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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" xml:lang="en" dtd-version="3.0">
  <front>
    <journal-meta><journal-id journal-id-type="publisher">TC</journal-id><journal-title-group>
    <journal-title>The Cryosphere</journal-title>
    <abbrev-journal-title abbrev-type="publisher">TC</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">The Cryosphere</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1994-0424</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/tc-12-3097-2018</article-id><title-group><article-title>Simulation of the future sea level contribution of Greenland
with a new glacial system model</article-title><alt-title>Future sea level contribution of Greenland</alt-title>
      </title-group><?xmltex \runningtitle{Future sea level contribution of Greenland}?><?xmltex \runningauthor{R. Calov et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Calov</surname><given-names>Reinhard</given-names></name>
          <email>calov@pik-potsdam.de</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Beyer</surname><given-names>Sebastian</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3731-0278</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Greve</surname><given-names>Ralf</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1341-4777</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Beckmann</surname><given-names>Johanna</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Willeit</surname><given-names>Matteo</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3998-6404</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Kleiner</surname><given-names>Thomas</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7825-5765</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Rückamp</surname><given-names>Martin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2512-7238</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Humbert</surname><given-names>Angelika</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0244-8760</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Ganopolski</surname><given-names>Andrey</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Potsdam Institute for Climate Impact Research (PIK), Member of the Leibniz Association,
P.O. Box 601203, 14412 Potsdam, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Alfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, Bremerhaven, Germany</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>University of Bremen, Bremen, Germany</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Institute of Low Temperature Science, Hokkaido University, Sapporo, Japan</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Reinhard Calov (calov@pik-potsdam.de)</corresp></author-notes><pub-date><day>2</day><month>October</month><year>2018</year></pub-date>
      
      <volume>12</volume>
      <issue>10</issue>
      <fpage>3097</fpage><lpage>3121</lpage>
      <history>
        <date date-type="received"><day>26</day><month>January</month><year>2018</year></date>
           <date date-type="rev-request"><day>20</day><month>March</month><year>2018</year></date>
           <date date-type="rev-recd"><day>14</day><month>August</month><year>2018</year></date>
           <date date-type="accepted"><day>7</day><month>September</month><year>2018</year></date>
      </history>
      <permissions>
        
        
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://tc.copernicus.org/articles/.html">This article is available from https://tc.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://tc.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://tc.copernicus.org/articles/.pdf</self-uri>
      <abstract>
    <p id="d1e174">We introduce the coupled model of the Greenland glacial system IGLOO 1.0,
including the polythermal ice sheet model SICOPOLIS (version 3.3) with hybrid
dynamics, the model of basal hydrology HYDRO and a parameterization of
submarine melt for marine-terminated outlet glaciers. The aim of this glacial
system model is to gain a better understanding of the processes important for
the future contribution of the Greenland ice sheet to sea level rise under
future climate change scenarios. The ice sheet is initialized via a
relaxation towards observed surface elevation, imposing the palaeo-surface
temperature over the last glacial cycle. As a present-day reference, we use
the 1961–1990 standard climatology derived from simulations of the regional
atmosphere model MAR with ERA reanalysis boundary conditions. For the
palaeo-part of the spin-up, we add the temperature anomaly derived from the
GRIP ice core to the years 1961–1990 average surface temperature field. For
our projections, we apply surface temperature and surface mass balance
anomalies derived from RCP 4.5 and RCP 8.5 scenarios created by MAR with
boundary conditions from simulations with three CMIP5 models. The hybrid ice
sheet model is fully coupled with the model of basal hydrology. With this
model and the MAR scenarios, we perform simulations to estimate the
contribution of the Greenland ice sheet to future sea level rise until the
end of the 21st and 23rd centuries. Further on, the impact of
elevation–surface mass balance feedback, introduced via the MAR data, on
future sea level rise is inspected. In our projections, we found the
Greenland ice sheet to contribute between 1.9 and
13.0 cm to global sea level rise until the year 2100 and between 3.5 and 76.4 cm until the year
2300, including our simulated additional sea level rise due to
elevation–surface mass balance feedback. Translated into additional sea
level rise, the strength of this feedback in the year 2100 varies from 0.4 to
1.7 cm, and in the year 2300 it ranges from 1.7 to 21.8 cm. Additionally,
taking the Helheim and Store glaciers as examples, we investigate the role of
ocean warming and surface runoff
change for the melting of outlet glaciers.
It shows that ocean temperature and subglacial discharge are about equally
important for the melting of the examined outlet glaciers.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e184">Since the last decade of the 20th century, the Greenland ice sheet
(GrIS) has lost mass with accelerating speed
<xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx98" id="paren.1"><named-content content-type="pre">e. g.</named-content></xref>, shaping one of the most
important contributors to sea level rise <xref ref-type="bibr" rid="bib1.bibx89 bib1.bibx78 bib1.bibx27" id="paren.2"/>. This mass loss is not only
driven by decreasing surface mass balance (SMB), but also by increasing ice
discharge via outlet glaciers. The partition between these two
contributions to GrIS mass loss is about equal
<xref ref-type="bibr" rid="bib1.bibx80 bib1.bibx10 bib1.bibx24 bib1.bibx100" id="paren.3"/>. Understanding the processes determining the
GrIS ice loss is vital for estimates of its contribution to future sea
level rise.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p id="d1e200">Flow diagram of the model IGLOO and the interaction between its components.
The 1-D outlet glacier and plume models are generic models, i.e. they can be applied
to each outlet glacier of the Greenland ice sheet. Coupling between the ice sheet model
and the generic outlet glacier models is not implemented yet, denoted by dashed arrows.
In this paper, coupling between HYDRO and the plume model is offline. Simulations
with the coupled generic outlet glacier models and plume models, as well as details
on the coupling between them are described in <xref ref-type="bibr" rid="bib1.bibx7" id="text.4"/>. The exchange
variables are explained in Table <xref ref-type="table" rid="Ch1.T1"/>.</p></caption>
        <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f01.pdf"/>

      </fig>

      <?pagebreak page3098?><p id="d1e214">Nowadays, the scientific community recognizes Greenland
as a complex system mainly composed of the ice sheet and
numerous outlet glaciers <xref ref-type="bibr" rid="bib1.bibx52 bib1.bibx79" id="paren.5"/>,
in subtle interaction with the surrounding ocean via fjord circulation
<xref ref-type="bibr" rid="bib1.bibx95 bib1.bibx66" id="paren.6"/>, and uprising meltwater plumes
in an interplay with the calving outlet glaciers
<xref ref-type="bibr" rid="bib1.bibx69" id="paren.7"/>. In our paper, we introduce the model
IGLOO (Ice sheet model for Greenland including Ocean and Outlet
glaciers, Fig. <xref ref-type="fig" rid="Ch1.F1"/>) intended to represent the
major processes important for the future mass changes of the GrIS on
the timescale of a few centuries. The contribution to future sea
level rise of the several glaciers and ice caps detached from the
GrIS is small compared to the ice sheet and its attached outlet glaciers
<xref ref-type="bibr" rid="bib1.bibx27" id="paren.8"/>. However, these glacial bodies are taken into
account
by SICOPOLIS in our approach.
The idea of IGLOO is to capture the complexity of the
system by its involved model components and, at the same time, to
make the description of all single components as detailed as
necessary <xref ref-type="bibr" rid="bib1.bibx20" id="paren.9"/>. We aim to have a tool with
sufficient computational efficiency to enable large ensemble
simulations on timescales important for future climate change.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p id="d1e239">Abbreviations in Fig. <xref ref-type="fig" rid="Ch1.F1"/>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="2">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Abbreviations</oasis:entry>
         <oasis:entry colname="col2">Physical meaning</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Observed present-day elevation of the GrIS</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M2" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Simulated elevation of the GrIS</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">GRIP</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Reconstruction of temperature anomaly from GRIP ice core</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Anomaly of surface temperature simulated by MAR</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>M</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Anomaly of SMB simulated by MAR</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>R</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Anomaly of runoff simulated by MAR</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Surface temperature</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M8" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Surface mass balance (SMB)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M9" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Surface runoff</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M10" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Subglacial discharge into the given fjord</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M11" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Bottom melt simulated by SICOPOLIS</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M12" display="inline"><mml:mi>W</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Thickness of basal water layer</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M13" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Ocean temperature (function of depth)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M14" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Ocean salinity (function of depth)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M15" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Submerged part of the outlet glaciers</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">Submarine melt of the outlet glaciers</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e524">Knowledge of the present-day state of the GrIS has been improving
considerably. Not only are there reliable data from
numerous observations <xref ref-type="bibr" rid="bib1.bibx101 bib1.bibx4 bib1.bibx65" id="paren.10"><named-content content-type="pre">e.g.</named-content></xref>, but several modelling studies also
exist. Present-day GrIS velocities are resolved by ice sheet models in
horizontal resolutions as high as 600 m, including flow patterns of
outlet glaciers <xref ref-type="bibr" rid="bib1.bibx3" id="paren.11"/>. <xref ref-type="bibr" rid="bib1.bibx84" id="text.12"/>
explicitly demonstrated the multistable-hysteresis behaviour of the
GrIS with a threshold of 1.6 <inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C above present-day
global temperature for the decay of the GrIS; although such a decay
will last at least about 1000 years. The past climate is an important
element for GrIS ice sheet modelling as well, as it serves as
a constraint for parameters particularly capturing the present-day GrIS
<xref ref-type="bibr" rid="bib1.bibx83 bib1.bibx93" id="paren.13"/>, and as it provides the
history of the temperature field inside the present-day GrIS
<xref ref-type="bibr" rid="bib1.bibx33" id="paren.14"/>, which is important for the initialization of
the GrIS in future warming simulations. However, palaeo-simulations
with a free surface have the drawback that their resulting present-day
ice thickness can differ considerably from observations
<xref ref-type="bibr" rid="bib1.bibx14" id="paren.15"><named-content content-type="pre">e. g.</named-content></xref>. Such a simulated ice thickness is an
unfavourable initial condition for projections because, in this case,
the future simulation would start with ice which resides at the wrong
locations or is absent at positions where it should reside according to
observations. This leads to an erroneous drift in projected ice volume
evolution. Therefore, we opt for a fixed domain approach
<xref ref-type="bibr" rid="bib1.bibx13" id="paren.16"/> in our palaeo-spin-ups or, more precisely, for a
scheme that relaxes the simulated surface elevation towards the
observed one <xref ref-type="bibr" rid="bib1.bibx2" id="paren.17"/>. This approach has the<?pagebreak page3099?> advantage
that it provides a good approximation of the present-day temperature–velocity
field for initialization and at the same time prevents a spurious response
in volume during future simulations of several hundred years.
Different initialization methods are discussed by <xref ref-type="bibr" rid="bib1.bibx86" id="text.18"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p id="d1e570">Geographical position of the outlet glaciers mentioned in the
main text. “St” indicates the location of Store Glacier, while “He”
marks the position of Helheim Glacier.</p></caption>
        <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f02.png"/>

      </fig>

      <p id="d1e579">There are several approaches for projecting future ice mass change of the
GrIS, often with a special focus on a certain component of the Greenland
glacial system. Classical SMB approaches assume a
passive ice sheet, but resolve the atmosphere with general circulation
models of the atmosphere <xref ref-type="bibr" rid="bib1.bibx34" id="paren.19"><named-content content-type="pre">e.g.</named-content></xref> or
additionally with a regional model <xref ref-type="bibr" rid="bib1.bibx99 bib1.bibx76 bib1.bibx26" id="paren.20"/>. Several pioneering studies used
three-dimensional dynamic ice sheet models in the shallow ice
approximation (SIA) for projections of GrIS sea level contribution
<xref ref-type="bibr" rid="bib1.bibx48 bib1.bibx37" id="paren.21"><named-content content-type="pre">e.g.</named-content></xref>.  Later, higher-order
<xref ref-type="bibr" rid="bib1.bibx29" id="paren.22"/> or even full-Stokes
<xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx88" id="paren.23"/> ice dynamics were
included for GrIS future projections. In a higher-order ice sheet
model, <xref ref-type="bibr" rid="bib1.bibx30" id="text.24"/> parameterizes ice sliding via
ocean-temperature rise, due to future climate change, to investigate the
impact of ocean warming on future projections of GrIS sea level
contribution. Studies with an atmosphere–ocean general circulation
model coupled to a SIA ice sheet model via surface-energy fluxes were
undertaken by <xref ref-type="bibr" rid="bib1.bibx103" id="text.25"/>. Inspections of GrIS sea level
contribution with a special focus on outlet glaciers were accomplished
with a 3-D ice sheet model by <xref ref-type="bibr" rid="bib1.bibx71" id="text.26"/> or with a 1-D
shallow shelf model <xref ref-type="bibr" rid="bib1.bibx67" id="paren.27"/>.</p>
      <p id="d1e614">Here, we opt for the new
version of SICOPOLIS v3.3 <xref ref-type="bibr" rid="bib1.bibx9" id="paren.28"/>. This version
includes hybrid dynamics, incorporating longitudinal and lateral stresses via the shelfy-stream
approximation <xref ref-type="bibr" rid="bib1.bibx61" id="paren.29"><named-content content-type="pre">SStA;</named-content></xref> longitudinal and lateral
stresses, which are important for nearer-margin fast flow areas, along
with horizontal plane shear <xref ref-type="bibr" rid="bib1.bibx44" id="paren.30"/> via the shallow ice
approximation (SIA), important for the slow-flow regions in the more
central regions of the ice sheet. Hybrid models have been developed
before by <xref ref-type="bibr" rid="bib1.bibx72" id="text.31"/>, <xref ref-type="bibr" rid="bib1.bibx73" id="text.32"/>,
<xref ref-type="bibr" rid="bib1.bibx12" id="text.33"/>, <xref ref-type="bibr" rid="bib1.bibx46" id="text.34"/>, <xref ref-type="bibr" rid="bib1.bibx106" id="text.35"/>, <xref ref-type="bibr" rid="bib1.bibx29" id="text.36"/>
and <xref ref-type="bibr" rid="bib1.bibx70" id="text.37"/>. They are a compromise between the shallow ice
approximation and the full-Stokes approach. Key to these hybrid models is
that SIA and SStA operate on a common domain, although there are other
approaches to treat longitudinal and lateral stresses
<xref ref-type="bibr" rid="bib1.bibx82" id="paren.38"/>. Compared to the SIA, the hybrid dynamics is more
promising for reproducing the velocity field of the GrIS in the
catchment area of ice streams, where there is already fast flow
<xref ref-type="bibr" rid="bib1.bibx79" id="paren.39"/>. We do not employ ice-shelf dynamics in
SICOPOLIS because the dynamics of outlet glaciers, which can
have a floating ice tongue, are part of the outlet glacier component of
IGLOO. We investigate the response of GrIS outlet glaciers to global warming
(including ocean warming) with IGLOO in a separate paper
<xref ref-type="bibr" rid="bib1.bibx7" id="paren.40"/>.</p>
      <?pagebreak page3100?><p id="d1e661">Models assuming a basal water layer for treatment of subglacial hydrology
<xref ref-type="bibr" rid="bib1.bibx90" id="paren.41"/> were often applied to the Antarctic ice
sheet <xref ref-type="bibr" rid="bib1.bibx56 bib1.bibx53" id="paren.42"/>. Here, we apply such
a model to the GrIS, because it captures the major pathways of basal
water toward the outlet glaciers <xref ref-type="bibr" rid="bib1.bibx59" id="paren.43"/>, i.e. the
model resolves in a good approximation the partition of basal water
for the main GrIS outlet glaciers. This is important for reproducing
the subglacial discharge of outlet glaciers, which is fed into our model
of meltwater plumes. Further,
our model for basal hydrology simulates a thickening of the basal water
layer toward the major GrIS outlet glaciers, regions  over which the
ice velocity becomes higher <xref ref-type="bibr" rid="bib1.bibx79" id="paren.44"/>. Therefore,
we couple the ice velocities to the basal water layer, while the basal
melt rate of the ice sheet model provides the input to the model
of basal hydrology. We expect this approach to be suitable for large-scale
modelling of ice sheets on decadal timescales.</p>
      <p id="d1e676">Simulating submarine melt rates at tidewater glaciers has been
accomplished with different models that all share the core of the
buoyant plume theory <xref ref-type="bibr" rid="bib1.bibx87 bib1.bibx107 bib1.bibx91 bib1.bibx92 bib1.bibx16 bib1.bibx22" id="paren.45"/>. Recent studies <xref ref-type="bibr" rid="bib1.bibx50 bib1.bibx8" id="paren.46"/> show that the line plume model by
<xref ref-type="bibr" rid="bib1.bibx51" id="text.47"/> is an adequate tool to determine submarine melt
rates for tidewater glaciers. In our paper, we apply the recently
developed line plume model by <xref ref-type="bibr" rid="bib1.bibx8" id="text.48"/>, based on
the equations by <xref ref-type="bibr" rid="bib1.bibx51" id="normal.49"/>, to two outlet glaciers, the Store and
Helheim glaciers (Fig. <xref ref-type="fig" rid="Ch1.F2"/>), of the Greenland ice
sheet.  We have chosen the Helheim and Store glaciers for investigating
the impact of future warming on glacier melt and for testing our
methods because they are well examined glaciers. Numerous studies on
these glaciers and their connecting fjord systems to the open ocean
exist <xref ref-type="bibr" rid="bib1.bibx94 bib1.bibx97 bib1.bibx81 bib1.bibx49 bib1.bibx18" id="paren.50"/>. Some provide data on
temperature
and salinity profiles inside the fjord from
conductivity–temperature–depth (CTD) measurements or moorings.</p>
      <p id="d1e700">We start with a description of the elements of the glacial system model
IGLOO 1.0, including the future and past forcings utilized in our paper
(Sect. <xref ref-type="sec" rid="Ch1.S2"/>). In Sect. <xref ref-type="sec" rid="Ch1.S3"/>, we describe
our initialization method, while Sect. <xref ref-type="sec" rid="Ch1.S4"/> compares the
simulated present-day surface elevation and velocity with
observations. Further on, modelled basal properties are compared with
findings of other works. In Sect. <xref ref-type="sec" rid="Ch1.S5"/>, we present
projections of the GrIS sea level contribution, the GrIS total basal and
surface runoff and the submarine melt rates for two GrIS outlet
glaciers (Store and Helheim glaciers). The paper closes with a
discussion (Sect. <xref ref-type="sec" rid="Ch1.S6"/>) and conclusions
(Sect. <xref ref-type="sec" rid="Ch1.S7"/>).</p>
</sec>
<sec id="Ch1.S2">
  <title>Ice sheet model for Greenland including ocean and outlet glaciers (IGLOO),
version 1.0</title>
<sec id="Ch1.S2.SS1">
  <title>Overview of IGLOO</title>
      <p id="d1e727">IGLOO is designed for better understanding the response of the
Greenland glacial system to climate change on centennial
timescales. It consists of sub-models for the Greenland ice sheet, the
basal hydrology, the outlet glaciers and the turbulent meltwater
plumes. For initialization via palaeo-runs, the model is forced by the
temperature anomaly from GRIP ice core data, while for future
projections we make use of data from climate models. The design of
IGLOO is shown in Fig. <xref ref-type="fig" rid="Ch1.F1"/>.</p>
      <p id="d1e732">While the ice sheet model SICOPOLIS is coupled bi-directionally with the
model for basal hydrology (HYDRO), the coupling between the turbulent
meltwater plume and HYDRO is so far only implemented offline. In the
model set-up of this paper, SICOPOLIS does not simulate ice
shelves. However, the impact of ocean temperature and subglacial ice
discharge on submarine melt in future warming scenarios is investigated
by the offline coupling with HYDRO for Store Glacier and Helheim
Glacier (Fig. <xref ref-type="fig" rid="Ch1.F2"/>). The coupling between outlet
glaciers and turbulent meltwater plumes, and future warming scenarios
with this model configuration, are described in an accompanying paper by
<xref ref-type="bibr" rid="bib1.bibx7" id="text.51"/>. The coupling between SICOPOLIS and outlet
glaciers is not implemented yet.</p>
      <p id="d1e740">In the following subsections, we will present the parts of IGLOO
relevant for this paper, including coupling and forcing of these
model components.</p>
</sec>
<?pagebreak page3101?><sec id="Ch1.S2.SS2">
  <title>Ice sheet model SICOPOLIS version 3.3</title>
      <p id="d1e749">SICOPOLIS (Simulation Code for Polythermal Ice Sheets;
<uri>http://www.sicopolis.net/</uri>; last access: 21 September 2018)
is a dynamic and thermodynamic ice sheet model that was
originally created by <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx36" id="text.52"/> in a version for the
GrIS. Since then, SICOPOLIS has been developed continuously and
applied to problems of past, present and future glaciation of
Greenland <xref ref-type="bibr" rid="bib1.bibx83" id="paren.53"><named-content content-type="pre">e.g.</named-content></xref>, Antarctica
<xref ref-type="bibr" rid="bib1.bibx54" id="paren.54"><named-content content-type="pre">e.g.</named-content></xref>, the Eurasian ice sheet including
subglacial water <xref ref-type="bibr" rid="bib1.bibx41" id="paren.55"/>, the entire Northern
Hemisphere <xref ref-type="bibr" rid="bib1.bibx31" id="paren.56"/>, the polar ice caps of the planet
Mars and others (see <uri>http://www.sicopolis.net/publ</uri>; last access:
21 September 2018, for a comprehensive
publication list). The description given here follows
<xref ref-type="bibr" rid="bib1.bibx40" id="text.57"/> very closely.</p>
      <p id="d1e781">The model simulates the large-scale dynamics and thermodynamics (ice
extent, thickness, velocity, temperature, water content and age) of ice
sheets three-dimensionally and as a function of time. It is based on the
shallow ice approximation for grounded ice <xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx63" id="paren.58"/>
and the shallow shelf approximation for floating ice <xref ref-type="bibr" rid="bib1.bibx64 bib1.bibx61" id="paren.59"/>. Recently, hybrid shallow-ice and shelfy-stream dynamics have
been added as an option for ice streams <xref ref-type="bibr" rid="bib1.bibx9" id="paren.60"/>. The
rheology is that of an incompressible, heat-conducting, power-law fluid
(Glen's flow law; e.g. <xref ref-type="bibr" rid="bib1.bibx38" id="altparen.61"/>).</p>
      <p id="d1e796">A particular feature of SICOPOLIS is its very detailed treatment of ice
thermodynamics. A variety of different thermodynamics solvers are
available, namely the polythermal two-layer method, two versions of the
one-layer enthalpy method, the cold-ice method and the isothermal method
<xref ref-type="bibr" rid="bib1.bibx39" id="paren.62"/>. The polythermal and enthalpy methods account
in a physically adequate way for the possible co-existence of cold ice
(with a temperature below the pressure-melting point) and temperate ice
(with a temperature at the pressure-melting point) in the ice body, a
condition that is referred to as “polythermal”. It is hereby assumed
that cold ice makes up the largest part of the ice volume, while
temperate ice exists as thin layers overlying a temperate base. In the
temperate ice layers, the water content is computed, and its reducing
effect on the ice viscosity is taken into account <xref ref-type="bibr" rid="bib1.bibx60" id="paren.63"/>.</p>
      <p id="d1e805">SICOPOLIS is coded in Fortran and uses finite difference discretization
techniques on a staggered Arakawa C grid, the velocity components being
taken between grid points <xref ref-type="bibr" rid="bib1.bibx1" id="paren.64"/>. For solving the
thickness evolution equation, we added a further option to the SICOPOLIS
code (Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/>). The simulations of the GrIS discussed
here are carried out in a stereographic plane (WGS 84 reference
ellipsoid, standard parallel 71<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, central meridian
39<inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W), spanned by the Cartesian coordinates <inline-formula><mml:math id="M20" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M21" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>.
The coordinate <inline-formula><mml:math id="M22" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> points upward.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Subglacial hydrology model HYDRO</title>
      <p id="d1e859">HYDRO is a diagnostic model that determines the subglacial water fluxes
instantaneously via the hydrological potential <inline-formula><mml:math id="M23" display="inline"><mml:mi mathvariant="normal">Φ</mml:mi></mml:math></inline-formula>, which
depends on the elevation potential and the
water pressure <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx90" id="paren.65"/>:
            <disp-formula id="Ch1.E1" content-type="numbered"><mml:math id="M25" display="block"><mml:mrow><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mi>g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>b</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          with the ice base <inline-formula><mml:math id="M26" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula>, acceleration due to gravity <inline-formula><mml:math id="M27" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> and
density of water <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mtext>kg m</mml:mtext><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. The
water pressure depends on the ice overburden pressure and the
effective pressure <inline-formula><mml:math id="M29" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> (normal stress at the bed minus water
pressure):
            <disp-formula id="Ch1.E2" content-type="numbered"><mml:math id="M30" display="block"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub><mml:mi>g</mml:mi><mml:mi>H</mml:mi><mml:mo>-</mml:mo><mml:mi>N</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          wherein <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">910</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mtext>kg m</mml:mtext><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> is the density of ice
and <inline-formula><mml:math id="M32" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> is the ice thickness.</p>
      <p id="d1e1017">Following previous authors such as <xref ref-type="bibr" rid="bib1.bibx56" id="text.66"/> and
<xref ref-type="bibr" rid="bib1.bibx59" id="text.67"/>, we assume the water moving in a thin (a few mm) and
distributed water film. Under this premise, the water pressure and the
ice overburden pressure are in equilibrium, and thus the effective
pressure is zero.  This enables us to reformulate Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>) as
            <disp-formula id="Ch1.E3" content-type="numbered"><mml:math id="M33" display="block"><mml:mrow><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mi>g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>b</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub><mml:mi>g</mml:mi><mml:mi>H</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          and then computing the water flux with a simple flux routing scheme as described
by <xref ref-type="bibr" rid="bib1.bibx55" id="text.68"/>.
This approach is only valid at large (km) scales and is not able to
include local processes such as channels.</p>
      <p id="d1e1064">The flux routing method requires that every cell has a defined flow
direction and that, by successively following these directions,
the boundary of the study area is reached. Therefore, local sinks
and flat areas must be removed prior to applying the routing scheme.
We accomplish this by using a Priority-Flood algorithm as described
in <xref ref-type="bibr" rid="bib1.bibx6" id="text.69"/>, which fills depressions in a single pass and
then adds a small gradient to the resulting flats.
Adding a gradient towards the outlet of the depression ensures
that the hydraulic potential is altered in the smallest possible way.
This procedure is a very efficient way to guarantee
that all water is drained into the ocean.</p>
      <p id="d1e1070">The hydraulic potential is computed following Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>), and
we use the basal melt rates from SICOPOLIS as the water input for the
routing scheme (see Sect. <xref ref-type="sec" rid="Ch1.S2.SS5.SSS1"/>). The
timescales of the water flow are much smaller than for the ice flow,
thus, the steady-state water flux <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ψ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> can be obtained by
integrating the basal melt rate along the hydraulic potential.</p>
      <p id="d1e1089">From the resulting water flux <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ψ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, we can compute the
water layer thickness <inline-formula><mml:math id="M36" display="inline"><mml:mi>W</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx105 bib1.bibx104" id="paren.70"/>:
            <disp-formula id="Ch1.E4" content-type="numbered"><mml:math id="M37" display="block"><mml:mrow><mml:mi>W</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">12</mml:mn><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="italic">ψ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mtext>grad</mml:mtext><mml:mi mathvariant="normal">Φ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d1e1153">At locations where sinks in the hydraulic potential have been filled, we
set <inline-formula><mml:math id="M38" display="inline"><mml:mi>W</mml:mi></mml:math></inline-formula> to a very high value (10 m) to account for the presence of a
subglacial lake.</p>
</sec>
<?pagebreak page3102?><sec id="Ch1.S2.SS4">
  <title>Meltwater plume model</title>
      <p id="d1e1169">A further element of IGLOO is the line plume model by
<xref ref-type="bibr" rid="bib1.bibx8" id="text.71"/>, based on <xref ref-type="bibr" rid="bib1.bibx51" id="text.72"/>. It simulates the
width-averaged submarine melt rate of a glacier and accounts for a
uniformly distributed subglacial discharge along the grounding
line. The plume model describes buoyancy-driven rise of subglacial
meltwater until it reaches either neutral buoyancy or the water
surface. Two counteracting processes control the maintenance or
reduction of the plume buoyancy: submarine melting at the ice–ocean
interface preserves the plume buoyancy, while simultaneously turbulent
entrainment and mixing with the surrounding salty fjord water reduces
it. The line plume equations are derived under the assumption that the
plume is in equilibrium and are thus time-independent. The
melt rate is determined by the plume velocity and temperature, which
adapts to the boundary conditions along the glacier front or under the
floating tongue. As input parameters, it requires the submerged part
of the glacier front <inline-formula><mml:math id="M39" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> and the subglacial discharge <inline-formula><mml:math id="M40" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> that leaves
the glaciers grounding line over
the whole glacier width, and a temperature–salinity depth (TSD)
profile close to the glacier. The determination of the input
parameters of the plume model is described in Sect. <xref ref-type="sec" rid="Ch1.S2.SS5.SSS2"/>.</p>
</sec>
<sec id="Ch1.S2.SS5">
  <title>Coupling of model components</title>
<sec id="Ch1.S2.SS5.SSS1">
  <title>Coupling of SICOPOLIS with HYDRO</title>
      <p id="d1e1206">We use a slightly modified version of the Weertman-type sliding law proposed by
<xref ref-type="bibr" rid="bib1.bibx53" id="text.73"/> to couple the basal hydrology model to the ice dynamics:
              <disp-formula id="Ch1.E5" content-type="numbered"><mml:math id="M41" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">v</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>|</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">τ</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:msup><mml:mo>|</mml:mo><mml:mrow><mml:mi>p</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:msubsup><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">n</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mi>q</mml:mi></mml:mrow></mml:msubsup><mml:msub><mml:mi mathvariant="bold-italic">τ</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            with the sliding velocity <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">v</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, basal sliding parameter <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, basal
shear stress <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">τ</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, basal normal pressure
<inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
(assumed as the ice overburden pressure) and the stress and pressure exponents <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mi>q</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>.
We introduce the dimensionless factor
              <disp-formula id="Ch1.E6" content-type="numbered"><mml:math id="M48" display="block"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>(</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>∈</mml:mo><mml:mo>[</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.9</mml:mn><mml:mo>]</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            with
              <disp-formula id="Ch1.E7" content-type="numbered"><mml:math id="M49" display="block"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>T</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">pmp</mml:mi></mml:msub></mml:mrow><mml:mi mathvariant="italic">ν</mml:mi></mml:mfrac></mml:mstyle></mml:mfenced><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mtext>and</mml:mtext><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi>W</mml:mi><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            where <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> incorporate sub-melt sliding and basal hydrology, respectively.
Sub-melt sliding allows sliding below the pressure melting point <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">pmp</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> according to the
decay parameter <inline-formula><mml:math id="M53" display="inline"><mml:mi mathvariant="italic">ν</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx45" id="paren.74"/>, whereas the basal hydrology term depends on the
water layer thickness <inline-formula><mml:math id="M54" display="inline"><mml:mi>W</mml:mi></mml:math></inline-formula> divided by a typical scale
of the layer thickness <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d1e1541">The parameter <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="Ch1.E6"/>) is a weighting factor
between “background sliding” – determined by <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> – and
enhanced sliding due to the basal water layer.  Using <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>
yields the standard model without any effect of basal hydrology, while
<inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.9</mml:mn></mml:mrow></mml:math></inline-formula> leads to the same expression as
<xref ref-type="bibr" rid="bib1.bibx53" id="text.75"/>. In our simulation with basal hydrology, we
apply their parameter value, i.e. we set <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.9</mml:mn></mml:mrow></mml:math></inline-formula>, while
we specify the typical scale of the layer thickness by <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.005</mml:mn><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>.
Further, our decay parameter is <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mi mathvariant="italic">ν</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.</p>
      <p id="d1e1656">The coupling is bi-directional. Basal melt <inline-formula><mml:math id="M64" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> (including the water drainage
from the temperate basal layer of the ice sheet) computed by SICOPOLIS is
used to calculate the thickness of the basal water layer in HYDRO,
which in turn affects the basal sliding via Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>).
Components and data exchange of the complete coupled model IGLOO are
illustrated in Fig. <xref ref-type="fig" rid="Ch1.F1"/>.</p>
</sec>
<sec id="Ch1.S2.SS5.SSS2">
  <title>Offline coupling of SICOPOLIS and HYDRO with the plume model</title>
      <p id="d1e1676">We establish a procedure of determining submarine melt rates with
our line plume model (Sect. <xref ref-type="sec" rid="Ch1.S2.SS4"/>) for all Greenland
outlet glaciers. This procedure applies only offline so far, i.e. the input and
output of the model components are exchanged manually via data files. To clarify,
as this coupling is offline, the sliding of ice (Sect. <xref ref-type="sec" rid="Ch1.S2.SS5.SSS1"/>)
is affected solely by basal melt, while the surface melt and basal melt can impact
the meltwater plume.</p>
      <p id="d1e1683">For the subglacial discharge required by the plume model, we use HYDRO
to route both the basal melt of SICOPOLIS and the surface runoff by
MAR as basal water to the grounding lines of the outlet glaciers. We
route on a monthly timescale to resolve seasonality. For the surface
runoff, we assume that it penetrates directly down to the
bedrock. Among others, <xref ref-type="bibr" rid="bib1.bibx79" id="text.76"/> provide data of the
geographical position of many outlet glaciers. We use these data to
allocate the water leaving the ice sheet to the individual outlet
glaciers.</p>
      <p id="d1e1689">Although we simulate future scenarios, the grounding line position is
considered to be fixed for this procedure. Of course, for glaciers
close to another that share the same catchment area, a moving
grounding line position might have severe effects. We will account for
these dynamic glacier processes in the next version of IGLOO.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e1694">Forcings derived from the MAR regional model. <bold>(a)</bold> Anomaly of annual average
surface temperature, <bold>(b)</bold> total annual SMB anomaly and <bold>(c)</bold> total annual
runoff. Anomalies are taken with respect to the period 1961–1990 from the respective CMIP5
models. RCP 8.5 scenarios are indicated by the solid lines, while RCP 4.5 scenarios
are shown by the dashed lines.
</p></caption>
            <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f03.png"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S2.SS6">
  <title>Evaluating the data from the regional atmosphere model MAR</title>
      <p id="d1e1719">The ice sheet model needs the mean annual surface temperature and
SMB as climate forcings at the surface. In
addition, the plume model requires monthly runoff. Here, we explain
how we derive these forcing fields and their gradients from data of
simulations by the MAR regional climate model
<xref ref-type="bibr" rid="bib1.bibx26" id="paren.77"/>. These fields and their gradients serve to
define our climate forcing of the GrIS for the past
(Sect. <xref ref-type="sec" rid="Ch1.S2.SS7"/>) and for the future
(Sect. <xref ref-type="sec" rid="Ch1.S2.SS8"/>).</p>
      <p id="d1e1729">Historical MAR simulations, using different climate reanalysis products
to define the boundary conditions for the<?pagebreak page3103?> regional simulations, are
available. The boundary conditions for MAR future projections up to
2100 are provided by the output of several CMIP5 general circulation
models for different RCP scenarios. As the MAR simulations are
performed for fixed surface elevation of the GrIS, and we expect
substantial changes in the ice elevation under future warming
scenarios, we correct the regional model output for the change in
surface elevation by applying the gradient method of
<xref ref-type="bibr" rid="bib1.bibx43" id="text.78"/>. In their method, they derived a representative
local elevation gradient of the SMB in each grid point from a
regression of simulated SMB and surface elevation within a given
radius. <xref ref-type="bibr" rid="bib1.bibx43" id="text.79"/> did this separately for accumulation
and ablation regimes. Here, we extend their method by also applying it
to surface temperature and runoff.</p>
      <?pagebreak page3104?><p id="d1e1738">In our scheme, the search radius is set to 100 <inline-formula><mml:math id="M65" display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>, but is extended
until it includes at least 100 grid points if necessary. Our evaluation of
the MAR data for the SMB revealed that the regression is
in many cases not well defined for the accumulation regime.
This issue can be also seen in Fig. 2 by
<xref ref-type="bibr" rid="bib1.bibx43" id="text.80"/>. Therefore, we apply the gradient method only
to the ablation regime and set the SMB elevation gradient for the
accumulation regime to zero.</p>
</sec>
<sec id="Ch1.S2.SS7">
  <title>Past climate forcing and implied SMB of the GrIS</title>
      <p id="d1e1757">Our past climate forcing consists of the surface temperature and the
SMB. By running the model over
one glacial cycle, we determine an initial temperature–velocity field
for our future warming scenarios. In particular, we determine the implied
SMB for the present day, which is used in our future simulations as the
climatological present-day SMB.</p>
      <p id="d1e1760">The surface temperature for the past simulation is computed from the
sum of the climatological field of the present-day surface temperature
simulated by MAR, the temperature anomaly from the GRIP ice core and our
temperature elevation correction obtained from the present-day MAR
simulations:

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M66" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>=</mml:mo><mml:msubsup><mml:mi>T</mml:mi><mml:mrow><mml:mi mathvariant="normal">s</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">rean</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">Clim</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">1961</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1990</mml:mn></mml:mrow></mml:msubsup><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">GRIP</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E8"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>+</mml:mo><mml:msubsup><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">rean</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Clim</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">1961</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1990</mml:mn></mml:mrow></mml:msubsup><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d1e1925">The elevation correction in the last term of Eq. (<xref ref-type="disp-formula" rid="Ch1.E8"/>) is
the surface temperature elevation gradient (Sect. <xref ref-type="sec" rid="Ch1.S2.SS6"/>)
from the MAR reanalysis data times a surface elevation difference, which reads
            <disp-formula id="Ch1.E9" content-type="numbered"><mml:math id="M67" display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          with the surface elevation <inline-formula><mml:math id="M68" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>, simulated with the ice sheet model
SICOPOLIS, and the observed surface elevation
<inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. For the observed surface elevation, we use the one
by <xref ref-type="bibr" rid="bib1.bibx5" id="text.81"/>, which is the same as that utilized by
<xref ref-type="bibr" rid="bib1.bibx26" id="text.82"/>.</p>
      <p id="d1e2020">Here, the SMB <inline-formula><mml:math id="M70" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> is defined by relaxing the ice
sheet's surface elevation towards the observed surface elevation as
            <disp-formula id="Ch1.E10" content-type="numbered"><mml:math id="M71" display="block"><mml:mrow><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">relax</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where
<inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">relax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a relaxation constant. With this relaxation
method, we follow <xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx3" id="text.83"/>.
Outside the ice sheet, we assign the high negative value of
<inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m ice yr<inline-formula><mml:math id="M74" 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>, which prevents the ice to
flow outside its domain. Running the ice sheet model in time
by applying Eq. (<xref ref-type="disp-formula" rid="Ch1.E10"/>) specifies an iteration
for the surface elevation and the SMB. Therefore, we do not need
any further input here.</p>
      <p id="d1e2143">Applying the forcing fields for the surface temperature
(Eq. <xref ref-type="disp-formula" rid="Ch1.E8"/>) and the SMB (Eq. <xref ref-type="disp-formula" rid="Ch1.E10"/>),
we run the model over one glacial cycle. As we start the palaeo-simulation
with the observed surface elevation, the simulated surface
elevation soon relaxes towards the observed elevation. The relaxation
constant <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">relax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> determines how close the simulated
surface elevation is to the observed elevation. When the model
reaches its present-day state (<inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>), we obtain the present-day implied
SMB <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">impl</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which is used in the future simulations, as
            <disp-formula id="Ch1.E11" content-type="numbered"><mml:math id="M78" display="block"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">impl</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>:=</mml:mo><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d1e2226">This SMB field corresponds approximately to the observed SMB, but
compensates for errors of the ice sheet model.
We will discuss further the relaxation approach and its
limitations in Sects. <xref ref-type="sec" rid="Ch1.S3"/> and <xref ref-type="sec" rid="Ch1.S6"/>.</p>
      <p id="d1e2233">Outputs of this procedure are the present-day implied SMB and a
nearly present-day topography set (surface and bedrock elevation)
belonging to this implied SMB. Later on, the present-day implied SMB
field (Eq. <xref ref-type="disp-formula" rid="Ch1.E11"/>) is added to the anomaly forcing of future climate
simulations (see Eq. <xref ref-type="disp-formula" rid="Ch1.E13"/>).</p>
</sec>
<sec id="Ch1.S2.SS8">
  <title>Future climate forcing of the GrIS</title>
      <p id="d1e2246">The surface temperature forcing is computed from the climatological
temperature of MAR simulations for 1961–1990 forced by the ERA
reanalysis boundary conditions, the anomalies from MAR simulations
forced by CMIP5 model output and a temperature elevation correction
as follows:

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M79" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:msubsup><mml:mi>T</mml:mi><mml:mrow><mml:mi mathvariant="normal">s</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">rean</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Clim</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">1961</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1990</mml:mn></mml:mrow></mml:msubsup><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi mathvariant="normal">s</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">5</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msubsup><mml:mi>T</mml:mi><mml:mrow><mml:mi mathvariant="normal">s</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">5</mml:mn><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Clim</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">1961</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1990</mml:mn></mml:mrow></mml:msubsup><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E12"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>+</mml:mo><mml:msub><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">5</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d1e2472">Here, the temperature elevation correction is determined via the
product of the surface temperature elevation gradient (Sect. <xref ref-type="sec" rid="Ch1.S2.SS6"/>) of
the MAR model with boundary condition from the CMIP5 models and
the elevation anomalies simulated with the ice sheet model SICOPOLIS. As
for the palaeoclimate, <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>  are the simulated surface
elevation anomalies (Eq. <xref ref-type="disp-formula" rid="Ch1.E9"/>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p id="d1e2505">Time series of the rate of sea level change produced by the GrIS,
illustrating the impact of the timing of the last two switches during
the initialization. The green curve is from the simulation used for
initialization of our future projections, which switches from the
shallow ice approximation to the hybrid mode at the year 1500 (green square).
The orange curve is from a test simulation (not used for
initialization of our future projections), where we switch from
the shallow ice approximation to the hybrid mode at the year 1900 (orange square).
Both simulations switch from relaxing surface to free surface at the year 1900
(blue square), i.e. for the test simulation, the two switches appear at the
same time.
</p></caption>
          <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f04.png"/>

        </fig>

      <p id="d1e2514">The SMB for future projections is computed as the
sum of the implied SMB, simulated SMB anomalies relative to the reference
period 1961–1990 and an elevation SMB correction as follows:

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M81" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">impl</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>M</mml:mi><mml:mrow><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">5</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msubsup><mml:mi>M</mml:mi><mml:mrow><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">5</mml:mn><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Clim</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">1961</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1990</mml:mn></mml:mrow></mml:msubsup><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E13"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>+</mml:mo><mml:msub><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>M</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">5</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d1e2709">Similar to temperature, the elevation SMB correction is calculated
from the SMB elevation gradient (Sect. <xref ref-type="sec" rid="Ch1.S2.SS6"/>) of<?pagebreak page3105?> the
MAR model with boundary condition from the CMIP5 models, multiplied by
the simulated surface elevation anomalies.</p>
      <p id="d1e2714">Surface runoff is computed for each month from the climatological runoff
of MAR simulations for 1961–1990 forced by the ERA
reanalysis boundary conditions, the anomalies from MAR simulations
forced by CMIP5 models output and a runoff elevation correction
(Sect. <xref ref-type="sec" rid="Ch1.S2.SS6"/>),
which again is computed similarly to the temperature elevation correction:

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M82" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi>R</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:msubsup><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">rean</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Clim</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">1961</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1990</mml:mn></mml:mrow></mml:msubsup><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">5</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msubsup><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">5</mml:mn><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Clim</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">1961</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1990</mml:mn></mml:mrow></mml:msubsup><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E14"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>+</mml:mo><mml:msub><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">MAR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">5</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d1e2927">Negative runoff values, which can result from this approach, are set to zero.</p>
      <p id="d1e2930">Figure <xref ref-type="fig" rid="Ch1.F3"/> shows time series derived from the MAR
data. During the 20th century, all curves show rather minor changes in
average, besides a visible climate variability. This is in line with
general knowledge <xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx10" id="paren.84"><named-content content-type="pre">e.g.</named-content></xref>. In the
21st century, the anomaly of the SMB over Greenland is strongest for
CanESM2, weakest for NorESM1, and MIROC5 lies in between. Of course,
these 21st-century warming trends correspond to IPCC AR5
<xref ref-type="bibr" rid="bib1.bibx21" id="paren.85"/> because the MAR forcing is from the CMIP5
models. The annual average temperature change over Greenland is
stronger than the global one.</p>
      <p id="d1e2943">Over the years 1900–1949, MAR provides data only for MIROC5, and after
the year 2100, MAR does not provide data for any of the GCMs
used. To obtain complete forcings for the years 1900–2300,
we closed the data gaps with an extrapolation procedure
(described in detail in Appendix <xref ref-type="sec" rid="App1.Ch1.S2"/>).
We extended our forcings to the year 2300 for the sake of
comparability with other studies involving ice sheet models, in which
also long projections were made <xref ref-type="bibr" rid="bib1.bibx23" id="paren.86"><named-content content-type="pre">e.g.</named-content></xref>.</p>
</sec>
<sec id="Ch1.S2.SS9">
  <title>Future climate forcing of the plume model</title>
      <p id="d1e2959">As future forcing of the plume model, we employ the subglacial
discharge from HYDRO and SICOPOLIS (Sect. <xref ref-type="sec" rid="Ch1.S2.SS5.SSS2"/>)
under the RCP 8.5 scenario (Sect. <xref ref-type="sec" rid="Ch1.S2.SS8"/>) from MAR
with MIROC5 only. Additionally, a scenario of the temperature and
salinity profiles is needed to project future submarine melting.  Even
for the present day, measurements inside fjords are rare and do not
cover all of Greenland's fjords. We use CTD profiles close to the
glaciers obtained for the year 2016 for Store Glacier (data from
NASA's OMG mission (<uri>https://omg.jpl.nasa.gov/portal/</uri>, last access: 21 September 2018)) and the year
2012 for Helheim Glacier <xref ref-type="bibr" rid="bib1.bibx17" id="paren.87"/>. For the ocean
warming scenario, we assume a linear temperature trend of 0.03 <inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C per year over the years 2000–2100 for
the entire profiles.</p>
      <p id="d1e2981">The 3 <inline-formula><mml:math id="M84" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C ocean warming in
100 years lies in the upper range found by <xref ref-type="bibr" rid="bib1.bibx108" id="text.88"/> for SE
and W Greenland. The determined temperature and salinity profiles, in
combination with the HYDRO output, serve as the input parameters for
the line plume model to determine present and future submarine melting
for the Greenland outlet glaciers.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Model initialization via palaeo-runs</title>
      <?pagebreak page3106?><p id="d1e3003">For the initialization of the ice sheet model, we use the forcings for
the surface temperature and the SMB as described in
Sect. <xref ref-type="sec" rid="Ch1.S2.SS7"/>. Using a standard setting of
SICOPOLIS for palaeo runs, isostatic depression and
rebound of the lithosphere due to changing ice load is modelled
assuming a local lithosphere with relaxing asthenosphere with an
isostatic time lag <xref ref-type="bibr" rid="bib1.bibx58" id="paren.89"><named-content content-type="pre">LLRA approach,</named-content></xref>. For the
geothermal heat, we use the spatial dependent data by
<xref ref-type="bibr" rid="bib1.bibx75" id="text.90"/>. In order to cover one full glacial cycle, we run
the model over 135 kyrs. Initial conditions of these runs are the
present-day ice thickness and elevation by
<xref ref-type="bibr" rid="bib1.bibx5" id="text.91"/>.
The original data with 1 km  horizontal resolution are
downsampled to 5 and 10 km  grid
spacings. To perform a simulation in 5 km  horizontal resolution
over the entire glacial cycle with the hybrid model is illusive, as it
takes 1 day for 100 model years on one HLRS2015 Lenovo NeXtScale
nx360M5 processor. Therefore, we opt to perform the first 130 kyrs of
the glacial cycle in 10 km  horizontal resolution with the
classical shallow ice approximation (SIA) employing the diffusivity
method with an over-implicit ice-thickness solver. The last 5 kyr of
the palaeo-run are performed in 5 km  horizontal resolution. As we
use different model hierarchies and settings, we devote more of our
explanation to these last 5 kyr.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p id="d1e3021">Total ice sheet quantities at present day against relaxation constant. <bold>(a)</bold> Root
mean square error (RMSE) of modelled to observed surface
elevation. <bold>(b)</bold> Total difference between our simulated surface mass
balance and the SMB from the regional model MAR using
ERA reanalysis 1961–1990 climatology.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f05.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p id="d1e3038">Differences between simulated and observed present-day 2-D fields for
various relaxation constants, i.e. 1.5, 100 and 300 years. Panels <bold>(a)</bold>,
<bold>(b)</bold> and <bold>(c)</bold>:
deviation of surface elevation from observed. Panels <bold>(d)</bold>, <bold>(e)</bold> and <bold>(f)</bold>: deviation
of our implied SMB from the SMB from the
regional model MAR.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f06.png"/>

      </fig>

      <p id="d1e3067">During the last 5 kyrs of the run, we have three switches: one for
refining the horizontal resolution, one for switching from SIA mode to
hybrid mode, and a further one for switching from relaxing ice surface
to free ice surface. The first switch at 5 kyr BP refines the horizontal
resolution of the model from 10 to 5 km. The second
switch at 500 years BP changes from SIA to hybrid mode and
additionally applies the mass conservation scheme for the evolution
equation of ice thickness (Eq. <xref ref-type="disp-formula" rid="App1.Ch1.E1"/>). The third switch,
which releases the relaxing ice surface to free development, is
imposed at 100 years BP (year 1900). We introduced the three
switches at different times because they represent different
regime changes.</p>
      <p id="d1e3072">We chose the time of the resolution switch furthest back in time (5 kyr
BP) to allow the ice temperature to adapt to the refined basal
topography. Indeed, by comparing the simulated present-day basal
temperature in 10 km resolution with that in 5 km  resolution
from our simulation with the switches, one can observe that the 5 km
basal temperature shows a much finer structure of the temperate basal
regions at locations of outlet glaciers and their catchment areas;
see also Fig. S1c and d in <xref ref-type="bibr" rid="bib1.bibx15" id="text.92"/>. As these temperate
regions determine areas with basal sliding, enabling fast flow important for
ice dynamics, we regard a time of 5 kyr as sufficient for resolving the
major characteristics of the ice temperature field in the 5 km resolution.</p>
      <p id="d1e3078">Another important aspect for the
choice of an adequate timing of the switches is the rate of sea
level change, which quantifies the model drift and shows directly how
the model recovers from the transition shock. We demonstrate this by inspecting
different switching times and comparing our favourite initialization
run with a test simulation (Fig. <xref ref-type="fig" rid="Ch1.F4"/>). While
our initialization run has the switch from SIA to hybrid at the year 1500
and the switch from relaxing surface to free surface at the year 1900, the
test simulation has both of these switches at the year 1900. Both curves
of the rate of sea level change first rise fast to a maximum and
then drop slowly towards smaller values. For the test
simulation, the maximum is larger (0.06 cm yr<inline-formula><mml:math id="M85" 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>) compared to that of
our initialization run (0.05 cm yr<inline-formula><mml:math id="M86" 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>). More importantly, the test
simulation has not enough time to recover. While the rate of sea level
change of our initialization run at the year 2000 amounts only to
<inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.0007</mml:mn></mml:mrow></mml:math></inline-formula> cm yr<inline-formula><mml:math id="M88" 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>, it is much larger (0.03 cm yr<inline-formula><mml:math id="M89" 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 test
simulation. In future projections, a drift of 0.03 cm yr<inline-formula><mml:math id="M90" 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>
would yield a non-negligible contribution to modelled sea level rise
of 3 cm in 100 years. Therefore, our initialization with separate
switches for regime changes from SIA to hybrid and from relaxed
to free surface is much more favourable and thus used for our
projections (Sect. <xref ref-type="sec" rid="Ch1.S5.SS1"/>).</p>
      <p id="d1e3156">The choice of the relaxation constant rests on numerous simulations
in 10 km horizontal resolution in SIA mode, running the model
over one glacial cycle until the present day. Figure <xref ref-type="fig" rid="Ch1.F5"/> shows
the root mean square error (RMSE) in surface elevation and the total
difference in SMB (the total implied SMB over the GrIS minus the total SMB
simulated by MAR). With increasing relaxation constant, the RMSE in
surface elevation increases moderately, while the total difference in
SMB decreases strongly, i.e.
there is a tradeoff between the RMSE in elevation and the total
difference in SMB.</p>
      <p id="d1e3161">Figure <xref ref-type="fig" rid="Ch1.F6"/> shows the spatial differences between the
observed and modelled surface elevation and SMB for different
relaxation constants. Again, the tradeoff for representing both
surface elevation and SMB is visible. While the simulated elevation is
very close to the observation for small relaxation constants, the SMB
deviation is very high, even in the interior of the ice sheet, where
the deviations reach the amount of magnitude of the accumulation
rate. Therefore, too small relaxation constants should be
excluded. For larger relaxation constants, both difference fields
become<?pagebreak page3107?> smoother, but rather high deviations in surface elevation
appear over vast areas of the GrIS. Therefore, too high relaxation
constants should be excluded too. The spatial differences in
Fig. <xref ref-type="fig" rid="Ch1.F6"/>b, e are from the medium relaxation constant
of <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">relax</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> years. One can see that the simulated
surface elevation is too low over the north-western and south-eastern
marginal regions (Fig. <xref ref-type="fig" rid="Ch1.F6"/>b). Over these regions, the
simulated velocities are too high, which is compensated by an increased
implied SMB (Fig. <xref ref-type="fig" rid="Ch1.F6"/>e) compared to the SMB from
MAR. For most regions of the Northeast Greenland Ice Stream
(NEGIS), the opposite situation occurs. The simulated surface
elevation is too high, while the implied SMB is mostly
negative over that region, which compensates the too low simulated
velocities; see also Fig. <xref ref-type="fig" rid="Ch1.F7"/>. Again, the choice
of the relaxation constant <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">relax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a tradeoff
between the errors in the surface elevation and the errors in the
implied SMB.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p id="d1e3204">Comparison of simulated and observed present-day 2-D fields
with 100 years relaxation constant.
<bold>(a)</bold> Simulated surface elevation, <bold>(b)</bold> surface elevation by
<xref ref-type="bibr" rid="bib1.bibx5" id="text.93"/>, <bold>(c)</bold> simulated horizontal surface velocity and
<bold>(d)</bold> horizontal surface velocity by <xref ref-type="bibr" rid="bib1.bibx79" id="text.94"/>.
The rectangles in panel <bold>(c)</bold> indicate the regions around
Jakobshavn Isbræ, Helheim Glacier and Kangerlussuaq Glacier, which
are enlarged in Fig. <xref ref-type="fig" rid="Ch1.F8"/>.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f07.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p id="d1e3239">Comparison of simulated and observed
<xref ref-type="bibr" rid="bib1.bibx79" id="paren.95"/> velocity for major ice streams and outlet
glaciers.  Left side: modelled, right side: observed.
<bold>(a, b)</bold> Jakobshavn Isbræ, <bold>(c, d)</bold> Helheim Glacier, and <bold>(e, f)</bold> Kangerlussuaq
Glacier. The location of the three regions in Greenland is shown
in Fig. <xref ref-type="fig" rid="Ch1.F7"/>c.</p></caption>
        <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f08.png"/>

      </fig>

</sec>
<sec id="Ch1.S4">
  <title>Present-day Greenland ice sheet</title>
      <?pagebreak page3108?><p id="d1e3268">Here, we present our optimal simulation of the GrIS using the
SICOPOLIS model version 3.3 with hybrid dynamics and the model for
basal hydrology (HYDRO). Both models are fully coupled (see
Sect. <xref ref-type="sec" rid="Ch1.S2.SS5.SSS1"/>), and the horizontal resolution is
always 5 km  from now on. In the hybrid mode, a threshold of
<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">thr</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> applies to the slip ratio (Eq. 8 in
<xref ref-type="bibr" rid="bib1.bibx9" id="altparen.96"/>), i. e., the SStA equations are solved over
the entire ice sheet, and the ice velocities are the weighted sum from
the SIA and SStA velocities with the slip ratio as weight. The boundary
conditions and initialization method to yield the present-day GrIS are
described in Sects. <xref ref-type="sec" rid="Ch1.S2.SS7"/> and <xref ref-type="sec" rid="Ch1.S3"/>,
respectively. As relaxation constant for the surface elevation we use
<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">relax</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> years.  Optimal values for the sliding
parameters are found by minimizing the error of simulated horizontal
surface velocities for values <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> m yr<inline-formula><mml:math id="M96" 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>, using observations
by <xref ref-type="bibr" rid="bib1.bibx79" id="text.97"/>. For such velocities, we expect
basal sliding and hybrid ice dynamics to be
relevant. We found
<inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> m Pa<inline-formula><mml:math id="M98" 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> yr<inline-formula><mml:math id="M99" 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>
to be optimal for the hybrid model with basal hydrology.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p id="d1e3378">Simulated 2-D basal fields.
<bold>(a)</bold> Basal temperature relative to pressure melting
(in <inline-formula><mml:math id="M100" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C), <bold>(b)</bold> thickness of basal water layer (in <inline-formula><mml:math id="M101" display="inline"><mml:mi mathvariant="normal">mm</mml:mi></mml:math></inline-formula>).</p></caption>
        <?xmltex \igopts{width=327.206693pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f09.png"/>

      </fig>

      <p id="d1e3409">By design of the initialization, the simulated surface elevation
compares overall well with the observed one; see
Fig. <xref ref-type="fig" rid="Ch1.F7"/>a, b. However, as our surface relaxation
method leaves the ice sheet's surface a certain degree of freedom (see
also Fig. <xref ref-type="fig" rid="Ch1.F6"/>), the simulated ice surface over
Summit and South Dome as well as on the ridge in between them is
slightly lower. The simulated surface velocities
(<inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> m yr<inline-formula><mml:math id="M103" 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>) over the slow flow regions in the vicinity of
the ridges are somewhat smaller compared to the observed surface
velocities.  Such (small) mismatches also appear with other
higher-order models, even in higher resolution
<xref ref-type="bibr" rid="bib1.bibx3" id="paren.98"/>. As we adjusted the sliding parameter
<inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to match velocities higher than 50 m yr<inline-formula><mml:math id="M105" 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> with
observations, it is obvious that the model cannot resolve every detail
over the slow flow regions. Still, the model resolves the major flow
patterns of the GrIS, including the flow over the catchment area of
the outlet glaciers and the fast flow of the major outlet glaciers and
ice streams. Only the smaller-scale outlet glaciers, e.g. in
north-west Greenland, are not fully resolved. As we have excluded
ice shelves in SICOPOLIS, we cannot reproduce outlet
glaciers with floating tongues, such as Petermann,
Nioghalvfjerdsbræ and Zachariæ Isström. The
NEGIS is the only larger scale feature which we
cannot reproduce properly. This feature cannot be simulated without
additional assumptions (see the Discussion section).</p>
      <p id="d1e3465">Fast flow mainly appears over regions with a temperate ice bed. The
simulated basal temperature in Fig. <xref ref-type="fig" rid="Ch1.F9"/>a shows
a pattern which agrees basically with the reconstruction by
<xref ref-type="bibr" rid="bib1.bibx62" id="text.99"/>. Regions where there is basal melt, mainly
caused by basal friction, exhibit a 1 to 5 mm thick water layer
(Fig. <xref ref-type="fig" rid="Ch1.F9"/>b). There is a pronounced thickening
of the water layer with our Shreve-flow modelling toward major ice
streams and outlet glaciers, which is most visible for NEGIS,
Jakobshavn Isbræ and Helheim Glacier. Moreover, smaller outlet
glaciers like Store Glacier and Daugaard–Jensen Glacier receive
intensified basal water supply too. The red dots over central-east
Greenland correspond to sinks in the hydrological potential. These
sinks are interpreted as subglacial lakes, following
<xref ref-type="bibr" rid="bib1.bibx59" id="text.100"/> who reported similar results. In our
simulations, these sinks can appear over a frozen base too, because we
operate HYDRO with an option that allows computation of the
hydrological potential over the entire ice area. This has the
advantage that all basal water can safely reach the ocean. Allowing a
water layer over a frozen bed for such sinks in the hydrological
potential affects ice dynamics only very little because fully
developed sliding appears only over temperate basal areas, while
sub-melt sliding decays rapidly with decreasing temperature
(Sect. <xref ref-type="sec" rid="Ch1.S2.SS5.SSS1"/>).</p>
      <p id="d1e3481">Figure <xref ref-type="fig" rid="Ch1.F8"/> zooms in Jakobshavn Isbræ and the
two major outlet glaciers Helheim and Kangerlussuaq. Here, the
ability of the model to resolve the catchment areas of these outlet
glaciers in a 50 to 500 m yr<inline-formula><mml:math id="M106" 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> range can be seen in more
detail. However, the high-velocity patterns near the glacier
termini do not fully match the simulations. In particular,
the tributaries of Helheim and Kangerlussuaq
glaciers and the tip of Jakobshavn Isbræ appear rather smooth
compared to the observation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p id="d1e3500">Contribution of the Greenland ice sheet to future sea level
rise under MAR forcing for different scenarios. Sea level rise is
referenced to the year 2000. Beyond 2100, the forcings of the
projections are from prolongations of the original MAR data
(see main text for details). This is indicated by the vertical grey line at
the year 2100 in panels <bold>(b)</bold> and <bold>(d)</bold>. RCP 4.5 projections: <bold>(a)</bold> years 2000–2100
and <bold>(b)</bold> years 2000–2300. RCP 8.5 projections: <bold>(c)</bold> years 2000–2100 and
<bold>(d)</bold> years 2000–2300. The different CMIP5 general circulation models
utilized by MAR are indicated by colours. Different line
characteristics specify optimal simulations with (solid) and without
(long dashed) elevation correction for the SMB. The grey
curves in panels <bold>(a)</bold> to <bold>(d)</bold> indicate a control simulation with solely
the implied SMB (iSMB) as forcing. All simulations are with hybrid ice
dynamics and HYDRO basal hydrology.
</p></caption>
        <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f10.png"/>

      </fig>

</sec>
<?pagebreak page3109?><sec id="Ch1.S5">
  <title>Greenland glacial system projections</title>
<sec id="Ch1.S5.SS1">
  <title>Projections of the GrIS's sea level contribution</title>
      <p id="d1e3546">For our projections of the contribution of the GrIS to global sea
level rise, the GrIS is forced by SMB anomalies and surface
temperatures derived from the MAR regional climate model
(Sect. <xref ref-type="sec" rid="Ch1.S2.SS8"/>), making use of the initial ice sheet
configurations explained in Sect. <xref ref-type="sec" rid="Ch1.S3"/>. As for the
last 500 years of initialization, the fully coupled hybrid model
including basal hydrology is utilized. Outside of the present-day
GrIS area, similarly to the initialization, the prohibiting negative SMB
is applied. In Fig. <xref ref-type="fig" rid="Ch1.F10"/>, we show the GrIS sea level
contribution referenced to the year 2000. The control simulation forced solely
with the implied SMB illustrates the characteristics of our
initialization method. The sea level change from the control run
is always small compared to that of all projections; see Fig. <xref ref-type="fig" rid="Ch1.F10"/>.
Only compared to the RCP 4.5 projection over 300 years, a small change in ice volume
is visible for the control run (Fig. <xref ref-type="fig" rid="Ch1.F10"/>b). At the year 2300, the
control run shows a sea level rise of 3.0 mm. This corresponds to
a model drift of 1.0 mm per hundred years between 2000 and 2300.
Despite such a small change, we correct our simulated sea level contribution of
the GrIS in the simulation with MAR forcing for the implied SMB-only
simulations. This correction is based on the ice volumes from the future
simulations forced with the MAR data and the ice volume from the run
forced with implied SMB only. All simulated ice volumes – those from the runs
with MAR and that from the run forced with implied SMB only – are referenced
to their respective year 2000 volumes.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><caption><p id="d1e3562">Simulated GrIS contribution to sea level rise for the
years 2100 and 2300 in cm.
Rows specify the different GCMs used by MAR. Columns list
the RCP scenarios used by the MAR GCMs and whether we excluded or
included the elevation SMB feedback <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>M</mml:mi><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> in
our simulation.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="9">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right" colsep="1"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">MAR GCM</oasis:entry>
         <oasis:entry rowsep="1" namest="col2" nameend="col5" align="center" colsep="1">Year 2100 [cm] </oasis:entry>
         <oasis:entry rowsep="1" namest="col6" nameend="col9" align="center">Year 2300 [cm] </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry namest="col2" nameend="col3" align="center">RCP 4.5 </oasis:entry>
         <oasis:entry namest="col4" nameend="col5" align="center" colsep="1">RCP 8.5 </oasis:entry>
         <oasis:entry namest="col6" nameend="col7" align="center">RCP 4.5 </oasis:entry>
         <oasis:entry namest="col8" nameend="col9" align="center">RCP 8.5 </oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>M</mml:mi><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">off</oasis:entry>
         <oasis:entry colname="col3">on</oasis:entry>
         <oasis:entry colname="col4">off</oasis:entry>
         <oasis:entry colname="col5">on</oasis:entry>
         <oasis:entry colname="col6">off</oasis:entry>
         <oasis:entry colname="col7">on</oasis:entry>
         <oasis:entry colname="col8">off</oasis:entry>
         <oasis:entry colname="col9">on</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NorESM1</oasis:entry>
         <oasis:entry colname="col2">1.5</oasis:entry>
         <oasis:entry colname="col3">1.9</oasis:entry>
         <oasis:entry colname="col4">4.0</oasis:entry>
         <oasis:entry colname="col5">4.6</oasis:entry>
         <oasis:entry colname="col6">1.8</oasis:entry>
         <oasis:entry colname="col7">3.5</oasis:entry>
         <oasis:entry colname="col8">18.8</oasis:entry>
         <oasis:entry colname="col9">25.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MIROC5</oasis:entry>
         <oasis:entry colname="col2">3.7</oasis:entry>
         <oasis:entry colname="col3">4.3</oasis:entry>
         <oasis:entry colname="col4">7.7</oasis:entry>
         <oasis:entry colname="col5">8.8</oasis:entry>
         <oasis:entry colname="col6">8.5</oasis:entry>
         <oasis:entry colname="col7">10.8</oasis:entry>
         <oasis:entry colname="col8">33.7</oasis:entry>
         <oasis:entry colname="col9">46.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CanESM2</oasis:entry>
         <oasis:entry colname="col2">4.6</oasis:entry>
         <oasis:entry colname="col3">5.6</oasis:entry>
         <oasis:entry colname="col4">11.3</oasis:entry>
         <oasis:entry colname="col5">13.0</oasis:entry>
         <oasis:entry colname="col6">11.2</oasis:entry>
         <oasis:entry colname="col7">17.1</oasis:entry>
         <oasis:entry colname="col8">54.6</oasis:entry>
         <oasis:entry colname="col9">76.4</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e3779">Our projections of the GrIS sea level contribution for the year 2100 are close
to simulations with a fixed present-day GrIS applying the cumulative SMB
method <xref ref-type="bibr" rid="bib1.bibx19" id="paren.101"/>. This is in line with simulations with
an active ice sheet model by <xref ref-type="bibr" rid="bib1.bibx33" id="text.102"/>, who found that
SMB is the major factor determining the GrIS sea level contribution
over the 21st century. Our simulated GrIS sea level
contribution for 2100 ranges from 1.9 cm (RCP 4.5, NorESM1) to 13.0 cm (RCP 8.5,
CanESM2); see Table <xref ref-type="table" rid="Ch1.T2"/>. Still, the
ice dynamics<?pagebreak page3110?> (deformation and sliding velocities)
plays a role in our simulations, indirectly via the SMB change. This
can be seen when comparing the simulations with and without elevation
SMB correction <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mo>∂</mml:mo><mml:mi>M</mml:mi><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula>,
Eq. (<xref ref-type="disp-formula" rid="Ch1.E13"/>).  Ignoring the elevation SMB correction
diminishes simulated 21st-century GrIS sea level contribution between
0.4 and 1.7 cm. Of course, this effect is strongest for the extreme RCP
8.5 scenario together with CanESM2, which is the CMIP5 model used here
with the largest SMB anomaly. Interestingly, the relative
effect of the elevation SMB feedback at the year 2100 is smaller for RCP 8.5 compared
to RCP 4.5. This corresponds to the findings by <xref ref-type="bibr" rid="bib1.bibx103" id="text.103"/>, who
used the ECHAM5 AOGCM coupled to an ice sheet model for their projections.</p>
      <p id="d1e3820">At the end of the 23rd century, the contribution of the GrIS to sea
level rise ranges from 3.5 to 76.4 cm. The importance of the
elevation SMB feedback clearly increases with the elapsed time of the
projections, as the respective curves with <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>M</mml:mi><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula>
on/off diverge more and more from each other.  For RCP 8.5 with
CanESM2, the relative increase of additional loss in ice volume due to
elevation SMB correction nearly triples from 2100 to 2300, from 15 %
to 40 %. This increase of the relative effect of this feedback with
projection time was also observed by <xref ref-type="bibr" rid="bib1.bibx23" id="text.104"/>
and <xref ref-type="bibr" rid="bib1.bibx103" id="text.105"/>. Detailed
numbers for the sea level contributions of the GrIS for the years 2100
and 2300 are listed in Table <xref ref-type="table" rid="Ch1.T2"/>.</p>
      <p id="d1e3848">Overall, our simulations show a strong dependence of the GrIS sea
level contribution both on the RCP scenarios and the models used
to force MAR.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><caption><p id="d1e3853">Time series of the components of subglacial discharge. The
total basal melt (green) is nearly constant in time and ranges from
10 to 12 Gt yr<inline-formula><mml:math id="M111" 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>. Total surface runoff with surface elevation SMB
feedback (blue) and without the feedback (orange).
</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f11.pdf"/>

        </fig>

</sec>
<sec id="Ch1.S5.SS2">
  <title>Projections of the GrIS's total basal and surface runoff</title>
      <p id="d1e3880">For these projections, we use the basal melt from the two simulations by
SICOPOLIS (Sect. <xref ref-type="sec" rid="Ch1.S5.SS1"/>) forced by the MAR<?pagebreak page3111?> data
for which MAR used the MIROC5 GCM under the RCP 8.5 scenario.
Surface and basal melt are routed over the ice base and distributed to the GrIS
outlet glaciers. The details are explained  in Sect. <xref ref-type="sec" rid="Ch1.S2.SS5.SSS2"/>.
Figure <xref ref-type="fig" rid="Ch1.F11"/> depicts the total subglacial discharge split into
surface runoff and basal melt. Over the entire simulation time, the total basal melt
is small and ranges between 10 and 12 Gt yr<inline-formula><mml:math id="M112" 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>, while the total surface runoff increases up
to a peak value of 1700 Gt yr<inline-formula><mml:math id="M113" 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>. Note that, after the year 2100,
the total surface runoff decreases due to the shrinking ice sheet area.
Simultaneously, the effect of the elevation SMB feedback becomes
more important after the year 2100.
At 2100, the difference between the total surface
runoffs with and without elevation SMB feedback amounts to only 150 Gt yr<inline-formula><mml:math id="M114" 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>, while
the same difference for 2300 nearly doubles to 290 Gt yr<inline-formula><mml:math id="M115" 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>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><caption><p id="d1e3940"><bold>(a)</bold> Monthly subglacial discharge derived from runoff and
basal melt (<inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>+</mml:mo><mml:mi>B</mml:mi></mml:mrow></mml:math></inline-formula>) for Helheim Glacier and the scenario RCP 8.5 in the
years 2000 and 2100. <bold>(b)</bold> Temperature–depth and salinity–depth profiles
obtained from measurements for the years 2000 and 2100. The
corresponding submarine melt rates are depicted in panel <bold>(c)</bold>. The effects of
increased temperature and discharge only (orange dotted and green
dashed lines, respectively), as well as the combined effect (solid
lines) are displayed until the year 2100. Melt rates with subglacial
discharge from solely surface runoff are depicted in black. Melt rates
of subglacial discharge containing only surface runoff that was
calculated without the surface elevation feedback are depicted in grey.
</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f12.png"/>

        </fig>

</sec>
<sec id="Ch1.S5.SS3">
  <title>Projections of submarine melt rate for the GrIS outlet glaciers
Helheim and Store</title>
      <p id="d1e3975">Here, we inspect the impact of global warming under the RCP 8.5
scenario for two outlet glaciers: Helheim Glacier and Store
Glacier. In detail, we analyse the impact of both subglacial
discharge and ocean warming – as single and combined effects – on the
submarine melt rate of these outlet glaciers. While the subglacial
discharge comes from simulations with SICOPOLIS and HYDRO under the RCP
8.5 scenario, the ocean warming originates from a scenario similar to
RCP 8.5 (Sect. <xref ref-type="sec" rid="Ch1.S2.SS9"/>). For analysing
the impact of the elevation SMB feedback on submarine melt, the plume
model is forced by subglacial discharge computed with and without the
surface elevation correction of surface runoff (Eq. <xref ref-type="disp-formula" rid="Ch1.E14"/>).
We calculate all submarine melt rates under the assumptions of both
glaciers being tidewater glaciers (no floating tongues) and of their
grounding-line depths and widths remaining constant in time. These
depths and widths are acquired from present-day observations and
amount to 500 m depth and 5 km width for Store Glacier
<xref ref-type="bibr" rid="bib1.bibx18" id="paren.106"/> and 650 m depth <xref ref-type="bibr" rid="bib1.bibx17" id="paren.107"/> and 6 km
width <xref ref-type="bibr" rid="bib1.bibx96" id="paren.108"/> for Helheim Glacier. We chose
the entrainment parameter to be <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.036</mml:mn></mml:mrow></mml:math></inline-formula>, as recommended by
<xref ref-type="bibr" rid="bib1.bibx8" id="text.109"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><caption><p id="d1e4012">Similar to Fig. <xref ref-type="fig" rid="Ch1.F12"/>, but for Store Glacier.
</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f13.pdf"/>

        </fig>

      <?pagebreak page3112?><p id="d1e4023">Figures <xref ref-type="fig" rid="Ch1.F12"/> and <xref ref-type="fig" rid="Ch1.F13"/> illustrate the
monthly subglacial discharge and the temperature profiles for the
years 2000 and 2100 and the resulting submarine melt rates for the RCP
8.5 scenario. For both glaciers, the increasing subglacial discharge
and the increasing ocean temperature have an about equal effect on the
rising submarine melt, with the ocean temperature becoming more
important towards the end of the year 2100. However, the combined
effect of increased subglacial discharge and temperature exceeds the
single effects alone.  As a result, submarine melt exhibits a 2.5-fold
increase for Helheim Glacier and a 4-fold increase for Store Glacier
in the year 2100 (Figs. <xref ref-type="fig" rid="Ch1.F12"/>c and
<xref ref-type="fig" rid="Ch1.F13"/>c). Although for the year 2000 the amount of basal
melt (38 m<inline-formula><mml:math id="M118" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M119" 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 Helheim, 5 m<inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M121" 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 Store) was small compared to summer subglacial discharge
(818 m<inline-formula><mml:math id="M122" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M123" 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 Helheim, 439 m<inline-formula><mml:math id="M124" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M125" 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
Store), it has a significant effect on the annual submarine melt
rate. Due to the basal melt in the winter months (including early
spring and late autumn), the submarine melt rate enlarges in those
months substantially as illustrated by Fig. <xref ref-type="fig" rid="Ch1.F14"/> for
Helheim Glacier. The slight increase in subglacial discharge for all
months (Fig. <xref ref-type="fig" rid="Ch1.F14"/>a) shows clearly the biggest increase
in submarine melt rate for the winter months
(Fig. <xref ref-type="fig" rid="Ch1.F14"/>b) due to the cubic root dependence of
submarine melt rate on subglacial discharge <xref ref-type="bibr" rid="bib1.bibx51" id="paren.110"/>. On
annual average, this effect led, for the year 2000, to an increase
of submarine melt for Helheim Glacier by 40 % and for Store Glacier by
20 % compared to the case when basal melt was not accounted for
(Figs. <xref ref-type="fig" rid="Ch1.F12"/>c and <xref ref-type="fig" rid="Ch1.F13"/>c). At 2100,
the elevation SMB feedback increases the submarine melt
rate of Helheim Glacier and Store Glacier from 787 by 76 to 863 m yr<inline-formula><mml:math id="M126" 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 from 804 by 81 to 723 m yr<inline-formula><mml:math id="M127" 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>, respectively
(Figs. <xref ref-type="fig" rid="Ch1.F12"/>c and <xref ref-type="fig" rid="Ch1.F13"/>c). With about 10 %
for both outlet glaciers, this effect is relatively small. However, as
Fig. <xref ref-type="fig" rid="Ch1.F11"/> suggests, the effect will become more
important for the submarine melt rate after the year 2100.</p>
      <p id="d1e4164">In these experiments, the future submarine melt rate was calculated
assuming a constant glacier terminus position and geometry. These
calculation have to be seen as a first approximation because we neglect
several factors that may influence the submarine melt
rate. For instance, if the glacier retreats, the resulting grounding
line depth may change depending on the underlying bedrock. Another
factor that might change the melt rate estimation considerably is
the distribution of subglacial discharge within the year. Here, we
assumed no time lag in between runoff and its emergence as subglacial
discharge. Due to the cubic root dependence of submarine melting on
subglacial discharge, we already see the possible strong effect of
basal runoff from the ice sheet on the distribution of the submarine
melt rate of an outlet glacier over the year (see
Fig. <xref ref-type="fig" rid="Ch1.F14"/>). Thus, an inefficient drainage system that
is delayed by, e.g. storage of water in subglacial lakes
<xref ref-type="bibr" rid="bib1.bibx68" id="paren.111"/> might substantially affect the seasonal distribution of
subglacial discharge and thus the annual submarine melt rate.</p>
</sec>
</sec>
<sec id="Ch1.S6">
  <title>Discussion</title>
      <p id="d1e4179">In Sect. <xref ref-type="sec" rid="Ch1.S3"/>, we investigated the role of the
relaxation constant for initialization. For very small
relaxation constants, i.e. an essentially fixed ice surface, the
difference between implied and observed SMB at present day becomes
very large (more than 2000 Gt yr<inline-formula><mml:math id="M128" 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>, compared to an insignificant amount
for <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">relax</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> years). Note that the present-day
magnitude of observed total SMB is only about 500 Gt yr<inline-formula><mml:math id="M130" 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>
<xref ref-type="bibr" rid="bib1.bibx25" id="paren.112"><named-content content-type="pre">e .g.</named-content></xref>. This means that computations with
fully fixed surface should be treated with care, as the required total
implied SMB is
very high. A further advantage of the relaxation of the ice surface
is that this smoothes the ice surface because it
has a certain degree of freedom due to the relaxation constant
while solving the ice thickness equation. A similar
smoothing effect when running an ice sheet model with free surface
evolution over 100 years was already observed by <xref ref-type="bibr" rid="bib1.bibx13" id="text.113"/>.
Furthermore, they demonstrated that a smooth ice surface avoids irregular
variations in the vertical velocity field.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><caption><p id="d1e4234">Subglacial discharge of Helheim Glacier <bold>(a)</bold> for the year 2000
determined by runoff (<inline-formula><mml:math id="M131" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>) only (dashed lines), with and without surface
elevation feedback (orange, green) and runoff together with basal melt
(<inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>+</mml:mo><mml:mi>B</mml:mi></mml:mrow></mml:math></inline-formula>, blue solid line). The corresponding submarine melt rates
<bold>(b)</bold> with the same line colour and line style.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f14.pdf"/>

      </fig>

      <?pagebreak page3114?><p id="d1e4268">For our initialization method, we made a number of simplifications.  We
ignored changes in surface elevation and spatial extent of the GrIS
during the past glacial cycle. However, the elevation changes during
the last glacial cycle over central parts of Greenland like Summit
<xref ref-type="bibr" rid="bib1.bibx77" id="paren.114"><named-content content-type="pre">about 100 m,</named-content></xref> or Dye 3 <xref ref-type="bibr" rid="bib1.bibx102" id="paren.115"><named-content content-type="pre">some 100 m,</named-content></xref>
were rather small compared to the ice
thickness. These rather small differences in elevation limit the
inaccuracies in the ice temperature field caused by our relaxation
approach, also because the maxima of these
changes appeared about 10 000 years ago during the Holocene.
Furthermore, due to slowly flowing ice there, a slightly different
temperature–velocity field will not play an important role in
the overall ice dynamic. Also, ignoring the larger areal extension
<xref ref-type="bibr" rid="bib1.bibx28" id="paren.116"/> at the Last Glacial Maximum (LGM) should not
affect the ice temperature field too strongly because over the more
peripheral regions of the ice sheet the velocities are rather high and
the LGM is 21 000 years ago. Here, the ice temperature will adapt
faster and has more time to adapt compared to the central regions of
the ice sheet. The assumption that the derived present-day elevation
correction is valid over the entire glacial cycle is reasonable. We
have examined this by evaluating the temporal dependence of the
vertical temperature gradient from the MAR data. Indeed, for the
future, this temperature gradient does not change too strongly in time,
which does not mean that the elevation correction itself can be neglected
here. Regardless, for the palaeo-run, our ice surface is rather constant
in time due to our relaxation approach, which makes the elevation
correction small in this case.  As a further simplification, we applied
the temperature anomaly from the GRIP record to the entire GrIS. This
is a standard approach; however, we are aware that this anomaly is
spatially dependent in reality. Possible errors in this
anomaly will become less and less important the nearer the
palaeo-simulation approaches the present day. That our present-day
temperature–velocity field is reasonable is supported by the fact that
it lies in the range found by <xref ref-type="bibr" rid="bib1.bibx62" id="text.117"/>. In this
context, we would like to repeat that our initialization serves the
purpose of having the simulated surface elevation in the present day as
close as possible to the observed one to minimize the drift in the future
projections.</p>
      <p id="d1e4287">In our simulations, we cannot reproduce the NEGIS
correctly. Certainly, one reason is that we do not optimize the surface velocity by
a spatially dependent basal sliding coefficient. With spatially
dependent basal sliding coefficients, other studies such as
<xref ref-type="bibr" rid="bib1.bibx74" id="text.118"/> and more recently <xref ref-type="bibr" rid="bib1.bibx71" id="text.119"/>
simulated the NEGIS in better agreement with observations. Nowadays,
there are process-oriented approaches to capture effects important for
basal sliding. For example, stronger basal melting at the onset of the NEGIS
caused by increased geothermal heat due to a palaeo-hotspot
<xref ref-type="bibr" rid="bib1.bibx85" id="paren.120"/> could be a factor speeding up the simulated
NEGIS velocity.</p>
      <p id="d1e4300">For our 300-year sea level projections, which reach beyond the 21st
century, we prolong the forcing data of the MAR model
until the year 2300.  Because we merely held the forcing constant between
2101 and 2300, the real RCP 8.5 forcing could be larger, i.e. we
expect our simulations with the RCP 8.5 scenario to be a lower
estimate of sea level contribution of the GrIS, i.e. the estimate is
a rather conservative one. Most certainly, even all our projections
including RCP 4.5 are a conservative estimate because a full coupling
with ice–ocean interactions is missing in our model yet, and
<xref ref-type="bibr" rid="bib1.bibx30" id="text.121"/> found that ocean warming caused additional mass
loss of the GrIS in his projections by applying a parameterization of
ocean warming.</p>
      <p id="d1e4306">Our additional sea level rise for the year 2100 due to elevation SMB
feedback is somewhat higher than that by <xref ref-type="bibr" rid="bib1.bibx57" id="text.122"/>, who
used the regional model MAR actively coupled to an ice sheet model for
their simulations. For the year 2100, <xref ref-type="bibr" rid="bib1.bibx23" id="text.123"/> give an
additional contribution to sea level rise of the GrIS due to this
feedback, ranging between 0.25 and 0.32 cm under the SRES A1B scenario;
after all,
we excluded their outlier of 0.1 cm. Still, their estimates of this
feedback are rather small compared to our estimates lying between 0.6 and
1.7 cm, which we produced with the RCP 8.5 scenario.
The SRES A1B scenario
is somewhat more moderate that the RCP 8.5 scenario. However, this
cannot explain such low numbers for the elevation SMB feedback. As
demonstrated to be of importance by <?xmltex \hack{\mbox\bgroup}?><xref ref-type="bibr" rid="bib1.bibx57" id="text.124"/><?xmltex \hack{\egroup}?> with fully
interactive two-way coupling, this feedback deserves a detailed
inspection in the future.</p>
      <p id="d1e4320">Our presented projections for the GrIS contribution to global sea level
rise in the 21st century (1.9–13.0 cm) are<?pagebreak page3115?> consistent with previous
publications. However, they do not account for the dynamic response of
Greenland outlet glaciers to ocean warming and increase of
subglacial discharge. This effect will be accounted for in a forthcoming
paper. We also intend to couple the 3-D ice sheet model SICOPOLIS with the 1-D
model for many outlet glaciers.</p>
</sec>
<sec id="Ch1.S7" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e4329">We introduced the coupled Greenland glacial system model IGLOO 1.0,
designed to describe the most important parts of the Greenland glacial
system: the ice sheet, the subglacial hydrological system, the outlet
glaciers and the ice–ocean interaction in the Greenland fjords. The
applicability of the hybrid mode of the ice sheet model SICOPOLIS 3.3
to the Greenland ice sheet was demonstrated.  Full coupling between
the ice sheet model and the model of subglacial water HYDRO has been
accomplished, while the coupling between HYDRO and the meltwater plume
only works offline so far.</p>
      <p id="d1e4332">As initialization, we used a relaxation method similar to
<xref ref-type="bibr" rid="bib1.bibx2" id="text.125"/>, but with a higher relaxation constant of
100 years. For this choice of the relaxation constant, we varied it
systematically and investigated the resulting model behaviour by
inspecting the RMSE in surface elevation as well as the
difference between total simulated SMB and total SMB from the MAR
regional climate model. It showed that, for a relaxation constant of
100 years, the relative error of our simulated total SMB is only 2 %
when using the total MAR SMB as reference, while – at the same time – the
root mean square of the simulated error in
surface elevation stays with a value of 63 m reasonably
small. Additionally, we showed that medium-value relaxation times lead
to smooth 2-D fields of the implied SMB, while for small relaxation
times the fields become noisier, and for large relaxation times
regional deviations of the simulated elevation from the observed one
become relatively large (RMSE of 95 m for <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">relax</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">300</mml:mn></mml:mrow></mml:math></inline-formula> years; see Fig. <xref ref-type="fig" rid="Ch1.F5"/>a).</p>
      <p id="d1e4355"><?xmltex \hack{\newpage}?>Furthermore, we performed projections of the contribution of the GrIS to sea
level rise until the year 2300 with hybrid ice dynamics forced by SMB
anomalies from the MAR regional model. For the RCP 4.5 and 8.5
scenarios generated by MAR, three CMIP5 GCMs with different climate
sensitivity were applied.  Altogether, our projected GrIS sea level
contribution for the year 2100, obtained with elevation SMB feedback, ranges from
1.9 to 13.0 cm, and for the year 2300 from 3.5 to 76.4 cm.
The effect of elevation SMB feedback contributes clearly to
our simulated contribution of the GrIS to sea level rise.
Generally, its impact increases in the long run with decreasing
surface elevation
(see Table <xref ref-type="table" rid="Ch1.T2"/>).</p>
      <p id="d1e4361">Moreover, we demonstrated the importance of the different factors
determining the increase of the melt rate of Greenland outlet glaciers
under the extreme RCP 8.5 scenario, using Store and Helheim Glaciers as
examples. It showed that the knowledge of near-terminus temperature
and subglacial discharge in the fjord are both about equally important
to determine the future melt of these two outlet glaciers. This
underlines the importance of our approach with the Greenland system model IGLOO 1.0.</p>
</sec>

      
      </body>
    <back><notes notes-type="codedataavailability">

      <p id="d1e4368">SICOPOLIS is available as free and open-source
software at <uri>http://www.sicopolis.net/</uri> (last access: 21 September).
The HYDRO module is not yet included in the repository.
The MAR data used as the basis for our forcing are available at
<uri>ftp://ftp.climato.be/fettweis/MARv3.5/Greenland/</uri>  (last access: 21 September).</p>
  </notes><?xmltex \hack{\clearpage}?><app-group>

<?pagebreak page3116?><app id="App1.Ch1.S1">
  <title>Mass-conserving scheme for ice thickness evolution</title>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.F1"><caption><p id="d1e4388">Prolongation of the MAR forcing illustrated for the SMB anomaly.
<bold>(a)</bold> For the years 2101–2300, the SMB anomalies are taken
from random years between 2091–2100.
<bold>(b)</bold> Variability for the years 2101–2300 reduced by 30 %.
The vertical grey line at the year 2100 indicates the beginning of the
prolongation.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/3097/2018/tc-12-3097-2018-f15.png"/>

      </fig>

      <p id="d1e4403">We included a new numerical scheme into SICOPOLIS 3.3,
which discretizes the advection term of
the ice thickness equation by a strictly mass-conserving scheme
in an upwind flux form as follows:

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M134" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><?xmltex \hack{\hbox\bgroup\fontsize{9.5}{9.5}\selectfont$\displaystyle}?><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>(</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>x</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:msubsup><mml:mi>H</mml:mi><mml:mi>x</mml:mi><mml:mo>+</mml:mo></mml:msubsup><mml:mo>-</mml:mo><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>x</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:msubsup><mml:mi>H</mml:mi><mml:mi>x</mml:mi><mml:mo>-</mml:mo></mml:msubsup><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>y</mml:mi><?xmltex \hack{$\egroup}?></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="App1.Ch1.E1"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>y</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:msubsup><mml:mi>H</mml:mi><mml:mi>y</mml:mi><mml:mo>+</mml:mo></mml:msubsup><mml:mo>-</mml:mo><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>y</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:msubsup><mml:mi>H</mml:mi><mml:mi>y</mml:mi><mml:mo>-</mml:mo></mml:msubsup><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math id="M135" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> is the advection term and <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the <inline-formula><mml:math id="M138" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>- and
<inline-formula><mml:math id="M139" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>-components of the depth averaged velocity, respectively. Further, <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:math></inline-formula> are the horizontal spacings. The upwind coefficients read as follows:
          <disp-formula id="App1.Ch1.Ex2"><mml:math id="M142" display="block"><mml:mrow><mml:mtable rowspacing="15pt 15pt 15pt" class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>H</mml:mi><mml:mi>x</mml:mi><mml:mo>-</mml:mo></mml:msubsup><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mfenced open="{" close=""><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>H</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>x</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>H</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>x</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>H</mml:mi><mml:mi>x</mml:mi><mml:mo>+</mml:mo></mml:msubsup><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>H</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>x</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>H</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>x</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>H</mml:mi><mml:mi>y</mml:mi><mml:mo>-</mml:mo></mml:msubsup><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>H</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>y</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>H</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>y</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>H</mml:mi><mml:mi>y</mml:mi><mml:mo>+</mml:mo></mml:msubsup><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mfenced open="{" close=""><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>H</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>y</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>H</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>y</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:mtd></mml:mtr></mml:mtable><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        with the ice thickness <inline-formula><mml:math id="M143" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula>. The pairs <inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, etc. indicate the indices
of the staggered Arakawa C grid.</p>
</app>

<app id="App1.Ch1.S2">
  <title>Filling the data gaps of the MAR forcing for initialization and future simulations</title>
      <p id="d1e5237">While the MIROC5 model provides data starting at the year 1900, the
CanESM2 and NorESM1 models start later in time at the year
1950. Therefore, there are no CanESM2 and NorESM1 data for the
years 1900–1949. The MAR data consist of the MAR fields, which are
longitudinally and latitudinally distributed fields for annual mean surface
temperature, SMB and monthly surface runoff. Because the climate over
Greenland changed relatively little during the 20th century, we took
the years 1950–1999 as a sampling interval and randomly determined
years out of this interval. The MAR fields of a single CMIP5 model
for these random years are
assigned to MAR fields of the subsequent years inside the target
interval, which is defined by the years 1900–1949. By this, we close
the data gaps of CanESM2 and NorESM1 for the years 1900–1949.</p>
      <p id="d1e5240">For the years 2101–2300, there are no direct scenario data available
from MAR for any of the three used CMIP5 models. For the MAR fields
from the RCP 4.5 scenario, we apply the same random procedure as
described above to fill the data gaps, but with the sampling
interval 2091–2100 and the target interval
2101–2300. While for RCP 4.5 forcing the climate-warming trend over
the 21st century is moderate, it is stronger for RCP 8.5,
see Fig. <xref ref-type="fig" rid="Ch1.F3"/>.</p>
      <p id="d1e5245">We found that the variability for the years 2100–2300 was relatively
high for RCP 8.5 scenarios; see Fig. <xref ref-type="fig" rid="App1.Ch1.F1"/>a. Therefore, we modified our random procedure for the MAR fields from
RCP 8.5. For RCP 8.5 forcing, we took only those MAR fields from the
sampling interval that belong to the lower 70 % of their total SMB
anomaly. In other words, we excluded the MAR fields for the upper
30 % of the total SMB anomaly; see Fig. <xref ref-type="fig" rid="App1.Ch1.F1"/>b.
Mathematically this reads as follows:
          <disp-formula id="App1.Ch1.E2" content-type="numbered"><mml:math id="M146" display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msubsup><mml:mi>M</mml:mi><mml:mi mathvariant="normal">tot</mml:mi><mml:mi mathvariant="normal">ave</mml:mi></mml:msubsup><mml:mo>+</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn><mml:mo>⋅</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msubsup><mml:mi>M</mml:mi><mml:mi mathvariant="normal">tot</mml:mi><mml:mi mathvariant="normal">max</mml:mi></mml:msubsup><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msubsup><mml:mi>M</mml:mi><mml:mi mathvariant="normal">tot</mml:mi><mml:mi mathvariant="normal">min</mml:mi></mml:msubsup><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        with the temporal average, the maximum and the minimum of the anomaly
of the total SMB, <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msubsup><mml:mi>M</mml:mi><mml:mi mathvariant="normal">tot</mml:mi><mml:mi mathvariant="normal">ave</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msubsup><mml:mi>M</mml:mi><mml:mi mathvariant="normal">tot</mml:mi><mml:mi mathvariant="normal">min</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msubsup><mml:mi>M</mml:mi><mml:mi mathvariant="normal">tot</mml:mi><mml:mi mathvariant="normal">max</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>,
respectively.</p><?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="authorcontribution">

      <p id="d1e5364">RC performed the coupled simulations
with SICOPOLIS and HYDRO and coordinated the scientific work between the
Alfred Wegener Institute, the Institute of Low Temperature Science and the
Potsdam Institute for Climate Impact Research. SB provided the model HYDRO,
coupled it with SICOPOLIS together with RG, determined the sliding parameters
and computed the monthly discharge for the plume model. JB developed the
plume model and performed the calculations with this model, coupled
<?xmltex \hack{\mbox{offline}}?> with HYDRO. RG supported the usage of SICOPOLIS. MW developed the procedures
for evaluating the MAR data and provided the forcing fields, including their
corrections for elevation changes. TK supported us with conceptual ideas for
the coupling of HYDRO and SICOPOLIS. MR supported the work with HYDRO and
gave conceptual input. AH supervised the developments and studies on
subglacial hydrology. AG designed the concept of IGLOO and the entire study.
RC wrote the manuscript with contributions from all co-authors. The research
related to the paper was discussed by all co-authors.</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e5372">The authors declare that they have no conflict
of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e5379">We wish to thank Fiamma Straneo and Dustin Carroll for providing
temperature and salinity profiles of Helheim glacier,
Xavier Fettweis for hosting the website with the MAR data, and
Ciarion Linstead for technical support with library installations.
Further, we are grateful for helpful suggestions from the
scientific editor Carlos Martin and two anonymous reviewers.
Johanna Beckmann, Reinhard Calov and Sebastian Beyer were funded by the Leibniz Association grant
SAW-2014-PIK-1. Martin Rückamp was supported by the Helmholtz Alliance Climate
Initiative (REKLIM). Matteo Willeit was supported by the Bundesministerium
für Bildung und Forschung (BMBF) grants PalMod-2.1 and PalMod-2.2.
Reinhard Calov was funded by the Bundesministerium für Bildung und
Forschung (BMBF) grants PalMod-1.1 and PalMod-1.3. Ralf Greve was supported
by Japan Society for the Promotion of Science (JSPS) KAKENHI grant
nos. 16H02224 and 17H06104, and by the Arctic Challenge for
Sustainability (ArCS) project of the Japanese Ministry of Education,
Culture, Sports, Science and Technology (MEXT).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
The article processing charges for this open-access <?xmltex \hack{\newline}?>
publication were covered by the Potsdam Institute<?xmltex \hack{\newline}?>
for Climate Impact Research (PIK).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: Carlos Martin<?xmltex \hack{\newline}?>
Reviewed by: two anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>Simulation of the future sea level contribution of Greenland with a new glacial system model</article-title-html>
<abstract-html><p>We introduce the coupled model of the Greenland glacial system IGLOO 1.0,
including the polythermal ice sheet model SICOPOLIS (version 3.3) with hybrid
dynamics, the model of basal hydrology HYDRO and a parameterization of
submarine melt for marine-terminated outlet glaciers. The aim of this glacial
system model is to gain a better understanding of the processes important for
the future contribution of the Greenland ice sheet to sea level rise under
future climate change scenarios. The ice sheet is initialized via a
relaxation towards observed surface elevation, imposing the palaeo-surface
temperature over the last glacial cycle. As a present-day reference, we use
the 1961–1990 standard climatology derived from simulations of the regional
atmosphere model MAR with ERA reanalysis boundary conditions. For the
palaeo-part of the spin-up, we add the temperature anomaly derived from the
GRIP ice core to the years 1961–1990 average surface temperature field. For
our projections, we apply surface temperature and surface mass balance
anomalies derived from RCP 4.5 and RCP 8.5 scenarios created by MAR with
boundary conditions from simulations with three CMIP5 models. The hybrid ice
sheet model is fully coupled with the model of basal hydrology. With this
model and the MAR scenarios, we perform simulations to estimate the
contribution of the Greenland ice sheet to future sea level rise until the
end of the 21st and 23rd centuries. Further on, the impact of
elevation–surface mass balance feedback, introduced via the MAR data, on
future sea level rise is inspected. In our projections, we found the
Greenland ice sheet to contribute between 1.9 and
13.0&thinsp;cm to global sea level rise until the year 2100 and between 3.5 and 76.4&thinsp;cm until the year
2300, including our simulated additional sea level rise due to
elevation–surface mass balance feedback. Translated into additional sea
level rise, the strength of this feedback in the year 2100 varies from 0.4 to
1.7&thinsp;cm, and in the year 2300 it ranges from 1.7 to 21.8&thinsp;cm. Additionally,
taking the Helheim and Store glaciers as examples, we investigate the role of
ocean warming and surface runoff
change for the melting of outlet glaciers.
It shows that ocean temperature and subglacial discharge are about equally
important for the melting of the examined outlet glaciers.</p></abstract-html>
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