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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" dtd-version="3.0"><?xmltex \makeatother\@nolinetrue\makeatletter?>
  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">CP</journal-id>
<journal-title-group>
<journal-title>Climate of the Past</journal-title>
<abbrev-journal-title abbrev-type="publisher">CP</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Clim. Past</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1814-9332</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/cp-11-1467-2015</article-id><title-group><article-title>How might the North American ice sheet influence
the northwestern Eurasian climate?</article-title>
      </title-group><?xmltex \runningtitle{North American ice sheet influence on the Eurasian climate}?><?xmltex \runningauthor{P.~Beghin et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Beghin</surname><given-names>P.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Charbit</surname><given-names>S.</given-names></name>
          <email>sylvie.charbit@lsce.ipsl.fr</email>
        <ext-link>https://orcid.org/0000-0003-1560-6462</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Dumas</surname><given-names>C.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Kageyama</surname><given-names>M.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Ritz</surname><given-names>C.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Laboratoire des Sciences du Climat et de l'Environnement, CEA-CNRS-UVSQ, UMR 8212, Gif-sur-Yvette, France</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Laboratoire de Glaciologie et de Géophysique de l'Environnement, CNRS-UJF, UMR 5183, Saint Martin d'Hères, France</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">S. Charbit (sylvie.charbit@lsce.ipsl.fr)</corresp></author-notes><pub-date><day>26</day><month>October</month><year>2015</year></pub-date>
      
      <volume>11</volume>
      <issue>10</issue>
      <fpage>1467</fpage><lpage>1490</lpage>
      <history>
        <date date-type="received"><day>8</day><month>December</month><year>2014</year></date>
           <date date-type="rev-request"><day>7</day><month>January</month><year>2015</year></date>
           <date date-type="rev-recd"><day>7</day><month>October</month><year>2015</year></date>
           <date date-type="accepted"><day>12</day><month>October</month><year>2015</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015.html">This article is available from https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015.html</self-uri>
<self-uri xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015.pdf">The full text article is available as a PDF file from https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015.pdf</self-uri>


      <abstract>
    <p>It is now widely acknowledged that past Northern Hemisphere ice sheets
covering Canada and northern Europe at the Last Glacial Maximum (LGM) exerted
a strong influence on climate by causing changes in atmospheric and oceanic
circulations. In turn, these changes may have impacted the development of the
ice sheets themselves through a combination of different feedback mechanisms.
The present study is designed to investigate the potential impact of the
North American ice sheet on the surface mass balance (SMB) of the Eurasian
ice sheet driven by simulated changes in the past glacial atmospheric
circulation. Using the LMDZ5 atmospheric circulation model, we carried out 12 experiments under constant LGM conditions for insolation, greenhouse
gases and ocean. In these experiments, the Eurasian ice sheet is removed. The 12 experiments differ in the North American ice-sheet topography, ranging
from a white and flat (present-day topography) ice sheet to a full-size LGM
ice sheet. This experimental design allows the albedo and the topographic
impacts of the North American ice sheet onto the climate to be disentangled.
The results are compared to our baseline experiment where both the North
American and the Eurasian ice sheets have been removed. In summer, the sole
albedo effect of the American ice sheet modifies the pattern of planetary
waves with respect to the no-ice-sheet case, resulting in a cooling of the
northwestern Eurasian region. By contrast, the atmospheric circulation
changes induced by the topography of the North American ice sheet lead to a
strong decrease of this cooling. In winter, the Scandinavian and the
Barents–Kara regions respond differently to the American ice-sheet albedo
effect: in response to atmospheric circulation changes, Scandinavia becomes warmer and
total precipitation is more abundant, whereas the Barents–Kara area becomes cooler
with a decrease of convective processes, causing a decrease of total precipitation.
The gradual increase of the altitude of the American ice sheet leads to less
total precipitation and snowfall and to colder temperatures over both the
Scandinavian and the Barents and Kara sea sectors. We then compute the resulting
annual surface mass balance over the Fennoscandian region from the simulated
temperature and precipitation fields used to force an ice-sheet model. It
clearly appears that the SMB is dominated by the ablation signal. In response
to the summer cooling induced by the American ice-sheet albedo, high positive
SMB values are obtained over the Eurasian region, leading thus to the growth
of an ice sheet. On the contrary, the gradual increase of the American ice-sheet altitude induces more ablation over the Eurasian sector, hence limiting
the growth of Fennoscandia. To test the robustness of our results with respect to the
Eurasian ice sheet state, we carried out two additional LMDZ experiments with
new boundary conditions involving both the American (flat or full LGM) and high Eurasian ice sheets. The most striking result is that the Eurasian ice
sheet is maintained under full-LGM North American ice-sheet conditions, but
loses <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10 % of its mass compared to the case in which the North
American ice sheet is flat. These new findings qualitatively confirm the
conclusions from our first series of experiments and suggest that the
development of the Eurasian ice sheet may have been slowed down by the growth
of the American ice sheet, offering thereby a new understanding of the
evolution of Northern Hemisphere ice sheets throughout glacial–interglacial
cycles.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The last million years is characterized by alternating glacial and
interglacial phases. During glacial periods, large ice sheets covering
present-day Canada and northwestern Eurasia (Dyke and Prest, 1987; Clark et
al., 1993; Peltier, 2004; Svendsen et al., 2004; Lambeck et al., 2006;
Tarasov et al., 2012) exerted a strong influence on climate. Several studies
highlighted the importance the climatic changes induced by continental-scale
ice sheets (e.g. Clark, 1999). It has been recognized that the ice-sheet
topography is likely to be the main factor altering the atmospheric
circulation in the Northern Hemisphere (Broccoli and Manabe, 1987; Pausata et
al., 2011). As an example, the pioneering study carried out by Manabe and
Broccoli (1985) with an atmospheric general circulation model shows that the
North American ice sheet caused a split of the westerlies. The authors also
highlight a larger amplitude of the planetary waves due to the presence of
ice sheets. Recently, Ullman et al. (2014) tested the influence of different
North American ice-sheet reconstructions on the climate. They showed that a
higher American ice sheet leads to a more zonal Atlantic jet, thereby
confirming the key role of ice-sheet topography on atmospheric circulation.
Using model outputs from the Paleo Modelling Intercomparison Project 2
(PMIP2) (Braconnot et al., 2007), Laîné et al. (2009) and
Rivière et al. (2010) highlight a strengthening and an equatorward
displacement of the sub-tropical jet-stream during the Last Glacial Maximum
(LGM) with respect to the pre-industrial period. Changes in the position and the
strength of the North Atlantic jet stream induce changes in the storm tracks,
and therefore in precipitation (Hall et al., 1996; Kageyama and Valdes,
2000; Laîné et al., 2009; Rivière et al., 2010). These changes
also have an influence on the energy transport and can therefore modify the
temperature.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p>Ice-sheet and oceanic boundary conditions used for the LMDZ
experiments. <bold>(a)</bold> Ice-sheet height (light blue scale) and land height
(brown scale) given as boundary conditions for the 5 selected experiments
out of 12. Dark blue–brown limits represent the sea-land mask, and
brown–light blue limits represent the land-ice mask. <bold>(b)</bold> Averaged
annual sea-surface temperature (shading) and sea-ice extent for boreal summer
(red contours) and winter (blue contours) from the PMIP3 IPSL-CM5A-LR
simulations. The averages are computed over 50 years which have been used to
create the boundary conditions for the LMDZ experiments.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f01.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Laurentide ice-sheet height for each LMDZ experiment (with name of
the corresponding experiment). The height of the LIS is defined as a relative
difference between PMIP3 Laurentide ice-sheet height and the present-day
topography (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msubsup><mml:mi>h</mml:mi><mml:mi mathvariant="normal">LIS</mml:mi><mml:mrow><mml:mi mathvariant="normal">PMIP</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f02.pdf"/>

      </fig>

      <p>The climatic changes induced by large-scale ice sheets exert an influence on
both temperature and precipitation that drive the ice-sheet surface mass
balance (SMB), defined as the sum of snow accumulation and snow and ice
ablation. Using a simple ice-sheet model based on an idealized geometry
coupled to a stationary-wave model, Roe and Lindzen (2001a, b) underline the
importance of accounting for the feedbacks between ice sheets and
temperatures induced by changes in stationary waves to properly simulate the
evolution of an ice sheet. They show that the self-induced temperature
anomaly due to an ice sheet leads to a warming over the ice-sheet western
part. This may explain the absence of ice over Alaska at the LGM. They also
suggest that the stationary waves excited by the North American ice sheet may
have contributed to a warming over Europe, influencing the development of the
Eurasian ice sheet. In the same way, with a three-dimensional stationary wave
model, Liakka et al. (2011) showed that the position of the southern margin
of ice sheets strongly depends on the temperature anomalies due to stationary
waves, which are modified by the ice sheet itself. More recently, with the
use of the CAM3 atmospheric model run under four different climatic contexts
(last interglacial, marine isotope stages 5b and 4 (MIS5b and MIS4), and LGM
periods), Löfverström et al. (2014) showed how the atmospheric
circulation changes induced by the ice sheets could have influenced the
growth of the ice sheets themselves. Similarly to Roe and Lindzen (2001a),
they show that the summer atmospheric circulation change due to the presence
of ice sheets may cause a sufficient warming over Siberia and Alaska to
inhibit ice growth. They also perform two experiments under MIS4 conditions
to test the influence of one ice sheet on the other. They conclude that the
summer temperature anomaly induced by the presence of the MIS4 American ice
sheet is too weak to explain the small size of the European ice sheet at that
period, but may have contributed to the westward shift of the ice-sheet mass
center. Although several studies have been devoted to the mutual influences
of the ice sheets (Roe and Lindzen, 2001a; Beghin et al., 2014;
Löfverström et al., 2014), no study has specifically investigated the
mechanisms through which the American ice sheet may have influenced the
European climate, and therefore the European ice-sheet surface mass balance.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p>2 m summer (left) and winter (right) temperature without the LIS
(noIS) and anomaly of the 2 m temperature between the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL experiments and
the noIS experiment; we can therefore quantify the impact of the LIS
presence, depending on its topography. The visible surface albedo difference
between <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL and noIS experiments are represented by orange contours
(albedo difference <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.4) and yellow contours (albedo
difference <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.2). The statistical significance of the patterns of
temperature anomalies has been checked using a two-sided Student <inline-formula><mml:math display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test
with a <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> value <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.05. The white shading indicates areas where the
anomaly is not significant.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f03.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>500 hPa summer geopotential height anomaly from zonal mean (left
panels) and 500 hPa horizontal wind (arrows) and meridional wind (shaded,
right panels).</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f04.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p>Same as Fig. 4 for the winter season.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f05.png"/>

      </fig>

      <p>The aim of this paper is to investigate the atmospheric response to changes
in the North American ice-sheet boundary conditions and to examine how the
related atmospheric circulation changes impact the climate over the
Scandinavian and Barents–Kara sea regions. To achieve this goal, we use the
LMDZ5 atmospheric general circulation model run with different thicknesses of
the North American ice sheet taken as boundary conditions, with no ice at all
over Eurasia. We investigate the mechanisms by which the American ice sheet
may change the surface mass balance of the Eurasian ice sheet. Besides
gradually increasing the altitude of the North American ice sheet, the
originality of the present study also relies on ice-sheet model simulations.
We use climatic fields simulated by the LMDZ5 model as inputs to a
three-dimensional ice-sheet model to compute the surface mass balance of the
Eurasian ice sheet. The description of the climate and ice-sheet models is
given in Sect. 2 as well as the experimental design. The model results,
presented in Sects. 3 and 4, are followed by a discussion (Sect. 5). Section 6
summarizes the main findings of our study.</p>
</sec>
<sec id="Ch1.S2">
  <title>Model and experiment</title>
<sec id="Ch1.S2.SS1">
  <title>The atmospheric model</title>
      <p>The LMDZ5 atmospheric model used in this study belongs to the LMDZ model family
developed at Laboratoire de Météorologie Dynamique (Sadourny and
Laval, 1984; Le Treut et al., 1994, 1998, Hourdin et al., 2006). LMDZ is the
atmospheric component of the IPSL-CM5A coupled ocean–atmosphere model
(Dufresne et al., 2013). The dynamical equations are discretized on a
longitude-latitude-staggered Arakawa C-grid (Kasahara, 1977). The model
ensures the conservation of both enstrophy (square of wind rotational) for
baroclinic flows (Sadourny, 1975a, b) and the axisymmetric component of the
angular momentum. The model version used in this study has 39 vertical levels
and runs on a 96 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 95 model grid resolution
(3.75<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>1.9<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). A complete description of the model
can be found in (Hourdin et al., 2013).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p>Same as Fig. 3 for annual precipitation (left column) and annual
snowfall (right column).</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p>Large-scale (left panels) and convective (right panels) annual
precipitation without LIS (noIS experiment, top panels), and anomalies of
large-scale and convective precipitation between the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL and
noIS experiments. The statistical significance of the patterns of temperature
anomalies has been checked using a two-sided Student-<inline-formula><mml:math display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test with a
<inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> value <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.05. The white shading indicates areas where the anomaly is
not significant.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f07.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p><bold>(a)</bold> Scandinavian and <bold>(b)</bold> Barents–Kara
precipitation anomalies (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL-noIS) during winter (circles) and summer
(triangles) vs. annual precipitation anomaly. The lower the Laurentide ice-sheet altitude, the lighter grey the symbols are.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f08.pdf"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS2">
  <title>The ice-sheet model</title>
      <p>The GRISLI ice-sheet model is a three-dimensional thermomechanical model
which simulates the evolution of ice-sheet geometry (extension and thickness)
and the coupled temperature–velocity fields in response to climate forcing. A
comprehensive description of the model can be found in (Ritz et al., 2001)
and (Peyaud et al., 2007). Here, we only summarize the main characteristics
of this model. The equations are solved on a cartesian grid
(40 km <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 40 km). Over the grounded part of the ice sheet, the ice
flow resulting from internal deformation is governed by the shallow-ice
approximation (Hutter, 1983; Morland et al., 1984). The model deals with ice
flow through ice shelves using the shallow-shelf approximation (MacAyeal, 1989). It also predicts the large-scale characteristics of the ice streams
using criteria based on the effective pressure and hydraulic load. At each
time step, the velocity and vertical profiles of temperature in the ice are
computed as well as the new geometry of the ice sheet. The isostatic
adjustment of bedrock in response to ice load is governed by the flow of the
asthenosphere, with a characteristic time constant of 3000 years, and by the
rigidity of the lithosphere. The temperature field is computed both in the
ice and in the bedrock by solving a time-dependent heat equation. The surface
mass balance is defined as the sum between accumulation and ablation computed
by the empirical positive degree-day (PDD) method (Reeh, 1991; Fausto et al.,
2009). This method assumes that melt rates of snow and ice are linearly
related to the number of PDD through degree-day factors for snow and ice
materials (Braithwaite, 1984, 1995).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p>(shaded) and position of the North Atlantic jet stream without LIS
(dashed) and for the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL experiment (solid line). Right column: summer
precipitation (shaded) and snowfall (contour every 0.1 mm day<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, blue
contour for positive values).</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f09.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><caption><p>850 hPa winter jet-stream shift (in latitude) vs. winter
precipitation anomaly over the Scandinavian region. The range of results has
been obtained by bootstrapping. Up and down triangles represent the 5th
precipitation percentile vs. the 95th jet position percentile, and the
95th precipitation percentile vs. the 5th jet position percentile
respectively. Circles are the average values and crosses indicate the 5th and
95th percentiles.</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f10.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><caption><p>Meridional cross sections of the 500hPa geopotential height anomaly
from zonal means over the East Laurentide (90–60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W, top panel) and
the Atlantic sectors (50–10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W, middle) in meters, and of the
500 hPa zonal wind (in m s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) for the Atlantic sector.</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f11.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><caption><p><bold>(a)</bold> Snow accumulation computed by the GRISLI ice-sheet
model for the noIS experiment (top panel), and differences of snow
accumulation between the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL and the noIS experiments (in m yr<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).
<bold>(b)</bold> same as <bold>(a)</bold> for the ablation (in m yr<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f12.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><caption><p><bold>(a)</bold> Surface mass balance at the beginning of the simulation
(in m yr<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and <bold>(b)</bold> surface elevation at the end of the
simulation computed by the ice-sheet model for the selected experiments (in
meters).</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f13.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><caption><p>Summer 2 m temperatures for the <bold>(a)</bold> 00dhL (flat LIS, no
FIS) experiment, <bold>(b)</bold> 00dhLFIS (flat LIS, high FIS),
<bold>(c)</bold> 100dhL (high LIS, no FIS) and <bold>(d)</bold> 100dhLFIS (high LIS,
high FIS). The extents of the ice sheets (blue contours) are superimposed on
right panels for 00100 and 100dhLFIS runs.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f14.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F15" specific-use="star"><caption><p>Same as Fig. 14 for the vertically integrated meridional (shaded)
and the horizontal heat transport (arrows) in summer. Numerical values are
given in 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>10</mml:mn></mml:msup></mml:math></inline-formula> J m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f15.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F16" specific-use="star"><caption><p>Same as Fig. 14 for the 850 hPa meridional wind (shaded) and the
850hPa horizontal winds (arrows) for the summer season (in m s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f16.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS3">
  <title>Experimental set-up</title>
      <p>In order to investigate the albedo and topography effects induced by the
North American ice sheet on the Eurasian climate at the LGM, we carried out
12 simulations under LGM conditions for greenhouse gases (GHGs), insolation,
sea-surface temperatures and sea-ice. In this series of simulations, the
altitude of the North American ice-sheet surface ranges from that of the
present-day surface to 100 % of that used in the PMIP3 LGM experiments.
The PMIP3 LGM ice sheets result from a combination of three reconstructions,
namely ICE-6G v2.0 (Toscano et al., 2011), GLAC-1 (Tarasov et al., 2012) and
ANU (Lambeck, 2001). The way this new reconstruction has been obtained is
explained in detail on the PMIP3 website
(<uri>https://wiki.lsce.ipsl.fr/pmip3/doku.php/pmip3:design:pi:final:icesheet</uri>)
and in Abe-Ouchi et al. (2015). In our baseline experiment (noIS), the
land-ice mask is modified (with respect to PMIP3) to remove both the European and the
American ice sheets and the altitude is that of the present day (Fig. 1). In
the other simulations, we only remove the European ice-sheet mask. These
simulations are referred to as <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL, where dhL represents the surface height
difference between the PMIP3 LGM Laurentide ice sheet and the present-day
surface, and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula> represents the percentage of dhL taken into account. To
simplify the writing, the American and Eurasian ice sheets are respectively
referred to as “Laurentide ice sheet” (LIS) and the “Fennoscandian ice
sheet” (FIS) in the following.</p>
      <p>The topography of the 00dhL experiment is therefore the same as today, but
the land-ice mask is set to the LGM one (Figs. 1 and 2). Greenland and
Antarctic ice sheets are the same as in the PMIP3 experimental set-up. Both
insolation and GHG boundary conditions are similar to those defined in the
PMIP3 protocol: the orbital forcing is taken at 21 kyr BP from (Berger,
1978), while atmospheric GHG concentrations are those recorded in Antarctic
ice cores (CO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 185 ppm, (Lüthi et al., 2008); CH<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 350 ppb, (Loulergue et al., 2008); N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 200 ppb, (Spahni et
al., 2005)). The LGM land–sea mask is also taken into account, with closed
Bering Strait, and land in Hudson Bay and Barents Sea (Fig. 1). The
sea-surface temperatures (SSTs) and sea-ice cover come from 50 consecutive
years of the IPSL PMIP3 LGM run outputs (Kageyama et al., 2013). These
oceanic surface conditions are depicted in Fig. 1. In the North Atlantic
area, the temperature meridional gradient is steep in the western part of the
basin and weakens in its eastern part, as for the pre-industrial period. The
sea-ice edge is located south of Iceland in winter and retreats to the
northern limits of the Nordic seas in summer. These rather warm North
Atlantic Ocean/Nordic sea conditions are due to a strong Atlantic meridional
overturning circulation (Kageyama et al., 2013). Using these boundary
conditions, the LMDZ5 simulations are run for 50 years, and we study the last
40 years to be at equilibrium. Two-sided Student <inline-formula><mml:math display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> tests with a <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> value <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.05 (von Storch and Zwiers, 2003) are performed on key diagnostics.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>AGCM results</title>
      <p>In this section, we focus on how the LIS influences the climatic fields
which can have an impact on the surface mass balance of an ice sheet. The
key climatic variables used to compute the amount of ablation with the PDD
method are the monthly temperatures and the monthly total (solid plus
liquid) precipitation.</p><?xmltex \hack{\newpage}?>
<sec id="Ch1.S3.SS1">
  <title>The northwestern Eurasian temperature</title>
<sec id="Ch1.S3.SS1.SSS1">
  <title>Impact of the Laurentide ice sheet </title>
      <p>Using the comparison between the 00dhL and the noIS experiments, we first
consider the impact of the LIS albedo on the 2 m summer air temperature over
the Scandinavia–Barents–Kara (SBK) region (Fig. 3, 00dhL experiment, left
column). The most striking feature is a cooling over the whole Eurasian
continent with a maximum (more than 10 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) centered over the
Barents and Kara seas and a moderate cooling (2 to 4 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) over
Scandinavia. The area experiencing the largest cooling also corresponds to
the area with the largest albedo (orange contours). This is a direct
consequence of the LGM land–sea mask used in this study for which the
Barents and Kara seas are represented as continental areas. This favors snow
accumulation and therefore higher albedo values in this area, causing in turn
a positive feedback on temperatures. Figure 3 also displays the 2 m mean
summer temperature over the SBK region for different altitudes of the LIS.
Here, we only give results of selected experiments to simplify the
presentation of our results. It appears that the SBK cooling gets smaller
when the LIS gets higher. Overall, the simulated summer surface air
temperature evolves together with the LIS altitude, with a progressive
reduction of the zonal and meridional extent of the largest cooling zone.
When the LIS reaches its full LGM size (100dhL-noIS), the summer cooling over
the Barents and Kara seas is reduced to 4–6 and to 2 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C at most over
Scandinavia. The topography of the LIS has therefore a warming effect on the
SBK region for the summer season.</p>
      <p>In winter, the response of the temperature to the LIS albedo and its
evolution with the LIS altitude are different from the summer response
(Fig. 3, right panels). First, the LIS albedo induces warmer temperatures
(<inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) over southern Scandinavia, the British Isles and the present-day
North and Baltic seas, and cooler temperatures over an area in the Barents
Sea expanding from Svalbard to Novaya Zemlya (3 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C). Surprisingly,
in the 30dhL experiment, the amplitude of these temperature changes (with respect to
noIS) is reduced, showing that the response of winter temperatures to changes
in LIS altitude is far from being linear. Beyond 60dhL, the cooling zone
progressively expands, and spreads across the entire British Isles and
Scandinavia–Barents–Kara area when the LIS has its full LGM size. In contrast
to the climatic response simulated for the summer season, the LIS topography
leads to colder surface air temperatures in winter.</p>
      <p>To understand the origin of these contrasted responses, we investigate the
processes through which the changes in the altitude of the Laurentide ice
sheet modify the atmospheric circulation.</p>
</sec>
<sec id="Ch1.S3.SS1.SSS2">
  <title>Atmospheric circulation processes</title>
      <p>The comparison of the zonal anomaly (00dhL vs. noIS) of the 500 hPa summer
geopotential height shows that the sole albedo effect of the LIS is
sufficient to drastically change the atmospheric circulation (Fig. 4, 00dhL
and noIS, left column). The ridge over the Rockies, clearly visible in noIS,
disappears in 00dhL, and the trough over the Labrador sector is more
extensive. Ridges over the North Atlantic, the Greenland ice sheet and
northern Europe are more developed in 00dhL (with respect to noIS). By contrast, the
troughs over Iceland, the Norwegian and Barents seas appearing in noIS are
weaker or even vanish in 00dhL. In noIS, the trough over Svalbard implies
southerlies over the Barents Sea (Fig. 4, right column) and therefore, warm
temperatures in this area (Fig. 3). The weakening of this trough in 00dhL as
well as the stronger ridge over Greenland induces northerlies over Svalbard
and the Barents Sea (Fig. 4) and therefore colder temperatures (Fig. 3).</p>
      <p>The Labrador trough and the North Atlantic ridge become stronger when the LIS
gets higher, until it reaches 60 % of its full size. Beyond 60dhL, the
Labrador trough and the Atlantic ridge keep more or less the same amplitude.
When the LIS gets higher, the Greenland ridge gets weaker, the European ridge
remains almost unchanged (Fig. 4), and there is a return of the
Iceland–Svalbard–Barents trough. This new trough, centered between Greenland
and Svalbard, along with the weakening of the Greenland ridge, brings
southerlies again over the northern Barents Sea. The Barents winds shift from
northerlies to southerlies when the LIS is 60 % of its full size. The
southerlies bring warmer temperatures, explaining the SBK warming with the
increase of the LIS height (Figs. 3 and 4).</p>
      <p>In winter (Fig. 5), the sole albedo effect of the LIS does not drastically
change the geopotential anomaly. However, the meridional wind field shows a
slight decrease of the southerlies over the Barents Sea, explaining the
slight cooling over this region. There is also a slight decrease of the
northerlies simulated over the British Isles, the eastern North Atlantic
Ocean and southern Scandinavia, consistent with the moderate warming
simulated over this region. In the 30dhL experiment, a strengthening of the
southerlies is observed (Fig. 5) inducing a warming (with respect to 00dhL) over the
SBK region (Fig. 3) and explaining the non-linear behavior on winter
temperatures. When the altitude of the LIS further increases, there is a
progressive emergence of a trough over the Scandinavian–Barents sector. This
trough comes with northerlies over the Norwegian Sea and weaker southerlies
over the Barents sea (Fig. 5, right column), consistently with colder
temperatures over this area, as seen in Fig. 3.</p>
      <p>This analysis explains why opposite sign temperature responses are obtained
for the summer and winter seasons. Since ablation is rather sensitive to the
summer season, more ice is expected over the Fennoscandian area when the
sole albedo effect of the LIS is operating (i.e. 00dhL experiment). However,
the development of an ice sheet in this area also depends on the amount of
snow accumulation. Therefore, we next examine hereafter the LIS impact on
the SBK total precipitation and snowfall.</p>
</sec>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Total and solid precipitation over northwestern Eurasia</title>
<sec id="Ch1.S3.SS2.SSS1">
  <title>Impact of the Laurentide ice sheet </title>
      <p>In this section, we investigate the impact of the LIS on the mean annual
precipitation and snowfall over northwestern Eurasia (Fig. 6). In response to
the LIS albedo effect (00dhL-noIS panel) a slight excess of precipitation is
simulated over the northeastern North Atlantic and the southern and western
parts of Scandinavia, but less precipitation is simulated over the
Barents–Kara sea area. However, over the whole SBK region, the snowfall
anomaly is positive. This increase in snowfall is due to the summer signal
(not shown) related to the cooling observed over this region (Fig. 3). This
cooling is strong enough to allow for an increase of the fraction of solid
precipitation and to maintain the snow cover.</p>
      <p>When the LIS reaches its full LGM altitude (100dhL-noIS), the positive
anomaly of total precipitation over Scandinavia simulated in the 00dhL
experiment shifts southward, reaching even the French and the Iberian
Peninsula Atlantic coasts. This results in dry conditions over the western
flank of the Scandinavian region, both in terms of total and solid
precipitation. Concomitantly, the negative anomaly of total precipitation
over the Barents–Kara sea region simulated in 00dhL expands westward leading
to a drier climate and to a decrease of snowfall over Scandinavia. These
results suggest that the Barents and Kara seas and the Scandinavian regions are
sensitive to different characteristics of the LIS; while the precipitation
over Scandinavia appears to be sensitive to the LIS height, the
precipitation anomaly over the Barents and Kara seas mainly appears to result
from the LIS albedo effect and is rather insensitive to height.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <title>Large-scale vs. convective precipitation</title>
      <p>To disentangle the mechanisms responsible for precipitation changes in these
regions, we split up the total precipitation into its large-scale and
convective components (Fig. 7). The large-scale component behaves similarly
to the total precipitation shown in Fig. 6 with a positive anomaly in the
00dhL experiment simulated over Scandinavia and the eastern North Atlantic
sector and the southward shift of this pattern simulated when the LIS gets
higher. Hence the drier signal over the western flank of Scandinavia obtained
with the full-LGM LIS (100dhL-noIS) can also be found in the large-scale
component of the total precipitation. This strongly suggests that the
Scandinavian precipitation, as expected, is driven by large-scale processes.</p>
      <p>The negative anomaly of precipitation appearing in the Arctic Ocean north of
the Barents–Kara area (Fig. 6) is also clearly visible in the large-scale
component (Fig. 7); by contrast, the large negative precipitation anomaly
south of the Novaya Zemlya clearly arises from convective processes. Over the
Barents–Kara area, the origin of the precipitation signal is less clear but
seems to be a combination of both convective and large-scale processes. The
decrease of convective precipitation negative anomaly (with respect to noIS) over the
entire SBK sector when the LIS is higher can be easily explained by the
weakening of the summer cooling discussed in section 3.1.</p>
      <p>To further investigate the mechanisms governing precipitation over
Scandinavia and the Barents–Kara area, we examine the seasonality of
precipitation. We first compute the average precipitation above Scandinavia
(55–70<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N : 0–20<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) (Fig. 8a) and the Barents–Kara
region (65–90<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N : 20–100<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) (Fig. 8b), then we
compare summer and winter precipitation anomalies with the annual
precipitation anomaly. Results displayed in Figure 8 show that over
Scandinavia winter precipitation changes are clearly correlated with annual
precipitation (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.99). This means that the annual signal observed over
Scandinavia (Figs. 6 and 7) is mainly due to winter precipitation.
Conversely, the Barents–Kara sector is rather governed by summer
precipitation (at least for LIS altitudes up to 60 % of the PMIP3 one),
as shown by the positive correlation (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.98) obtained for the summer
season (Fig. 8b).</p>
</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <title>Precipitation changes over Scandinavia: implication of the jet
stream shift</title>
      <p>We therefore look for a mechanism prevailing in winter to explain the
Scandinavian precipitation differences. Using the PMIP3 model outputs for the
LGM and the PI time slices, Beghin et al. (2015) found a correlation between
the southward shift of the North Atlantic jet stream from the pre-industrial
to the LGM periods and the winter precipitation changes over the Iberian
Peninsula. Following the same approach, we examine whether a similar
mechanism to the one found in (Beghin et al., 2015) may explain the
precipitation changes over Scandinavia when the LIS characteristics (albedo
and topography) are modified.</p>
      <p>Similarly to Chavaillaz et al. (2013), we use the 850 hPa zonal wind to
define the jet stream. The position of the jet displayed in Fig. 9
corresponds to the position of the 850 hPa meridional wind maximum. The LIS
albedo effect induces a slight northward shift (with respect to noIS) of the North
Atlantic jet stream (00dhL-noIS panel). As the LIS becomes higher, the jet
moves progressively southward and shifts southward of its noIS position
between 30 and 60dhL. From 60dhL and beyond, the Scandinavian winter
precipitation anomaly becomes more and more negative. This suggests a
relationship between the shift of the North Atlantic jet stream and the
precipitation over the Scandinavian region.</p>
      <p>To confirm this assumption, we plot the shift of the jet (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="italic">φ</mml:mi></mml:mrow></mml:math></inline-formula>)
as a function of the precipitation difference between the noIS and the
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL experiments over Scandinavia (Fig. 10). <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="italic">φ</mml:mi></mml:mrow></mml:math></inline-formula> is defined
as the difference of latitudes between noIS and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL experiments where the
850 hPa zonal wind is at its highest value. The latitude of this maximum has
been found by computing the zonal mean of the zonal wind over the Atlantic
basin (50–10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W). To minimize the uncertainties due to model
discretization, we used a parabolic interpolation around the grid point where
the mean zonal wind is largest. The maximum of the corresponding parabola
yields a better approximation of the exact latitude of the maximum jet wind. This method allows for a more accurate finding of the latitude of the jet maximum (Chavaillaz et al., 2013; Beghin et al., 2015). We find a good linear
correlation between the shift of the North Atlantic jet and the Scandinavian
precipitation anomaly during the winter season (Fig. 10). The quantification
of the range of the precipitation anomalies and of the jet shift is obtained
by bootstrapping: a sample of thousand values is obtained by calculating the
average of 1000 randomly picked samples of 40-year duration in the noIS and
the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL original samples. Linear regressions of the 5th and 95th
percentiles of the bootstrapping sample confirm the close link between the
shift of the North Atlantic jet stream and the winter precipitation changes
over Scandinavia due to the effect of LIS.</p>
      <p>The 500 hPa geopotential height (<inline-formula><mml:math display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>500) zonal anomaly over the East
Laurentide sector (90–60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W) does not change significantly when a
flat LIS is imposed (Figs. 5, 11). As the LIS gets higher, the Labrador
trough expands southward: Fig. 11 shows that the zero isoline is located at
<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 43<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in the noIS and 00dhL experiments and progressively
reaches 37<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N for a full-LGM LIS. Over the Atlantic sector
(50–10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W) the Icelandic low/Azores high pattern remain similar in
all experiments up to 60dhL and only show a significant change in the full
LIS experiment (Figs. 5, 11). Indeed, in 100dhL, the Icelandic low's
amplitude weakens but simultaneously expands southward (Fig. 11).
Consistently with these changes in the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mn>500</mml:mn></mml:mrow></mml:math></inline-formula> zonal anomaly, the 500 hPa
westerlies shift southward over the whole Atlantic sector (Fig. 11, bottom).
Again, the largest southward shift for this variable is between the 60 and
100dhL experiments, showing the non-linearity of the atmospheric circulation
to the LIS height.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS4">
  <title>Precipitation changes over the Barents–Kara area </title>
      <p>As previously mentioned in Sect. 3.2.2, the mean annual precipitation changes
over the Barents–Kara area are dominated by the summer signal when the LIS
remains at a relatively low level (i.e. up to 60dhL). This result is
confirmed by the comparison of the patterns of annual (Fig. 6), summer and
winter (Fig. 9) precipitation anomalies. The amount of summer precipitation is
at its lowest level when the sole albedo effect of the LIS is accounted for.
It increases with the LIS altitude in response to warmer temperatures
(Fig. 3). Conversely, the summer snowfall amount decreases from 00 to 100dhL
due to the progressive lowering of the fraction of solid vs. liquid
precipitation.</p>
</sec>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Summary</title>
      <p>To summarize, the LIS albedo effect induces colder summer temperatures over
the entire northwestern Eurasian region (SBK area) with respect to the noIS
experiment. Over southern Scandinavia, the winter temperatures (Fig. 3) are
warmer due to weaker northerlies (Fig. 5). More precipitation is also
simulated in winter in response to the poleward shift of the North Atlantic
jet stream (Fig. 6). As the Barents–Kara sector is dominated by the summer
signal, less precipitation is simulated in response to colder summer
temperatures (with respect to noIS), while a larger snowfall amount is obtained.</p>
      <p>When the LIS gets higher, the negative anomaly of summer temperatures over
the Barents–Kara region becomes weaker due to changes in the atmospheric
circulation. In addition, the higher the LIS, the smaller the amounts of
annual precipitation and snowfall over the Scandinavian and the Barents–Kara
areas, in response to the equatorward shift of the jet.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F17" specific-use="star"><caption><p>Differences in snow accumulation (in m yr<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) computed by the GRISLI
ice-sheet model between <bold>(a)</bold> 00dhLFIS and 00dhL experiments
<bold>(b)</bold> 00dhLFIS and 100dhL experiments, <bold>(c)</bold> 100dhLFIS and
100dhL experiments and <bold>(d)</bold> 00 and 100dhLFIS experiments.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f17.pdf"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>What is the influence of the LIS on the growth of the FIS? </title>
<sec id="Ch1.S4.SS1">
  <title>In case of no initial Fennoscandian ice sheet</title>
      <p>What are the impacts of the LIS on the surface mass balance of both
Scandinavian and Barents–Kara areas? To investigate this question, we use the
LMDZ5 monthly temperatures and precipitation fields of each experiment to
force the ice-sheet model GRISLI. LMDZ5 climatic fields are downscaled over
the GRISLI grid using a bilinear interpolation. Due to the difference of
resolution between the atmospheric and the ice-sheet models, temperature is
vertically corrected using a linear vertical gradient of 6 K km<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>.
Precipitation is also vertically corrected using an exponential function of
the temperature (Charbit et al., 2002, 2007). Snowfall is recalculated using
the downscaled precipitation and temperature because the more detailed
topography of GRISLI allows snowfall when LMDZ5 provides only liquid
precipitation.</p>
      <p>Figure 12 displays the snow accumulation and the ablation fields computed by
GRISLI for the five selected experiments. As expected from the LMDZ5 results
of annual precipitation and snowfall, snow accumulation over Scandinavia is
larger when the LIS is flat and decreases as the LIS is higher. A similar
observation can be made over the Barents–Kara region. Consistently with the
simulated summer temperatures (Fig. 3), when the LIS is flat, the ablation is
weaker over the entire SBK region, and increases as the LIS gets higher.
Nevertheless, even with the full-LGM LIS, the ablation remains weaker than in
the noIS experiment.</p>
      <p>The resulting surface mass balance is shown in Fig. 13a. The similarities
between the ablation (Fig. 12b) and the surface mass balance patterns
indicate that the surface mass balance is dominated by the ablation. In the
absence of LIS, the surface mass balance is positive over only a small part
of the SBK area, namely over Svalbard. Under these conditions, no ice sheet
grows (Fig. 13b). When the LIS is flat, the surface mass balance is positive
over the Barents and Kara seas and over the northern part of Scandinavia,
allowing the growth of ice. The resulting FIS is less extended than those
provided by the ICE-6G (Toscano et al., 2011) and the ANU (Lambeck, 2001)
reconstructions. This is likely due to the absence of the albedo feedback,
since our approach is not based on a full coupling method and does not allow
to account for the impact of ice-sheet changes onto the climate. As the LIS
gets higher, the limit of the positive surface mass balance shifts westward
and northward, excluding the Kara Sea and Scandinavia from the positive
surface-mass balance area. When the LIS has its full LGM size, the surface
mass balance is positive only over the Svalbard. As a consequence, the
simulated FIS is smaller.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F18" specific-use="star"><caption><p>Same as Fig. 14 for the precipitation (mm day<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and 850 hPa
horizontal winds in winter.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f18.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <title>What if the Fennoscandian ice sheet is initially high?</title>
      <p>The aim of this study is not to provide a fully realistic scenario of the
evolution of the ice sheets throughout an entire glacial cycle. Rather, based
on idealized cases, it is to investigate the impact of the Laurentide ice
sheet on the Eurasian ice sheet surface mass balance. In the first part of
this study, we have shown that the growth of the LIS prevents the development
of the FIS. However, back to a more realistic context in which both ice
sheets co-evolved, the relevance of this conclusion may be questioned and the
issue of the FIS inception under full LGM LIS conditions may appear somehow
artificial. Thus, to make our previous conclusions more robust, we perform
two additional LMDZ experiments with new ice-sheet boundary conditions. In
both simulations, the FIS has the elevation computed by the ice-sheet model
for the 00dhL run (i.e. the largest FIS elevation of all the GRISLI
experiments), while the LIS is either “flat” (00dhLFIS) or has its full LGM
altitude (100dhLFIS). Here, our objective is to test the self-consistency of
the overall study, by checking that the growth of the FIS is slowed down when
the LIS gets higher. We first examine how a high FIS modifies the
northwestern Eurasian climate under 00 and 100dhL conditions (i.e. with flat
or full LGM LIS ice sheet), in terms of the temperature and precipitation
fields used in our modeling  approach to compute the ice-sheet surface mass
balance. We then use the climatic outputs to force the ice-sheet model.</p>
<sec id="Ch1.S4.SS2.SSS1">
  <title>Response of the atmosphere</title>
      <p>Figure 14 displays the summer surface air temperature, which is the main
driver of the ablation, for the 00dhL (flat LIS, no FIS), 00dhLFIS (flat LIS,
high FIS), 100dhL (high LIS, noIS) and 100dhLFIS (high LIS, high FIS)
experiments. The comparison between Fig. 14a and b and c and d illustrate the
impact of the Fennoscandian ice sheet on the 2 m summer temperature. As
expected, the presence of Fennoscandia induces a large cooling over the ice
sheet itself, due to the temperature–altitude relationship and to the albedo
effect. In previous sections, we have shown that the cooling observed over
the Barents–Kara region is weakened when the LIS gets higher due to a
modification of the large-scale atmospheric circulation (Figs. 3–4). A
similar mechanism is observed when the Fennoscandian ice sheet is high
(100dhLFIS experiment): the cooling over the ice sheet is reduced and the
warming along the southern margin is amplified (Fig. 14d vs. 14b). These
features result from an increase of warm air advection in the Barents–Kara
sector and to a decrease of northerly heat flux in the south. The presence of
the FIS also induces a split of the North Atlantic jet stream in two branches
resulting in northward deflected heat fluxes along the western margin of the
ice sheet and the Barents Sea sector (Figs. 15b, d and 16b, d). The heat
advection modulates the ice-sheet altitude and albedo effects but is not
sufficient to cancel out the cooling observed over the ice sheet.</p>
      <p>Figure 17 displays maps of snow accumulation differences (after downscaling
on the GRISLI grid) between the four experiments computed by GRISLI after
downscaling. The presence of the Fennoscandian ice sheet results in an
increase of precipitation and snow accumulation over its western flank, along
the Norwegian Sea coast (Fig. 17a, c). This is due to the barrier effect of
the ice sheet and to the subsequent increase of the vertical wind. This
effect is less pronounced when the LIS is high (Fig. 17c) as a result of the
southward displacement of the North Atlantic jet stream (Figs. 6, 11). A
second striking feature is the increase of snow accumulation in the southern
part of the Eurasian ice sheet with respect to the no FIS situation. This is
mainly due to colder temperatures over the ice sheet, increasing the fraction
of total precipitation which falls as snow. In case of a flat LIS, this
accumulation zone is confined to the southern margin and drier conditions
(with respect to the noFIS case) in the interior of the Eurasian ice sheet are observed,
mainly located over the Kara Sea (Fig. 17a), and likely due to the strong
barrier effect. By contrast, when the LIS is high (Fig. 17c), differences
between FIS and no FIS experiments are larger and expand over more than the
southern half of the FIS. This coincides with a larger temperature difference
over the FIS area when the LIS is high (Figs. 14c, d) compared to the low LIS
situation (Fig. 14a, b).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F19" specific-use="star"><caption><p>Difference of simulated ice thickness of the Eurasian ice sheet
between 00d  and 100dhLFIS after 100 kyr (in meters).</p></caption>
            <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://cp.copernicus.org/articles/11/1467/2015/cp-11-1467-2015-f19.pdf"/>

          </fig>

      <p>As mentioned above (Sect. 3.2.1 and Fig. 6), in the absence of FIS, the total
precipitation is driven by large-scale processes over the Scandinavian region
and by convection over the Barents–Kara sector. When the LIS is high, the
southward shift of the winter jet stream (Fig. 9) and the increase of summer
temperature lead to an overall decrease of snowfall over the Eurasian region.
When the FIS is present, the situation is rather different and convective
precipitation is negligible (not shown) due to the cold temperatures induced
by the presence of the FIS. The differences between the 00 and
100dhLFIS experiments are mainly located over the western and southeastern
parts of the ice sheet with respectively larger and smaller snowfall amounts
simulated in the 00dhLFIS experiment (with respect to 100dhLFIS). The excess of
precipitation (total and solid) in the flat LIS/high FIS case is a direct
consequence of the increase of both zonal and meridional humidity transports
in winter (not shown) favored  by the enhanced strength of the 850 hPa
horizontal winds (Fig. 18).</p>
</sec>
<sec id="Ch1.S4.SS2.SSS2">
  <title>Consequences on the simulated Eurasian ice sheets </title>
      <p>The climatic outputs simulated in the 00 and 100dhLFIS experiments have been
used to compute the surface mass balance of the Eurasian ice sheet at the
GRISLI resolution and to force the ice-sheet model with the downscaling
procedure described in Sect. 4.1. Starting from the initial state provided by
the 00dhL GRISLI run with flat (00dhLFIS) or full LGM LIS (100dhLFIS), GRISLI
has been integrated during 100 kyr. At the end of the simulation, the
simulated ice volume and ice covered area simulated in the 00dhLFIS
experiment are respectively 10 and 11 % greater than those obtained with
the 100dhLFIS simulation. The differences in simulated ice thickness between
both simulations are displayed in Fig. 19 (00–100dhLFIS). In most parts of
the simulated ice covered areas, ice thickness differences are fully
consistent with the snow accumulation signal (Fig. 17). In particular, large
positive anomalies (&gt; 500 m) are found in the southwestern
sector, that are greater than 1000 m near the ice sheet margin. In the
northern part, lower ice thicknesses obtained in the 00dhLFIS experiment
correspond to the area of lower snow accumulation (with respect to 100dhLFIS), as
ablation is very small due to summer temperatures largely below
0 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. Surprisingly, another large positive difference is found in
the eastern part which is characterized by a lower amount of snow
accumulation in case of flat LIS. (with respect to full LIS). This pattern results from
warmer temperatures simulated in the southern and eastern parts of the
100dhLFIS Eurasian ice sheet in response to the decrease of cold air
advection (see Sect. 4.2.1). Warmer temperatures found in the south and east
of the FIS when the LIS has its full LGM size  favor the westward and the
northward retreats of the eastern and southern margins of the ice sheet.
Since our approach does not account for the feedback of the simulated ice
sheets on the climate, the amplitude of the different responses are likely to
be underestimated due to an underestimation of the albedo effect. However,
this analysis confirms that the growth of the FIS is slowed down when the LIS
is high and demonstrates the self-consistency of the overall study.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S5">
  <title>Discussion</title>
<sec id="Ch1.S5.SS1">
  <title>Glaciation scenario</title>
      <p>Geomorphological reconstructions revealed that the Fennoscandian ice sheet
eastern limit reached the Putorana Mountains in Siberia during the Early
Weichselian (90–80 kyr BP) (Mangerud et al., 1998; Svendsen et al., 2004).
According to Svendsen et al. (2004), this eastern limit moved back to the
Kara sea around 60 kyr BP, along with the southward extension of the
Scandinavian ice sheet (Andersen and Mangerud, 1989; Lundqvist, 1992;
Mangerud et al., 1998; Houmark-Nielsen, 1999). At the LGM, the ice sheet
finally reached the British Isles, and the Kara ice shelf did not cover the
entire Kara sea anymore (Landvik et al., 1998; Ehlers et al., 2004; Svendsen
et al., 2004). More recently, Kleman et al. (2013) combined geological
evidences and numerical modeling  to reconstruct the paleotopography of past
Northern Hemisphere ice sheets during MIS5b (<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 86 kyr), and MIS4
(<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 64 kyr) and 2 (LGM). They found that the LIS and the FIS grow in
concert in the early part of the last glacial cycle (i.e. until MIS5b), while
after MIS4, their evolution is radically different with a further growth of
the LIS and a significant shrinkage of the FIS due to its southwestward
retreat towards the main precipitation sources.</p>
      <p>Löfverström et al. (2014) propose to attribute the westward shift of
the FIS and the decrease of the Kara ice sheet to warm temperatures over the
southeastern part of the Fennoscandian region, induced by the FIS itself,
along with the upslope precipitation effect proposed by Sanberg and
Oerlemans (1983). In their study, the LIS exerts only a small influence on
the retreat of the Kara ice sheet. While Löfverström et al. (2014)
used realistic LIS topographies provided by the Kleman's et al. (2013)
reconstructions, we used idealized geometries to study separately the impact
of the LIS albedo and topography on climate. The results of our first series
of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhL experiments clearly show that a large but low LIS favors a
positive SMB over the SBK sector (Fig. 13, left panels) and therefore the FIS
maintenance (Fig. 13, right panels). By contrast, as the LIS gets higher,
ablation increases, leading to a smaller FIS. Back to a more realistic glacial
context in which both North American and Eurasian ice sheets exist
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>dhLFIS experiments), we also simulate a net decrease of snow
accumulation under full LGM LIS conditions (with respect to flat LIS) over the Kara
sector combined with an increase over the western part of FIS (Fig. 17d),
consistently with the upslope precipitation effect proposed by Sandberg and
Oerlemans (1983). The large positive SMB values over the SBK sector when the
LIS is low combined with the westward displacement of the Eurasian ice sheet
as the LIS gets higher are fully in line with the ice-sheet paleotopography
reconstructions provided by Kleman et al. (2013) for the last glacial cycle.
The remote interactions highlighted in the present study between the LIS and
the FIS systems also suggest that the ablation increase over the Barents and Kara
seas when the LIS has its LGM size may have contributed to the LGM FIS small
size. Conversely, the larger size of the FIS (Svendsen et al., 2004) during
the late Saalian (around 140 ka) with respect to the LGM may have been related to a
smaller LIS.</p>
      <p>The remote interactions highlighted in the present study between the LIS and
the FIS systems also suggest that the larger size of the FIS (Svendsen et
al., 2004) during the late Saalian (around 140 ka) with respect to the LGM may have
been related to a smaller LIS.</p>
      <p>Nevertheless, we must keep in mind that all experiments presented in this
study have used the LGM land–sea mask and therefore the Barents–Kara region
is considered to be a continental area. The consequences of this assumption on
the simulated large-scale atmospheric circulation are likely to be
negligible. However, accounting for a marine Barents–Kara area would decrease
the positive albedo feedback in this region, and thus the FIS inception (see
Sect. 3.1.1). Our experimental setup uses LGM SST and sea-ice boundary
conditions provided by the coupled atmosphere–ocean IPSL model (Kageyama et
al., 2013). This prevents us from studying the conditions that could have
prevailed with a marine Barents–Kara area, because this sector was covered by
the FIS in this run, and future studies will be necessary to further investigate the relationships between the LIS and the FIS within more realistic
contexts.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <title>Ocean–atmosphere interactions</title>
      <p>Our experimental setup has been designed to investigate how the atmospheric
circulation changes in response to the LIS albedo and topography effects may
impact the climate over the Eurasian region and therefore the evolution of
the surface mass balance of the Fennoscandian ice sheet. We have therefore
neglected the potential impact of the ocean and of its interactions with the
atmosphere</p>
      <p>Yet, changes in atmospheric circulation related to the presence of
continental ice sheets may induce large modifications of the oceanic
circulation. For example, Wunsch (2006) proposed a scenario in which phase
shifts of the stationary waves caused by the development of ice sheets modify
the wind direction and strength leading to abrupt changes in temperature and
precipitation fields (and thus to climatic events having similar features as
Dansgaard-Oeschger events). These changes eventually produce large-scale
modifications of the oceanic circulation. In turn, any change in the
large-scale oceanic circulation may influence the evolution of the Northern
Hemisphere ice sheets as well as their mutual interactions through the
atmosphere–ocean coupling.</p>
      <p>Recently, using the Earth system model COSMOS, Zhang et al. (2014) found that
a gradual increase of the Northern Hemisphere ice-sheet height is able of
causing abrupt transitions of the Atlantic meridonal overturning circulation through a positive
atmosphere–ocean–sea-ice feedback involving the North Atlantic westerlies,
the barotropic ocean circulation and sea-ice cover in the North Atlantic
ocean. In this study, abrupt AMOC transitions from a weak to a strong mode,
occurring for intermediate ice-sheet sizes, are accompanied by a noticeable
increase of surface air temperatures in the northeastern North Atlantic. This
result suggests that the warming effect simulated in our study over the
Eurasian region when the LIS gets higher could be therefore amplified through
North Atlantic warmer temperatures if ocean–atmosphere interactions were
accounted for. However, the mechanism highlighted in Zhang et al. (2014) is
primarily driven by the simulated northward shift of the westerlies when the
Northern Hemisphere ice sheet altitude gradually increases. Under full LGM
conditions, a split of the northern westerlies in two zonal-oriented branches
appears around the Laurentide ice sheet. The southward displacement of the
jet stream simulated in our study when the LIS altitude gradually increases
well supports the existence of the southern branch as shown in Zhang et
al. (2014) for the LGM, but their northern branch remains absent from our all
simulations.</p>
      <p>Actually, this comparison illustrates the diversity of model responses to
changes in the LIS characteristics. The recent inter-comparison study of the
North Atlantic jet stream in LGM vs. pre-industrial conditions in the PMIP3
coupled models (Braconnot et al., 2012) carried out by Beghin et al. (2015)
clearly shows that the response of the jet stream to LGM conditions is highly
model-dependent. This latter study confirms the range of various results
found in the recent literature. Using the outputs of four comprehensive
atmosphere–ocean models, Laîné et al. (2009) found a southward
displacement of the North Atlantic jet stream under LGM conditions. A similar
conclusion can be drawn from the study of Ullman et al. (2014) carried out
with the GISS model and two different LIS topographies as LGM ice-sheet
boundary conditions: the difference of the simulated jet speed obtained with
these different LIS reconstructions (see their Fig. 2) shows a more southward
position of the jet when the LIS is higher. As was found in our study,
Löfverström et al. (2014) found an equatorward position of the winter
zonal winds and a more zonal jet under LGM conditions (with respect to MIS5b and
MIS4). On the contrary, Roberts et al. (2014) found that a more zonal
structure is simulated with the FAMOUS model after the occurrence of a
Heinrich event, which in their experimental set-up corresponds to a decrease
of the Laurentide ice thickness. This indicates a southward shift of the
North Atlantic jet stream when the LIS altitude is lower, and, by contrast, a
northward displacement when it is higher.</p>
      <p>Besides these contrasted findings, other studies did not find any significant
influence of the ocean on the atmospheric circulation. As an example, by
using the coupled IPSL-CM4 model, Pausata et al. (2011) showed that the
position of the North Atlantic jet stream is not substantially influenced by
sea-surface temperatures or sea-ice cover, but rather by ice-sheet height. In
the same way, using the CAM3 atmospheric model coupled to a slab ocean,
Löfverström et al. (2014) did not find any significant changes in the
simulated temperature patterns over Alaska, Asia and the North Atlantic
sector when two different oceanic heat transports corresponding to
interglacial and LGM conditions are used.</p>
      <p>The variety of the model responses calls for further studies to investigate
why the results are so model-dependent. It also underlines the need for a
more in-depth investigation of the links between large-scale oceanic and
atmospheric circulations with different models run under climatic conditions
rather different from those of the present-day periods.</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions</title>
      <p>The goal of this study was to investigate the atmospheric processes through
which the LIS can influence the northwestern Eurasian climate, and therefore
how it can influence the FIS surface mass balance. We performed 12
simulations under LGM conditions, but with different ice-sheet
configurations. In our baseline experiment, the LIS and the FIS are removed.
In the first set of simulations, we only removed the FIS, and the LIS has
different heights. In the final series of experiments, we considered the
impact of the LIS height on a high FIS. We therefore identified the effect
of the LIS albedo and topography on the northwestern European climate. We
focused on the fields having an impact on ice-sheet surface mass balance,
i.e. the temperature and the precipitation. We showed the
following:</p>
      <p><list list-type="order">
          <list-item>

      <p>The LIS albedo acts to decrease the summer temperatures over the
Fennoscandian sector. This decrease is amplified by positive snow albedo
feedback. This positive feedback is somewhat related to our experimental
setup, which imposes land over the Barents–Kara sector instead of water, allowing snow
maintenance. The temperature decrease is weaker when the LIS is higher, due
to atmospheric circulation changes.</p>
          </list-item>
          <list-item>

      <p>In winter, the LIS albedo impact decreases the Barents–Kara temperature,
but increases the Scandinavian temperature. The higher the LIS, the colder
the temperature over the whole Fennoscandian sector.</p>
          </list-item>
          <list-item>

      <p>The effect of LIS albedo also tends to shift the North Atlantic jet
stream poleward, and to bring more precipitation and snowfall over
Scandinavia. When the LIS is higher, the Atlantic jet shifts equatorward,
bringing less precipitation over northern Europe. As a consequence,
precipitation and snowfall decrease over Scandinavia and Barents–Kara
sectors when the LIS is higher.</p>
          </list-item>
          <list-item>

      <p>The analysis of the GRISLI simulations forced by the LMDZ precipitation
and temperature fields shows that the LIS albedo favors the growth of the
FIS, essentially because of weak ablation. As the LIS gets higher, the FIS
gets smaller due to more ablation, in accordance with the LMDZ5 summer
temperature response. When the LIS reaches its full-LGM size, ice remains
over Svalbard only.</p>
          </list-item>
          <list-item>

      <p>Within the context of glacial-interglacial cycles, the FIS inception
under full-LGM LIS conditions appears to be unrealistic. Therefore, we
performed additional simulations with a high FIS and flat and full-LGM LIS.
The results of these new sensitivity experiments show a similar response to
the first series of experiments: in the presence of a full LIS, the FIS
undergoes a significant mass loss. This confirms that a large LIS
counteracts the growth of the FIS although it is still maintained, such as
it does within more realistic contexts, and highlights therefore the
self-consistency of the overall study.</p>

      <p>This study highlights the mechanisms by which the LIS can influence the FIS
surface mass balance. The use of the ice-sheet model allows for the quantification of the
impact of climatic changes due to the LIS presence on the FIS. It shows that
the albedo of the LIS favors the FIS growth, whereas the LIS topography acts
against the FIS development. This conclusion is reinforced by the results
obtained with a high FIS. It is worth noting that without a transient
simulation of the last glacial period, it is not possible to accurately
elaborate the lead–lag relationships of the Northern Hemisphere ice sheets
during the last glacial period. However, based on our results, a plausible
glaciation scenario can be proposed with an early phase of FIS glacial
inception favored by the areal expansion of the LIS, and followed by a
limited growth of the FIS with a progressive westward retreat of the FIS
itself as the LIS altitude gradually increased. Such proposed relationships
between ice-sheet build-up demonstrate that this study also provides new
insights in the understanding of the various Northern Hemisphere ice-sheet
configurations during the different glacial–interglacial cycles.</p>
          </list-item>
        </list></p>
</sec>

      
      </body>
    <back><ack><title>Acknowledgements</title><p>The authors would like to thank Daniel Lunt, Francis Codron, David Salas-y-Mélia
and Hubert Gallée for fruitful discussions about this
work. They are also very grateful to G.Lohmann as well as to two anonymous reviewers for their
constructive comments and suggestions that helped to improve the quality and
the clarity of this manuscript. Pauline Beghin received a grant from CEA
(Commissariat à l'Energie Atomique et aux Energies Alternatives) and this
work was supported by the Université Versailles-Saint-Quentin. This work
also benefited from the HPC resources of CCRT made available by GENCI (Grand
Equipement National de Calcul Intensif), CEA and CNRS (Centre National de la
Recherche Scientifique).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: G. Lohmann</p></ack><ref-list>
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