<?xml version="1.0" encoding="utf-8"?><!DOCTYPE rss PUBLIC "-//Netscape Communications//DTD RSS 0.91//EN" "http://my.netscape.com/publish/formats/rss-0.91.dtd"><rss version="0.91"><channel><title>TC - Latest Articles</title><link>http://www.the-cryosphere.net/</link> <description>The Cryosphere Latest Articles</description><language>en</language><item><title>Corrigendum to &quot;Influence of ablation-related processes in the build-up of simulated Northern Hemisphere ice sheets during the last glacial cycle&quot; published in The Cryosphere, 7, 681&amp;ndash;698, 2013</title><link>http://www.the-cryosphere.net/7/933/2013/</link><description>&lt;b&gt;Corrigendum to &quot;Influence of ablation-related processes in the build-up of simulated Northern Hemisphere ice sheets during the last glacial cycle&quot; published in The Cryosphere, 7, 681&amp;ndash;698, 2013&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 933-934, 2013&lt;br /&gt;&lt;br /&gt;Author(s): S. Charbit, C. Dumas, M. Kageyama, D. M. Roche, and C. Ritz&lt;br /&gt;&lt;br /&gt;No abstract available.</description><pubDate>Mon, 17 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Seasonal controls on snow distribution and aerial ablation at the snow-patch and landscape scales, McMurdo Dry Valleys, Antarctica</title><link>http://www.the-cryosphere.net/7/917/2013/</link><description>&lt;b&gt;Seasonal controls on snow distribution and aerial ablation at the snow-patch and landscape scales, McMurdo Dry Valleys, Antarctica&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 917-931, 2013&lt;br /&gt;&lt;br /&gt;Author(s): J. W. Eveland, M. N. Gooseff, D. J. Lampkin, J. E. Barrett, and C. D. Takacs-Vesbach&lt;br /&gt;&lt;br /&gt;Accumulated snow in the McMurdo Dry Valleys, while limited, has great
ecological significance to subnivian soil environments. Though sublimation
dominates the ablation process in this region, measurable increases in soil
moisture and insulation from temperature extremes provide more favorable
conditions with respect to subnivian soil communities. While precipitation
is not substantial, significant amounts of snow can accumulate, via wind
transport, in topographic lees along the valley bottoms, forming thousands
of discontinuous snow patches. These patches have the potential to act as
significant sources of local meltwater, controlling biogeochemical cycling
and the landscape distribution of microbial communities. Therefore,
determining the spatial and temporal dynamics of snow at multiple scales is
imperative to understanding the broader ecological role of snow in this
region.
&lt;br&gt;&lt;br&gt;
High-resolution satellite imagery acquired during the 2009–2010 and
2010–2011 austral summers was used to quantify the distribution of snow
across Taylor and Wright valleys. Extracted snow-covered area from the
imagery was used as the basis for assessing inter-annual variability and
seasonal controls on accumulation and ablation of snow at multiple scales.
In addition to landscape analyses, fifteen 1 km&lt;sup&gt;2&lt;/sup&gt; plots (3 in each of 5
study regions) were selected to assess the prevalence of snow cover at finer
spatial scales, referred to herein as the snow-patch scale. Results confirm
that snow patches tend to form in the same locations each year with some
minor deviations observed. At the snow-patch scale, neighboring patches
often exhibit considerable differences in aerial ablation rates, and
particular snow patches do not reflect trends for snow-covered area observed
at the landscape scale. These differences are presumably related to
microtopographic influences acting on individual snow patches, such as wind
sheltering and differences in snow depth due to the underlying topography.
This highlights the importance of both the landscape and snow-patch scales
in assessing the effects of snow cover on biogeochemical cycling and
microbial communities.</description><pubDate>Tue, 11 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Recent changes in spring snowmelt timing in the Yukon River basin detected by passive microwave satellite data</title><link>http://www.the-cryosphere.net/7/905/2013/</link><description>&lt;b&gt;Recent changes in spring snowmelt timing in the Yukon River basin detected by passive microwave satellite data&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 905-916, 2013&lt;br /&gt;&lt;br /&gt;Author(s): K. A. Semmens and J. M. Ramage&lt;br /&gt;&lt;br /&gt;Spring melt is a significant feature of high latitude snowmelt dominated
drainage basins influencing hydrological and ecological processes such as
snowmelt runoff and green-up. Melt duration, defined as the transition period
from snowmelt onset until the end of the melt refreeze, is characterized by
high diurnal amplitude variations (DAV) where the snowpack is melting during
the day and refreezing at night, after which the snowpack melts constantly
until depletion. Determining trends for this critical period is necessary for
understanding how the Arctic is changing with rising temperatures and
provides a baseline from which to assess future change. To study this dynamic
period, brightness temperature (&lt;i&gt;T&lt;/i&gt;&lt;sub&gt;b&lt;/sub&gt;) data from the Special Sensor
Microwave Imager (SSM/I) 37 V-GHz frequency from 1988 to 2010 were used to
assess snowmelt timing trends for the Yukon River basin, Alaska/Canada.
Annual &lt;i&gt;T&lt;/i&gt;&lt;sub&gt;b&lt;/sub&gt; and DAV for 1434 Equal-Area Scalable Earth (EASE)-Grid
pixels (25 km resolution) were processed to determine melt onset and melt
refreeze dates from &lt;i&gt;T&lt;/i&gt;&lt;sub&gt;b&lt;/sub&gt; and DAV thresholds previously established
in the region. Temporal and spatial trends in the timing of melt onset and
melt refreeze, and the duration of melt were analyzed for the 13 sub-basins
of the Yukon River basin with three different time interval approaches.
Results show a lengthening of the melt period for the majority of the
sub-basins with a significant trend toward later end of melt refreeze after
which the snowpack melts day and night leading to snow clearance, peak
discharge, and green-up. Earlier melt onset trends were also found in the
higher elevations and northernmost sub-basins (Porcupine, Chandalar, and
Koyukuk rivers). Latitude and elevation displayed the dominant controls on
melt timing variability and spring solar flux was highly correlated with melt
timing in middle (&amp;sim;600–1600 m) elevations.</description><pubDate>Wed, 05 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Quantifying present and future glacier melt-water contribution to runoff in a central Himalayan river basin</title><link>http://www.the-cryosphere.net/7/889/2013/</link><description>&lt;b&gt;Quantifying present and future glacier melt-water contribution to runoff in a central Himalayan river basin&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 889-904, 2013&lt;br /&gt;&lt;br /&gt;Author(s): M. Prasch, W. Mauser, and M. Weber&lt;br /&gt;&lt;br /&gt;Water supply of most lowland cultures heavily depends on rain and melt water
from the upstream mountains. Especially melt-water release of alpine
mountain ranges is usually attributed a pivotal role for the water supply of
large downstream regions. Water scarcity is assumed as consequence of
glacier shrinkage and possible disappearance due to global climate change (GCC),
in particular for large parts of Central and Southeast Asia. In this paper,
the application and validation of a coupled modeling approach with regional
climate model (RCM) outputs and a process-oriented glacier and hydrological model
is presented for the central Himalayan Lhasa River basin despite scarce data
availability. Current and possible future contributions of ice melt to
runoff along the river network are spatially explicitly shown. Its role
among the other water balance components is presented. Although glaciers
have retreated and will continue to retreat according to the chosen climate
scenarios, water availability is and will be primarily determined by monsoon
precipitation and snowmelt. Ice melt from glaciers is and will be a minor
runoff component in summer monsoon-dominated Himalayan river basins.</description><pubDate>Tue, 28 May 2013 00:00:00 +0200</pubDate></item><item><title>Density assumptions for converting geodetic glacier volume change to mass change</title><link>http://www.the-cryosphere.net/7/877/2013/</link><description>&lt;b&gt;Density assumptions for converting geodetic glacier volume change to mass change&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 877-887, 2013&lt;br /&gt;&lt;br /&gt;Author(s): M. Huss&lt;br /&gt;&lt;br /&gt;The geodetic method is widely used for assessing changes in the
      mass balance of mountain glaciers. However, comparison of
      repeated digital elevation models only provides a glacier volume
      change that must be converted to a change in mass using
      a density assumption or model. This study investigates the use
      of a constant factor for the volume-to-mass conversion based on
      a firn compaction model applied to simplified glacier geometries
      with idealized climate forcing, and two glaciers with long-term
      mass balance series.  It is shown that the &quot;density&quot; of
      geodetic volume change is not a constant factor and is
      systematically smaller than ice density in most cases. This is
      explained by the accretion/removal of low-density firn layers,
      and changes in the firn density profile with positive/negative
      mass balance. Assuming a value of 850 &amp;pm; 60 kg m&lt;sup&gt;&amp;minus;3&lt;/sup&gt;
      to convert volume change to mass change is appropriate for
      a wide range of conditions. For short time intervals
      (&amp;leq;3 yr), periods with limited volume change,
      and/or changing mass balance gradients, the conversion factor
      can however vary from 0–2000 kg m&lt;sup&gt;&amp;minus;3&lt;/sup&gt; and beyond,
      which requires caution when interpreting glacier mass changes
      based on geodetic surveys.</description><pubDate>Mon, 27 May 2013 00:00:00 +0200</pubDate></item><item><title>Mass balance, runoff and surges of Bering Glacier, Alaska</title><link>http://www.the-cryosphere.net/7/867/2013/</link><description>&lt;b&gt;Mass balance, runoff and surges of Bering Glacier, Alaska&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 867-875, 2013&lt;br /&gt;&lt;br /&gt;Author(s): W. Tangborn&lt;br /&gt;&lt;br /&gt;The historical net, ablation and accumulation daily balances, as well as runoff of
Bering Glacier, Alaska are determined for the 1951–2011 period with the PTAA
(precipitation-temperature-area-altitude) model, using daily precipitation
and temperature observations collected at the Cordova and Yakutat weather
stations, together with the area-altitude distribution of the glacier. The
model mean annual balance for this 61 yr period is −0.6 m w.e., the
accumulation balance is +1.4 and the ablation balance is −2.0 m w.e.
Average annual runoff is 2.5 m w.e. Periodic surges of this glacier
transport large volumes of ice to lower elevations where the ablation rate is
higher, producing more negative balances and increasing runoff. Runoff from
Bering Glacier (derived from simulated ablation and precipitation as rain) is
highly correlated with four of the glacier surges that have occurred since
1951. Ice volume loss for the 1972–2003 period measured with the PTAA model
is 2.7 km&lt;sup&gt;3&lt;/sup&gt; w.e. a&lt;sup&gt;−1&lt;/sup&gt; and closely agrees with losses for the same
period measured with the geodetic method. It is proposed that the timing and
magnitude of daily snow accumulation and runoff, both of which are controlled
by the glacier's area-altitude distribution and are calculated with the PTAA
model, can be used to determine the probability that a glacier will surge.</description><pubDate>Mon, 27 May 2013 00:00:00 +0200</pubDate></item><item><title>Radio-frequency probes of Antarctic ice at South Pole</title><link>http://www.the-cryosphere.net/7/855/2013/</link><description>&lt;b&gt;Radio-frequency probes of Antarctic ice at South Pole&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 855-866, 2013&lt;br /&gt;&lt;br /&gt;Author(s): D. Besson and I. Kravchenko&lt;br /&gt;&lt;br /&gt;Using hardware developed for the ARA (Askaryan Radio Array)
particle astrophysics experiment,
we herein report
on the amplitude and temporal characteristics of polarized surface radar
echo data collected in South Polar ice using
radio sounding equipment with 0.5-ns echo-time sampling.
We observe strong echoes at
6, 9.6, 13.9, 17, and 19 μs following
vertical pulse emission from the surface, corresponding to reflectors
in the upper half of the ice sheet. The synchronicity of those echoes
for all broadcast azimuthal polarizations affirms the lack of observable
birefringence over the upper half of the
ice sheet. Of the five strongest
echoes, three exhibit an evident amplitude
correlation with the local surface ice flow direction,
qualitatively consistent with measurements in East Antarctica.
Combined with other radio echo sounding data, we conclude that
observed birefringent asymmetries at South Pole are generated entirely
in the lower half of the ice sheet. By contrast, birefringent asymmetries
are observed at shallow depths in East Antarctica.</description><pubDate>Thu, 16 May 2013 00:00:00 +0200</pubDate></item><item><title>Snow cover thickness estimation using radial basis function networks</title><link>http://www.the-cryosphere.net/7/841/2013/</link><description>&lt;b&gt;Snow cover thickness estimation using radial basis function networks&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 841-854, 2013&lt;br /&gt;&lt;br /&gt;Author(s): E. Binaghi, V. Pedoia, A. Guidali, and M. Guglielmin&lt;br /&gt;&lt;br /&gt;This paper reports an experimental study designed for the in-depth
investigation of how the radial basis function network (RBFN) estimates snow
cover thickness as a function of climate and topographic parameters. The
estimation problem is modeled in terms of both function regression and
classification, obtaining continuous and discrete thickness values,
respectively. The model is based on a minimal set of climatic and topographic
data collected from a limited number of stations located in the Italian
Central Alps. Several experiments have been conceived and conducted adopting
different evaluation indexes. A comparison analysis was also developed for a
quantitative evaluation of the advantages of the RBFN method over to
conventional widely used spatial interpolation techniques when dealing with
critical situations originated by lack of data and limited &lt;i&gt;n&lt;/i&gt;-homogeneously
distributed instrumented sites. The RBFN model proved competitive behavior
and a valuable tool in critical situations in which conventional techniques
suffer from a lack of representative data.</description><pubDate>Tue, 14 May 2013 00:00:00 +0200</pubDate></item><item><title>Satellite-derived volume loss rates and glacier speeds for the Cordillera Darwin Icefield, Chile</title><link>http://www.the-cryosphere.net/7/823/2013/</link><description>&lt;b&gt;Satellite-derived volume loss rates and glacier speeds for the Cordillera Darwin Icefield, Chile&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 823-839, 2013&lt;br /&gt;&lt;br /&gt;Author(s): A. K. Melkonian, M. J. Willis, M. E. Pritchard, A. Rivera, F. Bown, and S. A. Bernstein&lt;br /&gt;&lt;br /&gt;We produce the first icefield-wide volume change rate and glacier velocity
estimates for the Cordillera Darwin Icefield (CDI), a 2605 km&lt;sup&gt;2&lt;/sup&gt;
temperate icefield in southern Chile (69.6° W, 54.6° S).
Velocities are measured from optical and radar imagery between 2001–2011.
Thirty-six digital elevation models (DEMs) from ASTER and the SRTM DEM are
stacked and a weighted linear regression is applied to elevations on a
pixel-by-pixel basis to estimate volume change rates.
&lt;br&gt;&lt;br&gt;
The CDI lost mass at an average rate of −3.9 ± 1.5 Gt yr&lt;sup&gt;−1&lt;/sup&gt;
between 2000 and 2011, equivalent to a sea level rise (SLR) of
0.01 ± 0.004 mm yr&lt;sup&gt;−1&lt;/sup&gt; and an area-averaged thinning rate of
−1.5 ± 0.6 m w.e.(water equivalent) yr&lt;sup&gt;−1&lt;/sup&gt;.
&lt;br&gt;&lt;br&gt;
Thinning is widespread, with concentrations near the front of two northern
glaciers (Marinelli, Darwin) and one western (CDI-08) glacier. Thickening is
apparent in the south, most notably over the advancing Garibaldi Glacier. The
northeastern part of the CDI has an average thinning rate of
−1.9 ± 0.7 m w.e. yr&lt;sup&gt;−1&lt;/sup&gt;, while the southwestern part has
an average thinning rate of −1.0 ± 0.4 m w.e. yr&lt;sup&gt;−1&lt;/sup&gt;.
&lt;br&gt;&lt;br&gt;
Velocities are obtained over many of the CDI glaciers for the first time. We
provide a repeat speed time series at the Marinelli Glacier. There we measure
maximum front speeds of 7.5 ± 0.2 m day&lt;sup&gt;−1&lt;/sup&gt; in 2001,
9.5 ± 0.6 m day&lt;sup&gt;−1&lt;/sup&gt; in 2003 and 10 ± 0.3 m day&lt;sup&gt;−1&lt;/sup&gt; in
2011. The maintenance of high front speeds from 2001 to 2011 supports the
hypothesis that Marinelli is in the retreat phase of the tidewater cycle,
with dynamic thinning governed by the fjord bathymetry.</description><pubDate>Tue, 14 May 2013 00:00:00 +0200</pubDate></item><item><title>Brief communication &quot;Global glacier volumes and sea level &amp;ndash; small but systematic effects of ice below the surface of the ocean and of new local lakes on land&quot;</title><link>http://www.the-cryosphere.net/7/817/2013/</link><description>&lt;b&gt;Brief communication &quot;Global glacier volumes and sea level &amp;ndash; small but systematic effects of ice below the surface of the ocean and of new local lakes on land&quot;&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 817-821, 2013&lt;br /&gt;&lt;br /&gt;Author(s): W. Haeberli and A. Linsbauer&lt;br /&gt;&lt;br /&gt;The potential contribution of glaciers and ice caps to sea level rise is
usually calculated by comparing the estimated total ice volume with the
surface area of the ocean. Part of this total ice volume, however, does not
contribute to sea level rise because it is below the surface of the ocean
or below the levels of future lakes on land. The present communication
points to this so far overlooked phenomenon and provides a first
order-of-magnitude estimate. It is shown that the effect is small (most
likely about 1 to 6 cm sea level equivalent) but systematic, could
primarily affect earlier stages of global glacier vanishing, and should
therefore be adequately considered. Now-available techniques of
slope-related high-resolution glacier bed modelling have the potential to
provide more detailed assessments in the future.</description><pubDate>Wed, 08 May 2013 00:00:00 +0200</pubDate></item><item><title>Speedup and fracturing of George VI Ice Shelf, Antarctic Peninsula</title><link>http://www.the-cryosphere.net/7/797/2013/</link><description>&lt;b&gt;Speedup and fracturing of George VI Ice Shelf, Antarctic Peninsula&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 797-816, 2013&lt;br /&gt;&lt;br /&gt;Author(s): T. O. Holt, N. F. Glasser, D. J. Quincey, and M. R. Siegfried&lt;br /&gt;&lt;br /&gt;George VI Ice Shelf (GVIIS) is located on the Antarctic Peninsula, a region
where several ice shelves have undergone rapid breakup in response to
atmospheric and oceanic warming. We use a combination of optical (Landsat),
radar (ERS 1/2 SAR) and laser altimetry (GLAS) datasets to examine the
response of GVIIS to environmental change and to offer an assessment on its
future stability. The spatial and structural changes of GVIIS (ca. 1973 to
ca. 2010) are mapped and surface velocities are calculated at different time
periods (InSAR and optical feature tracking from 1989 to 2009) to document
changes in the ice shelf's flow regime. Surface elevation changes are
recorded between 2003 and 2008 using repeat track ICESat acquisitions. We
note an increase in fracture extent and distribution at the south ice front,
ice-shelf acceleration towards both the north and south ice fronts and
spatially varied negative surface elevation change throughout, with greater
variations observed towards the central and southern regions of the ice
shelf. We propose that whilst GVIIS is in no imminent danger of collapse, it
is vulnerable to ongoing atmospheric and oceanic warming and is more
susceptible to breakup along its southern margin in ice preconditioned for
further retreat.</description><pubDate>Mon, 06 May 2013 00:00:00 +0200</pubDate></item><item><title>High-resolution interactive modelling of the mountain glacier–atmosphere interface: an application over the Karakoram</title><link>http://www.the-cryosphere.net/7/779/2013/</link><description>&lt;b&gt;High-resolution interactive modelling of the mountain glacier–atmosphere interface: an application over the Karakoram&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 779-795, 2013&lt;br /&gt;&lt;br /&gt;Author(s): E. Collier, T. Mölg, F. Maussion, D. Scherer, C. Mayer, and A. B. G. Bush&lt;br /&gt;&lt;br /&gt;The traditional approach to simulations of alpine glacier mass balance (MB) has been one-way, or
  offline, thus precluding feedbacks from changing glacier surface conditions on the atmospheric
  forcing. In addition, alpine glaciers have been only simply, if at all, represented in atmospheric
  models to date. Here, we extend a recently presented, novel technique for simulating
  glacier–atmosphere interactions without the need for statistical downscaling, through the use of
  a coupled high-resolution mesoscale atmospheric and physically-based climatic mass balance (CMB) modelling
  system that includes glacier CMB feedbacks to the atmosphere. We compare the
  model results over the Karakoram region of the northwestern Himalaya with remote sensing data for the
  ablation season of 2004 as well as with in situ glaciological and meteorological measurements from the
  Baltoro glacier. We find that interactive coupling has a localized but appreciable impact on the near-surface
  meteorological forcing data and that incorporation of CMB processes improves the simulation of
  variables such as land surface temperature and snow albedo. Furthermore, including feedbacks from
  the glacier model has a non-negligible effect on simulated CMB, reducing modelled ablation, on
  average, by 0.1 m w.e. (−6.0%) to a total of −1.5 m w.e. between
  25 June–31 August 2004. The interactively coupled model shows promise as a new, multi-scale tool
  for explicitly resolving atmospheric-CMB processes of mountain glaciers at the basin scale.</description><pubDate>Mon, 06 May 2013 00:00:00 +0200</pubDate></item><item><title>Mapping radiation transfer through sea ice using a remotely operated vehicle (ROV)</title><link>http://www.the-cryosphere.net/7/763/2013/</link><description>&lt;b&gt;Mapping radiation transfer through sea ice using a remotely operated vehicle (ROV)&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 763-777, 2013&lt;br /&gt;&lt;br /&gt;Author(s): M. Nicolaus and C. Katlein&lt;br /&gt;&lt;br /&gt;Transmission of sunlight into and through sea ice is of critical importance
for sea-ice associated organisms and photosynthesis because light is their
primary energy source. The amount of visible light transferred through sea
ice contributes to the energy budget of the sea ice and the uppermost ocean.
However, our current knowledge on the amount and distribution of light under
sea ice is still restricted to a few local observations, and our understanding
of light-driven processes and interdisciplinary interactions is still
sparse. The main reasons are that the under-ice environment is difficult to access
and that measurements require large logistical and instrumental efforts.
Hence, it has not been possible to map light conditions under sea ice over larger
areas and to quantify spatial variability on different scales. Here we
present a detailed methodological description for operating spectral
radiometers on a remotely operated vehicle (ROV) under sea ice. Recent
advances in ROV and radiation-sensor technology have allowed us to map under-ice
spectral radiance and irradiance on floe scales within a few hours of station
time. The ROV was operated directly from the sea ice, allowing for direct
relations of optical properties to other sea-ice and surface features. The
ROV was flown close to the sea ice in order to capture small-scale
variability. Results from the presented data set and similar future studies
will allow for better quantification of light conditions under sea ice. The
presented experiences will support further developments in order to gather
large data sets of under-ice radiation for different ice conditions and
during different seasons.</description><pubDate>Thu, 02 May 2013 00:00:00 +0200</pubDate></item><item><title>Intercomparison of retrieval algorithms for the specific surface area of snow from near-infrared  satellite data in mountainous terrain, and comparison with the output of a semi-distributed snowpack model</title><link>http://www.the-cryosphere.net/7/741/2013/</link><description>&lt;b&gt;Intercomparison of retrieval algorithms for the specific surface area of snow from near-infrared  satellite data in mountainous terrain, and comparison with the output of a semi-distributed snowpack model&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 741-761, 2013&lt;br /&gt;&lt;br /&gt;Author(s): A. Mary, M. Dumont, J.-P. Dedieu, Y. Durand, P. Sirguey, H. Milhem, O. Mestre, H. S. Negi, A. A. Kokhanovsky, M. Lafaysse, and S. Morin&lt;br /&gt;&lt;br /&gt;This study compares different methods to retrieve the specific surface area
(SSA) of snow from satellite radiance measurements in mountainous terrain.
It aims at addressing the effect on the retrieval of topographic corrections
of reflectance, namely slope and aspect of terrain, multiple reflections on
neighbouring slopes and accounting (or not) for the anisotropy of snow
reflectance. Using MODerate resolution Imaging Spectrometer (MODIS) data
for six different clear sky scenes spanning a wide range of snow conditions
during the winter season 2008–2009 over a domain of 46 × 50 km in
the French Alps,  we compared SSA retrievals with and without topographic
correction, with a spherical or non-spherical snow reflectance model and, in
spherical case, with or without anisotropy corrections. The retrieved SSA
values were compared to field measurements and to the results of the
detailed snowpack model Crocus, fed by driving data from the SAFRAN
meteorological analysis. It was found that the difference in terms of
surface SSA between retrieved values and SAFRAN-Crocus output was minimal
when the topographic correction was taken into account, when using a
retrieval method assuming disconnected spherical snow grains. In this case,
the root mean square deviation was 9.4 m&lt;sup&gt;2&lt;/sup&gt; kg&lt;sup&gt;−1&lt;/sup&gt; and the mean
difference was 0.1 m&lt;sup&gt;2&lt;/sup&gt; kg&lt;sup&gt;−1&lt;/sup&gt;, based on 3170 pairs of observation
and simulated values. The added-value of the anisotropy correction was
not significant in our case, which may be explained by the presence of
mixed pixels and surface roughness. MODIS retrieved data show SSA variations
with elevation and aspect which are physically consistent and in good
agreement with SAFRAN-Crocus outputs. The variability of the MODIS
retrieved SSA within the topographic classes of the model was found to be
relatively small (3.9 m&lt;sup&gt;2&lt;/sup&gt; kg&lt;sup&gt;−1&lt;/sup&gt;). This indicates that
semi-distributed snowpack simulations in mountainous terrain with a
sufficiently large number of classes provides a representation of the
snowpack variability consistent with the scale of MODIS 500 m pixels.</description><pubDate>Mon, 29 Apr 2013 00:00:00 +0200</pubDate></item><item><title>Transient thermal modeling of permafrost conditions in Southern Norway</title><link>http://www.the-cryosphere.net/7/719/2013/</link><description>&lt;b&gt;Transient thermal modeling of permafrost conditions in Southern Norway&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 719-739, 2013&lt;br /&gt;&lt;br /&gt;Author(s): S. Westermann, T. V. Schuler, K. Gisnås, and B. Etzelmüller&lt;br /&gt;&lt;br /&gt;Thermal modeling is a powerful tool to infer the temperature regime of the
ground in permafrost areas. We present a transient permafrost model, CryoGrid
2, that calculates ground temperatures according to conductive heat transfer
in the soil and in the snowpack. CryoGrid 2 is forced by operational air
temperature and snow-depth products for potential permafrost areas in
Southern Norway for the period 1958 to 2009 at 1 km&lt;sup&gt;2&lt;/sup&gt; spatial
resolution. In total, an area of about 80 000 km&lt;sup&gt;2&lt;/sup&gt; is covered. The
model results are validated against borehole temperatures, permafrost
probability maps from &quot;bottom temperature of snow&quot; measurements and
inventories of landforms indicative of permafrost occurrence. The validation
demonstrates that CryoGrid 2 can reproduce the observed lower permafrost
limit to within 100 m at all validation sites, while the agreement between
simulated and measured borehole temperatures is within 1 K for most sites.
The number of grid cells with simulated permafrost does not change
significantly between the 1960s and 1990s. In the 2000s, a significant
reduction of about 40% of the area with average 2 m ground temperatures
below 0 °C is found, which mostly corresponds to degrading permafrost
with still negative temperatures in deeper ground layers. The thermal
conductivity of the snow is the largest source of uncertainty in CryoGrid 2,
strongly affecting the simulated permafrost area. Finally, the prospects of
employing CryoGrid 2 as an operational soil-temperature product for Norway
are discussed.</description><pubDate>Thu, 25 Apr 2013 00:00:00 +0200</pubDate></item><item><title>Ikaite crystal distribution in winter sea ice and implications for CO&lt;sub&gt;2&lt;/sub&gt; system dynamics</title><link>http://www.the-cryosphere.net/7/707/2013/</link><description>&lt;b&gt;Ikaite crystal distribution in winter sea ice and implications for CO&lt;sub&gt;2&lt;/sub&gt; system dynamics&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 707-718, 2013&lt;br /&gt;&lt;br /&gt;Author(s): S. Rysgaard, D. H. Søgaard, M. Cooper, M. Pu&amp;cacute;ko, K. Lennert, T. N. Papakyriakou, F. Wang, N. X. Geilfus, R. N. Glud, J. Ehn, D. F. McGinnis, K. Attard, J. Sievers, J. W. Deming, and D. Barber&lt;br /&gt;&lt;br /&gt;The precipitation of ikaite (CaCO&lt;sub&gt;3&lt;/sub&gt; &amp;sdot; 6H&lt;sub&gt;2&lt;/sub&gt;O) in polar sea ice
is critical to the efficiency of the sea ice-driven carbon pump and
potentially important to the global carbon cycle, yet the spatial and
temporal occurrence of ikaite within the ice is poorly known. We report
unique observations of ikaite in unmelted ice and vertical profiles of
ikaite abundance and concentration in sea ice for the crucial season of
winter. Ice was examined from two locations: a 1 m thick land-fast ice site
and a 0.3 m thick polynya site, both in the Young Sound area (74&amp;deg; N,
 20&amp;deg; W) of NE Greenland. Ikaite crystals, ranging in size from a
few μm to 700 μm, were observed to concentrate in the
interstices between the ice platelets in both granular and columnar sea ice.
In vertical sea ice profiles from both locations, ikaite concentration
determined from image analysis, decreased with depth from surface-ice values
of 700–900 μmol kg&lt;sup&gt;−1&lt;/sup&gt; ice (~25 × 10&lt;sup&gt;6&lt;/sup&gt; crystals kg&lt;sup&gt;&amp;minus;1&lt;/sup&gt;)
 to values of 100–200 μmol kg&lt;sup&gt;−1&lt;/sup&gt; ice (1–7 × 10&lt;sup&gt;6&lt;/sup&gt; crystals kg&lt;sup&gt;&amp;minus;1&lt;/sup&gt;)
 near the sea ice–water interface, all of which are much
higher (4–10 times) than those reported in the few previous studies. Direct
measurements of total alkalinity (TA) in surface layers fell within the same
range as ikaite concentration, whereas TA concentrations in the lower half of
the sea ice were twice as high. This depth-related discrepancy suggests
interior ice processes where ikaite crystals form in surface sea ice
layers and partly dissolve in layers below. Melting of sea ice and
dissolution of observed concentrations of ikaite would result in meltwater
with a &lt;i&gt;p&lt;/i&gt;CO&lt;sub&gt;2&lt;/sub&gt; of &lt;15 μatm. This value is far below
atmospheric values of 390 μatm and surface water concentrations of
315 μatm. Hence, the meltwater increases the potential for seawater
uptake of CO&lt;sub&gt;2&lt;/sub&gt;.</description><pubDate>Tue, 23 Apr 2013 00:00:00 +0200</pubDate></item><item><title>New estimates of Arctic and Antarctic sea ice extent during September 1964 from recovered Nimbus I satellite imagery</title><link>http://www.the-cryosphere.net/7/699/2013/</link><description>&lt;b&gt;New estimates of Arctic and Antarctic sea ice extent during September 1964 from recovered Nimbus I satellite imagery&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 699-705, 2013&lt;br /&gt;&lt;br /&gt;Author(s): W. N. Meier, D. Gallaher, and G. G. Campbell&lt;br /&gt;&lt;br /&gt;Visible satellite imagery from the 1964 Nimbus I satellite has been
recovered, digitized, and processed to estimate Arctic and Antarctic sea ice
extent for September 1964. September is the month when the Arctic sea ice
reaches its minimum annual extent and the Antarctic sea ice reaches its
maximum. Images from a three-week period were manually analyzed to estimate
the location of the ice edge and then composited to obtain a hemispheric
estimate. Uncertainties were based on limitations in the image analysis and
the variation of the ice cover over the three-week period. The 1964
Antarctic extent is higher than estimates from the 1979–present passive
microwave record, but is in accord with previous indications of higher
extents during the 1960s. The Arctic 1964 extent is near the 1979–2000
average from the passive microwave record, suggesting relatively stable
summer extents during the 1960s and 1970s preceding the downward trend since
1979 and particularly the large decrease in the last decade. These early
satellite data put the recently observed record into a longer-term context.</description><pubDate>Tue, 23 Apr 2013 00:00:00 +0200</pubDate></item><item><title>Influence of ablation-related processes in the build-up of simulated Northern Hemisphere ice sheets during the last glacial cycle</title><link>http://www.the-cryosphere.net/7/681/2013/</link><description>&lt;b&gt;Influence of ablation-related processes in the build-up of simulated Northern Hemisphere ice sheets during the last glacial cycle&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 681-698, 2013&lt;br /&gt;&lt;br /&gt;Author(s): S. Charbit, C. Dumas, M. Kageyama, D. M. Roche, and C. Ritz&lt;br /&gt;&lt;br /&gt;Since the original formulation of the positive-degree-day (PDD) method,
different PDD calibrations have been proposed in the literature in response
to the increasing number of observations. Although these formulations
generally provide a satisfactory description of the present-day Greenland
geometry, they have not all been tested for paleo ice sheets. Using the
climate-ice sheet model CLIMBER-GRISLI coupled with different PDD models, we
evaluate how the parameterisation of the ablation may affect the evolution
of Northern Hemisphere ice sheets in the transient simulations of the last
glacial cycle. Results from fully coupled simulations are compared to
time-slice experiments carried out at different key periods of the last
glacial period. We find large differences in the simulated ice sheets
according to the chosen PDD model. These differences occur as soon as the
onset of glaciation, therefore affecting the subsequent evolution of the ice
system. To further investigate how the PDD method controls this evolution,
special attention is given to the role of each PDD parameter. We show that
glacial inception is critically dependent on the representation of the
impact of the temperature variability from the daily to the inter-annual
time scale, whose effect is modulated by the refreezing scheme. Finally, an
additional set of sensitivity experiments has been carried out to assess the
relative importance of melt processes with respect to initial ice sheet
configuration in the construction and the evolution of past Northern
Hemisphere ice sheets. Our analysis reveals that the impacts of the initial
ice sheet condition may range from quite negligible to explaining about half
of the LGM ice volume depending on the representation of stochastic
temperature variations which remain the main driver of the evolution of the
ice system. The main findings of this paper underline the need for
conducting studies with high resolution climate models coupled to detailed
snow models to better constrain the temporal and spatial variations of the
PDD parameters. The development of such approaches could improve the
calibration of the PDD formulation which is still widely used in climate-ice
sheet studies.</description><pubDate>Thu, 18 Apr 2013 00:00:00 +0200</pubDate></item><item><title>An approach to derive regional snow lines and glacier mass change from MODIS imagery, western North America</title><link>http://www.the-cryosphere.net/7/667/2013/</link><description>&lt;b&gt;An approach to derive regional snow lines and glacier mass change from MODIS imagery, western North America&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 667-680, 2013&lt;br /&gt;&lt;br /&gt;Author(s): J. M. Shea, B. Menounos, R. D. Moore, and C. Tennant&lt;br /&gt;&lt;br /&gt;We describe a method to calculate regional snow line elevations and annual
equilibrium line altitudes (ELAs) from daily MODIS imagery (MOD02QKM) on
large glaciers and icefields in western North America. An automated cluster
analysis of the cloud-masked visible and near-infrared bands at 250 m
resolution is used to delineate glacier facies (snow and ice) for ten
glacierized regions between 2000–2011. For each region and season, the
maximum observed value of the 20th percentile of snow-covered pixels
(&lt;i&gt;Z&lt;/i&gt;&lt;sub&gt;&lt;i&gt;S&lt;/i&gt;(20)&lt;/sub&gt;) is used to define a regional ELA proxy (ELA&lt;sub&gt;est&lt;/sub&gt;). Our
results indicate significant increases in the regional ELA proxy at two
continental sites (Peyto Glacier and Gulkana Glacier) over the period of
observation, though no statistically significant trends are identified at
other sites. To evaluate the utility of regional ELA proxies derived from
MOD02QKM imagery, we compare standard geodetic estimates of glacier mass
change with estimates derived from historical mass balance gradients and
observations of &lt;i&gt;Z&lt;/i&gt;&lt;sub&gt;&lt;i&gt;S&lt;/i&gt;(20)&lt;/sub&gt; at three large icefields. Our approach yields
estimates of mass change that more negative than traditional geodetic
approaches, though MODIS-derived estimates are within the margins of error at
all three sites. Both estimates of glacier mass change corroborate the
continued mass loss of glaciers in western North America. Between 2000 and
2009, the geodetic change approach yields mean annual rates of surface
elevation change for the Columbia, Lillooet, and Sittakanay icefields of
−0.29 ± 0.05, −0.26 ± 0.05, and
−0.63 ± 0.17 m a&lt;sup&gt;−1&lt;/sup&gt;, respectively. This study provides a new
technique for glacier facies detection at daily timescales, and contributes
to the development of regional estimates of glacier mass change, both of
which are critical for studies of glacier contributions to streamflow and global sea level rise.</description><pubDate>Thu, 18 Apr 2013 00:00:00 +0200</pubDate></item><item><title>Theoretical study of solar light reflectance from vertical snow surfaces</title><link>http://www.the-cryosphere.net/7/657/2013/</link><description>&lt;b&gt;Theoretical study of solar light reflectance from vertical snow surfaces&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;The Cryosphere, 7, 657-666, 2013&lt;br /&gt;&lt;br /&gt;Author(s): O. V. Nikolaeva and A. A. Kokhanovsky&lt;br /&gt;&lt;br /&gt;The influence of horizontal and vertical inhomogeneity of snow surfaces on
solar light reflectance is studied using the radiative transfer theory (RTT).
We compared 1-D RTT and 2-D RTT and found that large errors are produced if
the 1-D RTT is used for the calculation of the snow reflection function (and,
therefore, also in the retrievals of the snow grain radii) in 2-D measurement
geometries. Such 2-D geometries are common in the procedures for the
determination of the effective snow grain radii using near-infrared
photography and spectroscopy of vertical snow walls. In particular, we have
considered three cases for the numerical calculations: (1) the case with no
black film; (2) the case with a black film at the pit's bottom; (3) the case
with a black film at the pit's bottom and also at one of the vertical snow
walls.</description><pubDate>Fri, 05 Apr 2013 00:00:00 +0200</pubDate></item></channel></rss>