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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">CP</journal-id><journal-title-group>
    <journal-title>Climate of the Past</journal-title>
    <abbrev-journal-title abbrev-type="publisher">CP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Clim. Past</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1814-9332</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/cp-14-1119-2018</article-id><title-group><article-title>Testing the consistency between changes in simulated climate and Alpine
glacier length over the past millennium</article-title><alt-title>Simulated Alpine glacier length over the past millennium</alt-title>
      </title-group><?xmltex \runningtitle{Simulated Alpine glacier length over the past millennium}?><?xmltex \runningauthor{H.~Goosse et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Goosse</surname><given-names>Hugues</given-names></name>
          <email>hugues.goosse@uclouvain.be</email>
        <ext-link>https://orcid.org/0000-0002-5438-3612</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Barriat</surname><given-names>Pierre-Yves</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Dalaiden</surname><given-names>Quentin</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Klein</surname><given-names>François</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Marzeion</surname><given-names>Ben</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6185-3539</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Maussion</surname><given-names>Fabien</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3211-506X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Pelucchi</surname><given-names>Paolo</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff6">
          <name><surname>Vlug</surname><given-names>Anouk</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3347-3547</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Earth and Life Institute, Université catholique de Louvain,
Louvain-la-Neuve, Belgium</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Institut für Geographie, Universität Bremen, Bremen, Germany</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>MARUM – Center for Marine Environmental Sciences, University of
Bremen, Bremen, Germany</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of Atmospheric and Cryospheric Sciences, Universität
Innsbruck, Innsbruck, Austria</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Imperial College, London, UK</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Faculty of Geosciences, University of Bremen, Bremen, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Hugues Goosse (hugues.goosse@uclouvain.be)</corresp></author-notes><pub-date><day>9</day><month>August</month><year>2018</year></pub-date>
      
      <volume>14</volume>
      <issue>8</issue>
      <fpage>1119</fpage><lpage>1133</lpage>
      <history>
        <date date-type="received"><day>23</day><month>April</month><year>2018</year></date>
           <date date-type="rev-request"><day>4</day><month>May</month><year>2018</year></date>
           <date date-type="accepted"><day>10</day><month>July</month><year>2018</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2018 Hugues Goosse et al.</copyright-statement>
        <copyright-year>2018</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://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018.html">This article is available from https://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018.html</self-uri><self-uri xlink:href="https://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018.pdf">The full text article is available as a PDF file from https://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e176">It is standard to compare climate model results covering
the past millennium and reconstructions based on various archives in order
to test the ability of models to reproduce the observed climate variability.
Up to now, glacier length fluctuations have not been used systematically in
this framework even though they offer information on multi-decadal to
centennial variations complementary to other records. One reason is that
glacier length depends on several complex factors and so cannot be directly
linked to the simulated climate. However, climate model skill can be
measured by comparing the glacier length computed by a glacier model driven
by simulated temperature and precipitation to observed glacier length
variations. This is done here using the version 1.0 of the Open Global Glacier
Model (OGGM) forced by fields derived from a range of simulations performed
with global climate models over the past millennium. The glacier model is
applied to a set of Alpine glaciers for which observations cover at least
the 20th century. The observed glacier length fluctuations are
generally well within the range of the simulations driven by the various
climate model results, showing a general consistency with this ensemble of
simulations. Sensitivity experiments indicate that the results are much more
sensitive to the simulated climate than to OGGM parameters. This confirms
that the simulations of glacier length can be used to evaluate the climate
model performance, in particular the simulated summer temperatures that
largely control the glacier changes in our region of interest. Simulated
glacier length is strongly influenced by the internal variability in the
system, putting limitations on the model–data comparison for some variables
like the trends over the 20th century in the Alps. Nevertheless,
comparison of glacier length fluctuations on longer timescales, for instance
between the 18th century and the late 20th century, appear less
influenced by the natural variability and indicate clear differences in the
behaviour of the various climate models.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e186">As it offers a longer perspective compared to the so-called instrumental
period (from roughly 1850 CE to present), the past millennium is a key
period to study decadal to centennial climate variations. The syntheses of
the available climate records indicate a general temperature decrease from
the beginning of the second millennium to the beginning of the 19th
century, followed by a large warming over the 20th century (Jones et
al., 2009; Mann et al., 2009; PAGES 2k Consortium, 2013, 2017; Neukom et al.,
2014). Nevertheless, the spatio-temporal structure
of the temperature changes is complex, with warm and cold periods being
generally not synchronous between different regions (PAGES 2k Consortium,
2013). Those conclusions are in overall agreement with the results derived
from global climate models driven by estimates of natural and anthropogenic
forcings, although<?pagebreak page1120?> models tend to underestimate the magnitude of the changes
in some regions and to simulate more homogenous changes than in the
reconstructions (Goosse et al., 2005; Raibble et al., 2006; Gonzalez-Rouco
et al., 2006; Jungclaus et al., 2010; Phipps et al., 2013;
Fernández-Donado et al., 2013; Landrum et al., 2013; Neukom et al.,
2014; Moberg et al., 2015; PAGES2k-PMIP, 2015; Otto-Bliesner et al., 2016).</p>
      <p id="d1e189">The data syntheses covering the past millennium are based on many different
archives such as trees, corals, glacier ice, lake sediments, pollen,
speleothems and marine sediments. They generally do not include glacier
length fluctuations, although the latter can be used for independent tests
of reconstructed changes (Guiot et al., 2010; Luterbacher et al., 2016).
Glaciers are complex recorders of past conditions. Their fluctuations depend
on the surface mass balance, which is influenced by several factors, including temperature, precipitation and incoming radiation changes over the
glacier, as well as by the glacier dynamics and thus local geometry
(Oerlemans, 2001; Huss et al., 2008; Roe, 2011). Furthermore, because of
their long response time, glaciers integrate forcing over periods ranging
from a few years to several decades or even centuries (e.g. Jòhannesson
et al., 1989; Leysinger Vieli and Gudmundsson, 2004). Consequently, glacier
length fluctuations cannot be directly compared to records with a much
faster response or simply included in multi-proxy reconstructions of past
climate changes (Oerlemans, 2005; Roe, 2011; Solomina et al., 2016; Roe et
al., 2017).</p>
      <p id="d1e192">Despite these difficulties, it is possible to estimate the temperature and
precipitation variations that were at the origin of glacier length
fluctuations (Mackintosh et al., 2017). One method is to drive a glacier
model with a range of climate conditions to determine the ones that are
compatible with the glacier length records (Allison and Kruss, 1977;
Oerlemans, 1986; Jomelli et al., 2011; Leclercq et al., 2012; Luthi, 2014;
Malone et al., 2015; Sagredo et al., 2017; Zechetto et al., 2017; Doughty et
al., 2017). The temperature and precipitation reconstructions deduced from
glacier length fluctuations can also be compared to estimates obtained from
other records and climate model results to test the compatibility between
the different sources of information. At a large scale, temperature
reconstructions have been obtained using simple glacier models in inverse
mode (Oerlemans, 2005; Leclercq and Oerlemans, 2012), assuming that the
selected glaciers are mainly influenced by temperature. However, the
inversion required to obtain a temperature or a precipitation reconstruction
from observations can be ill-conditioned if the record is influenced by
several environmental factors, as is the case for glacier length. It thus
might be very difficult to disentangle, for instance, the contribution of
changes in precipitation and temperature, leading to large uncertainties or
biases in the reconstructed signal (Evans et al., 2013; Leclercq and
Oerlemans, 2012; Mackintosh et al., 2017).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><label>Table 1</label><caption><p id="d1e198">Climate model simulations used to drive OGGM.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="85.358268pt"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="56.905512pt"/>
     <oasis:colspec colnum="4" colname="col4" align="justify" colwidth="85.358268pt"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Name</oasis:entry>
         <oasis:entry colname="col2">Institution</oasis:entry>
         <oasis:entry colname="col3">Resolution in <?xmltex \hack{\hfill\break}?>the atmosphere (lat <inline-formula><mml:math id="M1" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> long)</oasis:entry>
         <oasis:entry colname="col4">Reference</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CCSM4</oasis:entry>
         <oasis:entry colname="col2">National Center for Atmospheric Research</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mn mathvariant="normal">192</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">288</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">Gent et al. (2011)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">National Center for Atmospheric Research</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:mn mathvariant="normal">96</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">144</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">Otto-Bliesner et<?xmltex \hack{\hfill\break}?>al. (2016)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">NASA Goddard Institute for Space Studies</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:mn mathvariant="normal">90</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">144</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">Schmidt et al. (2014)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">IPSL-CM5A-LR</oasis:entry>
         <oasis:entry colname="col2">Institut Pierre-Simon-<?xmltex \hack{\hfill\break}?>Laplace</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mn mathvariant="normal">96</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">96</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">Dufresne et al. (2013)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MPI-ESM-P</oasis:entry>
         <oasis:entry colname="col2">Max Planck Institute<?xmltex \hack{\hfill\break}?>for Meteorology</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:mn mathvariant="normal">96</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">192</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">Stevens et al. (2013)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">BCC-CSM1-1</oasis:entry>
         <oasis:entry colname="col2">Beijing Climate Center, China Meteorological Administration</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mn mathvariant="normal">64</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">128</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">Wu et al. (2014)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e403">An alternative method is to drive a glacier model directly with climate
model results and compare the simulated length with the observed one. A
similar approach, in which a proxy system model has been applied to simulate
directly the observed quantity, has been successfully applied to a wide
variety of variables such as tree ring widths, coral or speleothem composition (Evans et al., 2013; Dee et al., 2015). The advantages are that
the comparison is made on exactly the same variable for models and
observations and that the problems related to an inversion are avoided.
Until now, comparisons of climate model results with glacier length over the
past millennium and the Holocene have been rare and the few existing studies
were focused on a small number of glaciers (Weber and Oerlemans, 2003;
Leclerq et al., 2012). This limits the ability to assess the climate model
performance from glacier length records and the analysis of the origin of
observed glacier changes using climate model results.</p>
      <p id="d1e406">In addition to the simulated climate, the quality of the comparison between
modelled and observed glacier lengths depends on several factors that need
to be addressed. First, glacier models have their own limitations (Huss and
Hock, 2015; Maussion et al., 2018) and some of the disagreements between
simulated results and observations might be attributed to the glacier model
and its initial/boundary conditions (e.g. Farinotti et al., 2017) rather
than to the climate model. An additional source of uncertainty is related to
the internal variability in the climate, which can be dominant at a regional
scale for the past millennium (Goosse et al., 2005, 2012a; Jungclaus et al., 2010; Otto-Bliesner et al., 2016). As the climate
fluctuations are integrated by the glaciers, this induces glaciers length
changes reaching potentially several hundreds of metres (Oerlemans, 2000;
Roe et al., 2009; Roe and O'Neal, 2009; Barth et al., 2017).</p>
      <p id="d1e409">Our goal here is to perform a systematic evaluation of climate model behaviour by using the outputs of simulations covering the past millennium to
force a global glacier model (Maussion et al., 2018). The main objective is
to provide a new validation procedure for climate models complementary to
the existing ones. Specifically, we will estimate the compatibility of the
simulated multi-decadal to centennial-scale climate variability with glacier
length records, analysing the links between glacier fluctuations and
temperature changes. This implies an estimation of the sources of
uncertainty associated with glacier modelling and of the contribution of
internal variability to simulated changes. Additionally, the comparison will
provide a test of our ability to reproduce past glacier variations using
tools that are similar to the ones applied to estimate future changes in
glaciers and their contribution to sea level rise (e.g. Marzeion et al.,
2012, 2018; Gregory et al., 2013; Bliss et al., 2014; Huss and Hock, 2015; Slangen
et al., 2016). The initial focus here is on European
glaciers and more specifically on the Alps because of the availability of
records that are long enough for our analyses.</p>
      <p id="d1e412">The climate model results, the glacier model and the glacier length
observations are described in Sect. 2. The results of the glacier model
driven by a range of climate models are compared with observations in
Sect. 3. This includes a<?pagebreak page1121?> discussion of the contribution of internal
variability to glacier fluctuations and its impact on the conclusion of
a model–data comparison. The sensitivity of the results to key parameters of
the glacier model and to the experimental set-up are discussed in Sect. 4.
Final conclusions are proposed in Sect. 5.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
<sec id="Ch1.S2.SS1">
  <title>Climate model results</title>
      <p id="d1e426">The climate variables used to drive the glacier model are derived from
simulations following the Past Model Intercomparison Project (PMIP3) and the
Coupled Model Intercomparison Project (CMIP5) protocols (Schmidt et al.,
2011; Taylor et al., 2012; PAGES2k-PMIP3, 2015). They were downloaded from
the Program for Climate Model Diagnosis and Intercomparison (PCMDI;
<uri>http://pcmdi9.llnl.gov</uri>; last access: 15 November 2017) and the Earth
System Grid (<uri>https://www.earthsystemgrid.org/</uri>; last access:
15 November 2017) archives. We have selected the same simulations as in Klein
et al. (2016) (Table 1). Some of these simulations do not transition
continuously in 1850 from the experiments referred to as “past1000” in
CMIP/PMIP nomenclature (years 851–1850) to the “historical” (years
1851–2005) simulations. Because of this discontinuity associated with the experiment design, a jump
can be present on the simulated variables in 1850, but it is relatively small
for the selected experiments so they can be merged with a limited impact on
the results. Those simulations are driven by natural (orbital, solar,
volcanic) and anthropogenic (greenhouse gas, ozone, aerosol, land use)
forcings (Schmidt et al., 2011, 2012). Nevertheless, the simulations
performed with BCC-CSM1-1 and IPSL-CM5A-LR (for model abbreviations, please
see Table 1) do not include
land-use forcing. Additionally, the aerosol forcing is not activated in the
IPSL-CM5A-LR simulation. One simulation for CCSM4, GISS-E2-R, IPSL-CM5A-LR, MPI-ESM-P and
BCC-CSM1-1 and an ensemble of 10 simulations with CESM1 are used here. More
details about the simulations and the forcing applied in each of them can be
obtained in Klein et al. (2016) and PAGES2k-PMIP3 (2015).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>The Open Global Glacier Model</title>
      <p id="d1e441">The Open Global Glacier Model (OGGM; Maussion et al., 2018) is an open-source model that simulates the evolution of individual glaciers, explicitly
accounting for glacier geometry, even in complex configurations involving
contributory branches. The first step is to describe the glacier outlines
and topography from global public databases: the RGI version 5 (RGI
Consortium, 2015) and SRTM topography data version 4 (Jarvis et al., 2008).
The glacier main branches, tributaries and flow lines are then defined, and
the glacier ice thickness is estimated by solving the equations of ice flow and
mass conservation along the flow line.</p>
      <?pagebreak page1122?><p id="d1e444">The mass balance is computed from the equation (Marzeion et al., 2012):
            <disp-formula id="Ch1.E1" content-type="numbered"><mml:math id="M8" display="block"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:msubsup><mml:mi>P</mml:mi><mml:mi>i</mml:mi><mml:mi mathvariant="normal">solid</mml:mi></mml:msubsup><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>⋅</mml:mo><mml:mo movablelimits="false">max⁡</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">melt</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi mathvariant="italic">ε</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the mass balance of month <inline-formula><mml:math id="M10" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> at the altitude <inline-formula><mml:math id="M11" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>.
<inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msubsup><mml:mi>P</mml:mi><mml:mi>i</mml:mi><mml:mi mathvariant="normal">solid</mml:mi></mml:msubsup><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the monthly solid precipitation, and <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the
monthly mean temperature. The amount of solid precipitation is derived from
the total amount of precipitation assuming that precipitation is entirely
solid below 0 <inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, entirely liquid above 2 <inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and the
fraction of solid precipitation varies linearly with temperature between
those two values. <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a correction factor included to take into
account the larger precipitation over the glaciers than in the surrounding
terrain and at lower altitudes where observations are available. Its value
is constant for all the glaciers and is taken to be equal to 2.5 (e.g. Giesen and
Oerlemans, 2012). Melting occurs if monthly temperature is above
<inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">melt</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which is equal to <inline-formula><mml:math id="M18" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1 <inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in OGGM, as melting may occur
some days even though the monthly mean is below 0 <inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. This value
has been selected on the basis of a cross-validation procedure similar to
the one conducted by Marzeion et al. (2012). <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> is the temperature
sensitivity parameter, and <inline-formula><mml:math id="M22" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> a residual bias. <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and  <inline-formula><mml:math id="M24" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> are estimated first for glaciers where mass balance observations are
available and then extrapolated to the other glaciers following a procedure
described in Marzeion et al. (2012) and Maussion et al. (2018).</p>
      <p id="d1e699">The ice dynamics is based on the shallow-ice approximation and is computed
along the flow line. In the shallow-ice approximation, the vertical
variations in ice flow are neglected and only a depth-integrated ice
velocity is computed. This is a common approximation for computationally
efficient ice flow models, and it is largely valid as long as the considered
horizontal scales are much larger than the vertical scales (Hutter, 1981,
1983). Basal sliding is also neglected here. For the prefrontal areas, the
direction and path of ice flow are obtained by computing the route from the
glacier tongue toward the end of the domain that is the least costly in
terms of positive altitudinal change. The flow line therefore follows the
valley as a river would do. Along this flow line, we estimate the shape of
the bed by fitting a parabola to the intersection points between the actual
topography and the normal to the flow line. A main parameter of the model is
the creep parameter <inline-formula><mml:math id="M25" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula>. A low value of <inline-formula><mml:math id="M26" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> corresponds to stiff ice, low
velocities and generally a higher ice volume while a high value of <inline-formula><mml:math id="M27" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> is
associated with softer ice and leads to a faster flow and lower ice volumes.
The standard value of <inline-formula><mml:math id="M28" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> selected in OGGM is constant for all glaciers and is set
equal to <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.4</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">24</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M31" 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> Pa<inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, while in reality <inline-formula><mml:math id="M33" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> may change by a
factor of 10 between glaciers due to a wide range of processes (Cuffey and
Paterson, 2010).</p>
      <p id="d1e785">One advantage of OGGM is that it can be applied to any glacier. It does not
require any specific detailed information that would be lacking for the
majority of them. Besides, it includes simplifications compared to models
focused on a particular, well-observed glacier (e.g. Zekollari et al., 2014)
and is therefore computationally efficient.</p>
      <p id="d1e789">The climate model outputs required to drive OGGM are the monthly mean
temperature and precipitation. The local temperature is obtained by assuming a
constant lapse rate of 6.5 K km<inline-formula><mml:math id="M34" 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 take into account the biases of
the climate model, a simple correction procedure is applied: the model
results are adjusted to have the same climatological monthly mean values
over the reference period 1900–2000 as in the Climatic Research Unit (CRU)
data set (New et al., 2002; Harris et al., 2014) used in the standard version
of the model (Maussion et al., 2018). The simulations cover the period
850–2005, corresponding to the past1000 and historical simulations in the
PMIP3/CMIP5 protocol. However, the sensitivity tests that we have performed
have shown that the first century is influenced by the choice of initial
conditions for the selected glaciers. Consequently, we will only present the
results after 1000 CE.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Glacier length observations</title>
      <p id="d1e810">Glacier surface mass balance is the variable that is the most directly
related to climate, but only a few, generally short, records are available
(Zemp et al., 2009). The number and duration of glacier length observations
are much greater (Oerlemans, 2005; Leclercq et al., 2014; Zemp et al., 2015;
Solomina et al., 2016). The most accurate estimates are deduced from direct
observations of the glacier terminus position as recorded for instance by
the World Glacier Monitoring Service in the Fluctuations of Glaciers (WGMS,
2017). The modern observations can be complemented by historical sources
including old maps, painting, drawing and early photographs as well as
written documents (Grove, 2004; Nussbaumer and Zumbühl, 2012; Purdie et
al., 2014; Zumbühl and Nussbaumer, 2018). Additional evidence is
obtained by dating the position of moraines indicating the position of the
glacier at specific times or from the trees that have been overridden by the
advance of a glacier (Masiokas et al., 2009; Ivy-Ochs et al., 2009; Wiles et
al., 2011; Schimmelpfennig et al., 2014; Le Roy et al., 2015; Moran et al.,
2017).</p>
      <p id="d1e813">As the comparison of model results with observational estimates is a key
element of our methodology, we have applied OGGM to 71 glaciers from the
European Alps that have records covering at least the 20th century in
the global compilation of Leclercq et al. (2014). Twelve of these glacier length
series go back to 1800 CE, seven go back to 1700 CE, and the longest record starts in
1535 CE (Unterer Grindelwald), allowing for each of them a quantitative
comparison with model results at multi-decadal to centennial timescales. The
complete list of glaciers is provided in the Supplement (Table S1). Longer records are also available for many glaciers, but these are
discontinuous and more uncertain, as reviewed in Solomina et al. (2016).
Some of these records will be used for a qualitative evaluation of our
results.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Simulated glacier changes</title>
      <p id="d1e823">Enhanced winter precipitation has been suggested to be an important
contributor to some past changes in glacier length in the Alps (e.g.
Vincent et al., 2005; Steiner et al., 2005, 2008).
Nevertheless, summer temperature is generally considered as the major driver
of European glacier fluctuations at centennial timescales (Oerlemans, 2001;
Steiner et al., 2005; Huss et al., 2008; Steiner et al., 2008; Leclerq and
Oerlemans, 2012; Zekollari et al., 2014). It is thus instructive to first compare the simulated temperatures with reconstructions before analysing the
glacier themselves. Europe is<?pagebreak page1123?> probably the continent where the density of
records of past temperature changes is the highest and several large-scale
reconstructions are available (Luterbacher et al., 2004; Guiot et al., 2010;
Pages2k Consortium, 2013; Luterbacher et al., 2016). For simplicity, we will
only discuss here the most recent spatial reconstruction of summer
temperature, which is highly correlated with long thermometer observations
and the majority of individual records (see Luterbacher et al., 2016 for
more details).</p>
      <p id="d1e826">In agreement with previous studies (Raible et al., 2006; Hegerl et al.,
2011; Goosse et al., 2012b; PAGES2k-PMIP3, 2015; Luterbacher et al., 2016),
most models are able to reproduce the relatively warm conditions observed at
a continental scale during the first centuries of the millennium, the cold
conditions around 1600–1800 and the large warming of the 20th century
(Fig. 1). However, they underestimate the magnitude of the changes for some
(multi-)decadal-scale events compared to the reconstruction of Luterbacher
et al. (2016). Interestingly, some models display an industrial-era warming
that occurred earlier or later than observed (Abram et al., 2016), with a
potentially large impact on the glacier retreat over the recent period. At
a regional scale for the Alps, the conclusions are similar except that the
internal climate variability becomes large enough so that simulation results
cover nearly the full range provided by the reconstruction, even for the
decadal-scale warm or cold events.</p>
      <p id="d1e829">The comparison between OGGM results driven by the various climate models and
observations leads to contrasting results for individual glaciers
(Supplement Fig. S1). This was expected as we have specifically not modified or adapted the parameters in order to apply strictly the standard
configuration of the model in this first set of simulations. Nevertheless,
for the large majority of the glaciers, the observed length changes are well
within the range simulated by the model. For some others, all the
simulations overestimate or underestimate the trends over the 20th century or the variability in the pre-industrial period. This is illustrated in Fig. 2 for five well-known glaciers, but a similar behaviour is seen
for many others (see Supplement Fig. 1). In these examples, the
models tend to underestimate the retreat of the Unterer Grindelwald and Mer
de Glace during the 19th century but some of them have a larger retreat
than observed for those two glaciers over the 20th century. The
agreement is better for the Hintereis, Great Aletsch and Bossons glaciers
although for the latter most models overestimate the magnitude of the
changes compared to observations.</p>
      <p id="d1e832">A detailed comparison between simulations and observed results for each
glacier is beyond the scope of the present study as differences may have
their origin in the specific characteristics of the glacier such as its
stiffness or the presence of debris, in the links between the local climate
and large-scale changes, and in uncertainties in the calibration of the climate
sensitivity parameter of OGGM, etc. However, a behaviour common to a large
majority of the glaciers can be associated with a particular climate model and
can be described by simply calculating the mean changes over all the
glaciers. Conclusions are qualitatively similar for the mean of absolute
changes (Fig. 3a) and the mean of relative changes (Fig. 3b). For these
latter diagnostics, the glacier length changes are normalized using their
observed length in 1950 before calculating the average. This implies that the
absolute mean is not dominated by the long glaciers with large fluctuations
but reflects a general signal present in the majority of glaciers.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><label>Figure 1</label><caption><p id="d1e838">Summer temperature averaged over <bold>(a)</bold> Europe and <bold>(b)</bold> the
Alpine region (defined here as the area between 45 and 48<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and
between 6 and 13<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) in the reconstruction of Luterbacher et al. (2016) and as simulated by climate models over the past millennium. The
shaded area represents the mean plus and minus 1 standard deviation of the
CESM1 model ensemble. A 15-year Lowess smoothing has been applied to the
time series. The reference period is the years 1500–1850 CE as in
Luterbacher et al. (2016).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018-f01.pdf"/>

      </fig>

      <p id="d1e871">For some climate models (such as the IPSL model), OGGM simulates a relatively
stable mean glacier length in the pre-industrial period. When driven by the
other climate model outputs, the growth trend between 1000 and 1850 is
larger, in particular for the GISS model, CESM and CCSM4. This is followed
by a large retreat starting in the 19th century, except in CESM for
which the melting begins in the 20th century for nearly all members.</p>
      <p id="d1e874">Visually, the difference between simulated glacier lengths (Fig. 3) appears
to be much larger than for the temperature (Fig. 1), suggesting that glacier
length provides a clear constraint on climate model behaviour. However, part
of it may be related to the way the figure is presented. In particular,
using a reference period in the 20th century, as required because of
the short duration of the glacier records, tends to amplify the differences
in the pre-industrial period compared to the classical reference period
chosen for temperature (Fig. 1). This is illustrated in Supplement Fig. 2 in which temperature<?pagebreak page1124?> series have been plotted with a reference period in
the 20th century.</p>
      <p id="d1e877">Additionally, some of the differences between the simulated glacier lengths
may be due to the integration of the internal climate variability by the
glaciers and not to a systematic difference between climate models. This
impact of internal variability can be quantified from the ensemble of
simulations performed with CESM. We have to be careful since this estimate
is derived from one model only, which displays significant differences to some of the other models for the Alps. Nevertheless, this provides a
first-order estimate. The glacier retreat over the 20th century varies
strongly between CESM ensemble members, with the observed changes in the
lower range of the ensemble (Fig. 4a). Consequently, although the magnitude
of the changes varies considerably between simulations, it is impossible to
reject firmly the hypothesis that the differences between climate models and
between models and observations for the Alps over this period are due to
internal climate variability only.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><label>Figure 2</label><caption><p id="d1e882">Observed and simulated length for five selected glaciers
in the Alps. The shaded area represents the range of the ensemble of
simulations driven by CESM outputs. The reference period is 1901–1930 CE.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018-f02.pdf"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><label>Figure 3</label><caption><p id="d1e894"><bold>(a)</bold> Absolute and <bold>(b)</bold> relative length changes averaged
over the 71 glaciers. The relative length is obtained by dividing the
glacier changes by their length in 1950 in the compilation of Leclercq et al. (2014). The average for observations is calculated over the available
time series for each period, meaning that the number strongly decreases with
time and, in particular, is very low before 1700. The reference period is
1901–1930 CE.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018-f03.pdf"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><label>Figure 4</label><caption><p id="d1e910">Mean (black) and median (red) of the difference in
glacier length between <bold>(a)</bold> 1970–2000 and 1900–1930; <bold>(b)</bold> 1970–2000 and
1700–1850; <bold>(c)</bold> 1000–1150 and 1700–1850; and <bold>(d)</bold> 1970–2000 and 1000–1150. In panels
<bold>(a)</bold> and <bold>(b)</bold>, observations are given as a horizontal dashed line. No observation
is available for <bold>(c)</bold> and <bold>(d)</bold>. For <bold>(b)</bold>, the average of model results
is made only for the glaciers that have observations. For CESM, the bar
gives the ensemble range.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018-f04.pdf"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><label>Figure 5</label><caption><p id="d1e949">Proportion of glacier advances binned for 50-year
intervals.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018-f05.pdf"/>

      </fig>

      <p id="d1e958">The signal is clearer when comparing the late 20th century with the
years 1700–1850 (Fig. 4b), which roughly corresponds to the maximum extent
in the simulated results. All the simulations driven by CESM underestimate
the observed changes between those two periods, as the simulated glacier
retreat starts much later than in the observations (Fig. 3). The simulations
using the standard version of OGGM driven by the other climate models are at
the margin or out of the CESM ensemble range, suggesting that the difference
are not only due to internal climate variability but are related to
different characteristics of the simulations performed with the various
climate models. Those simulated results are closer to observations, in
particular the ones driven by CCSM4, IPSL and BCC (Beijing Climate Center) model results.</p>
      <p id="d1e961">Computing the difference between the years 1000 and 1150 CE (Fig. 4c), when the
glacier extent was close to its minimum in nearly all the simulations, and
the years 1700–1850 CE confirms the differences deduced qualitatively from
Fig. 3. Some models have a large positive growth trend over the
pre-industrial period while some others have a much smaller one, with
potentially a very large contribution of internal variability. The
comparison between the late 20th century and the beginning of the
millennium also reveals some clear differences between the simulations (Fig. 4d). For some of them, as the ones driven by the IPSL and MPI models, the
minimum is clearly reached in the late 20th century while many glaciers
were smaller during the period 1000–1150 CE in the simulations driven by
CESM and GISS outputs. It is difficult to estimate from observations when
glaciers were smaller than presently as the evidence may still be buried
under the ice (Goehring et al., 2011; Luthi et al., 2014; Solomina et al.,
2016). For the Alps, this might have occurred before 1000 CE or in the
periods 1200–1280 and 1400–1550 CE, but there is currently no direct evidence
that this was actually the case during the past millennium (Luthi et al.,
2014).</p>
      <p id="d1e965">Another instructive diagnostic is the proportion of glaciers that are
advancing over a specific period (Fig. 5), since it can potentially be
compared to observations (e.g. Solomina et al., 2016). However, this
diagnostic is by construction noisier than the glacier length itself and is
strongly influenced by internal variability, with the simulations driven by
CESM covering nearly the full range between 0 % and 100 % of advancing
glaciers for several periods. Estimates derived from observations also
display uncertainties. The evidence for a glacier advance, as derived for
instance from a moraine position, may actually correspond to a time where
the glacier is close to a maximum extent rather than still advancing (Grove,
2004; Solomina et al., 2016). The absence of evidence of advance may also only be due to the lack of a preserved signal in geomorphological features, not
to the glacier changes themselves. The model–data comparison can thus only
be qualitative and must be interpreted with caution.</p>
      <p id="d1e968">As described in the synthesis of Solomina et al. (2016) for the Alps, many
glaciers display a minimum extent around the 9th–11th century.
This is followed by a first advance in the 12th century, a retreat at the beginning of the 13th century and a general advance in the late
13th century (Holzhauser et al., 2005; Luthi et al., 2014; Le Roy et
al., 2015). This advance after the 11th century is in general agreement
with our results except that the majority of models simulates an increase in
glacier length for the beginning of the 13th century too, while the
12th century is generally characterized by a<?pagebreak page1125?> small number of advances.
This would suggest a wrong timing of the glacier advances in models and
would be consistent with the higher simulated European temperatures compared
to the reconstruction of Luterbacher et al. (2016) around 1100 CE and the
lower simulated values compared to the reconstructed ones around 1200 CE.
Nevertheless, the variability in the simulated results is too large to
obtain a clear answer from the diagnostics of glacier advances alone.</p>
      <p id="d1e971">Subsequently, observational evidence indicates a retreat around 1400 CE
before new advances in the late 15th century and the 16th century,
their timing varying between regions (Holzhauser et al., 2005;
Schimmelpfennig et al., 2014; Luthi et al., 2014; Le Roy et al., 2015;
Solomina et al., 2016). The early 15th century is also a period with
glacier retreats in models, preceding major advances in good agreement with
observations. The variability between models is larger for the years
1500–1850, when the extent was close to its maximum, and no clear common
signal can be deduced from the diagnostics of glacier advances in the
simulations for this period.</p>
      <p id="d1e974">The early 15th century corresponds to a minimum for glacier advances in
many models (Fig. 5) and a relative minimum in glacier length (Fig. 3).
Although the simulated temperatures are generally mild during this period,
they are not high and, in particular, are generally lower than at the beginning of the millennium (Fig. 1). This clearly illustrates the impact of
the long response timescales of glaciers. The simulated glacier retreats in
the early 15th century appear to be partly due to the temperatures at
that time but also to the recovery from the large advances in the 13th
and 14th century.</p>
      <p id="d1e977">The warming over the 20th century has a clear impact on glacier length,
inducing a simulated retreat of nearly all the glaciers in agreement with
observations, except in some experiments driven by CESM members that display
a weak temperature increase over the Alps (Fig. 3 and Supplement Fig. S1).
Nevertheless, the contemporaneous temperature does not appear to be the only
variable driving the glacier length changes when comparing two 30-year
period at the beginning and the end of the 20th century (Fig. 6a). The
contribution of temperature is present, but the response time of the glacier
as well as the influence of precipitation variability, for instance, can
still obscure the link between temperature and glacier length for those
relatively short periods.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><label>Figure 6</label><caption><p id="d1e983">Glacier length changes as a function of summer
temperature changes in the Alps for the differences between <bold>(a)</bold> 1970–2000 and
1900–1930; <bold>(b)</bold> 1970–2000 and 1700–1850; <bold>(c)</bold> 1000–1150 and 1700–1850; and <bold>(d)</bold>
1970–2000 and 1000–1150. For <bold>(b)</bold>, the average of model results is made only
for the glaciers that have observations. The crosses represent the
individual CESM ensemble members, the ensemble mean being represented by a
dot of the same colour.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018-f06.pdf"/>

      </fig>

      <p id="d1e1007">The association between summer temperature and glacier changes is more
direct and linear when analysing length<?pagebreak page1126?> changes on longer timescales. The
relative minimum in glacier length in the 12th century (Fig. 3) is
clearly due to the warm simulated temperatures at that time (Fig. 1). The
climate models that have the largest temperature changes over the
pre-industrial period and between pre-industrial period and the 20th century are also the ones that lead to the larger changes in glacier length
(Fig. 6b, c, d).</p>
      <p id="d1e1010">This confirms the dominant role of temperature fluctuations in glacier
evolution in the Alps (Oerlemans, 2001; Huss et al., 2008; Steiner et al.,
2008; Leclerq and Oerlemans, 2012; Zekollari et al., 2014). Furthermore,
although some simulations display smaller or larger values compared to
observations for each variable, the model ensemble agrees very well with
observations for the ratio between temperature and glacier length changes
between the pre-industrial period and the 20th century (Fig. 6b). This
suggests that the glacier model has a reasonable temperature sensitivity. An
alternative interpretation is to state that the link between reconstructed
temperatures and glacier length observations is compatible with model
results using the standard parameters of OGGM.</p>
</sec>
<sec id="Ch1.S4">
  <title>Sensitivity of glacier changes to model parameters</title>
      <p id="d1e1019">The parameter set and experimental design applied in the simulations
described in Sect. 3 are identical to the ones of the standard version of
the OGGM model (Maussion et al.,<?pagebreak page1127?> 2018). In order to estimate how our results
are sensitive to this choice, a series of sensitivity experiments has been
performed, addressing uncertainties in OGGM representation of the glacier
dynamics, the surface mass balance and the way climate model results are
processed before using them to drive the glacier model.</p>
      <p id="d1e1022">In the first two experiments, the creep parameter has been multiplied and
divided by a factor of 2 for all the glaciers, applying a value of
<inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.8</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">24</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.2</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">24</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M41" 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> Pa<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. In the next two experiments, the climate sensitivity parameter
<inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> has been uniformly decreased and increased by 10 %.
These experiments are not intended to correspond to a new calibration of
these parameters but are used to provide a measure of the impact of a variation
in their range of uncertainty (Marzeion et al., 2012; Maussion et al.,
2018).</p>
      <p id="d1e1107">In the standard simulations, a very simple bias correction is applied to
climate model results, ensuring that after the adjustment the climate models
have the same mean over the reference period as the CRU data set used to
calibrate OGGM climate sensitivity parameter (see Sect. 2). However, the
variance and the magnitude of the response to a perturbation is likely
different at the altitude of the glacier compared to the lower altitude
corresponding to the land surface at the scale of the global climate model
(Mountain Research Initiative EDW Working Group, 2015; Kotlarski et al.,
2015). Consequently, we have scaled simulated temperatures in the final
sensitivity experiment so that the variance for each month has the same value
as for CRU data set. The temperatures have not been detrended before
computing the variance and this thus includes a scaling of the warming over
the 20th century as well as of the interannual variability, but the
correction is not timescale dependent. This scaling takes into account not
only the elevation dependence of the changes but also any bias in the
simulated variance (Maraun and Widmann, 2018).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><label>Figure 7</label><caption><p id="d1e1112">Length changes averaged over the 71 glaciers for the
standard and sensitivity experiments using CCSM4 results.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/14/1119/2018/cp-14-1119-2018-f07.pdf"/>

      </fig>

      <p id="d1e1122">Those changes in parameters have a very large impact on glacier volume, in
agreement with previous tests performed with OGGM (Maussion et al., 2018).
The differences can reach up to a factor of 2 compared to the standard
experiment. They also have a clear impact on the mean length of the glacier.
However, when discarding the first 150 years of simulations (when the
adjustment to the new parameters occurs), the changes in glacier length
averaged over the 71 glaciers are very small. This is illustrated for CCSM4
in Fig. 7. Similar results have been obtained for the other climate models
(not shown). In particular, the sensitivity to glacier model parameters and
to the correction method applied to climate model results is much smaller
than the contribution of internal variability (see Fig. 3), whose role as a
dominant source of uncertainty in a model–data comparison is thus confirmed.
This conclusion is reached for the Alps and for the selected climate models.
Different results might be obtained for other regions or for other models
displaying larger biases. Additionally, sensitivity experiments with larger
perturbations of parameters would lead to larger differences with the
standard experiment. Nevertheless, the small changes in the results of our
sensitivity experiments indicate that the main conclusions obtained in
Sect. 3 are not critically dependent on the choices made in the
application of OGGM.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e1132">The simulations performed with OGGM driven by climate model results have
shown that there is no inconsistency between the climate provided by the
model ensemble and glacier length observations. Disagreements are found for
individual glaciers, but this was expected as global models are not able to
represent the small-scale processes that may rule some glacier changes.
However, when analysing the 71 selected glaciers, there is no systematic
bias in the timing or the amplitude of simulated glacier changes and the
observed length variations are generally well within the range of simulated
values. This agreement was achieved without any specific calibration of the
glacier model and does not appear critically dependent on the choice of some
model parameters.</p>
      <p id="d1e1135">This provides an additional positive evaluation of climate models and, by using a new type of data, confirms their ability to reproduce the dominant
changes over the past millennium. The successful application of global
climate models driving a global glacier model over the past millennium also
reinforces the validity of this approach to study future changes on similar
timescales.</p>
      <?pagebreak page1128?><p id="d1e1138"><?xmltex \hack{\newpage}?>Some studies have argued that the large melting of Alpine glaciers in the
19th century might be due to a modification of the ice albedo caused by the
deposition of black carbon of anthropogenic origin (Painter et al., 2013).
This hypothesis has recently been challenged (e.g. Luthi, 2014), in
particular because no evidence of a significant deposition at the time of
the retreat was found in an ice core collected in the Alps (Sigl et al.,
2018). Although the simulated changes are underestimated here for some
glaciers, this additional forcing does not seem to be required
systematically to reproduce past glacier changes in models.</p>
      <p id="d1e1142">In addition to the overall compatibility of the ensemble of simulations with
observations, the comparison between simulated results and estimates of past
glacier length fluctuations may help identify some specific
characteristics of individual climate model simulations. This comparison is
complicated because of the large contribution of internal climate
variability on glacier length fluctuations. Nevertheless, some diagnostics
appear robust enough to assess the overall climate model skill in the
region studied. In particular, some simulations underestimate the amplitude
of the glacier changes between the 18th century and the end of the
20th century. This disagreement may have several origins, such as model
biases in temperature or precipitation changes. However, an independent
comparison between simulated and reconstructed temperatures suggests that
these models have too weak a warming over the past 2 to 3 centuries,
suggesting an important contribution from this variable in the glacier model
behaviour.</p>
      <p id="d1e1146">Another robust characteristic of many simulations is the timing of the
minimum glacier extent over the past millennium. For some climate models,
this occurs clearly at the end of the simulation while for some other models
the minimum extent takes place at the beginning of the millennium.
Unfortunately, observations do not allow the determination of which behaviour is more
realistic. Although there are not enough observations in the Alps to argue
in favour of a systematic lower extent than today during some periods in the
past millennium, the evidence is maybe still hidden below the ice.</p>
      <p id="d1e1149">More generally, our experiments have demonstrated the interest of driving a
global glacier model by climate model outputs in order to have a direct
comparison between simulated and observed glacier length. This allows a more
quantitative evaluation of the models and a more precise interpretation of
the records. For instance, the beginning of the 15th century is
characterized by a general glacier retreat in simulations and
reconstructions but without particularly high temperatures, illustrating
that even though the link between summer temperature and glacier length is
strong in the Alps, it is not always straightforward because of the long
response time of glaciers. Our results thus open up the application of the same
approach to other regions and the integration of glacier records with others in multi-proxy assessments of past climate reconstructions.</p>
</sec>

      
      </body>
    <back><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e1156">The code of OGGM (DOI:
<uri>http://doi.org/10.5281/zenodo.1149701</uri>, Maussion et al., 2018) is freely
available online (<uri>http://oggm.org/</uri>; last access: 11 January 2018).
Simulated glacier lengths will be made available in a public repository
(<uri xlink:href="https://zenodo.org/record/1319334#.W2go2Lg6-M">https://zenodo.org/record/1319334\#.W2go2Lg6-M</uri>; last access:
23 July 2018) (Goosse et al., 2018).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e1168">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/cp-14-1119-2018-supplement" xlink:title="pdf">https://doi.org/10.5194/cp-14-1119-2018-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1177">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1183">This work was supported by Fonds National de la Recherche Scientifique
(F.R.S.-FNRS-Belgium) in the framework of the project “Evaluating simulated
centennial climate variability over the past millennium using global<?pagebreak page1129?> glacier
modelling” (grant agreement PDR T.0028.18). Hugues Goosse is Research
Director within the F.R.S.-FNRS. We would like to thank Olga Solomina for
sharing results of the synthesis of glacier records she led and for her
suggestions. We acknowledge the World Climate Research Programme's Working
Group on Coupled Modelling, which is responsible for CMIP, and we thank the
climate modelling groups (listed in Table 1 of this paper) for producing and
making available their model output. For CMIP, the US Department of Energy's
Program for Climate Model Diagnosis and Intercomparison provides coordinating
support and led the development of software infrastructure in partnership
with the Global Organization for Earth System Science Portals.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by: Ed Brook<?xmltex \hack{\newline}?> Reviewed by: three
anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>Testing the consistency between changes in simulated climate and Alpine glacier length over the past millennium</article-title-html>
<abstract-html><p>It is standard to compare climate model results covering
the past millennium and reconstructions based on various archives in order
to test the ability of models to reproduce the observed climate variability.
Up to now, glacier length fluctuations have not been used systematically in
this framework even though they offer information on multi-decadal to
centennial variations complementary to other records. One reason is that
glacier length depends on several complex factors and so cannot be directly
linked to the simulated climate. However, climate model skill can be
measured by comparing the glacier length computed by a glacier model driven
by simulated temperature and precipitation to observed glacier length
variations. This is done here using the version 1.0 of the Open Global Glacier
Model (OGGM) forced by fields derived from a range of simulations performed
with global climate models over the past millennium. The glacier model is
applied to a set of Alpine glaciers for which observations cover at least
the 20th century. The observed glacier length fluctuations are
generally well within the range of the simulations driven by the various
climate model results, showing a general consistency with this ensemble of
simulations. Sensitivity experiments indicate that the results are much more
sensitive to the simulated climate than to OGGM parameters. This confirms
that the simulations of glacier length can be used to evaluate the climate
model performance, in particular the simulated summer temperatures that
largely control the glacier changes in our region of interest. Simulated
glacier length is strongly influenced by the internal variability in the
system, putting limitations on the model–data comparison for some variables
like the trends over the 20th century in the Alps. Nevertheless,
comparison of glacier length fluctuations on longer timescales, for instance
between the 18th century and the late 20th century, appear less
influenced by the natural variability and indicate clear differences in the
behaviour of the various climate models.</p></abstract-html>
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