> Ostwald ripening were not an issue.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120009528','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120009528"><span>Antarctic Sea <span class="hlt">Ice</span> <span class="hlt">Variability</span> and Trends, 1979-2010</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, C. L.; Cavalieri, D. J.</p> <p>2012-01-01</p> <p>In sharp contrast to the decreasing sea <span class="hlt">ice</span> coverage of the Arctic, in the Antarctic the sea <span class="hlt">ice</span> cover has, on average, expanded since the late 1970s. More specifically, satellite passive-microwave data for the period November 1978 - December 2010 reveal an overall positive trend in <span class="hlt">ice</span> extents of 17,100 +/- 2,300 square km/yr. Much of the increase, at 13,700 +/- 1,500 square km/yr, has occurred in the region of the Ross Sea, with lesser contributions from the Weddell Sea and Indian Ocean. One region, that of the Bellingshausen/Amundsen Seas, has, like the Arctic, instead experienced significant sea <span class="hlt">ice</span> decreases, with an overall <span class="hlt">ice</span> extent trend of -8,200 +/- 1,200 square km/yr. When examined through the annual cycle over the 32-year period 1979-2010, the Southern Hemisphere sea <span class="hlt">ice</span> cover as a whole experienced positive <span class="hlt">ice</span> extent trends in every month, ranging in magnitude from a low of 9,100 +/- 6,300 square km/yr in February to a high of 24,700 +/- 10,000 square km/yr in May. The Ross Sea and Indian Ocean also had positive trends in each month, while the Bellingshausen/Amundsen Seas had negative trends in each month, and the Weddell Sea and Western Pacific Ocean had a mixture of positive and negative trends. Comparing <span class="hlt">ice</span>-area results to <span class="hlt">ice</span>-extent results, in each case the <span class="hlt">ice</span>-area trend has the same sign as the <span class="hlt">ice</span>-extent trend, but differences in the magnitudes of the two trends identify regions with overall increasing <span class="hlt">ice</span> concentrations and others with overall decreasing <span class="hlt">ice</span> concentrations. The strong pattern of decreasing <span class="hlt">ice</span> coverage in the Bellingshausen/Amundsen Seas region and increasing <span class="hlt">ice</span> coverage in the Ross Sea region is suggestive of changes in atmospheric circulation. This is a key topic for future research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..43.9113J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..43.9113J"><span>How predictable is the timing of a summer <span class="hlt">ice</span>-free Arctic?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jahn, Alexandra; Kay, Jennifer E.; Holland, Marika M.; Hall, David M.</p> <p>2016-09-01</p> <p>Climate model simulations give a large range of over 100 years for predictions of when the Arctic could first become <span class="hlt">ice</span> free in the summer, and many studies have attempted to narrow this uncertainty range. However, given the chaotic nature of the climate system, what amount of spread in the prediction of an <span class="hlt">ice</span>-free summer Arctic is inevitable? Based on results from large ensemble simulations with the Community Earth System Model, we show that internal <span class="hlt">variability</span> alone leads to a prediction uncertainty of about two decades, while scenario uncertainty between the strong (Representative Concentration Pathway (RCP) 8.5) and medium (RCP4.5) forcing scenarios adds at least another 5 years. Common metrics of the past and present mean sea <span class="hlt">ice</span> state (such as <span class="hlt">ice</span> extent, <span class="hlt">volume</span>, and thickness) as well as global mean temperatures do not allow a reduction of the prediction uncertainty from internal <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998JApMe..37...23S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998JApMe..37...23S"><span><span class="hlt">Variability</span> of AVHRR-Derived Clear-Sky Surface Temperature over 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>Stroeve, Julienne; Steffen, Konrad</p> <p>1998-01-01</p> <p>The Advanced Very High Resolution Radiometer is used to derive surface temperatures for one satellite pass under clear skies over the Greenland <span class="hlt">ice</span> sheet from 1989 through 1993. The results of these temperatures are presented as monthly means, and their spatial and temporal <span class="hlt">variability</span> are discussed. Accuracy of the dry snow surface temperatures is estimated to be better than 1 K during summer. This error is expected to increase during polar night due to problems in cloud identification. Results indicate the surface temperature of the Greenland <span class="hlt">ice</span> sheet is strongly dominated by topography, with minimum surface temperatures associated with the high elevation regions. In the summer, maximum surface temperatures occur during July along the western coast and southern tip of the <span class="hlt">ice</span> sheet. Minimum temperatures are found at the summit during summer and move farther north during polar night. Large interannual <span class="hlt">variability</span> in surface temperatures occurs during winter associated with katabatic storm events. Summer temperatures show little variation, although 1992 stands out as being colder than the other years. The reason for the lower temperatures during 1992 is believed to be a result of the 1991 eruption of Mount Pinatubo.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130013431','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130013431"><span>On the <span class="hlt">Ice</span> Nucleation Spectrum</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barahona, D.</p> <p>2012-01-01</p> <p>This work presents a novel formulation of the <span class="hlt">ice</span> nucleation spectrum, i.e. the function relating the <span class="hlt">ice</span> crystal concentration to cloud formation conditions and aerosol properties. The new formulation is physically-based and explicitly accounts for the dependency of the <span class="hlt">ice</span> crystal concentration on temperature, supersaturation, cooling rate, and particle size, surface area and composition. This is achieved by introducing the concepts of <span class="hlt">ice</span> nucleation coefficient (the number of <span class="hlt">ice</span> germs present in a particle) and nucleation probability dispersion function (the distribution of <span class="hlt">ice</span> nucleation coefficients within the aerosol population). The new formulation is used to generate <span class="hlt">ice</span> nucleation parameterizations for the homogeneous freezing of cloud droplets and the heterogeneous deposition <span class="hlt">ice</span> nucleation on dust and soot <span class="hlt">ice</span> nuclei. For homogeneous freezing, it was found that by increasing the dispersion in the droplet <span class="hlt">volume</span> distribution the fraction of supercooled droplets in the population increases. For heterogeneous <span class="hlt">ice</span> nucleation the new formulation consistently describes singular and stochastic behavior within a single framework. Using a fundamentally stochastic approach, both cooling rate independence and constancy of the <span class="hlt">ice</span> nucleation fraction over time, features typically associated with singular behavior, were reproduced. Analysis of the temporal dependency of the <span class="hlt">ice</span> nucleation spectrum suggested that experimental methods that measure the <span class="hlt">ice</span> nucleation fraction over few seconds would tend to underestimate the <span class="hlt">ice</span> nuclei concentration. It is shown that inferring the aerosol heterogeneous <span class="hlt">ice</span> nucleation properties from measurements of the onset supersaturation and temperature may carry significant error as the <span class="hlt">variability</span> in <span class="hlt">ice</span> nucleation properties within the aerosol population is not accounted for. This work provides a simple and rigorous <span class="hlt">ice</span> nucleation framework where theoretical predictions, laboratory measurements and field campaign data can be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28116688','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28116688"><span>Spatiotemporal <span class="hlt">variability</span> in surface energy balance across tundra, snow and <span class="hlt">ice</span> in Greenland.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lund, Magnus; Stiegler, Christian; Abermann, Jakob; Citterio, Michele; Hansen, Birger U; van As, Dirk</p> <p>2017-02-01</p> <p>The surface energy balance (SEB) is essential for understanding the coupled cryosphere-atmosphere system in the Arctic. In this study, we investigate the spatiotemporal <span class="hlt">variability</span> in SEB across tundra, snow and <span class="hlt">ice</span>. During the snow-free period, the main energy sink for <span class="hlt">ice</span> sites is surface melt. For tundra, energy is used for sensible and latent heat flux and soil heat flux leading to permafrost thaw. Longer snow-free period increases melting of the Greenland <span class="hlt">Ice</span> Sheet and glaciers and may promote tundra permafrost thaw. During winter, clouds have a warming effect across surface types whereas during summer clouds have a cooling effect over tundra and a warming effect over <span class="hlt">ice</span>, reflecting the spatial variation in albedo. The complex interactions between factors affecting SEB across surface types remain a challenge for understanding current and future conditions. Extended monitoring activities coupled with modelling efforts are essential for assessing the impact of warming in the Arctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1364126','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1364126"><span>CICE, The Los Alamos Sea <span class="hlt">Ice</span> 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>Hunke, Elizabeth; Lipscomb, William; Jones, Philip</p> <p></p> <p>The Los Alamos sea <span class="hlt">ice</span> model (CICE) is the result of an effort to develop a computationally efficient sea <span class="hlt">ice</span> component for a fully coupled atmosphere–land–ocean–<span class="hlt">ice</span> global climate model. It was originally designed to be compatible with the Parallel Ocean Program (POP), an ocean circulation model developed at Los Alamos National Laboratory for use on massively parallel computers. CICE has several interacting components: a vertical thermodynamic model that computes local growth rates of snow and <span class="hlt">ice</span> due to vertical conductive, radiative and turbulent fluxes, along with snowfall; an elastic-viscous-plastic model of <span class="hlt">ice</span> dynamics, which predicts the velocity field of themore » <span class="hlt">ice</span> pack based on a model of the material strength of the <span class="hlt">ice</span>; an incremental remapping transport model that describes horizontal advection of the areal concentration, <span class="hlt">ice</span> and snow <span class="hlt">volume</span> and other state <span class="hlt">variables</span>; and a ridging parameterization that transfers <span class="hlt">ice</span> among thickness categories based on energetic balances and rates of strain. It also includes a biogeochemical model that describes evolution of the <span class="hlt">ice</span> ecosystem. The CICE sea <span class="hlt">ice</span> model is used for climate research as one component of complex global earth system models that include atmosphere, land, ocean and biogeochemistry components. It is also used for operational sea <span class="hlt">ice</span> forecasting in the polar regions and in numerical weather prediction models.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP24A..05X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP24A..05X"><span><span class="hlt">Variability</span> in Organic-Carbon Sources and Sea-<span class="hlt">Ice</span> Coverage North of Iceland (Subarctic) During the Past 15,000 Years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiao, X.; Zhao, M.; Knudsen, K. L.; Eiriksson, J.; Gudmundsdottir, E. R.; Jiang, H.; Guo, Z.</p> <p>2017-12-01</p> <p>Sea <span class="hlt">ice</span>, prevailing in the polar region and characterized by distinct seasonal and interannual <span class="hlt">variability</span>, plays a pivotal role in Earth's climate system (Thomas and Dieckmann, 2010). Studies of spatial and temporal changes in modern and past sea-<span class="hlt">ice</span> occurrence may help to understand the processes controlling the recent decrease in Arctic sea-<span class="hlt">ice</span> cover. Here, we determined the concentrations of sea-<span class="hlt">ice</span> diatom-derived biomarker "IP25" (monoene highly-branched isoprenoid with 25 carbon atom; Belt et al., 2007), phytoplankton-derived biomarker brassicasterol and terrigenous biomarker long-chain n-alkanols in a sediment core from the North Icelandic shelf to reconstruct the high-resolution sea-<span class="hlt">ice</span> <span class="hlt">variability</span> and the organic-matter sources during the past 15,000 years. During the Bølling/Allerød, the North Icelandic shelf was characterized by extensive spring sea-<span class="hlt">ice</span> cover linked to reduced flow of warm Atlantic Water and dominant Polar water influence; the input of terrestrial and sea-<span class="hlt">ice</span> organic matters was high while the marine organic matter derived from phytoplankton productivity was low. Prolonged sea-<span class="hlt">ice</span> cover with occasional occurrence of seasonal sea <span class="hlt">ice</span> prevailed during the Younger Dryas interrupted by a brief interval of enhanced Irminger Current; the organic carbon input from sea-<span class="hlt">ice</span> productivity, terrestrial matter and phytoplankton productivity all decreased. The seasonal sea <span class="hlt">ice</span> decreased gradually from the Younger Dryas to the onset of the Holocene corresponding to increasing insolation. Therefore, the sea-<span class="hlt">ice</span> productivity decreased but the phytoplankton productivity increased during this time interval. The biomarker records from this sediment core give insights into the <span class="hlt">variability</span> in sea <span class="hlt">ice</span> and organic-carbon sources in the Arctic marginal area during the last deglacial and Holocene. References Belt, S.T., Massé, G., Rowland, S.J., Poulin, M., Michel, C., LeBlanc, B., 2007. A novel chemical fossil of palaeo sea <span class="hlt">ice</span>: IP25. Org. Geochem. 38, 16</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110015207','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110015207"><span>Regional Changes in the Sea <span class="hlt">Ice</span> Cover and <span class="hlt">Ice</span> Production in the Antarctic</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comiso, Josefino C.</p> <p>2011-01-01</p> <p>Coastal polynyas around the Antarctic continent have been regarded as sea <span class="hlt">ice</span> factories because of high <span class="hlt">ice</span> production rates in these regions. The observation of a positive trend in the extent of Antarctic sea <span class="hlt">ice</span> during the satellite era has been intriguing in light of the observed rapid decline of the <span class="hlt">ice</span> extent in the Arctic. The results of analysis of the time series of passive microwave data indicate large regional <span class="hlt">variability</span> with the trends being strongly positive in the Ross Sea, strongly negative in the Bellingshausen/Amundsen Seas and close to zero in the other regions. The atmospheric circulation in the Antarctic is controlled mainly by the Southern Annular Mode (SAM) and the marginal <span class="hlt">ice</span> zone around the continent shows an alternating pattern of advance and retreat suggesting the presence of a propagating wave (called Antarctic Circumpolar Wave) around the circumpolar region. The results of analysis of the passive microwave data suggest that the positive trend in the Antarctic sea <span class="hlt">ice</span> cover could be caused primarily by enhanced <span class="hlt">ice</span> production in the Ross Sea that may be associated with more persistent and larger coastal polynyas in the region. Over the Ross Sea shelf, analysis of sea <span class="hlt">ice</span> drift data from 1992 to 2008 yields a positive rate-of-increase in the net <span class="hlt">ice</span> export of about 30,000 km2 per year. For a characteristic <span class="hlt">ice</span> thickness of 0.6 m, this yields a <span class="hlt">volume</span> transport of about 20 km3/year, which is almost identical, within error bars, to our estimate of the trend in <span class="hlt">ice</span> production. In addition to the possibility of changes in SAM, modeling studies have also indicated that the ozone hole may have a role in that it causes the deepening of the lows in the western Antarctic region thereby causing strong winds to occur offthe Ross-<span class="hlt">ice</span> shelf.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP43B1345K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP43B1345K"><span>Antarctic Circumpolar Current Dynamics and Their Relation to Antarctic <span class="hlt">Ice</span> Sheet and Perennial Sea-<span class="hlt">Ice</span> <span class="hlt">Variability</span> in the Central Drake Passage During the Last Climate Cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuhn, G.; Wu, S.; Hass, H. C.; Klages, J. P.; Zheng, X.; Arz, H. W.; Esper, O.; Hillenbrand, C. D.; Lange, C.; Lamy, F.; Lohmann, G.; Müller, J.; McCave, I. N. N.; Nürnberg, D.; Roberts, J.; Tiedemann, R.; Timmermann, A.; Titschack, J.; Zhang, X.</p> <p>2017-12-01</p> <p>The evolution of the Antarctic <span class="hlt">Ice</span> Sheet during the last climate cycle and the interrelation to global atmospheric and ocean circulation remains controversial and plays an important role for our understanding of <span class="hlt">ice</span> sheet response to modern global warming. The timing and sequence of deglacial warming is relevant for understanding the <span class="hlt">variability</span> and sensitivity of the Antarctic <span class="hlt">Ice</span> Sheet to climatic changes, and the continuing rise of atmospheric greenhouse gas concentrations. The Antarctic <span class="hlt">Ice</span> Sheet is a pivotal component of the global water budget. Freshwater fluxes from the <span class="hlt">ice</span> sheet may affect the Antarctic Circumpolar Current (ACC), which is strongly impacted by the westerly wind belt in the Southern Hemisphere (SHWW) and constricted to its narrowest extent in the Drake Passage. The flow of ACC water masses through Drake Passage is, therefore, crucial for advancing our understanding of the Southern Ocean's role in global meridional overturning circulation and global climate change. In order to address orbital and millennial-scale <span class="hlt">variability</span> of the Antarctic <span class="hlt">ice</span> sheet and the ACC, we applied a multi-proxy approach on a sediment core from the central Drake Passage including grain size, iceberg-rafted debris, mineral dust, bulk chemical and mineralogical composition, and physical properties. In combination with already published and new sediment records from the Drake Passage and Scotia Sea, as well as high-resolution data from Antarctic <span class="hlt">ice</span> cores (WDC, EDML), we now have evidence that during glacial times a more northerly extent of the perennial sea-<span class="hlt">ice</span> zone decreased ACC current velocities in the central Drake Passage. During deglaciation the SHWW shifted southwards due to a decreasing temperature gradient between subtropical and polar latitudes caused by sea <span class="hlt">ice</span> and <span class="hlt">ice</span> sheet decline. This in turn caused Southern Hemisphere warming, a more vigorous ACC, stronger Southern Ocean ventilation, and warm Circumpolar Deep Water (CDW) upwelling on Antarctic shelves</p> </li> </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/2010EGUGA..12.6551F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.6551F"><span>Constraints on <span class="hlt">ice</span> <span class="hlt">volume</span> changes of the WAIS and Ross <span class="hlt">Ice</span> Shelf since the LGM based on cosmogenic exposure ages in the Darwin-Hatherton glacial system of the Transantarctic Mountains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fink, David; Storey, Bryan; Hood, David; Joy, Kurt; Shulmeister, James</p> <p>2010-05-01</p> <p>Quantitative assessment of the spatial and temporal scale of <span class="hlt">ice</span> <span class="hlt">volume</span> change of the West Antarctic <span class="hlt">ice</span> sheet (WAIS) and Ross <span class="hlt">Ice</span> Shelf since the last glacial maximum (LGM) ~20 ka is essential to accurately predict <span class="hlt">ice</span> sheet response to current and future climate change. Although global sea level rose by approximately 120 metres since the LGM, the contribution of polar <span class="hlt">ice</span> sheets is uncertain and the timing of any such contribution is controversial. Mackintosh et al (2007) suggest that sectors of the EAIS, similar to those studied at Framnes Mountains where the <span class="hlt">ice</span> sheet slowly calves at coastal margins, have made marginal contributions to global sea-level rise between 13 and 7 ka. In contrast, Stone et al (2003) document continuing WAIS decay during the mid-late Holocene, raising the question of what was the response of the WAIS since LGM and into the Holocene. Terrestrial evidence is restricted to sparse coastal oasis and <span class="hlt">ice</span> free mountains which archive limits of former <span class="hlt">ice</span> advances. Mountain ranges flanking the Darwin-Hatherton glaciers exhibit well-defined moraines, weathering signatures, boulder rich plateaus and glacial tills, which preserve the evidence of advance and retreat of the <span class="hlt">ice</span> sheet during previous glacial cycles. Previous studies suggest a WAIS at the LGM in this location to be at least 1,000 meters thicker than today. As part of the New Zealand Latitudinal Gradient Project along the Transantarctic, we collected samples for cosmogenic exposure dating at a) Lake Wellman area bordering the Hatherton Glacier, (b) Roadend Nunatak at the confluence of the Darwin and Hatherton glaciers and (c) Diamond Hill which is positioned at the intersection of the Ross <span class="hlt">Ice</span> Shelf and Darwin Glacier outlet. While the technique of exposure dating is very successful in mid-latitude alpine glacier systems, it is more challenging in polar <span class="hlt">ice</span>-sheet regions due to the prevalence of cold-based <span class="hlt">ice</span> over-riding events and absence of outwash processes which removes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850038332&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=19850038332&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmarginal"><span>A coupled <span class="hlt">ice</span>-ocean model of <span class="hlt">ice</span> breakup and banding in the marginal <span class="hlt">ice</span> zone</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smedstad, O. M.; Roed, L. P.</p> <p>1985-01-01</p> <p>A coupled <span class="hlt">ice</span>-ocean numerical model for the marginal <span class="hlt">ice</span> zone is considered. The model consists of a nonlinear sea <span class="hlt">ice</span> model and a two-layer (reduced gravity) ocean model. The dependence of the upwelling response on wind stress direction is discussed. The results confirm earlier analytical work. It is shown that there exist directions for which there is no upwelling, while other directions give maximum upwelling in terms of the <span class="hlt">volume</span> of uplifted water. The <span class="hlt">ice</span> and ocean is coupled directly through the stress at the <span class="hlt">ice</span>-ocean interface. An interesting consequence of the coupling is found in cases when the <span class="hlt">ice</span> edge is almost stationary. In these cases the <span class="hlt">ice</span> tends to break up a few tenths of kilometers inside of the <span class="hlt">ice</span> edge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70031764','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70031764"><span>Fluctuating Arctic Sea <span class="hlt">ice</span> thickness changes estimated by an in situ learned and empirically forced neural network model</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Belchansky, G.I.; Douglas, David C.; Platonov, Nikita G.</p> <p>2008-01-01</p> <p>Sea <span class="hlt">ice</span> thickness (SIT) is a key parameter of scientific interest because understanding the natural spatiotemporal <span class="hlt">variability</span> of <span class="hlt">ice</span> thickness is critical for improving global climate models. In this paper, changes in Arctic SIT during 1982-2003 are examined using a neural network (NN) algorithm trained with in situ submarine <span class="hlt">ice</span> draft and surface drilling data. For each month of the study period, the NN individually estimated SIT of each <span class="hlt">ice</span>-covered pixel (25-km resolution) based on seven geophysical parameters (four shortwave and longwave radiative fluxes, surface air temperature, <span class="hlt">ice</span> drift velocity, and <span class="hlt">ice</span> divergence/convergence) that were cumulatively summed at each monthly position along the pixel's previous 3-yr drift track (or less if the <span class="hlt">ice</span> was <3 yr old). Average January SIT increased during 1982-88 in most regions of the Arctic (+7.6 ?? 0.9 cm yr-1), decreased through 1996 Arctic-wide (-6.1 ?? 1.2 cm yr-1), then modestly increased through 2003 mostly in the central Arctic (+2.1 ?? 0.6 cm yr-1). Net <span class="hlt">ice</span> <span class="hlt">volume</span> change in the Arctic Ocean from 1982 to 2003 was negligible, indicating that cumulative <span class="hlt">ice</span> growth had largely replaced the estimated 45 000 km3 of <span class="hlt">ice</span> lost by cumulative export. Above 65??N, total annual <span class="hlt">ice</span> <span class="hlt">volume</span> and interannual <span class="hlt">volume</span> changes were correlated with the Arctic Oscillation (AO) at decadal and annual time scales, respectively. Late-summer <span class="hlt">ice</span> thickness and total <span class="hlt">volume</span> varied proportionally until the mid-1990s, but <span class="hlt">volume</span> did not increase commensurate with the thickening during 1996-2002. The authors speculate that decoupling of the <span class="hlt">ice</span> thickness-<span class="hlt">volume</span> relationship resulted from two opposing mechanisms with different latitudinal expressions: a recent quasi-decadal shift in atmospheric circulation patterns associated with the AO's neutral state facilitated <span class="hlt">ice</span> thickening at high latitudes while anomalously warm thermal forcing thinned and melted the <span class="hlt">ice</span> cap at its periphery. ?? 2008 American Meteorological Society.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1365483','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1365483"><span>County-Level Climate Uncertainty for Risk Assessments: <span class="hlt">Volume</span> 23 Appendix V - Forecast Sea <span class="hlt">Ice</span> Thickness</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>Backus, George A.; Lowry, Thomas Stephen; Jones, Shannon M.</p> <p>2017-04-01</p> <p>This report uses the CMIP5 series of climate model simulations to produce country- level uncertainty distributions for use in socioeconomic risk assessments of climate change impacts. It provides appropriate probability distributions, by month, for 169 countries and autonomous-areas on temperature, precipitation, maximum temperature, maximum wind speed, humidity, runoff, soil moisture and evaporation for the historical period (1976-2005), and for decadal time periods to 2100. It also provides historical and future distributions for the Arctic region on <span class="hlt">ice</span> concentration, <span class="hlt">ice</span> thickness, age of <span class="hlt">ice</span>, and <span class="hlt">ice</span> ridging in 15-degree longitude arc segments from the Arctic Circle to 80 degrees latitude, plusmore » two polar semicircular regions from 80 to 90 degrees latitude. The uncertainty is meant to describe the lack of knowledge rather than imprecision in the physical simulation because the emphasis is on unfalsified risk and its use to determine potential socioeconomic impacts. The full report is contained in 27 <span class="hlt">volumes</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1367443','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1367443"><span>County-Level Climate Uncertainty for Risk Assessments: <span class="hlt">Volume</span> 24 Appendix W - Historical Sea <span class="hlt">Ice</span> Age.</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>Backus, George A.; Lowry, Thomas Stephen; Jones, Shannon M</p> <p>2017-05-01</p> <p>This report uses the CMIP5 series of climate model simulations to produce country- level uncertainty distributions for use in socioeconomic risk assessments of climate change impacts. It provides appropriate probability distributions, by month, for 169 countries and autonomous-areas on temperature, precipitation, maximum temperature, maximum wind speed, humidity, runoff, soil moisture and evaporation for the historical period (1976-2005), and for decadal time periods to 2100. It also provides historical and future distributions for the Arctic region on <span class="hlt">ice</span> concentration, <span class="hlt">ice</span> thickness, age of <span class="hlt">ice</span>, and <span class="hlt">ice</span> ridging in 15-degree longitude arc segments from the Arctic Circle to 80 degrees latitude, plusmore » two polar semicircular regions from 80 to 90 degrees latitude. The uncertainty is meant to describe the lack of knowledge rather than imprecision in the physical simulation because the emphasis is on unfalsified risk and its use to determine potential socioeconomic impacts. The full report is contained in 27 <span class="hlt">volumes</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1364754','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1364754"><span>County-Level Climate Uncertainty for Risk Assessments: <span class="hlt">Volume</span> 22 Appendix U - Historical Sea <span class="hlt">Ice</span> Thickness</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>Backus, George A.; Lowry, Thomas Stephen; Jones, Shannon M</p> <p>2017-06-01</p> <p>This report uses the CMIP5 series of climate model simulations to produce country- level uncertainty distributions for use in socioeconomic risk assessments of climate change impacts. It provides appropriate probability distributions, by month, for 169 countries and autonomous-areas on temperature, precipitation, maximum temperature, maximum wind speed, humidity, runoff, soil moisture and evaporation for the historical period (1976-2005), and for decadal time periods to 2100. It also provides historical and future distributions for the Arctic region on <span class="hlt">ice</span> concentration, <span class="hlt">ice</span> thickness, age of <span class="hlt">ice</span>, and <span class="hlt">ice</span> ridging in 15-degree longitude arc segments from the Arctic Circle to 80 degrees latitude, plusmore » two polar semicircular regions from 80 to 90 degrees latitude. The uncertainty is meant to describe the lack of knowledge rather than imprecision in the physical simulation because the emphasis is on unfalsified risk and its use to determine potential socioeconomic impacts. The full report is contained in 27 <span class="hlt">volumes</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1367304','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1367304"><span>County-Level Climate Uncertainty for Risk Assessments: <span class="hlt">Volume</span> 25 Appendix X - Forecast Sea <span class="hlt">Ice</span> Age.</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>Backus, George A.; Lowry, Thomas Stephen; Jones, Shannon M.</p> <p>2017-05-01</p> <p>This report uses the CMIP5 series of climate model simulations to produce country- level uncertainty distributions for use in socioeconomic risk assessments of climate change impacts. It provides appropriate probability distributions, by month, for 169 countries and autonomous-areas on temperature, precipitation, maximum temperature, maximum wind speed, humidity, runoff, soil moisture and evaporation for the historical period (1976-2005), and for decadal time periods to 2100. It also provides historical and future distributions for the Arctic region on <span class="hlt">ice</span> concentration, <span class="hlt">ice</span> thickness, age of <span class="hlt">ice</span>, and <span class="hlt">ice</span> ridging in 15-degree longitude arc segments from the Arctic Circle to 80 degrees latitude, plusmore » two polar semicircular regions from 80 to 90 degrees latitude. The uncertainty is meant to describe the lack of knowledge rather than imprecision in the physical simulation because the emphasis is on unfalsified risk and its use to determine potential socioeconomic impacts. The full report is contained in 27 <span class="hlt">volumes</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP41D..04B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP41D..04B"><span>High Northern Latitude Insolation Forcing of Tropical Monsoons or Monsoon Forcing of High Northern Latitude <span class="hlt">Ice</span> <span class="hlt">Volume</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beck, W.; Zhou, W.; Cheng, L.; Wu, Z.; Xian, F.; Kong, X.; Cottam, T.; An, Z.; White, L.</p> <p>2017-12-01</p> <p>We show that atmospheric 10Be flux is a quantitative proxy for rainfall, and use it to derive a 530Ka-long record of East Asian summer monsoon rainfall from Chinese Loess. Our record strongly resembles the Red Sea paleosea level and LR04 benthic foram δ18O records, with 53% & 45% of its variance reflected in each of these two global <span class="hlt">ice</span> <span class="hlt">volume</span> proxies. This suggests EASM intensity is closely coupled to <span class="hlt">ice</span> <span class="hlt">volume</span> by some mechanism. At first glance, this seems to support the claim based on strongly correlated Chinese cave δ18O and 65°N summer solar insolation that Asian monsoon intensity is controlled by high northern latitude insolation. Nevertheless, our 10Be-proxy has only 17% common variance with cave δ18O. Furthermore, Chinese cave δ18O records are very poorly correlated with sea-level/global <span class="hlt">ice</span> <span class="hlt">volume</span>, conflicting with both our proxy and Milankovitch theory, if interpreted as a monsoon intensity proxy. We argue that cave δ18O is instead a mixing proxy for monsoon moisture derived from (δ18O depleted) Indian vs Pacific monsoon sectors. We suggest both this mixing ratio and EASM intensity are not governed by high northern latitude insolation, but rather by orbital forcing of the low latitude interhemispheric insolation gradient, which mimics the 65°N insolation pattern. We show this gradient regulates the ratio of Asian monsoon outflow to the Indian vs. North Pacific subtropical highs, providing a coupling to both Hadley and Walker circulations. When outflow strengthens in one of these sectors it weakens in the other, regulating the relative strength of the Trade and Westerly winds in each sector. Trade wind coupling to monsoon strength in each sector controls the ISM/Pacific monsoon moisture mixing ratio and EASM intensity, although intensity is also influenced by other factors. This model provides mechanisms by which the monsoons may influence <span class="hlt">ice</span> <span class="hlt">volume</span>. Westerlies strength adjacent to the North Pacific Subtropical High strongly regulates transient</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JQSRT.131...95L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JQSRT.131...95L"><span>Modeling <span class="hlt">variability</span> in dendritic <span class="hlt">ice</span> crystal backscattering cross sections at millimeter wavelengths using a modified Rayleigh-Gans theory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, Yinghui; Clothiaux, Eugene E.; Aydin, Kültegin; Botta, Giovanni; Verlinde, Johannes</p> <p>2013-12-01</p> <p>Using the Generalized Multi-particle Mie-method (GMM), Botta et al. (in this issue) [7] created a database of backscattering cross sections for 412 different <span class="hlt">ice</span> crystal dendrites at X-, Ka- and W-band wavelengths for different incident angles. The Rayleigh-Gans theory, which accounts for interference effects but ignores interactions between different parts of an <span class="hlt">ice</span> crystal, explains much, but not all, of the <span class="hlt">variability</span> in the database of backscattering cross sections. Differences between it and the GMM range from -3.5 dB to +2.5 dB and are highly dependent on the incident angle. To explain the residual <span class="hlt">variability</span> a physically intuitive iterative method was developed to estimate the internal electric field within an <span class="hlt">ice</span> crystal that accounts for interactions between the neighboring regions within it. After modifying the Rayleigh-Gans theory using this estimated internal electric field, the difference between the estimated backscattering cross sections and those from the GMM method decreased to within 0.5 dB for most of the <span class="hlt">ice</span> crystals. The largest percentage differences occur when the form factor from the Rayleigh-Gans theory is close to zero. Both interference effects and neighbor interactions are sensitive to the morphology of <span class="hlt">ice</span> crystals. Improvements in <span class="hlt">ice</span>-microphysical models are necessary to predict or diagnose internal structures within <span class="hlt">ice</span> crystals to aid in more accurate interpretation of radar returns. Observations of the morphology of <span class="hlt">ice</span> crystals are, in turn, necessary to guide the development of such <span class="hlt">ice</span>-microphysical models and to better understand the statistical properties of <span class="hlt">ice</span> crystal morphologies in different environmental conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..4411482W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..4411482W"><span>Snow Accumulation <span class="hlt">Variability</span> Over the West Antarctic <span class="hlt">Ice</span> Sheet Since 1900: A Comparison of <span class="hlt">Ice</span> Core Records With ERA-20C Reanalysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Yetang; Thomas, Elizabeth R.; Hou, Shugui; Huai, Baojuan; Wu, Shuangye; Sun, Weijun; Qi, Shanzhong; Ding, Minghu; Zhang, Yulun</p> <p>2017-11-01</p> <p>This study uses a set of 37 firn core records over the West Antarctic <span class="hlt">Ice</span> Sheet (WAIS) to test the performance of the twentieth century from the European Centre for Medium-Range Weather Forecasts (ERA-20C) reanalysis for snow accumulation and quantify temporal <span class="hlt">variability</span> in snow accumulation since 1900. The firn cores are allocated to four geographical areas demarcated by drainage divides (i.e., Antarctic Peninsula (AP), western WAIS, central WAIS, and eastern WAIS) to calculate stacked records of regional snow accumulation. Our results show that the interannual <span class="hlt">variability</span> in ERA-20C precipitation minus evaporation (P - E) agrees well with the corresponding <span class="hlt">ice</span> core snow accumulation composites in each of the four geographical regions, suggesting its skill for simulating snow accumulation changes before the modern satellite era (pre-1979). Snow accumulation experiences significantly positive trends for the AP and eastern WAIS, a negative trend for the western WAIS, and no significant trend for the central WAIS from 1900 to 2010. The contrasting trends are associated with changes in the large-scale moisture transport driven by a deepening of the low-pressure systems and anomalies of sea <span class="hlt">ice</span> in the Amundsen Sea Low region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G11D..08F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G11D..08F"><span>Water storage in marine sediment and implications for inferences of past global <span class="hlt">ice</span> <span class="hlt">volume</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferrier, K.; Li, Q.; Pico, T.; Austermann, J.</p> <p>2017-12-01</p> <p>Changes in past sea level are of wide interest because they provide information on the sensitivity of <span class="hlt">ice</span> sheets to climate change, and thus inform predictions of future sea-level change. Sea level changes are influenced by many processes, including the storage of water in sedimentary pore space. Here we use a recent extension of gravitationally self-consistent sea-level models to explore the effects of marine sedimentary water storage on the global seawater balance and inferences of past global <span class="hlt">ice</span> <span class="hlt">volume</span>. Our analysis suggests that sedimentary water storage can be a significant component of the global seawater budget over the 105-year timescales associated with glacial-interglacial cycles, and an even larger component over longer timescales. Estimates of global sediment fluxes to the oceans suggest that neglecting marine sedimentary water storage may produce meter-scale errors in estimates of peak global mean sea level equivalent (GMSL) during the Last Interglacial (LIG). These calculations show that marine sedimentary water storage can be a significant contributor to the overall effects of sediment redistribution on sea-level change, and that neglecting sedimentary water storage can lead to substantial errors in inferences of global <span class="hlt">ice</span> <span class="hlt">volume</span> at past interglacials. This highlights the importance of accounting for the influences of sediment fluxes and sedimentary water storage on sea-level change over glacial-interglacial timescales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.3907W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.3907W"><span>Fram Strait: Atmospheric Forcing of The Sea <span class="hlt">Ice</span> Flux</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Widell, K.; Østerhus, S.; Gammelsrød, T.</p> <p></p> <p>Measuring the magnitude and <span class="hlt">variability</span> of the <span class="hlt">ice</span> and freshwater flux through Fram Strait is an important element in understanding climate <span class="hlt">variability</span> in the Arctic. Since the major part of the <span class="hlt">ice</span> and freshwater that leaves the Arctic passes through Fram Strait, this passage can be considered a key area for estimating the net <span class="hlt">ice</span> production in the Arctic Ocean. In 1990, the Norwegian Polar Institute (NPI) started a monitoring program in the strait, most years by means of two moorings with Upward Looking Sonars (ULS) measuring <span class="hlt">ice</span> draft. From 1995 and on, these moorings were also equipped with Doppler Current Meters (DCM) to measure the <span class="hlt">ice</span> velocity. These measurements give an opportunity to investigate the different forces affecting <span class="hlt">ice</span> motion in the strait. Maximum correlation coefficient between atmospheric sea level pressure (from NCEP/NCAR reanalysed data) and southward <span class="hlt">ice</span> velocity is found when using the cross strait pressure difference along 80N between 10W and 5E (R = 0.72) consider- ing monthly means. Subtracting current velocity at 50 m depth (also measured by the DCM) from <span class="hlt">ice</span> velocity improves the correlation to R = 0.84. This gives insight in the relative importance of current and wind on the <span class="hlt">ice</span> motion, and indicates that pressure data can be used to make fairly good estimates of the <span class="hlt">ice</span> velocity in the strait. In combination with data on <span class="hlt">ice</span> thickness and <span class="hlt">ice</span> stream width, this result is used to calculate the <span class="hlt">ice</span> <span class="hlt">volume</span> transport. By making assumptions on the parameters in- volved, the time series is extended back to 1948, the start of the pressure record. This time series will be presented and compared to literature, and annual and seasonal vari- ation of the <span class="hlt">ice</span> flux will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.A12B..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.A12B..01M"><span>Overview of Sea-<span class="hlt">Ice</span> Properties, Distribution and Temporal Variations, for Application to <span class="hlt">Ice</span>-Atmosphere Chemical Processes.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moritz, R. E.</p> <p>2005-12-01</p> <p>The properties, distribution and temporal variation of sea-<span class="hlt">ice</span> are reviewed for application to problems of <span class="hlt">ice</span>-atmosphere chemical processes. Typical vertical structure of sea-<span class="hlt">ice</span> is presented for different <span class="hlt">ice</span> types, including young <span class="hlt">ice</span>, first-year <span class="hlt">ice</span> and multi-year <span class="hlt">ice</span>, emphasizing factors relevant to surface chemistry and gas exchange. Time average annual cycles of large scale <span class="hlt">variables</span> are presented, including <span class="hlt">ice</span> concentration, <span class="hlt">ice</span> extent, <span class="hlt">ice</span> thickness and <span class="hlt">ice</span> age. Spatial and temporal <span class="hlt">variability</span> of these large scale quantities is considered on time scales of 1-50 years, emphasizing recent and projected changes in the Arctic pack <span class="hlt">ice</span>. The amount and time evolution of open water and thin <span class="hlt">ice</span> are important factors that influence ocean-<span class="hlt">ice</span>-atmosphere chemical processes. Observations and modeling of the sea-<span class="hlt">ice</span> thickness distribution function are presented to characterize the range of <span class="hlt">variability</span> in open water and thin <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GML....36..101M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GML....36..101M"><span>High-resolution IP25-based reconstruction of sea-<span class="hlt">ice</span> <span class="hlt">variability</span> in the western North Pacific and Bering Sea during the past 18,000 years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Méheust, Marie; Stein, Ruediger; Fahl, Kirsten; Max, Lars; Riethdorf, Jan-Rainer</p> <p>2016-04-01</p> <p>Due to its strong influence on heat and moisture exchange between the ocean and the atmosphere, sea <span class="hlt">ice</span> is an essential component of the global climate system. In the context of its alarming decrease in terms of concentration, thickness and duration, understanding the processes controlling sea-<span class="hlt">ice</span> <span class="hlt">variability</span> and reconstructing paleo-sea-<span class="hlt">ice</span> extent in polar regions have become of great interest for the scientific community. In this study, for the first time, IP25, a recently developed biomarker sea-<span class="hlt">ice</span> proxy, was used for a high-resolution reconstruction of the sea-<span class="hlt">ice</span> extent and its <span class="hlt">variability</span> in the western North Pacific and western Bering Sea during the past 18,000 years. To identify mechanisms controlling the sea-<span class="hlt">ice</span> <span class="hlt">variability</span>, IP25 data were associated with published sea-surface temperature as well as diatom and biogenic opal data. The results indicate that a seasonal sea-<span class="hlt">ice</span> cover existed during cold periods (Heinrich Stadial 1 and Younger Dryas), whereas during warmer intervals (Bølling-Allerød and Holocene) reduced sea <span class="hlt">ice</span> or <span class="hlt">ice</span>-free conditions prevailed in the study area. The <span class="hlt">variability</span> in sea-<span class="hlt">ice</span> extent seems to be linked to climate anomalies and sea-level changes controlling the oceanographic circulation between the subarctic Pacific and the Bering Sea, especially the Alaskan Stream injection though the Aleutian passes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980021232','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980021232"><span>Sea <span class="hlt">Ice</span> on the Southern Ocean</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jacobs, Stanley S.</p> <p>1998-01-01</p> <p>Year-round satellite records of sea <span class="hlt">ice</span> distribution now extend over more than two decades, providing a valuable tool to investigate related characteristics and circulations in the Southern Ocean. We have studied a variety of features indicative of oceanic and atmospheric interactions with Antarctic sea <span class="hlt">ice</span>. In the Amundsen & Bellingshausen Seas, sea <span class="hlt">ice</span> extent was found to have decreased by approximately 20% from 1973 through the early 1990's. This change coincided with and probably contributed to recently warmer surface conditions on the west side of the Antarctic Peninsula, where air temperatures have increased by approximately 0.5 C/decade since the mid-1940's. The sea <span class="hlt">ice</span> decline included multiyear cycles of several years in length superimposed on high interannual <span class="hlt">variability</span>. The retreat was strongest in summer, and would have lowered the regional mean <span class="hlt">ice</span> thickness, with attendant impacts upon vertical heat flux and the formation of snow <span class="hlt">ice</span> and brine. The cause of the regional warming and loss of sea <span class="hlt">ice</span> is believed to be linked to large-scale circulation changes in the atmosphere and ocean. At the eastern end of the Weddell Gyre, the Cosmonaut Polyna revealed greater activity since 1986, a recurrence pattern during recent winters and two possible modes of formation. Persistence in polynya location was noted off Cape Ann, where the coastal current can interact more strongly with the Antarctic Circumpolar Current. As a result of vorticity conservation, locally enhanced upwelling brings warmer deep water into the mixed layer, causing divergence and melting. In the Ross Sea, <span class="hlt">ice</span> extent fluctuates over periods of several years, with summer minima and winter maxima roughly in phase. This leads to large interannual cycles of sea <span class="hlt">ice</span> range, which correlate positively with meridinal winds, regional air temperatures and subsequent shelf water salinities. Deep shelf waters display considerable interannual <span class="hlt">variability</span>, but have freshened by approximately 0.03/decade</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790012519','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790012519"><span>Variations of the earth's magnetic field and rapid climatic cooling: A possible link through changes in global <span class="hlt">ice</span> <span class="hlt">volume</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rampino, M. R.</p> <p>1979-01-01</p> <p>A possible relationship between large scale changes in global <span class="hlt">ice</span> <span class="hlt">volume</span>, variations in the earth's magnetic field, and short term climatic cooling is investigated through a study of the geomagnetic and climatic records of the past 300,000 years. The calculations suggest that redistribution of the Earth's water mass can cause rotational instabilities which lead to geomagnetic excursions; these magnetic variations in turn may lead to short-term coolings through upper atmosphere effects. Such double coincidences of magnetic excursions and sudden coolings at times of <span class="hlt">ice</span> <span class="hlt">volume</span> changes have occurred at 13,500, 30,000, 110,000, and 135,000 YBP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP31A1265K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP31A1265K"><span>Sub-annual North Pacific hydroclimate <span class="hlt">variability</span> since 1450AD from updated St. Elias <span class="hlt">ice</span> core isotope and accumulation rate records</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kreutz, K. J.; Campbell, S. W.; Winski, D.; Osterberg, E. C.; Kochtitzky, W. H.; Copland, L.; Dixon, D.; Introne, D.; Medrzycka, D.; Main, B.; Bernsen, S.; Wake, C. P.</p> <p>2017-12-01</p> <p>A growing array of high-resolution paleoclimate records from the terrestrial region bordering the Gulf of Alaska (GoA) continues to reveal details about ocean-atmosphere <span class="hlt">variability</span> in the region during the Common Era. <span class="hlt">Ice</span> core records from high-elevation ranges in proximity to the GoA provide key information on extratropical hydroclimate, and potential teleconnections to low latitude regions. In particular, stable water isotope and snow accumulation reconstructions from <span class="hlt">ice</span> cores collected in high precipitation locations are uniquely tied to regional water cycle changes. Here we present new data collected in 2016 and 2017 from the St. Elias Mountains (Eclipse Icefield, Yukon Territories, Canada), including a range of <span class="hlt">ice</span> core and geophysical measurements. Low- and high-frequency <span class="hlt">ice</span> penetrating radar data enable detailed mapping of icefield bedrock topography and internal reflector stratigraphy. The 1911 Katmai eruption layer can be clearly traced across the icefield, and tied definitively to the coeval ash layer found in the 345 meter <span class="hlt">ice</span> core drilled at Eclipse Icefield in 2002. High-resolution radar data are used to map spatial <span class="hlt">variability</span> in 2015/16 and 2016/17 snow accumulation. <span class="hlt">Ice</span> velocity data from repeat GPS stake measurements and remote sensing feature tracking reveal a clear divide flow regime on the icefield. Shallow firn/<span class="hlt">ice</span> cores (20 meters in 2017 and 65 meters in 2016) are used to update the 345 meter <span class="hlt">ice</span> core drilled at Eclipse Icefield in 2002. We use new algorithm-based layer counting software to improve and provide error estimates on the new <span class="hlt">ice</span> core chronology, which extends from 2017 to 1450AD. 3D finite element modeling, incorporating all available geophysical data, is used to refine the reconstructed accumulation rate record and account for vertical and horizontal <span class="hlt">ice</span> flow. Together with high-resolution stable water isotope data, the updated Eclipse record provides detailed, sub-annual resolution data on several aspects of the regional</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20403839','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20403839"><span>Response of faults to climate-driven changes in <span class="hlt">ice</span> and water <span class="hlt">volumes</span> on Earth's surface.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hampel, Andrea; Hetzel, Ralf; Maniatis, Georgios</p> <p>2010-05-28</p> <p>Numerical models including one or more faults in a rheologically stratified lithosphere show that climate-induced variations in <span class="hlt">ice</span> and water <span class="hlt">volumes</span> on Earth's surface considerably affect the slip evolution of both thrust and normal faults. In general, the slip rate and hence the seismicity of a fault decreases during loading and increases during unloading. Here, we present several case studies to show that a postglacial slip rate increase occurred on faults worldwide in regions where <span class="hlt">ice</span> caps and lakes decayed at the end of the last glaciation. Of note is that the postglacial amplification of seismicity was not restricted to the areas beneath the large Laurentide and Fennoscandian <span class="hlt">ice</span> sheets but also occurred in regions affected by smaller <span class="hlt">ice</span> caps or lakes, e.g. the Basin-and-Range Province. Our results do not only have important consequences for the interpretation of palaeoseismological records from faults in these regions but also for the evaluation of the future seismicity in regions currently affected by deglaciation like Greenland and Antarctica: shrinkage of the modern <span class="hlt">ice</span> sheets owing to global warming may ultimately lead to an increase in earthquake frequency in these regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890024803&hterms=Phytoplankton&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DPhytoplankton','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890024803&hterms=Phytoplankton&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DPhytoplankton"><span>Phytoplankton standing crops within an Antarctic <span class="hlt">ice</span> edge assessed by satellite remote sensing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sullivan, C. W.; Mcclain, C. R.; Comiso, J. C.; Smith, W. O., Jr.</p> <p>1988-01-01</p> <p>The dynamic interactions between the pack-<span class="hlt">ice</span> recession and the occurrence of <span class="hlt">ice</span> blooms of phytoplankton in waters of the marginal <span class="hlt">ice</span> zone within an Antarctic <span class="hlt">ice</span> edge were investigated using CZCS and SMMR imageries from the Nimbus 7 satellite (September 16-December 17, 1983), together with in situ measurements of pigments and sea <span class="hlt">ice</span> concentration carried out from November 7 to December 2. A substantial amount of spatial <span class="hlt">variability</span> in pigment concentration was observed to occur along the <span class="hlt">ice</span> edge in the Weddell Sea. The relationships among light, <span class="hlt">ice</span> distribution, and vertical stability and their effects on observed spatial variations in phytoplankton biomass are discussed. The results of this investigation suggest that the retreat of <span class="hlt">ice</span> provides an input of significant <span class="hlt">volumes</span> of meltwater which creates vertical stability for a period necessary to permit growth and accumulation of phytoplankton.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CliPa..13.1243S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CliPa..13.1243S"><span>The influence of <span class="hlt">ice</span> sheets on temperature during the past 38 million years inferred from a one-dimensional <span class="hlt">ice</span> sheet-climate model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stap, Lennert B.; van de Wal, Roderik S. W.; de Boer, Bas; Bintanja, Richard; Lourens, Lucas J.</p> <p>2017-09-01</p> <p>Since the inception of the Antarctic <span class="hlt">ice</span> sheet at the Eocene-Oligocene transition (˜ 34 Myr ago), land <span class="hlt">ice</span> has played a crucial role in Earth's climate. Through feedbacks in the climate system, land <span class="hlt">ice</span> <span class="hlt">variability</span> modifies atmospheric temperature changes induced by orbital, topographical, and greenhouse gas variations. Quantification of these feedbacks on long timescales has hitherto scarcely been undertaken. In this study, we use a zonally averaged energy balance climate model bidirectionally coupled to a one-dimensional <span class="hlt">ice</span> sheet model, capturing the <span class="hlt">ice</span>-albedo and surface-height-temperature feedbacks. Potentially important transient changes in topographic boundary conditions by tectonics and erosion are not taken into account but are briefly discussed. The relative simplicity of the coupled model allows us to perform integrations over the past 38 Myr in a fully transient fashion using a benthic oxygen isotope record as forcing to inversely simulate CO2. Firstly, we find that the results of the simulations over the past 5 Myr are dependent on whether the model run is started at 5 or 38 Myr ago. This is because the relation between CO2 and temperature is subject to hysteresis. When the climate cools from very high CO2 levels, as in the longer transient 38 Myr run, temperatures in the lower CO2 range of the past 5 Myr are higher than when the climate is initialised at low temperatures. Consequently, the modelled CO2 concentrations depend on the initial state. Taking the realistic warm initialisation into account, we come to a best estimate of CO2, temperature, <span class="hlt">ice-volume</span>-equivalent sea level, and benthic δ18O over the past 38 Myr. Secondly, we study the influence of <span class="hlt">ice</span> sheets on the evolution of global temperature and polar amplification by comparing runs with <span class="hlt">ice</span> sheet-climate interaction switched on and off. By passing only albedo or surface height changes to the climate model, we can distinguish the separate effects of the <span class="hlt">ice</span>-albedo and surface</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1916446D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1916446D"><span>Fives decades of strong temporal <span class="hlt">variability</span> in the flow of the Brunt <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>De Rydt, Jan; Gudmundsson, Hilmar; Nagler, Thomas</p> <p>2017-04-01</p> <p>The Brunt <span class="hlt">Ice</span> Shelf, East Antarctica, is a complex conglomerate of meteoric and marine <span class="hlt">ice</span>, weakly connected to the much larger and faster-flowing Stancomb Wills Glacier Tongue to the east, and pinned down to the seabed in a small area around the McDonalds <span class="hlt">Ice</span> Rumples in the north. The <span class="hlt">ice</span> shelf is home to the UK research station Halley, from which changes to the <span class="hlt">ice</span> shelf have been monitored closely since the 1960s. A unique 50-year record of the flow speed and an intense surveying programme over the past 10 years, have revealed a strong temporal <span class="hlt">variability</span> in the flow. In particular, the speed of the <span class="hlt">ice</span> shelf has increased by 10% each year over the past few years. In order to understand these rapid changes, we use a state-of-the-art flow model in combination with a range of satellite, ground-based and airborne radar data, to accurately simulate the historical flow and recent changes. In particular, we model the effects of a recently formed rift that is propagating at a speed of up to 600m/day and threatens to dislodge the <span class="hlt">ice</span> shelf from its pinning point at the McDonalds <span class="hlt">Ice</span> Rumples. We also report on the recent reactivation of a large chasm which has prompted the relocation of the station during the 2016/17 austral summer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1364752','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1364752"><span>County-Level Climate Uncertainty for Risk Assessments: <span class="hlt">Volume</span> 21 Appendix T - Forecast Sea <span class="hlt">Ice</span> Area Fraction.</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>Backus, George A.; Lowry, Thomas Stephen; Jones, Shannon M.</p> <p>2017-06-01</p> <p>This report uses the CMIP5 series of climate model simulations to produce country- level uncertainty distributions for use in socioeconomic risk assessments of climate change impacts. It provides appropriate probability distributions, by month, for 169 countries and autonomous-areas on temperature, precipitation, maximum temperature, maximum wind speed, humidity, runoff, soil moisture and evaporation for the historical period (1976-2005), and for decadal time periods to 2100. It also provides historical and future distributions for the Arctic region on <span class="hlt">ice</span> concentration, <span class="hlt">ice</span> thickness, age of <span class="hlt">ice</span>, and <span class="hlt">ice</span> ridging in 15-degree longitude arc segments from the Arctic Circle to 80 degrees latitude, plusmore » two polar semicircular regions from 80 to 90 degrees latitude. The uncertainty is meant to describe the lack of knowledge rather than imprecision in the physical simulation because the emphasis is on unfalsified risk and its use to determine potential socioeconomic impacts. The full report is contained in 27 <span class="hlt">volumes</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511590V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511590V"><span>Translating hydrologically-relevant <span class="hlt">variables</span> from the <span class="hlt">ice</span> sheet model SICOPOLIS to the Greenland Analog Project hydrologic modeling domain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vallot, Dorothée; Applegate, Patrick; Pettersson, Rickard</p> <p>2013-04-01</p> <p>Projecting future climate and <span class="hlt">ice</span> sheet development requires sophisticated models and extensive field observations. Given the present state of our knowledge, it is very difficult to say what will happen with certainty. Despite the ongoing increase in atmospheric greenhouse gas concentrations, the possibility that a new <span class="hlt">ice</span> sheet might form over Scandinavia in the far distant future cannot be excluded. The growth of a new Scandinavian <span class="hlt">Ice</span> Sheet would have important consequences for buried nuclear waste repositories. The Greenland Analogue Project, initiated by the Swedish Nuclear Fuel and Waste Management Company (SKB), is working to assess the effects of a possible future <span class="hlt">ice</span> sheet on groundwater flow by studying a constrained domain in Western Greenland by field measurements (including deep bedrock drilling in front of the <span class="hlt">ice</span> sheet) combined with numerical modeling. To address the needs of the GAP project, we interpolated results from an ensemble of <span class="hlt">ice</span> sheet model runs to the smaller and more finely resolved modeling domain used in the GAP project's hydrologic modeling. Three runs have been chosen with three fairly different positive degree-day factors among those that reproduced the modern <span class="hlt">ice</span> margin at the borehole position. The interpolated results describe changes in hydrologically-relevant <span class="hlt">variables</span> over two time periods, 115 ka to 80 ka, and 20 ka to 1 ka. In the first of these time periods, the <span class="hlt">ice</span> margin advances over the model domain; in the second time period, the <span class="hlt">ice</span> margin retreats over the model domain. The spatially-and temporally dependent <span class="hlt">variables</span> that we treated include the <span class="hlt">ice</span> thickness, basal melting rate, surface mass balance, basal temperature, basal thermal regime (frozen or thawed), surface temperature, and basal water pressure. The melt flux is also calculated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23558172','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23558172"><span>Annually resolved <span class="hlt">ice</span> core records of tropical climate <span class="hlt">variability</span> over the past ~1800 years.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thompson, L G; Mosley-Thompson, E; Davis, M E; Zagorodnov, V S; Howat, I M; Mikhalenko, V N; Lin, P-N</p> <p>2013-05-24</p> <p><span class="hlt">Ice</span> cores from low latitudes can provide a wealth of unique information about past climate in the tropics, but they are difficult to recover and few exist. Here, we report annually resolved <span class="hlt">ice</span> core records from the Quelccaya <span class="hlt">ice</span> cap (5670 meters above sea level) in Peru that extend back ~1800 years and provide a high-resolution record of climate <span class="hlt">variability</span> there. Oxygen isotopic ratios (δ(18)O) are linked to sea surface temperatures in the tropical eastern Pacific, whereas concentrations of ammonium and nitrate document the dominant role played by the migration of the Intertropical Convergence Zone in the region of the tropical Andes. Quelccaya continues to retreat and thin. Radiocarbon dates on wetland plants exposed along its retreating margins indicate that it has not been smaller for at least six millennia.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFM.P72B0507D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFM.P72B0507D"><span>Cumulates, Dykes and Pressure Solution in the <span class="hlt">Ice</span>-Salt Mantle of Europa: Geological Consequences of Pressure Dependent Liquid Compositions and <span class="hlt">Volume</span> Changes During <span class="hlt">Ice</span>-Salt Melting Reactions.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Day, S.; Asphaug, E.; Bruesch, L.</p> <p>2002-12-01</p> <p>Water-salt analogue experiments used to investigate cumulate processes in silicate magmas, along with observations of sea <span class="hlt">ice</span> and <span class="hlt">ice</span> shelf behaviour, indicate that crystal-melt separation in water-salt systems is a rapid and efficient process even on scales of millimetres and minutes. Squeezing-out of residual melts by matrix compaction is also predicted to be rapid on geological timescales. We predict that the <span class="hlt">ice</span>-salt mantle of Europa is likely to be strongly stratified, with a layered structure predictable from density and phase relationships between <span class="hlt">ice</span> polymorphs, aqueous saline solutions and crystalline salts such as hydrated magnesium sulphates (determined experimentally by, inter alia, Hogenboom et al). A surface layer of water <span class="hlt">ice</span> flotation cumulate will be separated from denser salt cumulates by a cotectic horizon. This cotectic horizon will be both the site of subsequent lowest-temperature melting and a level of neutral buoyancy for the saline melts produced. Initial melting will be in a narrow depth range owing to increasing melting temperature with decreasing pressure: the phase relations argue against direct melt-though to the surface unless vesiculation occurs. Overpressuring of dense melts due to <span class="hlt">volume</span> expansion on cotectic melting is predicted to lead to lateral dyke emplacement and extension above the dyke tips. Once the liquid leaves the cotectic, melting of water <span class="hlt">ice</span> will involve negative <span class="hlt">volume</span> change. Impact-generated melts will drain downwards through the fractured zones beneath crater floors. A feature in the complex crater Mannan'an, with elliptical ring fractures around a conical depression with a central pit, bears a close resemblance to Icelandic glacier collapse cauldrons produced by subglacial eruptions. Other structures resembling Icelandic cauldrons occur along Europan banded structures, while resurgence of <span class="hlt">ice</span> rubble within collapse structures may produce certain types of chaos region. More general contraction of the <span class="hlt">ice</span> mantle</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26PSL.472...14X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26PSL.472...14X"><span>Deglacial and Holocene sea-<span class="hlt">ice</span> <span class="hlt">variability</span> north of Iceland and response to ocean circulation changes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiao, Xiaotong; Zhao, Meixun; Knudsen, Karen Luise; Sha, Longbin; Eiríksson, Jón; Gudmundsdóttir, Esther; Jiang, Hui; Guo, Zhigang</p> <p>2017-08-01</p> <p>Sea-<span class="hlt">ice</span> conditions on the North Icelandic shelf constitute a key component for the study of the climatic gradients between the Arctic and the North Atlantic Oceans at the Polar Front between the cold East Icelandic Current delivering Polar surface water and the relatively warm Irminger Current derived from the North Atlantic Current. The <span class="hlt">variability</span> of sea <span class="hlt">ice</span> contributes to heat reduction (albedo) and gas exchange between the ocean and the atmosphere, and further affects the deep-water formation. However, lack of long-term and high-resolution sea-<span class="hlt">ice</span> records in the region hinders the understanding of palaeoceanographic change mechanisms during the last glacial-interglacial cycle. Here, we present a sea-<span class="hlt">ice</span> record back to 15 ka (cal. ka BP) based on the sea-<span class="hlt">ice</span> biomarker IP25, phytoplankton biomarker brassicasterol and terrestrial biomarker long-chain n-alkanols in piston core MD99-2272 from the North Icelandic shelf. During the Bølling/Allerød (14.7-12.9 ka), the North Icelandic shelf was characterized by extensive spring sea-<span class="hlt">ice</span> cover linked to reduced flow of warm Atlantic Water and dominant Polar water influence, as well as strong meltwater input in the area. This pattern showed an anti-phase relationship with the <span class="hlt">ice</span>-free/less <span class="hlt">ice</span> conditions in marginal areas of the eastern Nordic Seas, where the Atlantic Water inflow was strong, and contributed to an enhanced deep-water formation. Prolonged sea-<span class="hlt">ice</span> cover with occasional occurrence of seasonal sea <span class="hlt">ice</span> prevailed during the Younger Dryas (12.9-11.7 ka) interrupted by a brief interval of enhanced Irminger Current and deposition of the Vedde Ash, as opposed to abruptly increased sea-<span class="hlt">ice</span> conditions in the eastern Nordic Seas. The seasonal sea <span class="hlt">ice</span> decreased gradually from the Younger Dryas to the onset of the Holocene corresponding to increasing insolation. <span class="hlt">Ice</span>-free conditions and sea surface warming were observed for the Early Holocene, followed by expansion of sea <span class="hlt">ice</span> during the Mid-Holocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.5442L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.5442L"><span>Observed platelet <span class="hlt">ice</span> distributions in Antarctic sea <span class="hlt">ice</span>: An index for ocean-<span class="hlt">ice</span> shelf heat flux</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Langhorne, P. J.; Hughes, K. G.; Gough, A. J.; Smith, I. J.; Williams, M. J. M.; Robinson, N. J.; Stevens, C. L.; Rack, W.; Price, D.; Leonard, G. H.; Mahoney, A. R.; Haas, C.; Haskell, T. G.</p> <p>2015-07-01</p> <p>Antarctic sea <span class="hlt">ice</span> that has been affected by supercooled <span class="hlt">Ice</span> Shelf Water (ISW) has a unique crystallographic structure and is called platelet <span class="hlt">ice</span>. In this paper we synthesize platelet <span class="hlt">ice</span> observations to construct a continent-wide map of the winter presence of ISW at the ocean surface. The observations demonstrate that, in some regions of coastal Antarctica, supercooled ISW drives a negative oceanic heat flux of -30 Wm-2 that persists for several months during winter, significantly affecting sea <span class="hlt">ice</span> thickness. In other regions, particularly where the thinning of <span class="hlt">ice</span> shelves is believed to be greatest, platelet <span class="hlt">ice</span> is not observed. Our new data set includes the longest <span class="hlt">ice</span>-ocean record for Antarctica, which dates back to 1902 near the McMurdo <span class="hlt">Ice</span> Shelf. These historical data indicate that, over the past 100 years, any change in the <span class="hlt">volume</span> of very cold surface outflow from this <span class="hlt">ice</span> shelf is less than the uncertainties in the measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC21D1126A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC21D1126A"><span>Sensitivity of Great Lakes <span class="hlt">Ice</span> Cover to Air Temperature</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Austin, J. A.; Titze, D.</p> <p>2016-12-01</p> <p><span class="hlt">Ice</span> cover is shown to exhibit a strong linear sensitivity to air temperature. Upwards of 70% of <span class="hlt">ice</span> cover <span class="hlt">variability</span> on all of the Great Lakes can be explained in terms of air temperature, alone, and nearly 90% of <span class="hlt">ice</span> cover <span class="hlt">variability</span> can be explained in some lakes. <span class="hlt">Ice</span> cover sensitivity to air temperature is high, and a difference in seasonally-averaged (Dec-May) air temperature on the order of 1°C to 2°C can be the difference between a low-<span class="hlt">ice</span> year and a moderate- to high- <span class="hlt">ice</span> year. The total amount of seasonal <span class="hlt">ice</span> cover is most influenced by air temperatures during the meteorological winter, contemporaneous with the time of <span class="hlt">ice</span> formation. Air temperature conditions during the pre-winter conditioning period and during the spring melting period were found to have less of an impact on seasonal <span class="hlt">ice</span> cover. This is likely due to the fact that there is a negative feedback mechanism when heat loss goes toward cooling the lake, but a positive feedback mechanism when heat loss goes toward <span class="hlt">ice</span> formation. <span class="hlt">Ice</span> cover sensitivity relationships were compared between shallow coastal regions of the Great Lakes and similarly shallow smaller, inland lakes. It was found that the sensitivity to air temperature is similar between these coastal regions and smaller lakes, but that the absolute amount of <span class="hlt">ice</span> that forms varies significantly between small lakes and the Great Lakes, and amongst the Great Lakes themselves. The Lake Superior application of the ROMS three-dimensional hydrodynamic numerical model verifies a deterministic linear relationship between air temperature and <span class="hlt">ice</span> cover, which is also strongest around the period of <span class="hlt">ice</span> formation. When the Lake Superior bathymetry is experimentally adjusted by a constant vertical multiplier, average lake depth is shown to have a nonlinear relationship with seasonal <span class="hlt">ice</span> cover, and this nonlinearity may be associated with a nonlinear increase in the lake-wide <span class="hlt">volume</span> of the surface mixed layer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70175509','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70175509"><span>Water, <span class="hlt">ice</span> and mud: Lahars and lahar hazards at <span class="hlt">ice</span>- and snow-clad volcanoes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Waythomas, Christopher F.</p> <p>2014-01-01</p> <p>Large-<span class="hlt">volume</span> lahars are significant hazards at <span class="hlt">ice</span> and snow covered volcanoes. Hot eruptive products produced during explosive eruptions can generate a substantial <span class="hlt">volume</span> of melt water that quickly evolves into highly mobile flows of <span class="hlt">ice</span>, sediment and water. At present it is difficult to predict the size of lahars that can form at <span class="hlt">ice</span> and snow covered volcanoes due to their complex flow character and behaviour. However, advances in experiments and numerical approaches are producing new conceptual models and new methods for hazard assessment. Eruption triggered lahars that are <span class="hlt">ice</span>-dominated leave behind thin, almost unrecognizable sedimentary deposits, making them likely to be under-represented in the geological record.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.6966S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.6966S"><span>The local environment of <span class="hlt">ice</span> particles in 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>Schlenczek, Oliver; Fugal, Jacob P.; Schledewitz, Waldemar; Borrmann, Stephan</p> <p>2015-04-01</p> <p>During the RACEPAC field campaign in April and May 2014, research flights were made with the Polar 5 and Polar 6 aircraft from the Alfred Wegener Institute in Arctic clouds near Inuvik, Northwest Territories, Canada. One flight with the Polar 6 aircraft, done on May 16, 2014, flew under precipitating, stratiform, mid-level clouds with several penetrations through cloud base. Measurements with HALOHolo, an airborne digital in-line holographic instrument for cloud particles, show <span class="hlt">ice</span> particles in a field of other cloud particles in a local three-dimensional sample <span class="hlt">volume</span> (~14x19x130 mm3 or ~35 cm^3). Each holographic sample <span class="hlt">volume</span> is a snapshot of a 3-dimensional piece of cloud at the cm-scale with typically thousands of cloud droplets per sample <span class="hlt">volume</span>, so each sample <span class="hlt">volume</span> yields a statistically significant droplet size distribution. Holograms are recorded at a rate of six times per second, which provides one <span class="hlt">volume</span> sample approx. every 12 meters along the flight path. The size resolution limit for cloud droplets is better than 1 µm due to advanced sizing algorithms. Shown are preliminary results of, (1) the <span class="hlt">ice</span>/liquid water partitioning at the cloud base and the distribution of water droplets around each <span class="hlt">ice</span> particle, and (2) spatial and temporal <span class="hlt">variability</span> of the cloud droplet size distributions at cloud base.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C13G..01F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C13G..01F"><span>Investigating <span class="hlt">ice</span> shelf mass loss processes from continuous 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>Fricker, H. A.</p> <p>2017-12-01</p> <p>The Antarctic <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> shelves surrounding the continent. Small amounts of mass are also lost by surface melting, which occurs on many <span class="hlt">ice</span> shelves every summer to varying degrees, and has been linked to <span class="hlt">ice</span>-shelf collapse via hydrofracture on <span class="hlt">ice</span> shelves that have been pre-weakened. <span class="hlt">Ice</span> shelves provide mechanical support to `buttress' seaward flow of grounded <span class="hlt">ice</span>, so that <span class="hlt">ice</span>-shelf thinning and retreat result in enhanced <span class="hlt">ice</span> discharge to the ocean. <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> sheet itself. Mass loss from iceberg calving is episodic, with typical intervals between calving events on the order of decades. Since <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-shelf surface height since the early 1990s. The continuous time series show accelerated losses in total Antarctic <span class="hlt">ice</span>-shelf <span class="hlt">volume</span> from 1994 to 2017, and allow us to investigate the processes causing <span class="hlt">ice</span>-shelf mass change. For Larsen C, much of the <span class="hlt">variability</span> comes from changing atmospheric conditions affecting firn state. In the Amundsen Sea, the rapid thinning is a combination of accelerated ocean-driven thinning and <span class="hlt">ice</span> dynamics. This long-term thinning signal is, however, is strongly modulated by ENSO-driven interannual <span class="hlt">variability</span>. However, observations of ocean <span class="hlt">variability</span> around Antarctica are sparse, since these regions are often covered in sea <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C32B..05B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C32B..05B"><span>Expanding Antarctic Sea <span class="hlt">Ice</span>: Anthropogenic or Natural <span class="hlt">Variability</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bitz, C. M.</p> <p>2016-12-01</p> <p>Antarctic sea <span class="hlt">ice</span> extent has increased over the last 36 years according to the satellite record. Concurrent with Antarctic sea-<span class="hlt">ice</span> expansion has been broad cooling of the Southern Ocean sea-surface temperature. Not only are Southern Ocean sea <span class="hlt">ice</span> and SST trends at odds with expectations from greenhouse gas-induced warming, the trend patterns are not reproduced in historical simulations with comprehensive global climate models. While a variety of different factors may have contributed to the observed trends in recent decades, we propose that it is atmospheric circulation changes - and the changes in ocean circulation they induce - that have emerged as the most likely cause of the observed Southern Ocean sea <span class="hlt">ice</span> and SST trends. I will discuss deficiencies in models that could explain their incorrect response. In addition, I will present results from a series of experiments where the Antarctic sea <span class="hlt">ice</span> and ocean are forced by atmospheric perturbations imposed within a coupled climate model. Figure caption: Linear trends of annual-mean SST (left) and annual-mean sea-<span class="hlt">ice</span> concentration (right) over 1980-2014. SST is from NOAA's Optimum Interpolation SST dataset (version 2; Reynolds et al. 2002). Sea-<span class="hlt">ice</span> concentration is from passive microwave observations using the NASA Team algorithm. Only the annual means are shown here for brevity and because the signal to noise is greater than in the seasonal means. Figure from Armour and Bitz (2015).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140005670','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140005670"><span>Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Perovich, D.; Gerland, S.; Hendricks, S.; Meier, Walter N.; Nicolaus, M.; Richter-Menge, J.; Tschudi, M.</p> <p>2013-01-01</p> <p>During 2013, Arctic sea <span class="hlt">ice</span> extent remained well below normal, but the September 2013 minimum extent was substantially higher than the record-breaking minimum in 2012. Nonetheless, the minimum was still much lower than normal and the long-term trend Arctic September extent is -13.7 per decade relative to the 1981-2010 average. The less extreme conditions this year compared to 2012 were due to cooler temperatures and wind patterns that favored retention of <span class="hlt">ice</span> through the summer. Sea <span class="hlt">ice</span> thickness and <span class="hlt">volume</span> remained near record-low levels, though indications are of slightly thicker <span class="hlt">ice</span> compared to the record low of 2012.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.C11B0499S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.C11B0499S"><span>Expanding research capabilities with sea <span class="hlt">ice</span> climate records for analysis of long-term climate change and short-term <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scott, D. J.; Meier, W. N.</p> <p>2008-12-01</p> <p>Recent sea <span class="hlt">ice</span> analysis is leading to predictions of a sea <span class="hlt">ice</span>-free summertime in the Arctic within 20 years, or even sooner. Sea <span class="hlt">ice</span> topics, such as concentration, extent, motion, and age, are predominately studied using satellite data. At the National Snow and <span class="hlt">Ice</span> Data Center (NSIDC), passive microwave sea <span class="hlt">ice</span> data sets provide timely assessments of seasonal-scale <span class="hlt">variability</span> as well as consistent long-term climate data records. Such data sets are crucial to understanding changes and assessing their impacts. Noticeable impacts of changing sea <span class="hlt">ice</span> conditions on native cultures and wildlife in the Arctic region are now being documented. With continued deterioration in Arctic sea <span class="hlt">ice</span>, global economic impacts will be seen as new shipping routes open. NSIDC is at the forefront of making climate data records available to address the changes in sea <span class="hlt">ice</span> and its global impacts. By focusing on integrated data sets, NSIDC leads the way by broadening the studies of sea <span class="hlt">ice</span> beyond the traditional cryospheric community.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1513402T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1513402T"><span>Export of <span class="hlt">Ice</span>-Cavity Water from Pine Island <span class="hlt">Ice</span> Shelf, West Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thurnherr, Andreas; Jacobs, Stanley; Dutrieux, Pierre</p> <p>2013-04-01</p> <p>Stability of the West Antarctic <span class="hlt">Ice</span> Sheet is sensitive to changes in melting at the bottom of floating <span class="hlt">ice</span> shelves that form the seaward extensions of Antarctic glaciers flowing into the ocean. Not least because observations in the cavities beneath <span class="hlt">ice</span> shelves are difficult, heat fluxes and melt rates have been inferred from oceanographic measurements obtained near the <span class="hlt">ice</span> edge (calving fronts). Here, we report on a set of hydrographic and velocity data collected in early 2009 near the calving front of the Amundsen Sea's fast-moving and (until recently) accelerating Pine Island Glacier and its associated <span class="hlt">ice</span> shelf. CTD profiles collected along the southern half of the meridionally-trending <span class="hlt">ice</span> front show clear evidence for export of <span class="hlt">ice</span>-cavity water. That water was carried in the upper ocean along the <span class="hlt">ice</span> front by a southward current that is possibly related to a striking clockwise gyre that dominated the (summertime) upper-ocean circulation in Pine Island Bay. Signatures of <span class="hlt">ice</span>-cavity water appear unrelated to current direction along most of the <span class="hlt">ice</span> front, suggesting that cross-frontal exchange is dominated by temporal <span class="hlt">variability</span>. However, repeated hydrographic and velocity measurements in a small "<span class="hlt">ice</span> cove" at the southern end of the calving front show a persistent strong (mean velocity peaking near 0.5 ms-1) outflow of <span class="hlt">ice</span>-cavity water in the upper 500 m. While surface features (boils) suggested upwelling from deep below the <span class="hlt">ice</span> shelf, vertical velocity measurements reveal 1) that the mean upwelling within the confines of the cove was too weak to feed the observed outflow, and 2) that large high-frequency internal waves dominated the vertical motion of water inside the cove. These observations indicate that water exchange between the Pine Island <span class="hlt">Ice</span> Shelf cavity and the Amundsen sea is strongly asymmetric with weak broad inflow at depth and concentrated surface-intensified outflow of melt-laden deep water at the southern edge of the calving front. The lack of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018IzAOP..54...65I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018IzAOP..54...65I"><span>The Effect of Seasonal <span class="hlt">Variability</span> of Atlantic Water on the Arctic Sea <span class="hlt">Ice</span> Cover</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ivanov, V. V.; Repina, I. A.</p> <p>2018-01-01</p> <p>Under the influence of global warming, the sea <span class="hlt">ice</span> in the Arctic Ocean (AO) is expected to reduce with a transition toward a seasonal <span class="hlt">ice</span> cover by the end of this century. A comparison of climate-model predictions with measurements shows that the actual rate of <span class="hlt">ice</span> cover decay in the AO is higher than the predicted one. This paper argues that the rapid shrinking of the Arctic summer <span class="hlt">ice</span> cover is due to its increased seasonality, while seasonal oscillations of the Atlantic origin water temperature create favorable conditions for the formation of negative anomalies in the <span class="hlt">ice</span>-cover area in winter. The basis for this hypothesis is the fundamental possibility of the activation of positive feedback provided by a specific feature of the seasonal cycle of the inflowing Atlantic origin water and the peaking of temperature in the Nansen Basin in midwinter. The recently accelerated reduction in the summer <span class="hlt">ice</span> cover in the AO leads to an increased accumulation of heat in the upper ocean layer during the summer season. The extra heat content of the upper ocean layer favors prerequisite conditions for winter thermohaline convection and the transfer of heat from the Atlantic water (AW) layer to the <span class="hlt">ice</span> cover. This, in turn, contributes to further <span class="hlt">ice</span> thinning and a decrease in <span class="hlt">ice</span> concentration, accelerated melting in summer, and a greater accumulation of heat in the ocean by the end of the following summer. An important role is played by the seasonal <span class="hlt">variability</span> of the temperature of AW, which forms on the border between the North European and Arctic basins. The phase of seasonal oscillation changes while the AW is moving through the Nansen Basin. As a result, the timing of temperature peak shifts from summer to winter, additionally contributing to enhanced <span class="hlt">ice</span> melting in winter. The formulated theoretical concept is substantiated by a simplified mathematical model and comparison with observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41C1243L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41C1243L"><span>Greenland Regional and <span class="hlt">Ice</span> Sheet-wide Geometry Sensitivity to Boundary and Initial conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Logan, L. C.; Narayanan, S. H. K.; Greve, R.; Heimbach, P.</p> <p>2017-12-01</p> <p><span class="hlt">Ice</span> sheet and glacier model outputs require inputs from uncertainly known initial and boundary conditions, and other parameters. Conservation and constitutive equations formalize the relationship between model inputs and outputs, and the sensitivity of model-derived quantities of interest (e.g., <span class="hlt">ice</span> sheet <span class="hlt">volume</span> above floatation) to model <span class="hlt">variables</span> can be obtained via the adjoint model of an <span class="hlt">ice</span> sheet. We show how one particular <span class="hlt">ice</span> sheet model, SICOPOLIS (SImulation COde for POLythermal <span class="hlt">Ice</span> Sheets), depends on these inputs through comprehensive adjoint-based sensitivity analyses. SICOPOLIS discretizes the shallow-<span class="hlt">ice</span> and shallow-shelf approximations for <span class="hlt">ice</span> flow, and is well-suited for paleo-studies of Greenland and Antarctica, among other computational domains. The adjoint model of SICOPOLIS was developed via algorithmic differentiation, facilitated by the source transformation tool OpenAD (developed at Argonne National Lab). While model sensitivity to various inputs can be computed by costly methods involving input perturbation simulations, the time-dependent adjoint model of SICOPOLIS delivers model sensitivities to initial and boundary conditions throughout time at lower cost. Here, we explore both the sensitivities of the Greenland <span class="hlt">Ice</span> Sheet's entire and regional <span class="hlt">volumes</span> to: initial <span class="hlt">ice</span> thickness, precipitation, basal sliding, and geothermal flux over the Holocene epoch. Sensitivity studies such as described here are now accessible to the modeling community, based on the latest version of SICOPOLIS that has been adapted for OpenAD to generate correct and efficient adjoint code.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..12210820G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..12210820G"><span>Spring snow conditions on Arctic sea <span class="hlt">ice</span> north of Svalbard, during the Norwegian Young Sea <span class="hlt">ICE</span> (N-<span class="hlt">ICE</span>2015) expedition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gallet, Jean-Charles; Merkouriadi, Ioanna; Liston, Glen E.; Polashenski, Chris; Hudson, Stephen; Rösel, Anja; Gerland, Sebastian</p> <p>2017-10-01</p> <p>Snow is crucial over sea <span class="hlt">ice</span> due to its conflicting role in reflecting the incoming solar energy and reducing the heat transfer so that its temporal and spatial <span class="hlt">variability</span> are important to estimate. During the Norwegian Young Sea <span class="hlt">ICE</span> (N-<span class="hlt">ICE</span>2015) campaign, snow physical properties and <span class="hlt">variability</span> were examined, and results from April until mid-June 2015 are presented here. Overall, the snow thickness was about 20 cm higher than the climatology for second-year <span class="hlt">ice</span>, with an average of 55 ± 27 cm and 32 ± 20 cm on first-year <span class="hlt">ice</span>. The average density was 350-400 kg m-3 in spring, with higher values in June due to melting. Due to flooding in March, larger <span class="hlt">variability</span> in snow water equivalent was observed. However, the snow structure was quite homogeneous in spring due to warmer weather and lower amount of storms passing over the field camp. The snow was mostly consisted of wind slab, faceted, and depth hoar type crystals with occasional fresh snow. These observations highlight the more dynamic character of evolution of snow properties over sea <span class="hlt">ice</span> compared to previous observations, due to more <span class="hlt">variable</span> sea <span class="hlt">ice</span> and weather conditions in this area. The snowpack was isothermal as early as 10 June with the first onset of melt clearly identified in early June. Based on our observations, we estimate than snow could be accurately represented by a three to four layers modeling approach, in order to better consider the high <span class="hlt">variability</span> of snow thickness and density together with the rapid metamorphose of the snow in springtime.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE44D1538R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE44D1538R"><span>Friend or Foe: <span class="hlt">Variability</span> in How Sea <span class="hlt">Ice</span> Can Both Hinder and Enhance Phytoplankton Blooms Across the Southern Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rohr, T.</p> <p>2016-02-01</p> <p>Globally, a suite of physical and biogeochemical controls govern the structure, size, and timing of seasonal phytoplankton blooms. In the Southern Ocean, the introduction of seasonal sea <span class="hlt">ice</span> provides an additional constraining factor. From a bottom-up perspective, a reduction in sea <span class="hlt">ice</span> can both enhance bloom development by permitting greater levels of surface PAR uninhibited by <span class="hlt">ice</span> and suppress a bloom when reduced fresh melt-water inputs and increased vulnerability to wind stress combine to create deeper mixed layers and decrease depth integrated light availability. Regions along the Western Antarctic Peninsula have already seen a contradictory response to reduced <span class="hlt">ice</span> cover, with enhanced summertime chlorophyll concentrations in the South, and large declines to the North. This dichotomy is thought to arise from differences in the interannual mean sea <span class="hlt">ice</span> state, with extensively <span class="hlt">ice</span> covered regions benefiting from reduced coverage and more sparsely covered regions hindered by further reductions. The questions arises: 1) At what threshold does a reduction in sea <span class="hlt">ice</span> transition from amplifying blooms to suppressing them? 2) How do additional environmental considerations such as nutrient availability and trophic interactions complicate this transition? Here, we combine remote sensing observations and in-situ data (from PAL LTER) with a hierarchy of 1-D water column and global general circulation (CESM) models to access the <span class="hlt">variability</span> in how regional differences in mean <span class="hlt">ice</span> state combine with other environmental forcings to dictate how interannual <span class="hlt">variability</span> (or long term trends) in <span class="hlt">ice</span> coverage will affect bloom structure, size and dynamics. In doing so we will gain a better understanding of how predicted changes in sea <span class="hlt">ice</span> will effect Southern Ocean productivity, which of course will have important consequences in the global carbon cycle and sustainability of healthy marine ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GML....37..515H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GML....37..515H"><span>Evidence for Holocene centennial <span class="hlt">variability</span> in sea <span class="hlt">ice</span> cover based on IP25 biomarker reconstruction in the southern Kara Sea (Arctic Ocean)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hörner, Tanja; Stein, Rüdiger; Fahl, Kirsten</p> <p>2017-10-01</p> <p>The Holocene is characterized by the late Holocene cooling trend as well as by internal short-term centennial fluctuations. Because Arctic sea <span class="hlt">ice</span> acts as a significant component (amplifier) within the climate system, investigating its past long- and short-term <span class="hlt">variability</span> and controlling processes is beneficial for future climate predictions. This study presents the first biomarker-based (IP25 and PIP25) sea <span class="hlt">ice</span> reconstruction from the Kara Sea (core BP00-07/7), covering the last 8 ka. These biomarker proxies reflect conspicuous short-term sea <span class="hlt">ice</span> <span class="hlt">variability</span> during the last 6.5 ka that is identified unprecedentedly in the source region of Arctic sea <span class="hlt">ice</span> by means of a direct sea <span class="hlt">ice</span> indicator. Prominent peaks of extensive sea <span class="hlt">ice</span> cover occurred at 3, 2, 1.3 and 0.3 ka. Spectral analysis of the IP25 record revealed 400- and 950-year cycles. These periodicities may be related to the Arctic/North Atlantic Oscillation, but probably also to internal climate system fluctuations. This demonstrates that sea <span class="hlt">ice</span> belongs to a complex system that more likely depends on multiple internal forcing.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/9443674','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/9443674"><span>Psychologic, situational, and physiologic <span class="hlt">variables</span> and on-<span class="hlt">ice</span> performance of youth hockey goalkeepers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Smith, A M; Sim, F H; Smith, H C; Stuart, M J; Laskowski, E R</p> <p>1998-01-01</p> <p>To determine the relationship between psychologic, situational, and physiologic <span class="hlt">variables</span> and on-<span class="hlt">ice</span> performance of youth hockey goalkeepers. This study was structured to identify relationships and predictors of goalie performance. Because athletes playing solo positions in team sports have not been analyzed in depth in terms of precompetition anxiety and because goalkeeper performance is critical to game outcome, we undertook a study of 43 goalies at a hockey camp. These goalies completed psychometric inventories to assess trait and state anxiety, confidence, life stress, and social support. Holter monitors measured heart rate while the goalies rotated through on-<span class="hlt">ice</span> stations. Goalies were videotaped at the puck-shooting machine station, and performance (percent saves) was calculated. Trait (somatic) anxiety and positive mood state (ability to share) had different but significant relationships with on-<span class="hlt">ice</span> performance. Heart rates ranged from 88 to 208 beats/min at the on-<span class="hlt">ice</span> stations. Mean heart rate for older goalies (14 to 18 years of age) was 164 beats/min at the puck-shooting machine and 176 beats/min at other stations such as the slap-shot station. Older goalies performed well at a high level of arousal. Better performing goalies were more experienced, had faster heart rates "in the net," and had lower scores on all measures of anxiety.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6760381-iceberg-severity-off-eastern-north-america-its-relationship-sea-ice-variability-climate-change','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6760381-iceberg-severity-off-eastern-north-america-its-relationship-sea-ice-variability-climate-change"><span>Iceberg severity off eastern North America: Its relationship to sea <span class="hlt">ice</span> <span class="hlt">variability</span> and climate change</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Marko, J.R.; Fissel, D.B.; Wadhams, P.</p> <p>1994-09-01</p> <p>Iceberg trajectory, deterioration (mass loss), and sea <span class="hlt">ice</span> data are reviewed to identify the sources of observed interannual and seasonal variations in the numbers of icebergs passing south of 48[degrees]N off eastern North America. The results show the dominant role of sea <span class="hlt">ice</span> in the observed variations. Important mechanisms involved include both seasonal modulation of the southerly iceberg flow by <span class="hlt">ice</span> cover control of probabilities for entrapment and decay in shallow water, and the suppression of iceberg melt/deterioration rates by high concentrations of sea <span class="hlt">ice</span>. The Labrador spring <span class="hlt">ice</span> extent, shown to be the critical parameter in interannual iceberg numbermore » <span class="hlt">variability</span>, was found to be either determined by or closely correlated with midwinter Davis Strait <span class="hlt">ice</span> extents. Agreement obtained between observed year-to-year and seasonal number variations with computations based upon a simple iceberg dissipation model suggests that downstream iceberg numbers are relatively insensitive to iceberg production rates and to fluctuations in southerly iceberg fluxes in areas north of Baffin Island. Past variations in the Davis Strait <span class="hlt">ice</span> index and annual <span class="hlt">ice</span> extents are studied to identify trends and relationships between regional and larger-scale global climate parameters. It was found that, on decadal timescales in the post-1960 period of reasonable data quality, regional climate parameters have varied, roughly, out of phase with corresponding global and hemispheric changes. These observations are compared with expectations in terms of model results to evaluate current GCM-based capabilities for simulating recent regional behavior. 64 refs., 11 figs., 3 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JGRC..116.3007T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JGRC..116.3007T"><span>Trends and <span class="hlt">variability</span> in summer sea <span class="hlt">ice</span> cover in the Canadian Arctic based on the Canadian <span class="hlt">Ice</span> Service Digital Archive, 1960-2008 and 1968-2008</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tivy, Adrienne; Howell, Stephen E. L.; Alt, Bea; McCourt, Steve; Chagnon, Richard; Crocker, Greg; Carrieres, Tom; Yackel, John J.</p> <p>2011-03-01</p> <p>The Canadian <span class="hlt">Ice</span> Service Digital Archive (CISDA) is a compilation of weekly <span class="hlt">ice</span> charts covering Canadian waters from the early 1960s to present. The main sources of uncertainty in the database are reviewed and the data are validated for use in climate studies before trends and <span class="hlt">variability</span> in summer averaged sea <span class="hlt">ice</span> cover are investigated. These data revealed that between 1968 and 2008, summer sea <span class="hlt">ice</span> cover has decreased by 11.3% ± 2.6% decade-1 in Hudson Bay, 2.9% ± 1.2% decade-1 in the Canadian Arctic Archipelago (CAA), 8.9% ± 3.1% decade-1 in Baffin Bay, and 5.2% ± 2.4% decade-1 in the Beaufort Sea with no significant reductions in multiyear <span class="hlt">ice</span>. Reductions in sea <span class="hlt">ice</span> cover are linked to increases in early summer surface air temperature (SAT); significant increases in SAT were observed in every season and they are consistently greater than the pan-Arctic change by up to ˜0.2°C decade-1. Within the CAA and Baffin Bay, the El Niño-Southern Oscillation index correlates well with multiyear <span class="hlt">ice</span> coverage (positive) and first-year <span class="hlt">ice</span> coverage (negative) suggesting that El Niño episodes precede summers with more multiyear <span class="hlt">ice</span> and less first-year <span class="hlt">ice</span>. Extending the trend calculations back to 1960 along the major shipping routes revealed significant decreases in summer sea <span class="hlt">ice</span> coverage ranging between 11% and 15% decade-1 along the route through Hudson Bay and 6% and 10% decade-1 along the southern route of the Northwest Passage, the latter is linked to increases in SAT. Between 1960 and 2008, no significant trends were found along the northern western Parry Channel route of the Northwest Passage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1614162B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1614162B"><span>The role of <span class="hlt">ice</span> shelves in the Holocene evolution of the Antarctic <span class="hlt">ice</span> sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bernales, Jorge; Rogozhina, Irina; Thomas, Maik</p> <p>2014-05-01</p> <p>Using the continental-scale <span class="hlt">ice</span> sheet-shelf model SICOPOLIS (Greve, 1997 [1]; Sato and Greve, 2012 [2]), we assess the influence of <span class="hlt">ice</span> shelves on the Holocene evolution and present-day geometry of the Antarctic <span class="hlt">ice</span> sheet. We have designed a series of paleoclimate simulations driven by a time-evolved climate forcing that couples the surface temperature record from the Vostok <span class="hlt">ice</span> core with precipitation pattern using an empirical relation of Dahl-Jensen et al., (1998) [3]. Our numerical experiments show that the geometry of <span class="hlt">ice</span> shelves is determined by the evolution of climate and ocean conditions over time scales of 15 to 25 kyr. This implies that the initial configuration of <span class="hlt">ice</span> shelves at the Last Glacial Maximum (LGM, about 21 kyr before present) has a significant effect on the modelled Early Holocene <span class="hlt">volume</span> of <span class="hlt">ice</span> shelves (up to 20%) that gradually diminishes to a negligible level for the present-day <span class="hlt">ice</span> shelf configuration. Thus, the present-day geometry of the Antarctic <span class="hlt">ice</span> shelves can be attained even if an <span class="hlt">ice</span>-shelf-free initial condition is chosen at the LGM. However, the grounded <span class="hlt">ice</span> <span class="hlt">volume</span>, thickness and dynamic states are found to be sensitive to the <span class="hlt">ice</span> shelf dynamics over a longer history spanning several tens of thousands of years. A presence of extensive marine <span class="hlt">ice</span> at the LGM, supported by sediment core reconstructions (e.g. Naish et al., 2009 [4]), has a clear buttressing effect on the grounded <span class="hlt">ice</span> that remains significant over a period of 30 to 50 kyr. If <span class="hlt">ice</span>-shelf-free conditions are prescribed at the LGM, the modelled Early Holocene and present-day grounded <span class="hlt">ice</span> <span class="hlt">volumes</span> are underestimated by up to 10%, as opposed to simulations incorporating <span class="hlt">ice</span> shelf dynamics over longer periods. The use of <span class="hlt">ice</span>-shelf-free LGM conditions thus results in 50 to over 200 meters thinner <span class="hlt">ice</span> sheet across much of East Antarctica. References [1] Greve, R. (1997). Application of a polythermal three-dimensional <span class="hlt">ice</span> sheet model to the Greenland <span class="hlt">ice</span> sheet: response to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1242825','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1242825"><span>Investigations of Spatial and Temporal <span class="hlt">Variability</span> of Ocean and <span class="hlt">Ice</span> Conditions in and Near the Marginal <span class="hlt">Ice</span> Zone. The “Marginal <span class="hlt">Ice</span> Zone Observations and Processes Experiment” (MIZOPEX) Final Campaign Summary</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>DeMott, P. J.; Hill, T. C.J.</p> <p></p> <p>Despite the significance of the marginal <span class="hlt">ice</span> zones of the Arctic Ocean, basic parameters such as sea surface temperature (SST) and a range of sea-<span class="hlt">ice</span> characteristics are still insufficiently understood in these areas, and especially so during the summer melt period. The field campaigns summarized here, identified collectively as the “Marginal <span class="hlt">Ice</span> Zone Ocean and <span class="hlt">Ice</span> Observations and Processes Experiment” (MIZOPEX), were funded by U.S. National Aeronautic and Space Administration (NASA) with the intent of helping to address these information gaps through a targeted, intensive observation field campaign that tested and exploited unique capabilities of multiple classes of unmanned aerialmore » systems (UASs). MIZOPEX was conceived and carried out in response to NASA’s request for research efforts that would address a key area of science while also helping to advance the application of UASs in a manner useful to NASA for assessing the relative merits of different UASs. To further exercise the potential of unmanned systems and to expand the science value of the effort, the field campaign added further challenges such as air deployment of miniaturized buoys and coordinating missions involving multiple aircraft. Specific research areas that MIZOPEX data were designed to address include relationships between ocean skin temperatures and subsurface temperatures and how these evolve over time in an Arctic environment during summer; <span class="hlt">variability</span> in sea-<span class="hlt">ice</span> conditions such as thickness, age, and albedo within the marginal <span class="hlt">ice</span> zone (MIZ); interactions of SST, salinity, and <span class="hlt">ice</span> conditions during the melt cycle; and validation of satellite-derived SST and <span class="hlt">ice</span> concentration fields provided by satellite imagery and models.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26993670','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26993670"><span><span class="hlt">Variability</span> of Arthroscopy Case <span class="hlt">Volume</span> in Orthopaedic Surgery Residency.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gil, Joseph A; Waryasz, Gregory R; Owens, Brett D; Daniels, Alan H</p> <p>2016-05-01</p> <p>To examine orthopaedic surgery case logs for arthroscopy case <span class="hlt">volume</span> during residency training and to evaluate trends in case <span class="hlt">volume</span> and <span class="hlt">variability</span> over time. Publicly available Accreditation Council for Graduate Medical Education surgical case logs from 2007 to 2013 for orthopaedic surgery residency were assessed for <span class="hlt">variability</span> and case <span class="hlt">volume</span> trends in shoulder, elbow, wrist, hip, knee, and ankle arthroscopy. The national average number of procedures performed in each arthroscopy category reported was directly compared from 2009 to 2013. The 10th and 90th percentile arthroscopy case <span class="hlt">volume</span> was compared between 2007 and 2013 for shoulder and knee arthroscopy procedures. Subsequently, the difference between the 10th and 90th percentile arthroscopy case <span class="hlt">volume</span> in each category in 2007 was compared with the difference between the 10th and 90th percentile arthroscopy case <span class="hlt">volume</span> in each category in 2013. From 2007 to 2013, shoulder arthroscopy procedures performed per resident increased by 43.1% (P = .0001); elbow arthroscopy procedures increased by 28.0% (P = .00612); wrist arthroscopy procedures increased by 8.6% (P = .05); hip arthroscopy procedures, which were first reported in 2012, increased by 588.9%; knee arthroscopy procedures increased by 8.5% (P = .0435); ankle arthroscopy increased by 27.6% (P = .00149). The difference in knee and shoulder arthroscopy <span class="hlt">volume</span> between residents in the 10th and 90th percentile in 2007 and residents in the 10th and 90th percentile in 2013 was not significant (P > .05). There was a 3.66-fold difference in knee arthroscopy <span class="hlt">volume</span> between residents in the 10th and 90th percentile in 2007, whereas the difference was 3.36-fold in 2013 (P = .70). There was a 5.86-fold difference in shoulder arthroscopy case <span class="hlt">volume</span> between residents in the 10th and 90th percentile in 2007, whereas the difference was 4.96-fold in 2013 (P = .29). The <span class="hlt">volume</span> of arthroscopy cases performed by graduating orthopaedic surgery residents has</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA617649','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA617649"><span>Acquisition of <span class="hlt">Ice</span> Thickness and <span class="hlt">Ice</span> Surface Characteristics in the Seasonal <span class="hlt">Ice</span> Zone by CULPIS-X during the US Coast Guard’s Arctic Domain Awareness Program</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-09-30</p> <p>OBJECTIVES • What is the <span class="hlt">volume</span> of sea <span class="hlt">ice</span> in the Beaufort Sea Seasonal <span class="hlt">Ice</span> Zone (SIZ) and how does this evolve during summer as the <span class="hlt">ice</span> edge...retreats? Recent observations suggest that the remaining <span class="hlt">ice</span> in the Beaufort Sea is younger and thinner in recent years in part because even the oldest...surrounding <span class="hlt">ice</span> . Recent analyses have indicated that ponds on thinner <span class="hlt">ice</span> are often darker, accelerating the <span class="hlt">ice</span> - albedo feedback over thin <span class="hlt">ice</span> in summer</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/1013572','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/1013572"><span>Duration of the Arctic sea <span class="hlt">ice</span> melt season: Regional and interannual <span class="hlt">variability</span>, 1979-2001</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Belchansky, G.I.; Douglas, David C.; Platonov, Nikita G.</p> <p>2004-01-01</p> <p>Melt onset dates, freeze onset dates, and melt season duration were estimated over Arctic sea <span class="hlt">ice</span>, 1979–2001, using passive microwave satellite imagery and surface air temperature data. Sea <span class="hlt">ice</span> melt duration for the entire Northern Hemisphere varied from a 104-day minimum in 1983 and 1996 to a 124-day maximum in 1989. Ranges in melt duration were highest in peripheral seas, numbering 32, 42, 44, and 51 days in the Laptev, Barents-Kara, East Siberian, and Chukchi Seas, respectively. In the Arctic Ocean, average melt duration varied from a 75-day minimum in 1987 to a 103-day maximum in 1989. On average, melt onset in annual <span class="hlt">ice</span> began 10.6 days earlier than perennial <span class="hlt">ice</span>, and freeze onset in perennial <span class="hlt">ice</span> commenced 18.4 days earlier than annual <span class="hlt">ice</span>. Average annual melt dates, freeze dates, and melt durations in annual <span class="hlt">ice</span> were significantly correlated with seasonal strength of the Arctic Oscillation (AO). Following high-index AO winters (January–March), spring melt tended to be earlier and autumn freeze later, leading to longer melt season durations. The largest increases in melt duration were observed in the eastern Siberian Arctic, coincident with cyclonic low pressure and <span class="hlt">ice</span> motion anomalies associated with high-index AO phases. Following a positive AO shift in 1989, mean annual melt duration increased 2–3 weeks in the northern East Siberian and Chukchi Seas. Decreasing correlations between consecutive-year maps of melt onset in annual <span class="hlt">ice</span> during 1979–2001 indicated increasing spatial <span class="hlt">variability</span> and unpredictability in melt distributions from one year to the next. Despite recent declines in the winter AO index, recent melt distributions did not show evidence of reestablishing spatial patterns similar to those observed during the 1979–88 low-index AO period. Recent freeze distributions have become increasingly similar to those observed during 1979–88, suggesting a recurrent spatial pattern of freeze chronology under low-index AO conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/17337','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/17337"><span>Measurement <span class="hlt">variability</span> error for estimates of <span class="hlt">volume</span> change</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>James A. Westfall; Paul L. Patterson</p> <p>2007-01-01</p> <p>Using quality assurance data, measurement <span class="hlt">variability</span> distributions were developed for attributes that affect tree <span class="hlt">volume</span> prediction. Random deviations from the measurement <span class="hlt">variability</span> distributions were applied to 19381 remeasured sample trees in Maine. The additional error due to measurement variation and measurement bias was estimated via a simulation study for...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730022274','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730022274"><span><span class="hlt">Ice</span> pack heat sink subsystem - Phase 1, <span class="hlt">Volume</span> 1</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roebelen, G. J., Jr.</p> <p>1973-01-01</p> <p>The design, development, fabrication, and test at one-g of a functional laboratory model (non-flight) <span class="hlt">ice</span> pack heat sink subsystem to be used eventually for astronaut cooling during manned space missions are discussed. In normal use, excess heat in the liquid cooling garment (LCG) coolant is transferred to a reusable/regenerable <span class="hlt">ice</span> pack heat sink. For emergency operation, or for extension of extravehicular activity mission time after all the <span class="hlt">ice</span> has melted, water from the <span class="hlt">ice</span> pack is boiled to vacuum, thereby continuing to remove heat from the LCG coolant. This subsystem incorporates a quick connect/disconnect thermal interface between the <span class="hlt">ice</span> pack heat sink and the subsystem heat exchanger.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000070367&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dtemperature%2Bvariability','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000070367&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dtemperature%2Bvariability"><span>Seasonal-to-Interannual <span class="hlt">Variability</span> in Antarctic Sea-<span class="hlt">Ice</span> Dynamics, and Its Impact on Surface Fluxes and Water Mass Production</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Drinkwater, Mark R.</p> <p>1999-01-01</p> <p>Strong seasonal and interannual signals in Antarctic bottom-water outflow remain unexplained yet are highly correlated with anomalies in net sea-<span class="hlt">ice</span> growth in coastal polynyas. The mechanisms responsible for driving salination and replenishment and rejuvenation of the dense shelf "source" waters likely also generate pulses of bottom water outflow. The objective of this research is to investigate time-scales of <span class="hlt">variability</span> in the dynamics of sea-<span class="hlt">ice</span> in the Southern Ocean in order to determine the primary sites for production of dense shelf waters. We are using a merged satellite/buoy sea-<span class="hlt">ice</span> motion data set for the period 1978-present day to compute the dynamics of opening and closing of coastal polynyas over the continental shelf. The Ocean Circulation and Climate Advanced Model (OCCAM) ocean general circulation model with coupled sea-<span class="hlt">ice</span> dynamics is presently forced using National Center for Environmental Prediction (NCEP) data to simulate fluxes and the salination impact of the ocean shelf regions. This work is relevant in the context of measuring the influence of polar sea-<span class="hlt">ice</span> dynamics upon polar ocean characteristics, and thereby upon global thermohaline ocean circulation. Interannual <span class="hlt">variability</span> in simulated net freezing rate in the Southern Weddell Sea is shown for the period 1986-1993. There is a pronounced maximum of <span class="hlt">ice</span> production in 1988 and minimum in 1991 in response to anomalies in equatorward meridional wind velocity. This follows a similar approximate 8-year interannual cycle in Sea Surface Temperature (SST) and satellite-derived <span class="hlt">ice</span>-edge anomalies reported elsewhere as the "Antarctic Circumpolar Wave." The amplitude of interannual fluctuations in annual net <span class="hlt">ice</span> production are about 40% of the mean value, implying significant interannual variance in brine rejection and upper ocean heat loss. Southward anomalies in wind stress induce negative anomalies in open water production, which are observed in passive microwave satellite images. Thus, cycles of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1413317A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1413317A"><span>Atmospheric <span class="hlt">icing</span> of structures: Observations and simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ágústsson, H.; Elíasson, Á. J.; Thorsteins, E.; Rögnvaldsson, Ó.; Ólafsson, H.</p> <p>2012-04-01</p> <p>This study compares observed <span class="hlt">icing</span> in a test span in complex orography at Hallormsstaðaháls (575 m) in East-Iceland with parameterized <span class="hlt">icing</span> based on an <span class="hlt">icing</span> model and dynamically downscaled weather at high horizontal resolution. Four <span class="hlt">icing</span> events have been selected from an extensive dataset of observed atmospheric <span class="hlt">icing</span> in Iceland. A total of 86 test-spans have been erected since 1972 at 56 locations in complex terrain with more than 1000 <span class="hlt">icing</span> events documented. The events used here have peak observed <span class="hlt">ice</span> load between 4 and 36 kg/m. Most of the <span class="hlt">ice</span> accretion is in-cloud <span class="hlt">icing</span> but it may partly be mixed with freezing drizzle and wet snow <span class="hlt">icing</span>. The calculation of atmospheric <span class="hlt">icing</span> is made in two steps. First the atmospheric data is created by dynamically downscaling the ECMWF-analysis to high resolution using the non-hydrostatic mesoscale Advanced Research WRF-model. The horizontal resolution of 9, 3, 1 and 0.33 km is necessary to allow the atmospheric model to reproduce correctly local weather in the complex terrain of Iceland. Secondly, the Makkonen-model is used to calculate the <span class="hlt">ice</span> accretion rate on the conductors based on the simulated temperature, wind, cloud and precipitation <span class="hlt">variables</span> from the atmospheric data. In general, the atmospheric model correctly simulates the atmospheric <span class="hlt">variables</span> and <span class="hlt">icing</span> calculations based on the atmospheric <span class="hlt">variables</span> correctly identify the observed <span class="hlt">icing</span> events, but underestimate the load due to too slow <span class="hlt">ice</span> accretion. This is most obvious when the temperature is slightly below 0°C and the observed <span class="hlt">icing</span> is most intense. The model results improve significantly when additional observations of weather from an upstream weather station are used to nudge the atmospheric model. However, the large <span class="hlt">variability</span> in the simulated atmospheric <span class="hlt">variables</span> results in high temporal and spatial <span class="hlt">variability</span> in the calculated <span class="hlt">ice</span> accretion. Furthermore, there is high sensitivity of the <span class="hlt">icing</span> model to the droplet size and the possibility that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://nora.nerc.ac.uk/12794/1/Hill_111-122.pdf','USGSPUBS'); return false;" href="http://nora.nerc.ac.uk/12794/1/Hill_111-122.pdf"><span>Sensitivity of the Greenland <span class="hlt">Ice</span> Sheet to Pliocene sea surface temperatures</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hill, Daniel J.; Dolan, Aisling M.; Haywood, Alan M.; Hunter, Stephen J.; Stoll, Danielle K.</p> <p>2010-01-01</p> <p>PRISM3).Use of these different SSTswithin theHadley CentreGCM(GeneralCirculationModel) and BASISM (BritishAntarctic Survey <span class="hlt">Ice</span> Sheet Model), consistently show large reductions of Pliocene Greenland <span class="hlt">ice</span> <span class="hlt">volumes</span> compared to modern. The changes in climate introduced by the use of different SST reconstructions do change the predicted <span class="hlt">ice</span> <span class="hlt">volumes</span>, mainly through precipitation feedbacks. However, the models show a relatively low sensitivity of modelled Greenland <span class="hlt">ice</span> <span class="hlt">volumes</span> to different mid-Piacenzian SST reconstructions, with the largest SST induced changes being 20% of Pliocene <span class="hlt">ice</span> <span class="hlt">volume</span> or less than a metre of sea-level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP41C2260G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP41C2260G"><span>The Role of Arctic Sea <span class="hlt">Ice</span> in Last Millennium Climate <span class="hlt">Variability</span>: Model-Proxy Comparisons Using Ensemble Members and Novel Model Experiments.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gertler, C. G.; Monier, E.; Prinn, R. G.</p> <p>2016-12-01</p> <p><span class="hlt">Variability</span> in sea <span class="hlt">ice</span> extent is a prominent feature of forced simulations of the last millennium and reconstructions of paleoclimate using proxy records. The rapid 20th century decline in sea <span class="hlt">ice</span> extent is most likely due to greenhouse gas forcing, but the accuracy of future projections depend on the characterization of natural <span class="hlt">variability</span>. Declining sea <span class="hlt">ice</span> extent affects regional climate and society, but also plays a large role in Arctic amplification, with implications for mid-latitude circulation and even large-scale climate oscillations. To characterize the effects of natural and anthropogenic climate forcing on sea <span class="hlt">ice</span> and the related changes in large-scale atmospheric circulation, a combination of instrumental record, paleoclimate reconstructions, and general circulation models can be employed to recreate sea <span class="hlt">ice</span> extents and the corresponding atmosphere-ocean states. Model output from the last millennium ensemble (LME) is compared to a proxy-based sea <span class="hlt">ice</span> reconstruction and a global proxy network using a variety of statistical and data assimilation techniques. Further model runs using the Community Earth Systems Model (CESM) are performed with the same inputs as LME but forced with experimental sea <span class="hlt">ice</span> extents, and results are contextualized within the larger ensemble by a variety of metrics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.7308S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.7308S"><span><span class="hlt">Variability</span>, trends, and predictability of seasonal sea <span class="hlt">ice</span> retreat and advance in the Chukchi Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Serreze, Mark C.; Crawford, Alex D.; Stroeve, Julienne C.; Barrett, Andrew P.; Woodgate, Rebecca A.</p> <p>2016-10-01</p> <p>As assessed over the period 1979-2014, the date that sea <span class="hlt">ice</span> retreats to the shelf break (150 m contour) of the Chukchi Sea has a linear trend of -0.7 days per year. The date of seasonal <span class="hlt">ice</span> advance back to the shelf break has a steeper trend of about +1.5 days per year, together yielding an increase in the open water period of 80 days. Based on detrended time series, we ask how interannual <span class="hlt">variability</span> in advance and retreat dates relate to various forcing parameters including radiation fluxes, temperature and wind (from numerical reanalyses), and the oceanic heat inflow through the Bering Strait (from in situ moorings). Of all <span class="hlt">variables</span> considered, the retreat date is most strongly correlated (r ˜ 0.8) with the April through June Bering Strait heat inflow. After testing a suite of statistical linear models using several potential predictors, the best model for predicting the date of retreat includes only the April through June Bering Strait heat inflow, which explains 68% of retreat date variance. The best model predicting the <span class="hlt">ice</span> advance date includes the July through September inflow and the date of retreat, explaining 67% of advance date variance. We address these relationships by discussing heat balances within the Chukchi Sea, and the hypothesis of oceanic heat transport triggering ocean heat uptake and <span class="hlt">ice</span>-albedo feedback. Developing an operational prediction scheme for seasonal retreat and advance would require timely acquisition of Bering Strait heat inflow data. Predictability will likely always be limited by the chaotic nature of atmospheric circulation patterns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601788','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601788"><span>Acquisition of <span class="hlt">Ice</span> Thickness and <span class="hlt">Ice</span> Surface Characteristics in the Seasonal <span class="hlt">Ice</span> Zone by CULPIS-X During the US Coast Guard’s Arctic Domain Awareness Program</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-30</p> <p>What is the <span class="hlt">volume</span> of sea <span class="hlt">ice</span> in the Beaufort Sea SIZ and how does this evolve during summer as the <span class="hlt">ice</span> edge retreats? Recent observations...suggest that the remaining <span class="hlt">ice</span> in the Beaufort Sea is younger and thinner in recent years in part because even the oldest <span class="hlt">ice</span> advected into the region does...indicated that ponds on thinner <span class="hlt">ice</span> are often darker, accelerating the <span class="hlt">ice</span> - albedo feedback over thin <span class="hlt">ice</span> in summer. During winter, leads and very</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014CliPa..10.2135S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014CliPa..10.2135S"><span>Interaction of <span class="hlt">ice</span> sheets and climate during the past 800 000 years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stap, L. B.; van de Wal, R. S. W.; de Boer, B.; Bintanja, R.; Lourens, L. J.</p> <p>2014-12-01</p> <p>During the Cenozoic, land <span class="hlt">ice</span> and climate interacted on many different timescales. On long timescales, the effect of land <span class="hlt">ice</span> on global climate and sea level is mainly set by large <span class="hlt">ice</span> sheets in North America, Eurasia, Greenland and Antarctica. The climatic forcing of these <span class="hlt">ice</span> sheets is largely determined by the meridional temperature profile resulting from radiation and greenhouse gas (GHG) forcing. As a response, the <span class="hlt">ice</span> sheets cause an increase in albedo and surface elevation, which operates as a feedback in the climate system. To quantify the importance of these climate-land <span class="hlt">ice</span> processes, a zonally averaged energy balance climate model is coupled to five one-dimensional <span class="hlt">ice</span> sheet models, representing the major <span class="hlt">ice</span> sheets. In this study, we focus on the transient simulation of the past 800 000 years, where a high-confidence CO2 record from <span class="hlt">ice</span> core samples is used as input in combination with Milankovitch radiation changes. We obtain simulations of atmospheric temperature, <span class="hlt">ice</span> <span class="hlt">volume</span> and sea level that are in good agreement with recent proxy-data reconstructions. We examine long-term climate-<span class="hlt">ice</span>-sheet interactions by a comparison of simulations with uncoupled and coupled <span class="hlt">ice</span> sheets. We show that these interactions amplify global temperature anomalies by up to a factor of 2.6, and that they increase polar amplification by 94%. We demonstrate that, on these long timescales, the <span class="hlt">ice</span>-albedo feedback has a larger and more global influence on the meridional atmospheric temperature profile than the surface-height-temperature feedback. Furthermore, we assess the influence of CO2 and insolation by performing runs with one or both of these <span class="hlt">variables</span> held constant. We find that atmospheric temperature is controlled by a complex interaction of CO2 and insolation, and both <span class="hlt">variables</span> serve as thresholds for northern hemispheric glaciation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JESS..126...70K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JESS..126...70K"><span>Ocean sea-<span class="hlt">ice</span> modelling in the Southern Ocean around Indian Antarctic stations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, Anurag; Dwivedi, Suneet; Rajak, D. Ram</p> <p>2017-07-01</p> <p>An eddy-resolving coupled ocean sea-<span class="hlt">ice</span> modelling is carried out in the Southern Ocean region (9°-78°E; 51°-71°S) using the MITgcm. The model domain incorporates the Indian Antarctic stations, Maitri (11.7{°}E; 70.7{°}S) and Bharati (76.1{°}E; 69.4{°}S). The realistic simulation of the surface <span class="hlt">variables</span>, namely, sea surface temperature (SST), sea surface salinity (SSS), surface currents, sea <span class="hlt">ice</span> concentration (SIC) and sea <span class="hlt">ice</span> thickness (SIT) is presented for the period of 1997-2012. The horizontal resolution of the model varies between 6 and 10 km. The highest vertical resolution of 5 m is taken near the surface, which gradually increases with increasing depths. The seasonal <span class="hlt">variability</span> of the SST, SSS, SIC and currents is compared with the available observations in the region of study. It is found that the SIC of the model domain is increasing at a rate of 0.09% per month (nearly 1% per year), whereas, the SIC near Maitri and Bharati regions is increasing at a rate of 0.14 and 0.03% per month, respectively. The <span class="hlt">variability</span> of the drift of the sea-<span class="hlt">ice</span> is also estimated over the period of simulation. It is also found that the sea <span class="hlt">ice</span> <span class="hlt">volume</span> of the region increases at the rate of 0.0004 km3 per month (nearly 0.005 km3 per year). Further, it is revealed that the accumulation of sea <span class="hlt">ice</span> around Bharati station is more as compared to Maitri station.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1212967E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1212967E"><span>Unveiling climate and <span class="hlt">ice</span>-sheet history from drilling in high-latitude margins and future perspectives</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Escutia Dotti, Carlota</p> <p>2010-05-01</p> <p>Polar <span class="hlt">ice</span> is an important component of the climate system, affecting global sea level, ocean circulation and heat transport, marine productivity, and albedo. During the last decades drilling in the Arctic (IODP ACEX and Bering Expeditions) and in Antarctica (ODP Legs 178, 188, IODP Expedition 318 and ANDRILL) has revealed regional information about sea <span class="hlt">ice</span> and <span class="hlt">ice</span> sheets development and evolution. Integration of this data with numerical modeling provide an understanding of the early development of the <span class="hlt">ice</span> sheets and their <span class="hlt">variability</span> through the Cenozoic. Much of this work points to atmospheric CO2 and other greenhouse gases concentrations as important triggering mechanism driving the onset of glaciation and subsequent <span class="hlt">ice</span> <span class="hlt">volume</span> <span class="hlt">variability</span>. With current increasing atmospheric greenhouse gases concentrations resulting in rapidly rising global temperatures, studies of polar climates become increasingly prominent on the research agenda. Despite of the relevance of the high-latitudes in the global climate systems, the short- and long-term history of the <span class="hlt">ice</span> sheets and sea-<span class="hlt">ice</span> and its relationships with paleoclimatic, paleoceanographic, and sea level changes is still poorly understood. A multinational, multiplatform scientific drilling strategy is being developed to recover key physical evidence from selected high-latitude areas. This strategy is aimed at addressing key knowledge gaps about the role of polar <span class="hlt">ice</span> in climate change, targeting questions such as timing of events, rates of change, tipping points, regional variations, and northern vs. southern hemispheres (in phase or out-of-phase) <span class="hlt">variability</span>. This data is critical to provide constrains to sea-<span class="hlt">ice</span> and <span class="hlt">ice</span> sheet models, which are the basis for forecasting the future of the cryosphere in a warming world.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP13A2047K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP13A2047K"><span>Biomarker-based reconstruction of late Holocene sea-<span class="hlt">ice</span> <span class="hlt">variability</span>: East versus West Greenland continental shelf.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kolling, H. M.; Stein, R. H.; Fahl, K.</p> <p>2016-12-01</p> <p>Sea is a critical component of the climate system and its role is not yet fully understood e.g. the recent rapid decrease in sea <span class="hlt">ice</span> is not clearly reflected in climate models. This illustrates the need for high-resolution proxy-based sea-<span class="hlt">ice</span> reconstructions going beyond the time scale of direct measurements in order to understand the processes controlling present and past natural <span class="hlt">variability</span> of sea <span class="hlt">ice</span> on short time scales. Here we present the first comparison of two high-resolution biomarker records from the East and West Greenland Shelf for the late Holocene. Both areas are highly sensitive to sea-<span class="hlt">ice</span> changes as they are influenced by the East Greenland Current, the main exporter of Arctic freshwater and sea <span class="hlt">ice</span>. On the East Greenland Shelf, we do not find any clear evidence for a long-term increase of sea <span class="hlt">ice</span> during the late Holocene Neoglacial. This sea-<span class="hlt">ice</span> record seems to be more sensitive to short-term climate events, such as the Roman Warm Period, the Dark Ages, the Medieval Warm Period and the Little <span class="hlt">Ice</span> Age. In contrary, the West Greenland Shelf record shows a strong and gradual increase in sea <span class="hlt">ice</span> concentration and a reduction in marine productivity markers starting near 1.6 ka. In general, the increase in sea <span class="hlt">ice</span> seems to follow the decreasing solar insolation trend. Short-term events are not as clearly pronounced as on the East Greenland Shelf. A comparison to recently published foraminiferal records from the same cores (Perner et al., 2011, 2015) illuminates the differences of biomarker and micropaleontoligical proxies. It seems that the general trend is reflected in both proxies but the signal of small-scale events is preserved rather differently, pointing towards different environmental requirements of the species behind both proxies. References: Perner, K., et al., 2011. Quat. Sci. Revs. 30, 2815-2826 Perner, K., et al., 2015. Quat. Sci. Revs. 129, 296-307</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP54A..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP54A..01S"><span>Late Quaternary <span class="hlt">Variability</span> of Arctic Sea <span class="hlt">Ice</span>: Insights From Biomarker Proxy Records and Model Simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stein, R. H.; Fahl, K.; Gierz, P.; Niessen, F.; Lohmann, G.</p> <p>2017-12-01</p> <p>Over the last about four decades, coinciding with global warming and atmospheric CO2increase, the extent and thickness of Arctic sea <span class="hlt">ice</span> has decreased dramatically, a decrease much more rapid than predicted by climate models. The driving forces of this change are still not fully understood. In this context, detailed paleoclimatic records going back beyond the timescale of direct observations, i.e., high-resolution Holocene records but also records representing more distant warm periods, may help to to distinguish and quantify more precisely the natural and anthropogenic greenhouse gas forcing of global climate change and related sea <span class="hlt">ice</span> decrease. Here, we concentrate on sea <span class="hlt">ice</span> biomarker records representing the penultimate glacial/last interglacial (MIS 6/MIS 5e) and the Holocene time intervals. Our proxy records are compared with climate model simulations using a coupled atmosphere-ocean general circulation model (AOGCM). Based on our data, polynya-type sea <span class="hlt">ice</span> conditions probably occurred off the major <span class="hlt">ice</span> sheets along the northern Barents and East Siberian continental margins during late MIS 6. Furthermore, we demonstrate that even during MIS 5e, i.e., a time interval when the high latitudes have been significantly warmer than today, sea <span class="hlt">ice</span> existed in the central Arctic Ocean during summer, whereas sea <span class="hlt">ice</span> was significantly reduced along the Barents Sea continental margin influenced by Atlantic Water inflow. Assuming a closed Bering Strait (no Pacific Water inflow) during early MIS 5, model simulations point to a significantly reduced sea <span class="hlt">ice</span> cover in the central Arctic Ocean, a scenario that is however not supported by the proxy record and thus seems to be less realistic. Our Holocene biomarker proxy records from the Chukchi Sea indicate that main factors controlling the millennial Holocene <span class="hlt">variability</span> in sea <span class="hlt">ice</span> are probably changes in surface water and heat flow from the Pacific into the Arctic Ocean as well as the long-term decrease in summer insolation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.T44A..02A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.T44A..02A"><span><span class="hlt">Ice</span> Age Sea Level Change on a Dynamic Earth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Austermann, J.; Mitrovica, J. X.; Latychev, K.; Rovere, A.; Moucha, R.</p> <p>2014-12-01</p> <p>Changes in global mean sea level (GMSL) are a sensitive indicator of climate <span class="hlt">variability</span> during the current <span class="hlt">ice</span> age. Reconstructions are largely based on local sea level records, and the mapping to GMSL is computed from simulations of glacial isostatic adjustment (GIA) on 1-D Earth models. We argue, using two case studies, that resolving important, outstanding issues in <span class="hlt">ice</span> age paleoclimate requires a more sophisticated consideration of mantle structure and dynamics. First, we consider the coral record from Barbados, which is widely used to constrain global <span class="hlt">ice</span> <span class="hlt">volume</span> changes since the Last Glacial Maximum (LGM, ~21 ka). Analyses of the record using 1-D viscoelastic Earth models have estimated a GMSL change since LGM of ~120 m, a value at odds with analyses of other far field records, which range from 130-135 m. We revisit the Barbados case using a GIA model that includes laterally varying Earth structure (Austermann et al., Nature Geo., 2013) and demonstrate that neglecting this structure, in particular the high-viscosity slab in the mantle linked to the subduction of the South American plate, has biased (low) previous estimates of GMSL change since LGM by ~10 m. Our analysis brings the Barbados estimate into accord with studies from other far-field sites. Second, we revisit estimates of GMSL during the mid-Pliocene warm period (MPWP, ~3 Ma), which was characterized by temperatures 2-3°C higher than present. The <span class="hlt">ice</span> <span class="hlt">volume</span> deficit during this period is a source of contention, with estimates ranging from 0-40 m GMSL equivalent. We argue that refining estimates of <span class="hlt">ice</span> <span class="hlt">volume</span> during MPWP requires a correction for mantle flow induced dynamic topography (DT; Rowley et al., Science, 2013), a signal neglected in previous studies of <span class="hlt">ice</span> age sea level change. We present estimates of GIA- and DT-corrected elevations of MPWP shorelines from the U.S. east coast, Australia and South Africa in an attempt to reconcile these records with a single GMSL value.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMEP41B0695P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMEP41B0695P"><span>Constraints on Lobate Debris Apron Evolution and Rheology from Numerical Modeling of <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>Parsons, R.; Nimmo, F.</p> <p>2010-12-01</p> <p> <span class="hlt">variables</span> are spatially heterogeneous. We conclude that there are important regional differences in either the amount of dust mixed in with the <span class="hlt">ice</span>, or in the presence of a basal slope below the LDA <span class="hlt">ice</span>. Alternatively, the <span class="hlt">ice</span> temperature and/or timing of <span class="hlt">ice</span> deposition may vary significantly between different mid-latitude regions. a) Topographic profiles plotted every 200 My (thin, solid lines) from a 1 Gy simulation of <span class="hlt">ice</span> flow for an initial <span class="hlt">ice</span> deposit (thick, solid line) 5 km long and 1 km thick using an <span class="hlt">ice</span> temperature of 205 K and a dust fraction, φ, of 0.047%. A MOLA profile of an LDA at 38.6oN, 24.3oE (dashed line) is shown for comparison. b) Final profiles for simulations lasting 100 My using temperatures of 195, 205 and 215 K illustrate the effect of both temperature and increasing the dust <span class="hlt">volume</span> fraction to 1.2% (resulting in an <span class="hlt">ice</span> grain size of 1 mm).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..12210131K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..12210131K"><span>Oceanographic Controls on the <span class="hlt">Variability</span> of <span class="hlt">Ice</span>-Shelf Basal Melting and Circulation of Glacial Meltwater in the Amundsen Sea Embayment, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kimura, Satoshi; Jenkins, Adrian; Regan, Heather; Holland, Paul R.; Assmann, Karen M.; Whitt, Daniel B.; Van Wessem, Melchoir; van de Berg, Willem Jan; Reijmer, Carleen H.; Dutrieux, Pierre</p> <p>2017-12-01</p> <p><span class="hlt">Ice</span> shelves in the Amundsen Sea Embayment have thinned, accelerating the seaward flow of <span class="hlt">ice</span> sheets upstream over recent decades. This imbalance is caused by an increase in the ocean-driven melting of the <span class="hlt">ice</span> shelves. Observations and models show that the ocean heat content reaching the <span class="hlt">ice</span> shelves is sensitive to the depth of thermocline, which separates the cool, fresh surface waters from warm, salty waters. Yet the processes controlling the <span class="hlt">variability</span> of thermocline depth remain poorly constrained. Here we quantify the oceanic conditions and ocean-driven melting of Cosgrove, Pine Island Glacier (PIG), Thwaites, Crosson, and Dotson <span class="hlt">ice</span> shelves in the Amundsen Sea Embayment from 1991 to 2014 using a general circulation model. <span class="hlt">Ice</span>-shelf melting is coupled to <span class="hlt">variability</span> in the wind field and the sea-<span class="hlt">ice</span> motions over the continental shelf break and associated onshore advection of warm waters in deep troughs. The layer of warm, salty waters at the calving front of PIG and Thwaites is thicker in austral spring (June-October) than in austral summer (December-March), whereas the seasonal cycle at the calving front of Dotson is reversed. Furthermore, the ocean-driven melting in PIG is enhanced by an asymmetric response to changes in ocean heat transport anomalies at the continental shelf break: melting responds more rapidly to increases in ocean heat transport than to decreases. This asymmetry is caused by the inland deepening of bathymetry and the glacial meltwater circulation around the <span class="hlt">ice</span> shelf.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C32B..05A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C32B..05A"><span>Spatial <span class="hlt">variability</span> and trends of seasonal snowmelt processes over Antarctic sea <span class="hlt">ice</span> observed by satellite scatterometers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arndt, S.; Haas, C.</p> <p>2017-12-01</p> <p>Snow is one of the key drivers determining the seasonal energy and mass budgets of sea <span class="hlt">ice</span> in the Southern Ocean. Here, we analyze radar backscatter time series from the European Remote Sensing Satellites (ERS)-1 and-2 scatterometers, from the Quick Scatterometer (QSCAT), and from the Advanced Scatterometer (ASCAT) in order to observe the regional and inter-annual <span class="hlt">variability</span> of Antarctic snowmelt processes from 1992 to 2014. On perennial <span class="hlt">ice</span>, seasonal backscatter changes show two different snowmelt stages: A weak backscatter rise indicating the initial warming and metamorphosis of the snowpack (pre-melt), followed by a rapid rise indicating the onset of internal snowmelt and thaw-freeze cycles (snowmelt). In contrast, similar seasonal backscatter cycles are absent on seasonal <span class="hlt">ice</span>, preventing the periodic retrieval of spring/summer transitions. This may be due to the dominance of <span class="hlt">ice</span> bottom melt over snowmelt, leading to flooding and <span class="hlt">ice</span> disintegration before strong snowmelt sets in. Resulting snowmelt onset dates on perennial sea <span class="hlt">ice</span> show the expected latitudinal gradient from early melt onsets (mid-November) in the northern Weddell Sea towards late (end-December) or even absent snowmelt conditions further south. This result is likely related to seasonal variations in solar shortwave radiation (absorption). In addition, observations with different microwave frequencies allow to detect changing snow properties at different depths. We show that short wavelengths of passive microwave observations indicate earlier pre-melt and snowmelt onset dates than longer wavelength scatterometer observations, in response to earlier warming of upper snow layers compared to lower snow layers. Similarly, pre-melt and snowmelt onset dates retrieved from Ku-Band radars were earlier by an average of 11 and 23 days, respectively, than those retrieved from C-Band. This time difference was used to correct melt onset dates retrieved from Ku-Band to compile a consistent time series from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1048800','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1048800"><span>Converting Constant <span class="hlt">Volume</span>, Multizone Air Handling Systems to Energy Efficient <span class="hlt">Variable</span> Air <span class="hlt">Volume</span> Multizone Systems</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-10-26</p> <p>1 FINAL REPORT Converting Constant <span class="hlt">Volume</span>, Multizone Air Handling Systems to Energy Efficient <span class="hlt">Variable</span> Air <span class="hlt">Volume</span> Multizone...Systems Energy and Water Projects Project Number: EW-201152 ERDC-CERL 26 October 2017 2 TABLE OF CONTENTS ACKNOWLEDGEMENTS...16 3.2.1 Energy Usage (Quantitative</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51E2106B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51E2106B"><span>Spatio Temporal <span class="hlt">Variability</span> of the Global Transmittance During the Arctic POLARSTERN Expedition 106/1 <span class="hlt">Ice</span> Floe Station</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barrientos Velasco, C.; Macke, A.; Griesche, H.; Engelmann, R.; Deneke, H.; Seifert, P.</p> <p>2017-12-01</p> <p>The Arctic is warming at a higher rate than the rest of the planet. This has been leading to a dramatically decrease of snow coverage and sea <span class="hlt">ice</span> thickness in recent years and several studies have suggested that a similar trend is expected in the upcoming years. Large uncertainties in predicting the Arctic climate arise from our lack of understanding the role clouds play in sea <span class="hlt">ice</span> / atmosphere interaction. During summer the shortwave radiation dominates and clouds have a net cooling effect at the surface. The strength of this cooling critically depends on cloud phase, composition and height. Clouds interactions with aerosols, and its sensitivity to surface properties further complicates their role in the Arctic system. Scattering between the surface and cloud layers amplifies the cloud shortwave contribution, especially over a highly reflective surface such as snow or <span class="hlt">ice</span>. Therefore, to comprehend how the Arctic's surface is significantly modulated by solar radiation is necessary to more clearly understand the cloud-induced spatio-temporal <span class="hlt">variability</span> at process relevant scales. Irradiance <span class="hlt">variability</span> may also have an effect on the biological productivity of various plankton species below the <span class="hlt">ice</span>. The present study provides an overview of spatio-temporal <span class="hlt">variability</span> at spatial scales ranging from several decameters to 1 kilometer of the global transmittance derived from 15 pyranometer stations installed at an <span class="hlt">ice</span> floe station (June 4-16 2017) during the POLARSTERN expedition PS106/1. Specific irradiance statistics under clear sky, broken clouds and overcast conditions will be described considering the combination of a Cloud Radar Mira 35 and a Polly Raman polarization Lidar. Ultimately, radiative closure studies will be performed to quantify our abilities to reproduce realistic cloud solar radiative forcing under Arctic conditions. Acknowledgements. This research is funded by Deutsche Forschunsgemeinschaft (DFG) and involves the active participation of Leibniz</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> masses have shrunk below an anticipated critical extent, the <span class="hlt">ice</span>-albedo feedback might lead to the irreversible and unstoppable loss of the remaining <span class="hlt">ice</span>. We here give an overview of our current understanding of such threshold behavior. By using conceptual arguments, we review the recent findings that such a tipping point probably does not exist for the loss of Arctic summer sea <span class="hlt">ice</span>. Hence, in a cooler climate, sea <span class="hlt">ice</span> could recover rapidly from the loss it has experienced in recent years. In addition, we discuss why this recent rapid retreat of Arctic summer sea <span class="hlt">ice</span> might largely be a consequence of a slow shift in <span class="hlt">ice</span>-thickness distribution, which will lead to strongly increased year-to-year <span class="hlt">variability</span> of the Arctic summer sea-<span class="hlt">ice</span> extent. This <span class="hlt">variability</span> 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('https://ntrs.nasa.gov/search.jsp?R=20070034942&hterms=solar+energy&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dsolar%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070034942&hterms=solar+energy&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dsolar%2Benergy"><span>Seasonal Evolution and Interannual <span class="hlt">Variability</span> of the Local Solar Energy Absorbed by the Arctic Sea <span class="hlt">Ice</span>-Ocean System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Perovich, Donald K.; Nghiem, Son V.; Markus, Thorsten; Schwieger, Axel</p> <p>2007-01-01</p> <p>The melt season of the Arctic sea <span class="hlt">ice</span> cover is greatly affected by the partitioning of the incident solar radiation between reflection to the atmosphere and absorption in the <span class="hlt">ice</span> and ocean. This partitioning exhibits a strong seasonal cycle and significant interannual <span class="hlt">variability</span>. Data in the period 1998, 2000-2004 were analyzed in this study. Observations made during the 1997-1998 SHEBA (Surface HEat Budget of the Arctic Ocean) field experiment showed a strong seasonal dependence of the partitioning, dominated by a five-phase albedo evolution. QuikSCAT scatterometer data from the SHEBA region in 1999-2004 were used to further investigate solar partitioning in summer. The time series of scatterometer data were used to determine the onset of melt and the beginning of freezeup. This information was combined with SSM/I-derived <span class="hlt">ice</span> concentration, TOVS-based estimates of incident solar irradiance, and SHEBA results to estimate the amount of solar energy absorbed in the <span class="hlt">ice</span>-ocean system for these years. The average total solar energy absorbed in the <span class="hlt">ice</span>-ocean system from April through September was 900 MJ m(sup -2). There was considerable interannual <span class="hlt">variability</span>, with a range of 826 to 1044 MJ m(sup -2). The total amount of solar energy absorbed by the <span class="hlt">ice</span> and ocean was strongly related to the date of melt onset, but only weakly related to the total duration of the melt season or the onset of freezeup. The timing of melt onset is significant because the incident solar energy is large and a change at this time propagates through the entire melt season, affecting the albedo every day throughout melt and freezeup.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AIPC.1100..384H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AIPC.1100..384H"><span>Retrieval of <span class="hlt">Ice</span> Cloud Properties Using <span class="hlt">Variable</span> Phase Functions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heck, Patrick W.; Minnis, Patrick; Yang, Ping; Chang, Fu-Lung; Palikonda, Rabindra; Arduini, Robert F.; Sun-Mack, Sunny</p> <p>2009-03-01</p> <p>An enhancement to NASA Langley's Visible Infrared Solar-infrared Split-window Technique (VISST) is developed to identify and account for situations when errors are induced by using smooth <span class="hlt">ice</span> crystals. The retrieval scheme incorporates new <span class="hlt">ice</span> cloud phase functions that utilize hexagonal crystals with roughened surfaces. In some situations, cloud optical depths are reduced, hence, cloud height is increased. Cloud effective particle size also changes with the roughened <span class="hlt">ice</span> crystal models which results in varied effects on the calculation of <span class="hlt">ice</span> water path. Once validated and expanded, the new approach will be integrated in the CERES MODIS algorithm and real-time retrievals at Langley.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A13C0281K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A13C0281K"><span>Low-latitude <span class="hlt">variability</span> of <span class="hlt">ice</span> cloud properties and cloud thermodynamic phase observed by the Atmospheric Infrared Sounder (AIRS)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kahn, B. H.; Yue, Q.; Davis, S. M.; Fetzer, E. J.; Schreier, M. M.; Tian, B.; Wong, S.</p> <p>2016-12-01</p> <p>We will quantify the time and space dependence of <span class="hlt">ice</span> cloud effective radius (CER), optical thickness (COT), cloud top temperature (CTT), effective cloud fraction (ECF), and cloud thermodynamic phase (<span class="hlt">ice</span>, liquid, or unknown) with the Version 6 Atmospheric Infrared Sounder (AIRS) satellite observational data set from September 2002 until present. We show that cloud frequency, CTT, COT, and ECF have substantially different responses to ENSO variations. Large-scale changes in <span class="hlt">ice</span> CER are also observed with a several micron tropics-wide increase during the 2015-2016 El Niño and similar decreases during the La Niña phase. We show that the <span class="hlt">ice</span> CER variations reflect fundamental changes in the spatial distributions and relative frequencies of different <span class="hlt">ice</span> cloud types. Lastly, the high spatial and temporal resolution <span class="hlt">variability</span> of the cloud fields are explored and we show that these data capture a multitude of convectively coupled tropical waves such as Kelvin, westward and eastward intertio-gravity, equatorial Rossby, and mixed Rossby-gravity waves.</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> masses have shrunk below an anticipated critical extent, the ice–albedo feedback might lead to the irreversible and unstoppable loss of the remaining <span class="hlt">ice</span>. We here give an overview of our current understanding of such threshold behavior. By using conceptual arguments, we review the recent findings that such a tipping point probably does not exist for the loss of Arctic summer sea <span class="hlt">ice</span>. Hence, in a cooler climate, sea <span class="hlt">ice</span> could recover rapidly from the loss it has experienced in recent years. In addition, we discuss why this recent rapid retreat of Arctic summer sea <span class="hlt">ice</span> might largely be a consequence of a slow shift in <span class="hlt">ice</span>-thickness distribution, which will lead to strongly increased year-to-year <span class="hlt">variability</span> of the Arctic summer sea-<span class="hlt">ice</span> extent. This <span class="hlt">variability</span> 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('https://www.ncbi.nlm.nih.gov/pubmed/26206628','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26206628"><span>Capillary ion chromatography with on-column focusing for ultra-trace analysis of methanesulfonate and inorganic anions in limited <span class="hlt">volume</span> Antarctic <span class="hlt">ice</span> core samples.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rodriguez, Estrella Sanz; Poynter, Sam; Curran, Mark; Haddad, Paul R; Shellie, Robert A; Nesterenko, Pavel N; Paull, Brett</p> <p>2015-08-28</p> <p>Preservation of ionic species within Antarctic <span class="hlt">ice</span> yields a unique proxy record of the Earth's climate history. Studies have been focused until now on two proxies: the ionic components of sea salt aerosol and methanesulfonic acid. Measurement of the all of the major ionic species in <span class="hlt">ice</span> core samples is typically carried out by ion chromatography. Former methods, whilst providing suitable detection limits, have been based upon off-column preconcentration techniques, requiring larger sample <span class="hlt">volumes</span>, with potential for sample contamination and/or carryover. Here, a new capillary ion chromatography based analytical method has been developed for quantitative analysis of limited <span class="hlt">volume</span> Antarctic <span class="hlt">ice</span> core samples. The developed analytical protocol applies capillary ion chromatography (with suppressed conductivity detection) and direct on-column sample injection and focusing, thus eliminating the requirement for off-column sample preconcentration. This limits the total sample <span class="hlt">volume</span> needed to 300μL per analysis, allowing for triplicate sample analysis with <1mL of sample. This new approach provides a reliable and robust analytical method for the simultaneous determination of organic and inorganic anions, including fluoride, methanesulfonate, chloride, sulfate and nitrate anions. Application to composite <span class="hlt">ice</span>-core samples is demonstrated, with coupling of the capillary ion chromatograph to high resolution mass spectrometry used to confirm the presence and purity of the observed methanesulfonate peak. Copyright © 2015 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=ice&pg=2&id=EJ996849','ERIC'); return false;" href="https://eric.ed.gov/?q=ice&pg=2&id=EJ996849"><span>Everyday Engineering: Should <span class="hlt">Ice</span> Be Cubed?</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>Moyer, Richard H.; Everett, Susan A.</p> <p>2012-01-01</p> <p>While <span class="hlt">ice</span> is usually referred to as <span class="hlt">ice</span> cubes, indeed, most are not really cubes at all. In this 5E learning-cycle lesson, students will investigate different shapes of <span class="hlt">ice</span> and how shape affects the speed of melting and the rate of cooling a glass of water. Students will compare three different shapes of <span class="hlt">ice</span> with the same <span class="hlt">volume</span> but different…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110014308','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110014308"><span><span class="hlt">Ice</span> Lens Formation and Frost Heave at the Phoenix Landing Site</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zent, A. P.; Sizemore, H. G.; Remple, A. W.</p> <p>2011-01-01</p> <p>Several lines of evidence indicate that the <span class="hlt">volume</span> of shallow ground <span class="hlt">ice</span> in the martian high latitudes exceeds the pore <span class="hlt">volume</span> of the host regolith. Boynton et al. found an optimal fit to the Mars Odyssey Gamma Ray Spectrometer (GRS) data at the Phoenix landing site by modeling a buried layer of 50-75% <span class="hlt">ice</span> by mass (up to 90% <span class="hlt">ice</span> by <span class="hlt">volume</span>). Thermal and optical observations of recent impact craters in the northern hemisphere have revealed nearly pure <span class="hlt">ice</span>. <span class="hlt">Ice</span> deposits containing only 1-2% soil by <span class="hlt">volume</span> were excavated by Phoenix. The leading hypothesis for the origin of this excess <span class="hlt">ice</span> is that it developed in situ by a mechanism analogous to the formation of terrestrial <span class="hlt">ice</span> lenses and needle <span class="hlt">ice</span>. Problematically, terrestrial soil-<span class="hlt">ice</span> segregation is driven by freeze/thaw cycling and the movement of bulk water, neither of which are expected to have occurred in the geologically recent past on Mars. If however <span class="hlt">ice</span> lens formation is possible at temperatures less than 273 K, there are possible implications for the habitability of Mars permafrost, since the same thin films of unfrozen water that lead to <span class="hlt">ice</span> segregation are used by terrestrial psychrophiles to metabolize and grow down to temperatures of at least 258 K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.C53A..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.C53A..05S"><span>Discharge of New Subglacial Lake on Whillians <span class="hlt">Ice</span> Stream: Implication for <span class="hlt">Ice</span> Stream Flow Dynamics.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sergienko, O. V.; Fricker, H. A.; Bindschadler, R. A.; Vornberger, P. L.; Macayeal, D. R.</p> <p>2006-12-01</p> <p>One of the surprise discoveries made possible by the ICESat laser altimeter mission of 2004-2006 is the presence of a large subglacial lake below the grounding zone of Whillians <span class="hlt">Ice</span> Stream (dubbed here `Lake Helen' after the discoverer, Helen Fricker). What is even more surprising is the fact that this lake discharged a substantial portion of its <span class="hlt">volume</span> during the ICESat mission, and changes in lake <span class="hlt">volume</span> and surface elevation of the <span class="hlt">ice</span> stream are documented in exquisite detail [Fricker et al., in press]. The presence and apparent dynamism of large subglacial lakes in the grounding zone of a major <span class="hlt">ice</span> stream raises questions about their effects on <span class="hlt">ice</span>-stream dynamics. Being liquid and movable, water modifies basal friction spatially and temporally. Melting due to shear heating and geothermal flux reduces basal traction, making the <span class="hlt">ice</span> stream move fast. However, when water collects in a depression to form a lake, it potentially deprives the surrounding bed of lubricating water, and additionally makes the <span class="hlt">ice</span> surface flat, thereby locally decreasing the <span class="hlt">ice</span> stream driving stress. We study the effect of formation and discharge of a subglacial lake at the mouth of and <span class="hlt">ice</span> stream using a two dimensional, vertically integrated, <span class="hlt">ice</span>-stream model. The model is forced by the basal friction, <span class="hlt">ice</span> thickness and surface elevation. The basal friction is obtained by inversion of the <span class="hlt">ice</span> surface velocity, <span class="hlt">ice</span> thickness and surface elevation come from observations. To simulate the lake formation we introduce zero basal friction and "inflate" the basal elevation of the <span class="hlt">ice</span> stream at the site of the lake. Sensitivity studies of the response of the surrounding <span class="hlt">ice</span> stream and <span class="hlt">ice</span> shelf flow are performed to delineate the influence of near-grounding-line subglacial water storage for <span class="hlt">ice</span> streams in general.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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. Mass 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 mass loss and sea level rise. A major problem is that observations of modern-day <span class="hlt">ice</span> streams typically span just a few decades and, at the <span class="hlt">ice</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 mass loss over centuries or millennia, beyond those expected for a given ocean-climate forcing. To address this issue, numerous workers have sought to understand <span class="hlt">ice</span> stream dynamics over longer time-scales using their glacial geomorphology in the palaeo-record. Indeed, our understanding of their geomorphology has grown rapidly in the last three decades, from almost complete ignorance to a detailed knowledge of their geomorphological products. Building on this body of work, this paper uses the glacial geomorphology of 117 <span class="hlt">ice</span> streams in the North American Laurentide <span class="hlt">Ice</span> 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 <span class="hlt">variability</span> in both time and space, with <span class="hlt">ice</span> streams switching on and off in different locations. During deglaciation, we find that their overall number decreased, they occupied a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1042252','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1042252"><span>Converting Constant <span class="hlt">Volume</span>, Multizone Air Handling Systems to Energy Efficient <span class="hlt">Variable</span> Air <span class="hlt">Volume</span> Multizone Systems</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-10-26</p> <p>30. Energy Information Agency Natural Gas Price Data ..................................................................................... 65 Figure...different market sectors (residential, commercial, and industrial). Figure 30. Energy Information Agency Natural Gas Price Data 7.2.3 AHU Size...1 FINAL REPORT Converting Constant <span class="hlt">Volume</span>, Multizone Air Handling Systems to Energy Efficient <span class="hlt">Variable</span> Air <span class="hlt">Volume</span> Multizone</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.4343A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.4343A"><span>The impact of dynamic topography on the bedrock elevation and <span class="hlt">volume</span> of the Pliocene 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>Austermann, Jacqueline; Pollard, David; Mitrovica, Jerry X.; Moucha, Robert; Forte, Alessandro M.; DeConto, Robert M.</p> <p>2015-04-01</p> <p>Reconstructions of the Antarctic <span class="hlt">ice</span> sheet over long timescales (i.e. Myrs) require estimates of bedrock elevation through time. <span class="hlt">Ice</span> sheet models have accounted, with varying levels of sophistication, for changes in the bedrock elevation due to glacial isostatic adjustment (GIA), but they have neglected other processes that may perturb topography. One notable example is dynamic topography, the deflection of the solid surface of the Earth due to convective flow within the mantle. Numerically predicted changes in dynamic topography have been used to correct paleo shorelines for this departure from eustasy, but the effect of such changes on <span class="hlt">ice</span> sheet stability is unknown. In this study we use numerical predictions of time-varying dynamic topography to reconstruct bedrock elevation below the Antarctic <span class="hlt">ice</span> sheet during the mid Pliocene warm period (~3 Ma). Moreover, we couple this reconstruction to a three-dimensional <span class="hlt">ice</span> sheet model to explore the impact of dynamic topography on the evolution of the Antarctic <span class="hlt">ice</span> sheet since the Pliocene. Our modeling indicates significant uplift in the area of the Transantarctic Mountains (TAM) and the adjacent Wilkes basin. This predicted uplift, which is at the lower end of geological inferences of uplift of the TAM, implies a lower elevation of the basin in the Pliocene. Relative to simulations that do not include dynamic topography, the lower elevation leads to a smaller Antarctic <span class="hlt">Ice</span> Sheet <span class="hlt">volume</span> and a more significant retreat of the grounding line in the Wilkes basin, both of which are consistent with offshore sediment core data. We conclude that reconstructions of the Antarctic <span class="hlt">Ice</span> Sheet during the mid-Pliocene warm period should be based on bedrock elevation models that include the impact of both GIA and dynamic topography.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70171003','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70171003"><span>Role of ground <span class="hlt">ice</span> dynamics and ecological feedbacks in recent <span class="hlt">ice</span> wedge degradation and stabilization</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Mark Torre Jorgenson,; Mikhail Kanevskiy,; Yuri Shur,; Natalia Moskalenko,; Dana Brown,; Wickland, Kimberly P.; Striegl, Robert G.; Koch, Joshua C.</p> <p>2015-01-01</p> <p>Ground <span class="hlt">ice</span> is abundant in the upper permafrost throughout the Arctic and fundamentally affects terrain responses to climate warming. <span class="hlt">Ice</span> wedges, which form near the surface and are the dominant type of massive <span class="hlt">ice</span> in the Arctic, are particularly vulnerable to warming. Yet processes controlling <span class="hlt">ice</span> wedge degradation and stabilization are poorly understood. Here we quantified <span class="hlt">ice</span> wedge <span class="hlt">volume</span> and degradation rates, compared ground <span class="hlt">ice</span> characteristics and thermal regimes across a sequence of five degradation and stabilization stages and evaluated biophysical feedbacks controlling permafrost stability near Prudhoe Bay, Alaska. Mean <span class="hlt">ice</span> wedge <span class="hlt">volume</span> in the top 3 m of permafrost was 21%. Imagery from 1949 to 2012 showed thermokarst extent (area of water-filled troughs) was relatively small from 1949 (0.9%) to 1988 (1.5%), abruptly increased by 2004 (6.3%) and increased slightly by 2012 (7.5%). Mean annual surface temperatures varied by 4.9°C among degradation and stabilization stages and by 9.9°C from polygon center to deep lake bottom. Mean thicknesses of the active layer, <span class="hlt">ice</span>-poor transient layer, <span class="hlt">ice</span>-rich intermediate layer, thermokarst cave <span class="hlt">ice</span>, and wedge <span class="hlt">ice</span> varied substantially among stages. In early stages, thaw settlement caused water to impound in thermokarst troughs, creating positive feedbacks that increased net radiation, soil heat flux, and soil temperatures. Plant growth and organic matter accumulation in the degraded troughs provided negative feedbacks that allowed ground <span class="hlt">ice</span> to aggrade and heave the surface, thus reducing surface water depth and soil temperatures in later stages. The ground <span class="hlt">ice</span> dynamics and ecological feedbacks greatly complicate efforts to assess permafrost responses to climate change.</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/2015JGRF..120.2280J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRF..120.2280J"><span>Role of ground <span class="hlt">ice</span> dynamics and ecological feedbacks in recent <span class="hlt">ice</span> wedge degradation and stabilization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jorgenson, M. T.; Kanevskiy, M.; Shur, Y.; Moskalenko, N.; Brown, D. R. N.; Wickland, K.; Striegl, R.; Koch, J.</p> <p>2015-11-01</p> <p>Ground <span class="hlt">ice</span> is abundant in the upper permafrost throughout the Arctic and fundamentally affects terrain responses to climate warming. <span class="hlt">Ice</span> wedges, which form near the surface and are the dominant type of massive <span class="hlt">ice</span> in the Arctic, are particularly vulnerable to warming. Yet processes controlling <span class="hlt">ice</span> wedge degradation and stabilization are poorly understood. Here we quantified <span class="hlt">ice</span> wedge <span class="hlt">volume</span> and degradation rates, compared ground <span class="hlt">ice</span> characteristics and thermal regimes across a sequence of five degradation and stabilization stages and evaluated biophysical feedbacks controlling permafrost stability near Prudhoe Bay, Alaska. Mean <span class="hlt">ice</span> wedge <span class="hlt">volume</span> in the top 3 m of permafrost was 21%. Imagery from 1949 to 2012 showed thermokarst extent (area of water-filled troughs) was relatively small from 1949 (0.9%) to 1988 (1.5%), abruptly increased by 2004 (6.3%) and increased slightly by 2012 (7.5%). Mean annual surface temperatures varied by 4.9°C among degradation and stabilization stages and by 9.9°C from polygon center to deep lake bottom. Mean thicknesses of the active layer, <span class="hlt">ice</span>-poor transient layer, <span class="hlt">ice</span>-rich intermediate layer, thermokarst cave <span class="hlt">ice</span>, and wedge <span class="hlt">ice</span> varied substantially among stages. In early stages, thaw settlement caused water to impound in thermokarst troughs, creating positive feedbacks that increased net radiation, soil heat flux, and soil temperatures. Plant growth and organic matter accumulation in the degraded troughs provided negative feedbacks that allowed ground <span class="hlt">ice</span> to aggrade and heave the surface, thus reducing surface water depth and soil temperatures in later stages. The ground <span class="hlt">ice</span> dynamics and ecological feedbacks greatly complicate efforts to assess permafrost responses to climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24172978','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24172978"><span>Gradual demise of a thin southern Laurentide <span class="hlt">ice</span> sheet recorded by Mississippi drainage.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wickert, Andrew D; Mitrovica, Jerry X; Williams, Carlie; Anderson, Robert S</p> <p>2013-10-31</p> <p>At the Last Glacial Maximum (LGM), about 21,000 years before present, land-based <span class="hlt">ice</span> sheets held enough water to reduce global mean sea level by 130 metres. Yet after decades of study, major uncertainties remain as to the distribution of that <span class="hlt">ice</span>. Here we test four reconstructions of North American deglacial <span class="hlt">ice</span>-sheet history by quantitatively connecting them to high-resolution oxygen isotope (δ(18)O) records from the Gulf of Mexico using a water mixing model. For each reconstruction, we route meltwater and seasonal runoff through the time-evolving Mississippi drainage basin, which co-evolves with <span class="hlt">ice</span> geometry and changing topography as <span class="hlt">ice</span> loads deform the solid Earth and produce spatially <span class="hlt">variable</span> sea level in a process known as glacial isostatic adjustment. The δ(18)O records show that the Mississippi-drained southern Laurentide <span class="hlt">ice</span> sheet contributed only 5.4 ± 2.1 metres to global sea level rise, of which 0.66 ± 0.07 metres were released during the meltwater pulse 1A event 14,650-14,310 years before present, far less water than previously thought. In contrast, the three reconstructions based on glacial isostatic adjustment overpredict the δ(18)O-based post-LGM meltwater <span class="hlt">volume</span> by a factor of 1.6 to 3.6. The fourth reconstruction, which is based on <span class="hlt">ice</span> physics, has a low enough Mississippi-routed meltwater discharge to be consistent with δ(18)O constraints, but also contains the largest LGM North American <span class="hlt">ice</span> <span class="hlt">volume</span>. This suggests that modelling based on <span class="hlt">ice</span> physics may be the best way of matching isotopic records while also sequestering enough water in the North American <span class="hlt">ice</span> sheets to match the observed LGM sea level fall.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015E%26PSL.429...60S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015E%26PSL.429...60S"><span>Unstable AMOC during glacial intervals and millennial <span class="hlt">variability</span>: The role of mean sea <span class="hlt">ice</span> extent</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sévellec, Florian; Fedorov, Alexey V.</p> <p>2015-11-01</p> <p>A striking feature of paleoclimate records is the greater stability of the Holocene epoch relative to the preceding glacial interval, especially apparent in the North Atlantic region. In particular, strong irregular <span class="hlt">variability</span> with an approximately 1500 yr period, known as the Dansgaard-Oeschger (D-O) events, punctuates the last glaciation, but is absent during the interglacial. Prevailing theories, modeling and data suggest that these events, seen as abrupt warming episodes in Greenland <span class="hlt">ice</span> cores and sea surface temperature records in the North Atlantic, are linked to reorganizations of the Atlantic Meridional Overturning Circulation (AMOC). In this study, using a new low-order ocean model that reproduces a realistic power spectrum of millennial <span class="hlt">variability</span>, we explore differences in the AMOC stability between glacial and interglacial intervals of the 100 kyr glacial cycle of the Late Pleistocene (1 kyr = 1000 yr). Previous modeling studies show that the edge of sea <span class="hlt">ice</span> in the North Atlantic shifts southward during glacial intervals, moving the region of the North Atlantic Deep Water formation and the AMOC also southward. Here we demonstrate that, by shifting the AMOC with respect to the mean atmospheric precipitation field, such a displacement makes the system unstable, which explains chaotic millennial <span class="hlt">variability</span> during the glacials and the persistence of stable ocean conditions during the interglacials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011ACP....11.8363P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011ACP....11.8363P"><span>The <span class="hlt">variability</span> of tropical <span class="hlt">ice</span> cloud properties as a function of the large-scale context from ground-based radar-lidar observations over Darwin, Australia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Protat, A.; Delanoë, J.; May, P. T.; Haynes, J.; Jakob, C.; O'Connor, E.; Pope, M.; Wheeler, M. C.</p> <p>2011-08-01</p> <p>The high complexity of cloud parameterizations now held in models puts more pressure on observational studies to provide useful means to evaluate them. One approach to the problem put forth in the modelling community is to evaluate under what atmospheric conditions the parameterizations fail to simulate the cloud properties and under what conditions they do a good job. It is the ambition of this paper to characterize the <span class="hlt">variability</span> of the statistical properties of tropical <span class="hlt">ice</span> clouds in different tropical "regimes" recently identified in the literature to aid the development of better process-oriented parameterizations in models. For this purpose, the statistical properties of non-precipitating tropical <span class="hlt">ice</span> clouds over Darwin, Australia are characterized using ground-based radar-lidar observations from the Atmospheric Radiation Measurement (ARM) Program. The <span class="hlt">ice</span> cloud properties analysed are the frequency of <span class="hlt">ice</span> cloud occurrence, the morphological properties (cloud top height and thickness), and the microphysical and radiative properties (<span class="hlt">ice</span> water content, visible extinction, effective radius, and total concentration). The <span class="hlt">variability</span> of these tropical <span class="hlt">ice</span> cloud properties is then studied as a function of the large-scale cloud regimes derived from the International Satellite Cloud Climatology Project (ISCCP), the amplitude and phase of the Madden-Julian Oscillation (MJO), and the large-scale atmospheric regime as derived from a long-term record of radiosonde observations over Darwin. The vertical <span class="hlt">variability</span> of <span class="hlt">ice</span> cloud occurrence and microphysical properties is largest in all regimes (1.5 order of magnitude for <span class="hlt">ice</span> water content and extinction, a factor 3 in effective radius, and three orders of magnitude in concentration, typically). 98 % of <span class="hlt">ice</span> clouds in our dataset are characterized by either a small cloud fraction (smaller than 0.3) or a very large cloud fraction (larger than 0.9). In the <span class="hlt">ice</span> part of the troposphere three distinct layers characterized by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21G1186T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21G1186T"><span>There goes the sea <span class="hlt">ice</span>: following Arctic sea <span class="hlt">ice</span> parcels and their properties.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tschudi, M. A.; Tooth, M.; Meier, W.; Stewart, S.</p> <p>2017-12-01</p> <p>Arctic sea <span class="hlt">ice</span> distribution has changed considerably over the last couple of decades. Sea <span class="hlt">ice</span> extent record minimums have been observed in recent years, the distribution of <span class="hlt">ice</span> age now heavily favors younger <span class="hlt">ice</span>, and sea <span class="hlt">ice</span> is likely thinning. This new state of the Arctic sea <span class="hlt">ice</span> cover has several impacts, including effects on marine life, feedback on the warming of the ocean and atmosphere, and on the future evolution of the <span class="hlt">ice</span> pack. The shift in the state of the <span class="hlt">ice</span> cover, from a pack dominated by older <span class="hlt">ice</span>, to the current state of a pack with mostly young <span class="hlt">ice</span>, impacts specific properties of the <span class="hlt">ice</span> pack, and consequently the pack's response to the changing Arctic climate. For example, younger <span class="hlt">ice</span> typically contains more numerous melt ponds during the melt season, resulting in a lower albedo. First-year <span class="hlt">ice</span> is typically thinner and more fragile than multi-year <span class="hlt">ice</span>, making it more susceptible to dynamic and thermodynamic forcing. To investigate the response of the <span class="hlt">ice</span> pack to climate forcing during summertime melt, we have developed a database that tracks individual Arctic sea <span class="hlt">ice</span> parcels along with associated properties as these parcels advect during the summer. Our database tracks parcels in the Beaufort Sea, from 1985 - present, along with <span class="hlt">variables</span> such as <span class="hlt">ice</span> surface temperature, albedo, <span class="hlt">ice</span> concentration, and convergence. We are using this database to deduce how these thousands of tracked parcels fare during summer melt, i.e. what fraction of the parcels advect through the Beaufort, and what fraction melts out? The tracked <span class="hlt">variables</span> describe the thermodynamic and dynamic forcing on these parcels during their journey. This database will also be made available to all interested investigators, after it is published in the near future. The attached image shows the <span class="hlt">ice</span> surface temperature of all parcels (right) that advected through the Beaufort Sea region (left) in 2014.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24587084','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24587084"><span>Neurobiological degeneracy and affordance perception support functional intra-individual <span class="hlt">variability</span> of inter-limb coordination during <span class="hlt">ice</span> climbing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Seifert, Ludovic; Wattebled, Léo; Herault, Romain; Poizat, Germain; Adé, David; Gal-Petitfaux, Nathalie; Davids, Keith</p> <p>2014-01-01</p> <p>This study investigated the functional intra-individual movement <span class="hlt">variability</span> of <span class="hlt">ice</span> climbers differing in skill level to understand how icefall properties were used by participants as affordances to adapt inter-limb coordination patterns during performance. Seven expert climbers and seven beginners were observed as they climbed a 30 m icefall. Movement and positioning of the left and right hand <span class="hlt">ice</span> tools, crampons and the climber's pelvis over the first 20 m of the climb were recorded and digitized using video footage from a camera (25 Hz) located perpendicular to the plane of the icefall. Inter-limb coordination, frequency and types of action and vertical axis pelvis displacement exhibited by each climber were analysed for the first five minutes of ascent. Participant perception of climbing affordances was assessed through: (i) calculating the ratio between exploratory movements and performed actions, and (ii), identifying, by self-confrontation interviews, the perceptual <span class="hlt">variables</span> of environmental properties, which were significant to climbers for their actions. Data revealed that experts used a wider range of upper and lower limb coordination patterns, resulting in the emergence of different types of action and fewer exploratory movements, suggesting that effective holes in the icefall provided affordances to regulate performance. In contrast, beginners displayed lower levels of functional intra-individual <span class="hlt">variability</span> of motor organization, due to repetitive swinging of <span class="hlt">ice</span> tools and kicking of crampons to achieve and maintain a deep anchorage, suggesting lack of perceptual attunement and calibration to environmental properties to support climbing performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE14B1411P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE14B1411P"><span>Atmospheric form drag over Arctic sea <span class="hlt">ice</span> derived from high-resolution <span class="hlt">Ice</span>Bridge elevation data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Petty, A.; Tsamados, M.; Kurtz, N. T.</p> <p>2016-02-01</p> <p>Here we present a detailed analysis of atmospheric form drag over Arctic sea <span class="hlt">ice</span>, using high resolution, three-dimensional surface elevation data from the NASA Operation <span class="hlt">Ice</span>Bridge Airborne Topographic Mapper (ATM) laser altimeter. Surface features in the sea <span class="hlt">ice</span> cover are detected using a novel feature-picking algorithm. We derive information regarding the height, spacing and orientation of unique surface features from 2009-2014 across both first-year and multiyear <span class="hlt">ice</span> regimes. The topography results are used to explicitly calculate atmospheric form drag coefficients; utilizing existing form drag parameterizations. The atmospheric form drag coefficients show strong regional <span class="hlt">variability</span>, mainly due to <span class="hlt">variability</span> in <span class="hlt">ice</span> type/age. The transition from a perennial to a seasonal <span class="hlt">ice</span> cover therefore suggest a decrease in the atmospheric form drag coefficients over Arctic sea <span class="hlt">ice</span> in recent decades. These results are also being used to calibrate a recent form drag parameterization scheme included in the sea <span class="hlt">ice</span> model CICE, to improve the representation of form drag over Arctic sea <span class="hlt">ice</span> in global climate models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AsBio..17..941B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AsBio..17..941B"><span>Plume Activity and Tidal Deformation on Enceladus Influenced by Faults and <span class="hlt">Variable</span> <span class="hlt">Ice</span> Shell Thickness</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Běhounková, Marie; Souček, Ondřej; Hron, Jaroslav; Čadek, Ondřej</p> <p>2017-09-01</p> <p>We investigated the effect of variations in <span class="hlt">ice</span> shell thickness and of the tiger stripe fractures crossing Enceladus' south polar terrain on the moon's tidal deformation by performing finite element calculations in three-dimensional geometry. The combination of thinning in the polar region and the presence of faults has a synergistic effect that leads to an increase of both the displacement and stress in the south polar terrain by an order of magnitude compared to that of the traditional model with a uniform shell thickness and without faults. Assuming a simplified conductive heat transfer and neglecting the heat sources below the <span class="hlt">ice</span> shell, we computed the global heat budget of the <span class="hlt">ice</span> shell. For the inelastic properties of the shell described by a Maxwell viscoelastic model, we show that unrealistically low average viscosity of the order of 10^{13} Pa s is necessary for preserving the <span class="hlt">volume</span> of the ocean, suggesting the important role of the heat sources in the deep interior. Similarly, low viscosity is required to predict the observed delay of the plume activity, which hints at other delaying mechanisms than just the viscoelasticity of the <span class="hlt">ice</span> shell. The presence of faults results in large spatial and temporal heterogeneity of geysering activity compared to the traditional models without faults. Our model contributes to understanding the physical mechanisms that control the fault activity, and it provides potentially useful information for future missions that will sample the plume for evidence of life.</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><span class="hlt">Variable</span> 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 mass balance, firn state, <span class="hlt">ice</span> dynamics, and basal mass 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 mass 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/2016AGUFM.C33B0821P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C33B0821P"><span>RADARSAT-2 Polarimetric Radar Imaging for Lake <span class="hlt">Ice</span> Mapping</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pan, F.; Kang, K.; Duguay, C. R.</p> <p>2016-12-01</p> <p>Changes in lake <span class="hlt">ice</span> dates and duration are useful indicators for assessing long-term climate trends and <span class="hlt">variability</span> in northern countries. Lake <span class="hlt">ice</span> cover observations are also a valuable data source for predictions with numerical <span class="hlt">ice</span> and weather forecasting models. In recent years, satellite remote sensing has assumed a greater role in providing observations of lake <span class="hlt">ice</span> cover extent for both modeling and climate monitoring purposes. Polarimetric radar imaging has become a promising tool for lake <span class="hlt">ice</span> mapping at high latitudes where meteorological conditions and polar darkness severely limit observations from optical sensors. In this study, we assessed and characterized the physical scattering mechanisms of lake <span class="hlt">ice</span> from fully polarimetric RADARSAT-2 datasets obtained over Great Bear Lake, Canada, with the intent of classifying open water and different <span class="hlt">ice</span> types during the freeze-up and break-up periods. Model-based and eigen-based decompositions were employed to construct the coherency matrix into deterministic scattering mechanisms. These procedures as well as basic polarimetric parameters were integrated into modified convolutional neural networks (CNN). The CNN were modified via introduction of a Markov random field into the higher iterative layers of networks for acquiring updated priors and classifying <span class="hlt">ice</span> and open water areas over the lake. We show that the selected polarimetric parameters can help with interpretation of radar-<span class="hlt">ice</span>/water interactions and can be used successfully for water-<span class="hlt">ice</span> segmentation, including different <span class="hlt">ice</span> types. As more satellite SAR sensors are being launched or planned, such as the Sentinel-1a/b series and the upcoming RADARSAT Constellation Mission, the rapid <span class="hlt">volume</span> growth of data and their analysis require the development of robust automated algorithms. The approach developed in this study was therefore designed with the intent of moving towards fully automated mapping of lake <span class="hlt">ice</span> for consideration by <span class="hlt">ice</span> services.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFMPP31B0418F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFMPP31B0418F"><span>The Search for Eight Glacial Cycles of Deep-Water Temperatures and Global <span class="hlt">ice</span> <span class="hlt">Volume</span> From the Southern Hemisphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferretti, P.; Elderfield, H.; Greaves, M.; McCave, N.</p> <p>2007-12-01</p> <p>/Ca and B/Ca on planktonic species, which also provides evidence on carbonate saturation state. These results permit preliminary discussion of the magnitude of the deep-water temperature changes during glacial/interglacial transitions and the interglacials themselves. In particular, our deep-water temperature estimates confirm that interglacial stages before 430 ka were characterized by less pronounced warmth - at least in the deeper southern Pacific - than those of the past four climatic cycles, a pattern previously observed in the deuterium record from EPICA Dome C. We examine the relative contributions of deep-water temperature and <span class="hlt">ice</span> <span class="hlt">volume</span> to the benthic δ18O signal. The phase relationship between the two signals is tentatively assessed for the middle/late Pleistocene, when different patterns of climate <span class="hlt">variability</span> have been inferred from marine and <span class="hlt">ice</span> cores records.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C13E..07L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C13E..07L"><span>EM Bias-Correction for <span class="hlt">Ice</span> Thickness and Surface Roughness Retrievals over Rough Deformed Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, L.; Gaiser, P. W.; Allard, R.; Posey, P. G.; Hebert, D. A.; Richter-Menge, J.; Polashenski, C. M.</p> <p>2016-12-01</p> <p>The very rough ridge sea <span class="hlt">ice</span> accounts for significant percentage of total <span class="hlt">ice</span> areas and even larger percentage of total <span class="hlt">volume</span>. The commonly used Radar altimeter surface detection techniques are empirical in nature and work well only over level/smooth sea <span class="hlt">ice</span>. Rough sea <span class="hlt">ice</span> surfaces can modify the return waveforms, resulting in significant Electromagnetic (EM) bias in the estimated surface elevations, and thus large errors in the <span class="hlt">ice</span> thickness retrievals. To understand and quantify such sea <span class="hlt">ice</span> surface roughness effects, a combined EM rough surface and <span class="hlt">volume</span> scattering model was developed to simulate radar returns from the rough sea <span class="hlt">ice</span> `layer cake' structure. A waveform matching technique was also developed to fit observed waveforms to a physically-based waveform model and subsequently correct the roughness induced EM bias in the estimated freeboard. This new EM Bias Corrected (EMBC) algorithm was able to better retrieve surface elevations and estimate the surface roughness parameter simultaneously. In situ data from multi-instrument airborne and ground campaigns were used to validate the <span class="hlt">ice</span> thickness and surface roughness retrievals. For the surface roughness retrievals, we applied this EMBC algorithm to co-incident LiDAR/Radar measurements collected during a Cryosat-2 under-flight by the NASA <span class="hlt">Ice</span>Bridge missions. Results show that not only does the waveform model fit very well to the measured radar waveform, but also the roughness parameters derived independently from the LiDAR and radar data agree very well for both level and deformed sea <span class="hlt">ice</span>. For sea <span class="hlt">ice</span> thickness retrievals, validation based on in-situ data from the coordinated CRREL/NRL field campaign demonstrates that the physically-based EMBC algorithm performs fundamentally better than the empirical algorithm over very rough deformed sea <span class="hlt">ice</span>, suggesting that sea <span class="hlt">ice</span> surface roughness effects can be modeled and corrected based solely on the radar return waveforms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14765804','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14765804"><span><span class="hlt">Ice</span> cream structural elements that affect melting rate and hardness.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Muse, M R; Hartel, R W</p> <p>2004-01-01</p> <p>Statistical models were developed to reveal which structural elements of <span class="hlt">ice</span> cream affect melting rate and hardness. <span class="hlt">Ice</span> creams were frozen in a batch freezer with three types of sweetener, three levels of the emulsifier polysorbate 80, and two different draw temperatures to produce <span class="hlt">ice</span> creams with a range of microstructures. <span class="hlt">Ice</span> cream mixes were analyzed for viscosity, and finished <span class="hlt">ice</span> creams were analyzed for air cell and <span class="hlt">ice</span> crystal size, overrun, and fat destabilization. The <span class="hlt">ice</span> phase <span class="hlt">volume</span> of each <span class="hlt">ice</span> cream were calculated based on the freezing point of the mix. Melting rate and hardness of each hardened <span class="hlt">ice</span> cream was measured and correlated with the structural attributes by using analysis of variance and multiple linear regression. Fat destabilization, <span class="hlt">ice</span> crystal size, and the consistency coefficient of the mix were found to affect the melting rate of <span class="hlt">ice</span> cream, whereas hardness was influenced by <span class="hlt">ice</span> phase <span class="hlt">volume</span>, <span class="hlt">ice</span> crystal size, overrun, fat destabilization, and the rheological properties of the mix.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70022940','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70022940"><span><span class="hlt">Variability</span> of Mars' North Polar Water <span class="hlt">Ice</span> Cap: I. Analysis of Mariner 9 and Viking Orbiter Imaging Data</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bass, Deborah S.; Herkenhoff, Kenneth; Paige, David A.</p> <p>2000-01-01</p> <p>Previous studies interpreted differences in <span class="hlt">ice</span> coverage between Mariner 9 and Viking Orbiter observations of Mars' north residual polar cap as evidence of interannual <span class="hlt">variability</span> of <span class="hlt">ice</span> deposition on the cap. However, these investigators did not consider the possibility that there could be significant changes in the <span class="hlt">ice</span> coverage within the northern residual cap over the course of the summer season. Our more comprehensive analysis of Mariner 9 and Viking Orbiter imaging data shows that the appearance of the residual cap does not show large-scale variance on an interannual basis. Rather we find evidence that regions that were dark at the beginning of summer look bright by the end of summer and that this seasonal variation of the cap repeats from year to year. Our results suggest that this brightening was due to the deposition of newly formed water <span class="hlt">ice</span> on the surface. We find that newly formed <span class="hlt">ice</span> deposits in the summer season have the same red-to-violet band image ratios as permanently bright deposits within the residual cap. We believe the newly formed <span class="hlt">ice</span> accumulates in a continuous layer. To constrain the minimum amount of deposited <span class="hlt">ice</span>, we used observed albedo data in conjunction with calculations using Mie theory for single scattering and a delta-Eddington approximation of radiative transfer for multiple scattering. The brightening could have been produced by a minimum of (1) a ~35-μm-thick layer of 50-μm-sized <span class="hlt">ice</span> particles with 10% dust or (2) a ~14-μm-thick layer of 10-μm-sized <span class="hlt">ice</span> particles with 50% dust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011Icar..214..246P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011Icar..214..246P"><span>Constraints on martian lobate debris apron evolution and rheology from numerical modeling of <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>Parsons, Reid A.; Nimmo, Francis; Miyamoto, Hideaki</p> <p>2011-07-01</p> <p>Radar observations in the Deuteronilus Mensae region by Mars Reconnaissance Orbiter have constrained the thickness and dust concentration found within mid-latitude <span class="hlt">ice</span> deposits, providing an opportunity to more accurately estimate the rheology of <span class="hlt">ice</span> responsible for the formation of lobate debris aprons based on their apparent age of ˜100 Myr. We developed a numerical model simulating <span class="hlt">ice</span> flow under martian conditions using results from <span class="hlt">ice</span> deformation experiments, theory of <span class="hlt">ice</span> grain growth based on terrestrial <span class="hlt">ice</span> cores, and observational constraints from radar profiles and laser altimetry. By varying the <span class="hlt">ice</span> grain size, the <span class="hlt">ice</span> temperature, the subsurface slope, and the initial <span class="hlt">ice</span> <span class="hlt">volume</span> we determine the combination of parameters that best reproduce the observed LDA lengths and thicknesses over a period of time comparable to the apparent ages of LDA surfaces (90-300 Myr). We find that an <span class="hlt">ice</span> temperature of 205 K, an <span class="hlt">ice</span> grain size of 5 mm, and a flat subsurface slope give reasonable ages for many LDAs in the northern mid-latitudes of Mars. Assuming that the <span class="hlt">ice</span> grain size is limited by the grain boundary pinning effect of incorporated dust, these results limit the dust <span class="hlt">volume</span> concentration to less than 4%. However, assuming all LDAs were emplaced by a single event, we find that there is no single combination of grain size, temperature, and subsurface slope which can give realistic ages for all LDAs, suggesting that some or all of these <span class="hlt">variables</span> are spatially heterogeneous. Based on our model we conclude that the majority of northern mid-latitude LDAs are composed of clean (⩽4 vol%), coarse (⩾1 mm) grained <span class="hlt">ice</span>, but regional differences in either the amount of dust mixed in with the <span class="hlt">ice</span>, or in the presence of a basal slope below the LDA <span class="hlt">ice</span> must be invoked. Alternatively, the <span class="hlt">ice</span> temperature and/or timing of <span class="hlt">ice</span> deposition may vary significantly between different mid-latitude regions. Either eventuality can be tested with future observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016QuRes..86..373O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016QuRes..86..373O"><span>The complexity of millennial-scale <span class="hlt">variability</span> in southwestern Europe during MIS 11</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oliveira, Dulce; Desprat, Stéphanie; Rodrigues, Teresa; Naughton, Filipa; Hodell, David; Trigo, Ricardo; Rufino, Marta; Lopes, Cristina; Abrantes, Fátima; Sánchez Goñi, Maria Fernanda</p> <p>2016-11-01</p> <p>Climatic <span class="hlt">variability</span> of Marine Isotope Stage (MIS) 11 is examined using a new high-resolution direct land-sea comparison from the SW Iberian margin Site U1385. This study, based on pollen and biomarker analyses, documents regional vegetation, terrestrial climate and sea surface temperature (SST) <span class="hlt">variability</span>. Suborbital climate <span class="hlt">variability</span> is revealed by a series of forest decline events suggesting repeated cooling and drying episodes in SW Iberia throughout MIS 11. Only the most severe events on land are coeval with SST decreases, under larger <span class="hlt">ice</span> <span class="hlt">volume</span> conditions. Our study shows that the diverse expression (magnitude, character and duration) of the millennial-scale cooling events in SW Europe relies on atmospheric and oceanic processes whose predominant role likely depends on baseline climate states. Repeated atmospheric shifts recalling the positive North Atlantic Oscillation mode, inducing dryness in SW Iberia without systematical SST changes, would prevail during low <span class="hlt">ice</span> <span class="hlt">volume</span> conditions. In contrast, disruption of the Atlantic meridional overturning circulation (AMOC), related to iceberg discharges, colder SST and increased hydrological regime, would be responsible for the coldest and driest episodes of prolonged duration in SW Europe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G31C0924M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G31C0924M"><span>Temporal <span class="hlt">variability</span> of the Antarctic <span class="hlt">Ice</span> sheet observed from space-based geodesy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Memin, A.; King, M. A.; Boy, J. P.; Remy, F.</p> <p>2017-12-01</p> <p>Quantifying the Antarctic <span class="hlt">Ice</span> Sheet (AIS) mass balance still remains challenging as several processes compete to differing degrees at the basin scale with regional variations, leading to multiple mass redistribution patterns. For instance, analysis of linear trends in surface-height variations from 1992-2003 and 2002-2006 shows that the AIS is subject to decimetric scale <span class="hlt">variability</span> over periods of a few years. Every year, snowfalls in Antarctica represent the equivalent of 6 mm of the mean sea level. Therefore, any fluctuation in precipitation can lead to changes in sea level. Besides, over the last decade, several major glaciers have been thinning at an accelerating rate. Understanding the processes that interact on the <span class="hlt">ice</span> sheet is therefore important to precisely determine the response of the <span class="hlt">ice</span> sheet to a rapid changing climate and estimate its contribution to sea level changes. We estimate seasonal and interannual changes of the AIS between January 2003 and October 2010 and to the end of 2016 from a combined analysis of surface-elevation and surface-mass changes derived from Envisat data and GRACE solutions, and from GRACE solutions only, respectively. While we obtain a good correlation for the interannual signal between the two techniques, important differences (in amplitude, phase, and spatial pattern) are obtained for the seasonal signal. We investigate these discrepancies by comparing the crustal motion observed by GPS and those predicted using monthly surface mass balance derived from the regional atmospheric climate model RACMO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036459','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036459"><span>Whole-edifice <span class="hlt">ice</span> <span class="hlt">volume</span> change A.D. 1970 to 2007/2008 at Mount Rainier, Washington, based on LiDAR surveying</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sisson, T.W.; Robinson, J.E.; Swinney, D.D.</p> <p>2011-01-01</p> <p>Net changes in thickness and <span class="hlt">volume</span> of glacial <span class="hlt">ice</span> and perennial snow at Mount Rainier, Washington State, have been mapped over the entire edifice by differencing between a highresolution LiDAR (light detection and ranging) topographic survey of September-October 2007/2008 and the 10 m lateral resolution U.S. Geological Survey digital elevation model derived from September 1970 aerial photography. Excepting the large Emmons and Winthrop Glaciers, all of Mount Rainier's glaciers thinned and retreated in their terminal regions, with substantial thinning mainly at elevations <2000 m and the greatest thinning on southfacing glaciers. Mount Rainier's glaciers and snowfields also lost <span class="hlt">volume</span> over the interval, excepting the east-flank Fryingpan and Emmons Glaciers and minor near-summit snowfields; maximum <span class="hlt">volume</span> losses were centered from ~1750 m (north flank) to ~2250 m (south fl ank) elevation. The greatest single <span class="hlt">volume</span> loss was from the Carbon Glacier, despite its northward aspect, due to its sizeable area at <2000 m elevation. Overall, Mount Rainier lost ~14 vol% glacial <span class="hlt">ice</span> and perennial snow over the 37 to 38 yr interval between surveys. Enhanced thinning of south-flank glaciers may be meltback from the high snowfall period of the mid-1940s to mid-1970s associated with the cool phase of the Pacific Decadal Oscillation.</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> <span class="hlt">volume</span>, the mass 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://adsabs.harvard.edu/abs/2018TCry...12.1681P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1681P"><span><span class="hlt">Variability</span> of sea salts in <span class="hlt">ice</span> and firn cores from Fimbul <span class="hlt">Ice</span> Shelf, Dronning Maud Land, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paulina Vega, Carmen; Isaksson, Elisabeth; Schlosser, Elisabeth; Divine, Dmitry; Martma, Tõnu; Mulvaney, Robert; Eichler, Anja; Schwikowski-Gigar, Margit</p> <p>2018-05-01</p> <p>Major ions were analysed in firn and <span class="hlt">ice</span> cores located at Fimbul <span class="hlt">Ice</span> Shelf (FIS), Dronning Maud Land - DML, Antarctica. FIS is the largest <span class="hlt">ice</span> shelf in the Haakon VII Sea, with an extent of approximately 36 500 km2. Three shallow firn cores (about 20 m deep) were retrieved in different <span class="hlt">ice</span> rises, Kupol Ciolkovskogo (KC), Kupol Moskovskij (KM), and Blåskimen Island (BI), while a 100 m long core (S100) was drilled near the FIS edge. These sites are distributed over the entire FIS area so that they provide a variety of elevation (50-400 m a.s.l.) and distance (3-42 km) to the sea. Sea-salt species (mainly Na+ and Cl-) generally dominate the precipitation chemistry in the study region. We associate a significant sixfold increase in median sea-salt concentrations, observed in the S100 core after the 1950s, to an enhanced exposure of the S100 site to primary sea-salt aerosol due to a shorter distance from the S100 site to the <span class="hlt">ice</span> front, and to enhanced sea-salt aerosol production from blowing salty snow over sea <span class="hlt">ice</span>, most likely related to the calving of Trolltunga occurred during the 1960s. This increase in sea-salt concentrations is synchronous with a shift in non-sea-salt sulfate (nssSO42-) toward negative values, suggesting a possible contribution of fractionated aerosol to the sea-salt load in the S100 core most likely originating from salty snow found on sea <span class="hlt">ice</span>. In contrast, there is no evidence of a significant contribution of fractionated sea salt to the <span class="hlt">ice</span>-rises sites, where the signal would be most likely masked by the large inputs of biogenic sulfate estimated for these sites. In summary, these results suggest that the S100 core contains a sea-salt record dominated by the proximity of the site to the ocean, and processes of sea <span class="hlt">ice</span> formation in the neighbouring waters. In contrast, the <span class="hlt">ice</span>-rises firn cores register a larger-scale signal of atmospheric flow conditions and a less efficient transport of sea-salt aerosols to these sites. These findings are a</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870007787&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmarginal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870007787&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmarginal"><span>Microwave properties of sea <span class="hlt">ice</span> in the marginal <span class="hlt">ice</span> zone</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Onstott, R. G.; Larson, R. W.</p> <p>1986-01-01</p> <p>Active microwave properties of summer sea <span class="hlt">ice</span> were measured. Backscatter data were acquired at frequencies from 1 to 17 GHz, at angles from 0 to 70 deg from vertical, and with like and cross antenna polarizations. Results show that melt-water, snow thickness, snowpack morphology, snow surface roughness, <span class="hlt">ice</span> surface roughness, and deformation characteristics are the fundamental scene parameters which govern the summer sea <span class="hlt">ice</span> backscatter response. A thick, wet snow cover dominates the backscatter response and masks any <span class="hlt">ice</span> sheet features below. However, snow and melt-water are not distributed uniformly and the stage of melt may also be quite <span class="hlt">variable</span>. These nonuniformities related to <span class="hlt">ice</span> type are not necessarily well understood and produce unique microwave signature characteristics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28561343','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28561343"><span>Pan-Arctic sea <span class="hlt">ice</span>-algal chl a biomass and suitable habitat are largely underestimated for multiyear <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lange, Benjamin A; Flores, Hauke; Michel, Christine; Beckers, Justin F; Bublitz, Anne; Casey, John Alec; Castellani, Giulia; Hatam, Ido; Reppchen, Anke; Rudolph, Svenja A; Haas, Christian</p> <p>2017-11-01</p> <p>There is mounting evidence that multiyear <span class="hlt">ice</span> (MYI) is a unique component of the Arctic Ocean and may play a more important ecological role than previously assumed. This study improves our understanding of the potential of MYI as a suitable habitat for sea <span class="hlt">ice</span> algae on a pan-Arctic scale. We sampled sea <span class="hlt">ice</span> cores from MYI and first-year sea <span class="hlt">ice</span> (FYI) within the Lincoln Sea during four consecutive spring seasons. This included four MYI hummocks with a mean chl a biomass of 2.0 mg/m 2 , a value significantly higher than FYI and MYI refrozen ponds. Our results support the hypothesis that MYI hummocks can host substantial <span class="hlt">ice</span>-algal biomass and represent a reliable <span class="hlt">ice</span>-algal habitat due to the (quasi-) permanent low-snow surface of these features. We identified an <span class="hlt">ice</span>-algal habitat threshold value for calculated light transmittance of 0.014%. <span class="hlt">Ice</span> classes and coverage of suitable <span class="hlt">ice</span>-algal habitat were determined from snow and <span class="hlt">ice</span> surveys. These <span class="hlt">ice</span> classes and associated coverage of suitable habitat were applied to pan-Arctic CryoSat-2 snow and <span class="hlt">ice</span> thickness data products. This habitat classification accounted for the <span class="hlt">variability</span> of the snow and <span class="hlt">ice</span> properties and showed an areal coverage of suitable <span class="hlt">ice</span>-algal habitat within the MYI-covered region of 0.54 million km 2 (8.5% of total <span class="hlt">ice</span> area). This is 27 times greater than the areal coverage of 0.02 million km 2 (0.3% of total <span class="hlt">ice</span> area) determined using the conventional block-model classification, which assigns single-parameter values to each grid cell and does not account for subgrid cell <span class="hlt">variability</span>. This emphasizes the importance of accounting for <span class="hlt">variable</span> snow and <span class="hlt">ice</span> conditions in all sea <span class="hlt">ice</span> studies. Furthermore, our results indicate the loss of MYI will also mean the loss of reliable <span class="hlt">ice</span>-algal habitat during spring when food is sparse and many organisms depend on <span class="hlt">ice</span>-algae. © 2017 The Authors. Global Change Biology Published by John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRF..122.2488C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRF..122.2488C"><span>Seasonal <span class="hlt">Variability</span> in Regional <span class="hlt">Ice</span> Flow Due to Meltwater Injection Into the Shear Margins of Jakobshavn Isbræ</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cavanagh, J. P.; Lampkin, D. J.; Moon, T.</p> <p>2017-12-01</p> <p>The impact of meltwater injection into the shear margins of Jakobshavn Isbræ via drainage from water-filled crevasses on <span class="hlt">ice</span> flow is examined. We use Landsat-8 Operational Land Imager panchromatic, high-resolution imagery to monitor the spatiotemporal <span class="hlt">variability</span> of seven water-filled crevasse ponds during the summers of 2013 to 2015. The timing of drainage from water-filled crevasses coincides with an increase of 2 to 20% in measured <span class="hlt">ice</span> velocity beyond Jakobshavn Isbræ shear margins, which we define as extramarginal <span class="hlt">ice</span> velocity. Some water-filled crevasse groups demonstrate multiple drainage events within a single melt season. Numerical simulations show that hydrologic shear weakening due to water-filled crevasse drainage can accelerate extramarginal flow by as much as 35% within 10 km of the margins and enhance mass flux through the shear margins by 12%. This work demonstrates a novel mechanism through which surface melt can influence regional <span class="hlt">ice</span> flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1210105-unstable-amoc-during-glacial-intervals-millennial-variability-role-mean-sea-ice-extent','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1210105-unstable-amoc-during-glacial-intervals-millennial-variability-role-mean-sea-ice-extent"><span>Unstable AMOC during glacial intervals and millennial <span class="hlt">variability</span>: The role of mean sea <span class="hlt">ice</span> extent</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>Sevellec, Florian; Fedorov, Alexey V.</p> <p></p> <p>A striking feature of paleoclimate records is the greater stability of the Holocene epoch relative to the preceding glacial interval, especially apparent in the North Atlantic region. In particular, strong irregular <span class="hlt">variability</span> with an approximately 1500 yr period, known as the Dansgaard-Oeschger (D-O) events, punctuates the last glaciation, but is absent during the interglacial. Prevailing theories, modeling and data suggest that these events, seen as abrupt warming episodes in Greenland <span class="hlt">ice</span> cores and sea surface temperature records in the North Atlantic, are linked to reorganizations of the Atlantic Meridional Overturning Circulation (AMOC). In this study, using a new low-order oceanmore » model that reproduces a realistic power spectrum of millennial <span class="hlt">variability</span>, we explore differences in the AMOC stability between glacial and interglacial intervals of the 100 kyr glacial cycle of the Late Pleistocene (1 kyr = 1000 yr). Previous modeling studies show that the edge of sea <span class="hlt">ice</span> in the North Atlantic shifts southward during glacial intervals, moving the region of the North Atlantic Deep Water formation and the AMOC also southward. Finally, here we demonstrate that, by shifting the AMOC with respect to the mean atmospheric precipitation field, such a displacement makes the system unstable, which explains chaotic millennial <span class="hlt">variability</span> during the glacials and the persistence of stable ocean conditions during the interglacials.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1210105-unstable-amoc-during-glacial-intervals-millennial-variability-role-mean-sea-ice-extent','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1210105-unstable-amoc-during-glacial-intervals-millennial-variability-role-mean-sea-ice-extent"><span>Unstable AMOC during glacial intervals and millennial <span class="hlt">variability</span>: The role of mean sea <span class="hlt">ice</span> extent</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Sevellec, Florian; Fedorov, Alexey V.</p> <p>2015-11-01</p> <p>A striking feature of paleoclimate records is the greater stability of the Holocene epoch relative to the preceding glacial interval, especially apparent in the North Atlantic region. In particular, strong irregular <span class="hlt">variability</span> with an approximately 1500 yr period, known as the Dansgaard-Oeschger (D-O) events, punctuates the last glaciation, but is absent during the interglacial. Prevailing theories, modeling and data suggest that these events, seen as abrupt warming episodes in Greenland <span class="hlt">ice</span> cores and sea surface temperature records in the North Atlantic, are linked to reorganizations of the Atlantic Meridional Overturning Circulation (AMOC). In this study, using a new low-order oceanmore » model that reproduces a realistic power spectrum of millennial <span class="hlt">variability</span>, we explore differences in the AMOC stability between glacial and interglacial intervals of the 100 kyr glacial cycle of the Late Pleistocene (1 kyr = 1000 yr). Previous modeling studies show that the edge of sea <span class="hlt">ice</span> in the North Atlantic shifts southward during glacial intervals, moving the region of the North Atlantic Deep Water formation and the AMOC also southward. Finally, here we demonstrate that, by shifting the AMOC with respect to the mean atmospheric precipitation field, such a displacement makes the system unstable, which explains chaotic millennial <span class="hlt">variability</span> during the glacials and the persistence of stable ocean conditions during the interglacials.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMED33B..03E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMED33B..03E"><span>Indigenous Knowledge and Sea <span class="hlt">Ice</span> Science: What Can We Learn from Indigenous <span class="hlt">Ice</span> Users?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eicken, H.</p> <p>2010-12-01</p> <p>Drawing on examples mostly from Iñupiaq and Yup’ik sea-<span class="hlt">ice</span> expertise in coastal Alaska, this contribution examines how local, indigenous knowledge (LIK) can inform and guide geophysical and biological sea-<span class="hlt">ice</span> research. Part of the relevance of LIK derives from its linkage to sea-<span class="hlt">ice</span> use and the services coastal communities derive from the <span class="hlt">ice</span> cover. As a result, indigenous experts keep track of a broad range of sea-<span class="hlt">ice</span> <span class="hlt">variables</span> at a particular location. These observations are embedded into a broader worldview that speaks to both long-term <span class="hlt">variability</span> or change and to the system of values associated with <span class="hlt">ice</span> use. The contribution examines eight different contexts in which LIK in study site selection and assessment of a sampling campaign in the context of inter annual <span class="hlt">variability</span>, the identification of rare or inconspicuous phenomena or events, the contribution by indigenous experts to hazard assessment and emergency response, the record of past and present climate embedded in LIK, and the value of holistic sea-<span class="hlt">ice</span> knowledge in detecting subtle, intertwined patterns of environmental change. The relevance of local, indigenous sea-<span class="hlt">ice</span> expertise in helping advance adaptation and responses to climate change as well as its potential role in guiding research questions and hypotheses are also examined. The challenges that may have to be overcome in creating an interface for exchange between indigenous experts and seaice researchers are considered. Promising approaches to overcome these challenges include cross-cultural, interdisciplinary education, and the fostering of Communities of Practice.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C31A..03A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C31A..03A"><span>Interactions Between <span class="hlt">Ice</span> Thickness, Bottom <span class="hlt">Ice</span> Algae, and Transmitted Spectral Irradiance in the Chukchi Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arntsen, A. E.; Perovich, D. K.; Polashenski, C.; Stwertka, C.</p> <p>2015-12-01</p> <p>The amount of light that penetrates the Arctic sea <span class="hlt">ice</span> cover impacts sea-<span class="hlt">ice</span> mass balance as well as ecological processes in the upper ocean. The seasonally evolving macro and micro spatial <span class="hlt">variability</span> of transmitted spectral irradiance observed in the Chukchi Sea from May 18 to June 17, 2014 can be primarily attributed to variations in snow depth, <span class="hlt">ice</span> thickness, and bottom <span class="hlt">ice</span> algae concentrations. This study characterizes the interactions among these dominant <span class="hlt">variables</span> using observed optical properties at each sampling site. We employ a normalized difference index to compute estimates of Chlorophyll a concentrations and analyze the increased attenuation of incident irradiance due to absorption by biomass. On a kilometer spatial scale, the presence of bottom <span class="hlt">ice</span> algae reduced the maximum transmitted irradiance by about 1.5 orders of magnitude when comparing floes of similar snow and <span class="hlt">ice</span> thicknesses. On a meter spatial scale, the combined effects of disparities in the depth and distribution of the overlying snow cover along with algae concentrations caused maximum transmittances to vary between 0.0577 and 0.282 at a single site. Temporal <span class="hlt">variability</span> was also observed as the average integrated transmitted photosynthetically active radiation increased by one order of magnitude to 3.4% for the last eight measurement days compared to the first nine. Results provide insight on how interrelated physical and ecological parameters of sea <span class="hlt">ice</span> in varying time and space may impact new trends in Arctic sea <span class="hlt">ice</span> extent and the progression of melt.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1346837','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1346837"><span>A New Discrete Element Sea-<span class="hlt">Ice</span> Model for Earth System Modeling</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Turner, Adrian Keith</p> <p></p> <p>Sea <span class="hlt">ice</span> forms a frozen crust of sea water oating in high-latitude oceans. It is a critical component of the Earth system because its formation helps to drive the global thermohaline circulation, and its seasonal waxing and waning in the high north and Southern Ocean signi cantly affects planetary albedo. Usually 4{6% of Earth's marine surface is covered by sea <span class="hlt">ice</span> at any one time, which limits the exchange of heat, momentum, and mass between the atmosphere and ocean in the polar realms. Snow accumulates on sea <span class="hlt">ice</span> and inhibits its vertical growth, increases its albedo, and contributes to pooledmore » water in melt ponds that darken the Arctic <span class="hlt">ice</span> surface in the spring. <span class="hlt">Ice</span> extent and <span class="hlt">volume</span> are subject to strong seasonal, inter-annual and hemispheric variations, and climatic trends, which Earth System Models (ESMs) are challenged to simulate accurately (Stroeve et al., 2012; Stocker et al., 2013). This is because there are strong coupled feedbacks across the atmosphere-<span class="hlt">ice</span>-ocean boundary layers, including the <span class="hlt">ice</span>-albedo feedback, whereby a reduced <span class="hlt">ice</span> cover leads to increased upper ocean heating, further enhancing sea-<span class="hlt">ice</span> melt and reducing incident solar radiation re ected back into the atmosphere (Perovich et al., 2008). A reduction in perennial Arctic sea-<span class="hlt">ice</span> during the satellite era has been implicated in mid-latitude weather changes, including over North America (Overland et al., 2015). Meanwhile, most ESMs have been unable to simulate observed inter-annual <span class="hlt">variability</span> and trends in Antarctic sea-<span class="hlt">ice</span> extent during the same period (Gagne et al., 2014).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C12B..06B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C12B..06B"><span>North Atlantic Oscillation Drives Regional Greenland Glacier <span class="hlt">Volume</span> During the 20th Century</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bjork, A. A.; Aagaard, S.; Hallander, A. M.; Khan, S. A.; Box, J. E.; Kjeldsen, K. K.; Larsen, N. K.; Korsgaard, N. J.; Cappelen, J.; Colgan, W. T.; Machguth, H.; Andresen, C. S.; Kjaer, K. H.</p> <p>2016-12-01</p> <p>While most areas of the Greenland <span class="hlt">ice</span> sheet have undergone rapid mass loss since c. 1990, the central eastern section of the <span class="hlt">ice</span> sheet has advanced and gained mass. This contrasting regional trend has been attributed to positive surface mass balance (SMB) in the absence of significant dynamic mass loss. To constrain the atypical behavior in this region, we mapped glacier length fluctuations of nearly 200 peripheral glaciers and <span class="hlt">ice</span> caps (PGICs) over a 103-year period, and compare the results with c. 150 new glacier length records from central west Greenland. We demonstrate that the regional response in <span class="hlt">ice</span> <span class="hlt">volume</span> is closely correlated to changes in precipitation, governed by circulation patterns associated with the North Atlantic Oscillation (NAO) and secondarily influenced by temperature forcing in certain periods. More broadly, we find that the NAO contributes to contrasting precipitation <span class="hlt">variability</span> in East and West Greenland, where it appears to be responsible for at least 10% and more than 25%, respectively, of the <span class="hlt">variability</span> in <span class="hlt">ice</span> sheet accumulation rate. This east-west asymmetry, which influences both LGICs and the <span class="hlt">ice</span> sheet, illustrates how substantial uncertainty in NAO projections directly contributes to uncertainty in mass balance projections.</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> mass and mixed layer properties. The results for the climatological seasonal cycle are discussed first and include the salt and heat balance in the upper ocean. The coupled model is then applied to the period 1880-1985, using the surface air temperature fluctuations from Hansen et al. (1983) and from Wigley et al. (1981). The analysis of the simulated large variations of the Arctic <span class="hlt">ice</span> mass during this period (with similar changes in the mixed layer salinity) shows that the <span class="hlt">variability</span> in the summer melt determines to a high degree the <span class="hlt">variability</span> 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> mass is minimal for the range of atmospheric <span class="hlt">variability</span> tested.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.9151B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.9151B"><span>A sensitivity analysis for a thermomechanical model of the Antarctic <span class="hlt">ice</span> sheet and <span class="hlt">ice</span> shelves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baratelli, F.; Castellani, G.; Vassena, C.; Giudici, M.</p> <p>2012-04-01</p> <p>The outcomes of an <span class="hlt">ice</span> sheet model depend on a number of parameters and physical quantities which are often estimated with large uncertainty, because of lack of sufficient experimental measurements in such remote environments. Therefore, the efforts to improve the accuracy of the predictions of <span class="hlt">ice</span> sheet models by including more physical processes and interactions with atmosphere, hydrosphere and lithosphere can be affected by the inaccuracy of the fundamental input data. A sensitivity analysis can help to understand which are the input data that most affect the different predictions of the model. In this context, a finite difference thermomechanical <span class="hlt">ice</span> sheet model based on the Shallow-<span class="hlt">Ice</span> Approximation (SIA) and on the Shallow-Shelf Approximation (SSA) has been developed and applied for the simulation of the evolution of the Antarctic <span class="hlt">ice</span> sheet and <span class="hlt">ice</span> shelves for the last 200 000 years. The sensitivity analysis of the model outcomes (e.g., the <span class="hlt">volume</span> of the <span class="hlt">ice</span> sheet and of the <span class="hlt">ice</span> shelves, the basal melt rate of the <span class="hlt">ice</span> sheet, the mean velocity of the Ross and Ronne-Filchner <span class="hlt">ice</span> shelves, the wet area at the base of the <span class="hlt">ice</span> sheet) with respect to the model parameters (e.g., the basal sliding coefficient, the geothermal heat flux, the present-day surface accumulation and temperature, the mean <span class="hlt">ice</span> shelves viscosity, the melt rate at the base of the <span class="hlt">ice</span> shelves) has been performed by computing three synthetic numerical indices: two local sensitivity indices and a global sensitivity index. Local sensitivity indices imply a linearization of the model and neglect both non-linear and joint effects of the parameters. The global variance-based sensitivity index, instead, takes into account the complete <span class="hlt">variability</span> of the input parameters but is usually conducted with a Monte Carlo approach which is computationally very demanding for non-linear complex models. Therefore, the global sensitivity index has been computed using a development of the model outputs in a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DyAtO..79...10S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DyAtO..79...10S"><span>Sensitivity of open-water <span class="hlt">ice</span> growth and <span class="hlt">ice</span> concentration evolution in a coupled atmosphere-ocean-sea <span class="hlt">ice</span> model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, Xiaoxu; Lohmann, Gerrit</p> <p>2017-09-01</p> <p>A coupled atmosphere-ocean-sea <span class="hlt">ice</span> model is applied to investigate to what degree the area-thickness distribution of new <span class="hlt">ice</span> formed in open water affects the <span class="hlt">ice</span> and ocean properties. Two sensitivity experiments are performed which modify the horizontal-to-vertical aspect ratio of open-water <span class="hlt">ice</span> growth. The resulting changes in the Arctic sea-<span class="hlt">ice</span> concentration strongly affect the surface albedo, the ocean heat release to the atmosphere, and the sea-<span class="hlt">ice</span> production. The changes are further amplified through a positive feedback mechanism among the Arctic sea <span class="hlt">ice</span>, the Atlantic Meridional Overturning Circulation (AMOC), and the surface air temperature in the Arctic, as the Fram Strait sea <span class="hlt">ice</span> import influences the freshwater budget in the North Atlantic Ocean. Anomalies in sea-<span class="hlt">ice</span> transport lead to changes in sea surface properties of the North Atlantic and the strength of AMOC. For the Southern Ocean, the most pronounced change is a warming along the Antarctic Circumpolar Current (ACC), owing to the interhemispheric bipolar seasaw linked to AMOC weakening. Another insight of this study lies on the improvement of our climate model. The ocean component FESOM is a newly developed ocean-sea <span class="hlt">ice</span> model with an unstructured mesh and multi-resolution. We find that the subpolar sea-<span class="hlt">ice</span> boundary in the Northern Hemisphere can be improved by tuning the process of open-water <span class="hlt">ice</span> growth, which strongly influences the sea <span class="hlt">ice</span> concentration in the marginal <span class="hlt">ice</span> zone, the North Atlantic circulation, salinity and Arctic sea <span class="hlt">ice</span> <span class="hlt">volume</span>. Since the distribution of new <span class="hlt">ice</span> on open water relies on many uncertain parameters and the knowledge of the detailed processes is currently too crude, it is a challenge to implement the processes realistically into models. Based on our sensitivity experiments, we conclude a pronounced uncertainty related to open-water sea <span class="hlt">ice</span> growth which could significantly affect the climate system sensitivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.5058G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.5058G"><span>Frozen waterfall (or <span class="hlt">ice</span> cascade) growth and decay: a thermodynamic approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gauthier, Francis; Montagnat, Maurine; Weiss, Jérôme; Allard, Michel; Hétu, Bernard</p> <p>2013-04-01</p> <p>The <span class="hlt">ice</span> <span class="hlt">volume</span> evolution of an <span class="hlt">ice</span> cascade was studied using a thermodynamic model. The model was developed from meteorological data collected in the vicinity of the waterfall and validated from <span class="hlt">ice</span> <span class="hlt">volume</span> measurements estimated from terrestrial LiDAR images. The <span class="hlt">ice</span> cascade forms over a 45 m high rockwall located in northern Gaspésie, Québec, Canada. Two stages of formation were identified. During the first stage, the growth is mainly controlled by air convection around the flowing and freefalling water. The <span class="hlt">ice</span> cascade growth rate increases with the decreasing air temperature below 0°C and when the water flow reaches its lowest level. During the second stage, the <span class="hlt">ice</span> cascade covers the entire rockwall surface, water flow is isolated from the outside environment and <span class="hlt">ice</span> <span class="hlt">volume</span> increases asymptotically. Heat is evacuated from the water flow through the <span class="hlt">ice</span> cover by conduction. The growth is mainly controlled by the radiation energy balance but more specifically by the longwave radiation emitted at the <span class="hlt">ice</span> surface during the night. In spring, melting of the <span class="hlt">ice</span> cascade is clearly dependant on the sensible heat carried by the increasing water flow and the diffuse solar radiation received at the <span class="hlt">ice</span> surface during the day.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCry....8.2293A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCry....8.2293A"><span>Assessing spatio-temporal <span class="hlt">variability</span> and trends in modelled and measured Greenland <span class="hlt">Ice</span> Sheet albedo (2000-2013)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alexander, P. M.; Tedesco, M.; Fettweis, X.; van de Wal, R. S. W.; Smeets, C. J. P. P.; van den Broeke, M. R.</p> <p>2014-12-01</p> <p>Accurate measurements and simulations of Greenland <span class="hlt">Ice</span> Sheet (GrIS) surface albedo are essential, given the role of surface albedo in modulating the amount of absorbed solar radiation and meltwater production. In this study, we assess the spatio-temporal <span class="hlt">variability</span> of GrIS albedo during June, July, and August (JJA) for the period 2000-2013. We use two remote sensing products derived from data collected by the Moderate Resolution Imaging Spectroradiometer (MODIS), as well as outputs from the Modèle Atmosphérique Régionale (MAR) regional climate model (RCM) and data from in situ automatic weather stations. Our results point to an overall consistency in spatio-temporal <span class="hlt">variability</span> between remote sensing and RCM albedo, but reveal a difference in mean albedo of up to ~0.08 between the two remote sensing products north of 70° N. At low elevations, albedo values simulated by the RCM are positively biased with respect to remote sensing products by up to ~0.1 and exhibit low <span class="hlt">variability</span> compared with observations. We infer that these differences are the result of a positive bias in simulated bare <span class="hlt">ice</span> albedo. MODIS albedo, RCM outputs, and in situ observations consistently indicate a decrease in albedo of -0.03 to -0.06 per decade over the period 2003-2013 for the GrIS ablation area. Nevertheless, satellite products show a decline in JJA albedo of -0.03 to -0.04 per decade for regions within the accumulation area that is not confirmed by either the model or in situ observations. These findings appear to contradict a previous study that found an agreement between in situ and MODIS trends for individual months. The results indicate a need for further evaluation of high elevation albedo trends, a reconciliation of MODIS mean albedo at high latitudes, and the importance of accurately simulating bare <span class="hlt">ice</span> albedo in RCMs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C53C..03D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C53C..03D"><span>A Decade of High-Resolution Arctic Sea <span class="hlt">Ice</span> Measurements from Airborne Altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Duncan, K.; Farrell, S. L.; Connor, L. N.; Jackson, C.; Richter-Menge, J.</p> <p>2017-12-01</p> <p>Satellite altimeters carried on board ERS-1,-2, EnviSat, ICESat, CryoSat-2, AltiKa and Sentinel-3 have transformed our ability to map the thickness and <span class="hlt">volume</span> of the polar sea <span class="hlt">ice</span> cover, on seasonal and decadal time-scales. The era of polar satellite altimetry has coincided with a rapid decline of the Arctic <span class="hlt">ice</span> cover, which has thinned, and transitioned from a predominantly multi-year to first-year <span class="hlt">ice</span> cover. In conjunction with basin-scale satellite altimeter observations, airborne surveys of the Arctic Ocean at the end of winter are now routine. These surveys have been targeted to monitor regions of rapid change, and are designed to obtain the full snow and <span class="hlt">ice</span> thickness distribution, across a range of <span class="hlt">ice</span> types. Sensors routinely deployed as part of NASA's Operation <span class="hlt">Ice</span>Bridge (OIB) campaigns include the Airborne Topographic Mapper (ATM) laser altimeter, the frequency-modulated continuous-wave snow radar, and the Digital Mapping System (DMS). Airborne measurements yield high-resolution data products and thus present a unique opportunity to assess the quality and characteristics of the satellite observations. We present a suite of sea <span class="hlt">ice</span> data products that describe the snow depth and thickness of the Arctic <span class="hlt">ice</span> cover during the last decade. Fields were derived from OIB measurements collected between 2009-2017, and from reprocessed data collected during ad-hoc sea <span class="hlt">ice</span> campaigns prior to OIB. Our bespoke algorithms are designed to accommodate the heterogeneous sea <span class="hlt">ice</span> surface topography, that varies at short spatial scales. We assess regional and inter-annual <span class="hlt">variability</span> in the sea <span class="hlt">ice</span> thickness distribution. Results are compared to satellite-derived <span class="hlt">ice</span> thickness fields to highlight the sensitivities of satellite footprints to the tails of the thickness distribution. We also show changes in the dynamic forcing shaping the <span class="hlt">ice</span> pack over the last eight years through an analysis of pressure-ridge sail-height distributions and surface roughness conditions</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 <span class="hlt">variability</span> 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 <span class="hlt">variability</span> 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 mass 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://www.dtic.mil/docs/citations/ADA238039','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA238039"><span>Aircraft <span class="hlt">Icing</span> Handbook. <span class="hlt">Volume</span> 1</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1991-03-01</p> <p>Maryland - . . . Kohiman Aviation, Lawrence , Kansas Ohio State University, Columbus, Ohio .I --- t-r 1-- - -t I.Q,,- t ../e . Pratt and Whitney...lower; about six percent at -22 ’F (-30 *C). 1.2.3 Variations with Season The summer or warm season months create large warm air masses which can...on Aircraft Surfaces," NASA TM 87184, May 1986. 2-54 Hausman , R.J. and Turnock, S.R., "Investigation of Surface Water Behavior During Glaze <span class="hlt">Ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C43B0760A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C43B0760A"><span>Do Atmospheric Circulation Patterns Explain <span class="hlt">Variability</span> and Trends in The Seasonality of Oulu-Hailuoto <span class="hlt">Ice</span> Road in Northern Finland?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ahmadi, B.; Kiani, S.; Irannezhad, M.; Ronkanen, A. K.; Kløve, B.; Moradkhani, H.</p> <p>2016-12-01</p> <p>In cold climate regions, <span class="hlt">ice</span> roads are engineered as temporary winter transportation routes on the frozen seas, lakes and rivers. The <span class="hlt">ice</span> road season parameters (start, end and length) are principally dependent on the thickness of <span class="hlt">ice</span>, which is naturally controlled by temperature in terms of freezing (FDDs) and thawing (TDDs) degree-days. It has been shown that the variations in FDDs and TDDs are influenced by large-scale atmospheric circulation patterns (ACPs). Therefore, this study aims at understanding the role of ACPs in <span class="hlt">variability</span> and trends in the seasonality of Oulu-Hailuoto <span class="hlt">ice</span> road in northern Finland during 1974-2009. The Mann-Kendall nonparametric trend test determined significant shortening in the length of <span class="hlt">ice</span> road season over the study period of 1974-2009, which can be attributed to later start and earlier end days. In the study area, the maximum <span class="hlt">ice</span> thickness of the Baltic Sea also showed significant declines over time. Such sea <span class="hlt">ice</span> thinning can be associated with the wintertime temperature warming manifested by the decreasing trend found in the cumulative FDD during October-January in the water year (September-August). The increased cumulative TDD during February-April also reflects warmer climate in spring, which has resulted in the earlier end day of the <span class="hlt">ice</span> road season. Measuring the Spearman's rank correlation identified the Arctic Oscillation as the most significant ACP influencing variations in the cumulative FDD, and accordingly in the <span class="hlt">ice</span> thickness and the start day. However, the cumulative TDD during February-April shows significant positive correlation with the East Atlantic (EA) pattern, which appears to control the end day of the Oulu-Hailuoto <span class="hlt">ice</span> road season.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhDT.......110D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhDT.......110D"><span>Alaska shorefast <span class="hlt">ice</span>: Interfacing geophysics with local sea <span class="hlt">ice</span> knowledge and use</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Druckenmiller, Matthew L.</p> <p></p> <p> north of Alaska. This research further illustrates how Barrow's whaling community copes with year-to-year <span class="hlt">variability</span> and significant intra-seasonal changes in <span class="hlt">ice</span> conditions. Hence, arctic communities that have coped with such short-term <span class="hlt">variability</span> may be more adaptive to future environmental change than communities located in less dynamic environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.1821W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.1821W"><span>Satellite microwave observations of the interannual <span class="hlt">variability</span> of snowmelt on sea <span class="hlt">ice</span> in the Southern Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Willmes, S.; Haas, C.; Nicolaus, M.; Bareiss, J.</p> <p>2009-04-01</p> <p>Snowmelt processes on Antarctic sea <span class="hlt">ice</span> are examined. We present a simple snowmelt indicator based on diurnal brightness temperature variations from microwave satellite data. The method is validated through extensive field data from the western Weddell Sea and lends itself to the investigation of interannual and spatial variations of the typical snowmelt on Antarctic sea <span class="hlt">ice</span>. We use in situ measurements of physical snow properties to show that despite the absence of strong melting, the summer period is distinct from all other seasons with enhanced diurnal variations of snow wetness. A microwave emission model reveals that repeated thawing and refreezing causes the typical microwave emissivity signatures that are found on perennial Antarctic sea <span class="hlt">ice</span> during summer. The proposed melt indicator accounts for the characteristic phenomenological stages of snowmelt in the Southern Ocean and detects the onset of diurnal snow wetting. An algorithm is presented to map large-scale snowmelt onset, based on satellite data from the period between 1988 and 2006. The results indicate strong meridional gradients of snowmelt onset with the Weddell, Amundsen and Ross Seas showing earliest (beginning of October) and most frequent snowmelt. Moreover, a distinct interannual <span class="hlt">variability</span> of melt onset dates and large areas of first-year <span class="hlt">ice</span> where no diurnal freeze-thawing occurs at the surface are determined.</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/2009JGRC..114.3006W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JGRC..114.3006W"><span>Satellite microwave observations of the interannual <span class="hlt">variability</span> of snowmelt on sea <span class="hlt">ice</span> in the Southern Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Willmes, Sascha; Haas, Christian; Nicolaus, Marcel; Bareiss, JöRg</p> <p>2009-03-01</p> <p>Snowmelt processes on Antarctic sea <span class="hlt">ice</span> are examined. We present a simple snowmelt indicator based on diurnal brightness temperature variations from microwave satellite data. The method is validated through extensive field data from the western Weddell Sea and lends itself to the investigation of interannual and spatial variations of the typical snowmelt on Antarctic sea <span class="hlt">ice</span>. We use in-situ measurements of physical snow properties to show that despite the absence of strong melting, the summer period is distinct from all other seasons with enhanced diurnal variations of snow wetness. A microwave emission model reveals that repeated thawing and refreezing cause the typical microwave emissivity signatures that are found on perennial Antarctic sea <span class="hlt">ice</span> during summer. The proposed melt indicator accounts for the characteristic phenomenological stages of snowmelt in the Southern Ocean and detects the onset of diurnal snow wetting. An algorithm is presented to map large-scale snowmelt onset based on satellite data from the period between 1988 and 2006. The results indicate strong meridional gradients of snowmelt onset with the Weddell, Amundsen, and Ross Seas showing earliest (beginning of October) and most frequent snowmelt. Moreover, a distinct interannual <span class="hlt">variability</span> of melt onset dates and large areas of first-year <span class="hlt">ice</span> where no diurnal freeze thawing occurs at the surface are determined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.igsoc.org/annals/8/','USGSPUBS'); return false;" href="https://www.igsoc.org/annals/8/"><span>Glacier <span class="hlt">volume</span> estimation of Cascade Volcanoes—an analysis and comparison with other methods</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Driedger, Carolyn L.; Kennard, P.M.</p> <p>1986-01-01</p> <p>During the 1980 eruption of Mount St. Helens, the occurrence of floods and mudflows made apparent a need to assess mudflow hazards on other Cascade volcanoes. A basic requirement for such analysis is information about the <span class="hlt">volume</span> and distribution of snow and <span class="hlt">ice</span> on these volcanoes. An analysis was made of the <span class="hlt">volume</span>-estimation methods developed by previous authors and a <span class="hlt">volume</span> estimation method was developed for use in the Cascade Range. A radio echo-sounder, carried in a backpack, was used to make point measurements of <span class="hlt">ice</span> thickness on major glaciers of four Cascade volcanoes (Mount Rainier, Washington; Mount Hood and the Three Sisters, Oregon; and Mount Shasta, California). These data were used to generate <span class="hlt">ice</span>-thickness maps and bedrock topographic maps for developing and testing <span class="hlt">volume</span>-estimation methods. Subsequently, the methods were applied to the unmeasured glaciers on those mountains and, as a test of the geographical extent of applicability, to glaciers beyond the Cascades having measured <span class="hlt">volumes</span>. Two empirical relationships were required in order to predict <span class="hlt">volumes</span> for all the glaciers. Generally, for glaciers less than 2.6 km in length, <span class="hlt">volume</span> was found to be estimated best by using glacier area, raised to a power. For longer glaciers, <span class="hlt">volume</span> was found to be estimated best by using a power law relationship, including slope and shear stress. The necessary <span class="hlt">variables</span> can be estimated from topographic maps and aerial photographs.</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> mass and heat across the MIZ can reach O(200 m2 s-1). Submesoscale ocean <span class="hlt">variability</span> 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://hdl.handle.net/2060/20050179461','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050179461"><span>Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.; Cavalieri, Donald J.</p> <p>2005-01-01</p> <p>Sea <span class="hlt">ice</span> covers vast areas of the polar oceans, with <span class="hlt">ice</span> extent in the Northern Hemisphere ranging from approximately 7 x 10(exp 6) sq km in September to approximately 15 x 10(exp 6) sq km in March and <span class="hlt">ice</span> extent in the Southern Hemisphere ranging from approximately 3 x 10(exp 6) sq km in February to approximately 18 x 10(exp 6) sq km in September. These <span class="hlt">ice</span> covers have major impacts on the atmosphere, oceans, and ecosystems of the polar regions, and so as changes occur in them there are potential widespread consequences. Satellite data reveal considerable interannual <span class="hlt">variability</span> in both polar sea <span class="hlt">ice</span> covers, and many studies suggest possible connections between the <span class="hlt">ice</span> and various oscillations within the climate system, such as the Arctic Oscillation, North Atlantic Oscillation, and Antarctic Oscillation, or Southern Annular Mode. Nonetheless, statistically significant long-term trends are also apparent, including overall trends of decreased <span class="hlt">ice</span> coverage in the Arctic and increased <span class="hlt">ice</span> coverage in the Antarctic from late 1978 through the end of 2003, with the Antarctic <span class="hlt">ice</span> increases following marked decreases in the Antarctic <span class="hlt">ice</span> during the 1970s. For a detailed picture of the seasonally varying <span class="hlt">ice</span> cover at the start of the 21st century, this chapter includes <span class="hlt">ice</span> concentration maps for each month of 2001 for both the Arctic and the Antarctic, as well as an overview of what the satellite record has revealed about the two polar <span class="hlt">ice</span> covers from the 1970s through 2003.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA536479','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA536479"><span>Understanding the Importance of Oceanic Forcing on Sea <span class="hlt">Ice</span> <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-12-01</p> <p>problem, which includes <span class="hlt">ice</span> thickness. Thorndike et al. (1975) recognized that many of the physical properties of sea <span class="hlt">ice</span> depend upon its thickness...IMB2005B are presented below. In agreement with previous studies (e.g., Thorndike and Colony 1982), they show that during the winter months (December...During the Past 100 Years, 33, 2, 143– 154. 148 Thorndike , A.S., and R. Colony, 1982: Sea <span class="hlt">ice</span> motion in response to geostrophic winds. Journal of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601293','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601293"><span>Coupling of Waves, Turbulence and Thermodynamics Across the Marginal <span class="hlt">Ice</span> Zone</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-30</p> <p><span class="hlt">ice</span> . The albedo of sea <span class="hlt">ice</span> is large compared to open water, and most of the incoming solar radiation...ocean and the <span class="hlt">ice</span> pack where the seasonal retreat of the main <span class="hlt">ice</span> pack takes place. It is a highly <span class="hlt">variable</span> sea <span class="hlt">ice</span> environment, usually comprised of...many individual floes of <span class="hlt">variable</span> shape and size and made of mixed <span class="hlt">ice</span> types, from young forming <span class="hlt">ice</span> to fragmented multiyear <span class="hlt">ice</span> . The presence of sea</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49..775T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49..775T"><span>Arctic sea <span class="hlt">ice</span> in the global eddy-permitting ocean reanalysis ORAP5</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tietsche, Steffen; Balmaseda, Magdalena A.; Zuo, Hao; Mogensen, Kristian</p> <p>2017-08-01</p> <p>We discuss the state of Arctic sea <span class="hlt">ice</span> in the global eddy-permitting ocean reanalysis Ocean ReAnalysis Pilot 5 (ORAP5). Among other innovations, ORAP5 now assimilates observations of sea <span class="hlt">ice</span> concentration using a univariate 3DVar-FGAT scheme. We focus on the period 1993-2012 and emphasize the evaluation of model performance with respect to recent observations of sea <span class="hlt">ice</span> thickness. We find that sea <span class="hlt">ice</span> concentration in ORAP5 is close to assimilated observations, with root mean square analysis residuals of less than 5 % in most regions. However, larger discrepancies exist for the Labrador Sea and east of Greenland during winter owing to biases in the free-running model. Sea <span class="hlt">ice</span> thickness is evaluated against three different observational data sets that have sufficient spatial and temporal coverage: ICESat, <span class="hlt">Ice</span>Bridge and SMOSIce. Large-scale features like the gradient between the thickest <span class="hlt">ice</span> in the Canadian Arctic and thinner <span class="hlt">ice</span> in the Siberian Arctic are simulated well by ORAP5. However, some biases remain. Of special note is the model's tendency to accumulate too thick <span class="hlt">ice</span> in the Beaufort Gyre. The root mean square error of ORAP5 sea <span class="hlt">ice</span> thickness with respect to ICESat observations is 1.0 m, which is on par with the well-established PIOMAS model sea <span class="hlt">ice</span> reconstruction. Interannual <span class="hlt">variability</span> and trend of sea <span class="hlt">ice</span> <span class="hlt">volume</span> in ORAP5 also compare well with PIOMAS and ICESat estimates. We conclude that, notwithstanding a relatively simple sea <span class="hlt">ice</span> data assimilation scheme, the overall state of Arctic sea <span class="hlt">ice</span> in ORAP5 is in good agreement with observations and will provide useful initial conditions for predictions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014P%26SS...91...60F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014P%26SS...91...60F"><span>Amazonian mid- to high-latitude glaciation on Mars: Supply-limited <span class="hlt">ice</span> sources, <span class="hlt">ice</span> accumulation patterns, and concentric crater fill glacial flow and <span class="hlt">ice</span> sequestration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fastook, James L.; Head, James W.</p> <p>2014-02-01</p> <p>Concentric crater fill (CCF) occurs in the interior of impact craters in mid- to high latitudes on Mars and is interpreted to have formed by glacial <span class="hlt">ice</span> flow and debris covering. We use the characteristics and orientation of deposits comprising CCF, the thickness of pedestal deposits in mid- to high-latitude pedestal craters (Pd), the <span class="hlt">volumes</span> of the current polar caps, and information about regional slopes and <span class="hlt">ice</span> rheology to address questions about (1) the maximum thickness of regional <span class="hlt">ice</span> deposits during the Late Amazonian, (2) the likelihood that these deposits flowed regionally, (3) the geological regions and features most likely to induce <span class="hlt">ice</span>-flow, and (4) the locations and environments in which <span class="hlt">ice</span> is likely to have been sequestered up to the present. We find that regional <span class="hlt">ice</span> flow under Late Amazonian climate conditions requires <span class="hlt">ice</span> thicknesses exceeding many hundreds of meters for slopes typical of the vast majority of the surface of Mars, a thickness for the mid-latitudes that is well in excess of the total <span class="hlt">volume</span> available from polar <span class="hlt">ice</span> reservoirs. This indicates that although conditions for mid- to high-latitude glaciation may have persisted for tens to hundreds of millions of years, the process is “supply limited”, with a steady state reached when the polar <span class="hlt">ice</span> cap water <span class="hlt">ice</span> supply becomes exhausted. Impact craters are by far the most abundant landform with associated slopes (interior wall and exterior rim) sufficiently high to induce glacial <span class="hlt">ice</span> flow under Late Amazonian climate conditions, and topographic slope data show that Amazonian impact craters have been clearly modified, undergoing crater interior slope reduction and floor shallowing. We show that these trends are the predictable response of <span class="hlt">ice</span> deposition and preferential accumulation and retention in mid- to high-latitude crater interiors during episodes of enhanced spin-axis obliquity. We demonstrate that flow from a single episode of an inter-crater terrain layer comparable to Pedestal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910017259','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910017259"><span>West Antarctic <span class="hlt">Ice</span> Sheet Initiative. <span class="hlt">Volume</span> 2: Discipline Reviews</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bindschadler, Robert A. (Editor)</p> <p>1991-01-01</p> <p>Seven discipline review papers are presented on the state of the knowledge of West Antarctica and opinions on how that knowledge must be increased to predict the future behavior of this <span class="hlt">ice</span> sheet and to assess its potential to collapse, rapidly raising the global sea level. These are the goals of the West Antarctic <span class="hlt">Ice</span> Sheet Initiative (WAIS).</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 <span class="hlt">volume</span> 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 mass balance. Basal melt of 1325 ± 235 gigatons per year (Gt/year) exceeds a calving flux of 1089 ± 139 Gt/year, making <span class="hlt">ice</span>-shelf melting the largest ablation process in Antarctica. The giant cold-cavity Ross, Filchner, and Ronne <span class="hlt">ice</span> shelves covering two-thirds of the total <span class="hlt">ice</span>-shelf area account for only 15% of net melting. Half of the meltwater comes from 10 small, warm-cavity Southeast Pacific <span class="hlt">ice</span> shelves occupying 8% of the area. A similar high melt/area ratio is found for six East Antarctic <span class="hlt">ice</span> shelves, implying undocumented strong ocean thermal forcing on their deep grounding lines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28765493','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28765493"><span><span class="hlt">Variability</span> of Tidal <span class="hlt">Volume</span> in Patient-Triggered Mechanical Ventilation in ARDS.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Perinel-Ragey, Sophie; Baboi, Loredana; Guérin, Claude</p> <p>2017-11-01</p> <p>Limiting tidal <span class="hlt">volume</span> (V T ) in patients with ARDS may not be achieved once patient-triggered breaths occur. Furthermore, ICU ventilators offer numerous patient-triggered modes that work differently across brands. We systematically investigated, using a bench model, the effect of patient-triggered modes on the size and <span class="hlt">variability</span> of V T at different breathing frequencies (f), patient effort, and ARDS severity. We used a V500 Infinity ICU ventilator connected to an ASL 5000 lung model whose compliance was mimicking mild, moderate, and severe ARDS. Thirteen patient-triggered modes were tested, falling into 3 categories, namely <span class="hlt">volume</span> control ventilation with mandatory minute ventilation; pressure control ventilation, including airway pressure release ventilation (APRV); and pressure support ventilation. Two levels of f and effort were tested for each ARDS severity in each mode. Median (first-third quartiles) V T was compared across modes using non-parametric tests. The probability of V T > 6 mL/kg ideal body weight was assessed by binomial regression and expressed as the odds ratio (OR) with 95% CI. V T <span class="hlt">variability</span> was measured from the coefficient of variation. V T distribution over all f, effort, and ARDS categories significantly differed across modes ( P < .001, Kruskal-Wallis test). V T was significantly greater with pressure support (OR 420 mL, 95% CI 332-527 mL) than with any other mode except for <span class="hlt">variable</span> pressure support level. Risk for V T to be > 6 mL/kg was significantly increased with spontaneous breaths patient-triggered by pressure support (OR 19.36, 95% CI 12.37-30.65) and significantly reduced in APRV (OR 0.44, 95% CI 0.26-0.72) and pressure support with guaranteed <span class="hlt">volume</span> mode. The risk increased with increasing effort and decreasing f. Coefficient of variation of V T was greater for low f and <span class="hlt">volume</span> control-mandatory minute ventilation and pressure control modes. APRV had the greatest within-mode <span class="hlt">variability</span>. Risk of V T > 6 mL/kg was significantly</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4987822','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4987822"><span>Stochastic <span class="hlt">ice</span> stream dynamics</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bertagni, Matteo Bernard; Ridolfi, Luca</p> <p>2016-01-01</p> <p><span class="hlt">Ice</span> streams are narrow corridors of fast-flowing <span class="hlt">ice</span> that constitute the arterial drainage network of <span class="hlt">ice</span> sheets. Therefore, changes in <span class="hlt">ice</span> stream flow are key to understanding paleoclimate, sea level changes, and rapid disintegration of <span class="hlt">ice</span> sheets during deglaciation. The dynamics of <span class="hlt">ice</span> flow are tightly coupled to the climate system through atmospheric temperature and snow recharge, which are known exhibit stochastic <span class="hlt">variability</span>. Here we focus on the interplay between stochastic climate forcing and <span class="hlt">ice</span> stream temporal dynamics. Our work demonstrates that realistic climate fluctuations are able to (i) induce the coexistence of dynamic behaviors that would be incompatible in a purely deterministic system and (ii) drive <span class="hlt">ice</span> stream flow away from the regime expected in a steady climate. We conclude that environmental noise appears to be crucial to interpreting the past behavior of <span class="hlt">ice</span> sheets, as well as to predicting their future evolution. PMID:27457960</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24936905','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24936905"><span>A simple video-based timing system for on-<span class="hlt">ice</span> team testing in <span class="hlt">ice</span> hockey: a technical report.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Larson, David P; Noonan, Benjamin C</p> <p>2014-09-01</p> <p>The purpose of this study was to describe and evaluate a newly developed on-<span class="hlt">ice</span> timing system for team evaluation in the sport of <span class="hlt">ice</span> hockey. We hypothesized that this new, simple, inexpensive, timing system would prove to be highly accurate and reliable. Six adult subjects (age 30.4 ± 6.2 years) performed on <span class="hlt">ice</span> tests of acceleration and conditioning. The performance times of the subjects were recorded using a handheld stopwatch, photocell, and high-speed (240 frames per second) video. These results were then compared to allow for accuracy calculations of the stopwatch and video as compared with filtered photocell timing that was used as the "gold standard." Accuracy was evaluated using maximal differences, typical error/coefficient of variation (CV), and intraclass correlation coefficients (ICCs) between the timing methods. The reliability of the video method was evaluated using the same <span class="hlt">variables</span> in a test-retest analysis both within and between evaluators. The video timing method proved to be both highly accurate (ICC: 0.96-0.99 and CV: 0.1-0.6% as compared with the photocell method) and reliable (ICC and CV within and between evaluators: 0.99 and 0.08%, respectively). This video-based timing method provides a very rapid means of collecting a high <span class="hlt">volume</span> of very accurate and reliable on-<span class="hlt">ice</span> measures of skating speed and conditioning, and can easily be adapted to other testing surfaces and parameters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830045130&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmarginal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830045130&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmarginal"><span>A coupled <span class="hlt">ice</span>-ocean model of upwelling in the marginal <span class="hlt">ice</span> zone</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roed, L. P.; Obrien, J. J.</p> <p>1983-01-01</p> <p>A dynamical coupled <span class="hlt">ice</span>-ocean numerical model for the marginal <span class="hlt">ice</span> zone (MIZ) is suggested and used to study upwelling dynamics in the MIZ. The nonlinear sea <span class="hlt">ice</span> model has a <span class="hlt">variable</span> <span class="hlt">ice</span> concentration and includes internal <span class="hlt">ice</span> stress. The model is forced by stresses on the air/ocean and air/<span class="hlt">ice</span> surfaces. The main coupling between the <span class="hlt">ice</span> and the ocean is in the form of an interfacial stress on the <span class="hlt">ice</span>/ocean interface. The ocean model is a linear reduced gravity model. The wind stress exerted by the atmosphere on the ocean is proportional to the fraction of open water, while the interfacial stress <span class="hlt">ice</span>/ocean is proportional to the concentration of <span class="hlt">ice</span>. A new mechanism for <span class="hlt">ice</span> edge upwelling is suggested based on a geostrophic equilibrium solution for the sea <span class="hlt">ice</span> medium. The upwelling reported in previous models invoking a stationary <span class="hlt">ice</span> cover is shown to be replaced by a weak downwelling due to the <span class="hlt">ice</span> motion. Most of the upwelling dynamics can be understood by analysis of the divergence of the across <span class="hlt">ice</span> edge upper ocean transport. On the basis of numerical model, an analytical model is suggested that reproduces most of the upwelling dynamics of the more complex numerical model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030110723&hterms=BELT+CONVEYOR&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DBELT%2BCONVEYOR','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030110723&hterms=BELT+CONVEYOR&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DBELT%2BCONVEYOR"><span>The Broken Belt: Meteorite Concentrations on Stranded <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Harvey, R. P.</p> <p>2003-01-01</p> <p>Since the first Antarctic meteorite concentrations were discovered more than 25 years ago, many theories regarding the role of iceflow in the production of meteorite concentrations have been put forward, and most agree on the basic principles. These models suggest that as the East Antarctic icesheet flows toward the margins of the continent, meteorites randomly located within the <span class="hlt">volume</span> of <span class="hlt">ice</span> are transported toward the icesheet margin. Where mountains or subsurface obstructions block glacial flow, diversion of <span class="hlt">ice</span> around or over an obstruction reduces horizontal <span class="hlt">ice</span> movement rates adjacent to the barriers and creates a vertical (upward) component of movement. If local mechanisms for <span class="hlt">ice</span> loss (ablation) exist at such sites, an equilibrium surface will develop according to the balance between <span class="hlt">ice</span> supply and loss, and the cargo of meteorites is exhumed on a blue <span class="hlt">ice</span> surface. The result is a conceptual conveyor belt bringing meteorite-bearing <span class="hlt">volumes</span> of <span class="hlt">ice</span> from the interior of the continent to stagnant or slowmoving surfaces where <span class="hlt">ice</span> is then lost and a precious cargo is left as a lag deposit. Cassidy et al. provides an excellent overview of how this model has been adapted to several Antarctic stranding surfaces.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4782H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4782H"><span>Deglacial-Holocene short-term <span class="hlt">variability</span> in sea-<span class="hlt">ice</span> distribution on the Eurasian shelf (Arctic Ocean) - An IP25 biomarker reconstruction.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hörner, Tanja; Stein, Ruediger; Fahl, Kirsten</p> <p>2016-04-01</p> <p>Four well-dated sediment cores from the Eurasian continental shelf, i.e., the Kara Sea (Cores BP99/07 and BP00/07) and Laptev Sea (Cores PS51/154 and PS51/159), were selected for high-resolution reconstruction of past Arctic environmental conditions during the deglacial-Holocene time interval. These marginal seas are strongly affected by the post-glacial sea-level rise of about 120m. The major focus of our study was the reconstruction of the paleo-sea-<span class="hlt">ice</span> distribution as sea-<span class="hlt">ice</span> plays a key role within the modern and past climate system. For reconstruction of paleo-sea <span class="hlt">ice</span>, the sea-<span class="hlt">ice</span> proxy IP25 in combination with open-water phytoplankton biomarkers was used (for approach see Belt et al., 2007; Müller et al., 2009, 2011). In addition, specific sterols were determined to reconstruct changes in river run-off and biological production. The post-glacial sea-level rise is especially reflected in prominent decrease in terrigenous biomarkers. Deglacial variations in sea-<span class="hlt">ice</span> cover sustained for thousand of years, mostly following climatic changes like the Bølling/Allerød (14.7-12.9 ka), Younger Dryas (12.9-11.6 ka) and Holocene warm phase (10-8 ka). Superimposed on a (Late) Holocene cooling trend, short-term fluctuations in sea-<span class="hlt">ice</span> cover (on centennial scale) are distinctly documented in the distal/off-shore Core BP00/07 from the Kara Sea, less pronounced in the proximal/near-shore Core PS99/07 and in the Laptev Sea cores. Interestingly, this short-term <span class="hlt">variability</span> in sea-<span class="hlt">ice</span> cover correlates quite well to changes in Siberian river run-off (e.g., Stein et al. 2004), pointing to a direct linkage between precipitation (atmospheric circulation) and sea-<span class="hlt">ice</span> formation. References Belt, S.T., Massé, G., Rowland, S.J., Poulin, M., Michel, C., LeBlanc, B., 2007. A novel chemical fossil of palaeo sea <span class="hlt">ice</span>: IP25. Organic Geochemistry 38, 16-27. Müller, J., Masse, G., Stein, R., Belt, S.T., 2009. <span class="hlt">Variability</span> of sea-<span class="hlt">ice</span> conditions in the Fram Strait over the past 30,000 years</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050071088&hterms=sauber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsauber','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20050071088&hterms=sauber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsauber"><span>Southern Alaska Glaciers: Spatial and Temporal Variations in <span class="hlt">Ice</span> <span class="hlt">Volume</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sauber, J.; Molnia, B. F.; Lutchke, S.; Rowlands, D.; Harding, D.; Carabajal, C.; Hurtado, J. M.; Spade, G.</p> <p>2004-01-01</p> <p>Although temperate mountain glaciers comprise less than 1% of the glacier-covered area on Earth, they are important because they appear to be melting rapidly under present climatic conditions and, therefore, make significant contributions to rising sea level. In this study, we use ICESat observations made in the last 1.5 years of southern Alaska glaciers to estimate <span class="hlt">ice</span> elevation profiles, <span class="hlt">ice</span> surface slopes and roughness, and bi-annual and/or annual <span class="hlt">ice</span> elevation changes. We report initial results from the near coastal region between Yakutat Bay and Cape Suckling that includes the Malaspina and Bering Glaciers. We show and interpret <span class="hlt">ice</span> elevations changes across the lower reaches of the Bagley <span class="hlt">Ice</span> Valley for the period between October 2003 and May 2004. In addition, we use off-nadir pointing observations to reference tracks over the Bering and Malaspina Glaciers in order to estimate annual <span class="hlt">ice</span> elevation change. Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) and Shuttle Radar Topography Mission (SRTM) derived DEMs are used to estimate across track regional slopes between ICESat data acquisitions. Although the distribution and quantity of ICESat elevation profiles with multiple, exact repeat data is currently limited in Alaska, individual ICESat data tracks, provide an accurate reference surface for comparison to other elevation data (e.g. ASTER and SRTM X- and C-band derived DEMs). Specifically we report the elevation change over the Malaspina Glacier's piedmont lobe between a DEM derived from SRTM C-band data acquired in Feb. 2000 and ICESat Laser #2b data from Feb.-March 2004. We also report use of ICESat elevation data to enhance ASTER derived absolute DEMs. Mountain glaciers generally have rougher surfaces and steeper regional slopes than the <span class="hlt">ice</span> sheets for which the ICESat design was optimized. Therefore, rather than averaging ICESat observations over large regions or relying on crossovers, we are working with well-located ICESat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170003112&hterms=core&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcore','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170003112&hterms=core&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcore"><span>Holocene Accumulation and <span class="hlt">Ice</span> Flow near the West Antarctic <span class="hlt">Ice</span> Sheet Divide <span class="hlt">Ice</span> Core Site</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Koutnik, Michelle R.; Fudge, T.J.; Conway, Howard; Waddington, Edwin D.; Neumann, Thomas A.; Cuffey, Kurt M.; Buizert, Christo; Taylor, Kendrick C.</p> <p>2016-01-01</p> <p>The West Antarctic <span class="hlt">Ice</span> Sheet Divide Core (WDC) provided a high-resolution climate record from near the Ross-Amundsen Divide in Central West Antarctica. In addition, radar-detected internal layers in the vicinity of the WDC site have been dated directly from the <span class="hlt">ice</span> core to provide spatial variations in the age structure of the region. Using these two data sets together, we first infer a high-resolution Holocene accumulation-rate history from 9.2 thousand years of the <span class="hlt">ice</span>-core timescale and then confirm that this climate history is consistent with internal layers upstream of the core site. Even though the WDC was drilled only 24 kilometers from the modern <span class="hlt">ice</span> divide, advection of <span class="hlt">ice</span> from upstream must be taken into account. We evaluate histories of accumulation rate by using a flowband model to generate internal layers that we compare to observed layers. Results show that the centennially averaged accumulation rate was over 20 percent lower than modern at 9.2 thousand years before present (B.P.), increased by 40 percent from 9.2 to 2.3 thousand years B.P., and decreased by at least 10 percent over the past 2 thousand years B.P. to the modern values; these Holocene accumulation-rate changes in Central West Antarctica are larger than changes inferred from East Antarctic <span class="hlt">ice</span>-core records. Despite significant changes in accumulation rate, throughout the Holocene the regional accumulation pattern has likely remained similar to today, and the <span class="hlt">ice</span>-divide position has likely remained on average within 5 kilometers of its modern position. Continent-scale <span class="hlt">ice</span>-sheet models used for reconstructions of West Antarctic <span class="hlt">ice</span> <span class="hlt">volume</span> should incorporate this accumulation history.</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> mass and heat across the MIZ can reach O(200 m2 s-1). Submesoscale ocean <span class="hlt">variability</span> 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/2016AGUFM.C44B..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C44B..02G"><span>Global glacier and <span class="hlt">ice</span> sheet surface velocities derived from 31 years of Landsat imagery</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gardner, A. S.; Scambos, T. A.; Fahnestock, M. A.</p> <p>2016-12-01</p> <p>Glaciers and <span class="hlt">ice</span> sheets are contributing substantial <span class="hlt">volumes</span> of water to the world's oceans due to enhanced melt resulting from changes in ocean and atmospheric conditions and respective feedbacks. Improving understanding of the processes leading to accelerated rates of <span class="hlt">ice</span> loss is necessary for reducing uncertainties sea level projections. One key to doing this is to assemble and analyze long records of glacier change that characterize grounded <span class="hlt">ice</span> response to changes in driving stress, buttressing, and basal conditions. As part of the NASA funded GO_LIVE project we exploit 31 years of Landsat imagery to construct detailed time histories of global glacier velocities. Early exploration of the dataset reveals the diversity of information to be gleaned: sudden tidewater glacier speedups in the Antarctic Peninsula, rifting of Antarctic <span class="hlt">ice</span> shelves, high <span class="hlt">variability</span> in velocities near glacier grounding lines, frequent surge activity in the mountainous regions of Alaska and High Mountain Asia, and the slowdown of land-terminating valley glaciers in Arctic Canada and elsewhere.</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/2014AGUFM.C21B0326B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C21B0326B"><span>Antarctic <span class="hlt">Ice</span> Mass Balance 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>Boening, C.; Firing, Y. L.; Wiese, D. N.; Watkins, M. M.; Schlegel, N.; Larour, E. Y.</p> <p>2014-12-01</p> <p>The Antarctic <span class="hlt">ice</span> mass balance and rates of change of <span class="hlt">ice</span> 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 <span class="hlt">variability</span>, 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 <span class="hlt">ice</span> discharge rates based on radar-derived <span class="hlt">ice</span> velocities and thicknesses. GRACE also resolves accelerations in regional <span class="hlt">ice</span> mass change rates, including increasing rates of mass gain in East Antarctica and accelerating <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">variability</span> 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 <span class="hlt">ice</span> discharge rates. An <span class="hlt">Ice</span> 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 <span class="hlt">variability</span> in discharge, highlighting the potential importance of ocean forcing for setting <span class="hlt">ice</span> discharge rates at interannual to decadal time scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFMPP23C..05T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFMPP23C..05T"><span>1500 Years of Annual Climate and Environmental <span class="hlt">Variability</span> as Recorded in Bona-Churchill (Alaska) <span class="hlt">Ice</span> Cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thompson, L. G.; Mosley-Thompson, E. S.; Zagorodnov, V.; Davis, M. E.; Mashiotta, T. A.; Lin, P.</p> <p>2004-12-01</p> <p>In 2003, six <span class="hlt">ice</span> cores measuring 10.5, 11.5, 11.8, 12.4, 114 and 460 meters were recovered from the col between Mount Bona and Mount Churchill (61° 24'N; 141° 42'W; 4420 m asl). These cores have been analyzed for stable isotopic ratios, insoluble dust content and concentrations of major chemical species. Total Beta radioactivity was measured in the upper sections. The 460-meter core, extending to bedrock, captured the entire depositional record at this site where <span class="hlt">ice</span> temperatures ranged from -24° C at 10 meters to -19.8° C at the <span class="hlt">ice</span>/bedrock contact. The shallow cores allow assessment of surface processes under modern meteorological conditions while the deep core offers a ˜1500-year climate and environmental perspective. The average annual net balance is ˜~1000 mm of water equivalent and distinct annual signals in dust and calcium concentrations along with δ 18O allow annual resolution over most of the core. The excess sulfate record reflects many known large volcanic eruptions such as Katmai, Krakatau, Tambora, and Laki which allow validation of the time scale in the upper part of the core. The lower part of the core yields a history of earlier volcanic events. The 460-m Bona-Churchill <span class="hlt">ice</span> core provides a detailed history of the `Little <span class="hlt">Ice</span> Age' and medieval warm periods for southeastern Alaska. The source of the White River Ash will be discussed in light of the evidence from this core. The 460-m core also provides a long-term history of the dust fall that originates in north-central China. The annual <span class="hlt">ice</span> core-derived climate records from southeastern Alaska will facilitate an investigation of the likelihood that the high resolution 1500-year record from the tropical Quelccaya <span class="hlt">Ice</span> Cap (Peru) preserves a history of the <span class="hlt">variability</span> of both the PDO and the Aleutian Low.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080023287','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080023287"><span>Arctic Sea <span class="hlt">Ice</span> <span class="hlt">Variability</span> and Trends, 1979-2006</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.; Cavalieri, Donald J.</p> <p>2008-01-01</p> <p>Analysis of Arctic sea <span class="hlt">ice</span> extents derived from satellite passive-microwave data for the 28 years, 1979-2006 yields an overall negative trend of -45,100 +/- 4,600 km2/yr (-3.7 +/- 0.4%/decade) in the yearly averages, with negative <span class="hlt">ice</span>-extent trends also occurring for each of the four seasons and each of the 12 months. For the yearly averages the largest decreases occur in the Kara and Barents Seas and the Arctic Ocean, with linear least squares slopes of -10,600 +/- 2,800 km2/yr (-7.4 +/- 2.0%/decade) and -10,100 +/- 2,200 km2/yr (-1.5 +/- 0.3%/decade), respectively, followed by Baffin Bay/Labrador Sea, with a slope of -8,000 +/- 2,000 km2/yr) -9.0 +/- 2.3%/decade), the Greenland Sea, with a slope of -7,000 +/- 1,400 km2/yr (-9.3 +/- 1.9%/decade), and Hudson Bay, with a slope of -4,500 +/- 900 km2/yr (-5.3 +/- 1.1%/decade). These are all statistically significant decreases at a 99% confidence level. The Seas of Okhotsk and Japan also have a statistically significant <span class="hlt">ice</span> decrease, although at a 95% confidence level, and the three remaining regions, the Bering Sea, Canadian Archipelago, and Gulf of St. Lawrence, have negative slopes that are not statistically significant. The 28-year trends in <span class="hlt">ice</span> areas for the Northern Hemisphere total are also statistically significant and negative in each season, each month, and for the yearly averages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43D2472C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43D2472C"><span>Sensitivity of the sea <span class="hlt">ice</span> concentration over the Kara-Barents Sea in autumn to the winter temperature <span class="hlt">variability</span> over East Asia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cho, K. H.; Chang, E. C.</p> <p>2017-12-01</p> <p>In this study, we performed sensitivity experiments by utilizing the Global/Regional Integrated Model system with different conditions of the sea <span class="hlt">ice</span> concentration over the Kara-Barents (KB) Sea in autumn, which can affect winter temperature <span class="hlt">variability</span> over East Asia. Prescribed sea <span class="hlt">ice</span> conditions are 1) climatological autumn sea <span class="hlt">ice</span> concentration obtained from 1982 to 2016, 2) reduced autumn sea <span class="hlt">ice</span> concentration by 50% of the climatology, and 3) increased autumn sea <span class="hlt">ice</span> concentration by 50% of climatology. Differently prescribed sea <span class="hlt">ice</span> concentration changes surface albedo, which affects surface heat fluxes and near-surface air temperature. The reduced (increased) sea <span class="hlt">ice</span> concentration over the KB sea increases (decreases) near-surface air temperature that leads the lower (higher) sea level pressure in autumn. These patterns are maintained from autumn to winter season. Furthermore, it is shown that the different sea <span class="hlt">ice</span> concentration over the KB sea has remote effects on the sea level pressure patterns over the East Asian region. The lower (higher) sea level pressure over the KB sea by the locally decreased (increased) <span class="hlt">ice</span> concentration is related to the higher (lower) pressure pattern over the Siberian region, which induces strengthened (weakened) cold advection over the East Asian region. From these sensitivity experiments it is clarified that the decreased (increased) sea <span class="hlt">ice</span> concentration over the KB sea in autumn can lead the colder (warmer) surface air temperature over East Asia in winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PrOce.156...17L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PrOce.156...17L"><span>Under the sea <span class="hlt">ice</span>: Exploring the relationship between sea <span class="hlt">ice</span> and the foraging behaviour of southern elephant seals in East Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Labrousse, Sara; Sallée, Jean-Baptiste; Fraser, Alexander D.; Massom, Robert A.; Reid, Phillip; Sumner, Michael; Guinet, Christophe; Harcourt, Robert; McMahon, Clive; Bailleul, Frédéric; Hindell, Mark A.; Charrassin, Jean-Benoit</p> <p>2017-08-01</p> <p>Investigating ecological relationships between predators and their environment is essential to understand the response of marine ecosystems to climate <span class="hlt">variability</span> and change. This is particularly true in polar regions, where sea <span class="hlt">ice</span> (a sensitive climate <span class="hlt">variable</span>) plays a crucial yet highly dynamic and <span class="hlt">variable</span> role in how it influences the whole marine ecosystem, from phytoplankton to top predators. For mesopredators such as seals, sea <span class="hlt">ice</span> both supports a rich (under-<span class="hlt">ice</span>) food resource, access to which depends on local to regional coverage and conditions. Here, we investigate sex-specific relationships between the foraging strategies of southern elephant seals (Mirounga leonina) in winter and spatio-temporal <span class="hlt">variability</span> in sea <span class="hlt">ice</span> concentration (SIC) and coverage in East Antarctica. We satellite-tracked 46 individuals undertaking post-moult trips in winter from Kerguelen Islands to the peri-Antarctic shelf between 2004 and 2014. These data indicate distinct general patterns of sea <span class="hlt">ice</span> usage: while females tended to follow the sea <span class="hlt">ice</span> edge as it extended northward, the males remained on the continental shelf despite increasing sea <span class="hlt">ice</span>. Seal hunting time, a proxy of foraging activity inferred from the diving behaviour, was longer for females in late autumn in the outer part of the pack <span class="hlt">ice</span>, ∼150-370 km south of the <span class="hlt">ice</span> edge. Within persistent regions of compact sea <span class="hlt">ice</span>, females had a longer foraging activity (i) in the highest sea <span class="hlt">ice</span> concentration at their position, but (ii) their foraging activity was longer when there were more patches of low concentration sea <span class="hlt">ice</span> around their position (either in time or in space; 30 days & 50 km). The high spatio-temporal <span class="hlt">variability</span> of sea <span class="hlt">ice</span> around female positions is probably a key factor allowing them to exploit these concentrated patches. Despite lack of information on prey availability, females may exploit mesopelagic finfishes and squids that concentrate near the <span class="hlt">ice</span>-water interface or within the water column (from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010095442&hterms=Global+Warming+Climate+Change+Warning&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DGlobal%2BWarming%2BClimate%2BChange%2BWarning','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010095442&hterms=Global+Warming+Climate+Change+Warning&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DGlobal%2BWarming%2BClimate%2BChange%2BWarning"><span>Sea <span class="hlt">Ice</span> and <span class="hlt">Ice</span> Temperature <span class="hlt">Variability</span> as Observed by Microwave and Infrared Satellite Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comiso, Josefino C.; Koblinsky, Chester J. (Technical Monitor)</p> <p>2001-01-01</p> <p>Recent reports of a retreating and thinning sea <span class="hlt">ice</span> cover in the Arctic have pointed to a strong suggestion of significant warming in the polar regions. It is especially important to understand what these reports mean in light of the observed global warning and because the polar regions are expected to be most sensitive to changes in climate. To gain insight into this phenomenon, co-registered <span class="hlt">ice</span> concentrations and surface temperatures derived from two decades of satellite microwave and infrared data have been processed and analyzed. While observations from meteorological stations indicate consistent surface warming in both regions during the last fifty years, the last 20 years of the same data set show warming in the Arctic but a slight cooling in the Antarctic. These results are consistent with the retreat in the Arctic <span class="hlt">ice</span> cover and the advance in the Antarctic <span class="hlt">ice</span> cover as revealed by historical satellite passive microwave data. Surface temperatures derived from satellite infrared data are shown to be consistent within 3 K with surface temperature data from the limited number of stations. While not as accurate, the former provides spatially detailed changes over the twenty year period. In the Arctic, for example, much of the warming occurred in the Beaufort Sea and the North American region in 1998 while slight cooling actually happened in parts of the Laptev Sea and Northern Siberia during the same time period. Big warming anomalies are also observed during the last five years but a periodic cycle of about ten years is apparent suggesting a possible influence of the North Atlantic Oscillation. In the Antarctic, large interannual and seasonal changes are also observed in the circumpolar <span class="hlt">ice</span> cover with regional changes showing good coherence with surface temperature anomalies. However, a mode 3 is observed to be more dominant than the mode 2 wave reported in the literature. Some of these spatial and temporal changes appear to be influenced by the Antarctic</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 <span class="hlt">variable</span> 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 mass 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 mass 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 content using a novel algorithm that includes traveltime inversion and ray tracing with a prescribed shape of the depth-density relationship. For the particular case of an <span class="hlt">ice</span>-shelf channel, where <span class="hlt">ice</span> thickness and surface slope change substantially over a few kilometers, the radar data suggest that firn inside the channel is about 5 % denser than outside the channel. Although this density difference is at the detection limit of the radar, it is consistent with a similar density anomaly reconstructed from optical televiewing, which reveals that the firn inside the channel is 4.7 % denser than that outside the channel. Hydrostatic <span class="hlt">ice</span> thickness calculations used for determining basal melt rates should account for the denser firn in <span class="hlt">ice</span>-shelf channels. The radar method presented here is robust and can easily be adapted to different radar frequencies and data-acquisition geometries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080045469&hterms=conversion+rate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dconversion%2Brate%2527','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080045469&hterms=conversion+rate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dconversion%2Brate%2527"><span>Antarctic Sea <span class="hlt">Ice</span> Thickness and Snow-to-<span class="hlt">Ice</span> Conversion from Atmospheric Reanalysis and Passive Microwave Snow Depth</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Markus, Thorsten; Maksym, Ted</p> <p>2007-01-01</p> <p>Passive microwave snow depth, <span class="hlt">ice</span> concentration, and <span class="hlt">ice</span> motion estimates are combined with snowfall from the European Centre for Medium Range Weather Forecasting (ECMWF) reanalysis (ERA-40) from 1979-200 1 to estimate the prevalence of snow-to-<span class="hlt">ice</span> conversion (snow-<span class="hlt">ice</span> formation) on level sea <span class="hlt">ice</span> in the Antarctic for April-October. Snow <span class="hlt">ice</span> is ubiquitous in all regions throughout the growth season. Calculated snow- <span class="hlt">ice</span> thicknesses fall within the range of estimates from <span class="hlt">ice</span> core analysis for most regions. However, uncertainties in both this analysis and in situ data limit the usefulness of snow depth and snow-<span class="hlt">ice</span> production to evaluate the accuracy of ERA-40 snowfall. The East Antarctic is an exception, where calculated snow-<span class="hlt">ice</span> production exceeds observed <span class="hlt">ice</span> thickness over wide areas, suggesting that ERA-40 precipitation is too high there. Snow-<span class="hlt">ice</span> thickness <span class="hlt">variability</span> is strongly controlled not just by snow accumulation rates, but also by <span class="hlt">ice</span> divergence. Surprisingly, snow-<span class="hlt">ice</span> production is largely independent of snow depth, indicating that the latter may be a poor indicator of total snow accumulation. Using the presence of snow-<span class="hlt">ice</span> formation as a proxy indicator for near-zero freeboard, we examine the possibility of estimating level <span class="hlt">ice</span> thickness from satellite snow depths. A best estimate for the mean level <span class="hlt">ice</span> thickness in September is 53 cm, comparing well with 51 cm from ship-based observations. The error is estimated to be 10-20 cm, which is similar to the observed interannual and regional <span class="hlt">variability</span>. Nevertheless, this is comparable to expected errors for <span class="hlt">ice</span> thickness determined by satellite altimeters. Improvement in satellite snow depth retrievals would benefit both of these methods.</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 <span class="hlt">variabilities</span> of Antarctic <span class="hlt">ice</span> mass 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 mass change is thus essential in determining and predicting its contribution to sea level. While the <span class="hlt">ice</span> mass loss estimates for West Antarctica (WA) and the Antarctic Peninsula (AP) are in good agreement, what the mass balance over East Antarctica (EA) is, and whether or not it compensates for the mass loss is under debate. Besides the different error sources and sensitivities of different measurement types, complex spatial and temporal <span class="hlt">variabilities</span> would be another factor complicating the accurate estimation of the AIS mass balance. Therefore, a model that allows for <span class="hlt">variabilities</span> in both melting rate and seasonal signals would seem appropriate in the estimation of present-day AIS melting. We present a stochastic filter technique, which enables the Bayesian separation of the systematic stripe noise and mass signal in decade-length GRACE monthly gravity series, and allows the estimation of time-<span class="hlt">variable</span> 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 <span class="hlt">variabilities</span> of the AIS mass balance at basin scale, particularly over East Antarctica, and decipher the EA mass variations in the past decade, and their role in affecting overall AIS mass balance and sea level.</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 <span class="hlt">variability</span> within the Ross <span class="hlt">ice</span> streams of West Antarctica suggests that the present-day positive mass 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) mass balance within decades and a net loss of <span class="hlt">ice</span> within two centuries. This hitherto unaccounted for flow <span class="hlt">variability</span> 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('http://adsabs.harvard.edu/abs/2013AGUFM.C11C..05F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C11C..05F"><span>A Decade of Arctic Sea <span class="hlt">Ice</span> Thickness Change from Airborne and Satellite Altimetry (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farrell, S. L.; Richter-Menge, J.; Kurtz, N. T.; McAdoo, D. C.; Newman, T.; Zwally, H.; Ruth, J.</p> <p>2013-12-01</p> <p>Altimeters on both airborne and satellite platforms provide direct measurements of sea <span class="hlt">ice</span> freeboard from which sea <span class="hlt">ice</span> thickness may be calculated. Satellite altimetry observations of Arctic sea <span class="hlt">ice</span> from ICESat and CryoSat-2 indicate a significant decline in <span class="hlt">ice</span> thickness, and <span class="hlt">volume</span>, over the last decade. During this time the <span class="hlt">ice</span> pack has experienced a rapid change in its composition, transitioning from predominantly thick, multi-year <span class="hlt">ice</span> to thinner, increasingly seasonal <span class="hlt">ice</span>. We will discuss the regional trends in <span class="hlt">ice</span> thickness derived from ICESat and <span class="hlt">Ice</span>Bridge altimetry between 2003 and 2013, contrasting observations of the multi-year <span class="hlt">ice</span> pack with seasonal <span class="hlt">ice</span> zones. ICESat ceased operation in 2009, and the final, reprocessed data set became available recently. We extend our analysis to April 2013 using data from the <span class="hlt">Ice</span>Bridge airborne mission, which commenced operations in 2009. We describe our current efforts to more accurately convert from freeboard to <span class="hlt">ice</span> thickness, with a modified methodology that corrects for range errors, instrument biases, and includes an enhanced treatment of snow depth, with respect to <span class="hlt">ice</span> type. With the planned launch by NASA of ICESat-2 in 2016 we can expect continuity of the sea <span class="hlt">ice</span> thickness time series through the end of this decade. Data from the ICESat-2 mission, together with ongoing observations from CryoSat-2, will allow us to understand both the decadal trends and inter-annual <span class="hlt">variability</span> in the Arctic sea <span class="hlt">ice</span> thickness record. We briefly present the status of planned ICESat-2 sea <span class="hlt">ice</span> data products, and demonstrate the utility of micro-pulse, photon-counting laser altimetry over sea <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSME12B..03L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSME12B..03L"><span>Under the Sea <span class="hlt">Ice</span>: Exploration of the Relationships Between Sea <span class="hlt">Ice</span> Patterns and Foraging Movements of a Marine Predator in East Antarctica.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Labrousse, S.; Sallee, J. B.; Fraser, A. D.; Massom, R. A.; Reid, P.; Sumner, M.; Guinet, C.; Harcourt, R.; Bailleul, F.; Hindell, M.; Charrassin, J. B.</p> <p>2016-02-01</p> <p>Investigating ecological relationships between top predators and their environment is essential to understand the response of marine ecosystems to climate <span class="hlt">variability</span>. Specifically, <span class="hlt">variability</span> and changes in sea <span class="hlt">ice</span>, which is known as an important habitat for marine ecosystems, presents complex patterns in East Antarctic. The impact for ecosystems of such changes of their habitat is however still unknown. Acting as an ecological double-edged sword, sea <span class="hlt">ice</span> can impede access to marine resources while harboring a rich ecosystem during winter. Here, we investigated which type of sea <span class="hlt">ice</span> habitat is used by male and female southern elephant seals during winter and examine if and how the spatio-temporal <span class="hlt">variability</span> of sea <span class="hlt">ice</span> concentration (SIC) influence their foraging strategies. We also examined over a 10 years time-series the impact of SIC and sea <span class="hlt">ice</span> advance anomaly on foraging activity. To do this, we studied 46 individuals equipped with Satellite linked data recorders between 2004 and 2014, undertaking post-moult trips in winter from Kerguelen to the peri-Antarctic shelf. The general patterns of sea <span class="hlt">ice</span> use by males and females are clearly distinct; while females tended to follow the sea <span class="hlt">ice</span> edge as it extended northward, males remained on the continental shelf. Female foraging activity was higher in late autumn in the outer part of the pack <span class="hlt">ice</span> in concentrated SIC and spatially stable. They remained in areas of <span class="hlt">variable</span> SIC over time and low persistence. The seal hunting time, a proxy of foraging activity inferred from the diving behaviour, was much higher during earlier advance of sea <span class="hlt">ice</span> over female time-series. The females were possibly taking advantage of the <span class="hlt">ice</span> algal autumn bloom sustaining krill and an under <span class="hlt">ice</span> ecosystem without being trapped in sea <span class="hlt">ice</span>. Males foraging activity increased when they remained deep inside sea <span class="hlt">ice</span> over the shelf using <span class="hlt">variable</span> SIC in time and space, presumably in polynyas or flaw leads between fast and pack <span class="hlt">ice</span>. This strategy</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMMR13A1698A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMMR13A1698A"><span>The <span class="hlt">ice</span> VII-<span class="hlt">ice</span> X phase transition with implications for planetary interiors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aarestad, B.; Frank, M. R.; Scott, H.; Bricker, M.; Prakapenka, V.</p> <p>2008-12-01</p> <p>A significant amount of research on the high pressure polymorphs of H2O have detailed the lattice structure and density of these phases, namely <span class="hlt">ice</span> VI, <span class="hlt">ice</span> VII, and <span class="hlt">ice</span> X. These high pressure <span class="hlt">ices</span> are noteworthy as they may comprise a considerable part of the interior of large icy planets and satellites. However, there is a dearth of data on how the incorporation of an impurity, charged or non-charged, affects the <span class="hlt">ice</span> VII-<span class="hlt">ice</span> X transition. This study examined the <span class="hlt">ice</span> VII-<span class="hlt">ice</span> X transition that occurs at approximately 62 GPa with a pure system and two select impure systems. Solutions of pure H2O, 1.6 mole percent NaCl in H2O, and 1.60 mole percent CH3OH in H2O were compressed in a diamond anvil cell (DAC). The experiments were performed at the GSECARS 13-BM-D beam line at the Advanced Photon Source at Argonne National Laboratory. Powder diffraction data of the <span class="hlt">ice</span> samples were collected using monochromatic X-ray radiation, 0.2755 Å, and a MAR 345 online imaging system at intervals of approximately 2 GPa up to ~71.5, ~74.5, and ~68 GPa, respectively. Analyses of the data provided <span class="hlt">volume</span>-pressure relations (at 298 K) which were used to detail the <span class="hlt">ice</span> VII-<span class="hlt">ice</span> X phase transition. The pressure of the phase transition, based upon an interpretation of the X-ray diffraction data, was found to vary as a function of the impurity type. Thus, the depth of the <span class="hlt">ice</span> VII-<span class="hlt">ice</span> X phase transition within an <span class="hlt">ice</span>-rich planetary body can be influenced by trace-level impurities.</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 <span class="hlt">volume</span>, 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> masses 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://ntrs.nasa.gov/search.jsp?R=20170008473&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170008473&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsea"><span>Atmospheric Form Drag Coefficients Over Arctic Sea <span class="hlt">Ice</span> Using Remotely Sensed <span class="hlt">Ice</span> Topography Data, Spring 2009-2015</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Petty, Alek A.; Tsamados, Michel C.; Kurtz, Nathan T.</p> <p>2017-01-01</p> <p>Sea <span class="hlt">ice</span> topography significantly impacts turbulent energy/momentum exchange, e.g., atmospheric (wind) drag, over Arctic sea <span class="hlt">ice</span>. Unfortunately, observational estimates of this contribution to atmospheric drag <span class="hlt">variability</span> are spatially and temporally limited. Here we present new estimates of the neutral atmospheric form drag coefficient over Arctic sea <span class="hlt">ice</span> in early spring, using high-resolution Airborne Topographic Mapper elevation data from NASA's Operation <span class="hlt">Ice</span>Bridge mission. We utilize a new three-dimensional <span class="hlt">ice</span> topography data set and combine this with an existing parameterization scheme linking surface feature height and spacing to form drag. To be consistent with previous studies investigating form drag, we compare these results with those produced using a new linear profiling topography data set. The form drag coefficient from surface feature <span class="hlt">variability</span> shows lower values [less than 0.5-1 × 10(exp. -3)] in the Beaufort/Chukchi Seas, compared with higher values [greater than 0.5-1 ×10(exp. -3)] in the more deformed <span class="hlt">ice</span> regimes of the Central Arctic (north of Greenland and the Canadian Archipelago), which increase with coastline proximity. The results show moderate interannual <span class="hlt">variability</span>, including a strong increase in the form drag coefficient from 2013 to 2014/2015 north of the Canadian Archipelago. The form drag coefficient estimates are extrapolated across the Arctic with Advanced Scatterometer satellite radar backscatter data, further highlighting the regional/interannual drag coefficient <span class="hlt">variability</span>. Finally, we combine the results with existing parameterizations of form drag from floe edges (a function of <span class="hlt">ice</span> concentration) and skin drag to produce, to our knowledge, the first pan-Arctic estimates of the total neutral atmospheric drag coefficient (in early spring) from 2009 to 2015.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JaJAP..56eFB03W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JaJAP..56eFB03W"><span>Structural incorporation of MgCl2 into <span class="hlt">ice</span> VII at room temperature</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watanabe, Mao; Komatsu, Kazuki; Noritake, Fumiya; Kagi, Hiroyuki</p> <p>2017-05-01</p> <p>Raman spectra and X-ray diffraction patterns were obtained from 1:100 and 1:200 \\text{MgCl}2:\\text{H}2\\text{O} solutions (in molar ratio) at pressures up to 6 GPa using diamond anvil cells (DACs) and compared with those of pure water. The O-H stretching band from <span class="hlt">ice</span> VII crystallized from the 1:200 solution was approximately 10 cm-1 higher than that of pure <span class="hlt">ice</span> VII. The phase boundaries between <span class="hlt">ice</span> VII and VIII crystallized from the MgCl2 solutions at 4 GPa were 2 K lower than those of pure <span class="hlt">ice</span> VII and VIII. These observations indicate that <span class="hlt">ice</span> VII incorporates MgCl2 into its structure. The unit cell <span class="hlt">volumes</span> of <span class="hlt">ice</span> VII crystallized from pure water and the two solutions coincided with each other within the experimental error, and salt incorporation was not detectable from the cell <span class="hlt">volume</span>. Possible configurations of ion substitution and excess <span class="hlt">volume</span> of <span class="hlt">ice</span> VIII were simulated on the basis of density functional theory (DFT) calculations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036603','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036603"><span>Integration of MODIS-derived metrics to assess interannual <span class="hlt">variability</span> in snowpack, lake <span class="hlt">ice</span>, and NDVI in southwest Alaska</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Reed, Bradley C.; Budde, Michael E.; Spencer, Page; Miller, Amy E.</p> <p>2009-01-01</p> <p>Impacts of global climate change are expected to result in greater variation in the seasonality of snowpack, lake <span class="hlt">ice</span>, and vegetation dynamics in southwest Alaska. All have wide-reaching physical and biological ecosystem effects in the region. We used Moderate Resolution Imaging Spectroradiometer (MODIS) calibrated radiance, snow cover extent, and vegetation index products for interpreting interannual variation in the duration and extent of snowpack, lake <span class="hlt">ice</span>, and vegetation dynamics for southwest Alaska. The approach integrates multiple seasonal metrics across large ecological regions. Throughout the observation period (2001-2007), snow cover duration was stable within ecoregions, with <span class="hlt">variable</span> start and end dates. The start of the lake <span class="hlt">ice</span> season lagged the snow season by 2 to 3??months. Within a given lake, freeze-up dates varied in timing and duration, while break-up dates were more consistent. Vegetation phenology varied less than snow and <span class="hlt">ice</span> metrics, with start-of-season dates comparatively consistent across years. The start of growing season and snow melt were related to one another as they are both temperature dependent. Higher than average temperatures during the El Ni??o winter of 2002-2003 were expressed in anomalous <span class="hlt">ice</span> and snow season patterns. We are developing a consistent, MODIS-based dataset that will be used to monitor temporal trends of each of these seasonal metrics and to map areas of change for the study area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1610105F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1610105F"><span><span class="hlt">Variability</span> of IN measured with the Fast <span class="hlt">Ice</span> Nucleus Chamber (FINCH) at the high altitude research station Jungfraujoch during wintertime 2013</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frank, Fabian; Nillius, Björn; Bundke, Ulrich; Curtius, Joachim</p> <p>2014-05-01</p> <p><span class="hlt">Ice</span> nuclei (IN) are an important component of the atmospheric aerosol. Despite their low concentrations in the atmosphere, they have an influence on the formation of <span class="hlt">ice</span> crystals in mixed-phase clouds and therefore on precipitation. The Fast <span class="hlt">Ice</span> Nucleus CHamber (FINCH)1, a counter for <span class="hlt">ice</span> nucleating particles developed at the Goethe University Frankfurt am Main allows long-term measurements of the IN number concentration. In FINCH the <span class="hlt">ice</span> activation of the aerosol particles is achieved by mixing air flows with different temperature and humidity. The IN number concentration measurements at different meteorological conditions during the INUIT-JFJ campaign at the high altitude research station Jungfraujoch in Switzerland are presented and its <span class="hlt">variability</span> are discussed. The good operational performance of the instrument allowed up to 10 hours of continuous measurements. Acknowledgment: This work was supported by the German Research Foundation, DFG Grant: BU 1432/3-2 BU 1432/4-1 in the framework of INUIT (FOR 1525) and SPP 1294 HALO. 1- Bundke, U., Nillius, B., Jaenicke, R., Wetter, T., Klein, H., and Bingemer, H. (2008). The fast <span class="hlt">ice</span> nucleus chamber finch. Atmospheric Research, 90:180-186.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140011509','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011509"><span>Quantifying the Amount of <span class="hlt">Ice</span> in Cold Tropical Cirrus Clouds</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Avery, Melody A.; Winker, David M.; Garnier, Anne; Lawson, R. Paul; Heymsfield, Andrew J.; Mo, Qixu; Schoeberl, Mark R.; Woods, Sarah; Lance, Sara; Young, Stuart A.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20140011509'); toggleEditAbsImage('author_20140011509_show'); toggleEditAbsImage('author_20140011509_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20140011509_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20140011509_hide"></p> <p>2014-01-01</p> <p>How much <span class="hlt">ice</span> is there in the Tropical Tropopause layer, globally? How does one begin to answer that question? Clouds are currently the largest source of uncertainty in climate models, and the <span class="hlt">ice</span> water content (IWC) of cold cirrus clouds is needed to understand the total water and radiation budgets of the upper troposphere and lower stratosphere (UT/LS). The Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO) satellite, originally a "pathfinder" mission only expected to last for three years, has now been operational for more than eight years. Lidar data from CALIPSO can provide information about how IWC is vertically distributed in the UT/LS, and about inter-annual <span class="hlt">variability</span> and seasonal changes in cloud <span class="hlt">ice</span>. However, cloud IWC is difficult to measure accurately with either remote or in situ instruments because IWC from cold cirrus clouds is derived from the particle cross-sectional area or visible extinction coefficient. Assumptions must be made about the relationship between the area, <span class="hlt">volume</span> and density of <span class="hlt">ice</span> particles with various crystal habits. Recently there have been numerous aircraft field campaigns providing detailed information about cirrus <span class="hlt">ice</span> water content from cloud probes. This presentation evaluates the assumptions made when creating the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) global IWC data set, using recently reanalyzed aircraft particle probe measurements of very cold, thin TTL cirrus from the 2006 CR-AVE.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950023826','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950023826"><span>Sea <span class="hlt">ice</span> motions in the Central Arctic pack <span class="hlt">ice</span> as inferred from AVHRR imagery</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Emery, William; Maslanik, James; Fowler, Charles</p> <p>1995-01-01</p> <p>Synoptic observations of <span class="hlt">ice</span> motion in the Arctic Basin are currently limited to those acquired by drifting buoys and, more recently, radar data from ERS-1. Buoys are not uniformly distributed throughout the Arctic, and SAR coverage is currently limited regionally and temporally due to the data <span class="hlt">volume</span>, swath width, processing requirements, and power needs of the SAR. Additional <span class="hlt">ice</span>-motion observations that can map <span class="hlt">ice</span> responses simultaneously over large portions of the Arctic on daily to weekly time intervals are thus needed to augment the SAR and buoys data and to provide an intermediate-scale measure of <span class="hlt">ice</span> drift suitable for climatological analyses and <span class="hlt">ice</span> modeling. Principal objectives of this project were to: (1) demonstrate whether sufficient <span class="hlt">ice</span> features and <span class="hlt">ice</span> motion existed within the consolidated <span class="hlt">ice</span> pack to permit motion tracking using AVHRR imagery; (2) determine the limits imposed on AVHRR mapping by cloud cover; and (3) test the applicability of AVHRR-derived motions in studies of <span class="hlt">ice</span>-atmosphere interactions. Each of these main objectives was addressed. We conclude that AVHRR data, particularly when blended with other available observations, provide a valuable data set for studying sea <span class="hlt">ice</span> processes. In a follow-on project, we are now extending this work to cover larger areas and to address science questions in more detail.</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://adsabs.harvard.edu/abs/2018TCry...12.1233H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1233H"><span>Thermodynamic and dynamic <span class="hlt">ice</span> thickness contributions in the Canadian Arctic Archipelago in NEMO-LIM2 numerical simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hu, Xianmin; Sun, Jingfan; Chan, Ting On; Myers, Paul G.</p> <p>2018-04-01</p> <p>Sea <span class="hlt">ice</span> thickness evolution within the Canadian Arctic Archipelago (CAA) is of great interest to science, as well as local communities and their economy. In this study, based on the NEMO numerical framework including the LIM2 sea <span class="hlt">ice</span> module, simulations at both 1/4 and 1/12° horizontal resolution were conducted from 2002 to 2016. The model captures well the general spatial distribution of <span class="hlt">ice</span> thickness in the CAA region, with very thick sea <span class="hlt">ice</span> (˜ 4 m and thicker) in the northern CAA, thick sea <span class="hlt">ice</span> (2.5 to 3 m) in the west-central Parry Channel and M'Clintock Channel, and thin ( < 2 m) <span class="hlt">ice</span> (in winter months) on the east side of CAA (e.g., eastern Parry Channel, Baffin Island coast) and in the channels in southern areas. Even though the configurations still have resolution limitations in resolving the exact observation sites, simulated <span class="hlt">ice</span> thickness compares reasonably (seasonal cycle and amplitudes) with weekly Environment and Climate Change Canada (ECCC) New <span class="hlt">Ice</span> Thickness Program data at first-year landfast <span class="hlt">ice</span> sites except at the northern sites with high concentration of old <span class="hlt">ice</span>. At 1/4 to 1/12° scale, model resolution does not play a significant role in the sea <span class="hlt">ice</span> simulation except to improve local dynamics because of better coastline representation. Sea <span class="hlt">ice</span> growth is decomposed into thermodynamic and dynamic (including all non-thermodynamic processes in the model) contributions to study the <span class="hlt">ice</span> thickness evolution. Relatively smaller thermodynamic contribution to <span class="hlt">ice</span> growth between December and the following April is found in the thick and very thick <span class="hlt">ice</span> regions, with larger contributions in the thin <span class="hlt">ice</span>-covered region. No significant trend in winter maximum <span class="hlt">ice</span> <span class="hlt">volume</span> is found in the northern CAA and Baffin Bay while a decline (r2 ≈ 0.6, p < 0.01) is simulated in Parry Channel region. The two main contributors (thermodynamic growth and lateral transport) have high interannual <span class="hlt">variabilities</span> which largely balance each other, so that maximum <span class="hlt">ice</span> <span class="hlt">volume</span> can</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.488...36L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.488...36L"><span>Precession and atmospheric CO2 modulated <span class="hlt">variability</span> of sea <span class="hlt">ice</span> in the central Okhotsk Sea since 130,000 years ago</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lo, Li; Belt, Simon T.; Lattaud, Julie; Friedrich, Tobias; Zeeden, Christian; Schouten, Stefan; Smik, Lukas; Timmermann, Axel; Cabedo-Sanz, Patricia; Huang, Jyh-Jaan; Zhou, Liping; Ou, Tsong-Hua; Chang, Yuan-Pin; Wang, Liang-Chi; Chou, Yu-Min; Shen, Chuan-Chou; Chen, Min-Te; Wei, Kuo-Yen; Song, Sheng-Rong; Fang, Tien-Hsi; Gorbarenko, Sergey A.; Wang, Wei-Lung; Lee, Teh-Quei; Elderfield, Henry; Hodell, David A.</p> <p>2018-04-01</p> <p>Recent reduction in high-latitude sea <span class="hlt">ice</span> extent demonstrates that sea <span class="hlt">ice</span> is highly sensitive to external and internal radiative forcings. In order to better understand sea <span class="hlt">ice</span> system responses to external orbital forcing and internal oscillations on orbital timescales, here we reconstruct changes in sea <span class="hlt">ice</span> extent and summer sea surface temperature (SSST) over the past 130,000 yrs in the central Okhotsk Sea. We applied novel organic geochemical proxies of sea <span class="hlt">ice</span> (IP25), SSST (TEX86L) and open water marine productivity (a tri-unsaturated highly branched isoprenoid and biogenic opal) to marine sediment core MD01-2414 (53°11.77‧N, 149°34.80‧E, water depth 1123 m). To complement the proxy data, we also carried out transient Earth system model simulations and sensitivity tests to identify contributions of different climatic forcing factors. Our results show that the central Okhotsk Sea was <span class="hlt">ice</span>-free during Marine Isotope Stage (MIS) 5e and the early-mid Holocene, but experienced <span class="hlt">variable</span> sea <span class="hlt">ice</span> cover during MIS 2-4, consistent with intervals of relatively high and low SSST, respectively. Our data also show that the sea <span class="hlt">ice</span> extent was governed by precession-dominated insolation changes during intervals of atmospheric CO2 concentrations ranging from 190 to 260 ppm. However, the proxy record and the model simulation data show that the central Okhotsk Sea was near <span class="hlt">ice</span>-free regardless of insolation forcing throughout the penultimate interglacial, and during the Holocene, when atmospheric CO2 was above ∼260 ppm. Past sea <span class="hlt">ice</span> conditions in the central Okhotsk Sea were therefore strongly modulated by both orbital-driven insolation and CO2-induced radiative forcing during the past glacial/interglacial cycle.</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 <span class="hlt">Volume</span>, (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 Masses, ( 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('http://adsabs.harvard.edu/abs/2017AGUFM.C42A..04B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C42A..04B"><span>Endmembers of <span class="hlt">Ice</span> Shelf Melt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boghosian, A.; Child, S. F.; Kingslake, J.; Tedesco, M.; Bell, R. E.; Alexandrov, O.; McMichael, S.</p> <p>2017-12-01</p> <p>Studies of surface melt on <span class="hlt">ice</span> shelves have defined a spectrum of meltwater behavior. On one end the storage of meltwater in persistent surface ponds can trigger <span class="hlt">ice</span> shelf collapse as in the 2002 event leading to the disintegration of the Larsen B <span class="hlt">Ice</span> Shelf. On the other, meltwater export by rivers can stabilize an <span class="hlt">ice</span> shelf as was recently shown on the Nansen <span class="hlt">Ice</span> Shelf. We explore this dichotomy by quantifying the partitioning between stored and transported water on two glaciers adjacent to floating <span class="hlt">ice</span> shelves, Nimrod (Antarctica) and Peterman (Greenland). We analyze optical satellite imagery (LANDSAT, WorldView), airborne imagery (Operation <span class="hlt">Ice</span>Bridge, Trimetrogon Aerial Phototography), satellite radar (Sentinel-1), and digital elevation models (DEMs) to categorize surface meltwater fate and map the evolution of <span class="hlt">ice</span> shelf hydrology and topographic features through time. On the floating Peterman Glacier tongue a sizable river exports water to the ocean. The surface hydrology of Nimrod Glacier, geometrically similar to Peterman but with ten times shallower surface slope, is dominated by storage in surface lakes. In contrast, the Nansen has the same surface slope as Nimrod but transports water through surface rivers. Slope alone is not the sole control on <span class="hlt">ice</span> shelf hydrology. It is essential to track the storage and transport <span class="hlt">volumes</span> for each of these systems. To estimate water storage and transport we analyze high resolution (40 cm - 2 m) modern and historical DEMs. We produce historical (1957 onwards) DEMs with structure-from-motion photogrammetry. The DEMs are used to constrain water storage potential estimates of observed basins and water routing/transport potential. We quantify the total <span class="hlt">volume</span> of water stored seasonally and interannually. We use the normalize difference water index to map meltwater extent, and estimate lake water depth from optical data. We also consider the role of stored water in subsurface aquifers in recharging surface water after</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P43C2889P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P43C2889P"><span><span class="hlt">Variability</span> in radar returns from Martian debris-covered glaciers attributed to surface debris layer roughness and composition: implications for the regional distribution of massive subsurface <span class="hlt">ice</span> and near-surface pore-filling <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>Petersen, E.; Holt, J. W.; Levy, J. S.; Lalich, D.</p> <p>2017-12-01</p> <p>Lobate debris aprons, lineated valley fill, and concentric crater fill are a class of Martian landform thought to be glaciers blanketed by a lithic debris layer. They are found in the mid latitudes (roughly 30-50°N and S) where surface <span class="hlt">ice</span> is presently unstable. Shallow Radar (SHARAD) sounder observations are in many cases able to resolve the basal contact between the glacier and underlying bedrock, showing that the bulk composition of these features is water <span class="hlt">ice</span> with < 20% lithic debris; they are thus often referred to as debris-covered glaciers (DCG). The basal contact of candidate glaciers is not always present in SHARAD radargrams, and <span class="hlt">variable</span> reflection power between glacier sites suggests that non-detections may be due to a reduction of echo power below the noise floor. A likely candidate for signal loss is the <span class="hlt">variable</span> roughness of different glacial surface textures. We test this mechanism of signal reduction via analysis of SHARAD reflections augmented by surface roughness analyses generated from HiRISE stereo DEMs. This method provides a means of constraining the electrical properties of the surface debris. We show that measured surface roughness is sufficient to explain basal reflection signal loss for five glacier sites in the region of Deuteronilus/Protonilus Mensae (R2 = 0.90), with the dielectric constant for the surface debris layer constrained to 4.9 ± 0.3. Assuming debris formed of basalt rock, this value is consistent with a porous debris layer containing up to 64% <span class="hlt">ice</span>, or an <span class="hlt">ice</span>-free debris layer with porosity of 28-34%. From this work, we conclude that (1) weak or non-existent basal reflections at these sites are due to roughness-induced radar signal loss and not due to differing properties of the basal interface, (2) all DCG candidates in this study exhibit similar bulk compositions of relatively pure water <span class="hlt">ice</span>, and (3) the surface debris layer is formed of porous lithic debris which may contain a significant fraction of pore <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C21A0658Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21A0658Z"><span>Changes in Arctic Sea <span class="hlt">Ice</span> Thickness and Floe Size</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, J.; Schweiger, A. J. B.; Stern, H. L., III; Steele, M.</p> <p>2016-12-01</p> <p>A thickness, floe size, and enthalpy distribution sea <span class="hlt">ice</span> model was implemented into the Pan-arctic <span class="hlt">Ice</span>-Ocean Modeling and Assimilation System (PIOMAS) by coupling the Zhang et al. [2015] sea <span class="hlt">ice</span> floe size distribution (FSD) theory with the Thorndike et al. [1975] <span class="hlt">ice</span> thickness distribution (ITD) theory in order to explicitly simulate multicategory FSD and ITD simultaneously. A range of <span class="hlt">ice</span> thickness and floe size observations were used for model calibration and validation. The expanded, validated PIOMAS was used to study sea <span class="hlt">ice</span> response to atmospheric and oceanic changes in the Arctic, focusing on the interannual <span class="hlt">variability</span> and trends of <span class="hlt">ice</span> thickness and floe size over the period 1979-2015. It is found that over the study period both <span class="hlt">ice</span> thickness and floe size have been decreasing steadily in the Arctic. The simulated <span class="hlt">ice</span> thickness shows considerable spatiotemporal <span class="hlt">variability</span> in recent years. As the <span class="hlt">ice</span> cover becomes thinner and weaker, the model simulates an increasing number of small floes (at the low end of the FSD), which affects sea <span class="hlt">ice</span> properties, particularly in the marginal <span class="hlt">ice</span> zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=nano&id=EJ934970','ERIC'); return false;" href="https://eric.ed.gov/?q=nano&id=EJ934970"><span>We Scream for Nano <span class="hlt">Ice</span> Cream</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>Jones, M. Gail; Krebs, Denise L.; Banks, Alton J.</p> <p>2011-01-01</p> <p>There is a wide range of new products emerging from nanotechnology, and "nano <span class="hlt">ice</span> cream" is an easy one that you can use to teach topics from surface area to <span class="hlt">volume</span> applications. In this activity, students learn how <span class="hlt">ice</span> cream can be made smoother and creamier tasting through nanoscience. By using liquid nitrogen to cool the cream mixture, students…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A43F0302B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A43F0302B"><span>Development of a balloon-borne device for analysis of high-altitude <span class="hlt">ice</span> and aerosol particulates: <span class="hlt">Ice</span> Cryo Encapsulator by Balloon (<span class="hlt">ICE</span>-Ball)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boaggio, K.; Bandamede, M.; Bancroft, L.; Hurler, K.; Magee, N. B.</p> <p>2016-12-01</p> <p>We report on details of continuing instrument development and deployment of a novel balloon-borne device for capturing and characterizing atmospheric <span class="hlt">ice</span> and aerosol particles, the <span class="hlt">Ice</span> Cryo Encapsulator by Balloon (<span class="hlt">ICE</span>-Ball). The device is designed to capture and preserve cirrus <span class="hlt">ice</span> particles, maintaining them at cold equilibrium temperatures, so that high-altitude particles can recovered, transferred intact, and then imaged under SEM at an unprecedented resolution (approximately 3 nm maximum resolution). In addition to cirrus <span class="hlt">ice</span> particles, high altitude aerosol particles are also captured, imaged, and analyzed for geometry, chemical composition, and activity as <span class="hlt">ice</span> nucleating particles. Prototype versions of <span class="hlt">ICE</span>-Ball have successfully captured and preserved high altitude <span class="hlt">ice</span> particles and aerosols, then returned them for recovery and SEM imaging and analysis. New improvements include 1) ability to capture particles from multiple narrowly-defined altitudes on a single payload, 2) high quality measurements of coincident temperature, humidity, and high-resolution video at capture altitude, 3) ability to capture particles during both ascent and descent, 4) better characterization of particle collection <span class="hlt">volume</span> and collection efficiency, and 5) improved isolation and characterization of capture-cell cryo environment. This presentation provides detailed capability specifications for anyone interested in using measurements, collaborating on continued instrument development, or including this instrument in ongoing or future field campaigns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C53C0725H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C53C0725H"><span>Sediment <span class="hlt">Volume</span> Record of Paleogene-Neogene Transantarctic Mountains Erosion and Landscape Modification, McMurdo Sound Region, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hall, T.; Wilson, T. J.; Henrys, S.; Speece, M. A.</p> <p>2016-12-01</p> <p>The interplay of tectonics and climate is recorded in the sedimentary strata within Victoria Land Basin, McMurdo Sound, Antarctica. Patterns of Cenozoic sedimentation are documented from interpretation of seismic reflection profiles calibrated by drillhole data in McMurdo Sound, and these patterns provide enhanced constraints on the evolution of the coupled Transantarctic Mountains-West Antarctic Rift System and on <span class="hlt">ice</span> sheet advance/retreat through multiple climate cycles. The research focuses on shifts from warm based to cold based <span class="hlt">ice</span> sheets through the <span class="hlt">variable</span> climate and <span class="hlt">ice</span> sheet conditions that characterized the early to middle Miocene. The study seeks to test the view that cold based <span class="hlt">ice</span> sheets in arid, polar deserts minimally erode the landscape by calculating sediment <span class="hlt">volumes</span> for critical climatic intervals. Revised seismic mapping through McMurdo Sound has been completed, utilizing the seismic stratigraphic framework first established by Fielding et al. (2006) and new reflectors marking unconformities identified from the AND-2A core (Levy et al., 2016). Reflector age constraints are derived by tying surfaces to the Cape Roberts Project, CIROS-1, and AND-2A drillholes. Seismic facies coupled with AND-2A core provenance information provides insight into depositional mechanisms and <span class="hlt">ice</span> sheet behavior. Seismic facies transitions occur across the major unconformity surfaces in the AND-2A core. Sediment <span class="hlt">volume</span> calculations for subareas within McMurdo Sound where reflectors are most continuous indicate substantial decreases in preserved sediment <span class="hlt">volume</span> between the Oligocene and Early Miocene sequences, and between the early and mid-Miocene sequences. Sediment <span class="hlt">volumes</span>, used in combination with an <span class="hlt">ice</span> sheet model in a backstacking procedure, provide constraints on landscape modification and further understanding of how landscapes erode under warm and cold based <span class="hlt">ice</span> sheet regimes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013QSRv...79..168A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013QSRv...79..168A"><span>A review of sea <span class="hlt">ice</span> proxy information from polar <span class="hlt">ice</span> cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abram, Nerilie J.; Wolff, Eric W.; Curran, Mark A. J.</p> <p>2013-11-01</p> <p>Sea <span class="hlt">ice</span> plays an important role in Earth's climate system. The lack of direct indications of past sea <span class="hlt">ice</span> coverage, however, means that there is limited knowledge of the sensitivity and rate at which sea <span class="hlt">ice</span> dynamics are involved in amplifying climate changes. As such, there is a need to develop new proxy records for reconstructing past sea <span class="hlt">ice</span> conditions. Here we review the advances that have been made in using chemical tracers preserved in <span class="hlt">ice</span> cores to determine past changes in sea <span class="hlt">ice</span> cover around Antarctica. <span class="hlt">Ice</span> core records of sea salt concentration show promise for revealing patterns of sea <span class="hlt">ice</span> extent particularly over glacial-interglacial time scales. In the coldest climates, however, the sea salt signal appears to lose sensitivity and further work is required to determine how this proxy can be developed into a quantitative sea <span class="hlt">ice</span> indicator. Methane sulphonic acid (MSA) in near-coastal <span class="hlt">ice</span> cores has been used to reconstruct quantified changes and interannual <span class="hlt">variability</span> in sea <span class="hlt">ice</span> extent over shorter time scales spanning the last ˜160 years, and has potential to be extended to produce records of Antarctic sea <span class="hlt">ice</span> changes throughout the Holocene. However the MSA <span class="hlt">ice</span> core proxy also requires careful site assessment and interpretation alongside other palaeoclimate indicators to ensure reconstructions are not biased by non-sea <span class="hlt">ice</span> factors, and we summarise some recommended strategies for the further development of sea <span class="hlt">ice</span> histories from <span class="hlt">ice</span> core MSA. For both proxies the limited information about the production and transfer of chemical markers from the sea <span class="hlt">ice</span> zone to the Antarctic <span class="hlt">ice</span> sheets remains an issue that requires further multidisciplinary study. Despite some exploratory and statistical work, the application of either proxy as an indicator of sea <span class="hlt">ice</span> change in the Arctic also remains largely unknown. As information about these new <span class="hlt">ice</span> core proxies builds, so too does the potential to develop a more comprehensive understanding of past changes in sea</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C51A0683R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C51A0683R"><span>Inter-comparison of isotropic and anisotropic sea <span class="hlt">ice</span> rheology in a fully coupled model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roberts, A.; Cassano, J. J.; Maslowski, W.; Osinski, R.; Seefeldt, M. W.; Hughes, M.; Duvivier, A.; Nijssen, B.; Hamman, J.; Hutchings, J. K.; Hunke, E. C.</p> <p>2015-12-01</p> <p>We present the sea <span class="hlt">ice</span> climate of the Regional Arctic System Model (RASM), using a suite of new physics available in the Los Alamos Sea <span class="hlt">Ice</span> Model (CICE5). RASM is a high-resolution fully coupled pan-Arctic model that also includes the Parallel Ocean Program (POP), the Weather Research and Forecasting Model (WRF) and <span class="hlt">Variable</span> Infiltration Capacity (VIC) land model. The model domain extends from ~45˚N to the North Pole and is configured to run at ~9km resolution for the <span class="hlt">ice</span> and ocean components, coupled to 50km resolution atmosphere and land models. The baseline sea <span class="hlt">ice</span> model configuration includes mushy-layer sea <span class="hlt">ice</span> thermodynamics and level-<span class="hlt">ice</span> melt ponds. Using this configuration, we compare the use of isotropic and anisotropic sea <span class="hlt">ice</span> mechanics, and evaluate model performance using these two variants against observations including Arctic buoy drift and deformation, satellite-derived drift and deformation, and sea <span class="hlt">ice</span> <span class="hlt">volume</span> estimates from ICESat. We find that the isotropic rheology better approximates spatial patterns of thickness observed across the Arctic, but that both rheologies closely approximate scaling laws observed in the pack using buoys and RGPS data. A fundamental component of both <span class="hlt">ice</span> mechanics variants, the so called Elastic-Viscous-Plastic (EVP) and Anisotropic-Elastic-Plastic (EAP), is that they are highly sensitive to the timestep used for elastic sub-cycling in an inertial-resolving coupled framework, and this has a significant affect on surface fluxes in the fully coupled framework.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003145','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003145"><span>Antarctic Sea-<span class="hlt">Ice</span> Freeboard and Estimated Thickness from NASA's ICESat and <span class="hlt">Ice</span>Bridge Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yi, Donghui; Kurtz, Nathan; Harbeck, Jeremy; Manizade, Serdar; Hofton, Michelle; Cornejo, Helen G.; Zwally, H. Jay; Robbins, John</p> <p>2016-01-01</p> <p>ICESat completed 18 observational campaigns during its lifetime from 2003 to 2009. Data from all of the 18 campaign periods are used in this study. Most of the operational periods were between 34 and 38 days long. Because of laser failure and orbit transition from 8-day to 91-day orbit, there were four periods lasting 57, 16, 23, and 12 days. <span class="hlt">Ice</span>Bridge data from 2009, 2010, and 2011 are used in this study. Since 2009, there are 19 Airborne Topographic Mapper (ATM) campaigns, and eight Land, Vegetation, and <span class="hlt">Ice</span> Sensor (LVIS) campaigns over the Antarctic sea <span class="hlt">ice</span>. Freeboard heights are derived from ICESat, ATM and LVIS elevation and waveform data. With nominal densities of snow, water, and sea <span class="hlt">ice</span>, combined with snow depth data from AMSR-E/AMSR2 passive microwave observation over the southern ocean, sea-<span class="hlt">ice</span> thickness is derived from the freeboard. Combined with AMSR-E/AMSR2 <span class="hlt">ice</span> concentration, sea-<span class="hlt">ice</span> area and <span class="hlt">volume</span> are also calculated. During the 2003-2009 period, sea-<span class="hlt">ice</span> freeboard and thickness distributions show clear seasonal variations that reflect the yearly cycle of the growth and decay of the Antarctic pack <span class="hlt">ice</span>. We found no significant trend of thickness or area for the Antarctic sea <span class="hlt">ice</span> during the ICESat period. <span class="hlt">Ice</span>Bridge sea <span class="hlt">ice</span> freeboard and thickness data from 2009 to 2011 over the Weddell Sea and Amundsen and Bellingshausen Seas are compared with the ICESat results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C22A..07I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C22A..07I"><span>Retrieval of sea <span class="hlt">ice</span> thickness during Arctic summer using melt pond color</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Istomina, L.; Nicolaus, M.; Heygster, G.</p> <p>2016-12-01</p> <p>The thickness of sea <span class="hlt">ice</span> is an important climatic <span class="hlt">variable</span>. Together with the <span class="hlt">ice</span> concentration, it defines the total sea <span class="hlt">ice</span> <span class="hlt">volume</span>, is linked within the climatic feedback mechanisms and affects the Arctic energy balance greatly. During Arctic summer, the sea <span class="hlt">ice</span> cover changes rapidly, which includes the presence of melt ponds, as well as reduction of <span class="hlt">ice</span> albedo and <span class="hlt">ice</span> thickness. Currently available remote sensing retrievals of sea <span class="hlt">ice</span> thickness utilize data from altimeter, microwave, thermal infrared sensors and their combinations. All of these methods are compromised in summer in the presence of melt. This only leaves in situ and airborne sea <span class="hlt">ice</span> thickness data available in summer. At the same time, data of greater coverage is needed for assimilation in global circulation models and correct estimation of <span class="hlt">ice</span> mass balance.This study presents a new approach to estimate sea <span class="hlt">ice</span> thickness in summer in the presence of melt ponds. Analysis of field data obtained during the RV "Polarstern" cruise ARK27/3 (August - October 2012) has shown a clear connection of <span class="hlt">ice</span> thickness under melt ponds to their measured spectral albedo and to melt pond color in the hue-saturation-luminance color space from field photographs. An empirical function is derived from the HSL values and applied to aerial imagery obtained during various airborne campaigns. Comparison to in situ <span class="hlt">ice</span> thickness shows a good correspondence to the <span class="hlt">ice</span> thickness value retrieved in the melt ponds. A similar retrieval is developed for satellite spectral bands using the connection of the measured pond spectral albedo to the <span class="hlt">ice</span> thickness within the melt ponds. Correction of the retrieved <span class="hlt">ice</span> thickness in ponds to derive total thickness of sea <span class="hlt">ice</span> is discussed. Case studies and application to very high resolution optical data are presented, as well as a concept to transfer the method to satellite data of lower spatial resolution where melt ponds become subpixel features.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1812655S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1812655S"><span>Arctic sea-<span class="hlt">ice</span> melting: Effects on hydroclimatic <span class="hlt">variability</span> and on UV-induced carbon cycling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sulzberger, Barbara</p> <p>2016-04-01</p> <p>Since 1980 both the perennial and the multiyear central Arctic sea <span class="hlt">ice</span> areas have declined by approximately 13 and 15% per decade, respectively (IPCC, 2013). Arctic sea-<span class="hlt">ice</span> melting has led to an increase in the amplitude of the Northern Hemisphere jet stream and, as a consequence, in more slowly moving Rossby waves which results in blocking of weather patterns such as heat waves, droughts, cold spells, and heavy precipitation events (Francis and Vavrus, 2012). Changing Rossby waves account for more than 30% of the precipitation <span class="hlt">variability</span> over several regions of the northern middle and high latitudes, including the US northern Great Plains and parts of Canada, Europe, and Russia (Schubert et al., 2011). From 2007 to 2013, northern Europe experienced heavy summer precipitation events that were unprecedented in over a century, concomitant with Arctic sea <span class="hlt">ice</span> loss (Screen, 2013). Heavy precipitation events tend to increase the runoff intensity of terrigenous dissolved organic matter (tDOM) (Haaland et al., 2010). In surface waters tDOM is subject to UV-induced oxidation to produce atmospheric CO2. Mineralization of DOM also occurs via microbial respiration. However, not all chemical forms of DOM are available to bacterioplankton. UV-induced transformations generally increase the bioavailability of tDOM (Sulzberger and Durisch-Kaiser, 2009). Mineralization of tDOM is an important source of atmospheric CO2 and this process is likely to contribute to positive feedbacks on global warming (Erickson et al., 2015). However, the magnitudes of these potential feedbacks remain unexplored. This paper will discuss the following items: 1.) Links between Arctic sea-<span class="hlt">ice</span> melting, heavy precipitation events, and enhanced tDOM runoff. 2.) UV-induced increase in the bioavailability of tDOM. 3.) UV-mediated feedbacks on global warming. References Erickson, D. J. III, B. Sulzberger, R. G. Zepp, A. T. Austin (2015), Effects of stratospheric ozone depletion, solar UV radiation, and climate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007RvGeo..45.3007P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007RvGeo..45.3007P"><span>Pleistocene hydrology of North America: The role of <span class="hlt">ice</span> sheets in reorganizing groundwater flow systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Person, Mark; McIntosh, Jennifer; Bense, Victor; Remenda, V. H.</p> <p>2007-09-01</p> <p>While the geomorphic consequences of Pleistocene megafloods have been known for some time, it has been only in the past 2 decades that hydrogeologists and glaciologists alike have begun to appreciate the important impact that <span class="hlt">ice</span> sheet-aquifer interactions have had in controlling subsurface flow patterns, recharge rates, and the distribution of fresh water in confined aquifer systems across North America. In this paper, we document the numerous lines of geochemical, isotopic, and geomechanical evidence of <span class="hlt">ice</span> sheet hydrogeology across North America. We also review the mechanical, thermal, and hydrologic processes that control subsurface fluid migration beneath <span class="hlt">ice</span> sheets. Finite element models of subsurface fluid flow, permafrost formation, and <span class="hlt">ice</span> sheet loading are presented to investigate the coupled nature of transport processes during glaciation/deglaciation. These indicate that recharge rates as high as 10 times modern values occurred as the Laurentide <span class="hlt">Ice</span> Sheet overran the margins of sedimentary basins. The effects of <span class="hlt">ice</span> sheet loading and permafrost formation result in complex transient flow patterns within aquifers and confining units alike. Using geochemical and environmental isotopic data, we estimate that the <span class="hlt">volume</span> of glacial meltwater emplaced at the margins of sedimentary basins overrun by the Laurentide <span class="hlt">Ice</span> Sheet totals about 3.7 × 104 km3, which is about 0.2% of the <span class="hlt">volume</span> of the Laurentide <span class="hlt">Ice</span> Sheet. Subglacial infiltration estimates based on continental-scale hydrologic models are even higher (5-10% of meltwater generated). These studies in sum call into question the widely held notion that groundwater flow patterns within confined aquifer systems are controlled primarily by the water table configuration during the Pleistocene. Rather, groundwater flow patterns were likely much more complex and transient in nature than has previously been thought. Because Pleistocene recharge rates are believed to be highly <span class="hlt">variable</span>, these studies have profound</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19750049790&hterms=LOSS+SOIL&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DLOSS%2BSOIL','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19750049790&hterms=LOSS+SOIL&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DLOSS%2BSOIL"><span>Microwave signatures of snow, <span class="hlt">ice</span> and soil at several wavelengths</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gloersen, P.; Schmugge, T. J.; Chang, T. C.</p> <p>1974-01-01</p> <p>Analyses of data obtained from aircraft-borne radiometers have shown that the microwave signatures of various parts of the terrain depend on both the <span class="hlt">volume</span> scattering cross-section and the dielectric loss in the medium. In soil, it has been found that experimental data fit a model in which the scattering cross section is negligible compared to the dielectric loss. On the other hand, the <span class="hlt">volume</span> scattering cross-section in snow and continental <span class="hlt">ice</span> was found, from analyzing data obtained with aircraft- and spacecraft-borne radiometers, to be more important than the dielectric loss or surface reflectivity in determining the observed microwave emissivity. A model which assumes Mie scattering of <span class="hlt">ice</span> particles of various sizes was found to be the dominant <span class="hlt">volume</span> scattering mechanism in these media. Both spectral variation in the microwave signatures of snow and <span class="hlt">ice</span> fields, as well as the variation in the emissivity of continental <span class="hlt">ice</span> sheets such as those covering Greenland and Antarctica appear to be consistent with this model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A23L3414D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A23L3414D"><span>Small-Scale Spatial <span class="hlt">Variability</span> of <span class="hlt">Ice</span> Supersaturation and Cirrus in the TTL</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>DiGangi, J. P.; Podolske, J. R.; Rana, M.; Slate, T. A.; Diskin, G. S.</p> <p>2014-12-01</p> <p>The processes controlling cloud formation and evolution represent a significant uncertainty in models of global climate change. High altitude cirrus clouds contribute a large portion of this uncertainty due to their altitude and abundance. The mechanism behind the formation of cirrus clouds depends on the characteristics and composition of <span class="hlt">ice</span> supersaturation (ISS) regions, regions where the relative humidity with respect to <span class="hlt">ice</span> (RHi) is greater than 100%. Small-scale dynamics have recently been shown to have a strong effect on the RHi of the UT/LS, and therefore on cirrus cloud formation. Until now, there has been insufficient data in the Tropical Tropopause Layer (TTL) to investigate these effects. The Airborne Tropical TRopopause EXperiment (ATTREX) was a series of campaigns focused on improving our understanding of humidity in the TTL. During this campaign, the NASA Langley/Ames Diode Laser Hygrometer was part of the payload on the NASA Global Hawk, resulting in measurements of humidity with as low as 1-2 m vertical resolution at altitudes up to 19 km. We will present observations from ATTREX describing the small scale spatial <span class="hlt">variability</span> of water vapor along transects of ISSRs and cirrus clouds, as well as the dynamics driving the formation of ISS regions. These results will be discussed in context with results from prior UT/LS campaigns, such as DC3 and HIPPO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT.........9B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT.........9B"><span>Detection and Analysis of Complex Patterns of <span class="hlt">Ice</span> Dynamics in Antarctica from ICESat Laser Altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Babonis, Gregory Scott</p> <p></p> <p>There remains much uncertainty in estimating the amount of Antarctic <span class="hlt">ice</span> mass change, its dynamic component, and its spatial and temporal patterns. This work remedies the limitations of previous studies by generating the first detailed reconstruction of total and dynamic <span class="hlt">ice</span> thickness and mass changes across Antarctica, from ICESat satellite altimetry observations in 2003-2009 using the Surface Elevation Reconstruction and Change Detection (SERAC) method. <span class="hlt">Ice</span> sheet thickness changes are calculated with quantified error estimates for each time when ICESat flew over a ground-track crossover region, at approximately 110,000 locations across the Antarctic <span class="hlt">Ice</span> Sheet. The time series are partitioned into changes due to surficial processes and <span class="hlt">ice</span> dynamics. The new results markedly improve the spatial and temporal resolution of surface elevation, <span class="hlt">volume</span>, and mass change rates for the AIS, and can be sampled at annual temporal resolutions. The results indicate a complex spatiotemporal pattern of dynamic mass loss in Antarctica, especially along individual outlet glaciers, and allow for the quantification of the annual contribution of Antarctic <span class="hlt">ice</span> loss to sea level rise. Over 5000 individual locations exhibit either strong dynamic <span class="hlt">ice</span> thickness change patterns, accounting for approximately 500 unique spatial clusters that identify regions likely influenced by subglacial hydrology. The spatial distribution and temporal behavior of these regions reveal the complexity and short-time scale <span class="hlt">variability</span> in the subglacial hydrological system. From the 500 unique spatial clusters, over 370 represent newly identified, and not previously published, potential subglacial water bodies indicating an active subglacial hydrological system over a much larger region than previously observed. These numerous new observations of dynamic changes provide more than simply a larger set of data. Examination of both regional and local scale dynamic change patterns across Antarctica shows newly</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 <span class="hlt">variables</span> accurately from space. Submillimeter (submm) wave remote sensing has capability of penetrating clouds and measuring <span class="hlt">ice</span> mass 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://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> <span class="hlt">volume</span> currently is declining, but more needs to be known about mountain glacier and <span class="hlt">ice</span> sheet mass balances. -from Author</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080045474','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080045474"><span>Physical and Radiative Characteristic and Long-term <span class="hlt">Variability</span> of the Okhotsk Sea <span class="hlt">Ice</span> Cover</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nishio, Fumihiko; Comiso, Josefino C.; Gersten, Robert; Nakayama, Masashige; Ukita, Jinro; Gasiewski, Al; Stanko, Boba; Naoki, Kazuhiro</p> <p>2008-01-01</p> <p>Much of what we know about the large scale characteristics of the Okhotsk Sea <span class="hlt">ice</span> cover has been provided by <span class="hlt">ice</span> concentration maps derived from passive microwave data. To understand what satellite data represent in a highly divergent and rapidly changing environment like the Okhotsk Sea, we take advantage of concurrent satellite, aircraft, and ship data acquired on 7 February and characterized the sea <span class="hlt">ice</span> cover at different scales from meters to hundreds of kilometers. Through comparative analysis of surface features using co-registered data from visible, infrared and microwave channels we evaluated the general radiative and physical characteristics of the <span class="hlt">ice</span> cover as well as quantify the distribution of different <span class="hlt">ice</span> types in the region. <span class="hlt">Ice</span> concentration maps from AMSR-E using the standard sets of channels, and also only the 89 GHz channel for optimal resolution, are compared with aircraft and high resolution visible data and while the standard set provides consistent results, the 89 GHz provides the means to observe mesoscale patterns and some unique features of the <span class="hlt">ice</span> cover. Analysis of MODIS data reveals that thick <span class="hlt">ice</span> types represents about 37% of the <span class="hlt">ice</span> cover indicating that young and new <span class="hlt">ice</span> types represent a large fraction of the <span class="hlt">ice</span> cover that averages about 90% <span class="hlt">ice</span> concentration according to passive microwave data. These results are used to interpret historical data that indicate that the Okhotsk Sea <span class="hlt">ice</span> extent and area are declining at a rapid rate of about -9% and -12 % per decade, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7488S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7488S"><span>Integrated firn elevation change model for 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>Saß, Björn; Sauter, Tobias; Braun, Matthias</p> <p>2016-04-01</p> <p>We present the development of a firn compaction model in order to improve the <span class="hlt">volume</span> to mass conversion of geodetic glacier mass balance measurements. The model is applied on the Arctic <span class="hlt">ice</span> cap Vestfonna. Vestfonna is located on the island Nordaustlandet in the north east of Svalbard. Vestfonna covers about 2400 km² and has a dome like shape with well-defined outlet glaciers. Elevation and <span class="hlt">volume</span> changes measured by e.g. satellite techniques are becoming more and more popular. They are carried out over observation periods of <span class="hlt">variable</span> length and often covering different meteorological and snow hydrological regimes. The elevation change measurements compose of various components including dynamic adjustments, firn compaction and mass loss by downwasting. Currently, geodetic glacier mass balances are frequently converted from elevation change measurements using a constant conversion factor of 850 kg m-³ or the density of <span class="hlt">ice</span> (917 kg m-³) for entire glacier basins. However, the natural conditions are rarely that static. Other studies used constant densities for the ablation (900 kg m-³) and accumulation (600 kg m-³) areas, whereby density variations with varying meteorological and climate conditions are not considered. Hence, each approach bears additional uncertainties from the <span class="hlt">volume</span> to mass conversion that are strongly affected by the type and timing of the repeat measurements. We link and adapt existing models of surface energy balance, accumulation and snow and firn processes in order to improve the <span class="hlt">volume</span> to mass conversion by considering the firn compaction component. Energy exchange at the surface is computed by a surface energy balance approach and driven by meteorological <span class="hlt">variables</span> like incoming short-wave radiation, air temperature, relative humidity, air pressure, wind speed, all-phase precipitation, and cloud cover fraction. Snow and firn processes are addressed by a coupled subsurface model, implemented with a non-equidistant layer discretisation. On</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002PhDT........42D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002PhDT........42D"><span>Modeling of scattering from <span class="hlt">ice</span> surfaces</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dahlberg, Michael Ross</p> <p></p> <p>Theoretical research is proposed to study electromagnetic wave scattering from <span class="hlt">ice</span> surfaces. A mathematical formulation that is more representative of the electromagnetic scattering from <span class="hlt">ice</span>, with <span class="hlt">volume</span> mechanisms included, and capable of handling multiple scattering effects is developed. This research is essential to advancing the field of environmental science and engineering by enabling more accurate inversion of remote sensing data. The results of this research contributed towards a more accurate representation of the scattering from <span class="hlt">ice</span> surfaces, that is computationally more efficient and that can be applied to many remote-sensing applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060032490&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060032490&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar"><span>Combined Satellite - and ULS-Derived Sea-<span class="hlt">Ice</span> Flux in the Weddell Sea</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Drinkwater, M.; Liu, X.; Harms, S.</p> <p>2000-01-01</p> <p>Several years of daily microwave satellite <span class="hlt">ice</span>-drift are combined with moored Upward Looking Sonar (ULS) <span class="hlt">ice</span>-drafts into an <span class="hlt">ice</span> <span class="hlt">volume</span> flux record at points along a flux gate across the Weddell Sea, Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C13B0554F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C13B0554F"><span>Arctic Circle Traverse 2010 (ACT-10): South East Greenland snow accumulation <span class="hlt">variability</span> from firn coring and <span class="hlt">ice</span> sounding radar</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forster, R. R.; Miege, C.; Box, J. E.; McConnell, J.; Spikes, V. B.; Burgess, E. W.</p> <p>2010-12-01</p> <p>The Greenland <span class="hlt">Ice</span> Sheet plays an important role in Earth’s climate system evolution. The snow accumulation rate is the largest single mass budget term. With only 14% of the <span class="hlt">ice</span> sheet area, Southeast Greenland contains the highest accumulation rates, accounting for one third of the total snow accumulation and annual <span class="hlt">variability</span>. The high accumulation rates have made the region less desirable for long climate record <span class="hlt">ice</span> cores and therefore, contain relatively very few in situ measurements to constrain the <span class="hlt">ice</span> sheet mass budget. We present annual snow accumulation rates from the Arctic Circle Traverse 2010 (ACT-10). During April and May 2010 we acquired three 50 m firn cores connected by surface-based 400 MHz ground penetrating radar (GPR) in Southeast Greenland. The traverse repeated and extended the original Arctic Circle Traverse in 2004 (Spikes et al., 2004). Dating is achieved using geochemical analysis of the cores to identify isochronal layers detected by the GPR yielding annual accumulation estimates along the traverse between the core sites. The 300 km ACT-10 GPR snowmobile traverse extended the ACT-04 path 80 km to the lowest elevation core site at 1776 m. Meanwhile, airborne radars, operating as part of NASA’s Operation <span class="hlt">Ice</span>Bridge also acquired data over the full length of the ACT-10 path, simultaneously with a portion of the traverse and within days for the remaining segments. The <span class="hlt">Ice</span>Bridge and ACT-10 data are to be combined in a calibration effort such that snow accumulation rates may be mapped elsewhere in Greenland and even in Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27650478','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27650478"><span>Canadian Arctic sea <span class="hlt">ice</span> reconstructed from bromine in the Greenland NEEM <span class="hlt">ice</span> core.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Spolaor, Andrea; Vallelonga, Paul; Turetta, Clara; Maffezzoli, Niccolò; Cozzi, Giulio; Gabrieli, Jacopo; Barbante, Carlo; Goto-Azuma, Kumiko; Saiz-Lopez, Alfonso; Cuevas, Carlos A; Dahl-Jensen, Dorthe</p> <p>2016-09-21</p> <p>Reconstructing the past <span class="hlt">variability</span> of Arctic sea <span class="hlt">ice</span> provides an essential context for recent multi-year sea <span class="hlt">ice</span> decline, although few quantitative reconstructions cover the Holocene period prior to the earliest historical records 1,200 years ago. Photochemical recycling of bromine is observed over first-year, or seasonal, sea <span class="hlt">ice</span> in so-called "bromine explosions" and we employ a 1-D chemistry transport model to quantify processes of bromine enrichment over first-year sea <span class="hlt">ice</span> and depositional transport over multi-year sea <span class="hlt">ice</span> and land <span class="hlt">ice</span>. We report bromine enrichment in the Northwest Greenland Eemian NEEM <span class="hlt">ice</span> core since the end of the Eemian interglacial 120,000 years ago, finding the maximum extension of first-year sea <span class="hlt">ice</span> occurred approximately 9,000 years ago during the Holocene climate optimum, when Greenland temperatures were 2 to 3 °C above present values. First-year sea <span class="hlt">ice</span> extent was lowest during the glacial stadials suggesting complete coverage of the Arctic Ocean by multi-year sea <span class="hlt">ice</span>. These findings demonstrate a clear relationship between temperature and first-year sea <span class="hlt">ice</span> extent in the Arctic and suggest multi-year sea <span class="hlt">ice</span> will continue to decline as polar amplification drives Arctic temperatures beyond the 2 °C global average warming target of the recent COP21 Paris climate agreement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCry....8.2313F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCry....8.2313F"><span>Estimating the <span class="hlt">volume</span> of glaciers in the Himalayan-Karakoram region using different methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frey, H.; Machguth, H.; Huss, M.; Huggel, C.; Bajracharya, S.; Bolch, T.; Kulkarni, A.; Linsbauer, A.; Salzmann, N.; Stoffel, M.</p> <p>2014-12-01</p> <p><span class="hlt">Ice</span> <span class="hlt">volume</span> estimates are crucial for assessing water reserves stored in glaciers. Due to its large glacier coverage, such estimates are of particular interest for the Himalayan-Karakoram (HK) region. In this study, different existing methodologies are used to estimate the <span class="hlt">ice</span> reserves: three area-<span class="hlt">volume</span> relations, one slope-dependent <span class="hlt">volume</span> estimation method, and two <span class="hlt">ice</span>-thickness distribution models are applied to a recent, detailed, and complete glacier inventory of the HK region, spanning over the period 2000-2010 and revealing an <span class="hlt">ice</span> coverage of 40 775 km2. An uncertainty and sensitivity assessment is performed to investigate the influence of the observed glacier area and important model parameters on the resulting total <span class="hlt">ice</span> <span class="hlt">volume</span>. Results of the two <span class="hlt">ice</span>-thickness distribution models are validated with local <span class="hlt">ice</span>-thickness measurements at six glaciers. The resulting <span class="hlt">ice</span> <span class="hlt">volumes</span> for the entire HK region range from 2955 to 4737 km3, depending on the approach. This range is lower than most previous estimates. Results from the <span class="hlt">ice</span> thickness distribution models and the slope-dependent thickness estimations agree well with measured local <span class="hlt">ice</span> thicknesses. However, total <span class="hlt">volume</span> estimates from area-related relations are larger than those from other approaches. The study provides evidence on the significant effect of the selected method on results and underlines the importance of a careful and critical evaluation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C52A..03P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C52A..03P"><span>Characterizing Arctic sea <span class="hlt">ice</span> topography and atmospheric form drag using high-resolution <span class="hlt">Ice</span>Bridge data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Petty, A.; Tsamados, M.; Kurtz, N. T.; Farrell, S. L.; Newman, T.; Harbeck, J.; Feltham, D. L.; Richter-Menge, J.</p> <p>2015-12-01</p> <p>Here we present a detailed analysis of Arctic sea <span class="hlt">ice</span> topography using high resolution, three-dimensional surface elevation data from the NASA Operation <span class="hlt">Ice</span>Bridge Airborne Topographic Mapper (ATM) laser altimeter. We derive novel <span class="hlt">ice</span> topography statistics from 2009-2014 across both first-year and multiyear <span class="hlt">ice</span> regimes - including the height, area coverage, orientation and spacing of distinct surface features. The sea <span class="hlt">ice</span> topography exhibits strong spatial <span class="hlt">variability</span>, including increased surface feature (e.g. pressure ridge) height and area coverage within the multi-year <span class="hlt">ice</span> regions. The <span class="hlt">ice</span> topography also shows a strong coastal dependency, with the feature height and area coverage increasing as a function of proximity to the nearest coastline, especially north of Greenland and the Canadian Archipelago. The <span class="hlt">ice</span> topography data have also been used to explicitly calculate atmospheric drag coefficients over Arctic sea <span class="hlt">ice</span>; utilizing existing relationships regarding ridge geometry and their impact on form drag. The results are being used to calibrate the recent drag parameterization scheme included in the sea <span class="hlt">ice</span> model CICE.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMPP24A..03G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMPP24A..03G"><span>Environmental and <span class="hlt">ice</span> <span class="hlt">volume</span> changes based on seismic stratigraphy in Sabrina Coast, East Antarctica: Preliminary results from NBP1402</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gulick, S. P. S.; Fernandez-Vasquez, R. A.; Frederick, B.; Saustrup, S., Sr.; Domack, E. W.; Lavoie, C.; Shevenell, A.; Blankenship, D. D.; Leventer, A.</p> <p>2014-12-01</p> <p>In 2014, the R/V Nathaniel B. Palmer (NBP1402) sailed to a virtually unexplored continental shelf along the Sabrina Coast, East Antarctica. The shelf contains the sedimentary record of environmental and <span class="hlt">ice</span> <span class="hlt">volume</span> changes within the Aurora Subglacial Basin (ASB), which is presently occupied by ~7 m sea level-rise equivalent of <span class="hlt">ice</span>. We acquired 750 km of high-resolution seismic data proximal to the Reynolds Trough and Moscow University <span class="hlt">Ice</span> Shelf glacial systems west of the Dalton <span class="hlt">Ice</span> Tongue using dual 45/45 cu. in. G.I. guns and a 24 ch. streamer with 3.125 m groups providing a vertical resolution of ~3 m simultaneously with CHIRP data. These are the first images of this margin acquired and show a remarkable set of sequence stratigraphic transitions. Crystalline basement is at the seafloor landward and buried seaward with a transition to smoother reflection interface. Reflective sedimentary strata overlie the basement, dip seaward, and are capped by a landward-dipping regional angular unconformity. Above this are a series of transparent seismic facies that, along with the middle to outer shelf seafloor, dip landward towards a shelf-oblique glacial trough. The older, seaward-dipping strata include a deeper series of units that display at least three stratal architectures interpreted to be shelf deltas implying a pre-glacial, fluvial environment within the drainage basin. Above these sequences, the seismic facies transition to surfaces exhibiting significant erosion, small u-shaped valleys, and channel fill sequences, all of which are reminiscent of temperate glacial features. We interpret these sequences as including sub-<span class="hlt">ice</span> tunnel valleys and grounding zone wedges with interspersed non-glacial to pro-glacial deposits. Increasing glaciogenic facies upsection suggests a gradual fluvial to glacial transition and increasing glacial extent with time. The subsequent transition to <span class="hlt">ice</span> sheets is marked by erosion to basement landward and the angular unconformity seaward</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170008477','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170008477"><span>Improving Our Understanding of Antarctic Sea <span class="hlt">Ice</span> with NASA's Operation <span class="hlt">Ice</span>Bridge and the Upcoming ICESat-2 Mission</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Petty, Alek A.; Markus, Thorsten; Kurtz, Nathan T.</p> <p>2017-01-01</p> <p>Antarctic sea <span class="hlt">ice</span> is a crucial component of the global climate system. Rapid sea <span class="hlt">ice</span> production regimes around Antarctica feed the lower branch of the Southern Ocean overturning circulation through intense brine rejection and the formation of Antarctic Bottom Water (e.g., Orsi et al. 1999; Jacobs 2004), while the northward transport and subsequent melt of Antarctic sea <span class="hlt">ice</span> drives the upper branch of the overturning circulation through freshwater input (Abernathy et al. 2016). Wind-driven trends in Antarctic sea <span class="hlt">ice</span> (Holland Kwok 2012) have likely increased the transport of freshwater away from the Antarctic coastline, significantly altering the salinity distribution of the Southern Ocean (Haumann et al. 2016). Conversely, weaker sea <span class="hlt">ice</span> production and the lack of shelf water formation over the Amundsen and Bellingshausen shelf seas promote intrusion of warm Circumpolar Deep Water onto the continental shelf and the ocean-driven melting of several <span class="hlt">ice</span> shelves fringing the West Antarctic <span class="hlt">Ice</span> Sheet (e.g., Jacobs et al. 2011; Pritchard et al. 2012; Dutrieux et al. 2014). Sea <span class="hlt">ice</span> conditions around Antarctica are also increasingly considered an important factor impacting local atmospheric conditions and the surface melting of Antarctic <span class="hlt">ice</span> shelves (e.g., Scambos et al. 2017). Sea <span class="hlt">ice</span> formation around Antarctica is responsive to the strong regional <span class="hlt">variability</span> in atmospheric forcing present around Antarctica, driving this bimodal <span class="hlt">variability</span> in the behavior and properties of the underlying shelf seas (e.g., Petty et al. 2012; Petty et al. 2014).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70101982','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70101982"><span>Weakening of <span class="hlt">ice</span> by magnesium perchlorate hydrate</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lenferinka, Hendrick J.; Durhama, William B.; Sternb, Laura A.; Patharec, Asmin V.</p> <p>2013-01-01</p> <p>We show that perchlorate hydrates, which have been detected at high circumpolar martian latitudes, have a dramatic effect upon the rheological behavior of polycrystalline water <span class="hlt">ice</span> under conditions applicable to the North Polar Layered Deposits (NPLD). We conducted subsolidus creep tests on mixtures of <span class="hlt">ice</span> and magnesium perchlorate hydrate, Mg(ClO4)2·6H2O (MP6), of 0.02, 0.05, 0.10, and 0.47 <span class="hlt">volume</span> fraction MP6. We found these mixtures to be increasingly weak with increasing MP6 content. For mixtures with ⩽0.10 <span class="hlt">volume</span> fraction MP6, we resolved a stress exponent of n ≈ 2 at low stresses transitioning to n ≈ 4 above 10 MPa. Scanning electron microscopy of deformed specimens revealed MP6 to be distributed as an interconnected film between <span class="hlt">ice</span> grains. These results suggest that grain boundary sliding (GBS) may be enhanced with respect to pure <span class="hlt">ice</span>. As the enhancement of GBS is expected in polycrystalline aggregates containing a few percent melt or otherwise weak material distributed along grain boundaries, the observed n ≈ 2 is consistent with the mutual accommodation of basal slip and GBS. If <span class="hlt">ice</span> containing trace concentrations of MP6 is also much weaker than pure <span class="hlt">ice</span> at low stresses, flow in the NPLD could be significantly enhanced, particularly at the warmer basal temperatures associated with higher martian obliquities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24134671','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24134671"><span><span class="hlt">Volume</span> quantification by contrast-enhanced ultrasound: an in-vitro comparison with true <span class="hlt">volumes</span> and thermodilution.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Herold, Ingeborg H F; Russo, Gianna; Mischi, Massimo; Houthuizen, Patrick; Saidov, Tamerlan; van het Veer, Marcel; van Assen, Hans C; Korsten, Hendrikus H M</p> <p>2013-10-17</p> <p>Contrast-enhanced ultrasound (CEUS) has recently been proposed as a minimally- invasive, alternative method for blood <span class="hlt">volume</span> measurement. This study aims at comparing the accuracy of CEUS and the classical thermodilution techniques for <span class="hlt">volume</span> assessment in an in-vitro set-up. The in-vitro set-up consisted of a <span class="hlt">variable</span> network between an inflow and outflow tube and a roller pump. The inflow and outflow tubes were insonified with an ultrasound array transducer and a thermistor was placed in each tube. Indicator dilution curves were made by injecting indicator which consisted of an ultrasound-contrast-agent diluted in <span class="hlt">ice</span>-cold saline. Both acoustic intensity- and thermo-dilution curves were used to calculate the indicator mean transit time between the inflow and outflow tube. The <span class="hlt">volumes</span> were derived by multiplying the estimated mean transit time by the flow rate. We compared the <span class="hlt">volumes</span> measured by CEUS with the true <span class="hlt">volumes</span> of the <span class="hlt">variable</span> network and those measured by thermodilution by Bland-Altman and intraclass-correlation analysis. The measurements by CEUS and thermodilution showed a very strong correlation (rs = 0.94) with a modest <span class="hlt">volume</span> underestimation by CEUS of -40 ± 28 mL and an overestimation of 84 ± 62 mL by thermodilution compared with the true <span class="hlt">volumes</span>. Both CEUS and thermodilution showed a high statistically significant correlation with the true <span class="hlt">volume</span> (rs = 0.97 (95% CI, 0.95 - 0.98; P<0.0001) and rs = 0.96 (95% CI, 0.94 - 0.98; P<0.0001, respectively). CEUS <span class="hlt">volume</span> estimation provides a strong correlation with both the true <span class="hlt">volumes</span> in-vitro and <span class="hlt">volume</span> estimation by thermodilution. It may therefore represent an interesting alternative to the standard, invasive thermodilution technique.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RvGeo..56..142P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RvGeo..56..142P"><span>Ocean Tide Influences on the Antarctic and Greenland <span class="hlt">Ice</span> Sheets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Padman, Laurie; Siegfried, Matthew R.; Fricker, Helen A.</p> <p>2018-03-01</p> <p>Ocean tides are the main source of high-frequency <span class="hlt">variability</span> 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 mass balance and dynamics. In this review, we summarize in situ and satellite-based measurements of the tidal response of <span class="hlt">ice</span> shelves and grounded <span class="hlt">ice</span>, and spatial <span class="hlt">variability</span> of ocean tide heights and currents around the <span class="hlt">ice</span> sheets. We review sensitivity of tide heights and currents as ocean geometry responds to variations in sea level, <span class="hlt">ice</span> shelf thickness, and <span class="hlt">ice</span> sheet mass and extent. We then describe coupled <span class="hlt">ice</span>-ocean models and analytical glacier models that quantify the effect of ocean tides on lower-frequency <span class="hlt">ice</span> sheet mass loss and motion. We suggest new observations and model developments to improve the representation of tides in coupled models that are used to predict future <span class="hlt">ice</span> sheet mass loss and the associated contribution to sea level change. The most critical need is for new data to improve maps of bathymetry, <span class="hlt">ice</span> shelf draft, spatial <span class="hlt">variability</span> of the drag coefficient at the <span class="hlt">ice</span>-ocean interface, and higher-resolution models with improved representation of tidal energy sinks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060039967&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060039967&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar"><span>Fram Strait sea <span class="hlt">ice</span> outflow</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kwok, R.; Cunningham, G. F.; Pang, S. S.</p> <p>2004-01-01</p> <p>We summarize 24 years of <span class="hlt">ice</span> export estimates and examine, over a 9-year record, the associated <span class="hlt">variability</span> in the time-varying upward-looking sonar (ULS) thickness distributions of the Fram Strait. A more thorough assessment of the PMW (passive microwave) <span class="hlt">ice</span> motion with 5 years of synthetic aperture radar (SAR)observations shows the uncertainties to be consistent with that found by Kwok and Rothrock [1999], giving greater confidence to the record of <span class="hlt">ice</span> flux calculations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G31C0929H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G31C0929H"><span>Long term <span class="hlt">ice</span> sheet mass change rates and inter-annual <span class="hlt">variability</span> from GRACE gravimetry.</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.</p> <p>2017-12-01</p> <p>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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> velocity. Interannual variations in <span class="hlt">ice</span> mass are of particular interest since they can directly link changes in <span class="hlt">ice</span> 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 <span class="hlt">ice</span> sheet. We present GRACE observations of the 2013-2014 slowdown in mass loss of the Greenland <span class="hlt">ice</span> sheet, which was concentrated in specific parts of the <span class="hlt">ice</span> sheet and in certain months of the year. We also discuss estimating the relative importance of climate factors that control <span class="hlt">ice</span> mass balance, as a function of location of the glacier/<span class="hlt">ice</span> cap as well as the spatial variation within an <span class="hlt">ice</span> sheet by comparing gravimetry with observations of surface air temperature, ocean temperature, etc. as well as model data from climate reanalysis products.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990JGR....9513411C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990JGR....9513411C"><span>Arctic multiyear <span class="hlt">ice</span> classification and summer <span class="hlt">ice</span> cover using passive microwave satellite data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Comiso, J. C.</p> <p>1990-08-01</p> <p>The ability to classify and monitor Arctic multiyear sea <span class="hlt">ice</span> cover using multispectral passive microwave data is studied. Sea <span class="hlt">ice</span> concentration maps during several summer minima have been analyzed to obtain estimates of <span class="hlt">ice</span> surviving the summer. The results are compared with multiyear <span class="hlt">ice</span> concentrations derived from data the following winter, using an algorithm that assumes a certain emissivity for multiyear <span class="hlt">ice</span>. The multiyear <span class="hlt">ice</span> cover inferred from the winter data is approximately 25 to 40% less than the summer <span class="hlt">ice</span> cover minimum, suggesting that even during winter when the emissivity of sea <span class="hlt">ice</span> is most stable, passive microwave data may account for only a fraction of the total multiyear <span class="hlt">ice</span> cover. The difference of about 2×106 km2 is considerably more than estimates of advection through Fram Strait during the intervening period. It appears that as in the Antarctic, some multiyear <span class="hlt">ice</span> floes in the Arctic, especially those near the summer marginal <span class="hlt">ice</span> zone, have first-year <span class="hlt">ice</span> or intermediate signatures in the subsequent winter. A likely mechanism for this is the intrusion of seawater into the snow-<span class="hlt">ice</span> interface, which often occurs near the marginal <span class="hlt">ice</span> zone or in areas where snow load is heavy. Spatial variations in melt and melt ponding effects also contribute to the complexity of the microwave emissivity of multiyear <span class="hlt">ice</span>. Hence the multiyear <span class="hlt">ice</span> data should be studied in conjunction with the previous summer <span class="hlt">ice</span> data to obtain a more complete characterization of the state of the Arctic <span class="hlt">ice</span> cover. The total extent and actual areas of the summertime Arctic pack <span class="hlt">ice</span> were estimated to be 8.4×106 km2 and 6.2×106 km2, respectively, and exhibit small interannual <span class="hlt">variability</span> during the years 1979 through 1985, suggesting a relatively stable <span class="hlt">ice</span> cover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25119027','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25119027"><span>Abrupt glacial climate shifts controlled by <span class="hlt">ice</span> sheet changes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Xu; Lohmann, Gerrit; Knorr, Gregor; Purcell, Conor</p> <p>2014-08-21</p> <p>During glacial periods of the Late Pleistocene, an abundance of proxy data demonstrates the existence of large and repeated millennial-scale warming episodes, known as Dansgaard-Oeschger (DO) events. This ubiquitous feature of rapid glacial climate change can be extended back as far as 800,000 years before present (BP) in the <span class="hlt">ice</span> core record, and has drawn broad attention within the science and policy-making communities alike. Many studies have been dedicated to investigating the underlying causes of these changes, but no coherent mechanism has yet been identified. Here we show, by using a comprehensive fully coupled model, that gradual changes in the height of the Northern Hemisphere <span class="hlt">ice</span> sheets (NHISs) can alter the coupled atmosphere-ocean system and cause rapid glacial climate shifts closely resembling DO events. The simulated global climate responses--including abrupt warming in the North Atlantic, a northward shift of the tropical rainbelts, and Southern Hemisphere cooling related to the bipolar seesaw--are generally consistent with empirical evidence. As a result of the coexistence of two glacial ocean circulation states at intermediate heights of the <span class="hlt">ice</span> sheets, minor changes in the height of the NHISs and the amount of atmospheric CO2 can trigger the rapid climate transitions via a local positive atmosphere-ocean-sea-<span class="hlt">ice</span> feedback in the North Atlantic. Our results, although based on a single model, thus provide a coherent concept for understanding the recorded millennial-scale <span class="hlt">variability</span> and abrupt climate changes in the coupled atmosphere-ocean system, as well as their linkages to the <span class="hlt">volume</span> of the intermediate <span class="hlt">ice</span> sheets during glacials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019230','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019230"><span>The physical basis of glacier <span class="hlt">volume</span>-area scaling</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bahr, D.B.; Meier, M.F.; Peckham, S.D.</p> <p>1997-01-01</p> <p><span class="hlt">Ice</span> <span class="hlt">volumes</span> are known for only a few of the roughly 160,000 glaciers worldwide but are important components of many climate and sea level studies which require water flux estimates. A scaling analysis of the mass and momentum conservation equations shows that glacier <span class="hlt">volumes</span> can be related by a power law to more easily observed glacier surface areas. The relationship requires four closure choices for the scaling behavior of glacier widths, slopes, side drag and mass balance. Reasonable closures predict a <span class="hlt">volume</span>-area scaling exponent which is consistent with observations, giving a physical and practical basis for estimating <span class="hlt">ice</span> <span class="hlt">volumes</span>. Glacier <span class="hlt">volume</span> is insensitive to perturbations in the mass balance scaling, but changes in average accumulation area ratios reflect significant changes in the scaling of both mass balance and <span class="hlt">ice</span> <span class="hlt">volume</span>. Copyright 1997 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.1907W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1907W"><span>Estimation of Antarctic Land-Fast Sea <span class="hlt">Ice</span> Algal Biomass and Snow Thickness From Under-<span class="hlt">Ice</span> Radiance Spectra in Two Contrasting Areas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wongpan, P.; Meiners, K. M.; Langhorne, P. J.; Heil, P.; Smith, I. J.; Leonard, G. H.; Massom, R. A.; Clementson, L. A.; Haskell, T. G.</p> <p>2018-03-01</p> <p>Fast <span class="hlt">ice</span> is an important component of Antarctic coastal marine ecosystems, providing a prolific habitat for <span class="hlt">ice</span> algal communities. This work examines the relationships between normalized difference indices (NDI) calculated from under-<span class="hlt">ice</span> radiance measurements and sea <span class="hlt">ice</span> algal biomass and snow thickness for Antarctic fast <span class="hlt">ice</span>. While this technique has been calibrated to assess biomass in Arctic fast <span class="hlt">ice</span> and pack <span class="hlt">ice</span>, as well as Antarctic pack <span class="hlt">ice</span>, relationships are currently lacking for Antarctic fast <span class="hlt">ice</span> characterized by bottom <span class="hlt">ice</span> algae communities with high algal biomass. We analyze measurements along transects at two contrasting Antarctic fast <span class="hlt">ice</span> sites in terms of platelet <span class="hlt">ice</span> presence: near and distant from an <span class="hlt">ice</span> shelf, i.e., in McMurdo Sound and off Davis Station, respectively. Snow and <span class="hlt">ice</span> thickness, and <span class="hlt">ice</span> salinity and temperature measurements support our paired in situ optical and biological measurements. Analyses show that NDI wavelength pairs near the first chlorophyll a (chl a) absorption peak (≈440 nm) explain up to 70% of the total <span class="hlt">variability</span> in algal biomass. Eighty-eight percent of snow thickness <span class="hlt">variability</span> is explained using an NDI with a wavelength pair of 648 and 567 nm. Accounting for pigment packaging effects by including the ratio of chl a-specific absorption coefficients improved the NDI-based algal biomass estimation only slightly. Our new observation-based algorithms can be used to estimate Antarctic fast <span class="hlt">ice</span> algal biomass and snow thickness noninvasively, for example, by using moored sensors (time series) or mapping their spatial distributions using underwater vehicles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41E..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41E..01H"><span><span class="hlt">Ice</span> shelf structure and stability: Larsen C <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>Hubbard, B. P.; Ashmore, D.; Bevan, S. L.; Booth, A. D.; Holland, P.; Jansen, D.; Kuipers Munneke, P.; Kulessa, B.; Luckman, A. J.; Sevestre, H.; O'Leary, M.</p> <p>2017-12-01</p> <p>We report on recent empirical investigations of the internal structure and stability (or otherwise) of Larsen C <span class="hlt">Ice</span> Shelf (LCIS), Antarctica, focusing on research carried out for the MIDAS research project between 2014 and 2017. Borehole- and surface geophysics-based fieldwork carried out in austral springs 2014 and 2015 revealed that ephemeral surface ponds, preferentially located within the major inlets within the northern sector of the <span class="hlt">ice</span> shelf, result in the formation of several tens of metres of (relatively dense) subsurface <span class="hlt">ice</span> within what would otherwise have been a progressively densifying snow and firn column. Five boreholes were drilled throughout the sector and logged by optical televiewer, showing this refrozen <span class="hlt">ice</span> to be extensive and of <span class="hlt">variable</span> composition depending on its process of formation. Mapping the depth-distribution of the resulting <span class="hlt">ice</span> types and associating each with a simple flow-line model of <span class="hlt">ice</span> motion and accumulation indicates that this area of LCIS has experienced substantial melting for some centuries but that surface ponding has only occurred in recent decades, possibly restricted to the past 20 years. We also present near-surface temperature data that reveal surprising temporal patterns in foehn wind activity and intensity. Finally, we report on the geometrical extension and widening of a rift that was responsible for calving a 5,800 km^2 iceberg from the LCIS in July 2017. The nature of rift propagation through `suture' <span class="hlt">ice</span> bands, widely considered to be composed of marine <span class="hlt">ice</span>, is contrasted with that of its propagation through meteoric <span class="hlt">ice</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C34B..05H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C34B..05H"><span>Observing Radiative Properties of a Thinner, Seasonal Arctic <span class="hlt">Ice</span> Pack</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hudson, S. R.; Nicolaus, M.; Granskog, M.; Gerland, S.; Wang, C.</p> <p>2011-12-01</p> <p>The Arctic is coming to be dominated by young <span class="hlt">ice</span>, much of it seasonal. Many of our observations of the radiative properties of sea <span class="hlt">ice</span> come from drifting stations on thick, multi-year <span class="hlt">ice</span>. To better understand the Arctic climate system in a warmer world, we need more data about the radiative properties and their seasonal and spatial <span class="hlt">variability</span> on thinner, younger <span class="hlt">ice</span>. Since this younger <span class="hlt">ice</span> is not always thick enough to support lengthy drifting stations, there is a need for new technologies to help us get optical measurements on seasonal <span class="hlt">ice</span>. One challenge is obtaining seasonal data on <span class="hlt">ice</span> that is too weak to support even a ship-based camp, and especially to have these observations extend well into the melt season. For these situations, we have developed a spectral radiation monitoring buoy that can be deployed during a one-day <span class="hlt">ice</span> station, and that can then autonomously observe the spectral albedo and transmittance of the sea <span class="hlt">ice</span>, transmitting all data in near real time by satellite, until the buoy melts out. Similar installations at manned or regularly visited sites have provided good data, with surprisingly few data-quality problems due to frost, precipitation, or tilting. The buoys consist of 3 spectral radiometers, covering wavelengths 350 to 800 nm, and a datalogger with an Irridium modem. The datalogger and necessary batteries are inside a sealed housing which is frozen into a hole drilled in the <span class="hlt">ice</span>. Arms extend from both the top and bottom of the housing, holding sensors that measure incident, reflected, and transmitted spectra. The under-<span class="hlt">ice</span> radiometer is equipped with a bioshutter to avoid algal growth on the sensor. They will be deployed alongside <span class="hlt">ice</span> mass balance buoys, providing data about the physical development of the <span class="hlt">ice</span> and snow, as well as position. While the buoys provide an excellent record of diurnal, synoptic, and seasonal <span class="hlt">variability</span>, they are fixed to one location in the <span class="hlt">ice</span>, so other methods are still needed for measuring the spatial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140010420','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140010420"><span>Sea <span class="hlt">Ice</span> Thickness, Freeboard, and Snow Depth products from Operation <span class="hlt">Ice</span>Bridge Airborne Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kurtz, N. T.; Farrell, S. L.; Studinger, M.; Galin, N.; Harbeck, J. P.; Lindsay, R.; Onana, V. D.; Panzer, B.; Sonntag, J. G.</p> <p>2013-01-01</p> <p>The study of sea <span class="hlt">ice</span> using airborne remote sensing platforms provides unique capabilities to measure a wide variety of sea <span class="hlt">ice</span> properties. These measurements are useful for a variety of topics including model evaluation and improvement, assessment of satellite retrievals, and incorporation into climate data records for analysis of interannual <span class="hlt">variability</span> and long-term trends in sea <span class="hlt">ice</span> properties. In this paper we describe methods for the retrieval of sea <span class="hlt">ice</span> thickness, freeboard, and snow depth using data from a multisensor suite of instruments on NASA's Operation <span class="hlt">Ice</span>Bridge airborne campaign. We assess the consistency of the results through comparison with independent data sets that demonstrate that the <span class="hlt">Ice</span>Bridge products are capable of providing a reliable record of snow depth and sea <span class="hlt">ice</span> thickness. We explore the impact of inter-campaign instrument changes and associated algorithm adaptations as well as the applicability of the adapted algorithms to the ongoing <span class="hlt">Ice</span>Bridge mission. The uncertainties associated with the retrieval methods are determined and placed in the context of their impact on the retrieved sea <span class="hlt">ice</span> thickness. Lastly, we present results for the 2009 and 2010 <span class="hlt">Ice</span>Bridge campaigns, which are currently available in product form via the National Snow and <span class="hlt">Ice</span> Data Center</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C41A0684N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C41A0684N"><span>CryoSat-2 Processing and Model Interpretation of Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">Volume</span> Changes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nilsson, J.; Gardner, A. S.; Sandberg Sorensen, L.</p> <p>2015-12-01</p> <p>CryoSat-2 was launched in late 2010 tasked with monitoring the changes of the Earth's land and sea <span class="hlt">ice</span>. It carries a novel radar altimeter allowing the satellite to monitor changes in highly complex terrain, such as smaller <span class="hlt">ice</span> caps, glaciers and the marginal areas of the <span class="hlt">ice</span> sheets. Here we present on the development and validation of an independent elevation retrieval processing chain and respective elevation changes based on ESA's L1B data. Overall we find large improvement in both accuracy and precision over Greenland relative to ESA's L2 product when comparing against both airborne data and crossover analysis. The seasonal component and spatial sampling of the surface elevation changes where also compared against ICESat derived changes from 2003-2009. The comparison showed good agreement between the to product on a local scale. However, a global sampling bias was detected in the seasonal signal due to the clustering of CryoSat-2 data in higher elevation areas. The retrieval processing chain presented here does not correct for changes in surface scattering conditions and appears to be insensitive to the 2012 melt event (Nilsson et al., 2015). This in contrast to the elevation changes derived from ESA's L2 elevation product, which where found to be sensitive to the effects of the melt event. The positive elevation bias created by the event introduced a discrepancy between the two products with a magnitude of roughly 90 km3/year. This difference can directly be attributed to the differences in retracking procedure pointing to the importance of the retracking of the radar waveforms for altimetric <span class="hlt">volume</span> change studies. Greenland 2012 melt event effects on CryoSat-2 radar altimetry./ Nilsson, Johan; Vallelonga, Paul Travis; Simonsen, Sebastian Bjerregaard; Sørensen, Louise Sandberg; Forsberg, René; Dahl-Jensen, Dorthe; Hirabayashi, Motohiro; Goto-Azuma, Kumiko; Hvidberg, Christine S.; Kjær, Helle A.; Satow, Kazuhide.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21B1124W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21B1124W"><span>Synthesis of User Needs for Arctic Sea <span class="hlt">Ice</span> Predictions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wiggins, H. V.; Turner-Bogren, E. J.; Sheffield Guy, L.</p> <p>2017-12-01</p> <p>Forecasting Arctic sea <span class="hlt">ice</span> on sub-seasonal to seasonal scales in a changing Arctic is of interest to a diverse range of stakeholders. However, sea <span class="hlt">ice</span> forecasting is still challenging due to high <span class="hlt">variability</span> in weather and ocean conditions and limits to prediction capabilities; the science needs for observations and modeling are extensive. At a time of challenged science funding, one way to prioritize sea <span class="hlt">ice</span> prediction efforts is to examine the information needs of various stakeholder groups. This poster will present a summary and synthesis of existing surveys, reports, and other literature that examines user needs for sea <span class="hlt">ice</span> predictions. The synthesis will include lessons learned from the Sea <span class="hlt">Ice</span> Prediction Network (a collaborative, multi-agency-funded project focused on seasonal Arctic sea <span class="hlt">ice</span> predictions), the Sea <span class="hlt">Ice</span> for Walrus Outlook (a resource for Alaska Native subsistence hunters and coastal communities, that provides reports on weather and sea <span class="hlt">ice</span> conditions), and other efforts. The poster will specifically compare the scales and <span class="hlt">variables</span> of sea <span class="hlt">ice</span> forecasts currently available, as compared to what information is requested by various user groups.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070038189','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070038189"><span>Physical and Radiative Characteristics and Long Term <span class="hlt">Variability</span> of the Okhotsk Sea <span class="hlt">Ice</span> Cover</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nishio, Fumihiko; Comiso, Josefino C.; Gersten, Robert; Nakayama, Masashige; Ukita, Jinro; Gasiewski, Al; Stanko, Boba; Naoki, Kazuhiro</p> <p>2007-01-01</p> <p>Much of what we know about the large scale characteristics of the Okhotsk Sea <span class="hlt">ice</span> cover comes from <span class="hlt">ice</span> concentration maps derived from passive microwave data. To understand what these satellite data represents in a highly divergent and rapidly changing environment like the Okhotsk Sea, we analyzed concurrent satellite, aircraft, and ship data and characterized the sea <span class="hlt">ice</span> cover at different scales from meters to tens of kilometers. Through comparative analysis of surface features using co-registered data from visible, infrared and microwave channels we evaluated how the general radiative and physical characteristics of the <span class="hlt">ice</span> cover changes as well as quantify the distribution of different <span class="hlt">ice</span> types in the region. <span class="hlt">Ice</span> concentration maps from AMSR-E using the standard sets of channels, and also only the 89 GHz channel for optimal resolution, are compared with aircraft and high resolution visible data and while the standard set provides consistent results, the 89 GHz provides the means to observe mesoscale patterns and some unique features of the <span class="hlt">ice</span> cover. Analysis of MODIS data reveals that thick <span class="hlt">ice</span> types represents about 37% of the <span class="hlt">ice</span> cover indicating that young and new <span class="hlt">ice</span> represent a large fraction of the lice cover that averages about 90% <span class="hlt">ice</span> concentration, according to passive microwave data. A rapid decline of -9% and -12 % per decade is observed suggesting warming signals but further studies are required because of aforementioned characteristics and because the length of the <span class="hlt">ice</span> season is decreasing by only 2 to 4 days per decade.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037527','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037527"><span>Quaternary Sea-<span class="hlt">ice</span> history in the Arctic Ocean based on a new Ostracode sea-<span class="hlt">ice</span> proxy</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Cronin, T. M.; Gemery, L.; Briggs, W.M.; Jakobsson, M.; Polyak, L.; Brouwers, E.M.</p> <p>2010-01-01</p> <p>Paleo-sea-<span class="hlt">ice</span> history in the Arctic Ocean was reconstructed using the sea-<span class="hlt">ice</span> dwelling ostracode Acetabulastoma arcticum from late Quaternary sediments from the Mendeleyev, Lomonosov, and Gakkel Ridges, the Morris Jesup Rise and the Yermak Plateau. Results suggest intermittently high levels of perennial sea <span class="hlt">ice</span> in the central Arctic Ocean during Marine Isotope Stage (MIS) 3 (25-45 ka), minimal sea <span class="hlt">ice</span> during the last deglacial (16-11 ka) and early Holocene thermal maximum (11-5 ka) and increasing sea <span class="hlt">ice</span> during the mid-to-late Holocene (5-0 ka). Sediment core records from the Iceland and Rockall Plateaus show that perennial sea <span class="hlt">ice</span> existed in these regions only during glacial intervals MIS 2, 4, and 6. These results show that sea <span class="hlt">ice</span> exhibits complex temporal and spatial <span class="hlt">variability</span> during different climatic regimes and that the development of modern perennial sea <span class="hlt">ice</span> may be a relatively recent phenomenon. ?? 2010.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.4124D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.4124D"><span>Summer Drivers of Atmospheric <span class="hlt">Variability</span> Affecting <span class="hlt">Ice</span> Shelf Thinning in the Amundsen Sea Embayment, West Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deb, Pranab; Orr, Andrew; Bromwich, David H.; Nicolas, Julien P.; Turner, John; Hosking, J. Scott</p> <p>2018-05-01</p> <p>Satellite data and a 35-year hindcast of the Amundsen Sea Embayment summer climate using the Weather Research and Forecasting model are used to understand how regional and large-scale atmospheric <span class="hlt">variability</span> affects thinning of <span class="hlt">ice</span> shelves in this sector of West Antarctica by melting from above and below (linked to intrusions of warm water caused by anomalous westerlies over the continental shelf edge). El Niño episodes are associated with an increase in surface melt but do not have a statistically significant impact on westerly winds over the continental shelf edge. The location of the Amundsen Sea Low and the polarity of the Southern Annular Mode (SAM) have negligible impact on surface melting, although a positive SAM and eastward shift of the Amundsen Sea Low cause anomalous westerlies over the continental shelf edge. The projected future increase in El Niño episodes and positive SAM could therefore increase the risk of disintegration of West Antarctic <span class="hlt">ice</span> shelves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..188....1T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..188....1T"><span><span class="hlt">Ice</span> core records of climate <span class="hlt">variability</span> on the Third Pole with emphasis on the Guliya <span class="hlt">ice</span> cap, western Kunlun Mountains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thompson, Lonnie G.; Yao, Tandong; Davis, Mary E.; Mosley-Thompson, Ellen; Wu, Guangjian; Porter, Stacy E.; Xu, Baiqing; Lin, Ping-Nan; Wang, Ninglian; Beaudon, Emilie; Duan, Keqin; Sierra-Hernández, M. Roxana; Kenny, Donald V.</p> <p>2018-05-01</p> <p>Records of recent climate from <span class="hlt">ice</span> cores drilled in 2015 on the Guliya <span class="hlt">ice</span> cap in the western Kunlun Mountains of the Tibetan Plateau, which with the Himalaya comprises the Third Pole (TP), demonstrate that this region has become warmer and moister since at least the middle of the 19th century. Decadal-scale linkages are suggested between <span class="hlt">ice</span> core temperature and snowfall proxies, North Atlantic oceanic and atmospheric processes, Arctic temperatures, and Indian summer monsoon intensity. Correlations between annual-scale oxygen isotopic ratios (δ18O) and tropical western Pacific and Indian Ocean sea surface temperatures are also demonstrated. Comparisons of climate records during the last millennium from <span class="hlt">ice</span> cores acquired throughout the TP illustrate centennial-scale differences between monsoon and westerlies dominated regions. Among these records, Guliya shows the highest rate of warming since the end of the Little <span class="hlt">Ice</span> Age, but δ18O data over the last millennium from TP <span class="hlt">ice</span> cores support findings that elevation-dependent warming is most pronounced in the Himalaya. This, along with the decreasing precipitation rates in the Himalaya region, is having detrimental effects on the cryosphere. Although satellite monitoring of glaciers on the TP indicates changes in surface area, only a few have been directly monitored for mass balance and ablation from the surface. This type of ground-based study is essential to obtain a better understanding of the rate of <span class="hlt">ice</span> shrinkage on the TP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.4193S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.4193S"><span>Trend analysis of Arctic sea <span class="hlt">ice</span> extent</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Silva, M. E.; Barbosa, S. M.; Antunes, Luís; Rocha, Conceição</p> <p>2009-04-01</p> <p>The extent of Arctic sea <span class="hlt">ice</span> is a fundamental parameter of Arctic climate <span class="hlt">variability</span>. In the context of climate change, the area covered by <span class="hlt">ice</span> in the Arctic is a particularly useful indicator of recent changes in the Arctic environment. Climate models are in near universal agreement that Arctic sea <span class="hlt">ice</span> extent will decline through the 21st century as a consequence of global warming and many studies predict a <span class="hlt">ice</span> free Arctic as soon as 2012. Time series of satellite passive microwave observations allow to assess the temporal changes in the extent of Arctic sea <span class="hlt">ice</span>. Much of the analysis of the <span class="hlt">ice</span> extent time series, as in most climate studies from observational data, have been focussed on the computation of deterministic linear trends by ordinary least squares. However, many different processes, including deterministic, unit root and long-range dependent processes can engender trend like features in a time series. Several parametric tests have been developed, mainly in econometrics, to discriminate between stationarity (no trend), deterministic trend and stochastic trends. Here, these tests are applied in the trend analysis of the sea <span class="hlt">ice</span> extent time series available at National Snow and <span class="hlt">Ice</span> Data Center. The parametric stationary tests, Augmented Dickey-Fuller (ADF), Phillips-Perron (PP) and the KPSS, do not support an overall deterministic trend in the time series of Arctic sea <span class="hlt">ice</span> extent. Therefore, alternative parametrizations such as long-range dependence should be considered for characterising long-term Arctic sea <span class="hlt">ice</span> <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070016598&hterms=sea+ice+albedo&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dsea%2Bice%2Balbedo','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070016598&hterms=sea+ice+albedo&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dsea%2Bice%2Balbedo"><span>Observational Evidence of a Hemispheric-wide <span class="hlt">Ice</span>-ocean Albedo Feedback Effect on Antarctic Sea-<span class="hlt">ice</span> Decay</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nihashi, Sohey; Cavalieri, Donald J.</p> <p>2007-01-01</p> <p>The effect of <span class="hlt">ice</span>-ocean albedo feedback (a kind of <span class="hlt">ice</span>-albedo feedback) on sea-<span class="hlt">ice</span> decay is demonstrated over the Antarctic sea-<span class="hlt">ice</span> zone from an analysis of satellite-derived hemispheric sea <span class="hlt">ice</span> concentration and European Centre for Medium-Range Weather Forecasts (ERA-40) atmospheric data for the period 1979-2001. Sea <span class="hlt">ice</span> concentration in December (time of most active melt) correlates better with the meridional component of the wind-forced <span class="hlt">ice</span> drift (MID) in November (beginning of the melt season) than the MID in December. This 1 month lagged correlation is observed in most of the Antarctic sea-<span class="hlt">ice</span> covered ocean. Daily time series of <span class="hlt">ice</span> , concentration show that the <span class="hlt">ice</span> concentration anomaly increases toward the time of maximum sea-<span class="hlt">ice</span> melt. These findings can be explained by the following positive feedback effect: once <span class="hlt">ice</span> concentration decreases (increases) at the beginning of the melt season, solar heating of the upper ocean through the increased (decreased) open water fraction is enhanced (reduced), leading to (suppressing) a further decrease in <span class="hlt">ice</span> concentration by the oceanic heat. Results obtained fi-om a simple <span class="hlt">ice</span>-ocean coupled model also support our interpretation of the observational results. This positive feedback mechanism explains in part the large interannual <span class="hlt">variability</span> of the sea-<span class="hlt">ice</span> cover in summer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850017732&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=19850017732&hterms=BALANCE+SHEET&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DBALANCE%2BSHEET"><span>Greenland <span class="hlt">Ice</span> Sheet Mass Balance</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Reeh, N.</p> <p>1984-01-01</p> <p>Mass balance equation for glaciers; areal distribution and <span class="hlt">ice</span> <span class="hlt">volumes</span>; estimates of actual mass balance; loss by calving of icebergs; hydrological budget for Greenland; and temporal variations of Greenland mass balance are examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11..789S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11..789S"><span>Interactions between Antarctic sea <span class="hlt">ice</span> and large-scale atmospheric modes in CMIP5 models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schroeter, Serena; Hobbs, Will; Bindoff, Nathaniel L.</p> <p>2017-03-01</p> <p>The response of Antarctic sea <span class="hlt">ice</span> to large-scale patterns of atmospheric <span class="hlt">variability</span> varies according to sea <span class="hlt">ice</span> sector and season. In this study, interannual atmosphere-sea <span class="hlt">ice</span> interactions were explored using observations and reanalysis data, and compared with simulated interactions by models in the Coupled Model Intercomparison Project Phase 5 (CMIP5). Simulated relationships between atmospheric <span class="hlt">variability</span> and sea <span class="hlt">ice</span> <span class="hlt">variability</span> generally reproduced the observed relationships, though more closely during the season of sea <span class="hlt">ice</span> advance than the season of sea <span class="hlt">ice</span> retreat. Atmospheric influence on sea <span class="hlt">ice</span> is known to be strongest during advance, and it appears that models are able to capture the dominance of the atmosphere during advance. Simulations of ocean-atmosphere-sea <span class="hlt">ice</span> interactions during retreat, however, require further investigation. A large proportion of model ensemble members overestimated the relative importance of the Southern Annular Mode (SAM) compared with other modes of high southern latitude climate, while the influence of tropical forcing was underestimated. This result emerged particularly strongly during the season of sea <span class="hlt">ice</span> retreat. The zonal patterns of the SAM in many models and its exaggerated influence on sea <span class="hlt">ice</span> overwhelm the comparatively underestimated meridional influence, suggesting that simulated sea <span class="hlt">ice</span> <span class="hlt">variability</span> would become more zonally symmetric as a result. Across the seasons of sea <span class="hlt">ice</span> advance and retreat, three of the five sectors did not reveal a strong relationship with a pattern of large-scale atmospheric <span class="hlt">variability</span> in one or both seasons, indicating that sea <span class="hlt">ice</span> in these sectors may be influenced more strongly by atmospheric <span class="hlt">variability</span> unexplained by the major atmospheric modes, or by heat exchange in the ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050215215','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050215215"><span>Additional Study of Water Droplet Median <span class="hlt">Volume</span> Diameter (MVD) Effects on <span class="hlt">Ice</span> Shapes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tsao, Jen-Ching; Anderson, David N.</p> <p>2005-01-01</p> <p>This paper reports the result of an experimental study in the NASA Glenn <span class="hlt">Icing</span> Research Tunnel (IRT) to evaluate how well the MVD-independent effect identified previously might apply to SLD conditions in rime <span class="hlt">icing</span> situations. Models were NACA 0012 wing sections with chords of 53.3 and 91.4 cm. Tests were conducted with a nominal airspeed of 77 m/s (150 kt) and a number of MVD's ranging from 15 to 100 m with LWC of 0.5 to 1 g/cu m. In the present study, <span class="hlt">ice</span> shapes recorded from past studies and recent results at SLD and Appendix-C conditions are reviewed to show that droplet diameter is not important to rime <span class="hlt">ice</span> shape for MVD of 30 microns or larger, but for less than 30 m drop sizes a rime <span class="hlt">ice</span> shape transition from convex to wedge to spearhead type <span class="hlt">ice</span> shape is observed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C53C0754M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C53C0754M"><span>Quaternary evolution of the Fennoscandian <span class="hlt">Ice</span> Sheet from 3D seismic data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Montelli, A.; Dowdeswell, J. A.; Ottesen, D.; Johansen, S. E.</p> <p>2016-12-01</p> <p>The Quaternary seismic stratigraphy and architecture of the mid-Norwegian continental shelf and slope are investigated using extensive grids of marine 2D and 3D seismic reflection data that cover more than 100,000 km2 of the continental margin. At least 26 distinct regional palaeo-surfaces have been interpreted within the stratigraphy of the Quaternary Naust Formation on the mid-Norwegian margin. Multiple assemblages of buried glacigenic landforms are preserved within the Naust Formation across most of the study area, facilitating detailed palaeo-glaciological reconstructions. We document a marine-terminating, calving Fennoscandian <span class="hlt">Ice</span> Sheet (FIS) margin present periodically on the Norwegian shelf since at least the beginning of the Quaternary. Elongate, streamlined landforms interpreted as mega-scale glacial lineations (MSGLs) have been found within the upper part of the Naust sequence N ( 1.9-1.6 Ma), sugesting the development of fast-flowing <span class="hlt">ice</span> streams since that time. Shifts in the location of depocentres and direction of features indicative of fast <span class="hlt">ice</span>-flow suggest that several reorganisations in the FIS drainage have occurred since 1.5 Ma. Subglacial landforms reveal a complex and dynamic <span class="hlt">ice</span> sheet, with converging palaeo-<span class="hlt">ice</span> streams and several flow-switching events that may reflect major changes in topography and internal <span class="hlt">ice</span>-sheet structure. Lack of subglacial meltwater channels suggests a largely distributed, low-<span class="hlt">volume</span> meltwater system that drained the FIS through permeable subglacial till without leaving much erosional evidence. This regional palaeo-environmental examination of the FIS provides a useful framework for <span class="hlt">ice</span>-sheet modelling and shows that fragmentary preservation of buried surfaces and <span class="hlt">variability</span> of <span class="hlt">ice</span>-sheet dynamics should be taken into account when reconstructing glacial history from spatially limited datasets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ACPD...1531665L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ACPD...1531665L"><span>Investigation of <span class="hlt">ice</span> particle habits to be used for <span class="hlt">ice</span> cloud remote sensing for the GCOM-C satellite mission</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Letu, H.; Ishimoto, H.; Riedi, J.; Nakajima, T. Y.; -Labonnote, L. C.; Baran, A. J.; Nagao, T. M.; Skiguchi, M.</p> <p>2015-11-01</p> <p>Various <span class="hlt">ice</span> particle habits are investigated in conjunction with inferring the optical properties of <span class="hlt">ice</span> cloud for the Global Change Observation Mission-Climate (GCOM-C) satellite program. A database of the single-scattering properties of five <span class="hlt">ice</span> particle habits, namely, plates, columns, droxtals, bullet-rosettes, and Voronoi, is developed. The database is based on the specification of the Second Generation Global Imager (SGLI) sensor onboard the GCOM-C satellite, which is scheduled to be launched in 2017 by Japan Aerospace Exploration Agency (JAXA). A combination of the finite-difference time-domain (FDTD) method, Geometric Optics Integral Equation (GOIE) technique, and geometric optics method (GOM) are applied to compute the single-scattering properties of the selected <span class="hlt">ice</span> particle habits at 36 wavelengths, from the visible-to-infrared spectral region, covering the SGLI channels for the size parameter, which is defined with respect to the equivalent-<span class="hlt">volume</span> radius sphere, which ranges between 6 and 9000. The database includes the extinction efficiency, absorption efficiency, average geometrical cross-section, single-scattering albedo, asymmetry factor, size parameter of an equivalent <span class="hlt">volume</span> sphere, maximum distance from the center of mass, particle <span class="hlt">volume</span>, and six non-zero elements of the scattering phase matrix. The characteristics of the calculated extinction efficiency, single-scattering albedo, and asymmetry factor of the five <span class="hlt">ice</span> particle habits are compared. Furthermore, the optical thickness and spherical albedo of <span class="hlt">ice</span> clouds using the five <span class="hlt">ice</span> particle habit models are retrieved from the Polarization and Directionality of the Earth's Reflectances-3 (POLDER-3) measurements on board the Polarization and Anisotropy of Reflectances for Atmospheric Sciences coupled with Observations from a Lidar (PARASOL). The optimal <span class="hlt">ice</span> particle habit for retrieving the SGLI <span class="hlt">ice</span> cloud properties was investigated by adopting the spherical albedo difference (SAD) method. It is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA606667','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA606667"><span>Domestic <span class="hlt">Ice</span> Breaking (DOMICE) Simulation Model User Guide</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-02-01</p> <p>Second, add new <span class="hlt">ice</span> data to the <span class="hlt">variable</span> “D9 Historical <span class="hlt">Ice</span> Data (SIGRID Coded) NBL Waterways” (D9_historical_<span class="hlt">ice</span>_d3), which contains the...within that “ NBL ” scheme. The interpretation of the SIGRID <span class="hlt">ice</span> codes into <span class="hlt">ice</span> thickness estimates is also contained within the sub- module “District 9...User Guide)  “D9 Historical <span class="hlt">Ice</span> Data (SIGRID Coded) NBL Waterways” (see Section 5.1.1.3.2 of this User Guide)  “Historical District 1 Weekly Air</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1047/srp/srp029/of2007-1047srp029.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1047/srp/srp029/of2007-1047srp029.pdf"><span>Sea <span class="hlt">ice</span> concentration temporal <span class="hlt">variability</span> over the Weddell Sea and its relationship with tropical sea surface temperature</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Barreira, S.; Compagnucci, R.</p> <p>2007-01-01</p> <p>Principal Components Analysis (PCA) in S-Mode (correlation between temporal series) was performed on sea <span class="hlt">ice</span> monthly anomalies, in order to investigate which are the main temporal patterns, where are the homogenous areas located and how are they related to the sea surface temperature (SST). This analysis provides 9 patterns (4 in the Amundsen and Bellingshausen Seas and 5 in the Weddell Sea) that represent the most important temporal features that dominated sea <span class="hlt">ice</span> concentration anomalies (SICA) <span class="hlt">variability</span> in the Weddell, Amundsen and Bellingshausen Seas over the 1979-2000 period. Monthly Polar Gridded Sea <span class="hlt">Ice</span> Concentrations data set derived from satellite information generated by NASA Team algorithm and acquired from the National Snow and <span class="hlt">Ice</span> Data Center (NSIDC) were used. Monthly means SST are provided by the National Center for Environmental Prediction reanalysis. The first temporal pattern series obtained by PCA has its homogeneous area located at the external region of the Weddell and Bellingshausen Seas and Drake Passage, mostly north of 60°S. The second region is centered in 30°W and located at the southeast of the Weddell. The third area is localized east of 30°W and north of 60°S. South of the first area, the fourth PC series has its homogenous region, between 30° and 60°W. The last area is centered at 0° W and south of 60°S. Correlation charts between the five Principal Components series and SST were performed. Positive correlations over the Tropical Pacific Ocean were found for the five PCs when SST series preceded SICA PC series. The sign of the correlation could relate the occurrence of an El Niño/Southern Oscillation (ENSO) warm (cold) event with posterior positive (negative) anomalies of sea <span class="hlt">ice</span> concentration over the Weddell Sea.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16782603','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16782603"><span>Mass balance of the Antarctic <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>Wingham, D J; Shepherd, A; Muir, A; Marshall, G J</p> <p>2006-07-15</p> <p>The Antarctic contribution to sea-level rise has long been uncertain. While regional <span class="hlt">variability</span> in <span class="hlt">ice</span> dynamics has been revealed, a picture of mass changes throughout the continental <span class="hlt">ice</span> sheet is lacking. Here, we use satellite radar altimetry to measure the elevation change of 72% of the grounded <span class="hlt">ice</span> sheet during the period 1992-2003. Depending on the density of the snow giving rise to the observed elevation fluctuations, the <span class="hlt">ice</span> 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 <span class="hlt">variability</span>. Mass gains from accumulating snow, particularly on the Antarctic Peninsula and within East Antarctica, exceed the <span class="hlt">ice</span> dynamic mass loss from West Antarctica. The result exacerbates the difficulty of explaining twentieth century sea-level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1016900','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1016900"><span>Review of Anti-<span class="hlt">Icing/Ice</span> Release Systems</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-01-29</p> <p>be superhydrophobic and tend to be fragile, Figure 3. Note if the water completely wets the surface then the adhesion energy can be much higher due...to the increase in surface area. γSV γLV γSL θ 3 Figure 3: Water drops on a superhydrophobic coating [11]. Freezing of a drop... Superhydrophobic coatings. • Other: Phase change materials that change shape/<span class="hlt">volume</span> may reduce the adhesive strength of the <span class="hlt">ice</span>-coating bond. 4</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA617899','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA617899"><span>An Innovative Network to Improve Sea <span class="hlt">Ice</span> Prediction in a Changing Arctic</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>sea <span class="hlt">ice</span> <span class="hlt">volume</span>. The EXP ensemble is initialized with 1/5 of CNTL snow depths, thus resulting in a reduced snow cover and lower summer albedo ... Sea <span class="hlt">Ice</span> - Albedo Feedback in Sea <span class="hlt">Ice</span> Predictions is also about understanding sea <span class="hlt">ice</span> predictability. REFERENCES Blanchard-Wrigglesworth, E., K...1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. An Innovative Network to Improve Sea <span class="hlt">Ice</span> Prediction</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.7448F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.7448F"><span>Solving the riddle of interglacial temperatures over the last 1.5 million years with a future IPICS "Oldest <span class="hlt">Ice</span>" <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>Fischer, Hubertus</p> <p>2014-05-01</p> <p>The sequence of the last 8 glacial cycles is characterized by irregular 100,000 year cycles in temperature and sea level. In contrast, the time period between 1.5-1.2 million years ago is characterized by more regular cycles with an obliquity periodicity of 41,000 years. Based on a deconvolution of deep ocean temperature and <span class="hlt">ice</span> <span class="hlt">volume</span> contributions to benthic δ18O (Elderfield et al., Science, 2012), it is suggested that glacial sea level became progressively lower over the last 1.5 Myr, while glacial deep ocean temperatures were very similar. At the same time many interglacials prior to the Mid Brunhes event showed significantly cooler deep ocean temperatures than the Holocene, while at the same time interglacial <span class="hlt">ice</span> <span class="hlt">volume</span> remained essentially the same. In contrast, interglacial sea surface temperatures in the tropics changed little (Herbert et al., Science,2010) and proxy reconstructions of atmospheric CO2 using δ11B in planktic foraminifera (Hönisch et al., Science, 2009) suggest that prior to 900,000 yr before present interglacial CO2 levels did not differ substantially from those over the last 450,000 years. Accordingly, the conundrum arises how interglacials can differ in deep ocean temperature without any obvious change in <span class="hlt">ice</span> <span class="hlt">volume</span> or greenhouse gas forcing and what caused the change in cyclicity of glacial interglacial cycles over the Mid Pleistocene Transition. Probably the most important contribution to solve this riddle is the recovery of a 1.5 Myr old <span class="hlt">ice</span> core from Antarctica, which among others would provide an unambiguous, high-resolution record of the greenhouse gas history over this time period. Accordingly, the international <span class="hlt">ice</span> core community, as represented by the International Partnership for <span class="hlt">Ice</span> Core Science (IPICS), has identified such an 'Oldest <span class="hlt">Ice</span>' <span class="hlt">ice</span> core as one of the most important scientific targets for the future (http://www.pages.unibe.ch/ipics/white-papers). However, finding stratigraphically undisturbed <span class="hlt">ice</span>, which covers this</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=ice+AND+cream&pg=3&id=EJ116576','ERIC'); return false;" href="https://eric.ed.gov/?q=ice+AND+cream&pg=3&id=EJ116576"><span>Let's Make Metric <span class="hlt">Ice</span> Cream</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>Zimmerman, Marianna</p> <p>1975-01-01</p> <p>Describes a classroom activity which involved sixth grade students in a learning situation including making <span class="hlt">ice</span> cream, safety procedures in a science laboratory, calibrating a thermometer, using metric units of <span class="hlt">volume</span> and mass. (EB)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/39158','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/39158"><span>Rapid Assessment of Tree Debris Following Urban Forest <span class="hlt">Ice</span> Storms</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Richard J. Hauer; Angela J. Hauer; Dudley R. Hartel; Jill R. Johnson</p> <p>2011-01-01</p> <p>This paper presents a rapid assessment method to estimate urban tree debris following an <span class="hlt">ice</span> storm. Data were collected from 60 communities to quantify tree debris <span class="hlt">volumes</span>, mostly from public rights-of-way, following <span class="hlt">ice</span> storms based on community infrastructure, weather parameters, and urban forest structure. <span class="hlt">Ice</span> thickness, area of a community, and street distance are...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814313K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814313K"><span>The internal structure of the Brunt <span class="hlt">Ice</span> Shelf, Antarctica from <span class="hlt">ice</span>-penetrating radar</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>King, Edward; De Rydt, Jan; Gudmundsson, Hilmar</p> <p>2016-04-01</p> <p>The Brunt <span class="hlt">Ice</span> Shelf is a small feature on the Coats Land Coast of the Weddell Sea, Antarctica. It is unusual among Antarctic <span class="hlt">ice</span> shelves because the <span class="hlt">ice</span> crossing the grounding line from the <span class="hlt">ice</span> sheet retains no structural integrity, so the <span class="hlt">ice</span> shelf comprises icebergs of continental <span class="hlt">ice</span> cemented together by sea <span class="hlt">ice</span>, with the whole blanketed by in-situ snowfall. The size and distribution of the icebergs is governed by the thickness profile along the grounding line. Where bedrock troughs discharge thick <span class="hlt">ice</span> to the <span class="hlt">ice</span> shelf, the icebergs are large and remain close together with little intervening sea <span class="hlt">ice</span>. Where bedrock ridges mean the <span class="hlt">ice</span> crossing the grounding line is thin, the icebergs are small and widely-scattered with large areas of sea <span class="hlt">ice</span> between them. To better understand the internal structure of the Brunt <span class="hlt">Ice</span> Shelf and how this might affect the flow dynamics we conducted <span class="hlt">ice</span>-penetrating radar surveys during December 2015 and January 2016. Three different ground-based radar systems were used, operating at centre frequencies of 400, 50 and 10 MHz respectively. The 400 MHz system gave detailed firn structure and accumulation profiles as well as time-lapse profiles of the active propagation of a crevasse. The 50 MHz system provided intermediate-level detail of iceberg distribution and thickness as well as information on the degree of salt water infiltration into the accumulating snow pack. The 10 MHz system used a high-power transmitter in an attempt to measure <span class="hlt">ice</span> thickness beneath salt-impregnated <span class="hlt">ice</span>. In this poster we will present example data from each of the three radar systems which will demonstrate the <span class="hlt">variability</span> of the internal structure of the <span class="hlt">ice</span> shelf. We will also present preliminary correlations between the internal structure and the surface topography from satellite data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C21E..02I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21E..02I"><span>Measurements of sea <span class="hlt">ice</span> mass redistribution during <span class="hlt">ice</span> deformation event in Arctic winter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Itkin, P.; Spreen, G.; King, J.; Rösel, A.; Skourup, H.; Munk Hvidegaard, S.; Wilkinson, J.; Oikkonen, A.; Granskog, M. A.; Gerland, S.</p> <p>2016-12-01</p> <p>. From the freeboard change we calculate the sea <span class="hlt">ice</span> <span class="hlt">volume</span> change. Our results show exemplary sea-<span class="hlt">ice</span> mass redistribution caused by sea <span class="hlt">ice</span> dynamics during winter conditions in the Arctic, which can be used to estimate sea-<span class="hlt">ice</span> growth due to deformation processes in a wider region, and ultimately to distinguish between thermodynamic and dynamic <span class="hlt">ice</span> growth processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020441','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020441"><span>Greenland Sea Odden sea <span class="hlt">ice</span> feature: Intra-annual and interannual <span class="hlt">variability</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>Shuchman, R.A.; Josberger, E.G.; Russel, C.A.; Fischer, K.W.; Johannessen, O.M.; Johannessen, J.; Gloersen, P.</p> <p>1998-01-01</p> <p>The "Odden" is a large sea <span class="hlt">ice</span> feature that forms in the east Greenland Sea that may protrude eastward to 5??E from the main sea <span class="hlt">ice</span> pack (at about 8??W) between 73?? and 77??N. It generally forms at the beginning of the winter season and can cover 300,000 km2. Throughout the winter the outer edge of the Odden may advance and retreat by several hundred kilometers on timescales of a few days to weeks. Satellite passive microwave observations from 1978 through 1995 provide a continuous record of the spatial and temporal variations of this extremely dynamic phenomenon. Aircraft synthetic aperture radar, satellite passive microwave, and ship observations in the Odden show that the Odden consists of new <span class="hlt">ice</span> types, rather than older <span class="hlt">ice</span> types advected eastward from the main pack. The 17-year record shows both strong interannual and intra-annual variations in Odden extent and temporal behavior. For example, in 1983 the Odden was weak, in 1984 the Odden did not occur, and in 1985 the Odden returned late in the season. An analysis of the <span class="hlt">ice</span> area and extent time series derived from the satellite passive microwave observations along with meteorological data from the International Arctic Buoy Program (IABP) determined the meteorological forcing associated with Odden growth, maintenance, and decay. The key meteorological parameters that are related to the rapid <span class="hlt">ice</span> formation and decay associated with the Odden are, in order of importance, air temperature, wind speed, and wind direction. Oceanographic parameters must play an important role in controlling Odden formation, but it is not yet possible to quantify this role because of a lack of long-term oceanographic observations. Copyright 1998 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.1592C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.1592C"><span>Multi-centennial Record of Labrador Sea Primary Productivity and Sea-<span class="hlt">Ice</span> <span class="hlt">Variability</span> Archived in Coralline Algal Ba/Ca</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chan, Phoebe; Halfar, Jochen; Adey, Walter; Hetzinger, Steffen; Zack, Thomas; Moore, Kent; Wortmann, Ulrich; Williams, Branwen; Hou, Alicia</p> <p>2017-04-01</p> <p>Arctic sea-<span class="hlt">ice</span> thickness and concentration have dropped by approximately 9% per decade since 1978. Concurrent with this sea-<span class="hlt">ice</span> decline is an increase in rates of phytoplankton productivity, driven by shoaling of the mixed layer and enhanced transmittance of solar radiation into the surface ocean. This has recently been confirmed by phytoplankton studies in Arctic and Subarctic basins that have revealed earlier timing, prolonged duration, and increased primary productivity of the spring phytoplankton bloom. However, difficulties of navigating in remote <span class="hlt">ice</span>-laden waters and harsh polar climates have often resulted in short and incomplete records of in-situ plankton abundance in the northwestern Labrador Sea. Alternatively, information of past ocean productivity may be gained through the study of trace nutrient distributions in the surface water column. Investigations of dissolved barium (Ba) concentrations in the Arctic reveal significant depletions of Ba in surface seawaters due to biological scavenging during the spring phytoplankton bloom. Here we apply a barium-to-calcium (Ba/Ca) and carbon isotope (δ13C) multiproxy approach to long-lived crustose coralline algae in order to reconstruct an annually-resolved multi-centennial record of Labrador Sea productivity related to sea-<span class="hlt">ice</span> <span class="hlt">variability</span> in Labrador, Canada that extends well into the Little <span class="hlt">Ice</span> Age (LIA; 1646 AD). The crustose coralline alga Clathromorphum compactum is a shallow marine calcareous plant that is abundant along the eastern Canadian coastline, and produces annual growth increments which allow for the precise calendar dating and geochemical sampling of hard tissue. Algal Ba/Ca ratios can serve as a promising new proxy for surface water productivity, demonstrating a close correspondence to δ13C that does not suffer from the anthropogenically-induced carbon isotope decline (ex. Suess Effect) beginning in the 1960s. Coralline algal Ba/Ca demonstrates statistically significant correlations to both</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1171310-microphysical-consequences-spatial-distribution-ice-nucleation-mixed-phase-stratiform-clouds','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1171310-microphysical-consequences-spatial-distribution-ice-nucleation-mixed-phase-stratiform-clouds"><span>Microphysical Consequences of the Spatial Distribution of <span class="hlt">Ice</span> Nucleation in Mixed-Phase Stratiform Clouds</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Yang, Fan; Ovchinnikov, Mikhail; Shaw, Raymond A.</p> <p></p> <p>Mixed-phase stratiform clouds can persist even with steady <span class="hlt">ice</span> precipitation fluxes, and the origin and microphysical properties of the <span class="hlt">ice</span> crystals are of interest. Vapor deposition growth and sedimentation of <span class="hlt">ice</span> particles along with a uniform <span class="hlt">volume</span> source of <span class="hlt">ice</span> nucleation, leads to a power law relation between <span class="hlt">ice</span> water content wi and <span class="hlt">ice</span> number concentration ni with exponent 2.5. The result is independent of assumptions about the vertical velocity structure of the cloud and is therefore more general than the related expression of Yang et al. [2013]. The sensitivity of the wi-ni relationship to the spatial distribution of icemore » nucleation is confirmed by Lagrangian tracking and <span class="hlt">ice</span> growth with cloud-<span class="hlt">volume</span>, cloud-top, and cloud-base sources of <span class="hlt">ice</span> particles through a time-dependent cloud field. Based on observed wi and ni from ISDAC, a lower bound of 0.006 m^3/s is obtained for the <span class="hlt">ice</span> crystal formation rate.« less</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, mass balance, and interannual <span class="hlt">variability</span> 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/2017AGUFM.B51F1874A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B51F1874A"><span><span class="hlt">Ice</span> core carbonyl sulfide measurements from a new South Pole <span class="hlt">ice</span> core (SPICECORE)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aydin, M.; Nicewonger, M. R.; Saltzman, E. S.</p> <p>2017-12-01</p> <p>Carbonyl sulfide (COS) is the most abundant sulfur gas in the troposphere with a present-day mixing ratio of about 500 ppt. Direct and indirect emissions from the oceans are the predominant sources of atmospheric COS. The primary removal mechanism is uptake by terrestrial plants during photosynthesis. Because plants do not respire COS, atmospheric COS levels are linked to terrestrial gross primary productivity (GPP). Ancient air trapped in polar <span class="hlt">ice</span> cores has been used to reconstruct COS records of the past atmosphere, which can be used to infer past GPP <span class="hlt">variability</span> and potential changes in oceanic COS emission. We are currently analyzing samples from a newly drilled intermediate depth <span class="hlt">ice</span> core from South Pole, Antarctica (SPICECORE). This core is advantageous for studying COS because the cold temperatures of South Pole <span class="hlt">ice</span> lead to very slow rates of in situ loss due to hydrolysis. One hundred and eighty-four bubbly <span class="hlt">ice</span> core samples have been analyzed to date with gas ages ranging from about 9.2 thousand (733 m depth) to 75 years (126 m depth) before present. After a 2% correction for gravitational enrichment in the firn, the mean COS mixing ratio for the data set is 312±15 ppt (±1s), with the data set median also equal to 312 ppt. The only significant long-term trend in the record is a 5-10% increase in COS during the last 2-3 thousand years of the Holocene. The SPICECORE data agree with previously published <span class="hlt">ice</span> core COS records from other Antarctic sites during times of overlap, confirming earlier estimates of COS loss rates to in situ hydrolysis in <span class="hlt">ice</span> cores. Antarctic <span class="hlt">ice</span> core data place strict constraints on the COS mixing ratio and its range of <span class="hlt">variability</span> in the southern hemisphere atmosphere during the last several millennia. Implications for the atmospheric COS budget will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.2491T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.2491T"><span>Dark <span class="hlt">ice</span> dynamics of the south-west Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tedstone, Andrew J.; Bamber, Jonathan L.; Cook, Joseph M.; Williamson, Christopher J.; Fettweis, Xavier; Hodson, Andrew J.; Tranter, Martyn</p> <p>2017-11-01</p> <p>Runoff from the Greenland <span class="hlt">Ice</span> Sheet (GrIS) has increased in recent years due largely to changes in atmospheric circulation and atmospheric warming. Albedo reductions resulting from these changes have amplified surface melting. Some of the largest declines in GrIS albedo have occurred in the ablation zone of the south-west sector and are associated with the development of dark <span class="hlt">ice</span> surfaces. Field observations at local scales reveal that a variety of light-absorbing impurities (LAIs) can be present on the surface, ranging from inorganic particulates to cryoconite materials and <span class="hlt">ice</span> algae. Meanwhile, satellite observations show that the areal extent of dark <span class="hlt">ice</span> has varied significantly between recent successive melt seasons. However, the processes that drive such large interannual <span class="hlt">variability</span> in dark <span class="hlt">ice</span> extent remain essentially unconstrained. At present we are therefore unable to project how the albedo of bare <span class="hlt">ice</span> sectors of the GrIS will evolve in the future, causing uncertainty in the projected sea level contribution from the GrIS over the coming decades. Here we use MODIS satellite imagery to examine dark <span class="hlt">ice</span> dynamics on the south-west GrIS each year from 2000 to 2016. We quantify dark <span class="hlt">ice</span> in terms of its annual extent, duration, intensity and timing of first appearance. Not only does dark <span class="hlt">ice</span> extent vary significantly between years but so too does its duration (from 0 to > 80 % of June-July-August, JJA), intensity and the timing of its first appearance. Comparison of dark <span class="hlt">ice</span> dynamics with potential meteorological drivers from the regional climate model MAR reveals that the JJA sensible heat flux, the number of positive minimum-air-temperature days and the timing of bare <span class="hlt">ice</span> appearance are significant interannual synoptic controls. We use these findings to identify the surface processes which are most likely to explain recent dark <span class="hlt">ice</span> dynamics. We suggest that whilst the spatial distribution of dark <span class="hlt">ice</span> is best explained by outcropping of particulates from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.7271O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7271O"><span>Modeling Wave-<span class="hlt">Ice</span> Interactions in the Marginal <span class="hlt">Ice</span> Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Orzech, Mark; Shi, Fengyan; Bateman, Sam; Veeramony, Jay; Calantoni, Joe</p> <p>2015-04-01</p> <p>The small-scale (O(m)) interactions between waves and <span class="hlt">ice</span> floes in the marginal <span class="hlt">ice</span> zone (MIZ) are investigated with a coupled model system. Waves are simulated with the non-hydrostatic finite-<span class="hlt">volume</span> model NHWAVE (Ma et al., 2012) and <span class="hlt">ice</span> floes are represented as bonded collections of smaller particles with the discrete element system LIGGGHTS (Kloss et al., 2012). The physics of fluid and <span class="hlt">ice</span> are recreated as authentically as possible, to allow the coupled system to supplement and/or substitute for more costly and demanding field experiments. The presentation will first describe the development and validation of the coupled system, then discuss the results of a series of virtual experiments in which <span class="hlt">ice</span> floe and wave characteristics are varied to examine their effects on energy dissipation, MIZ floe size distribution, and <span class="hlt">ice</span> pack retreat rates. Although Wadhams et al. (1986) suggest that only a small portion (roughly 10%) of wave energy entering the MIZ is reflected, dissipation mechanisms for the remaining energy have yet to be delineated or measured. The virtual experiments are designed to focus on specific properties and processes - such as floe size and shape, collision and fracturing events, and variations in wave climate - and measure their relative roles the transfer of energy and momentum from waves to <span class="hlt">ice</span>. Questions to be examined include: How is energy dissipated by <span class="hlt">ice</span> floe collisions, fracturing, and drag, and how significant is the wave attenuation associated with each process? Do specific wave/floe length scale ratios cause greater wave attenuation? How does <span class="hlt">ice</span> material strength affect the rate of wave energy loss? The coupled system will ultimately be used to test and improve upon wave-<span class="hlt">ice</span> parameterizations for large-scale climate models. References: >Kloss, C., C. Goniva, A. Hager, S. Amberger, and S. Pirker (2012). Models, algorithms and validation for opensource DEM and CFD-DEM. Progress in Computational Fluid Dynamics 12(2/3), 140-152. >Ma, G</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23925242','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23925242"><span>Insolation-driven 100,000-year glacial cycles and hysteresis of <span class="hlt">ice</span>-sheet <span class="hlt">volume</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Abe-Ouchi, Ayako; Saito, Fuyuki; Kawamura, Kenji; Raymo, Maureen E; Okuno, Jun'ichi; Takahashi, Kunio; Blatter, Heinz</p> <p>2013-08-08</p> <p>The growth and reduction of Northern Hemisphere <span class="hlt">ice</span> sheets over the past million years is dominated by an approximately 100,000-year periodicity and a sawtooth pattern (gradual growth and fast termination). Milankovitch theory proposes that summer insolation at high northern latitudes drives the glacial cycles, and statistical tests have demonstrated that the glacial cycles are indeed linked to eccentricity, obliquity and precession cycles. Yet insolation alone cannot explain the strong 100,000-year cycle, suggesting that internal climatic feedbacks may also be at work. Earlier conceptual models, for example, showed that glacial terminations are associated with the build-up of Northern Hemisphere 'excess <span class="hlt">ice</span>', but the physical mechanisms underpinning the 100,000-year cycle remain unclear. Here we show, using comprehensive climate and <span class="hlt">ice</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 mass 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 mass 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 mass balance, leading to an almost complete retreat of the <span class="hlt">ice</span> sheet within several thousand years. This fast retreat is governed mainly by rapid ablation due to the lowered surface elevation resulting from delayed isostatic rebound, which is the lithosphere</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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> masses 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> masses have been shrinking in recent in years, but their mass balance is highly <span class="hlt">variable</span> 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> mass balance and the mechanisms that control it in one of the most climatically sensitive regions on Earth. As we continue to learn more through a combination of remote sensing observations, in situ measurements and improved modeling capabilities, it is important that we coordinate and integrate these approaches effectively in order to predict future changes and their impact on sea level, freshwater discharge, and ocean circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940026121','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940026121"><span>A toy model of sea <span class="hlt">ice</span> growth</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Thorndike, Alan S.</p> <p>1992-01-01</p> <p>My purpose here is to present a simplified treatment of the growth of sea <span class="hlt">ice</span>. By ignoring many details, it is possible to obtain several results that help to clarify the ways in which the sea <span class="hlt">ice</span> cover will respond to climate change. Three models are discussed. The first deals with the growth of sea <span class="hlt">ice</span> during the cold season. The second describes the cycle of growth and melting for perennial <span class="hlt">ice</span>. The third model extends the second to account for the possibility that the <span class="hlt">ice</span> melts away entirely in the summer. In each case, the objective is to understand what physical processes are most important, what <span class="hlt">ice</span> properties determine the <span class="hlt">ice</span> behavior, and to which climate <span class="hlt">variables</span> the system is most sensitive.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840019242','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840019242"><span>Method to estimate drag coefficient at the air/<span class="hlt">ice</span> interface over drifting open pack <span class="hlt">ice</span> from remotely sensed data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Feldman, U.</p> <p>1984-01-01</p> <p>A knowledge in near real time, of the surface drag coefficient for drifting pack <span class="hlt">ice</span> is vital for predicting its motions. And since this is not routinely available from measurements it must be replaced by estimates. Hence, a method for estimating this <span class="hlt">variable</span>, as well as the drag coefficient at the water/<span class="hlt">ice</span> interface and the <span class="hlt">ice</span> thickness, for drifting open pack <span class="hlt">ice</span> was developed. These estimates were derived from three-day sequences of LANDSAT-1 MSS images and surface weather charts and from the observed minima and maxima of these <span class="hlt">variables</span>. The method was tested with four data sets in the southeastern Beaufort sea. Acceptable results were obtained for three data sets. Routine application of the method depends on the availability of data from an all-weather air or spaceborne remote sensing system, producing images with high geometric fidelity and high resolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016QSRv..137...54B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016QSRv..137...54B"><span>Modelling sea level data from China and Malay-Thailand to estimate Holocene <span class="hlt">ice-volume</span> equivalent sea level change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bradley, Sarah L.; Milne, Glenn A.; Horton, Benjamin P.; Zong, Yongqiang</p> <p>2016-04-01</p> <p>This study presents a new model of Holocene <span class="hlt">ice-volume</span> equivalent sea level (ESL), extending a previously published global <span class="hlt">ice</span> sheet model (Bassett et al., 2005), which was unconstrained from 10 kyr BP to present. This new model was developed by comparing relative sea level (RSL) predictions from a glacial isostatic adjustment (GIA) model to a suite of Holocene sea level index points from China and Malay-Thailand. Three consistent data-model misfits were found using the Bassett et al. (2005) model: an over-prediction in the height of maximum sea level, the timing of this maximum, and the temporal variation of sea level from the time of the highstand to present. The data-model misfits were examined for a large suite of ESL scenarios and a range of earth model parameters to determine an optimum model of Holocene ESL. This model is characterised by a slowdown in melting at ∼7 kyr BP, associated with the final deglaciation of the Laurentide <span class="hlt">Ice</span> Sheet, followed by a continued rise in ESL until ∼1 kyr BP of ∼5.8 m associated with melting from the Antarctic <span class="hlt">Ice</span> Sheet. It was not possible to identify an earth viscosity model that provided good fits for both regions; with the China data preferring viscosity values in the upper mantle of less than 1.5 × 1020 Pa s and the Malay-Thailand data preferring greater values. We suggest that this inference of a very weak upper mantle for the China data originates from the nearby subduction zone and Hainan Plume. The low viscosity values may also account for the lack of a well-defined highstand at the China sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70179581','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70179581"><span>Final Laurentide <span class="hlt">ice</span>-sheet deglaciation and Holocene climate-sea level change</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ullman, David J.; Carlson, Anders E.; Hostetler, Steven W.; Clark, Peter U.; Cuzzone, Joshua; Milne, Glenn A.; Winsor, Kelsey; Caffee, Marc A.</p> <p>2016-01-01</p> <p>Despite elevated summer insolation forcing during the early Holocene, global <span class="hlt">ice</span> sheets retained nearly half of their <span class="hlt">volume</span> from the Last Glacial Maximum, as indicated by deglacial records of global mean sea level (GMSL). Partitioning the GMSL rise among potential sources requires accurate dating of <span class="hlt">ice</span>-sheet extent to estimate <span class="hlt">ice</span>-sheet <span class="hlt">volume</span>. Here, we date the final retreat of the Laurentide <span class="hlt">Ice</span> Sheet with 10Be surface exposure ages for the Labrador Dome, the largest of the remnant Laurentide <span class="hlt">ice</span> domes during the Holocene. We show that the Labrador Dome deposited moraines during North Atlantic cold events at ∼10.3 ka, 9.3 ka and 8.2 ka, suggesting that these regional climate events helped stabilize the retreating Labrador Dome in the early Holocene. After Hudson Bay became seasonally <span class="hlt">ice</span> free at ∼8.2 ka, the majority of Laurentide <span class="hlt">ice</span>-sheet melted abruptly within a few centuries. We demonstrate through high-resolution regional climate model simulations that the thermal properties of a seasonally <span class="hlt">ice</span>-free Hudson Bay would have increased Laurentide <span class="hlt">ice</span>-sheet ablation and thus contributed to the subsequent rapid Labrador Dome retreat. Finally, our new 10Be chronology indicates full Laurentide <span class="hlt">ice</span>-sheet had completely deglaciated by 6.7 ± 0.4 ka, which re quires that Antarctic <span class="hlt">ice</span> sheets contributed 3.6–6.5 m to GMSL rise since 6.3–7.1 ka.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110024198','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110024198"><span><span class="hlt">Ice</span> Lens Formation, Frost Heave, Thin Films, and the Importance of the Polar H2O Reservoir at High Obliquity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zent, A. P.; Sizemore, H. G.; Rempel, A. W.</p> <p>2011-01-01</p> <p>Several lines of evidence indicate that the <span class="hlt">volume</span> of shallow ground <span class="hlt">ice</span> in the martian high latitudes exceeds the pore <span class="hlt">volume</span> of the host regolith. Boynton et al. found an optimal fit to the Mars Odyssey Gamma Ray Spectrometer (GRS) data at the Phoenix landing site by modeling a buried layer of 50-75% <span class="hlt">ice</span> by mass (up to 90% <span class="hlt">ice</span> by <span class="hlt">volume</span>). Thermal and optical observations of recent impact craters in the northern hemisphere have revealed nearly pure <span class="hlt">ice</span>. <span class="hlt">Ice</span> deposits containing only 1-2% soil by <span class="hlt">volume</span> were excavaged by Phoenix. One hypothesis for the origin of this excess <span class="hlt">ice</span> is that it developed in situ by a mechanism analogous to the formation of terrestrial <span class="hlt">ice</span> lenses and needle <span class="hlt">ice</span>. Problematically, terrestrial soil-<span class="hlt">ice</span> segregation is driven by freeze/thaw cycling and the movement of bulk water, neither of which are expected to have occurred in the geologically recent past on Mars. If however <span class="hlt">ice</span> lens formation is possible at temperatures less than 273 K, there are possible implications for the habitability of Mars permafrost, since the same thin films of unfrozen water that lead to <span class="hlt">ice</span> segregation are used by terrestrial psychrophiles to metaboluze and grow down to temperatures of at least 258 K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ACP....1612287L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ACP....1612287L"><span>Investigation of <span class="hlt">ice</span> particle habits to be used for <span class="hlt">ice</span> cloud remote sensing for the GCOM-C satellite mission</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Letu, Husi; Ishimoto, Hiroshi; Riedi, Jerome; Nakajima, Takashi Y.; -Labonnote, Laurent C.; Baran, Anthony J.; Nagao, Takashi M.; Sekiguchi, Miho</p> <p>2016-09-01</p> <p>In this study, various <span class="hlt">ice</span> particle habits are investigated in conjunction with inferring the optical properties of <span class="hlt">ice</span> clouds for use in the Global Change Observation Mission-Climate (GCOM-C) satellite programme. We develop a database of the single-scattering properties of five <span class="hlt">ice</span> habit models: plates, columns, droxtals, bullet rosettes, and Voronoi. The database is based on the specification of the Second Generation Global Imager (SGLI) sensor on board the GCOM-C satellite, which is scheduled to be launched in 2017 by the Japan Aerospace Exploration Agency. A combination of the finite-difference time-domain method, the geometric optics integral equation technique, and the geometric optics method is applied to compute the single-scattering properties of the selected <span class="hlt">ice</span> particle habits at 36 wavelengths, from the visible to the infrared spectral regions. This covers the SGLI channels for the size parameter, which is defined as a single-particle radius of an equivalent <span class="hlt">volume</span> sphere, ranging between 6 and 9000 µm. The database includes the extinction efficiency, absorption efficiency, average geometrical cross section, single-scattering albedo, asymmetry factor, size parameter of a <span class="hlt">volume</span>-equivalent sphere, maximum distance from the centre of mass, particle <span class="hlt">volume</span>, and six nonzero elements of the scattering phase matrix. The characteristics of calculated extinction efficiency, single-scattering albedo, and asymmetry factor of the five <span class="hlt">ice</span> particle habits are compared. Furthermore, size-integrated bulk scattering properties for the five <span class="hlt">ice</span> particle habit models are calculated from the single-scattering database and microphysical data. Using the five <span class="hlt">ice</span> particle habit models, the optical thickness and spherical albedo of <span class="hlt">ice</span> clouds are retrieved from the Polarization and Directionality of the Earth's Reflectances-3 (POLDER-3) measurements, recorded on board the Polarization and Anisotropy of Reflectances for Atmospheric Sciences coupled with Observations from a</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://hdl.handle.net/2060/19930082126','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930082126"><span>The Calculation of the Heat Required for Wing Thermal <span class="hlt">Ice</span> Prevention in Specified <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>Bergrun, Norman R.; Jukoff, David; Schlaff, Bernard A.; Neel, Carr B., Jr.</p> <p>1947-01-01</p> <p>Flight tests were made in natural <span class="hlt">icing</span> conditions with two 8-ft-chord heated airfoils of different sections. Measurements of meteorological <span class="hlt">variables</span> conducive to <span class="hlt">ice</span> formation were made simultaneously with the procurement of airfoil thermal data. The extent of knowledge on the meteorology of <span class="hlt">icing</span>, the impingement of water drops on airfoil surfaces, and the processes of heat transfer and evaporation from a wetted airfoil surface have been increased to a point where the design of heated wings on a fundamental, wet-air basis now can be undertaken with reasonable certainty.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29284198','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29284198"><span>Signals from the south; humpback whales carry messages of Antarctic sea-<span class="hlt">ice</span> ecosystem <span class="hlt">variability</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bengtson Nash, Susan M; Castrillon, Juliana; Eisenmann, Pascale; Fry, Brian; Shuker, Jon D; Cropp, Roger A; Dawson, Amanda; Bignert, Anders; Bohlin-Nizzetto, Pernilla; Waugh, Courtney A; Polkinghorne, Bradley J; Dalle Luche, Greta; McLagan, David</p> <p>2018-04-01</p> <p>Southern hemisphere humpback whales (Megaptera novaeangliae) rely on summer prey abundance of Antarctic krill (Euphausia superba) to fuel one of the longest-known mammalian migrations on the planet. It is hypothesized that this species, already adapted to endure metabolic extremes, will be one of the first Antarctic consumers to show measurable physiological change in response to fluctuating prey availability in a changing climate; and as such, a powerful sentinel candidate for the Antarctic sea-<span class="hlt">ice</span> ecosystem. Here, we targeted the sentinel parameters of humpback whale adiposity and diet, using novel, as well as established, chemical and biochemical markers, and assembled a time trend spanning 8 years. We show the synchronous, inter-annual oscillation of two measures of humpback whale adiposity with Southern Ocean environmental <span class="hlt">variables</span> and climate indices. Furthermore, bulk stable isotope signatures provide clear indication of dietary compensation strategies, or a lower trophic level isotopic change, following years indicated as leaner years for the whales. The observed synchronicity of humpback whale adiposity and dietary markers, with climate patterns in the Southern Ocean, lends strength to the role of humpback whales as powerful Antarctic sea-<span class="hlt">ice</span> ecosystem sentinels. The work carries significant potential to reform current ecosystem surveillance in the Antarctic region. © 2017 John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..182...93K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..182...93K"><span>Changes in sea <span class="hlt">ice</span> cover and <span class="hlt">ice</span> sheet extent at the Yermak Plateau during the last 160 ka - Reconstructions from biomarker records</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kremer, A.; Stein, R.; Fahl, K.; Ji, Z.; Yang, Z.; Wiers, S.; Matthiessen, J.; Forwick, M.; Löwemark, L.; O'Regan, M.; Chen, J.; Snowball, I.</p> <p>2018-02-01</p> <p>The Yermak Plateau is located north of Svalbard at the entrance to the Arctic Ocean, i.e. in an area highly sensitive to climate change. A multi proxy approach was carried out on Core PS92/039-2 to study glacial-interglacial environmental changes at the northern Barents Sea margin during the last 160 ka. The main emphasis was on the reconstruction of sea <span class="hlt">ice</span> cover, based on the sea <span class="hlt">ice</span> proxy IP25 and the related phytoplankton - sea <span class="hlt">ice</span> index PIP25. Sea <span class="hlt">ice</span> was present most of the time but showed significant temporal <span class="hlt">variability</span> decisively affected by movements of the Svalbard Barents Sea <span class="hlt">Ice</span> Sheet. For the first time, we prove the occurrence of seasonal sea <span class="hlt">ice</span> at the eastern Yermak Plateau during glacial intervals, probably steered by a major northward advance of the <span class="hlt">ice</span> sheet and the formation of a coastal polynya in front of it. Maximum accumulation of terrigenous organic carbon, IP25 and the phytoplankton biomarkers (brassicasterol, dinosterol, HBI III) can be correlated to distinct deglaciation events. More severe, but <span class="hlt">variable</span> sea <span class="hlt">ice</span> cover prevailed at the Yermak Plateau during interglacials. The general proximity to the sea <span class="hlt">ice</span> margin is further indicated by biomarker (GDGT) - based sea surface temperatures below 2.5 °C.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRE..122.2250B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRE..122.2250B"><span>Preservation of Midlatitude <span class="hlt">Ice</span> Sheets on Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bramson, A. M.; Byrne, S.; Bapst, J.</p> <p>2017-11-01</p> <p>Excess <span class="hlt">ice</span> with a minimum age of tens of millions of years is widespread in Arcadia Planitia on Mars, and a similar deposit has been found in Utopia Planitia. The conditions that led to the formation and preservation of these midlatitude <span class="hlt">ice</span> sheets hold clues to past climate and subsurface structure on Mars. We simulate the thermal stability and retreat of buried excess <span class="hlt">ice</span> sheets over 21 Myr of Martian orbital solutions and find that the <span class="hlt">ice</span> sheets can be orders of magnitude older than the obliquity cycles that are typically thought to drive midlatitude <span class="hlt">ice</span> deposition and sublimation. Retreat of this <span class="hlt">ice</span> in the last 4 Myr could have contributed 6% of the <span class="hlt">volume</span> of the north polar layered deposits (NPLD) and more than 10% if the NPLD are older than 4 Myr. Matching the measured dielectric constants of the Arcadia and Utopia Planitia deposits requires <span class="hlt">ice</span> porosities of 25-35%. We model geothermally driven vapor migration through porous <span class="hlt">ice</span> under Martian temperatures and find that Martian firn may be able to maintain porosity for timescales longer than we predict for retreat of the <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4031135','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4031135"><span>An Improved Model for Nucleation-Limited <span class="hlt">Ice</span> Formation in Living Cells during Freezing</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zhao, Gang; He, Xiaoming</p> <p>2014-01-01</p> <p><span class="hlt">Ice</span> formation in living cells is a lethal event during freezing and its characterization is important to the development of optimal protocols for not only cryopreservation but also cryotherapy applications. Although the model for probability of <span class="hlt">ice</span> formation (PIF) in cells developed by Toner et al. has been widely used to predict nucleation-limited intracellular <span class="hlt">ice</span> formation (IIF), our data of freezing Hela cells suggest that this model could give misleading prediction of PIF when the maximum PIF in cells during freezing is less than 1 (PIF ranges from 0 to 1). We introduce a new model to overcome this problem by incorporating a critical cell <span class="hlt">volume</span> to modify the Toner's original model. We further reveal that this critical cell <span class="hlt">volume</span> is dependent on the mechanisms of <span class="hlt">ice</span> nucleation in cells during freezing, i.e., surface-catalyzed nucleation (SCN) and <span class="hlt">volume</span>-catalyzed nucleation (VCN). Taken together, the improved PIF model may be valuable for better understanding of the mechanisms of <span class="hlt">ice</span> nucleation in cells during freezing and more accurate prediction of PIF for cryopreservation and cryotherapy applications. PMID:24852166</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19005552','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19005552"><span>Transient nature of late Pleistocene climate <span class="hlt">variability</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Crowley, Thomas J; Hyde, William T</p> <p>2008-11-13</p> <p>Climate in the early Pleistocene varied with a period of 41 kyr and was related to variations in Earth's obliquity. About 900 kyr ago, <span class="hlt">variability</span> increased and oscillated primarily at a period of approximately 100 kyr, suggesting that the link was then with the eccentricity of Earth's orbit. This transition has often been attributed to a nonlinear response to small changes in external boundary conditions. Here we propose that increasing variablility within the past million years may indicate that the climate system was approaching a second climate bifurcation point, after which it would transition again to a new stable state characterized by permanent mid-latitude Northern Hemisphere glaciation. From this perspective the past million years can be viewed as a transient interval in the evolution of Earth's climate. We support our hypothesis using a coupled energy-balance/<span class="hlt">ice</span>-sheet model, which furthermore predicts that the future transition would involve a large expansion of the Eurasian <span class="hlt">ice</span> sheet. The process responsible for the abrupt change seems to be the albedo discontinuity at the snow-<span class="hlt">ice</span> edge. The best-fit model run, which explains almost 60% of the variance in global <span class="hlt">ice</span> <span class="hlt">volume</span> during the past 400 kyr, predicts a rapid transition in the geologically near future to the proposed glacial state. Should it be attained, this state would be more 'symmetric' than the present climate, with comparable areas of <span class="hlt">ice/sea-ice</span> cover in each hemisphere, and would represent the culmination of 50 million years of evolution from bipolar nonglacial climates to bipolar glacial climates.</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 <span class="hlt">volume</span> 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 content 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 <span class="hlt">volume</span> 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 content 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('http://adsabs.harvard.edu/abs/1992JGR....9720325W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992JGR....9720325W"><span>Relationship between sea <span class="hlt">ice</span> freeboard and draft in the Arctic Basin, and implications for <span class="hlt">ice</span> thickness monitoring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wadhams, P.; Tucker, W. B.; Krabill, W. B.; Swift, R. N.; Comiso, J. C.; Davis, N. R.</p> <p>1992-12-01</p> <p>We have confirmed our earlier finding that the probability density function (pdf) of <span class="hlt">ice</span> freeboard in the Arctic Ocean can be converted to a pdf of <span class="hlt">ice</span> draft by applying a simple coordinate transformation based on the measured mean draft and mean elevation. This applies in each of six 50-km sections (north of Greenland) of joint airborne laser and submarine sonar profile obtained along nearly coincident tracks from the Arctic Basin north of Greenland and tested for this study. Detailed differences in the shape of the pdf can be explained on the basis of snow load and can, in principle, be compensated by the use of a more sophisticated freeboard-dependent transformation. The measured "density ratio" R (actually mean draft/mean elevation ratio) for each section was found to be consistent over all sections tested, despite differences in the <span class="hlt">ice</span> regime, indicating that a single value of R might be used for measurements done in this season of the year. The mean value <R> from all six sections is 7.89; on the assumption that all six values are drawn from the same population, the standard deviation is 0.55 for a single 50-km section, and thus 0.22 for 300 km of track. In attempting to infer <span class="hlt">ice</span> draft from laser-measured freeboard, we would therefore expect an accuracy of about ±28 cm in 50 km of track (if mean draft is about 4 m) and about ±11 cm in 300 km of track; these accuracies are compatible with the resolution of predictions from numerical models. A simple model for the <span class="hlt">variability</span> of R with season and with mean <span class="hlt">ice</span> thickness gives results in reasonable agreement with observations. They show that although there is a large seasonal <span class="hlt">variability</span> due to snow load, there is a stable period from November to April when the <span class="hlt">variability</span> is chiefly dependent on the mean <span class="hlt">ice</span> thickness alone. Thus, in principle, R can be mapped over the Arctic Ocean as a basis for interpreting survey data. Better field data are needed on the seasonal and spatial <span class="hlt">variability</span> of three key</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Natur.541...72B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Natur.541...72B"><span>Centennial-scale Holocene climate variations amplified by Antarctic <span class="hlt">Ice</span> Sheet discharge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bakker, Pepijn; Clark, Peter U.; Golledge, Nicholas R.; Schmittner, Andreas; Weber, Michael E.</p> <p>2017-01-01</p> <p>Proxy-based indicators of past climate change show that current global climate models systematically underestimate Holocene-epoch climate <span class="hlt">variability</span> on centennial to multi-millennial timescales, with the mismatch increasing for longer periods. Proposed explanations for the discrepancy include ocean-atmosphere coupling that is too weak in models, insufficient energy cascades from smaller to larger spatial and temporal scales, or that global climate models do not consider slow climate feedbacks related to the carbon cycle or interactions between <span class="hlt">ice</span> sheets and climate. Such interactions, however, are known to have strongly affected centennial- to orbital-scale climate <span class="hlt">variability</span> during past glaciations, and are likely to be important in future climate change. Here we show that fluctuations in Antarctic <span class="hlt">Ice</span> Sheet discharge caused by relatively small changes in subsurface ocean temperature can amplify multi-centennial climate <span class="hlt">variability</span> regionally and globally, suggesting that a dynamic Antarctic <span class="hlt">Ice</span> Sheet may have driven climate fluctuations during the Holocene. We analysed high-temporal-resolution records of iceberg-rafted debris derived from the Antarctic <span class="hlt">Ice</span> Sheet, and performed both high-spatial-resolution <span class="hlt">ice</span>-sheet modelling of the Antarctic <span class="hlt">Ice</span> Sheet and multi-millennial global climate model simulations. <span class="hlt">Ice</span>-sheet responses to decadal-scale ocean forcing appear to be less important, possibly indicating that the future response of the Antarctic <span class="hlt">Ice</span> Sheet will be governed more by long-term anthropogenic warming combined with multi-centennial natural <span class="hlt">variability</span> than by annual or decadal climate oscillations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140011454','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011454"><span>Hydrogen-Bonding Surfaces for <span class="hlt">Ice</span> Mitigation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smith, Joseph G., Jr.; Wohl, Christopher J.; Kreeger, Richard E.; Hadley, Kevin R.; McDougall, Nicholas</p> <p>2014-01-01</p> <p><span class="hlt">Ice</span> formation on aircraft, either on the ground or in-flight, is a major safety issue. While ground <span class="hlt">icing</span> events occur predominantly during the winter months, in-flight <span class="hlt">icing</span> can happen anytime during the year. The latter is more problematic since it could result in increased drag and loss of lift. Under a Phase I ARMD NARI Seedling Activity, coated aluminum surfaces possessing hydrogen-bonding groups were under investigation for mitigating <span class="hlt">ice</span> formation. Hydroxyl and methyl terminated dimethylethoxysilanes were prepared via known chemistries and characterized by spectroscopic methods. These materials were subsequently used to coat aluminum surfaces. Surface compositions were based on pure hydroxyl and methyl terminated species as well as mixtures of the two. Coated surfaces were characterized by contact angle goniometry. Receding water contact angle data suggested several potential surfaces that may exhibit reduced <span class="hlt">ice</span> adhesion. Qualitative <span class="hlt">icing</span> experiments performed under representative environmental temperatures using supercooled distilled water delivered via spray coating were inconclusive. Molecular modeling studies suggested that chain mobility affected the interface between <span class="hlt">ice</span> and the surface more than terminal group chemical composition. Chain mobility resulted from the creation of "pockets" of increased free <span class="hlt">volume</span> for longer chains to occupy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGP34A..07G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGP34A..07G"><span>Experiments in <span class="hlt">Ice</span> Contaminant Remanent Magnetization of Dusty Frost Deposits</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grossman, Y.; Aharonson, O.; Shaar, R.</p> <p>2017-12-01</p> <p>Sedimentary rocks can acquire magnetization in the presence of an external field as grains settle out of suspension in a water column - a process known as Depositional Remanent Magnetization (DRM). In analogy with this, here we propose and experimentally demonstrate a new mechanism for acquisition of magnetization by <span class="hlt">ice</span> and particulate mixtures which we term <span class="hlt">Ice</span> Contaminant Remanent Magnetization (ICRM). This phenomenon results from the settling of atmospheric dust containing magnetic particles (e.g. magnetite or other iron oxides). Upon freezing, magnetic dust particles assume a preferential orientation that depends on the external planetary field, resulting in bulk magnetization of the dusty <span class="hlt">ice</span>. Hence over geologic timescales, the <span class="hlt">ice</span> stratigraphy is expected to record the geomagnetic history. To test this hypothesis, we designed a set of experiments in which mixtures of <span class="hlt">ice</span> and dust were deposited in a controlled ambient magnetic field environment. We measured the ratio between the <span class="hlt">volume</span> normalized magnetization of the dusty <span class="hlt">ice</span> (m) and the applied field (H) during deposition of the mixture, which is expressed as the effective ICRM susceptibility: m=χICRMH. A magnetic field was applied by a 3-axis Helmholtz coil at the Weizmann Simulating Planetary <span class="hlt">Ices</span> & Environments Laboratory, and the frozen samples were analyzed in a 2G-Entreprises SQUID Rock Magnetometer at the Hebrew University Institute for Earth Sciences. We measured a clear correlation in amplitude and direction between the ambient magnetic field applied during deposition and the remanent magnetic moment of the resulting samples. We studied various concentrations and particle sizes (diameters 5 µm to 50 µm) of iron and magnetite particles. Effective bulk susceptibilities show a range of values, starting from 10-3 and up to values that saturate the analytical instrument. Our preliminary results indicate that natural <span class="hlt">ice</span> deposits may acquire <span class="hlt">variable</span> magnetization due to ICRM, which may in turn be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1611876G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1611876G"><span>Towards an <span class="hlt">Ice</span>-Free Arctic Ocean in Summertime</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gascard, Jean Claude</p> <p>2014-05-01</p> <p>Dividing the Arctic Ocean in two parts, the so-called Atlantic versus the Pacific sector, two distinct modes of <span class="hlt">variability</span> appear for characterizing the Arctic sea-<span class="hlt">ice</span> extent from 70°N up to 80°N in both sectors. The Atlantic sector seasonal sea-<span class="hlt">ice</span> extent is characterized by a longer time scale than the Pacific sector with a break up melting season starting in May and reaching a peak in June-July, one month earlier than the Pacific sector of the Arctic Ocean revealing a faster time evolution and a larger spatial amplitude than the Atlantic sector. During recent years like 2007, sea-<span class="hlt">ice</span> extent with sea-<span class="hlt">ice</span> concentration above 15% retreated from 4 millions km2 to about 1 million km2 in the Arctic Pacific sector between 70° and 80°N except for 2012 when most of sea-<span class="hlt">ice</span> melted away in this region. That explained most of the differences between the two extreme years 2007 and 2012. In the Atlantic sector, Arctic sea-<span class="hlt">ice</span> retreated from 2 millions km2 to nearly 0 during recent years including 2007 and 2012. The Atlantic inflow North of Svalbard and Franz Josef Land is more likely responsible for a northward retreat of the <span class="hlt">ice</span> edge in that region. The important factor is not only that the Arctic summer sea-<span class="hlt">ice</span> minimum extent decreased by 3 or 4 millions km2 over the past 10 years but also that the melting period was steadily increasing by one to two days every year during that period. An important factor concerns the strength of the freezing that can be quantified in terms of Freezing Degree Days FDD accumulated during the winter-spring season and the strength of the melting (MDD) that can be accumulated during the summer season. FDD and MDD have been calculated for the past 30 years all over the Arctic Ocean using ERA Interim Reanalysis surface temperature at 2m height in the atmosphere. It is clear that FDD decreased significantly by more than 2000 FDD between 1980 and 2012 which is equivalent to the sensible heat flux corresponding to more than a meter of sea-<span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeoRL..41.2411S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeoRL..41.2411S"><span>Predicting September sea <span class="hlt">ice</span>: Ensemble skill of the SEARCH Sea <span class="hlt">Ice</span> Outlook 2008-2013</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stroeve, Julienne; Hamilton, Lawrence C.; Bitz, Cecilia M.; Blanchard-Wrigglesworth, Edward</p> <p>2014-04-01</p> <p>Since 2008, the Study of Environmental Arctic Change Sea <span class="hlt">Ice</span> Outlook has solicited predictions of September sea-<span class="hlt">ice</span> extent from the Arctic research community. Individuals and teams employ a variety of modeling, statistical, and heuristic approaches to make these predictions. Viewed as monthly ensembles each with one or two dozen individual predictions, they display a bimodal pattern of success. In years when observed <span class="hlt">ice</span> extent is near its trend, the median predictions tend to be accurate. In years when the observed extent is anomalous, the median and most individual predictions are less accurate. Statistical analysis suggests that year-to-year <span class="hlt">variability</span>, rather than methods, dominate the variation in ensemble prediction success. Furthermore, ensemble predictions do not improve as the season evolves. We consider the role of initial <span class="hlt">ice</span>, atmosphere and ocean conditions, and summer storms and weather in contributing to the challenge of sea-<span class="hlt">ice</span> prediction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4366H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4366H"><span>Deciphering the evolution of the last Eurasian <span class="hlt">ice</span> sheets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hughes, Anna; Gyllencreutz, Richard; Mangerud, Jan; Svendsen, John Inge</p> <p>2016-04-01</p> <p>Glacial geologists need <span class="hlt">ice</span> sheet-scale chronological reconstructions of former <span class="hlt">ice</span> extent to set individual records in a wider context and compare interpretations of <span class="hlt">ice</span> sheet response to records of past environmental changes. <span class="hlt">Ice</span> sheet modellers require empirical reconstructions on size and <span class="hlt">volume</span> of past <span class="hlt">ice</span> sheets that are fully documented, specified in time and include uncertainty estimates for model validation or constraints. Motivated by these demands, in 2005 we started a project (Database of the Eurasian Deglaciation, DATED) to compile and archive all published dates relevant to constraining the build-up and retreat of the last Eurasian <span class="hlt">ice</span> sheets, including the British-Irish, Scandinavian and Svalbard-Barents-Kara Seas <span class="hlt">ice</span> sheets (BIIS, SIS and SBKIS respectively). Over 5000 dates were assessed for reliability and used together with published <span class="hlt">ice</span>-sheet margin positions to reconstruct time-slice maps of the <span class="hlt">ice</span> sheets' extent, with uncertainty bounds, every 1000 years between 25-10 kyr ago and at four additional periods back to 40 kyr ago. Ten years after the idea for a database was conceived, the first version of results (DATED-1) has now been released (Hughes et al. 2016). We observe that: i) both the BIIS and SBKIS achieve maximum extent, and commence retreat earlier than the larger SIS; ii) the eastern terrestrial margin of the SIS reached its maximum extent up to 7000 years later than the westernmost marine margin; iii) the combined maximum <span class="hlt">ice</span> <span class="hlt">volume</span> (~24 m sea-level equivalent) was reached c. 21 ka; iv) large uncertainties exist; predominantly across marine sectors (e.g. the timing of coalescence and separation of the SIS and BKIS) but also in well-studied areas due to conflicting yet equally robust data. In just three years since the DATED-1 census (1 January 2013), the <span class="hlt">volume</span> of new information (from both dates and mapped glacial geomorphology) has grown significantly (~1000 new dates). Here, we present the DATED-1 results in the context of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730023097','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730023097"><span><span class="hlt">Ice</span> pack heat sink subsystem - phase 1, <span class="hlt">volume</span> 2</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roebelen, G. J., Jr.</p> <p>1973-01-01</p> <p>The design, development, and test of a functional laboratory model <span class="hlt">ice</span> pack heat sink subsystem are discussed. Operating instructions to include mechanical and electrical schematics, maintenance instructions, and equipment specifications are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27660738','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27660738"><span>Influence of <span class="hlt">ice</span> thickness and surface properties on light transmission through Arctic sea <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Katlein, Christian; Arndt, Stefanie; Nicolaus, Marcel; Perovich, Donald K; Jakuba, Michael V; Suman, Stefano; Elliott, Stephen; Whitcomb, Louis L; McFarland, Christopher J; Gerdes, Rüdiger; Boetius, Antje; German, Christopher R</p> <p>2015-09-01</p> <p>The observed changes in physical properties of sea <span class="hlt">ice</span> such as decreased thickness and increased melt pond cover severely impact the energy budget of Arctic sea <span class="hlt">ice</span>. Increased light transmission leads to increased deposition of solar energy in the upper ocean and thus plays a crucial role for amount and timing of sea-<span class="hlt">ice</span>-melt and under-<span class="hlt">ice</span> primary production. Recent developments in underwater technology provide new opportunities to study light transmission below the largely inaccessible underside of sea <span class="hlt">ice</span>. We measured spectral under-<span class="hlt">ice</span> radiance and irradiance using the new Nereid Under-<span class="hlt">Ice</span> (NUI) underwater robotic vehicle, during a cruise of the R/V Polarstern to 83°N 6°W in the Arctic Ocean in July 2014. NUI is a next generation hybrid remotely operated vehicle (H-ROV) designed for both remotely piloted and autonomous surveys underneath land-fast and moving sea <span class="hlt">ice</span>. Here we present results from one of the first comprehensive scientific dives of NUI employing its interdisciplinary sensor suite. We combine under-<span class="hlt">ice</span> optical measurements with three dimensional under-<span class="hlt">ice</span> topography (multibeam sonar) and aerial images of the surface conditions. We investigate the influence of spatially varying <span class="hlt">ice</span>-thickness and surface properties on the spatial <span class="hlt">variability</span> of light transmittance during summer. Our results show that surface properties such as melt ponds dominate the spatial distribution of the under-<span class="hlt">ice</span> light field on small scales (<1000 m 2 ), while sea <span class="hlt">ice</span>-thickness is the most important predictor for light transmission on larger scales. In addition, we propose the use of an algorithm to obtain histograms of light transmission from distributions of sea <span class="hlt">ice</span> thickness and surface albedo.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003226','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003226"><span>Does a Relationship Between Arctic Low Clouds and Sea <span class="hlt">Ice</span> Matter?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Taylor, Patrick C.</p> <p>2016-01-01</p> <p>Arctic low clouds strongly affect the Arctic surface energy budget. Through this impact Arctic low clouds influence important aspects of the Arctic climate system, namely surface and atmospheric temperature, sea <span class="hlt">ice</span> extent and thickness, and atmospheric circulation. Arctic clouds are in turn influenced by these elements of the Arctic climate system, and these interactions create the potential for Arctic cloud-climate feedbacks. To further our understanding of potential Arctic cloudclimate feedbacks, the goal of this paper is to quantify the influence of atmospheric state on the surface cloud radiative effect (CRE) and its covariation with sea <span class="hlt">ice</span> concentration (SIC). We build on previous research using instantaneous, active remote sensing satellite footprint data from the NASA A-Train. First, the results indicate significant differences in the surface CRE when stratified by atmospheric state. Second, there is a weak covariation between CRE and SIC for most atmospheric conditions. Third, the results show statistically significant differences in the average surface CRE under different SIC values in fall indicating a 3-5 W m(exp -2) larger LW CRE in 0% versus 100% SIC footprints. Because systematic changes on the order of 1 W m(exp -2) are sufficient to explain the observed long-term reductions in sea <span class="hlt">ice</span> extent, our results indicate a potentially significant amplifying sea <span class="hlt">ice</span>-cloud feedback, under certain meteorological conditions, that could delay the fall freeze-up and influence the <span class="hlt">variability</span> in sea <span class="hlt">ice</span> extent and <span class="hlt">volume</span>. Lastly, a small change in the frequency of occurrence of atmosphere states may yield a larger Arctic cloud feedback than any cloud response to sea <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10583952','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10583952"><span>Global Warming and Northern Hemisphere Sea <span class="hlt">Ice</span> Extent.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vinnikov; Robock; Stouffer; Walsh; Parkinson; Cavalieri; Mitchell; Garrett; Zakharov</p> <p>1999-12-03</p> <p>Surface and satellite-based observations show a decrease in Northern Hemisphere sea <span class="hlt">ice</span> extent during the past 46 years. A comparison of these trends to control and transient integrations (forced by observed greenhouse gases and tropospheric sulfate aerosols) from the Geophysical Fluid Dynamics Laboratory and Hadley Centre climate models reveals that the observed decrease in Northern Hemisphere sea <span class="hlt">ice</span> extent agrees with the transient simulations, and both trends are much larger than would be expected from natural climate variations. From long-term control runs of climate models, it was found that the probability of the observed trends resulting from natural climate <span class="hlt">variability</span>, assuming that the models' natural <span class="hlt">variability</span> is similar to that found in nature, is less than 2 percent for the 1978-98 sea <span class="hlt">ice</span> trends and less than 0.1 percent for the 1953-98 sea <span class="hlt">ice</span> trends. Both models used here project continued decreases in sea <span class="hlt">ice</span> thickness and extent throughout the next century.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030102176','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030102176"><span>30-Year Satellite Record Reveals Contrasting Arctic and Antarctic Decadal Sea <span class="hlt">Ice</span> <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cavalieri, D. J.; Parkinson, C. L.; Vinnikov, K. Y.</p> <p>2003-01-01</p> <p>A 30-year satellite record of sea <span class="hlt">ice</span> extents derived mostly from satellite microwave radiometer observations reveals that the Arctic sea <span class="hlt">ice</span> extent decreased by 0.30+0.03 x 10(exp 6) square kilometers per 10 yr from 1972 through 2002, but by 0.36 plus or minus 0.05 x 10(exp 6) square kilometers per 10yr from 1979 through 2002, indicating an acceleration of 20% in the rate of decrease. In contrast, the Antarctic sea <span class="hlt">ice</span> extent decreased dramatically over the period 1973-1977, then gradually increased. Over the full 30-year period, the Antarctic <span class="hlt">ice</span> extent decreased by 0.15 plus or minus 0.08 x 10(exp 6) square kilometers per 10 yr. The trend reversal is attributed to a large positive anomaly in Antarctic sea <span class="hlt">ice</span> extent in the early 1970's, an anomaly that apparently began in the late 1960's, as observed in early visible and infrared satellite images.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMPP21B1327O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMPP21B1327O"><span><span class="hlt">Ice</span> Core Records of Recent Northwest Greenland Climate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Osterberg, E. C.; Wong, G. J.; Ferris, D.; Lutz, E.; Howley, J. A.; Kelly, M. A.; Axford, Y.; Hawley, R. L.</p> <p>2014-12-01</p> <p>Meteorological station data from NW Greenland indicate a 3oC temperature rise since 1990, with most of the warming occurring in fall and winter. According to remote sensing data, the NW Greenland <span class="hlt">ice</span> sheet (GIS) and coastal <span class="hlt">ice</span> caps are responding with <span class="hlt">ice</span> mass loss and margin retreat, but the cryosphere's response to previous climate <span class="hlt">variability</span> is poorly constrained in this region. We are developing multi-proxy records (lake sediment cores, <span class="hlt">ice</span> cores, glacial geologic data, glaciological models) of Holocene climate change and cryospheric response in NW Greenland to improve projections of future <span class="hlt">ice</span> loss and sea level rise in a warming climate. As part of our efforts to develop a millennial-length <span class="hlt">ice</span> core paleoclimate record from the Thule region, we collected and analyzed snow pit samples and short firn cores (up to 21 m) from the coastal region of the GIS (2Barrel site; 76.9317o N, 63.1467o W, 1685 m el.) and the summit of North <span class="hlt">Ice</span> Cap (76.938o N, 67.671o W, 1273 m el.) in 2011, 2012 and 2014. The 2Barrel <span class="hlt">ice</span> core record has statistically significant relationships with regional spring and fall Baffin Bay sea <span class="hlt">ice</span> extent, summertime temperature, and annual precipitation. Here we evaluate relationships between the 2014 North <span class="hlt">Ice</span> Cap firn core glaciochemical record and climate <span class="hlt">variability</span> from regional instrumental stations and reanalysis datasets. We compare the coastal North <span class="hlt">Ice</span> Cap record to more inland records from 2Barrel, Camp Century and NEEM to evaluate spatial and elevational gradients in recent NW Greenland climate change.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23246475','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23246475"><span>Controlled <span class="hlt">ice</span> nucleation in cryopreservation--a review.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Morris, G John; Acton, Elizabeth</p> <p>2013-04-01</p> <p>We review here for the first time, the literature on control of <span class="hlt">ice</span> nucleation in cryopreservation. Water and aqueous solutions have a tendency to undercool before <span class="hlt">ice</span> nucleation occurs. Control of <span class="hlt">ice</span> nucleation has been recognised as a critical step in the cryopreservation of embryos and oocytes but is largely ignored for other cell types. We review the processes of <span class="hlt">ice</span> nucleation and crystal growth in the solution around cells and tissues during cryopreservation with an emphasis on non IVF applications. The extent of undercooling that is encountered during the cooling of various cryocontainers is defined and the methods that have been employed to control the nucleation of <span class="hlt">ice</span> are examined. The effects of controlled <span class="hlt">ice</span> nucleation on the structure of the sample and the outcome of cryopreservation of a range of cell types and tissues are presented and the physical events which define the cellular response are discussed. Nucleation of <span class="hlt">ice</span> is the most significant uncontrolled <span class="hlt">variable</span> in conventional cryopreservation leading to sample to sample variation in cell recovery, viability and function and should be controlled to allow standardisation of cryopreservation protocols for cells for biobanking, cell based assays or clinical application. This intervention allows a way of increasing viability of cells and reducing <span class="hlt">variability</span> between samples and should be included as standard operating procedures are developed. Copyright © 2012 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160004215&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160004215&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dsea"><span>How Will Sea <span class="hlt">Ice</span> Loss Affect the Greenland <span class="hlt">Ice</span> Sheet? On the Puzzling Features of Greenland <span class="hlt">Ice</span>-Core Isotopic Composition</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pausata, Francesco S. R.; Legrande, Allegra N.; Roberts, William H. G.</p> <p>2016-01-01</p> <p>The modern cryosphere, Earth's frozen water regime, is in fast transition. Greenland <span class="hlt">ice</span> cores show how fast theses changes can be, presenting evidence of up to 15 C warming events over timescales of less than a decade. These events, called Dansgaard/Oeschger (D/O) events, are believed to be associated with rapid changes in Arctic sea <span class="hlt">ice</span>, although the underlying mechanisms are still unclear. The modern demise of Arctic sea <span class="hlt">ice</span> may, in turn, instigate abrupt changes on the Greenland <span class="hlt">Ice</span> Sheet. The Arctic Sea <span class="hlt">Ice</span> and Greenland <span class="hlt">Ice</span> Sheet Sensitivity (<span class="hlt">Ice</span>2<span class="hlt">Ice</span> Chttps://<span class="hlt">ice</span>2<span class="hlt">ice</span>.b.uib.noD) initiative, sponsored by the European Research Council, seeks to quantify these past rapid changes to improve our understanding of what the future may hold for the Arctic. Twenty scientists gathered in Copenhagen as part of this initiative to discuss the most recent observational, technological, and model developments toward quantifying the mechanisms behind past climate changes in Greenland. Much of the discussion focused on the causes behind the changes in stable water isotopes recorded in <span class="hlt">ice</span> cores. The participants discussed sources of <span class="hlt">variability</span> for stable water isotopes and framed ways that new studies could improve understanding of modern climate. The participants also discussed how climate models could provide insights into the relative roles of local and nonlocal processes in affecting stable water isotopes within the Greenland <span class="hlt">Ice</span> Sheet. Presentations of modeling results showed how a change in the source or seasonality of precipitation could occur not only between glacial and modern climates but also between abrupt events. Recent fieldwork campaigns illustrate an important role of stable isotopes in atmospheric vapor and diffusion in the final stable isotope signal in <span class="hlt">ice</span>. Further, indications from recent fieldwork campaigns illustrate an important role of stable isotopes in atmospheric vapor and diffusion in the final stable isotope signal in <span class="hlt">ice</span>. This feature complicates</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070021400&hterms=relationships&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D50%26Ntt%3Drelationships','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070021400&hterms=relationships&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D50%26Ntt%3Drelationships"><span>Spatial <span class="hlt">Variability</span> of Barrow-Area Shore-Fast Sea <span class="hlt">Ice</span> and Its Relationships to Passive Microwave Emissivity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Maslanik, J. A.; Rivas, M. Belmonte; Holmgren, J.; Gasiewski, A. J.; Heinrichs, J. F.; Stroeve, J. C.; Klein, M.; Markus, T.; Perovich, D. K.; Sonntag, J. G.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20070021400'); toggleEditAbsImage('author_20070021400_show'); toggleEditAbsImage('author_20070021400_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20070021400_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20070021400_hide"></p> <p>2006-01-01</p> <p>Aircraft-acquired passive microwave data, laser radar height observations, RADARSAT synthetic aperture radar imagery, and in situ measurements obtained during the AMSR-<span class="hlt">Ice</span>03 experiment are used to investigate relationships between microwave emission and <span class="hlt">ice</span> characteristics over several space scales. The data fusion allows delineation of the shore-fast <span class="hlt">ice</span> and pack <span class="hlt">ice</span> in the Barrow area, AK, into several <span class="hlt">ice</span> classes. Results show good agreement between observed and Polarimetric Scanning Radiometer (PSR)-derived snow depths over relatively smooth <span class="hlt">ice</span>, with larger differences over ridged and rubbled <span class="hlt">ice</span>. The PSR results are consistent with the effects on snow depth of the spatial distribution and nature of <span class="hlt">ice</span> roughness, ridging, and other factors such as <span class="hlt">ice</span> age. Apparent relationships exist between <span class="hlt">ice</span> roughness and the degree of depolarization of emission at 10,19, and 37 GHz. This depolarization .would yield overestimates of total <span class="hlt">ice</span> concentration using polarization-based algorithms, with indications of this seen when the NT-2 algorithm is applied to the PSR data. Other characteristics of the microwave data, such as effects of grounding of sea <span class="hlt">ice</span> and large contrast between sea <span class="hlt">ice</span> and adjacent land, are also apparent in the PSR data. Overall, the results further demonstrate the importance of macroscale <span class="hlt">ice</span> roughness conditions such as ridging and rubbling on snow depth and microwave emissivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070010003&hterms=time+zone&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dtime%2Bzone','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070010003&hterms=time+zone&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dtime%2Bzone"><span>Contrasts in Sea <span class="hlt">Ice</span> Formation and Production in the Arctic Seasonal and Perennial <span class="hlt">Ice</span> Zones</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kwok, R.</p> <p>2006-01-01</p> <p>Four years (1997-2000) of RADARSAT Geophysical Processor System (RGPS) data are used to contrast the sea <span class="hlt">ice</span> deformation and production regionally, and in the seasonal (SIZ) and perennial (PIZ) <span class="hlt">ice</span> zones. <span class="hlt">Ice</span> production is of seasonal <span class="hlt">ice</span> in openings during the winter. 3-day estimates of these quantities are provided within Lagrangian elements initially 10 km on a side. A distinct seasonal cycle is seen in both zones with these estimates highest in the late fall and with seasonal minimums in the mid-winter. Regional divergence over the winter could be up to 30%. Spatially, the highest deformation is in the SIZ north of coastal Alaska. Both <span class="hlt">ice</span> deformation and production are higher in the SIZ: deformation-related <span class="hlt">ice</span> production in the SIZ (approx.0.5 m) is 1.5-2.3 times that of the PIZ (approx.0.3 m) - this is connected to <span class="hlt">ice</span> strength and thickness. Atmospheric forcing and boundary layer structure contribute to only the seasonal and interannual <span class="hlt">variability</span>. Seasonal <span class="hlt">ice</span> growth in <span class="hlt">ice</span> fractures accounts for approx.25-40% of the total <span class="hlt">ice</span> production of the Arctic Ocean. By itself, this deformation-<span class="hlt">ice</span> production relationship could be considered a negative feedback when thickness is perturbed. However, the overall effect on <span class="hlt">ice</span> production in the face of increasing seasonal and thinner/weaker <span class="hlt">ice</span> coverage could be modified by: local destabilization of the water column promoting overturning of warmer water due to increased brine rejection; and, the upwelling of the pynocline associated with increased occurrence of large shear motion in sea <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016OcMod..97...65D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OcMod..97...65D"><span>North Atlantic simulations in Coordinated Ocean-<span class="hlt">ice</span> Reference Experiments phase II (CORE-II). Part II: Inter-annual to decadal <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Danabasoglu, Gokhan; Yeager, Steve G.; Kim, Who M.; Behrens, Erik; Bentsen, Mats; Bi, Daohua; Biastoch, Arne; Bleck, Rainer; Böning, Claus; Bozec, Alexandra; Canuto, Vittorio M.; Cassou, Christophe; Chassignet, Eric; Coward, Andrew C.; Danilov, Sergey; Diansky, Nikolay; Drange, Helge; Farneti, Riccardo; Fernandez, Elodie; Fogli, Pier Giuseppe; Forget, Gael; Fujii, Yosuke; Griffies, Stephen M.; Gusev, Anatoly; Heimbach, Patrick; Howard, Armando; Ilicak, Mehmet; Jung, Thomas; Karspeck, Alicia R.; Kelley, Maxwell; Large, William G.; Leboissetier, Anthony; Lu, Jianhua; Madec, Gurvan; Marsland, Simon J.; Masina, Simona; Navarra, Antonio; Nurser, A. J. George; Pirani, Anna; Romanou, Anastasia; Salas y Mélia, David; Samuels, Bonita L.; Scheinert, Markus; Sidorenko, Dmitry; Sun, Shan; Treguier, Anne-Marie; Tsujino, Hiroyuki; Uotila, Petteri; Valcke, Sophie; Voldoire, Aurore; Wang, Qiang; Yashayaev, Igor</p> <p>2016-01-01</p> <p>Simulated inter-annual to decadal <span class="hlt">variability</span> and trends in the North Atlantic for the 1958-2007 period from twenty global ocean - sea-<span class="hlt">ice</span> coupled models are presented. These simulations are performed as contributions to the second phase of the Coordinated Ocean-<span class="hlt">ice</span> Reference Experiments (CORE-II). The study is Part II of our companion paper (Danabasoglu et al., 2014) which documented the mean states in the North Atlantic from the same models. A major focus of the present study is the representation of Atlantic meridional overturning circulation (AMOC) <span class="hlt">variability</span> in the participating models. Relationships between AMOC <span class="hlt">variability</span> and those of some other related <span class="hlt">variables</span>, such as subpolar mixed layer depths, the North Atlantic Oscillation (NAO), and the Labrador Sea upper-ocean hydrographic properties, are also investigated. In general, AMOC <span class="hlt">variability</span> shows three distinct stages. During the first stage that lasts until the mid- to late-1970s, AMOC is relatively steady, remaining lower than its long-term (1958-2007) mean. Thereafter, AMOC intensifies with maximum transports achieved in the mid- to late-1990s. This enhancement is then followed by a weakening trend until the end of our integration period. This sequence of low frequency AMOC <span class="hlt">variability</span> is consistent with previous studies. Regarding strengthening of AMOC between about the mid-1970s and the mid-1990s, our results support a previously identified <span class="hlt">variability</span> mechanism where AMOC intensification is connected to increased deep water formation in the subpolar North Atlantic, driven by NAO-related surface fluxes. The simulations tend to show general agreement in their temporal representations of, for example, AMOC, sea surface temperature (SST), and subpolar mixed layer depth <span class="hlt">variabilities</span>. In particular, the observed <span class="hlt">variability</span> of the North Atlantic SSTs is captured well by all models. These findings indicate that simulated <span class="hlt">variability</span> and trends are primarily dictated by the atmospheric datasets which</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160008690','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160008690"><span>North Atlantic Simulations in Coordinated Ocean-<span class="hlt">Ice</span> Reference Experiments Phase II (CORE-II) . Part II; Inter-Annual to Decadal <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Danabasoglu, Gokhan; Yeager, Steve G.; Kim, Who M.; Behrens, Erik; Bentsen, Mats; Bi, Daohua; Biastoch, Arne; Bleck, Rainer; Boening, Claus; Bozec, Alexandra; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160008690'); toggleEditAbsImage('author_20160008690_show'); toggleEditAbsImage('author_20160008690_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160008690_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160008690_hide"></p> <p>2015-01-01</p> <p>Simulated inter-annual to decadal <span class="hlt">variability</span> and trends in the North Atlantic for the 1958-2007 period from twenty global ocean - sea-<span class="hlt">ice</span> coupled models are presented. These simulations are performed as contributions to the second phase of the Coordinated Ocean-<span class="hlt">ice</span> Reference Experiments (CORE-II). The study is Part II of our companion paper (Danabasoglu et al., 2014) which documented the mean states in the North Atlantic from the same models. A major focus of the present study is the representation of Atlantic meridional overturning circulation (AMOC) <span class="hlt">variability</span> in the participating models. Relationships between AMOC <span class="hlt">variability</span> and those of some other related <span class="hlt">variables</span>, such as subpolar mixed layer depths, the North Atlantic Oscillation (NAO), and the Labrador Sea upper-ocean hydrographic properties, are also investigated. In general, AMOC <span class="hlt">variability</span> shows three distinct stages. During the first stage that lasts until the mid- to late-1970s, AMOC is relatively steady, remaining lower than its long-term (1958-2007) mean. Thereafter, AMOC intensifies with maximum transports achieved in the mid- to late-1990s. This enhancement is then followed by a weakening trend until the end of our integration period. This sequence of low frequency AMOC <span class="hlt">variability</span> is consistent with previous studies. Regarding strengthening of AMOC between about the mid-1970s and the mid-1990s, our results support a previously identified <span class="hlt">variability</span> mechanism where AMOC intensification is connected to increased deep water formation in the subpolar North Atlantic, driven by NAO-related surface fluxes. The simulations tend to show general agreement in their representations of, for example, AMOC, sea surface temperature (SST), and subpolar mixed layer depth <span class="hlt">variabilities</span>. In particular, the observed <span class="hlt">variability</span> of the North Atlantic SSTs is captured well by all models. These findings indicate that simulated <span class="hlt">variability</span> and trends are primarily dictated by the atmospheric datasets which include</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970009603','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970009603"><span>Polarimetric Signatures of Sea <span class="hlt">Ice</span>. Part 1; Theoretical Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nghiem, S. V.; Kwok, R.; Yueh, S. H.; Drinkwater, M. R.</p> <p>1995-01-01</p> <p>Physical, structural, and electromagnetic properties and interrelating processes in sea <span class="hlt">ice</span> are used to develop a composite model for polarimetric backscattering signatures of sea <span class="hlt">ice</span>. Physical properties of sea <span class="hlt">ice</span> constituents such as <span class="hlt">ice</span>, brine, air, and salt are presented in terms of their effects on electromagnetic wave interactions. Sea <span class="hlt">ice</span> structure and geometry of scatterers are related to wave propagation, attenuation, and scattering. Temperature and salinity, which are determining factors for the thermodynamic phase distribution in sea <span class="hlt">ice</span>, are consistently used to derive both effective permittivities and polarimetric scattering coefficients. Polarimetric signatures of sea <span class="hlt">ice</span> depend on crystal sizes and brine <span class="hlt">volumes</span>, which are affected by <span class="hlt">ice</span> growth rates. Desalination by brine expulsion, drainage, or other mechanisms modifies wave penetration and scattering. Sea <span class="hlt">ice</span> signatures are further complicated by surface conditions such as rough interfaces, hummocks, snow cover, brine skim, or slush layer. Based on the same set of geophysical parameters characterizing sea <span class="hlt">ice</span>, a composite model is developed to calculate effective permittivities and backscattering covariance matrices at microwave frequencies for interpretation of sea <span class="hlt">ice</span> polarimetric signatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMED11D0164D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMED11D0164D"><span>Quantifying Glacier <span class="hlt">Volume</span> Change Using UAV-Derived Imagery and Structure from Motion Photogrammetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Decker, C. R.; La Frenierre, J.</p> <p>2017-12-01</p> <p>Glaciers in the Tropical Andes, like those worldwide, are experiencing rapid <span class="hlt">ice</span> <span class="hlt">volume</span> loss due to climate change. Tropical areas are of significant interest in glacier studies because they are especially sensitive to climate change. Quantifying the rate of <span class="hlt">ice</span> <span class="hlt">volume</span> loss is important given their sensitivity to climate change and the importance of glacier meltwater for downstream human use. Past studies have found shrinking <span class="hlt">ice</span> surfaces areas, but finding the actual rate of <span class="hlt">volume</span> loss gives more information about how glaciers are reacting to climate change as well as the direct hydrological effects of <span class="hlt">ice</span> <span class="hlt">volume</span> loss. In this study we determined the rate of <span class="hlt">ice</span> <span class="hlt">volume</span> loss for a debris covered section of the Reschreiter Glacier and a portion of the clean <span class="hlt">ice</span> tongue of the Hans Meyer Glacier on Volcán Chimborazo in Ecuador. Traditional geodetic approaches of measuring <span class="hlt">ice</span> <span class="hlt">volume</span> change, including the use of satellite-derived digital elevation models and airborne LIDAR, are difficult in this case due to the small size of Chimborazo's glaciers, frequently cloudy conditions, and limited local resources. Instead, we obtained imagery with an Unmanned Aerial Vehicle (UAV) and processed this imagery using Structure from Motion photogrammetry. Our results are used to evaluate the role of elevation and debris cover as Chimborazo's glaciers respond to climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920062192&hterms=Thorndike&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DThorndike','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920062192&hterms=Thorndike&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DThorndike"><span>A toy model linking atmospheric thermal radiation and sea <span class="hlt">ice</span> growth</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Thorndike, A. S.</p> <p>1992-01-01</p> <p>A simplified analytical model of sea <span class="hlt">ice</span> growth is presented where the atmosphere is in thermal radiative equilibrium with the <span class="hlt">ice</span>. This makes the downwelling longwave radiation reaching the <span class="hlt">ice</span> surface an internal <span class="hlt">variable</span> rather than a specified forcing. Analytical results demonstrate how the <span class="hlt">ice</span> state depends on properties of the <span class="hlt">ice</span> and on the externally specified climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCry....8.2409L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCry....8.2409L"><span><span class="hlt">Ice</span> and AIS: ship speed data and sea <span class="hlt">ice</span> forecasts in the Baltic Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Löptien, U.; Axell, L.</p> <p>2014-12-01</p> <p>The Baltic Sea is a seasonally <span class="hlt">ice</span>-covered marginal sea located in a densely populated area in northern Europe. Severe sea <span class="hlt">ice</span> conditions have the potential to hinder the intense ship traffic considerably. Thus, sea <span class="hlt">ice</span> fore- and nowcasts are regularly provided by the national weather services. Typically, the forecast comprises several <span class="hlt">ice</span> properties that are distributed as prognostic <span class="hlt">variables</span>, but their actual usefulness is difficult to measure, and the ship captains must determine their relative importance and relevance for optimal ship speed and safety ad hoc. The present study provides a more objective approach by comparing the ship speeds, obtained by the automatic identification system (AIS), with the respective forecasted <span class="hlt">ice</span> conditions. We find that, despite an unavoidable random component, this information is useful to constrain and rate fore- and nowcasts. More precisely, 62-67% of ship speed variations can be explained by the forecasted <span class="hlt">ice</span> properties when fitting a mixed-effect model. This statistical fit is based on a test region in the Bothnian Sea during the severe winter 2011 and employs 15 to 25 min averages of ship speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S52A..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S52A..01B"><span>Chilean Tsunami Rocks the Ross <span class="hlt">Ice</span> Shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bromirski, P. D.; Gerstoft, P.; Chen, Z.; Stephen, R. A.; Diez, A.; Arcas, D.; Wiens, D.; Aster, R. C.; Nyblade, A.</p> <p>2016-12-01</p> <p>The response of the Ross <span class="hlt">Ice</span> Shelf (RIS) to the September 16, 2015 9.3 Mb Chilean earthquake tsunami (> 75 s period) and infragravity (IG) waves (50 - 300 s period) were recorded by a broadband seismic array deployed on the RIS from November 2014 to November 2015. The array included two linear transects, one approximately orthogonal to the shelf front extending 430 km southward toward the grounding zone, and an east-west transect spanning the RIS roughly parallel to the front about 100 km south of the <span class="hlt">ice</span> edge (https://scripps.ucsd.edu/centers/iceshelfvibes/). Signals generated by both the tsunami and IG waves were recorded at all stations on floating <span class="hlt">ice</span>, with little ocean wave-induced energy reaching stations on grounded <span class="hlt">ice</span>. Cross-correlation and dispersion curve analyses indicate that tsunami and IG wave-generated signals propagate across the RIS at gravity wave speeds (about 70 m/s), consistent with coupled water-<span class="hlt">ice</span> flexural-gravity waves propagating through the <span class="hlt">ice</span> shelf from the north. Gravity wave excitation at periods > 100 s is continuously observed during the austral winter, providing mechanical excitation of the RIS throughout the year. Horizontal displacements are typically about 3 times larger than vertical displacements, producing extensional motions that could facilitate expansion of existing fractures. The vertical and horizontal spectra in the IG band attenuate exponentially with distance from the front. Tsunami model data are used to assess <span class="hlt">variability</span> of excitation of the RIS by long period gravity waves. Substantial <span class="hlt">variability</span> across the RIS roughly parallel to the front is observed, likely resulting from a combination of gravity wave amplitude <span class="hlt">variability</span> along the front, signal attenuation, incident angle of the wave forcing at the front that depends on wave generation location as well as bathymetry under and north of the shelf, and water layer and <span class="hlt">ice</span> shelf thickness and properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.5204H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.5204H"><span>The Unprecedented 2016-2017 Arctic Sea <span class="hlt">Ice</span> Growth Season: The Crucial Role of Atmospheric Rivers and Longwave Fluxes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hegyi, Bradley M.; Taylor, Patrick C.</p> <p>2018-05-01</p> <p>The 2016-2017 Arctic sea <span class="hlt">ice</span> growth season (October-March) exhibited one of the lowest values for end-of-season sea <span class="hlt">ice</span> <span class="hlt">volume</span> and extent of any year since 1979. An analysis of Modern-Era Retrospective Analysis for Research and Applications, Version 2 atmospheric reanalysis data and Clouds and the Earth's Radiant Energy System radiative flux data reveals that a record warm and moist Arctic atmosphere supported the reduced sea <span class="hlt">ice</span> growth. Numerous regional episodes of increased atmospheric temperature and moisture, transported from lower latitudes, increased the cumulative energy input from downwelling longwave surface fluxes. In those same episodes, the efficiency of the atmosphere cooling radiatively to space was reduced, increasing the amount of energy retained in the Arctic atmosphere and reradiated back toward the surface. Overall, the Arctic radiative cooling efficiency shows a decreasing trend since 2000. The results presented highlight the increasing importance of atmospheric forcing on sea <span class="hlt">ice</span> <span class="hlt">variability</span> demonstrating that episodic Arctic atmospheric rivers, regions of elevated poleward water vapor transport, and the subsequent surface energy budget response is a critical mechanism actively contributing to the evolution of Arctic sea <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP12C..06S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP12C..06S"><span>Reconstruction of the extent and <span class="hlt">variability</span> of late Quaternary <span class="hlt">ice</span> sheets and Arctic sea <span class="hlt">ice</span>: Insights from new mineralogical and geochemical proxy records</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stein, R. H.; Niessen, F.; Fahl, K.; Forwick, M.; Kudriavtseva, A.; Ponomarenko, E.; Prim, A. K.; Quatmann-Hense, A.; Spielhagen, R. F.; Zou, H.</p> <p>2016-12-01</p> <p>The Arctic Ocean and surrounding continents are key areas within the Earth system and very sensitive to present and past climate change. In this context, the timing and extent of circum-Arctic <span class="hlt">ice</span> sheets and its interaction with oceanic and sea-<span class="hlt">ice</span> dynamics are major interest and focus of international research. New sediment cores recovered during the Polarstern Expeditions PS87 (Lomonosov Ridge/2014) and PS93.1 (Fram Strait/2015) together with several sediment cores available from previous Polarstern expeditions allow to carry out a detailed sedimentological and geochemical study that may help to unravel the changes in Arctic sea <span class="hlt">ice</span> and circum-Arctic <span class="hlt">ice</span> sheets during late Quaternary times. Our new data include biomarkers indicative for past sea-<span class="hlt">ice</span> extent, phytoplankton productivity and terrigenous input as well as grain size, physical property, XRD and XRF data indicative for sources and pathways of terrigenous sediments (<span class="hlt">ice</span>-rafted debris/IRD) related to glaciations in Eurasia, East Siberia, Canada and Greenland. Here, we present examples from selected sediment cores that give new insights into the timing and extent of sea <span class="hlt">ice</span> and glaciations during MIS 6 to MIS 2. To highlight one example: SE-NW oriented, streamlined landforms have been mapped on top of the southern Lomonosov Ridge (LR) at water depths between 800 and 1000 m over long distances during Polarstern Expedition PS87, interpreted to be glacial lineations that formed beneath grounded <span class="hlt">ice</span> sheets and <span class="hlt">ice</span> streams. The orientations of the lineations identified are similar to those on the East Siberian continental margin, suggesting an East Siberian Chukchi <span class="hlt">Ice</span> Sheet extended far to the north on LR during times of extreme Quaternary glaciations. Based on our new biomarker records from Core PS2757 (located on LR near 81°N) indicating a MIS 6 <span class="hlt">ice</span>-edge situation with some open-water phytoplankton productivity, the glacial erosional event should have been older than MIS 6 (e.g., MIS 12?).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41A0644M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41A0644M"><span>Modelling of Sea <span class="hlt">Ice</span> Thermodynamics and Biogeochemistry during the N-<span class="hlt">ICE</span>2015 Expedition in the Arctic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meyer, A.; Duarte, P.; Mork Olsen, L.; Kauko, H.; Assmy, P.; Rösel, A.; Itkin, P.; Hudson, S. R.; Granskog, M. A.; Gerland, S.; Sundfjord, A.; Steen, H.; Jeffery, N.; Hunke, E. C.; Elliott, S.; Turner, A. K.</p> <p>2016-12-01</p> <p>Changes in the sea <span class="hlt">ice</span> regime of the Arctic Ocean over the last decades from a thick perennial multiyear <span class="hlt">ice</span> to a first year <span class="hlt">ice</span> have been well documented. These changes in the sea <span class="hlt">ice</span> regime will affect feedback mechanisms between the sea <span class="hlt">ice</span>, atmosphere and ocean. Here we evaluate the performance of the Los Alamos Sea <span class="hlt">Ice</span> Model (CICE), a state of the art sea <span class="hlt">ice</span> model, to predict sea <span class="hlt">ice</span> physical and biogeochemical properties at time scales of a few weeks. We also identify the most problematic prognostic <span class="hlt">variables</span> and what is necessary to improve their forecast. The availability of a complete data set of forcing collected during the Norwegian Young sea <span class="hlt">Ice</span> (N-<span class="hlt">ICE</span>-2015) expedition north of Svalbard opens the possibility to properly test CICE. Oceanographic, atmospheric, sea <span class="hlt">ice</span>, snow, and biological data were collected above, on, and below the <span class="hlt">ice</span> using R/V Lance as the base for the <span class="hlt">ice</span> camps that were drifting south towards the Fram Strait. Over six months, four different drifts took place, from the Nansen Basin, through the marginal <span class="hlt">ice</span> zone, to the open ocean. Obtained results from the model show a good performance regarding <span class="hlt">ice</span> thickness, salinity and temperature. Nutrients and sea <span class="hlt">ice</span> algae are however not modelled as accurately. We hypothesize that improvements in biogeochemical modeling may be achieved by complementing brine drainage with a diffusion parameterization and biogeochemical modeling with the introduction of an explicit formulation to forecast chlorophyll and regulate photosynthetic efficiency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC21D1124D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC21D1124D"><span>Lake Stability and Winter-Spring Transitions: Decoupled <span class="hlt">Ice</span> Duration and Winter Stratification</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Daly, J.; Dana, S.; Neal, B.</p> <p>2016-12-01</p> <p><span class="hlt">Ice</span>-out is an important historical record demonstrating the impact of warmer air temperatures on lake <span class="hlt">ice</span>. To better understand regional differences in <span class="hlt">ice</span>-out trends, to characterize the thermal dynamics of smaller mountain lakes, and to develop baseline data for Maine's high elevations landscapes, sub-hourly water temperatures have been collected in over a dozen of Maine's mountain lakes since 2010. Both surface water and hypolimnion temperature data are recorded year-round, facilitating the determination of <span class="hlt">ice</span>-in, <span class="hlt">ice</span>-out, and the duration of winter stratification. The multi-year record from sites across as 250 km transect allows us to compare spatial <span class="hlt">variability</span> related to lake morphometry and location with inter-annual <span class="hlt">variability</span> related to local weather. All of the study lakes are large enough to stratify during the summer and mix extensively during the fall. Most years, our data show that the onset of winter stratification is nearly synchronous across the study area and is associated with cold air temperatures. Winter stratification can begin days to weeks before <span class="hlt">ice</span>-in; the timing of <span class="hlt">ice</span>-in shows more <span class="hlt">variability</span>, with both elevation and basin aspect influencing the timing. <span class="hlt">Ice</span>-out shows both the anticipated spatial and interannual <span class="hlt">variability</span>; some years there is strong coherence between locations while other years show high <span class="hlt">variability</span>, possibly a function of differences in snowpack. <span class="hlt">Ice</span>-out is not always immediately followed by the end of winter stratification, there is sometimes a lag of days to weeks before the lakes mix. If the warm temperatures that lead to <span class="hlt">ice</span>-out are followed by calm days without significant wind, the surface of some lakes begins to warm quickly maintaining the density difference and prolonging winter stratification. The longer the lag time, the stronger the density difference becomes which may also result in a very brief period of mixing in the spring prior to set-up of summer stratification. This year's El Niño event resulted</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C43B0802K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C43B0802K"><span>Towards Quantification of Glacier Dynamic <span class="hlt">Ice</span> Loss through Passive Seismic Monitoring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Köhler, A.; Nuth, C.; Weidle, C.; Schweitzer, J.; Kohler, J.; Buscaino, G.</p> <p>2015-12-01</p> <p>Global glaciers and <span class="hlt">ice</span> caps loose mass through calving, while existing models are currently not equipped to realistically predict dynamic <span class="hlt">ice</span> loss. This is mainly because long-term continuous calving records, that would help to better understand fine scale processes and key climatic-dynamic feedbacks between calving, climate, terminus evolution and marine conditions, do not exist. Combined passive seismic/acoustic strategies are the only technique able to capture rapid calving events continuously, independent of daylight or meteorological conditions. We have produced such a continuous calving record for Kronebreen, a tidewater glacier in Svalbard, using data from permanent seismic stations between 2001 and 2014. However, currently no method has been established in cryo-seismology to quantify the calving <span class="hlt">ice</span> loss directly from seismic data. Independent calibration data is required to derive 1) a realistic estimation of the dynamic <span class="hlt">ice</span> loss unobserved due to seismic noise and 2) a robust scaling of seismic calving signals to <span class="hlt">ice</span> <span class="hlt">volumes</span>. Here, we analyze the seismic calving record at Kronebreen and independent calving data in a first attempt to quantify <span class="hlt">ice</span> loss directly from seismic records. We make use of a) calving flux data with weekly to monthly resolution obtained from satellite remote sensing and GPS data between 2007 and 2013, and b) direct, visual calving observations in two weeks in 2009 and 2010. Furthermore, the magnitude-scaling property of seismic calving events is analyzed. We derive and discuss an empirical relation between seismic calving events and calving flux which for the first time allows to estimate a time series of calving <span class="hlt">volumes</span> more than one decade back in time. Improving our model requires to incorporate more precise, high-resolution calibration data. A new field campaign will combine innovative, multi-disciplinary monitoring techniques to measure calving <span class="hlt">ice</span> <span class="hlt">volumes</span> and dynamic <span class="hlt">ice</span>-ocean interactions simultaneously with terrestrial laser</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JGRF..118.1342S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRF..118.1342S"><span>Basal channels on <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>Sergienko, O. V.</p> <p>2013-09-01</p> <p>Recent surveys of floating <span class="hlt">ice</span> shelves associated with Pine Island Glacier (Antarctica) and Petermann Glacier (Greenland) indicate that there are channels incised upward into their bottoms that may serve as the conduits of meltwater outflow from the sub-<span class="hlt">ice</span>-shelf cavity. The formation of the channels, their evolution over time, and their impact on <span class="hlt">ice</span>-shelf flow are investigated using a fully-coupled <span class="hlt">ice-shelf/sub-ice</span>-shelf ocean model. The model simulations suggest that channels may form spontaneously in response to meltwater plume flow initiated at the grounding line if there are relatively high melt rates and if there is transverse to <span class="hlt">ice</span>-flow <span class="hlt">variability</span> in <span class="hlt">ice</span>-shelf thickness. Typical channels formed in the simulations have a width of about 1-3 km and a vertical relief of about 100-200 m. Melt rates and sea-water transport in the channels are significantly higher than on the smooth flat <span class="hlt">ice</span> bottom between the channels. The melt channels develop through melting, deformation, and advection with <span class="hlt">ice</span>-shelf flow. Simulations suggest that both steady state and cyclic state solutions are possible depending on conditions along the lateral <span class="hlt">ice</span>-shelf boundaries. This peculiar dynamics of the system has strong implications on the interpretation of observations. The richness of channel morphology and evolution seen in this study suggests that further observations and theoretical analysis are imperative for understanding <span class="hlt">ice</span>-shelf behavior in warm oceanic conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012GeoRL..39.8502N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012GeoRL..39.8502N"><span>Observations reveal external driver for Arctic sea-<span class="hlt">ice</span> retreat</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Notz, Dirk; Marotzke, Jochem</p> <p>2012-04-01</p> <p>The very low summer extent of Arctic sea <span class="hlt">ice</span> that has been observed in recent years is often casually interpreted as an early-warning sign of anthropogenic global warming. For examining the validity of this claim, previously IPCC model simulations have been used. Here, we focus on the available observational record to examine if this record allows us to identify either internal <span class="hlt">variability</span>, self-acceleration, or a specific external forcing as the main driver for the observed sea-<span class="hlt">ice</span> retreat. We find that the available observations are sufficient to virtually exclude internal <span class="hlt">variability</span> and self-acceleration as an explanation for the observed long-term trend, clustering, and magnitude of recent sea-<span class="hlt">ice</span> minima. Instead, the recent retreat is well described by the superposition of an externally forced linear trend and internal <span class="hlt">variability</span>. For the externally forced trend, we find a physically plausible strong correlation only with increasing atmospheric CO2 concentration. Our results hence show that the observed evolution of Arctic sea-<span class="hlt">ice</span> extent is consistent with the claim that virtually certainly the impact of an anthropogenic climate change is observable in Arctic sea <span class="hlt">ice</span> already today.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090023687','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090023687"><span>Effect of the Inhomogeneity of <span class="hlt">Ice</span> Crystals on Retrieving <span class="hlt">Ice</span> Cloud Optical Thickness and Effective Particle Size</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Xie, Yu; Minnis, Patrick; Hu, Yong X.; Kattawar, George W.; Yang, Ping</p> <p>2008-01-01</p> <p>Spherical or spheroidal air bubbles are generally trapped in the formation of rapidly growing <span class="hlt">ice</span> crystals. In this study the single-scattering properties of inhomogeneous <span class="hlt">ice</span> crystals containing air bubbles are investigated. Specifically, a computational model based on an improved geometric-optics method (IGOM) has been developed to simulate the scattering of light by randomly oriented hexagonal <span class="hlt">ice</span> crystals containing spherical or spheroidal air bubbles. A combination of the ray-tracing technique and the Monte Carlo method is used. The effect of the air bubbles within <span class="hlt">ice</span> crystals is to smooth the phase functions, diminish the 22deg and 46deg halo peaks, and substantially reduce the backscatter relative to bubble-free particles. These features vary with the number, sizes, locations and shapes of the air bubbles within <span class="hlt">ice</span> crystals. Moreover, the asymmetry factors of inhomogeneous <span class="hlt">ice</span> crystals decrease as the <span class="hlt">volume</span> of air bubbles increases. Cloud reflectance lookup tables were generated at wavelengths 0.65 m and 2.13 m with different air-bubble conditions to examine the impact of the bubbles on retrieving <span class="hlt">ice</span> cloud optical thickness and effective particle size. The reflectances simulated for inhomogeneous <span class="hlt">ice</span> crystals are slightly larger than those computed for homogenous <span class="hlt">ice</span> crystals at a wavelength of 0.65 microns. Thus, the retrieved cloud optical thicknesses are reduced by employing inhomogeneous <span class="hlt">ice</span> cloud models. At a wavelength of 2.13 microns, including air bubbles in <span class="hlt">ice</span> cloud models may also increase the reflectance. This effect implies that the retrieved effective particle sizes for inhomogeneous <span class="hlt">ice</span> crystals are larger than those retrieved for homogeneous <span class="hlt">ice</span> crystals, particularly, in the case of large air bubbles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A21C3032Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A21C3032Z"><span>Light Scattering by <span class="hlt">Ice</span> Crystals Containing Air Bubbles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, J.; Panetta, R. L.; Yang, P.; Bi, L.</p> <p>2014-12-01</p> <p>The radiative effects of <span class="hlt">ice</span> clouds are often difficult to estimate accurately, but are very important for interpretation of observations and for climate modeling. Our understanding of these effects is primarily based on scattering calculations, but due to the <span class="hlt">variability</span> in <span class="hlt">ice</span> habit it is computationally difficult to determine the required scattering and absorption properties, and the difficulties are only compounded by the need to include consideration of air and carbon inclusions of the sort frequently observed in collected samples. Much of the previous work on effects of inclusions in <span class="hlt">ice</span> particles on scattering properties has been conducted with variants of geometric optics methods. We report on simulations of scattering by <span class="hlt">ice</span> crystals with enclosed air bubbles using the pseudo-spectral time domain method (PSTD) and improved geometric optics method (IGOM). A Bouncing Ball Model (BBM) is proposed as a parametrization of air bubbles, and the results are compared with Monte Carlo radiative transfer calculations. Consistent with earlier studies, we find that air inclusions lead to a smoothing of variations in the phase function, weakening of halos, and a reduction of backscattering. We extend these studies by examining the effects of the particular arrangement of a fixed number of bubbles, as well as the effects of splitting a given number of bubbles into a greater number of smaller bubbles with the same total <span class="hlt">volume</span> fraction. The result shows that the phase function will not change much for stochastic distributed air bubbles. It also shows that local maxima of phase functions are smoothed out for backward directions, when we break bubbles into small ones, single big bubble scatter favors more forward scattering than multi small internal scatters.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C32B..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C32B..02S"><span>Structural Uncertainty in Antarctic sea <span class="hlt">ice</span> simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schneider, D. P.</p> <p>2016-12-01</p> <p>The inability of the vast majority of historical climate model simulations to reproduce the observed increase in Antarctic sea <span class="hlt">ice</span> has motivated many studies about the quality of the observational record, the role of natural <span class="hlt">variability</span> versus forced changes, and the possibility of missing or inadequate forcings in the models (such as freshwater discharge from thinning <span class="hlt">ice</span> shelves or an inadequate magnitude of stratospheric ozone depletion). In this presentation I will highlight another source of uncertainty that has received comparatively little attention: Structural uncertainty, that is, the systematic uncertainty in simulated sea <span class="hlt">ice</span> trends that arises from model physics and mean-state biases. Using two large ensembles of experiments from the Community Earth System Model (CESM), I will show that the model is predisposed towards producing negative Antarctic sea <span class="hlt">ice</span> trends during 1979-present, and that this outcome is not simply because the model's decadal <span class="hlt">variability</span> is out-of-synch with that in nature. In the "Tropical Pacific Pacemaker" ensemble, in which observed tropical Pacific SST anomalies are prescribed, the model produces very realistic atmospheric circulation trends over the Southern Ocean, yet the sea <span class="hlt">ice</span> trend is negative in every ensemble member. However, if the ensemble-mean trend (commonly interpreted as the forced response) is removed, some ensemble members show a sea <span class="hlt">ice</span> increase that is very similar to the observed. While this results does confirm the important role of natural <span class="hlt">variability</span>, it also suggests a strong bias in the forced response. I will discuss the reasons for this systematic bias and explore possible remedies. This an important problem to solve because projections of 21st -Century changes in the Antarctic climate system (including <span class="hlt">ice</span> sheet surface mass balance changes and related changes in the sea level budget) have a strong dependence on the mean state of and changes in the Antarctic sea <span class="hlt">ice</span> cover. This problem is not unique to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..260a2023A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..260a2023A"><span>Prediction of dry <span class="hlt">ice</span> mass for firefighting robot actuation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ajala, M. T.; Khan, Md R.; Shafie, A. A.; Salami, MJE; Mohamad Nor, M. I.</p> <p>2017-11-01</p> <p>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 <span class="hlt">ice</span>) as the power source. To satisfy the consumption requirement (9cfm) of the motor for efficient actuation of the robot in the fire environment, the <span class="hlt">volume</span> of carbon dioxide gas, as well as the corresponding mass of the dry <span class="hlt">ice</span> that will produce the required <span class="hlt">volume</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">volume</span> requirement of the CAFFR while the corresponding dry <span class="hlt">ice</span> mass for the CAFFR actuation ranges from 21.67kg to 75.83kg depending on the operating pressure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890009375&hterms=bank+canada&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbank%2Bcanada','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890009375&hterms=bank+canada&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbank%2Bcanada"><span>Use of SAR imagery and other remotely-sensed data in deriving <span class="hlt">ice</span> information during a severe <span class="hlt">ice</span> event on the Grand Banks (Newfoundland)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carsey, F. D.; Argus, S. D.</p> <p>1988-01-01</p> <p>Image data from synthetic aperture radar (SAR) are used to observe an <span class="hlt">ice</span> compaction event off the East Coast of Newfoundland in spring, 1987. The information developed from sequential SAR observations is shown to do a remarkably effective job of describing the <span class="hlt">ice</span> conditions; the difficult <span class="hlt">variable</span> is the <span class="hlt">ice</span> thickness which is found to be surprisingly large (2 to 4 times the thickness predictable from thermodynamic growth alone). It may be possible to model the <span class="hlt">ice</span> thickness using SAR-derived <span class="hlt">ice</span> motion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911309W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911309W"><span>Submarine melt rates under Greenland's <span class="hlt">ice</span> tongues</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, Nat; Straneo, Fiametta; Heimbach, Patrick; Cenedese, Claudia</p> <p>2017-04-01</p> <p>The few remaining <span class="hlt">ice</span> tongues (<span class="hlt">ice</span>-shelf like extensions) of Greenland's glaciers are undergoing rapid changes with potential implications for the stability of the <span class="hlt">ice</span> sheet. Submarine melting is recognized as a major contributor to mass loss, yet the magnitude and spatial distribution of melt are poorly known or understood. Here, we use high resolution satellite imagery to infer the magnitude and spatial <span class="hlt">variability</span> 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://hdl.handle.net/2060/19890018776','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890018776"><span>Arctic Sea <span class="hlt">ice</span> studies with passive microwave satellite observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cavalieri, D. J.</p> <p>1988-01-01</p> <p>The objectives of this research are: (1) to improve sea <span class="hlt">ice</span> concentration determinations from passive microwave space observations; (2) to study the role of Arctic polynyas in the production of sea <span class="hlt">ice</span> and the associated salinization of Arctic shelf water; and (3) to study large scale sea <span class="hlt">ice</span> <span class="hlt">variability</span> in the polar oceans. The strategy is to analyze existing data sets and data acquired from both the DMSP SSM/I and recently completed aircraft underflights. Special attention will be given the high resolution 85.5 GHz SSM/I channels for application to thin <span class="hlt">ice</span> algorithms and processes studies. Analysis of aircraft and satellite data sets is expected to provide a basis for determining the potential of the SSM/I high frequency channels for improving sea <span class="hlt">ice</span> algorithms and for investigating oceanic processes. Improved sea <span class="hlt">ice</span> algorithms will aid the study of Arctic coastal polynyas which in turn will provide a better understanding of the role of these polynyas in maintaining the Arctic watermass structure. Analysis of satellite and archived meteorological data sets will provide improved estimates of annual, seasonal and shorter-term sea <span class="hlt">ice</span> <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930022693&hterms=Glacier+retreat+global&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DGlacier%2Bretreat%2Bglobal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930022693&hterms=Glacier+retreat+global&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DGlacier%2Bretreat%2Bglobal"><span>The diatom record from beneath the West Antarctic <span class="hlt">Ice</span> Sheet and the global proxy perspective</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Scherer, Reed P.</p> <p>1993-01-01</p> <p>Recent glaciological evaluation and modeling of the marine-based West Antarctic <span class="hlt">Ice</span> Sheet (WAIS) support the possibility that the WAIS disintegrated during one or more Pleistocene interglacial period(s). The magnitude of sea level and oxygen isotope variation during certain late-Pleistocene interglacial periods is also consistent with the possibility of major retreat of the WAIS. Although oxygen isotopes from deep-sea sediments provide the best available proxy record for global <span class="hlt">ice</span> <span class="hlt">volume</span> (despite the ambiguities in the record), the source of <span class="hlt">ice</span> <span class="hlt">volume</span> changes must be hypothesized. Based on the intensity of interglacial isotopic shifts recorded in Southern Ocean marine sedimentary records, stage 11 (400,000 years ago) is the strongest candidate for WAIS collapse, but the records for stages 9, 7, and 5.5 are all consistent with the possibility of multiple late-Pleistocene collapses. Seismic reflection studies through the WAIS have revealed thick successions of strata with seismic characteristics comparable to upper Tertiary marine sediments. Small samples of glacial diamictons from beneath the <span class="hlt">ice</span> sheet have been collected via hot-water drilled access holes. These sediments include mixed diatom assemblages of varying ages. Late-Miocene diatoms dominate many samples, probably reflecting marine deposition in West Antarctic basins prior to development of a dominantly glacial phase in West Antarctica. In addition to late-Miocene diatoms, samples from Upstream B (1988/89) contain rare post-Miocene diatoms, many of which imply deposition in the West Antarctic interior during one or more Pleistocene deglaciation periods. Age-diagnostic fossils in glacial sediments beneath <span class="hlt">ice</span> sheets provide relatively coarse chronostratigraphic control, but they do contain direct evidence of regional deglaciation. Thus, sub-glacial till samples provide the evidence regarding the source of <span class="hlt">ice</span> sheet <span class="hlt">variability</span> seen in well-dated proxy records. Combined, these independent data sets can</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20120015245&hterms=TES&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DTES','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20120015245&hterms=TES&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DTES"><span>Interannual <span class="hlt">Variability</span> of Dust and <span class="hlt">Ice</span> in the Mars Atmosphere: Comparison of MRO Mars Climate Sounder Retrievals with MGS-TES Limb Sounding Retrievals</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shirley, J. H.; McConnochie, T. H.; Kleinbohl, A.; Schofield, J. T.; Kass, D.; Heavens, N. G.; Benson, J.; McCleese, D. J.</p> <p>2011-01-01</p> <p>Dust and <span class="hlt">ice</span> play important roles in Martian atmospheric dynamics on all time scales. Dust loading in particular exerts an important control on atmospheric temperatures and thereby on the strength of the atmospheric circulation in any given year. We present the first comparisons of MGS-TES aerosol opacity profiles with MRO-MCS aerosol opacity profiles. While the differences in vertical resolution are significant (a factor of 2), we find good agreement at particular seasons between nightside zonal average dust opacity profiles from the two instruments. Derived water <span class="hlt">ice</span> opacities are likewise similar but show greater <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C54A..08S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C54A..08S"><span>Tropical pacing of Antarctic sea <span class="hlt">ice</span> increase</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schneider, D. P.</p> <p>2015-12-01</p> <p>One reason why coupled climate model simulations generally do not reproduce the observed increase in Antarctic sea <span class="hlt">ice</span> extent may be that their internally generated climate <span class="hlt">variability</span> does not sync with the observed phases of phenomena like the Pacific Decadal Oscillation (PDO) and ENSO. For example, it is unlikely for a free-running coupled model simulation to capture the shift of the PDO from its positive to negative phase during 1998, and the subsequent ~15 year duration of the negative PDO phase. In previously presented work based on atmospheric models forced by observed tropical SSTs and stratospheric ozone, we demonstrated that tropical <span class="hlt">variability</span> is key to explaining the wind trends over the Southern Ocean during the past ~35 years, particularly in the Ross, Amundsen and Bellingshausen Seas, the regions of the largest trends in sea <span class="hlt">ice</span> extent and <span class="hlt">ice</span> season duration. Here, we extend this idea to coupled model simulations with the Community Earth System Model (CESM) in which the evolution of SST anomalies in the central and eastern tropical Pacific is constrained to match the observations. This ensemble of 10 "tropical pacemaker" simulations shows a more realistic evolution of Antarctic sea <span class="hlt">ice</span> anomalies than does its unconstrained counterpart, the CESM Large Ensemble (both sets of runs include stratospheric ozone depletion and other time-dependent radiative forcings). In particular, the pacemaker runs show that increased sea <span class="hlt">ice</span> in the eastern Ross Sea is associated with a deeper Amundsen Sea Low (ASL) and stronger westerlies over the south Pacific. These circulation patterns in turn are linked with the negative phase of the PDO, characterized by negative SST anomalies in the central and eastern Pacific. The timing of tropical decadal <span class="hlt">variability</span> with respect to ozone depletion further suggests a strong role for tropical <span class="hlt">variability</span> in the recent acceleration of the Antarctic sea <span class="hlt">ice</span> trend, as ozone depletion stabilized by late 1990s, prior to the most</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP31B2272K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP31B2272K"><span>Allan Hills Pleistocene <span class="hlt">Ice</span> Project (PIP)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kurbatov, A.; Brook, E.; Campbell, S. W.; Conway, H.; Dunbar, N. W.; Higgins, J. A.; Iverson, N. A.; Kehrl, L. M.; McIntosh, W. C.; Spaulding, N. E.; Yan, Y.; Mayewski, P. A.</p> <p>2016-12-01</p> <p>A major international effort to identify at least 1.5 Ma old <span class="hlt">ice</span> for paleoclimate reconstructions has successfully resulted in the selection of several potential drill sites in East Antarctica. At this point it is indisputable that the Antarctic <span class="hlt">ice</span> sheet captures a continuous envinronmental record of the Earth that spans the Mid Pleistocene Transition (MPT). In addition to traditional <span class="hlt">ice</span> coring approaches, the oldest <span class="hlt">ice</span> can also be recovered in Antarctic Blue <span class="hlt">Ice</span> Areas (BIA). We have already successfully demonstrated that the Allan Hills (AH) BIA captures a regional climate signal and robust record of 1Ma atmosphere that can be studied with a relatively uncomplicated logistical imprint and essentially unlimited sampling <span class="hlt">volume</span>. The attractiveness of unlimited sampling of known age <span class="hlt">ice</span> is the basis for the "<span class="hlt">ice</span> park" concept proposed earlier by our research team. The idea is that, once the age of <span class="hlt">ice</span> exposed along the flow line at the surface of BIA is mapped, it could be sampled for numerous research projects as needed. Here we propose an intermediate ( 1,150 m deep) <span class="hlt">ice</span> core drill site, located only 240 km away from McMurdo base that will help to develop a, continuous, high quality regional paleoclimate record that is at least 1Ma old. We will introduce and discuss the glaciological settings, paleoclimate signals and possible limitations and advantages of the 1 Ma AH BIA regional paleoclimate record. The research was funded by NSF Division of Polar Programs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.B52A..04G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.B52A..04G"><span>End of the trend: Cold desert ecosystem responses to climate <span class="hlt">variability</span></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.; Barrett, J. E.; Truhlar, A.; Adams, B.; Doran, P. T.; Fountain, A. G.; Lyons, W. B.; McKnight, D. M.; Priscu, J. C.; Takacs-Vesbach, C. D.; Virginia, R. A.; Wall, D. H.</p> <p>2013-12-01</p> <p>The McMurdo Dry Valleys (MDVs) of Antarctica represent a cold desert ecosystem defined by extensive soils (i.e., not <span class="hlt">ice</span>-covered), glacier meltwater streams, and closed-basin, <span class="hlt">ice</span>-covered lakes. Despite cold temperatures and very little precipitation, a vibrant ecosystem exists across these landscape units. Previous work in the MDVs documented significant responses of local aquatic and terrestrial ecosystems to a decadal cooling trend prior to 2000. However, an exceptionally high melt year occurred in 2002, influencing stream flow, lake dynamics and terrestrial ecosystems. Here we describe interannual variation in Dry Valley ecosystems, focusing on the contrasts in drivers of ecological responses pre- and post 2002, i.e., the flood year. In streams, ash-free dry mass (AFDM) and chlorophyll-a concentration in black Nostoc-dominated microbial mats were observed to decrease prior to 2002, and AFDM has been increasing since. Three MDV lakes were decreasing in <span class="hlt">volume</span> and increasing in total chlorophyll-a mass in the photic zones prior to 2002 and have been increasing <span class="hlt">volume</span> and decreasing total chlorophyll-a mass since. Soil nematode communities were decreasing in abundance prior to 2002, and show no significant trend since, but increased <span class="hlt">variability</span>. Since 2002, the MDV ecosystem has ceased responding to only a decadal cooling trend and is responding to several high-flow years with new trajectories in some cases and changed interannual <span class="hlt">variability</span> in others.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4415831','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4415831"><span>A Comparison of Somatic <span class="hlt">Variables</span> of Elite <span class="hlt">Ice</span> Hockey Players from the Czech ELH and Russian KHL</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kutáč, Petr; Sigmund, Martin</p> <p>2015-01-01</p> <p>The goals of this study were to evaluate the basic morphological <span class="hlt">variables</span> of contemporary elite <span class="hlt">ice</span> hockey players, compare the parameters of players in the top Russian <span class="hlt">ice</span> hockey league (KHL) with those of the top Czech <span class="hlt">ice</span> hockey league (ELH), and to evaluate the parameters of players according to their position in the game. The research participants included 30 KHL players (mean age: 27.1 ± 5.1 years) and 25 ELH players (mean age: 26.4 ± 5.8 years). We determined body height, body mass, and body composition (body fat, fat-free mass, segmental fat analysis). All measurements were performed at the end of preseason training. The KHL players had the following anthropometric characteristics: body height 182.97 ± 5.61 cm (forward) and 185.72 ± 3.57 cm (defenseman), body mass 89.70 ± 5.28 kg (forward) and 92.52 ± 4.01 kg (defenseman), body fat 10.76 ± 0.63 kg (forward) and 11.10 ± 0.48 kg (defenseman), fat-free mass 78.94 ± 4.65 kg (forward) and 81.42 ± 3.52 kg (defenseman). The values for ELH players were as follows: body height 182.06 ± 5.93 cm (forward) and 185.88 ± 7.13 cm (defenseman), body mass 88.47 ± 7.06 kg (forward) and 89.36 ± 10.91 kg (defenseman), body fat 12.57 ± 2.89 kg (forward) and 11.91 ± 3.10 kg (defenseman), fat-free mass 75.93 ± 6.54 kg (forward) and 77.46 ± 7.89 kg (defenseman). The results indicate that it is beneficial to <span class="hlt">ice</span> hockey players to have increased body mass and lower body fat, which leads to higher muscle mass, thus enabling a player to perform at the highest level and meet the specific challenges of the game. PMID:25949747</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070034034&hterms=time+zone&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dtime%2Bzone','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070034034&hterms=time+zone&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dtime%2Bzone"><span>Contrasts in Sea <span class="hlt">Ice</span> Deformation and Production in the Arctic Seasonal and Perennial <span class="hlt">Ice</span> Zones</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kwok, K.</p> <p>2006-01-01</p> <p>Four years (1997-2000) of RADARSAT Geophysical Processor System (RGPS) data are used to contrast the sea <span class="hlt">ice</span> deformation and production regionally, and in the seasonal (SIZ) and perennial (PIZ) <span class="hlt">ice</span> zones. <span class="hlt">Ice</span> production is of seasonal <span class="hlt">ice</span> in openings during the winter. Three-day estimates of these quantities are provided within Lagrangian elements initially 10 km on a side. A distinct seasonal cycle is seen in both zones with these estimates highest in the late fall and with seasonal minimums in the midwinter. Regional divergence over the winter could be up to 30%. Spatially, the highest deformation is seen in the SIZ north of coastal Alaska. Both <span class="hlt">ice</span> deformation and production are higher in the SIZ: deformation-related <span class="hlt">ice</span> production in the SIZ (approx.0.5 m) is 1.5-2.3 times that of the PIZ (approx.0.3 m): this is connected to <span class="hlt">ice</span> strength and thickness. Atmospheric forcing and boundary layer structure contribute to only the seasonal and interannual <span class="hlt">variability</span>. Seasonal <span class="hlt">ice</span> growth in <span class="hlt">ice</span> fractures accounts for approx.25-40% of the total <span class="hlt">ice</span> production of the Arctic Ocean. Uncertainties in these estimates are discussed. By itself, this deformation-<span class="hlt">ice</span> production relationship could be considered a negative feedback when thickness is perturbed. However, the overall effect on <span class="hlt">ice</span> production in the face of increasing seasonal and thinner/weaker <span class="hlt">ice</span> coverage could be modified by local destabilization of the water column promoting overturning of warmer water due to increased brine rejection; and the upwelling of the pynocline associated with increased occurrence of large shear motion in sea <span class="hlt">ice</span>. Divergence is shown to be negligibly correlated to cyclonic motion in summer and winter in both <span class="hlt">ice</span> zones.</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 mass 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 <span class="hlt">variability</span> 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('http://adsabs.harvard.edu/abs/2013EGUGA..15.7955K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7955K"><span>Springtime atmospheric transport controls Arctic summer sea-<span class="hlt">ice</span> extent</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kapsch, Marie; Graversen, Rune; Tjernström, Michael</p> <p>2013-04-01</p> <p>The sea-<span class="hlt">ice</span> extent in the Arctic has been steadily decreasing during the satellite remote sensing era, 1979 to present, with the highest rate of retreat found in September. Contributing factors causing the <span class="hlt">ice</span> retreat are among others: changes in surface air temperature (SAT; Lindsay and Zhang, 2005), <span class="hlt">ice</span> circulation in response to winds/pressure patterns (Overland et al., 2008) and ocean currents (Comiso et al., 2008), as well as changes in radiative fluxes (e.g. due to changes in cloud cover; Francis and Hunter, 2006; Maksimovich and Vihma, 2012) and ocean conditions. However, large interannual <span class="hlt">variability</span> is superimposed onto the declining trend - the <span class="hlt">ice</span> extent by the end of the summer varies by several million square kilometer between successive years (Serreze et al., 2007). But what are the processes causing the year-to-year <span class="hlt">ice</span> <span class="hlt">variability</span>? A comparison of years with an anomalously large September sea-<span class="hlt">ice</span> extent (HIYs - high <span class="hlt">ice</span> years) with years showing an anomalously small <span class="hlt">ice</span> extent (LIYs - low <span class="hlt">ice</span> years) reveals that the <span class="hlt">ice</span> <span class="hlt">variability</span> is most pronounced in the Arctic Ocean north of Siberia (which became almost entirely <span class="hlt">ice</span> free in September of 2007 and 2012). Significant <span class="hlt">ice</span>-concentration anomalies of up to 30% are observed for LIYs and HIYs in this area. Focusing on this area we find that the greenhouse effect associated with clouds and water-vapor in spring is crucial for the development of the sea <span class="hlt">ice</span> during the subsequent months. In years where the end-of-summer sea-<span class="hlt">ice</span> extent is well below normal, a significantly enhanced transport of humid air is evident during spring into the region where the <span class="hlt">ice</span> retreat is encountered. The anomalous convergence of humidity increases the cloudiness, resulting in an enhancement of the greenhouse effect. As a result, downward longwave radiation at the surface is larger than usual. In mid May, when the <span class="hlt">ice</span> anomaly begins to appear and the surface albedo therefore becomes anomalously low, the net shortwave radiation</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 <span class="hlt">variables</span> 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 mass (%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 mass 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('http://adsabs.harvard.edu/abs/2014AGUFM.B23G..08P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B23G..08P"><span>Sources and sinks of methane beneath polar <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>Priscu, J. C.; Adams, H. E.; Hand, K. P.; Dore, J. E.; Matheus-Carnevali, P.; Michaud, A. B.; Murray, A. E.; Skidmore, M. L.; Vick-Majors, T.</p> <p>2014-12-01</p> <p>Several icy moons of the outer solar system carry subsurface oceans containing many times the <span class="hlt">volume</span> of liquid water on Earth and may provide the greatest <span class="hlt">volume</span> of habitable space in our solar system. Functional sub-<span class="hlt">ice</span> polar ecosystems on Earth provide compelling models for the habitability of extraterrestrial sub-<span class="hlt">ice</span> oceans. A key feature of sub-<span class="hlt">ice</span> environments is that most of them receive little to no solar energy. Consequently, organisms inhabiting these environments must rely on chemical energy to assimilate either carbon dioxide or organic molecules to support their metabolism. Methane can be utilized by certain bacteria as both a carbon and energy source. Isotopic data show that methane in Earth's polar lakes is derived from both biogenic and thermogenic sources. Thermogenic sources of methane in the thermokarst lakes of the north slope of Alaska yield supersaturated water columns during winter <span class="hlt">ice</span> cover that support active populations of methanotrophs during the polar night. Methane in the permanently <span class="hlt">ice</span>-covered lakes of the McMurdo Dry Valleys, Antarctica varies widely in concentration and is produced either by contemporary methanogenesis or is a relic from subglacial flow. Rate measurements revealed that microbial methane oxidation occurs beneath the <span class="hlt">ice</span> in both the arctic and Antarctic lakes. The first samples collected from an Antarctic subglacial environment beneath 800 m of <span class="hlt">ice</span> (Subglacial Lake Whillans) revealed an active microbial ecosystem that has been isolated from the atmosphere for many thousands of years. The sediments of Lake Whillans contained high levels of methane with an isotopic signature that indicates it was produced via methanogenesis. The source of this methane appears to be from the decomposition of organic carbon deposited when this region of Antarctica was covered by the sea. Collectively, data from these sub-<span class="hlt">ice</span> environments show that methane transformations play a key role in microbial community metabolism. The discovery of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CliPa..14..619B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CliPa..14..619B"><span>Simulation of the Greenland <span class="hlt">Ice</span> Sheet over two glacial-interglacial cycles: investigating a sub-<span class="hlt">ice</span>-shelf melt parameterization and relative sea level forcing in an <span class="hlt">ice-sheet-ice</span>-shelf model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bradley, Sarah L.; Reerink, Thomas J.; van de Wal, Roderik S. W.; Helsen, Michiel M.</p> <p>2018-05-01</p> <p>Observational evidence, including offshore moraines and sediment cores, confirm that at the Last Glacial Maximum (LGM) the Greenland <span class="hlt">ice</span> sheet (GrIS) expanded to a significantly larger spatial extent than seen at present, grounding into Baffin Bay and out onto the continental shelf break. Given this larger spatial extent and its close proximity to the neighbouring Laurentide <span class="hlt">Ice</span> Sheet (LIS) and Innuitian <span class="hlt">Ice</span> Sheet (IIS), it is likely these <span class="hlt">ice</span> sheets will have had a strong non-local influence on the spatial and temporal behaviour of the GrIS. Most previous paleo <span class="hlt">ice</span>-sheet modelling simulations recreated an <span class="hlt">ice</span> sheet that either did not extend out onto the continental shelf or utilized a simplified marine <span class="hlt">ice</span> parameterization which did not fully include the effect of <span class="hlt">ice</span> shelves or neglected the sensitivity of the GrIS to this non-local bedrock signal from the surrounding <span class="hlt">ice</span> sheets. In this paper, we investigated the evolution of the GrIS over the two most recent glacial-interglacial cycles (240 ka BP to the present day) using the <span class="hlt">ice-sheet-ice</span>-shelf model IMAU-<span class="hlt">ICE</span>. We investigated the solid earth influence of the LIS and IIS via an offline relative sea level (RSL) forcing generated by a glacial isostatic adjustment (GIA) model. The RSL forcing governed the spatial and temporal pattern of sub-<span class="hlt">ice</span>-shelf melting via changes in the water depth below the <span class="hlt">ice</span> shelves. In the ensemble of simulations, at the glacial maximums, the GrIS coalesced with the IIS to the north and expanded to the continental shelf break to the southwest but remained too restricted to the northeast. In terms of the global mean sea level contribution, at the Last Interglacial (LIG) and LGM the <span class="hlt">ice</span> sheet added 1.46 and -2.59 m, respectively. This LGM contribution by the GrIS is considerably higher (˜ 1.26 m) than most previous studies whereas the contribution to the LIG highstand is lower (˜ 0.7 m). The spatial and temporal behaviour of the northern margin was highly <span class="hlt">variable</span> in all simulations</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A33A0124S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A33A0124S"><span>Classification and Feature Selection Algorithms for Modeling <span class="hlt">Ice</span> Storm Climatology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Swaminathan, R.; Sridharan, M.; Hayhoe, K.; Dobbie, G.</p> <p>2015-12-01</p> <p><span class="hlt">Ice</span> storms account for billions of dollars of winter storm loss across the continental US and Canada. In the future, increasing concentration of human populations in areas vulnerable to <span class="hlt">ice</span> storms such as the northeastern US will only exacerbate the impacts of these extreme events on infrastructure and society. Quantifying the potential impacts of global climate change on <span class="hlt">ice</span> storm prevalence and frequency is challenging, as <span class="hlt">ice</span> storm climatology is driven by complex and incompletely defined atmospheric processes, processes that are in turn influenced by a changing climate. This makes the underlying atmospheric and computational modeling of <span class="hlt">ice</span> storm climatology a formidable task. We propose a novel computational framework that uses sophisticated stochastic classification and feature selection algorithms to model <span class="hlt">ice</span> storm climatology and quantify storm occurrences from both reanalysis and global climate model outputs. The framework is based on an objective identification of <span class="hlt">ice</span> storm events by key <span class="hlt">variables</span> derived from vertical profiles of temperature, humidity and geopotential height. Historical <span class="hlt">ice</span> storm records are used to identify days with synoptic-scale upper air and surface conditions associated with <span class="hlt">ice</span> storms. Evaluation using NARR reanalysis and historical <span class="hlt">ice</span> storm records corresponding to the northeastern US demonstrates that an objective computational model with standard performance measures, with a relatively high degree of accuracy, identify <span class="hlt">ice</span> storm events based on upper-air circulation patterns and provide insights into the relationships between key climate <span class="hlt">variables</span> associated with <span class="hlt">ice</span> storms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CliPa..14..193B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CliPa..14..193B"><span>The Ross Sea Dipole - temperature, snow accumulation and sea <span class="hlt">ice</span> <span class="hlt">variability</span> in the Ross Sea region, Antarctica, over the past 2700 years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bertler, Nancy A. N.; Conway, Howard; Dahl-Jensen, Dorthe; Emanuelsson, Daniel B.; Winstrup, Mai; Vallelonga, Paul T.; Lee, James E.; Brook, Ed J.; Severinghaus, Jeffrey P.; Fudge, Taylor J.; Keller, Elizabeth D.; Baisden, W. Troy; Hindmarsh, Richard C. A.; Neff, Peter D.; Blunier, Thomas; Edwards, Ross; Mayewski, Paul A.; Kipfstuhl, Sepp; Buizert, Christo; Canessa, Silvia; Dadic, Ruzica; Kjær, Helle A.; Kurbatov, Andrei; Zhang, Dongqi; Waddington, Edwin D.; Baccolo, Giovanni; Beers, Thomas; Brightley, Hannah J.; Carter, Lionel; Clemens-Sewall, David; Ciobanu, Viorela G.; Delmonte, Barbara; Eling, Lukas; Ellis, Aja; Ganesh, Shruthi; Golledge, Nicholas R.; Haines, Skylar; Handley, Michael; Hawley, Robert L.; Hogan, Chad M.; Johnson, Katelyn M.; Korotkikh, Elena; Lowry, Daniel P.; Mandeno, Darcy; McKay, Robert M.; Menking, James A.; Naish, Timothy R.; Noerling, Caroline; Ollive, Agathe; Orsi, Anaïs; Proemse, Bernadette C.; Pyne, Alexander R.; Pyne, Rebecca L.; Renwick, James; Scherer, Reed P.; Semper, Stefanie; Simonsen, Marius; Sneed, Sharon B.; Steig, Eric J.; Tuohy, Andrea; Ulayottil Venugopal, Abhijith; Valero-Delgado, Fernando; Venkatesh, Janani; Wang, Feitang; Wang, Shimeng; Winski, Dominic A.; Winton, V. Holly L.; Whiteford, Arran; Xiao, Cunde; Yang, Jiao; Zhang, Xin</p> <p>2018-02-01</p> <p>High-resolution, well-dated climate archives provide an opportunity to investigate the dynamic interactions of climate patterns relevant for future projections. Here, we present data from a new, annually dated <span class="hlt">ice</span> core record from the eastern Ross Sea, named the Roosevelt Island Climate Evolution (RICE) <span class="hlt">ice</span> core. Comparison of this record with climate reanalysis data for the 1979-2012 interval shows that RICE reliably captures temperature and snow precipitation <span class="hlt">variability</span> in the region. Trends over the past 2700 years in RICE are shown to be distinct from those in West Antarctica and the western Ross Sea captured by other <span class="hlt">ice</span> cores. For most of this interval, the eastern Ross Sea was warming (or showing isotopic enrichment for other reasons), with increased snow accumulation and perhaps decreased sea <span class="hlt">ice</span> concentration. However, West Antarctica cooled and the western Ross Sea showed no significant isotope temperature trend. This pattern here is referred to as the Ross Sea Dipole. Notably, during the Little <span class="hlt">Ice</span> Age, West Antarctica and the western Ross Sea experienced colder than average temperatures, while the eastern Ross Sea underwent a period of warming or increased isotopic enrichment. From the 17th century onwards, this dipole relationship changed. All three regions show current warming, with snow accumulation declining in West Antarctica and the eastern Ross Sea but increasing in the western Ross Sea. We interpret this pattern as reflecting an increase in sea <span class="hlt">ice</span> in the eastern Ross Sea with perhaps the establishment of a modern Roosevelt Island polynya as a local moisture source for RICE.</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 <span class="hlt">volume</span> 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 mass conservation approach paired with shallow <span class="hlt">ice</span> physics using estimates of the surface mass 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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRC..120.7791S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRC..120.7791S"><span>Seasonal and interannual <span class="hlt">variability</span> of fast <span class="hlt">ice</span> extent in the southeastern Laptev Sea between 1999 and 2013</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Selyuzhenok, V.; Krumpen, T.; Mahoney, A.; Janout, M.; Gerdes, R.</p> <p>2015-12-01</p> <p>Along with changes in sea <span class="hlt">ice</span> extent, thickness, and drift speed, Arctic sea <span class="hlt">ice</span> regime is characterized by a decrease of fast <span class="hlt">ice</span> season and reduction of fast <span class="hlt">ice</span> extent. The most extensive fast <span class="hlt">ice</span> cover in the Arctic develops in the southeastern Laptev Sea. Using weekly operational sea <span class="hlt">ice</span> charts produced by Arctic and Antarctic Research Institute (AARI, Russia) from 1999 to 2013, we identified five main key events that characterize the annual evolution of fast <span class="hlt">ice</span> in the southeastern Laptev Sea. Linking the occurrence of the key events with the atmospheric forcing, bathymetry, freezeup, and melt onset, we examined the processes driving annual fast <span class="hlt">ice</span> cycle. The analysis revealed that fast <span class="hlt">ice</span> in the region is sensitive to thermodynamic processes throughout a season, while the wind has a strong influence only on the first stages of fast <span class="hlt">ice</span> development. The maximal fast <span class="hlt">ice</span> extent is closely linked to the bathymetry and local topography and is primarily defined by the location of shoals, where fast <span class="hlt">ice</span> is likely grounded. The annual fast <span class="hlt">ice</span> cycle shows significant changes over the period of investigation, with tendencies toward later fast <span class="hlt">ice</span> formation and earlier breakup. These tendencies result in an overall decrease of the fast <span class="hlt">ice</span> season by 2.8 d/yr, which is significantly higher than previously reported trends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24248343','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24248343"><span>Greenland <span class="hlt">ice</span> sheet motion insensitive to exceptional meltwater forcing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tedstone, Andrew J; Nienow, Peter W; Sole, Andrew J; Mair, Douglas W F; Cowton, Thomas R; Bartholomew, Ian D; King, Matt A</p> <p>2013-12-03</p> <p>Changes to the dynamics of the Greenland <span class="hlt">ice</span> sheet can be forced by various mechanisms including surface-melt-induced <span class="hlt">ice</span> acceleration and oceanic forcing of marine-terminating glaciers. We use observations of <span class="hlt">ice</span> motion to examine the surface melt-induced dynamic response of a land-terminating outlet glacier in southwest Greenland to the exceptional melting observed in 2012. During summer, meltwater generated on the Greenland <span class="hlt">ice</span> sheet surface accesses the <span class="hlt">ice</span> sheet bed, lubricating basal motion and resulting in periods of faster <span class="hlt">ice</span> flow. However, the net impact of varying meltwater <span class="hlt">volumes</span> upon seasonal and annual <span class="hlt">ice</span> flow, and thus sea level rise, remains unclear. We show that two extreme melt events (98.6% of the Greenland <span class="hlt">ice</span> sheet surface experienced melting on July 12, the most significant melt event since 1889, and 79.2% on July 29) and summer <span class="hlt">ice</span> sheet runoff ~3.9 σ above the 1958-2011 mean resulted in enhanced summer <span class="hlt">ice</span> motion relative to the average melt year of 2009. However, despite record summer melting, subsequent reduced winter <span class="hlt">ice</span> motion resulted in 6% less net annual <span class="hlt">ice</span> motion in 2012 than in 2009. Our findings suggest that surface melt-induced acceleration of land-terminating regions of the <span class="hlt">ice</span> sheet will remain insignificant even under extreme melting scenarios.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5016760','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5016760"><span>Influence of <span class="hlt">ice</span> thickness and surface properties on light transmission through Arctic sea <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Arndt, Stefanie; Nicolaus, Marcel; Perovich, Donald K.; Jakuba, Michael V.; Suman, Stefano; Elliott, Stephen; Whitcomb, Louis L.; McFarland, Christopher J.; Gerdes, Rüdiger; Boetius, Antje; German, Christopher R.</p> <p>2015-01-01</p> <p>Abstract The observed changes in physical properties of sea <span class="hlt">ice</span> such as decreased thickness and increased melt pond cover severely impact the energy budget of Arctic sea <span class="hlt">ice</span>. Increased light transmission leads to increased deposition of solar energy in the upper ocean and thus plays a crucial role for amount and timing of sea‐ice‐melt and under‐<span class="hlt">ice</span> primary production. Recent developments in underwater technology provide new opportunities to study light transmission below the largely inaccessible underside of sea <span class="hlt">ice</span>. We measured spectral under‐<span class="hlt">ice</span> radiance and irradiance using the new Nereid Under‐<span class="hlt">Ice</span> (NUI) underwater robotic vehicle, during a cruise of the R/V Polarstern to 83°N 6°W in the Arctic Ocean in July 2014. NUI is a next generation hybrid remotely operated vehicle (H‐ROV) designed for both remotely piloted and autonomous surveys underneath land‐fast and moving sea <span class="hlt">ice</span>. Here we present results from one of the first comprehensive scientific dives of NUI employing its interdisciplinary sensor suite. We combine under‐<span class="hlt">ice</span> optical measurements with three dimensional under‐<span class="hlt">ice</span> topography (multibeam sonar) and aerial images of the surface conditions. We investigate the influence of spatially varying ice‐thickness and surface properties on the spatial <span class="hlt">variability</span> of light transmittance during summer. Our results show that surface properties such as melt ponds dominate the spatial distribution of the under‐<span class="hlt">ice</span> light field on small scales (<1000 m2), while sea ice‐thickness is the most important predictor for light transmission on larger scales. In addition, we propose the use of an algorithm to obtain histograms of light transmission from distributions of sea <span class="hlt">ice</span> thickness and surface albedo. PMID:27660738</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41C1229S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41C1229S"><span>Simulating <span class="hlt">Ice</span> Dynamics in the Amundsen Sea Sector</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schwans, E.; Parizek, B. R.; Morlighem, M.; Alley, R. B.; Pollard, D.; Walker, R. T.; Lin, P.; St-Laurent, P.; LaBirt, T.; Seroussi, H. L.</p> <p>2017-12-01</p> <p>Thwaites and Pine Island Glaciers (TG; PIG) exhibit patterns of dynamic retreat forced from their floating margins, and could act as gateways for destabilization of deep marine basins in the West Antarctic <span class="hlt">Ice</span> Sheet (WAIS). Poorly constrained basal conditions can cause model predictions to diverge. Thus, there is a need for efficient simulations that account for shearing within the <span class="hlt">ice</span> column, and include adequate basal sliding and <span class="hlt">ice</span>-shelf melting parameterizations. To this end, UCI/NASA JPL's <span class="hlt">Ice</span> Sheet System Model (ISSM) with coupled SSA/higher-order physics is used in the Amundsen Sea Embayment (ASE) to examine threshold behavior of TG and PIG, highlighting areas particularly vulnerable to retreat from oceanic warming and <span class="hlt">ice</span>-shelf removal. These moving-front experiments will aid in targeting critical areas for additional data collection in ASE as well as for weighting accuracy in further melt parameterization development. Furthermore, a sub-shelf melt parameterization, resulting from Regional Ocean Modeling System (ROMS; St-Laurent et al., 2015) and coupled ISSM-Massachusetts Institute of Technology general circulation model (MITgcm; Seroussi et al., 2017) output, is incorporated and initially tested in ISSM. Data-guided experiments include <span class="hlt">variable</span> basal conditions and <span class="hlt">ice</span> hardness, and are also forced with constant modern climate in ISSM, providing valuable insight into i) effects of different basal friction parameterizations on <span class="hlt">ice</span> dynamics, illustrating the importance of constraining the <span class="hlt">variable</span> bed character beneath TG and PIG; ii) the impact of including vertical shear in <span class="hlt">ice</span> flow models of outlet glaciers, confirming its role in capturing complex feedbacks proximal to the grounding zone; and iii) ASE's sensitivity to sub-shelf melt and <span class="hlt">ice</span>-front retreat, possible thresholds, and how these affect <span class="hlt">ice</span>-flow evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009NatMa...8..405K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009NatMa...8..405K"><span>The preparation and structure of salty <span class="hlt">ice</span> VII under pressure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Klotz, Stefan; Bove, Livia E.; Strässle, Thierry; Hansen, Thomas C.; Saitta, Antonino M.</p> <p>2009-05-01</p> <p>It is widely accepted that <span class="hlt">ice</span>, no matter what phase, is unable to incorporate large amounts of salt into its structure. This conclusion is based on the observation that on freezing of salt water, <span class="hlt">ice</span> expels the salt almost entirely as brine. Here, we show that this behaviour is not an intrinsic physico-chemical property of <span class="hlt">ice</span> phases. We demonstrate by neutron diffraction that substantial amounts of dissolved LiCl can be built homogeneously into the <span class="hlt">ice</span> VII structure if it is produced by recrystallization of its glassy (amorphous) state under pressure. Such `alloyed' <span class="hlt">ice</span> VII has significantly different structural properties compared with pure <span class="hlt">ice</span> VII, such as an 8% larger unit cell <span class="hlt">volume</span>, 5 times larger displacement factors, an absence of a transition to an ordered <span class="hlt">ice</span> VIII structure and plasticity. Our study suggests that there could be a whole new class of `salty' high-pressure <span class="hlt">ice</span> forms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19349969','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19349969"><span>The preparation and structure of salty <span class="hlt">ice</span> VII under pressure.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Klotz, Stefan; Bove, Livia E; Strässle, Thierry; Hansen, Thomas C; Saitta, Antonino M</p> <p>2009-05-01</p> <p>It is widely accepted that <span class="hlt">ice</span>, no matter what phase, is unable to incorporate large amounts of salt into its structure. This conclusion is based on the observation that on freezing of salt water, <span class="hlt">ice</span> expels the salt almost entirely as brine. Here, we show that this behaviour is not an intrinsic physico-chemical property of <span class="hlt">ice</span> phases. We demonstrate by neutron diffraction that substantial amounts of dissolved LiCl can be built homogeneously into the <span class="hlt">ice</span> VII structure if it is produced by recrystallization of its glassy (amorphous) state under pressure. Such 'alloyed' <span class="hlt">ice</span> VII has significantly different structural properties compared with pure <span class="hlt">ice</span> VII, such as an 8% larger unit cell <span class="hlt">volume</span>, 5 times larger displacement factors, an absence of a transition to an ordered <span class="hlt">ice</span> VIII structure and plasticity. Our study suggests that there could be a whole new class of 'salty' high-pressure <span class="hlt">ice</span> forms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900033480&hterms=Ross+1986&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DRoss%2B1986','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900033480&hterms=Ross+1986&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DRoss%2B1986"><span>Sea <span class="hlt">ice</span> and oceanic processes on the Ross Sea continental shelf</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jacobs, S. S.; Comiso, J. C.</p> <p>1989-01-01</p> <p>The spatial and temporal <span class="hlt">variability</span> of Antarctic sea <span class="hlt">ice</span> concentrations on the Ross Sea continental shelf have been investigated in relation to oceanic and atmospheric forcing. Sea <span class="hlt">ice</span> data were derived from Nimbus 7 scanning multichannel microwave radiometer (SMMR) brightness temperatures from 1979-1986. <span class="hlt">Ice</span> cover over the shelf was persistently lower than above the adjacent deep ocean, averaging 86 percent during winter with little month-to-month of interannual <span class="hlt">variability</span>. The large spring Ross Sea polynya on the western shelf results in a longer period of summer insolation, greater surface layer heat storage, and later <span class="hlt">ice</span> formation in that region the following autumn.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/936331','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/936331"><span><span class="hlt">Ice</span> method for production of hydrogen clathrate hydrates</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Lokshin, Konstantin [Santa Fe, NM; Zhao, Yusheng [Los Alamos, NM</p> <p>2008-05-13</p> <p>The present invention includes a method for hydrogen clathrate hydrate synthesis. First, <span class="hlt">ice</span> and hydrogen gas are supplied to a containment <span class="hlt">volume</span> at a first temperature and a first pressure. Next, the containment <span class="hlt">volume</span> is pressurized with hydrogen gas to a second higher pressure, where hydrogen clathrate hydrates are formed in the process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT.......131M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT.......131M"><span>Investigating the Effects of Environmental Solutes on the Reaction Environment in <span class="hlt">Ice</span> and at <span class="hlt">Ice</span> Surfaces</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Malley, Philip Patrick Anthony</p> <p></p> <p>The reaction environments present in water, <span class="hlt">ice</span>, and at <span class="hlt">ice</span> surfaces are physically distinct from one another and studies have shown that photolytic reactions can take place at different rates in the different media. Kinetics of reactions in frozen media are measured in snow and <span class="hlt">ice</span> prepared from deionized water. This reduces experimental artifacts, but is not relevant to snow in the environment, which contains solutes. We have monitored the effect of nonchromophoric (will not absorb sunlight) organic matter on the photolytic fate of the polycyclic aromatic hydrocarbons (PAHs) phenanthrene, pyrene, and anthracene in <span class="hlt">ice</span> and at <span class="hlt">ice</span> surfaces. Nonchromophoric organic matter reduced photolysis rates to below our detection limit in bulk <span class="hlt">ice</span>, and reduced rates at <span class="hlt">ice</span> surfaces to a lesser extent due to the PAHs partially partitioning to the organics present. In addition, we have monitored the effect of chromophoric (will absorb sunlight) dissolved organic matter (cDOM) on the fate of anthracene in water, <span class="hlt">ice</span>, and <span class="hlt">ice</span> surfaces. cDOM reduced rates in all three media. Suppression in liquid water was due to physical interactions between anthracene and the cDOM, rather than to competitive photon absorbance. More suppression was observed in <span class="hlt">ice</span> cubes and <span class="hlt">ice</span> granules than in liquid water due to a freeze concentrating effect. Sodium Chloride (NaCl) is another ubiquitous environmental solute that can influence reaction kinetics in water, <span class="hlt">ice</span>, and at <span class="hlt">ice</span> surfaces. Using Raman microscopy, we have mapped the surface of <span class="hlt">ice</span> of frozen NaCl solutions at 0.02M and 0.6M, as well as the surface of frozen samples of Sargasso Sea Water. At temperatures above and below the eutectic temperature (-21.1°C). Above the eutectic, regions of <span class="hlt">ice</span> and liquid water were observed in all samples. Liquid regions generally took the form of channels. Channel widths and fractional liquid surface coverage increased with NaCl concentration and temperature. <span class="hlt">Volume</span> maps of the three samples at temperatures</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140005248','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140005248"><span>Discrete Surface Evolution and Mesh Deformation for Aircraft <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>Thompson, David; Tong, Xiaoling; Arnoldus, Qiuhan; Collins, Eric; McLaurin, David; Luke, Edward; Bidwell, Colin S.</p> <p>2013-01-01</p> <p>Robust, automated mesh generation for problems with deforming geometries, such as <span class="hlt">ice</span> accreting on aerodynamic surfaces, remains a challenging problem. Here we describe a technique to deform a discrete surface as it evolves due to the accretion of <span class="hlt">ice</span>. The surface evolution algorithm is based on a smoothed, face-offsetting approach. We also describe a fast algebraic technique to propagate the computed surface deformations into the surrounding <span class="hlt">volume</span> mesh while maintaining geometric mesh quality. Preliminary results presented here demonstrate the ecacy of the approach for a sphere with a prescribed accretion rate, a rime <span class="hlt">ice</span> accretion, and a more complex glaze <span class="hlt">ice</span> accretion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1613191V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1613191V"><span>Seasonal variabilty of surface velocities and <span class="hlt">ice</span> discharge of Columbia Glacier, Alaska using high-resolution TanDEM-X satellite time series and NASA <span class="hlt">Ice</span>Bridge data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vijay, Saurabh; Braun, Matthias</p> <p>2014-05-01</p> <p>Columbia Glacier is a grounded tidewater glacier located on the south coast of Alaska. It has lost half of its <span class="hlt">volume</span> during 1957-2007, more rapidly after 1980. It is now split into two branches, known as Main/East and West branch due to the dramatic retreat of ~ 23 km and calving of iceberg from its terminus in past few decades. In Alaska, a majority of the mass loss from glaciers is due to rapid <span class="hlt">ice</span> flow and calving icebergs into tidewater and lacustrine environments. In addition, submarine melting and change in the frontal position can accelerate the <span class="hlt">ice</span> flow and calving rate. We use time series of high-resolution TanDEM-X stripmap satellite imagery during 2011-2013. The active image of the bistatic TanDEM-X acquisitions, acquired over 11 or 22 day repeat intervals, are utilized to derive surface velocity fields using SAR intensity offset tracking. Due to the short temporal baselines, the precise orbit control and the high-resolution of the data, the accuracies of the velocity products are high. We observe a pronounce seasonal signal in flow velocities close to the glacier front of East/Main branch of Columbia Glacier. Maximum values at the glacier front reach up to 14 m/day were recorded in May 2012 and 12 m/day in June 2013. Minimum velocities at the glacier front are generally observed in September and October with lowest values below 2 m/day in October 2012. Months in between those dates show corresponding increase or deceleration resulting a kind of sinusoidal annual course of the surface velocity at the glacier front. The seasonal signal is consistently decreasing with the distance from the glacier front. At a distance of 17.5 km from the <span class="hlt">ice</span> front, velocities are reduced to 2 m/day and almost no seasonal <span class="hlt">variability</span> can be observed. We attribute these temporal and spatial <span class="hlt">variability</span> to changes in the basal hydrology and lubrification of the glacier bed. Closure of the basal drainage system in early winter leads to maximum speeds while during a fully</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016E%26PSL.444...75A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016E%26PSL.444...75A"><span>Late Miocene-Pliocene Asian monsoon intensification linked to Antarctic <span class="hlt">ice</span>-sheet growth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ao, Hong; Roberts, Andrew P.; Dekkers, Mark J.; Liu, Xiaodong; Rohling, Eelco J.; Shi, Zhengguo; An, Zhisheng; Zhao, Xiang</p> <p>2016-06-01</p> <p>Environmental conditions in one of Earth's most densely populated regions, East Asia, are dominated by the monsoon. While Quaternary monsoon <span class="hlt">variability</span> is reasonably well understood, pre-Quaternary monsoon <span class="hlt">variability</span> and dynamics remain enigmatic. In particular, little is known about potential relationships between northern hemispheric monsoon response and major Cenozoic changes in Antarctic <span class="hlt">ice</span> cover. Here we document long-term East Asian summer monsoon (EASM) intensification through the Late Miocene-Pliocene (∼8.2 to 2.6 Ma), and attribute this to progressive Antarctic glaciation. Our new high-resolution magnetic records of long-term EASM intensification come from the Late Miocene-Pliocene Red Clay sequence on the Chinese Loess Plateau; we identify underlying mechanisms using a numerical climate-model simulation of EASM response to an idealized stepwise increase in Antarctic <span class="hlt">ice</span> <span class="hlt">volume</span>. We infer that progressive Antarctic glaciation caused intensification of the cross-equatorial pressure gradient between an atmospheric high-pressure cell over Australia and a low-pressure cell over mid-latitude East Asia, as well as intensification of the cross-equatorial sea-surface temperature (SST) gradient. These combined atmospheric and oceanic adjustments led to EASM intensification. Our findings offer a new and more global perspective on the controls behind long-term Asian monsoon evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A23J0359A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A23J0359A"><span>Late Miocene-Pliocene Asian monsoon intensification linked to Antarctic <span class="hlt">ice</span>-sheet growth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ao, H.; Roberts, A. P.; Dekkers, M. J.; Liu, X.; Rohling, E. J.; Shi, Z.; An, Z.; Zhao, X.</p> <p>2016-12-01</p> <p>Environmental conditions in one of Earth's most densely populated regions, East Asia, are dominated by the monsoon. While Quaternary monsoon <span class="hlt">variability</span> is reasonably well understood, pre-Quaternary monsoon <span class="hlt">variability</span> and dynamics remain enigmatic. In particular, little is known about potential relationships between northern hemispheric monsoon response and major Cenozoic changes in Antarctic <span class="hlt">ice</span> cover. Here we document long-term East Asian summer monsoon (EASM) intensification through the Late Miocene-Pliocene (˜8.2 to 2.6 Ma), and attribute this to progressive Antarctic glaciation. Our new high-resolution magnetic records of long-term EASM intensification come from the Late Miocene-Pliocene Red Clay sequence on the Chinese Loess Plateau; we identify underlying mechanisms using a numerical climate-model simulation of EASM response to an idealized stepwise increase in Antarctic <span class="hlt">ice</span> <span class="hlt">volume</span>. We infer that progressive Antarctic glaciation caused intensification of the cross-equatorial pressure gradient between an atmospheric high-pressure cell over Australia and a low-pressure cell over mid-latitude East Asia, as well as intensification of the cross-equatorial sea-surface temperature (SST) gradient. These combined atmospheric and oceanic adjustments led to EASM intensification. Our findings offer a new and more global perspective on the controls behind long-term Asian monsoon evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060012295','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060012295"><span>A Model Assessment of Satellite Observed Trends in Polar Sea <span class="hlt">Ice</span> Extents</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vinnikov, Konstantin Y.; Cavalieri, Donald J.; Parkinson, Claire L.</p> <p>2005-01-01</p> <p>For more than three decades now, satellite passive microwave observations have been used to monitor polar sea <span class="hlt">ice</span>. Here we utilize sea <span class="hlt">ice</span> extent trends determined from primarily satellite data for both the Northern and Southern Hemispheres for the period 1972(73)-2004 and compare them with results from simulations by eleven climate models. In the Northern Hemisphere, observations show a statistically significant decrease of sea <span class="hlt">ice</span> extent and an acceleration of sea <span class="hlt">ice</span> retreat during the past three decades. However, from the modeled natural <span class="hlt">variability</span> of sea <span class="hlt">ice</span> extents in control simulations, we conclude that the acceleration is not statistically significant and should not be extrapolated into the future. Observations and model simulations show that the time scale of climate <span class="hlt">variability</span> in sea <span class="hlt">ice</span> extent in the Southern Hemisphere is much larger than in the Northern Hemisphere and that the Southern Hemisphere sea <span class="hlt">ice</span> extent trends are not statistically significant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/983033','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/983033"><span>Medical <span class="hlt">ice</span> slurry production device</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Kasza, Kenneth E [Palos Park, IL; Oras, John [Des Plaines, IL; Son, HyunJin [Naperville, IL</p> <p>2008-06-24</p> <p>The present invention relates to an apparatus for producing sterile <span class="hlt">ice</span> slurries for medical cooling applications. The apparatus is capable of producing highly loaded slurries suitable for delivery to targeted internal organs of a patient, such as the brain, heart, lungs, stomach, kidneys, pancreas, and others, through medical size diameter tubing. The <span class="hlt">ice</span> slurry production apparatus includes a slurry production reservoir adapted to contain a <span class="hlt">volume</span> of a saline solution. A flexible membrane crystallization surface is provided within the slurry production reservoir. The crystallization surface is chilled to a temperature below a freezing point of the saline solution within the reservoir such that <span class="hlt">ice</span> particles form on the crystallization surface. A deflector in the form of a reciprocating member is provided for periodically distorting the crystallization surface and dislodging the <span class="hlt">ice</span> particles which form on the crystallization surface. Using reservoir mixing the slurry is conditioned for easy pumping directly out of the production reservoir via medical tubing or delivery through other means such as squeeze bottles, squeeze bags, hypodermic syringes, manual hand delivery, and the like.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMOS31C1297H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMOS31C1297H"><span>Transient sensitivities of sea <span class="hlt">ice</span> export through the Canadian Arctic Archipelago inferred from a coupled ocean/sea-<span class="hlt">ice</span> adjoint model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heimbach, P.; Losch, M.; Menemenlis, D.; Campin, J.; Hill, C.</p> <p>2008-12-01</p> <p>The sensitivity of sea-<span class="hlt">ice</span> export through the Canadian Arctic Archipelago (CAA), measured in terms of its solid freshwater export through Lancaster Sound, to changes in various elements of the ocean and sea-<span class="hlt">ice</span> state, and to elements of the atmospheric forcing fields through time and space is assessed by means of a coupled ocean/sea-<span class="hlt">ice</span> adjoint model. The adjoint model furnishes full spatial sensitivity maps (also known as Lagrange multipliers) of the export metric to a variety of model <span class="hlt">variables</span> at any chosen point in time, providing the unique capability to quantify major drivers of sea-<span class="hlt">ice</span> export <span class="hlt">variability</span>. The underlying model is the MIT ocean general circulation model (MITgcm), which is coupled to a Hibler-type dynamic/thermodynamic sea-<span class="hlt">ice</span> model. The configuration is based on the Arctic face of the ECCO3 high-resolution cubed-sphere model, but coarsened to 36-km horizontal grid spacing. The adjoint of the coupled system has been derived by means of automatic differentiation using the software tool TAF. Finite perturbation simulations are performed to check the information provided by the adjoint. The sea-<span class="hlt">ice</span> model's performance in the presence of narrow straits is assessed with different sea-<span class="hlt">ice</span> lateral boundary conditions. The adjoint sensitivity clearly exposes the role of the model trajectory and the transient nature of the problem. The complex interplay between forcing, dynamics, and boundary condition is demonstrated in the comparison between the different calculations. The study is a step towards fully coupled adjoint-based ocean/sea-<span class="hlt">ice</span> state estimation at basin to global scales as part of the ECCO efforts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ClDy...46.2391T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ClDy...46.2391T"><span>Antarctic sea <span class="hlt">ice</span> increase consistent with intrinsic <span class="hlt">variability</span> of the Amundsen Sea Low</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Turner, John; Hosking, J. Scott; Marshall, Gareth J.; Phillips, Tony; Bracegirdle, Thomas J.</p> <p>2016-04-01</p> <p>We investigate the relationship between atmospheric circulation <span class="hlt">variability</span> and the recent trends in Antarctic sea <span class="hlt">ice</span> extent (SIE) using Coupled Model Intercomparison Project Phase 5 (CMIP5) atmospheric data, ECMWF Interim reanalysis fields and passive microwave satellite data processed with the Bootstrap version 2 algorithm. Over 1979-2013 the annual mean total Antarctic SIE increased at a rate of 195 × 103 km2 dec-1 (1.6 % dec-1), p < 0.01. The largest regional positive trend of annual mean SIE of 119 × 103 km2 dec-1 (4.0 % dec-1) has been in the Ross Sea sector. Off West Antarctica there is a high correlation between trends in SIE and trends in the near-surface winds. The Ross Sea SIE seasonal trends are positive throughout the year, but largest in spring. The stronger meridional flow over the Ross Sea has been driven by a deepening of the Amundsen Sea Low (ASL). Pre-industrial control and historical simulations from CMIP5 indicate that the observed deepening of the ASL and stronger southerly flow over the Ross Sea are within the bounds of modeled intrinsic <span class="hlt">variability</span>. The spring trend would need to continue for another 11 years for it to fall outside the 2 standard deviation range seen in 90 % of the simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012Icar..220.1112S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012Icar..220.1112S"><span>History and anatomy of subsurface <span class="hlt">ice</span> on Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schorghofer, Norbert; Forget, Francois</p> <p>2012-08-01</p> <p><span class="hlt">Ice</span> buried beneath a thin layer of soil has been revealed by neutron spectroscopy and explored by the Phoenix Mars Lander. It has also been exposed by recent impacts. This subsurface <span class="hlt">ice</span> is thought to lose and gain <span class="hlt">volume</span> in response to orbital variations (Milankovitch cycles). We use a powerful numerical model to follow the growth and retreat of near-surface <span class="hlt">ice</span> as a result of regolith-atmosphere exchange continuously over millions of years. If a thick layer of almost pure <span class="hlt">ice</span> has been deposited recently, it has not yet reached equilibrium with the atmospheric water vapor and may still remain as far equatorward as 43°N, where <span class="hlt">ice</span> has been revealed by recent impacts. A potentially observable consequence is present-day humidity output from the still retreating <span class="hlt">ice</span>. We also demonstrate that in a sublimation environment, subsurface pore <span class="hlt">ice</span> can accumulate in two ways. The first mode, widely known, is the progressive filling of pores by <span class="hlt">ice</span> over a range of depths. The second mode occurs on top of an already impermeable <span class="hlt">ice</span> layer; subsequent <span class="hlt">ice</span> accumulates in the form of pasted on horizontal layers such that beneath the <span class="hlt">ice</span> table, the pores are completely full with <span class="hlt">ice</span>. Most or all of the pore <span class="hlt">ice</span> on Mars today may be of the second type. At the Phoenix landing site, where such a layer is also expected to exist above an underlying <span class="hlt">ice</span> sheet, it may be extremely thin, due to exceptionally small variations in <span class="hlt">ice</span> stability over time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1614037S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1614037S"><span>Comparing the <span class="hlt">ice</span> nucleation efficiencies of <span class="hlt">ice</span> nucleating substrates to natural mineral dusts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steinke, Isabelle; Funk, Roger; Höhler, Kristina; Haarig, Moritz; Hoffmann, Nadine; Hoose, Corinna; Kiselev, Alexei; Möhler, Ottmar; Leisner, Thomas</p> <p>2014-05-01</p> <p>Mineral dust particles in the atmosphere may act as efficient <span class="hlt">ice</span> nuclei over a wide range of temperature and relative humidity conditions. The <span class="hlt">ice</span> nucleation capability of dust particles mostly depends on the particle surface area and the associated physico-chemical surface properties. It has been observed that the surface-related <span class="hlt">ice</span> nucleation efficiency of different dust particles and mineral species can vary by several orders of magnitude. However, the relation between aerosol surface properties and observed <span class="hlt">ice</span> nucleation efficiency is still not completely understood due to the large <span class="hlt">variability</span> of chemical compositions and morphological features. In order to gain a better understanding of small scale freezing processes, we investigated the freezing of several hundreds of small droplets (V=0.4 nl) deposited on materials with reasonably well defined surfaces such as crystalline silicon wafers, graphite and freshly cleaved mica sheets under atmospherically relevant conditions. These substrates are intended to serve as simple model structures compared to the surface of natural aerosol particles. To learn more about the impact of particle morphology on <span class="hlt">ice</span> nucleation processes, we also investigated micro-structured silicon wafers with prescribed trenches. The <span class="hlt">ice</span> nucleation efficiencies deduced from these experiments are expressed as <span class="hlt">ice</span> nucleation active surface site density values. With this approach, the freezing properties of the above-described substrates could be compared to those of natural mineral dusts such as agricultural soil dusts, volcanic ash and fossil diatoms, which have been investigated in AIDA cloud chamber experiments. All tested <span class="hlt">ice</span> nucleating substrates were consistently less efficient at nucleating <span class="hlt">ice</span> than the natural mineral dusts. Crystalline silicon only had a negligible influence on the freezing of small droplets, leading to freezing near the homogeneous freezing temperature threshold. Applying surface structures to silicon led to a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.6524D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.6524D"><span>The seasonal and inter-annual <span class="hlt">variability</span> of sea-<span class="hlt">ice</span>, ocean circulation and marine ecosystems in the Barents Sea: model results against satellite data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dvornikov, Anton; Sein, Dmitry; Ryabchenko, Vladimir; Gorchakov, Victor; Pugalova, Svetlana</p> <p>2015-04-01</p> <p>This study is aimed at modelling the seasonal and inter-annual <span class="hlt">variability</span> of sea-<span class="hlt">ice</span>, ocean circulation and marine ecosystems in the Barents Sea in the modern period. Adequate description of marine ecosystems in the <span class="hlt">ice</span>-covered seas crucially depends on the accuracy in determining of thicknesses of <span class="hlt">ice</span> and snow on the sea surface which control penetrating photosynthetically active radiation under the <span class="hlt">ice</span>. One of the few models of <span class="hlt">ice</span> able to adequately reproduce the dynamics of sea <span class="hlt">ice</span> is the sea <span class="hlt">ice</span> model HELMI [1], containing 7 different categories of <span class="hlt">ice</span>. This model has been imbedded into the Princeton Ocean Model. With this coupled model 2 runs for the period 1998-2007 were performed under different atmospheric forcing prescribed from NCEP/NCAR and ERA-40 archives. For prescribing conditions at the open boundary, all the necessary information about the horizontal velocity, level, temperature and salinity of the water, <span class="hlt">ice</span> thickness and compactness was taken from the results of the global ocean general circulation model of the Max Planck Institute for Meteorology (Hamburg, Germany) MPIOM [2]. The resulting solution with NCEP forcing with a high accuracy simulates the seasonal and inter-annual <span class="hlt">variability</span> of sea surface temperature (SST) estimated from MODIS data. The maximum difference between the calculated and satellite-derived SSTs (averaged over 4 selected areas of the Barents Sea) during the period 2000-2007 does not exceed 1.5 °C. Seasonal and inter-annual variations in the area of <span class="hlt">ice</span> cover are also in good agreement with satellite-derived estimates. Pelagic ecosystem model developed in [3] has been coupled into the above hydrodynamic model and used to calculate the changes in the characteristics of marine ecosystems under NCEP forcing. Preliminarily the ecosystem model has been improved by introducing a parameterization of detritus deposition on the bottom and through the selection of optimal parameters for photosynthesis and zooplankton grazing</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1422909','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1422909"><span>Climate Modeling and Causal Identification for Sea <span class="hlt">Ice</span> Predictability</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>Hunke, Elizabeth Clare; Urrego Blanco, Jorge Rolando; Urban, Nathan Mark</p> <p></p> <p>This project aims to better understand causes of ongoing changes in the Arctic climate system, particularly as decreasing sea <span class="hlt">ice</span> trends have been observed in recent decades and are expected to continue in the future. As part of the Sea <span class="hlt">Ice</span> Prediction Network, a multi-agency effort to improve sea <span class="hlt">ice</span> prediction products on seasonal-to-interannual time scales, our team is studying sensitivity of sea <span class="hlt">ice</span> to a collection of physical process and feedback mechanism in the coupled climate system. During 2017 we completed a set of climate model simulations using the fully coupled ACME-HiLAT model. The simulations consisted of experiments inmore » which cloud, sea <span class="hlt">ice</span>, and air-ocean turbulent exchange parameters previously identified as important for driving output uncertainty in climate models were perturbed to account for parameter uncertainty in simulated climate <span class="hlt">variables</span>. We conducted a sensitivity study to these parameters, which built upon a previous study we made for standalone simulations (Urrego-Blanco et al., 2016, 2017). Using the results from the ensemble of coupled simulations, we are examining robust relationships between climate <span class="hlt">variables</span> that emerge across the experiments. We are also using causal discovery techniques to identify interaction pathways among climate <span class="hlt">variables</span> which can help identify physical mechanisms and provide guidance in predictability studies. This work further builds on and leverages the large ensemble of standalone sea <span class="hlt">ice</span> simulations produced in our previous w14_seaice project.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAG...150...11L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAG...150...11L"><span>Estimating water <span class="hlt">volume</span> stored in the south-eastern Greenland firn aquifer using magnetic-resonance soundings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Legchenko, Anatoly; Miège, Clément; Koenig, Lora S.; Forster, Richard R.; Miller, Olivia; Solomon, D. K.; Schmerr, Nicholas; Montgomery, Lynn; Ligtenberg, Stefan; Brucker, Ludovic</p> <p>2018-03-01</p> <p>Recent observations of the Greenland <span class="hlt">ice</span> sheet show an increase of the area affected by progressive melt of snow and <span class="hlt">ice</span>, thus resulting in production of the additional meltwater. In 2011, an important storage of meltwater in the firn has been observed in the S-E Greenland. This water does not freeze during the wintertime and forms a perennial firn aquifer. The aquifer spatial extent has been initially monitored with combined ground and airborne radar observations, but these geophysical techniques are not able to inform us on the amount of meltwater stored at depth. In this study, we use the magnetic resonance soundings (MRS) method for estimating the <span class="hlt">volume</span> of water stored in the Greenland <span class="hlt">ice</span> sheet firn and mapping its spatial <span class="hlt">variability</span>. Our study area covers a firn aquifer along a 16-km E-W transect, ranging between elevations of 1520 and 1760 m. In July 2015 and July 2016, we performed MRS measurements that allow estimating the water <span class="hlt">volume</span> in the studied area as well as the one-year water <span class="hlt">volume</span> evolution. Water storage is not homogeneous, fluctuating between 0.2 and 2 m3/m2, and contains discontinuities in the hydrodynamic properties. We estimate an average <span class="hlt">volume</span> of water stored in the firn in 2016 to be 0.76 m3/m2, which corresponds to a 0.76-m-thick layer of bulk water. MRS monitoring reveals that from April 2015 to July 2016 the <span class="hlt">volume</span> of water stored at the location of our transect increases by about 36%. We found MRS-estimated depth to water in a good agreement with that obtained with the ground penetrating radar (GPR).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19900011246','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19900011246"><span>Satellite radar altimetry over <span class="hlt">ice</span>. <span class="hlt">Volume</span> 1: Processing and corrections of Seasat data over Greenland</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; Brenner, Anita C.; Major, Judith A.; Martin, Thomas V.; Bindschadler, Robert A.</p> <p>1990-01-01</p> <p>The data-processing methods and <span class="hlt">ice</span> data products derived from Seasat radar altimeter measurements over the Greenland <span class="hlt">ice</span> sheet and surrounding sea <span class="hlt">ice</span> are documented. The corrections derived and applied to the Seasat radar altimeter data over <span class="hlt">ice</span> are described in detail, including the editing and retracking algorithm to correct for height errors caused by lags in the automatic range tracking circuit. The methods for radial adjustment of the orbits and estimation of the slope-induced errors are given.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016STAdM..17..313S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016STAdM..17..313S"><span>Gas permeability of <span class="hlt">ice</span>-templated, unidirectional porous ceramics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seuba, Jordi; Deville, Sylvain; Guizard, Christian; Stevenson, Adam J.</p> <p>2016-01-01</p> <p>We investigate the gas flow behavior of unidirectional porous ceramics processed by <span class="hlt">ice</span>-templating. The pore <span class="hlt">volume</span> ranged between 54% and 72% and pore size between 2.9 ?m and 19.1 ?m. The maximum permeability (?? m?) was measured in samples with the highest total pore <span class="hlt">volume</span> (72%) and pore size (19.1 ?m). However, we demonstrate that it is possible to achieve a similar permeability (?? m?) at 54% pore <span class="hlt">volume</span> by modification of the pore shape. These results were compared with those reported and measured for isotropic porous materials processed by conventional techniques. In unidirectional porous materials tortuosity (?) is mainly controlled by pore size, unlike in isotropic porous structures where ? is linked to pore <span class="hlt">volume</span>. Furthermore, we assessed the applicability of Ergun and capillary model in the prediction of permeability and we found that the capillary model accurately describes the gas flow behavior of unidirectional porous materials. Finally, we combined the permeability data obtained here with strength data for these materials to establish links between strength and permeability of <span class="hlt">ice</span>-templated materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C41B0701R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C41B0701R"><span>The Relationship Between Arctic Sea <span class="hlt">Ice</span> Albedo and the Geophysical Parameters of the <span class="hlt">Ice</span> Cover</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Riihelä, A.</p> <p>2015-12-01</p> <p>The Arctic sea <span class="hlt">ice</span> cover is thinning and retreating. Remote sensing observations have also shown that the mean albedo of the remaining <span class="hlt">ice</span> cover is decreasing on decadal time scales, albeit with significant annual <span class="hlt">variability</span> (Riihelä et al., 2013, Pistone et al., 2014). Attribution of the albedo decrease between its different drivers, such as decreasing <span class="hlt">ice</span> concentration and enhanced surface melt of the <span class="hlt">ice</span>, remains an important research question for the forecasting of future conditions of the <span class="hlt">ice</span> cover. A necessary step towards this goal is understanding the relationships between Arctic sea <span class="hlt">ice</span> albedo and the geophysical parameters of the <span class="hlt">ice</span> cover. Particularly the question of the relationship between sea <span class="hlt">ice</span> albedo and <span class="hlt">ice</span> age is both interesting and not widely studied. The recent changes in the Arctic sea <span class="hlt">ice</span> zone have led to a substantial decrease of its multi-year sea <span class="hlt">ice</span>, as old <span class="hlt">ice</span> melts and is replaced by first-year <span class="hlt">ice</span> during the next freezing season. It is generally known that younger sea <span class="hlt">ice</span> tends to have a lower albedo than older <span class="hlt">ice</span> because of several reasons, such as wetter snow cover and enhanced melt ponding. However, the quantitative correlation between sea <span class="hlt">ice</span> age and sea <span class="hlt">ice</span> albedo has not been extensively studied to date, excepting in-situ measurement based studies which are, by necessity, focused on a limited area of the Arctic Ocean (Perovich and Polashenski, 2012).In this study, I analyze the dependencies of Arctic sea <span class="hlt">ice</span> albedo relative to the geophysical parameters of the <span class="hlt">ice</span> field. I use remote sensing datasets such as the CM SAF CLARA-A1 (Karlsson et al., 2013) and the NASA MeaSUREs (Anderson et al., 2014) as data sources for the analysis. The studied period is 1982-2009. The datasets are spatiotemporally collocated and analysed. The changes in sea <span class="hlt">ice</span> albedo as a function of sea <span class="hlt">ice</span> age are presented for the whole Arctic Ocean and for potentially interesting marginal sea cases. This allows us to see if the the albedo of the older sea</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23713125','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23713125"><span><span class="hlt">Ice</span> sheets and nitrogen.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wolff, Eric W</p> <p>2013-07-05</p> <p>Snow and <span class="hlt">ice</span> play their most important role in the nitrogen cycle as a barrier to land-atmosphere and ocean-atmosphere exchanges that would otherwise occur. The inventory of nitrogen compounds in the polar <span class="hlt">ice</span> sheets is approximately 260 Tg N, dominated by nitrate in the much larger Antarctic <span class="hlt">ice</span> sheet. <span class="hlt">Ice</span> cores help to inform us about the natural <span class="hlt">variability</span> of the nitrogen cycle at global and regional scale, and about the extent of disturbance in recent decades. Nitrous oxide concentrations have risen about 20 per cent in the last 200 years and are now almost certainly higher than at any time in the last 800 000 years. Nitrate concentrations recorded in Greenland <span class="hlt">ice</span> rose by a factor of 2-3, particularly between the 1950s and 1980s, reflecting a major change in NOx emissions reaching the background atmosphere. Increases in <span class="hlt">ice</span> cores drilled at lower latitudes can be used to validate or constrain regional emission inventories. Background ammonium concentrations in Greenland <span class="hlt">ice</span> show no significant recent trend, although the record is very noisy, being dominated by spikes of input from biomass burning events. Neither nitrate nor ammonium shows significant recent trends in Antarctica, although their natural variations are of biogeochemical and atmospheric chemical interest. Finally, it has been found that photolysis of nitrate in the snowpack leads to significant re-emissions of NOx that can strongly impact the regional atmosphere in snow-covered areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3682747','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3682747"><span><span class="hlt">Ice</span> sheets and nitrogen</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wolff, Eric W.</p> <p>2013-01-01</p> <p>Snow and <span class="hlt">ice</span> play their most important role in the nitrogen cycle as a barrier to land–atmosphere and ocean–atmosphere exchanges that would otherwise occur. The inventory of nitrogen compounds in the polar <span class="hlt">ice</span> sheets is approximately 260 Tg N, dominated by nitrate in the much larger Antarctic <span class="hlt">ice</span> sheet. <span class="hlt">Ice</span> cores help to inform us about the natural <span class="hlt">variability</span> of the nitrogen cycle at global and regional scale, and about the extent of disturbance in recent decades. Nitrous oxide concentrations have risen about 20 per cent in the last 200 years and are now almost certainly higher than at any time in the last 800 000 years. Nitrate concentrations recorded in Greenland <span class="hlt">ice</span> rose by a factor of 2–3, particularly between the 1950s and 1980s, reflecting a major change in NOx emissions reaching the background atmosphere. Increases in <span class="hlt">ice</span> cores drilled at lower latitudes can be used to validate or constrain regional emission inventories. Background ammonium concentrations in Greenland <span class="hlt">ice</span> show no significant recent trend, although the record is very noisy, being dominated by spikes of input from biomass burning events. Neither nitrate nor ammonium shows significant recent trends in Antarctica, although their natural variations are of biogeochemical and atmospheric chemical interest. Finally, it has been found that photolysis of nitrate in the snowpack leads to significant re-emissions of NOx that can strongly impact the regional atmosphere in snow-covered areas. PMID:23713125</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910017261','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910017261"><span>Sea-level response to <span class="hlt">ice</span> sheet evolution: An ocean perspective</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jacobs, Stanley S.</p> <p>1991-01-01</p> <p>The ocean's influence upon and response to Antarctic <span class="hlt">ice</span> sheet changes is considered in relation to sea level rise over recent and future decades. Assuming present day <span class="hlt">ice</span> fronts are in approximate equilibrium, a preliminary budget for the <span class="hlt">ice</span> sheet is estimated from accumulation vs. iceberg calving and the basal melting that occurs beneath floating <span class="hlt">ice</span> shelves. Iceberg calving is derived from the <span class="hlt">volume</span> of large bergs identified and tracked by the Navy/NOAA Joint <span class="hlt">Ice</span> Center and from shipboard observations. Basal melting exceeds 600 cu km/yr and is concentrated near the <span class="hlt">ice</span> fronts and <span class="hlt">ice</span> shelf grounding lines. An apparent negative mass balance for the Antarctic <span class="hlt">ice</span> sheet may result from an anomalous calving rate during the past decade, but there are large uncertainties associated with all components of the <span class="hlt">ice</span> budget. The results from general circulation models are noted in the context of projected precipitation increases and ocean temperature changes on and near the continent. An ocean research program that could help refine budget estimates is consistent with goals of the West Antarctic <span class="hlt">Ice</span> Sheet Initiative.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41E0717L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41E0717L"><span>Albedo Spatial <span class="hlt">Variability</span> and Causes on the Western Greenland <span class="hlt">Ice</span> Sheet Percolation Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, G.; Osterberg, E. C.; Hawley, R. L.; Koffman, B. G.; Marshall, H. P.; Birkel, S. D.; Dibb, J. E.</p> <p>2016-12-01</p> <p>Many recent studies have concluded that Greenland <span class="hlt">Ice</span> Sheet (GIS) mass loss has been accelerating over recent decades, but spatial and temporal variations in GIS mass balance remain poorly understood due to a complex relationship among precipitation and temperature changes, increasing melt and runoff, <span class="hlt">ice</span> discharge, and surface albedo. Satellite measurements from MODerate resolution Imaging Spectroradiometer (MODIS) indicate that albedo has been declining over the past decade, but the cause and extent of GIS albedo change remains poorly constrained by field data. As fresh snow (albedo > 0.85) warms and melts, its albedo decreases due to snow grain growth, promoting solar absorption, higher snowpack temperatures and further melt. However, dark impurities like soot and dust can also significantly reduce snow albedo, even in the dry snow zone. While many regional climate models (e.g. the Regional Atmospheric Climate MOdel - RACMO2) calculate albedo spatial resolutions on the order of 10-30 km, and MODIS averages albedo over 500 m, surface features like sastrugi can affect albedo on much smaller scales. Here we assess the relative importance of grain size and shape vs. impurity concentrations on albedo in the western GIS percolation zone. We collected broadband albedo measurements (300-2500 nm at 3-8 nm resolution) at 35 locations using an ASD FieldSpec4 spectroradiometer to simultaneously quantify radiative fluxes and spectral reflectance. Measurements were collected on 10 x 10 m, 1 x 1 km, 5 x 5 km, and 10 x 10 km grids to determine the spatial <span class="hlt">variability</span> of albedo as part of the 850-km Greenland Traverse for Accumulation and Climate Studies (GreenTrACS) traverse from Raven/Dye 2 to Summit. Additionally, we collected shallow (0-50 cm) snow pit samples every 5 cm at ASD measurement sites to quantify black carbon and mineral dust concentrations and size distributions using a Single Particle Soot Photometer and Coulter Counter, respectively. Preliminary results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C53B0574L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C53B0574L"><span><span class="hlt">Ice</span> Shelf-Ocean Interactions Near <span class="hlt">Ice</span> Rises and <span class="hlt">Ice</span> Rumples</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lange, M. A.; Rückamp, M.; Kleiner, T.</p> <p>2013-12-01</p> <p>The stability of <span class="hlt">ice</span> shelves depends on the existence of embayments and is largely influenced by <span class="hlt">ice</span> rises and <span class="hlt">ice</span> rumples, which act as 'pinning-points' for <span class="hlt">ice</span> shelf movement. Of additional critical importance are interactions between <span class="hlt">ice</span> shelves and the water masses underlying them in <span class="hlt">ice</span> shelf cavities, particularly melting and refreezing processes. The present study aims to elucidate the role of <span class="hlt">ice</span> rises and <span class="hlt">ice</span> rumples in the context of climate change impacts on Antarctic <span class="hlt">ice</span> shelves. However, due to their smaller spatial extent, <span class="hlt">ice</span> rumples react more sensitively to climate change than <span class="hlt">ice</span> rises. Different forcings are at work and need to be considered separately as well as synergistically. In order to address these issues, we have decided to deal with the following three issues explicitly: oceanographic-, cryospheric and general topics. In so doing, we paid particular attention to possible interrelationships and feedbacks in a coupled <span class="hlt">ice</span>-shelf-ocean system. With regard to oceanographic issues, we have applied the ocean circulation model ROMBAX to ocean water masses adjacent to and underneath a number of idealized <span class="hlt">ice</span> shelf configurations: wide and narrow as well as laterally restrained and unrestrained <span class="hlt">ice</span> shelves. Simulations were performed with and without small <span class="hlt">ice</span> rises located close to the calving front. For larger configurations, the impact of the <span class="hlt">ice</span> rises on melt rates at the <span class="hlt">ice</span> shelf base is negligible, while for smaller configurations net melting rates at the <span class="hlt">ice</span>-shelf base differ by a factor of up to eight depending on whether <span class="hlt">ice</span> rises are considered or not. We employed the thermo-coupled <span class="hlt">ice</span> flow model TIM-FD3 to simulate the effects of several <span class="hlt">ice</span> rises and one <span class="hlt">ice</span> rumple on the dynamics of <span class="hlt">ice</span> shelf flow. We considered the complete un-grounding of the <span class="hlt">ice</span> shelf in order to investigate the effect of pinning points of different characteristics (interior or near calving front, small and medium sized) on the resulting flow and stress fields</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAMES...9..854K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAMES...9..854K"><span>LIVVkit: An extensible, python-based, land <span class="hlt">ice</span> verification and validation toolkit for <span class="hlt">ice</span> sheet models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kennedy, Joseph H.; Bennett, Andrew R.; Evans, Katherine J.; Price, Stephen; Hoffman, Matthew; Lipscomb, William H.; Fyke, Jeremy; Vargo, Lauren; Boghozian, Adrianna; Norman, Matthew; Worley, Patrick H.</p> <p>2017-06-01</p> <p>To address the pressing need to better understand the behavior and complex interaction of <span class="hlt">ice</span> sheets within the global Earth system, significant development of continental-scale, dynamical <span class="hlt">ice</span> sheet models is underway. Concurrent to the development of the Community <span class="hlt">Ice</span> Sheet Model (CISM), the corresponding verification and validation (V&V) process is being coordinated through a new, robust, Python-based extensible software package, the Land <span class="hlt">Ice</span> Verification and Validation toolkit (LIVVkit). Incorporated into the typical <span class="hlt">ice</span> sheet model development cycle, it provides robust and automated numerical verification, software verification, performance validation, and physical validation analyses on a variety of platforms, from personal laptops to the largest supercomputers. LIVVkit operates on sets of regression test and reference data sets, and provides comparisons for a suite of community prioritized tests, including configuration and parameter variations, bit-for-bit evaluation, and plots of model <span class="hlt">variables</span> to indicate where differences occur. LIVVkit also provides an easily extensible framework to incorporate and analyze results of new intercomparison projects, new observation data, and new computing platforms. LIVVkit is designed for quick adaptation to additional <span class="hlt">ice</span> sheet models via abstraction of model specific code, functions, and configurations into an <span class="hlt">ice</span> sheet model description bundle outside the main LIVVkit structure. Ultimately, through shareable and accessible analysis output, LIVVkit is intended to help developers build confidence in their models and enhance the credibility of <span class="hlt">ice</span> sheet models overall.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1338808','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1338808"><span>The CMIP6 Sea-<span class="hlt">Ice</span> Model Intercomparison Project (SIMIP): Understanding sea <span class="hlt">ice</span> through climate-model simulations</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>Notz, Dirk; Jahn, Alexandra; Holland, Marika</p> <p></p> <p>A better understanding of the role of sea <span class="hlt">ice</span> for the changing climate of our planet is the central aim of the diagnostic Coupled Model Intercomparison Project 6 (CMIP6)-endorsed Sea-<span class="hlt">Ice</span> Model Intercomparison Project (SIMIP). To reach this aim, SIMIP requests sea-<span class="hlt">ice</span>-related <span class="hlt">variables</span> from climate-model simulations that allow for a better understanding and, ultimately, improvement of biases and errors in sea-<span class="hlt">ice</span> simulations with large-scale climate models. This then allows us to better understand to what degree CMIP6 model simulations relate to reality, thus improving our confidence in answering sea-<span class="hlt">ice</span>-related questions based on these simulations. Furthermore, the SIMIP protocol provides a standardmore » for sea-<span class="hlt">ice</span> model output that will streamline and hence simplify the analysis of the simulated sea-<span class="hlt">ice</span> evolution in research projects independent of CMIP. To reach its aims, SIMIP provides a structured list of model output that allows for an examination of the three main budgets that govern the evolution of sea <span class="hlt">ice</span>, namely the heat budget, the momentum budget, and the mass budget. Furthermore, we explain the aims of SIMIP in more detail and outline how its design allows us to answer some of the most pressing questions that sea <span class="hlt">ice</span> still poses to the international climate-research community.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1338808-cmip6-sea-ice-model-intercomparison-project-simip-understanding-sea-ice-through-climate-model-simulations','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1338808-cmip6-sea-ice-model-intercomparison-project-simip-understanding-sea-ice-through-climate-model-simulations"><span>The CMIP6 Sea-<span class="hlt">Ice</span> Model Intercomparison Project (SIMIP): Understanding sea <span class="hlt">ice</span> through climate-model simulations</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Notz, Dirk; Jahn, Alexandra; Holland, Marika; ...</p> <p>2016-09-23</p> <p>A better understanding of the role of sea <span class="hlt">ice</span> for the changing climate of our planet is the central aim of the diagnostic Coupled Model Intercomparison Project 6 (CMIP6)-endorsed Sea-<span class="hlt">Ice</span> Model Intercomparison Project (SIMIP). To reach this aim, SIMIP requests sea-<span class="hlt">ice</span>-related <span class="hlt">variables</span> from climate-model simulations that allow for a better understanding and, ultimately, improvement of biases and errors in sea-<span class="hlt">ice</span> simulations with large-scale climate models. This then allows us to better understand to what degree CMIP6 model simulations relate to reality, thus improving our confidence in answering sea-<span class="hlt">ice</span>-related questions based on these simulations. Furthermore, the SIMIP protocol provides a standardmore » for sea-<span class="hlt">ice</span> model output that will streamline and hence simplify the analysis of the simulated sea-<span class="hlt">ice</span> evolution in research projects independent of CMIP. To reach its aims, SIMIP provides a structured list of model output that allows for an examination of the three main budgets that govern the evolution of sea <span class="hlt">ice</span>, namely the heat budget, the momentum budget, and the mass budget. Furthermore, we explain the aims of SIMIP in more detail and outline how its design allows us to answer some of the most pressing questions that sea <span class="hlt">ice</span> still poses to the international climate-research community.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP33A2293H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP33A2293H"><span>Sea <span class="hlt">ice</span> cover <span class="hlt">variability</span> and river run-off in the western Laptev Sea (Arctic Ocean) since the last 18 ka</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hörner, T.; Stein, R.; Fahl, K.; Birgel, D.</p> <p>2015-12-01</p> <p>Multi-proxy biomarker measurements were performed on two sediment cores (PS51/154, PS51/159) with the objective reconstructing sea <span class="hlt">ice</span> cover (IP25, brassicasterol, dinosterol) and river-runoff (campesterol, β-sitosterol) in the western Laptev Sea over the last 18 ka with unprecedented temporal resolution. The sea <span class="hlt">ice</span> cover varies distinctly during the whole time period. The absence of IP25 during 18 and 16 ka indicate that the western Laptev Sea was mostly covered with permanent sea <span class="hlt">ice</span> (pack <span class="hlt">ice</span>). However, a period of temporary break-up of the permanent <span class="hlt">ice</span> coverage occurred at c. 17.2 ka (presence of IP25). Very little river-runoff occurred during this interval. Decreasing terrigenous (riverine) input and synchronous increase of marine produced organic matter around 16 ka until 7.5 ka indicate the gradual establishment of a marine environment in the western Laptev Sea related to the onset of the post-glacial transgression of the shelf. Strong river run-off and reduced sea <span class="hlt">ice</span> cover characterized the time interval between 15.2 and 12.9 ka, including the Bølling/Allerød warm period (14.7 - 12.9 ka). Moreover, the DIP25 Index (ratio of HBI-dienes and IP25) might document the presence of Atlantic derived water at the western Laptev Sea shelf area. A sudden return to severe sea <span class="hlt">ice</span> conditions occurred during the Younger Dryas (12.9 - 11.6 ka). This abrupt climate change was observed in the whole circum-Arctic realm (Chukchi Sea, Bering Sea, Fram Strait and Laptev Sea). At the onset of the Younger Dryas, a distinct alteration of the ecosystem (deep drop in terrigenous and phytoplankton biomarkers) may document the entry of a giant freshwater plume, possibly relating to the Lake Agassiz outburst at 13 ka. IP25 concentrations increase and higher values of the PIP25 Index during the last 7 ka reflect a cooling of the Laptev Sea spring season. Moreover, a short-term <span class="hlt">variability</span> of c. 1.5 thousand years occurred during the last 12 ka, most probably following Bond Cycles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980107899','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980107899"><span><span class="hlt">Ice</span> in Channels and <span class="hlt">Ice</span>-Rock Mixtures in Valleys on Mars: Did They Slide on Deformable Rubble Like Antarctic <span class="hlt">Ice</span> Streams?</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> 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 was 1 to 2 km, according to the height of bordering scarps. The similarity between Antarctic <span class="hlt">ice</span> streams and martian outflow channels suggests that <span class="hlt">ice</span> may have flowed through and shaped the outflow channels, and that perhaps the mechanism of motion of Antarctic <span class="hlt">ice</span> streams also operated in outflow channels. In addition, sliding on deformable rubble may explain the formation of small valley networks. The large Siple Coast Antarctic <span class="hlt">ice</span> streams are thought to slide over longitudinally grooved, deforming till, where much of the movement is within the till. The till is saturated with water at high pore pressures that nearly supports all of the weight of the <span class="hlt">ice</span>. The small differential between overburden pressure and pore pressure at the bed is more important than the <span class="hlt">volume</span> of water, but water needs to be supplied to the till interface. For pore pressures to remain high, the <span class="hlt">ice</span> streams have to act as a seal that blocks the flow of water through them, and the rock underneath has to be of low permeability to prevent the water from draining away.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3504962','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3504962"><span>Photophysiology and albedo-changing potential of the <span class="hlt">ice</span> algal community on the surface of 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>Yallop, Marian L; Anesio, Alexandre M; Perkins, Rupert G; Cook, Joseph; Telling, Jon; Fagan, Daniel; MacFarlane, James; Stibal, Marek; Barker, Gary; Bellas, Chris; Hodson, Andy; Tranter, Martyn; Wadham, Jemma; Roberts, Nicholas W</p> <p>2012-01-01</p> <p>Darkening of parts of the Greenland <span class="hlt">ice</span> sheet surface during the summer months leads to reduced albedo and increased melting. Here we show that heavily pigmented, actively photosynthesising microalgae and cyanobacteria are present on the bare <span class="hlt">ice</span>. We demonstrate the widespread abundance of green algae in the Zygnematophyceae on the <span class="hlt">ice</span> sheet surface in Southwest Greenland. Photophysiological measurements (<span class="hlt">variable</span> chlorophyll fluorescence) indicate that the <span class="hlt">ice</span> algae likely use screening mechanisms to downregulate photosynthesis when exposed to high intensities of visible and ultraviolet radiation, rather than non-photochemical quenching or cell movement. Using imaging microspectrophotometry, we demonstrate that intact cells and filaments absorb light with characteristic spectral profiles across ultraviolet and visible wavelengths, whereas inorganic dust particles typical for these areas display little absorption. Our results indicate that the phototrophic community growing directly on the bare <span class="hlt">ice</span>, through their photophysiology, most likely have an important role in changing albedo, and subsequently may impact melt rates on the <span class="hlt">ice</span> sheet. PMID:23018772</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23018772','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23018772"><span>Photophysiology and albedo-changing potential of the <span class="hlt">ice</span> algal community on the surface 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>Yallop, Marian L; Anesio, Alexandre M; Perkins, Rupert G; Cook, Joseph; Telling, Jon; Fagan, Daniel; MacFarlane, James; Stibal, Marek; Barker, Gary; Bellas, Chris; Hodson, Andy; Tranter, Martyn; Wadham, Jemma; Roberts, Nicholas W</p> <p>2012-12-01</p> <p>Darkening of parts of the Greenland <span class="hlt">ice</span> sheet surface during the summer months leads to reduced albedo and increased melting. Here we show that heavily pigmented, actively photosynthesising microalgae and cyanobacteria are present on the bare <span class="hlt">ice</span>. We demonstrate the widespread abundance of green algae in the Zygnematophyceae on the <span class="hlt">ice</span> sheet surface in Southwest Greenland. Photophysiological measurements (<span class="hlt">variable</span> chlorophyll fluorescence) indicate that the <span class="hlt">ice</span> algae likely use screening mechanisms to downregulate photosynthesis when exposed to high intensities of visible and ultraviolet radiation, rather than non-photochemical quenching or cell movement. Using imaging microspectrophotometry, we demonstrate that intact cells and filaments absorb light with characteristic spectral profiles across ultraviolet and visible wavelengths, whereas inorganic dust particles typical for these areas display little absorption. Our results indicate that the phototrophic community growing directly on the bare <span class="hlt">ice</span>, through their photophysiology, most likely have an important role in changing albedo, and subsequently may impact melt rates on the <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025982','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025982"><span>Medieval Warm Period, Little <span class="hlt">Ice</span> Age and 20th century temperature <span class="hlt">variability</span> from Chesapeake Bay</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Cronin, T. M.; Dwyer, G.S.; Kamiya, T.; Schwede, S.; Willard, D.A.</p> <p>2003-01-01</p> <p>We present paleoclimate evidence for rapid (< 100 years) shifts of ~2-4oC in Chesapeake Bay (CB) temperature ~2100, 1600, 950, 650, 400 and 150 years before present (years BP) reconstructed from magnesium/calcium (Mg/Ca) paleothermometry. These include large temperature excursions during the Little <span class="hlt">Ice</span> Age (~1400-1900 AD) and the Medieval Warm Period (~800-1300 AD) possibly related to changes in the strength of North Atlantic thermohaline circulation (THC). Evidence is presented for a long period of sustained regional and North Atlantic-wide warmth with low-amplitude temperature <span class="hlt">variability</span> between ~450 and 1000 AD. In addition to centennial-scale temperature shifts, the existence of numerous temperature maxima between 2200 and 250 years BP (average ~70 years) suggests that multi-decadal processes typical of the North Atlantic Oscillation (NAO) are an inherent feature of late Holocene climate. However, late 19th and 20th century temperature extremes in Chesapeake Bay associated with NAO climate <span class="hlt">variability</span> exceeded those of the prior 2000 years, including the interval 450-1000 AD, by 2-3oC, suggesting anomalous recent behavior of the climate system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010ACPD...1011513W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010ACPD...1011513W"><span>High <span class="hlt">variability</span> of the heterogeneous <span class="hlt">ice</span> nucleation potential of oxalic acid dihydrate and sodium oxalate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wagner, R.; Möhler, O.; Saathoff, H.; Schnaiter, M.; Leisner, T.</p> <p>2010-04-01</p> <p>The heterogeneous <span class="hlt">ice</span> nucleation potential of airborne oxalic acid dihydrate and sodium oxalate particles in the deposition and condensation mode has been investigated by controlled expansion cooling cycles in the AIDA aerosol and cloud chamber of the Karlsruhe Institute of Technology at temperatures between 244 and 228 K. Previous laboratory studies have highlighted the particular role of oxalic acid dihydrate as the only species amongst a variety of other investigated dicarboxylic acids to be capable of acting as a heterogeneous <span class="hlt">ice</span> nucleus in both the deposition and immersion mode. We could confirm a high deposition mode <span class="hlt">ice</span> activity for 0.03 to 0.8 μm sized oxalic acid dihydrate particles that were either formed by nucleation from a gaseous oxalic acid/air mixture or by rapid crystallisation of highly supersaturated aqueous oxalic acid solution droplets. The critical saturation ratio with respect to <span class="hlt">ice</span> required for deposition nucleation was found to be less than 1.1 and the size-dependent <span class="hlt">ice</span>-active fraction of the aerosol population was in the range from 0.1 to 22%. In contrast, oxalic acid dihydrate particles that had crystallised from less supersaturated solution droplets and had been allowed to slowly grow in a supersaturated environment from still unfrozen oxalic acid solution droplets over a time period of several hours were found to be much poorer heterogeneous <span class="hlt">ice</span> nuclei. We speculate that under these conditions a crystal surface structure with less-active sites for the initiation of <span class="hlt">ice</span> nucleation was generated. Such particles partially proved to be almost <span class="hlt">ice</span>-inactive in both the deposition and condensation mode. At times, the heterogeneous <span class="hlt">ice</span> nucleation ability of oxalic acid dihydrate significantly changed when the particles had been processed in preceding cloud droplet activation steps. Such behaviour was also observed for the second investigated species, namely sodium oxalate. Our experiments address the atmospheric scenario that coating layers</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010ACP....10.7617W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010ACP....10.7617W"><span>High <span class="hlt">variability</span> of the heterogeneous <span class="hlt">ice</span> nucleation potential of oxalic acid dihydrate and sodium oxalate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wagner, R.; Möhler, O.; Saathoff, H.; Schnaiter, M.; Leisner, T.</p> <p>2010-08-01</p> <p>The heterogeneous <span class="hlt">ice</span> nucleation potential of airborne oxalic acid dihydrate and sodium oxalate particles in the deposition and condensation mode has been investigated by controlled expansion cooling cycles in the AIDA aerosol and cloud chamber of the Karlsruhe Institute of Technology at temperatures between 244 and 228 K. Previous laboratory studies have highlighted the particular role of oxalic acid dihydrate as the only species amongst a variety of other investigated dicarboxylic acids to be capable of acting as a heterogeneous <span class="hlt">ice</span> nucleus in both the deposition and immersion mode. We could confirm a high deposition mode <span class="hlt">ice</span> activity for 0.03 to 0.8 μm sized oxalic acid dihydrate particles that were either formed by nucleation from a gaseous oxalic acid/air mixture or by rapid crystallisation of highly supersaturated aqueous oxalic acid solution droplets. The critical saturation ratio with respect to <span class="hlt">ice</span> required for deposition nucleation was found to be less than 1.1 and the size-dependent <span class="hlt">ice</span>-active fraction of the aerosol population was in the range from 0.1 to 22%. In contrast, oxalic acid dihydrate particles that had crystallised from less supersaturated solution droplets and had been allowed to slowly grow in a supersaturated environment from still unfrozen oxalic acid solution droplets over a time period of several hours were found to be much poorer heterogeneous <span class="hlt">ice</span> nuclei. We speculate that under these conditions a crystal surface structure with less-active sites for the initiation of <span class="hlt">ice</span> nucleation was generated. Such particles partially proved to be almost <span class="hlt">ice</span>-inactive in both the deposition and condensation mode. At times, the heterogeneous <span class="hlt">ice</span> nucleation ability of oxalic acid dihydrate significantly changed when the particles had been processed in preceding cloud droplet activation steps. Such behaviour was also observed for the second investigated species, namely sodium oxalate. Our experiments address the atmospheric scenario that coating layers</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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