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  <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-13-879-2019</article-id><title-group><article-title>The impact of model resolution on the simulated Holocene retreat<?xmltex \hack{\break}?> of the
southwestern Greenland ice sheet using the Ice Sheet<?xmltex \hack{\break}?> System Model (ISSM)</article-title><alt-title>The impact of model resolution on the simulated Holocene retreat</alt-title>
      </title-group><?xmltex \runningtitle{The impact of model resolution on the simulated Holocene retreat}?><?xmltex \runningauthor{J.~K.~Cuzzone et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Cuzzone</surname><given-names>Joshua K.</given-names></name>
          <email>joshua.k.cuzzone@jpl.nasa.gov</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Schlegel</surname><given-names>Nicole-Jeanne</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8035-448X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Morlighem</surname><given-names>Mathieu</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5219-1310</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Larour</surname><given-names>Eric</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Briner</surname><given-names>Jason P.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Seroussi</surname><given-names>Helene</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9201-1644</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Caron</surname><given-names>Lambert</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Earth System Science, Croul Hall, University of California Irvine, Irvine, CA 92697-3100, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Jet Propulsion Laboratory, California Institute of Technology, 4800
Oak Grove Drive MS 300-323, Pasadena,<?xmltex \hack{\break}?> CA 91109-8099, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Geology, University at Buffalo, Buffalo, NY 14260-4130, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Joshua K. Cuzzone (joshua.k.cuzzone@jpl.nasa.gov)</corresp></author-notes><pub-date><day>14</day><month>March</month><year>2019</year></pub-date>
      
      <volume>13</volume>
      <issue>3</issue>
      <fpage>879</fpage><lpage>893</lpage>
      <history>
        <date date-type="received"><day>14</day><month>November</month><year>2018</year></date>
           <date date-type="rev-request"><day>5</day><month>December</month><year>2018</year></date>
           <date date-type="rev-recd"><day>20</day><month>February</month><year>2019</year></date>
           <date date-type="accepted"><day>24</day><month>February</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 Joshua K. Cuzzone et al.</copyright-statement>
        <copyright-year>2019</copyright-year>
      <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/13/879/2019/tc-13-879-2019.html">This article is available from https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019.html</self-uri><self-uri xlink:href="https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019.pdf">The full text article is available as a PDF file from https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e154">Geologic archives constraining the variability of the Greenland
ice sheet (GrIS) during the Holocene provide targets for ice sheet models to
test sensitivities to variations in past climate and model formulation. Even
as data–model comparisons are becoming more common, many models simulating
the behavior of the GrIS during the past rely on meshes with coarse
horizontal resolutions (<inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> km). In this study, we explore the impact of
model resolution on the simulated nature of retreat across southwestern
Greenland during the Holocene. Four simulations are performed using the Ice
Sheet System Model (ISSM): three that use a uniform mesh and horizontal mesh
resolutions of 20, 10, and 5 km, and one that uses a nonuniform mesh with
a resolution ranging from 2 to 15 km. We find that the simulated retreat can
vary significantly between models with different horizontal resolutions based
on how well the bed topography is resolved. In areas of low topographic
relief, the horizontal resolution plays a negligible role in simulated
differences in retreat, with each model instead responding similarly to
retreat driven by surface mass balance (SMB). Conversely, in areas where the bed
topography is complex and high in relief, such as fjords, the lower-resolution models (10 and 20 km) simulate unrealistic retreat that occurs as
ice surface lowering intersects bumps in the bed topography that would
otherwise be resolved as troughs using the higher-resolution grids. Our
results highlight the important role that high-resolution grids play in
simulating retreat in areas of complex bed topography, but also suggest that
models using nonuniform grids can save computational resources through
coarsening the mesh in areas of noncomplex bed topography where the SMB
predominantly drives retreat. Additionally, these results emphasize that care
must be taken with ice sheet models when tuning model parameters to match
reconstructed margins, particularly for lower-resolution models in regions
where complex bed topography is poorly resolved.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e174">As the cryosphere community continues to make strides in understanding
processes that govern variability of the present-day ice sheets, geologic
proxies constraining past ice sheet change provide important clues as to how
ice sheets may have responded to past climate change (Alley et al., 2010).
Decades of research have led to the development of high-resolution geologic
reconstructions that detail the spatial pattern and rate of retreat of the
Greenland ice sheet (GrIS) over the last deglaciation as it evolved towards
its present-day geometry (Weidick, 1968; Bennike and Bjorck, 2002; Young and
Briner, 2015).</p>
      <p id="d1e177">Southwestern Greenland is an area that experienced a large reduction in ice
sheet extent. The ice margin retreated on the order of 150 km inland from
the present-day coastline in response to warming during the early and middle
Holocene (Briner et al., 2016). This landscape is punctuated<?pagebreak page880?> by widely
traceable moraine sequences (Weidick, 1968; Ten Brink and Weidick, 1974) that
extend nearly 600 km throughout western Greenland and provide a constraint
on the past retreat pattern of the GrIS in this region; the chronology of
these moraines continues to be refined (Weidick et al., 2004, 2012; Young et al., 2013;
Larsen et al., 2015; Lesnek and Briner, 2018). This history provides a
benchmark for ice sheet model–data comparisons that will further enhance our
understanding of the processes that influenced GrIS variability during the
past while at the same time helping to highlight deficiencies in existing
model frameworks.</p>
      <p id="d1e180">Currently, ice sheet models simulating the evolution of the GrIS are focused
either on long-term spin-ups over a glacial cycle (Huybrechts, 2002;
Applegate, 2012) or its evolution during the last deglaciation (Tarasov and
Peltier, 2002; Simpson et al., 2009; Lecavalier et al., 2014, 2017; Buizert et al.,
2018). While many of these studies were primarily
concerned with capturing the overall mass changes of the GrIS, one lineage of
studies incorporated datasets of past GrIS change to develop a data-constrained model of its evolution over the last deglaciation. This was
achieved by pairing an ice sheet model with a glacial isostatic adjustment
and relative sea level model (Tarasov and Peltier, 2002; Simpson et al.,
2009; Lecavalier et al., 2014, 2017). By incorporating data constraining the
location of the GrIS beyond the present-day coastline, its vertical extent
through time (i.e., ice thinning records), and records of relative sea level,
the studies by Lecavalier et al. (2014, 2017) represent the most
comprehensive model of GrIS change during the last deglaciation, with the
results recently being compared against geologic archives of ice margin
change (Larsen et al., 2015; Young and Briner, 2015; Sinclair et al, 2016).</p>
      <p id="d1e183">While the models of Lecavalier et al. (2014, 2017) capture the timing
and retreat pattern associated with the deglaciation in many locations well, large
mismatches occur, particularly in southwestern Greenland and in areas where
fast flow may have dominated (Young and Briner, 2015; Sinclair et al., 2016).
The climatology used to force ice sheet models through time remains a primary
source of uncertainty, and great strides have been made to improve our
understanding of past climate history in Greenland through improved
reconstructions of temperature (e.g., Kobashi et al., 2017; Lecavalier et
al., 2017) and methods involving data assimilation of paleoclimate proxies
with climate model output (Hakim et al., 2016; Buizert et al., 2018).
Although recent experiments have investigated sensitivities to model
formulation (Zekollari et al., 2017) and horizontal resolution over past
climates (Zekollari et al., 2017; Seguinot et al., 2016; Golledge et al.,
2012), testing the sensitivity of simulated ice retreat to the ice flow
dynamics model (i.e., the level of complexity in its numerical approximations)
and to model resolution, both in time and space, still remains an important
area of research.</p>
      <p id="d1e187">With regards to model setup, the use of coarse model resolutions (<inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> km grid spacing) might explain some of the model–data discrepancy
(Larsen et al., 2015; Young and Briner, 2015; Sinclair et al., 2016). Driven
by how well models resolve subglacial topography, simulations of the present-day GrIS have shown an important dependence on model resolution for
accurately simulating ice flow across Greenland (Greve and Herzfeld, 2013;
Aschwanden et al., 2016). Dependence on model resolution also extends to
modeling future ice mass loss, where higher-resolution models simulate more
mass loss than models with lower resolutions (Greve and Herzfeld, 2013).
Although some work has focused on model resolution and its impact on
simulated mass flux from the GrIS for in the present and the future, how model
resolution affects simulated retreat in paleo-ice-sheet modeling studies is
not well constrained. Prior work demonstrates that low-resolution grids limit
a model's ability to capture features such as ice streams and marine-terminating outlet glaciers (Aschwanden et al., 2016), which might be on the
order of a few kilometers in width. Additionally, in land-terminating
portions of an ice sheet, low model resolution may lead to large jumps in the
snowline, which ultimately can lead to large advances or retreats in the ice
margin on the order of the model resolution (Young and Briner, 2015; Sinclair
et al., 2016), and therefore limit the model's ability to capture smaller-scale ice
marginal fluctuations (i.e., km scale).</p>
      <p id="d1e200">In this study, we present results from regional ice sheet modeling
experiments in southwestern Greenland during the Holocene using the
three-dimensional thermomechanical Ice Sheet System Model (ISSM). We build on
earlier efforts that focused on this ice sheet sector (e.g., Van Tatenhove et
al., 1995). Ice model resolution is the primary target for assessment here,
with four separate simulations being run, each with its own horizontal
resolution ranging from 20 to 2 km. In this study we do not attempt to
obtain a perfect match between the simulated model retreat and that derived
from the geologic reconstructions, as that requires further sensitivity
studies that are not the current motivation for this work. Instead, since
model resolution is a constraint that is typically not explored when studying
the past due to the computational cost, in this study we aim to determine
whether increased model resolution is worth the computation time for
simulating past ice sheet retreat.</p>
</sec>
<sec id="Ch1.S2">
  <title>Model description and setup</title>
<sec id="Ch1.S2.SS1">
  <title>Ice sheet model</title>
      <p id="d1e214">We use the Ice Sheet System Model v4.13 (ISSM; Larour et al., 2012), a finite-element, thermomechanical ice sheet model. We choose the higher-order
approximation of Blatter (1995) and Pattyn (2003), hereafter referred to as BP,
to solve the momentum balance equations. Although recent work has used the
higher-order approximation in simulations over past time periods (Zekollari
et al., 2017), this ice flow approximation is still rarely used when
simulating over<?pagebreak page881?> paleoclimate timescales. We use this approximation, however,
as our choice is based upon representing the past dynamics of the ice sheet
history as best as possible even though computational time is increased over
conventional paleoclimate ice sheet models using the more common shallow ice
approximation (SIA; Hutter, 1983).</p>
      <p id="d1e217">The model domain for this study (Fig. 1) focuses on the southwestern region
of Greenland, where geologic proxies detail Holocene ice retreat from the
present-day coastline (Weidick, 1968; Ten Brink and Weidick, 1974). By
constraining our domain to southwestern Greenland, the number of mesh
elements within the model can be minimized when compared to modeling the
entire GrIS, thus reducing the computational load. The model domain extends
from the present-day coastline to the ice sheet divide. The southern and
northern borders of the domain coincide with areas of minimal north-to-south
across-boundary flow based upon present-day ice surface velocities from
Rignot and Mouginot (2012). The associated boundary conditions used to drive
the model are discussed in Sect. 2.6.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><label>Figure 1</label><caption><p id="d1e222">Present-day interferometric synthetic aperture radar (InSar) ice
surface velocities from Rignot and Mouginot (2012) for the Greenland ice
sheet. The regional model domain is highlighted in black. Marked locations
correspond to (1) Jakobshavn Isbræ, (2) Kangiata Nunâta Sermia (KNS),
and (3) Nuuk.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS2">
  <title>Domain discretization</title>
      <p id="d1e237">Typically, prior paleoclimate ice sheet modeling efforts across Greenland
have used uniform meshes with a horizontal resolution of 20 km (Simpson,
2009; Lecavalier, 2014); a more recent model used a 10 km horizontal mesh
resolution (Buizert et al., 2018). For the following experiments, the first
three models are generated using a uniform triangular grid with horizontal
resolutions of 20, 10, and 5 km. The fourth model (herein referred to as
<italic>nonuniform</italic>) relies on anisotropic mesh adaptation, whereby the
element size varies as a function of the bed topography (see Fig. S1 in the
Supplement for visualization of mesh resolutions). The maximum horizontal
mesh resolution is 15 km where gradients in the bed topography are smooth
(primarily the interior bed over the domain) and becomes progressively finer
in areas of high relief, with a minimum horizontal resolution of 2 km
(mainly in fjord regions). The bed topography for each model is taken from
BedMachine Greenland v3 (Morlighem et al., 2017) and is initialized with
present-day ice surface elevation from the Greenland Ice Mapping Project digital elevation model of Howat et al. (2014).
In Fig. 2, the corresponding bed height is shown for each model detailing the
associated differences based on horizontal grid resolution. Generally, the
bed topography is captured better using the higher-resolution mesh, with the
nonuniform mesh (Fig. 2a) being able to best resolve valleys along the
present-day coastline. The 5 km mesh captures the same general topographic
features as the nonuniform mesh, albeit with less detail. At 10 km,
individual valleys become unresolved, particularly around Nuuk and Jakobshavn
Isbræ (see Fig. 1 for locations). The 20 km model fails to capture any
topographic features that would hold glacier outlets.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><label>Figure 2</label><caption><p id="d1e245">Associated bed topography maps for the nonuniform high-resolution
mesh <bold>(a)</bold>, uniform 5 km mesh <bold>(b)</bold>, uniform 10 km mesh
<bold>(c)</bold>, and uniform 20 km mesh <bold>(d)</bold>.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS3">
  <title>Surface mass balance (SMB)</title>
      <?pagebreak page882?><p id="d1e272">We use the positive degree day method outlined in Tarasov and Peltier (1999)
to construct the necessary accumulation and ablation history used to drive
our ice sheet model during the past from monthly mean temperature and
precipitation fields. The spatial monthly mean surface air temperature and
precipitation climatology spanning the period 1980–2010 is taken from Box et
al. (2013). The surface air temperatures are then scaled based upon isotopic
variations in the Greenland Ice Core Project (GRIP) <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>
record (Dansgaard et al., 1993) as follows:
            <disp-formula id="Ch1.E1" content-type="numbered"><mml:math id="M4" display="block"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mfenced open="(" close=")"><mml:mi>t</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mi mathvariant="italic">δ</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mfenced open="(" close=")"><mml:mi>t</mml:mi></mml:mfenced><mml:mo>+</mml:mo><mml:mn mathvariant="normal">34.83</mml:mn></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mi>d</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.4</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C ‰<inline-formula><mml:math id="M7" 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> (Huybrechts, 2002). Anomalies
from Eq. (1) are applied to the present-day climatology to create a
temperature forcing back through time. Precipitation rate changes 7.3 %
for every 1 <inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C of temperature change derived in Eq. (1) (Huybrechts,
2002). For the positive degree day scheme, snow melts first (0.006 m
 <inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C<inline-formula><mml:math id="M10" 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> day<inline-formula><mml:math id="M11" 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>) followed by bare ice (0.0083 m
 <inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C<inline-formula><mml:math id="M13" 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> day<inline-formula><mml:math id="M14" 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 allocation for the formation of
superimposed ice included (see supplemental information in Le Morzadec et
al., 2015). The temperature forcing is adjusted throughout the run using a
lapse rate correction of 5 <inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C km<inline-formula><mml:math id="M16" 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> (Abe-Ouchi et al., 2007) to
account for changes in ice surface height throughout the simulation, while
elevation-dependent desertification is included (Budd and Smith, 1981) to
ensure reduction in precipitation by a factor of 2 for every kilometer change
in ice sheet surface elevation. Further details regarding the positive degree
day and accumulation scheme implemented within the ISSM can be found in Le
Morzadec et al. (2015).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Thermal model and basal drag</title>
      <p id="d1e462">The thermal evolution of the ice is captured using an enthalpy formulation
described in Aschwanden et al. (2012), which includes formulations for both
temperate and cold ice. Transient surface air temperatures are imposed at the
ice surface, while geothermal heat flux (from Shapiro and Ritzwoller, 2004)
is applied at the base. The model contains five vertical layers, with spacing
between layers decreasing modestly towards the base. To simulate the vertical
distribution of temperature within the ice sheet, we rely on quadratic finite
elements (i.e., P1 <inline-formula><mml:math id="M17" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> P2) along the <inline-formula><mml:math id="M18" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> axis as a means for our
vertical interpolation. Details of the implementation and description of
these higher-order vertical finite elements can be found in Cuzzone et
al. (2018). Through using higher-order finite elements as a means for
vertical interpolation, this method allows the ice sheet model to capture
sharp thermal vertical gradients particularly at the bed, which is an
improvement over conventional methods using a linear vertical interpolation,
despite having fewer vertical layers. This ultimately limits the necessity
for a large number of vertical layers in our ice model and therefore
decreases computational load.</p>
      <p id="d1e479">To capture spatial variations in sliding, the spatially varying basal drag
coefficient (<inline-formula><mml:math id="M19" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>) in Eq. (2) is derived using inverse methods (Morlighem et
al., 2010; Larour et al., 2012), providing the best match between modeled and
interferometric synthetic aperture radar (InSAR) surface velocities (Rignot and Mouginot, 2012). This is performed
independently for each model resolution.
            <disp-formula id="Ch1.E2" content-type="numbered"><mml:math id="M20" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msup><mml:mi>k</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi>N</mml:mi><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where the <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represents the basal stress, <inline-formula><mml:math id="M22" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> represents
effective pressure, and <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represents magnitude of the basal
velocity.</p>
      <?pagebreak page883?><p id="d1e547">Since the drag coefficient (<inline-formula><mml:math id="M24" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>) derived using this methodology is
constrained to modern day, we adopt an approach based upon Hindmarsh and
LeMeur (2001) and Greve (2005) to construct a spatially varying temperature-dependent scaling parameter (<inline-formula><mml:math id="M25" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>) as a function of time.
            <disp-formula id="Ch1.E3" content-type="numbered"><mml:math id="M26" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi mathvariant="normal">b</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">modern</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi mathvariant="normal">b</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mo>/</mml:mo><mml:mi mathvariant="italic">α</mml:mi></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi mathvariant="normal">b</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">modern</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the basal temperature relative to pressure
melting derived from a thermal steady-state computation for modern day
(Seroussi et al., 2013), <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi mathvariant="normal">b</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the basal temperature
relative to pressure melting at time <inline-formula><mml:math id="M29" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M30" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> is a constant scaling
factor (<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) often referred to as the sub-melt parameter (Hindmarsh
and Le Meur, 2001). For these simulations <inline-formula><mml:math id="M32" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> is set equal to 5. This
number was chosen as it allows for a Last Glacial Maximum (LGM) GrIS simulated ice volume that is consistent with other ice sheet models that
restrict ice extent to only present-day land (Applegate et al., 2012;
Robinson et al., 2011). It is noted that values for this parameter lack a
theoretical basis (Hindmarsh and Le Meur, 2001) and are often set to a value
that prevents numerical instabilities from arising. Lastly, we scale the
spatially varying basal drag coefficient (<inline-formula><mml:math id="M33" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>) as a function of <inline-formula><mml:math id="M34" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>,
with maximum values capped at 300 to limit numerical instabilities that may
arise from unreasonably large numbers:
            <disp-formula id="Ch1.Ex1"><mml:math id="M35" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub><mml:mo movablelimits="false">min⁡</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mn mathvariant="normal">300</mml:mn><mml:mo>,</mml:mo><mml:msup><mml:mi>k</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfenced><mml:mi>N</mml:mi><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          For this approach, the basal stress (<inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) increases as the
basal temperatures decrease relative to present day, with virtually no
sliding occurring for high values of <inline-formula><mml:math id="M37" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>. Conversely, the basal stress
<inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> decreases as basal temperatures increase, with high sliding
for low values of <inline-formula><mml:math id="M39" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>. Lastly, the ice hardness, <inline-formula><mml:math id="M40" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula>, is temperature
dependent following the rate factors given in Cuffey and Paterson (2010,
p. 75). We initialize <inline-formula><mml:math id="M41" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> by solving for a present-day thermal steady state
(Cuzzone et al., 2018), while during forward runs <inline-formula><mml:math id="M42" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> evolves transiently
through time.</p>
</sec>
<sec id="Ch1.S2.SS5">
  <title>Experimental setup and boundary conditions for the regional domain</title>
      <p id="d1e804">We impose Dirichlet boundary conditions for the southern, northern, and ice divide boundaries, while the flux at the ice front in unconstrained. To
create the necessary transient boundary conditions (ice thickness,
temperature, and velocity), we perform a continental-scale GrIS simulation
from the LGM (21 500 years ago) to present day. This
continental-scale simulation uses the BP ice flow approximation and is
performed on a five-layer nonuniform mesh ranging in horizontal resolution from
3 km in areas of high present-day surface velocities to 20 km over the ice
interior. It is performed using forcings and parameterizations similar to the
regional model, as described in Sect. 2.3, 2.4, and 2.5.</p>
      <p id="d1e807">For the regional model, we initialize the model with present-day geometry and
run a relaxation centered at 12 000 years ago, applying the appropriate
interior ice boundary conditions of ice thickness, ice temperature, and the
<inline-formula><mml:math id="M43" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M44" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> component of ice velocity from the continental-scale GrIS
simulation. This time period is chosen as the ice margin over southwestern
Greenland was near or at the present-day coastline with the margin remaining
stable during this interval (Young and Briner, 2015). The relaxation
simulates 20 000 years until the ice volume is in equilibrium. From here, the models
are run transiently to present day. Since the ISSM currently does not have
the capability of modeling solid earth viscoelastic deformation transiently, we
include an offline time-dependent forcing that accounts for changes in
relative sea level from glacial isostatic adjustment (Caron et al., 2018),
which modifies the land area available for glaciation and impacts the
presence of floating ice. While grounding line migration is simulated in
these experiments, calving and submarine melting of floating ice are not
included.</p>
</sec>
<sec id="Ch1.S2.SS6">
  <title>Present-day thermal steady-state ice surface velocities</title>
      <p id="d1e830">The thermal steady-state ice surface velocities for the present day are shown for
each individual model (Fig. 3). Generally, representation of faster ice flow
along the coast improves with increasing resolution (i.e., increasing RMSE for
lower-resolution models compared to Rignot and Mouginot, 2012). This is
primarily attributed to an improved representation of subglacial topography
and ice thickness in the more highly resolved models (Aschwanden et al.,
2016). As many of the outlet glaciers along this margin have troughs that are
on the order of a few kilometers in width, the lower-resolution models (10
and 20 km) do not fully resolve the fast-flowing ice streams of Jakobshavn
Isbræ and outlets to its north. Outlet glaciers in the southern portion of
the domain near Kangiata Nunâta Sermia (KNS) are also less well resolved
in the lower-resolution models, although the general swath of higher
velocities is captured well for most fast-flowing areas of the ice sheet when
compared to the observations (Rignot and Mouginot, 2012). It is noted that
the nonuniform mesh represents these faster flow features best when compared
to observations in most regions due to its high resolution. Accordingly, the
associated mass flux at the ice margin is representative of these differences
in model resolution, with the 10 and 20 km models having an approximately
25 % increase in mass flux (GT yr<inline-formula><mml:math id="M45" 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 the observations, while the 5 km and nonuniform mesh have an
approximately 5 % to 9 % increase in mass flux compared to
observations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><label>Figure 3</label><caption><p id="d1e847">Present-day steady-state ice surface velocities for each individual
model and their differences from observations (Rignot and Mouginot, 2012, shown in
Fig. 1).</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019-f03.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>
<sec id="Ch1.S3.SS1">
  <?xmltex \opttitle{Relaxed state at 12\,ka}?><title>Relaxed state at 12 ka</title>
      <p id="d1e869">The models are relaxed for 20 000 years using a constant climate
corresponding to 12 ka (Fig. 4a). The four models simulate decreasing ice
volume with decreasing model resolution; the 20 km model simulates
approximately 6 % less total ice volume than the nonuniform model. Ice
surface velocities for the relaxed states (Fig. 5) depict the role of model
horizontal resolution in capturing fjords and narrow outlets close to the
model domain edge (i.e., present-day coastline). Generally, the two
higher-resolution models (nonuniform and 5 km) capture narrow, fast flow in
these outlets, whereas the lower-resolution models simulate a more diffuse
pattern in ice surface velocities. This is primarily the case in areas
where the bed topography is better resolved in the higher-resolution models
and, therefore, confines the flow to narrow outlets. Ice velocities are reduced
in the higher-resolution models for areas where the low bed topography that
channels ice flow is interrupted by bumps and depressions in the bed. These
features become less resolved in the lower-resolution models, with the 20 km
model simulating much higher ice surface velocities in the Nuuk and
Jakobshavn areas. Consistently, ice mass flux (in GT yr<inline-formula><mml:math id="M46" 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>) along the
ice front (at the present-day coastline) is 34 % and 14 % higher than
the nonuniform model for the 20 and 10 km model, respectively, which is the
primary driver for lower simulated ice volumes for the relaxed 12 ka state.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><label>Figure 4</label><caption><p id="d1e886"><bold>(a)</bold> Ice volume evolution for the 12 ka constant climate
relaxation. <bold>(b)</bold> Transient ice volume evolution for the simulations
from 12 ka to present day.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019-f04.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><label>Figure 5</label><caption><p id="d1e902">Relaxed ice surface velocities at 12 ka for each model and
differences from the nonuniform model.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019-f05.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
<?pagebreak page884?><sec id="Ch1.S3.SS2">
  <?xmltex \opttitle{Simulated ice volume (12\,ka to present day)}?><title>Simulated ice volume (12 ka to present day)</title>
      <p id="d1e920">The ice volume evolution for each model is shown in Fig. 4b. Generally, the
20 and 10 km models simulate the lowest present-day ice volumes, but they
also begin at 12 ka with lower ice volumes than the higher-resolution
models. Each model follows a similar trend, with ice volume loss occurring
between 12 and 1 ka, followed by an increase in ice volume to present day.</p>
</sec>
<?pagebreak page885?><sec id="Ch1.S3.SS3">
  <title>Large-scale simulated retreat</title>
      <p id="d1e929">Figure 6 shows the simulated extent at 11.2, 10.5, and 9.5 ka for each model
(middle and bottom row). All four models generally show ice retreat from the
coastline occurring between 11.5 and 11.2 ka in the northern portion of the
model domain, whereas the ice margin experiences little to no retreat farther
south. Despite differences in horizontal resolution, all models show a
similar magnitude and pattern of retreat, with higher-resolution models
depicting details in the ice margin similar in scale and sinuosity to the
mapped pattern of moraines (see Fig. 6a for mapped moraines). Similarity
between the magnitude and pattern of retreat also occurs at 10.5 and 9.5 ka amongst
all models. In contrast to the northern portion of the model domain, the
southern portion features a simulated retreat that varies widely based upon
model resolution. For example, at 10.5 ka the higher-resolution models
(5 km and nonuniform) exhibit little retreat from the coastline, whereas
the 10 and 20 km models show upwards of 50–60 km of retreat. Differences
in retreat between the higher- and lower-resolution models are further seen
at 9.5 ka. Over land-terminating portions in the southern area, the modeled
ice margin retreats similarly within all models; however, in the fjord
regions (e.g., inland of Nuuk), only the 10 and 20 km models show ice margin
retreat (of <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula>–70 km), whereas the higher-resolution models exhibit
no ice margin retreat.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><label>Figure 6</label><caption><p id="d1e944"><bold>(a)</bold> Mapped moraines and the existing chronology of ice
retreat over the northern and southern portion of our domain. The mapped
moraines and corresponding ages of retreat were taken from Lesnek and
Briner (2018). <bold>(b, c)</bold> Simulated ice sheet margin for the different
model resolutions shown over locations in the northern <bold>(b)</bold> and
southern <bold>(c)</bold> domain. The present-day ice thickness is shown, derived
from Morlighem et al. (2017) and Howat et al. (2014).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <?xmltex \opttitle{Simulated retreat (12\,ka to present day) -- along flow lines}?><title>Simulated retreat (12 ka to present day) – along flow lines</title>
      <p id="d1e971">To better illustrate simulated ice margin behavior through time, we analyze
ice retreat along five specific flow lines (A through E; Fig. 7) across the
domain. In Fig. 7, ice retreat along flow line A is shown for each model. All
models show a similar trend with the highest retreat rate (upwards of
50–100 m yr<inline-formula><mml:math id="M48" 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>) occurring between approximately 11.5 and 10 ka.
Between <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> ka and the present, all simulated ice margins generally
reside within 10 km of the present-day ice margin. The retreat history
simulated by the 10 and 20 km models exhibits a relatively stable ice margin
for much of this period, whereas the higher-resolution models (i.e.,
nonuniform and 5 km) depict an ice margin that is characterized by
higher-frequency variability on the order of 5–8 km. The retreat history
along flow lines B and C is consistent in timing and pattern to flow line A
(shown in Figs. S2 and S3).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><label>Figure 7</label><caption><p id="d1e998"><bold>(a)</bold> Simulated retreat along flow line A for each model.
<bold>(b)</bold> Ice surface profiles shown at 500-year intervals
(blue: older; green: younger; the red line indicates the simulated
present-day ice surface profile), with the underlying bed topography (filled black
area). The red tick mark on the <inline-formula><mml:math id="M50" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis denotes the present-day ice margin
(Howat et al., 2014). Readers should refer to this figure for locations of
flow lines used in this study.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019-f07.png"/>

        </fig>

      <?pagebreak page887?><p id="d1e1019">Differences in the bed topography between the four models reflect model
resolution, with higher-resolution models capturing topography closer to
reality (Fig. 7). Nevertheless, the bed topography along the flow line A is
similar among the different models owing to the low-relief topography in this
region. The low-angle ice surface responds to surface melt similarly among
the four models along flow line A (see Fig. S2 for surface temperature and SMB
along flow lines) and is likely why the retreat history is similar. Along
flow line B (Fig. S3), bed topography in all models exhibits increasing
elevation into the ice sheet interior. Whereas the nonuniform and 5 km
models capture a trough between 30 and 120 km along the flow line, this
feature is subtle in the 10 km model and nonexistent in the 20 km model.
Similar to flow line A, however, the simulated retreat in flow line B is
similar amongst the different models both in rate and magnitude of retreat.
Generally, the ice margins exhibit retreat forced primarily through surface
lowering in response to negative SMB (Fig. S2) because the ice margin
retreats similarly through areas of varying bed topography. At approximately
150 km along the flow line, the ice retreats into an area with higher bed
topography, and the ice surface profiles become steeper, thereby raising the
equilibrium line altitude (ELA) and stabilizing the ice margin. Along flow line C (Fig. S4), the bed
topography for the nonuniform and 5 km model is characterized by low
elevations at the beginning and end of the flow line, with a peak in elevation
in the middle, while the 10 and 20 km models exhibit a more consistent bed
elevation along the flow line. The upward slope of the bed for the nonuniform
and 5 km model tends to slow the retreat of the ice margin along flow line C
during the early Holocene, although differences between the 10 and 20 km
models are not dramatic. After 8 ka, ice retreat stabilizes in all models,
similar to flow lines A and B, although the nonuniform and 5 km models
exhibit marginal ice fluctuations on the order of 5–8 km.</p>
      <p id="d1e1023">In the southern portion of the domain, the fjords within the Nuuk region
dominate the landscape. The ice margin in flow line D (Fig. 8) remains fixed
for the entire simulation in the nonuniform and 5 km model simulations. In
contrast, both the 10 and 20 km models depict retreat at <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">9.5</mml:mn></mml:mrow></mml:math></inline-formula> ka,
after which the 10 km model quickly stabilizes and the 20 km model exhibits
variability up to present day. All models fail to simulate a present-day ice
margin that comes close to today's observed ice margin (Fig. 8). The
lower-resolution models simulate retreat in this region on the order of 30 to
50 km, which is controlled primarily by the bed topography. In reality, a
trough extends much of the distance along this flow line, which is captured
well by both the nonuniform and 5 km mesh, where depths reach <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">500</mml:mn></mml:mrow></mml:math></inline-formula> m
below sea level. Consequently, the nonuniform and 5 km models are better
able to capture the stress balance and mass transport, as they simulate more
realistic ice flow and delivery of ice mass to the margin in this region. In
the 10 km model, surface lowering intersects a bed bump that is above sea
level at approximately 40 km along flow line D. Inland of this rise in the bed, the 10 km
model bed contains a shallow trough, which is capable of sustaining the ice
margin throughout the remainder of the simulation. The 20 km model lacks any
clear trough and instead captures a significant rise in the bed topography at
70 km along the flow line, where the other models resolve a trough. As the
ice surface lowers along flow line D, it becomes increasingly influenced by
this bed feature. Due to the upward slope and horizontal top of this bed
feature, the margin varies in response to the high-frequency climate
variability during the Holocene (Fig. S2).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><label>Figure 8</label><caption><p id="d1e1048">Same as in Fig. 7 but for flow line D.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://tc.copernicus.org/articles/13/879/2019/tc-13-879-2019-f08.png"/>

        </fig>

      <p id="d1e1057">Flow line E (Fig. S5) follows a narrow and shallow trough south of flow line D.
This shallow trough is only captured completely in the nonuniform model,
although the 5 km model captures low topography along the ice margin. In the
10 and 20 km models there is no indication of a trough and instead the bed
topography is high and generally flat. Similar to flow line D, downwasting via
negative SMB (Fig. S2) drives ice retreat in the 10 and 20 km models.
Because the nonuniform mesh captures a trough along flow line E, delivery of
ice mass to the margin continues through the Holocene, stabilizing the ice
margin position despite surface lowering through negative SMB.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>Discussion</title>
      <p id="d1e1067">We find that model resolution plays a negligible role in the simulated ice
margin history in the northern portion of our domain along flow lines A, B,
and C. In the southern domain along flow lines D and E, however, model
resolution plays a large role in the simulated ice margin history.</p>
<sec id="Ch1.S4.SS1">
  <title>Retreat within the northern domain</title>
      <p id="d1e1075">In the northern portion of our model domain, geologic archives indicate
retreat from the coast occurred between 12 and 11 ka (Kelly et al., 2015;
Young and Briner, 2015; Fig. 6a), which is generally consistent with our
simulations regardless of resolution. The subsequent retreat in all models
towards the present-day ice margin is also generally consistent with the
geologic reconstructions of ice margin retreat in this region (Fig. 6b and
c). Van Tatenhove et al. (1996) provide one of the earliest ice sheet model–data comparisons for this region (around flow line C) during the last
deglaciation. Van Tatenhove et al. (1996) compared three different ice sheet
models ranging in resolution from 20 to 40 km to ice margin reconstructions
constrained by radiocarbon ages from the region and indicated that model
resolution played little role in the inter-model retreat differences. Van
Tatenhove et al. (1996) pointed to the strong governing role of SMB in this
region with little influence from ice streams. Likewise, simulations from the
20 km resolution model of Lecavalier et al. (2014) show reasonable agreement
in the retreat across this region when compared to geologic reconstructions.
Our results indicate that the bed topography in this region is well
represented among the different models, despite their differences in
resolution, and thus simulated ice margin history faithfully responds to SMB
forcing and is not complicated by ice flow adjustments to underlying
topography. However, one feature that stands out in the higher-resolution
models<?pagebreak page888?> (5 km and nonuniform) is the presence of high-frequency ice marginal
fluctuations on the order of 5–8 km (Figs. 7, S3, S4). The geologic record
indicates that small-scale marginal fluctuations are likely responsible for
the moraine record and seem to be related to high-frequency variability in
temperature (e.g., Young et al., 2013). Thus, models capable of capturing
small-scale fluctuations in the ice margin history are valuable for comparing
with geologic constraints of past ice sheet change. The inability of
lower-resolution models to capture these features has been highlighted in
previous work (Van Tatenhove et al., 1996; Larsen et al., 2015) and hampers
data–model comparisons.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <title>Retreat within the southern domain</title>
      <p id="d1e1084">In the southern portion of the model domain, fjord systems provide a
different bed setting than in the north, presenting a significant challenge
for modeling ice margin change. Deep and narrow troughs up to 500 m below
sea level and 3–5 km wide seemingly played an important role in governing
ice margin retreat. Many geologic archives that constrain past ice margin
variability in this region (Sinclair et al., 2016) reveal rapid deglaciation
from the present-day coastline to near the present-day margin at <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> ka (e.g., Larsen et al., 2014; Fig. 6a). None of our experiments match
the geologic observations.</p>
      <p id="d1e1097">Our simulated ice retreat is highly dependent on model resolution in this
area because the different models represent the bed topography quite
differently. For example, only the nonuniform and 5 km models capture the
deep fjords, whereas the 10 and 20 km models have unrealistic bed features
that end up driving retreat (Figs. 8 and S5). Our simulations do not include
calving or submarine melting, and, therefore, each model's simulated ice
surface responds similarly to negative SMB. However, the ability of the
high-resolution models to resolve the narrow and deep fjords allows the ice
margin to persist, as the stress balance and mass transport is well captured.
Since the fjords are not well represented in the low-resolution models, there
is lower delivery of ice mass to the margin, and the simulated retreat is
driven as the ice surface lowers and intersects elevated bump artifacts in
the bed topography. While none of the models capture the timing or amount of
retreat accurately, the high-resolution models in this case perform the
worst, capturing negligible retreat. The rapid ice margin recession recorded
by the geologic reconstructions in this marine-dominated region probably
highlight the influence of calving and enhanced submarine melting of floating
ice, neither of which are included in our model simulations. The lack of
submarine melting, in particular, may lead to the model–data mismatch;
available evidence (e.g., Dyke et al., 2014) supports influence of the
warm Irminger Current during the early Holocene, which likely penetrated
fjords up to the ice margin.</p>
</sec>
<?pagebreak page889?><sec id="Ch1.S4.SS3">
  <title>Different drivers of retreat</title>
      <p id="d1e1106">There are stark differences in processes affecting retreat of the
land-dominated ice margin (i.e., SMB in the northern section of the model
domain) and the marine-dominated ice margin (i.e., calving and submarine melt
in the southern portion of the domain). These different drivers of ice
margin change also affect different sectors of the contemporary GrIS (Sole
et al., 2008; Straneo and Heimbach, 2013). Our results highlight that in
areas of simple, low-relief bed topography, SMB drives the simulated retreat
with few differences existing between models of varying spatial
resolution. Therefore, efforts that attempt to match geologic
reconstructions will be better served by focusing on representing SMB as
accurately as possible. Conversely, in areas with complex, high-relief bed
topography, such as in fjord settings, models that are unable to capture the
deep and narrow troughs may unreasonably simulate retreat (see Åkesson
et al., 2018). Anisotropic mesh capabilities play an important role in
allowing a model to adjust its resolution spatially while using computer
time efficiently.</p>
      <p id="d1e1109">For low-resolution models, care must be taken when attempting to capture the
reconstructed retreat in areas of complex bed topography. For example, in
order to satisfy relative sea level records used to constrain an ice sheet
model of the GrIS, Lecavalier at al. (2014) artificially increased middle
Holocene temperatures used to drive the ice sheet model. Although this
resulted in a simulated ice margin history consistent with available geologic
records, it is noted that such external forcings may drive unphysical retreat
in areas of complex bed topography that may otherwise have been driven by ice
dynamics. Another consideration is the regional setting presented here. Since
these experiments are focused on the southwestern GrIS, an area that may be
relatively topographically uniform, we expect the results of the
marine-influenced region in the southern part of our domain to be most
relevant for other portions of the GrIS, in particular in eastern Greenland
where fjords dominate the landscape (Morlighem et al., 2017).</p>
</sec>
<sec id="Ch1.S4.SS4">
  <title>Model limitations</title>
      <p id="d1e1119">When simulating the retreat of the southwestern GrIS, our choice of climate
forcing, using the GRIP <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> record (Dansgaard et al., 1993),
follows what has been a cornerstone in forcing Greenland ice sheet modeling
over the paleoclimate record (Huybrechts, 2002; Greve et al., 2011; Applegate et
al., 2012). This approach has been adjusted in Tarasov and Peltier (2002),
Simpson et al. (2009) and Lecavalier et al. (2014) by synthetically
increasing Holocene temperatures, with more recent simulations of the
deglaciation of Greenland making use of more recent
temperature proxy
reconstructions that are better constrained throughout Greenland (Lecavalier
et al., 2017; Buizert et al., 2018). Nevertheless, using a single, scaled
paleoclimate record from Summit ignores the more likely history of a
spatiotemporally variable climate history spanning the Holocene around
Greenland (cf. Vinther et al., 2009). In any case, since the traditional
approach (i.e., the GRIP <inline-formula><mml:math id="M55" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> scaling) assumes that the spatial
variability in temperature and seasonality remains fixed to modern day, our
results cannot fully reconcile how changes in the magnitude of warming and
spatial variation of that warming affects our results. Additionally, the
scaling of the basal friction coefficient introduces some uncertainties
particularly when considering the temperature forcing throughout the
simulation. Our method for scaling the basal friction coefficient through
time follows a common approach used in many modeling studies over
paleoclimate timescales (Hindmarsh and LeMeur, 2001; Greve ,2005). For these
simulations, the evolution of the basal temperatures through time depends on
the surface temperature forcing which is derived from the GRIP <inline-formula><mml:math id="M56" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> scaling. Therefore, changes to the surface temperature forcing can
impact the evolution of the basal temperatures over time, which ultimately
affects the ice sliding following this approach. This model limitation falls
within the bounds of current ice sheet modeling efforts, whereby a lack of
physically based basal sliding parameterizations exist. Despite this
limitation, the conclusions presented here remain unaffected.</p>
      <p id="d1e1161">Although these simulations have no reasonable representation of calving, the
results do indicate that models with a resolution of 10 km or greater would
be likely unable to address calving processes in fjords, as typical fjord
width is <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> km. In ice sheet models, calving is often related to water
depth, considering past changes in eustatic and relative sea level
(Huybrechts, 2002; Simpson et al., 2009; Lecavalier et al., 2014). Although
the high-resolution models presented here do capture the narrow fjords,
implementation of a calving scheme would currently be computationally
intensive. One possibility for future work would be to force the model with
high submarine basal melt rates as a proxy for calving, as done in
Åkesson et al. (2018). Submarine melt has been shown to be an important
mechanism driving both contemporary ice mass loss (Rignot, 2010) and past
GrIS variability on glacial and interglacial timescales (Bradley et al., 2018;
Tabone et al., 2018). Although few constraints do exist detailing past
variations in ocean temperature for the Labrador Sea (Winsor et al., 2012; Gibb et al., 2015) and
Disko Bay (Jennings et al., 2006), applying submarine melt rates to marine
termini throughout our model domain would not be possible without significant
uncertainty. Additionally, in applying basal melting to floating ice, it is
uncertain whether 2 km resolution would be sufficient to accurately capture
grounding line migration, as recent research (Seroussi and Morlighem, 2018)
suggests that resolutions of 1 km or higher are often necessary to match
present-day fluctuations.</p>
</sec>
</sec>
<?pagebreak page890?><sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e1182">We investigated how ice sheet model resolution influences the simulated
Holocene retreat of the southwestern GrIS using the ISSM. Our focus on the
southwestern GrIS is driven by two factors: first, the regional approach
allowed for modeling at a high resolution (for the nonuniform and 5 km
mesh) while minimizing computational costs that would increase significantly
while running a GrIS-wide simulation. Second, the southwestern GrIS is an
area where geologic archives indicate the ice sheet underwent large-scale and
relatively well-known retreat during the Holocene.</p>
      <p id="d1e1185">The results presented here indicate that model resolution has a selective
influence in the simulated retreat over southwestern Greenland during the
Holocene. In areas where the bed topography is relatively simple, low-relief,
and free from marine influence, model resolution plays an insignificant role
in influencing the pattern and rate of retreat. Here, models with different
resolutions respond similarly to SMB-driven retreat. On the
other hand, in areas with complex and high-relief bed topography, such as
deep troughs and fjords, the low-resolution models lead to unrealistic
retreat. As all models in these simulations only respond to surface melt and,
therefore, ice surface lowering (and no mass loss via calving or submarine
melt), the low-resolution models (10 and 20 km) simulate ice retreat driven
purely as a consequence of incorrectly capturing the bed geometry. As one
example, ice surface lowering in these models intersects bed bumps that would
otherwise be resolved as a trough in higher-resolution models.</p>
      <p id="d1e1188">Our results imply that computational resources can be saved when modeling
certain portions of the GrIS. Conversely, the results also highlight the
importance of model resolution in areas of complex topography. Ice sheet
models using a nonuniform mesh can adapt grids to fit these constraints
while using computation time efficiently. However, for models using uniform
fine-scale meshing, resolving such features becomes computationally
difficult, especially over long paleoclimate timescales. As ice sheet models
sometimes rely on the geologic record for validation, care must be taken in
evaluating model–data misfits. In areas of complex topography, over-tuning
of model parameters or climatology may occur in low-resolution models that
seek to match the reconstructed margin. We suggest that increased model
resolution is critical in regions dominated by fjords (e.g., southeastern
Greenland).</p>
      <p id="d1e1191">Future work with the ISSM will focus on using a model that has a lower resolution
in areas driven mainly by SMB and a higher resolution in areas influenced by
dynamical ice processes using nonuniform mesh capabilities. Future work
will also seek to evaluate the sensitivity of using improved climate
forcings (Hakim et al., 2016; Buizert et al., 2018), better representations
of ice dynamics (calving and submarine melt), and more quantitative
comparisons to improved ice margin reconstructions.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e1198">The simulations performed for this paper made use of the open-source Ice Sheet System Model (ISSM) and are publicly
available at  <uri>https://issm.jpl.nasa.gov/</uri> (last access: 14 February 2019, Larour et al., 2012).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e1204">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/tc-13-879-2019-supplement" xlink:title="pdf">https://doi.org/10.5194/tc-13-879-2019-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1213">All authors contributed to the discussion of the results in this paper. JKC led the numerical modeling carried out in this paper,
with help from NJS and MM.  JKC, NJS, and MM designed the experiments presented in this paper.  NJS and JKC led the development of the friction scaling
implemented in these simulations.  MM, HS, and JKC led the development and implementation of the higher-order finite elements used in the thermal
modeling for these simulations.  JKC and JPB led comparison of the simulated margin history with the geologic record of past margin migration.
LC provided output constraining past relative sea level variations.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1219">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1225">Funding for this study was provided by the National Science Foundation Grant
ARC no. 1504230. We would like to thank Surendra Adhikari and Mark Richardson
for their helpful discussion and Alia Lesnek for providing the geologic data
constraining past ice history. Lastly, we thank Andreas Vieli and the two reviewers, Alexander Robinson and Julien Seguinot for their constructive feedback regarding this work.
<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by: Andreas Vieli <?xmltex \hack{\newline}?>
Reviewed by: Alexander Robinson and Julien Seguinot</p></ack><ref-list>
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    <!--<article-title-html>The impact of model resolution on the simulated Holocene retreat of the southwestern Greenland ice sheet using the Ice Sheet System Model (ISSM)</article-title-html>
<abstract-html><p>Geologic archives constraining the variability of the Greenland
ice sheet (GrIS) during the Holocene provide targets for ice sheet models to
test sensitivities to variations in past climate and model formulation. Even
as data–model comparisons are becoming more common, many models simulating
the behavior of the GrIS during the past rely on meshes with coarse
horizontal resolutions ( ≥ 10&thinsp;km). In this study, we explore the impact of
model resolution on the simulated nature of retreat across southwestern
Greenland during the Holocene. Four simulations are performed using the Ice
Sheet System Model (ISSM): three that use a uniform mesh and horizontal mesh
resolutions of 20, 10, and 5&thinsp;km, and one that uses a nonuniform mesh with
a resolution ranging from 2 to 15&thinsp;km. We find that the simulated retreat can
vary significantly between models with different horizontal resolutions based
on how well the bed topography is resolved. In areas of low topographic
relief, the horizontal resolution plays a negligible role in simulated
differences in retreat, with each model instead responding similarly to
retreat driven by surface mass balance (SMB). Conversely, in areas where the bed
topography is complex and high in relief, such as fjords, the lower-resolution models (10 and 20&thinsp;km) simulate unrealistic retreat that occurs as
ice surface lowering intersects bumps in the bed topography that would
otherwise be resolved as troughs using the higher-resolution grids. Our
results highlight the important role that high-resolution grids play in
simulating retreat in areas of complex bed topography, but also suggest that
models using nonuniform grids can save computational resources through
coarsening the mesh in areas of noncomplex bed topography where the SMB
predominantly drives retreat. Additionally, these results emphasize that care
must be taken with ice sheet models when tuning model parameters to match
reconstructed margins, particularly for lower-resolution models in regions
where complex bed topography is poorly resolved.</p></abstract-html>
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