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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESD</journal-id><journal-title-group>
    <journal-title>Earth System Dynamics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Dynam.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">2190-4987</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/esd-13-321-2022</article-id><title-group><article-title>The Mediterranean climate change hotspot <?xmltex \hack{\break}?> in the CMIP5 and CMIP6 projections</article-title><alt-title>The Mediterranean climate change hotspot in the CMIP5 and CMIP6 projections</alt-title>
      </title-group><?xmltex \runningtitle{The Mediterranean climate change hotspot in the CMIP5 and CMIP6 projections}?><?xmltex \runningauthor{J.~Cos et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Cos</surname><given-names>Josep</given-names></name>
          <email>josep.cos@bsc.es</email>
        <ext-link>https://orcid.org/0000-0002-3050-2306</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Doblas-Reyes</surname><given-names>Francisco</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6622-4280</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff3">
          <name><surname>Jury</surname><given-names>Martin</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Marcos</surname><given-names>Raül</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3610-3445</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Bretonnière</surname><given-names>Pierre-Antoine</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3066-6685</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Samsó</surname><given-names>Margarida</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Earth Sciences Department, Barcelona Supercomputing Center (BSC), Barcelona, Spain</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Institució Catalana de Recerca i Estudis Avançats (ICREA), Barcelona, Spain</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Wegener Center for Climate and Global Change, University of Graz, Graz, Austria</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Josep Cos (josep.cos@bsc.es)</corresp></author-notes><pub-date><day>8</day><month>February</month><year>2022</year></pub-date>
      
      <volume>13</volume>
      <issue>1</issue>
      <fpage>321</fpage><lpage>340</lpage>
      <history>
        <date date-type="received"><day>27</day><month>July</month><year>2021</year></date>
           <date date-type="accepted"><day>3</day><month>January</month><year>2022</year></date>
           <date date-type="rev-recd"><day>22</day><month>December</month><year>2021</year></date>
           <date date-type="rev-request"><day>30</day><month>July</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 Josep Cos et al.</copyright-statement>
        <copyright-year>2022</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://esd.copernicus.org/articles/13/321/2022/esd-13-321-2022.html">This article is available from https://esd.copernicus.org/articles/13/321/2022/esd-13-321-2022.html</self-uri><self-uri xlink:href="https://esd.copernicus.org/articles/13/321/2022/esd-13-321-2022.pdf">The full text article is available as a PDF file from https://esd.copernicus.org/articles/13/321/2022/esd-13-321-2022.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e143">The enhanced warming trend and precipitation decline in the Mediterranean region make it a climate change hotspot. We compare projections of multiple Coupled Model Intercomparison Project Phase 5 (CMIP5) and Phase 6 (CMIP6) historical and future scenario simulations to quantify the impacts of the already changing climate in the region. In particular, we investigate changes in temperature and precipitation during the 21st century following scenarios RCP2.6, RCP4.5 and RCP8.5 for CMIP5 and SSP1-2.6, SSP2-4.5 and SSP5-8.5 from CMIP6, as well as for the HighResMIP high-resolution experiments. A model weighting scheme is applied to obtain constrained estimates of projected changes, which accounts for historical model performance and inter-independence in the multi-model ensembles, using an observational ensemble as reference. Results indicate a robust and significant warming over the Mediterranean region during the 21st century over all seasons, ensembles and experiments. The temperature changes vary between CMIPs, CMIP6 being the ensemble that projects a stronger warming. The Mediterranean amplified warming with respect to the global mean is mainly found during summer. The projected Mediterranean warming during the summer season can span from 1.83 to 8.49 <inline-formula><mml:math id="M1" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> in CMIP6 and 1.22 to 6.63 <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> in CMIP5 considering three different scenarios and the 50 % of inter-model spread by the end of the century. Contrarily to temperature projections, precipitation changes show greater uncertainties and spatial heterogeneity. However, a robust and significant precipitation decline is projected over large parts of the region during summer by the end of the century and for the high emission scenario (<inline-formula><mml:math id="M3" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>49 % to <inline-formula><mml:math id="M4" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>16 % in CMIP6 and <inline-formula><mml:math id="M5" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>47 % to <inline-formula><mml:math id="M6" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22 % in CMIP5). While there is less disagreement in projected precipitation than in temperature between CMIP5 and CMIP6, the latter shows larger precipitation declines in some regions. Results obtained from the model weighting scheme indicate larger warming trends in CMIP5 and a weaker warming trend in CMIP6, thereby reducing the difference between the multi-model ensemble means from 1.32 <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> before weighting to 0.68 <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> after weighting.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e232">The Mediterranean region (10<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W, 40<inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, 30<inline-formula><mml:math id="M11" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 45<inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N; <xref ref-type="bibr" rid="bib1.bibx37" id="altparen.1"/>) is located between the arid and warm
northern African climate and the humid and mild European climate <xref ref-type="bibr" rid="bib1.bibx17" id="paren.2"/>. The contrast between them is partly explained by the influence of
the surrounding oceans, their interaction with the land surface and the general atmospheric circulation characteristics in the mid-latitudes
<xref ref-type="bibr" rid="bib1.bibx5" id="paren.3"/>.</p>
      <p id="d1e281">Global warming is not homogeneous, and <xref ref-type="bibr" rid="bib1.bibx43" id="text.4"/> suggests that the Mediterranean region is a climate change hotspot. Consequently,
adaptation to changing climate threats is paramount to countries located around the Mediterranean Sea <xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx17" id="paren.5"/>, which
live in a complex and diverse socioeconomic situation<?pagebreak page322?> and have severe vulnerabilities to climate change and variability <xref ref-type="bibr" rid="bib1.bibx3" id="paren.6"/>. The
observed warming in the Mediterranean region during the last decades is expected to continue and grow larger than the global-mean warming
<xref ref-type="bibr" rid="bib1.bibx43" id="paren.7"/>. Additionally, total precipitation declines were observed during the late 20th century <xref ref-type="bibr" rid="bib1.bibx44" id="paren.8"/>, and have been
projected by different multi-model ensembles for the 21st century <xref ref-type="bibr" rid="bib1.bibx54 bib1.bibx80" id="paren.9"/>. Characteristics of the projected Mediterranean
climate change have been linked to thermodynamic sources such as land–ocean warming contrast and lapse rate change in summer <xref ref-type="bibr" rid="bib1.bibx10" id="paren.10"/>, and to
dynamical processes such as the changes in upper-tropospheric large-scale flow in winter <xref ref-type="bibr" rid="bib1.bibx69" id="paren.11"/>.</p>
      <p id="d1e309">Numerical models are used to estimate future climate change. Accounting for the physical processes and interactions in each climate subsystem
(atmosphere, biosphere, cryosphere, hydrosphere and land-surface), global climate models (GCMs) aim to project the state of the future climate
system. Model runs over long historical or future periods are driven by natural forcings (i.e. solar irradiance and volcanic aerosols) and
anthropogenic emissions that alter greenhouse gas (GHG) concentrations, leading to changes in the radiative forcing <xref ref-type="bibr" rid="bib1.bibx33" id="paren.12"/>. GCMs are
developed by a number of institutions who always apply the same physical principles but might use slightly different assumptions. This opens the door
to performing the same experiments with multiple GCM outputs, leading to more robust estimates. Modelling uncertainty can be sampled by ensembling
various models <xref ref-type="bibr" rid="bib1.bibx66" id="paren.13"/>, while running the same model multiple times (referred to as members), with differing initial conditions
<xref ref-type="bibr" rid="bib1.bibx24" id="paren.14"/>, under the same experiment samples' internal variability <xref ref-type="bibr" rid="bib1.bibx33" id="paren.15"/>. To make the results comparable, intercomparison
projects, where several models perform standardized experiments, have been organized by the international community <xref ref-type="bibr" rid="bib1.bibx50 bib1.bibx58" id="paren.16"/>. The main community effort is the Coupled Model Intercomparison Project (CMIP). In this study, we consider the two latest CMIP phases,
CMIP5 and CMIP6 <xref ref-type="bibr" rid="bib1.bibx65 bib1.bibx24" id="paren.17"/>, and explore their similarities and differences over the Mediterranean region. The almost 10 years
between CMIP5 and CMIP6 allowed for improvements in the modelling of certain Earth system processes such as cloud feedbacks, aerosol forcings and
aerosol–cloud interactions <xref ref-type="bibr" rid="bib1.bibx74 bib1.bibx76" id="paren.18"/>.</p>
      <p id="d1e334">CMIP experiments were performed with a large set of models and therefore show many differences in projected changes due to internal variability and
the diverse model designs used by the modelling teams. Weighting single model runs according to their performance in simulating the observed past
allows constraining the climate modelling uncertainty and obtaining a potentially more accurate estimate of regional climate change signals. Various
studies have used different subsetting/weighting approaches such as emergent constraints <xref ref-type="bibr" rid="bib1.bibx16 bib1.bibx30 bib1.bibx67" id="paren.19"/>, performance-based
model subsets <xref ref-type="bibr" rid="bib1.bibx48 bib1.bibx41 bib1.bibx34" id="paren.20"/> and model weighting accounting for performance and independence <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx45 bib1.bibx11" id="paren.21"/>. The last approach has been used in this study as it additionally considers the interdependencies existing between the
models.</p>
      <p id="d1e347">This study evaluates and quantifies the Mediterranean climate change hotspot for each season over the 21st century by looking into surface air
temperature and precipitation changes in the Mediterranean and how they relate to larger-scale responses. We consider three different emission
scenarios in order to assess the impact of anthropogenic emission uncertainties over the Mediterranean climate. The CMIP5 and CMIP6 multi-model ensembles are
used to estimate the climate change signal, its uncertainty and to illustrate the differences between the two experiments in the region. Finally, a
weighting method is applied to each CMIP ensemble based on the criteria of model performance and independence to obtain more robust projections.</p>
      <p id="d1e350">Section <xref ref-type="sec" rid="Ch1.S2"/> describes the climate models and observational data used, and explains the methods used to quantify climate change and weight
the projection members. The climate change hotspot in the Mediterranean and the weighted and unweighted projected changes are presented in
Sect. <xref ref-type="sec" rid="Ch1.S3"/>, while these results are discussed in Sect. <xref ref-type="sec" rid="Ch1.S4"/>. Section <xref ref-type="sec" rid="Ch1.S5"/> concludes and raises questions for further
investigation.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Model data</title>
      <p id="d1e376">This study is based on the CMIP5 and CMIP6 historical and future climate projections experiments. The historical CMIP5 experiments span from 1850 to
2005 <xref ref-type="bibr" rid="bib1.bibx65" id="paren.22"/> and from 1850 to 2014 in CMIP6 <xref ref-type="bibr" rid="bib1.bibx24" id="paren.23"/>. The future projections are a continuation of the historical simulations,
and we have used runs continuing until the year 2100. The variables are monthly mean near-surface air temperature (TAS), precipitation rate (PR) and
sea-level pressure (PSL). The latter is used to weight the ensemble members together with TAS (see Sect. <xref ref-type="sec" rid="Ch1.S2.SS3"/>).</p>
      <p id="d1e387">The increasing computational power over time has allowed for increased model resolution and complexity, which leads to the expectation that models
have improved from CMIP5 to CMIP6. Additionally, we have used the High Resolution Model Intercomparison Project (HighResMIP), a CMIP6-endorsed MIP
<xref ref-type="bibr" rid="bib1.bibx29" id="paren.24"/> that aims to compare lower- and higher-resolution versions of the same global models. The historical and future HighResMIP periods
span from 1950 to 2014 and from 2015 to 2050 respectively. Though only a subset of the CMIP6 models contributed to HighResMIP, this smaller ensemble has
also been<?pagebreak page323?> considered in this study in order to assess the impact of increasing model resolution on the Mediterranean climate.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e396"> Summary of the observational references for near-surface air temperature (TAS), precipitation rate (PR) and sea-level pressure (PSL).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="48mm"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Name</oasis:entry>
         <oasis:entry colname="col2">Type</oasis:entry>
         <oasis:entry colname="col3">Institute</oasis:entry>
         <oasis:entry colname="col4">Variables</oasis:entry>
         <oasis:entry colname="col5">Reference</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">JRA55</oasis:entry>
         <oasis:entry colname="col2">Reanalysis</oasis:entry>
         <oasis:entry colname="col3">Japan Meteorological Agency (JMA)</oasis:entry>
         <oasis:entry colname="col4">TAS, PR, PSL</oasis:entry>
         <oasis:entry colname="col5">
                    <xref ref-type="bibr" rid="bib1.bibx40" id="text.25"/>
                  </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">ERA5</oasis:entry>
         <oasis:entry colname="col2">Reanalysis</oasis:entry>
         <oasis:entry colname="col3">European Centre for Medium-Range<?xmltex \hack{\hfill\break}?>Weather Forecasts (ECMWF)</oasis:entry>
         <oasis:entry colname="col4">TAS, PSL</oasis:entry>
         <oasis:entry colname="col5">
                    <xref ref-type="bibr" rid="bib1.bibx35" id="text.26"/>
                  </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CRU (v4.04)</oasis:entry>
         <oasis:entry colname="col2">Gridded observations</oasis:entry>
         <oasis:entry colname="col3">University of East Anglia (UEA)</oasis:entry>
         <oasis:entry colname="col4">TAS, PR</oasis:entry>
         <oasis:entry colname="col5">
                    <xref ref-type="bibr" rid="bib1.bibx31" id="text.27"/>
                  </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">GPCC (v2018)</oasis:entry>
         <oasis:entry colname="col2">Gridded observations</oasis:entry>
         <oasis:entry colname="col3">Deutscher Wetterdienst (DWD)</oasis:entry>
         <oasis:entry colname="col4">PR</oasis:entry>
         <oasis:entry colname="col5">
                    <xref ref-type="bibr" rid="bib1.bibx64" id="text.28"/>
                  </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">BerkeleyEarth</oasis:entry>
         <oasis:entry colname="col2">Gridded observations</oasis:entry>
         <oasis:entry colname="col3">Berkeley Earth</oasis:entry>
         <oasis:entry colname="col4">TAS</oasis:entry>
         <oasis:entry colname="col5">
                    <xref ref-type="bibr" rid="bib1.bibx62" id="text.29"/>
                  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadSLP2</oasis:entry>
         <oasis:entry colname="col2">Gridded observations</oasis:entry>
         <oasis:entry colname="col3">Met Office (UKMO)</oasis:entry>
         <oasis:entry colname="col4">PSL</oasis:entry>
         <oasis:entry colname="col5">
                    <xref ref-type="bibr" rid="bib1.bibx1" id="text.30"/>
                  </oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e569">Three radiative forcing scenarios are used to account for uncertainty in future emissions: the CMIP5 Representative Concentration Pathways (RCPs;
<xref ref-type="bibr" rid="bib1.bibx73" id="altparen.31"/>) 2.6, 4.5 and 8.5 and the CMIP6 Shared Socioeconomic Pathways (SSPs; <xref ref-type="bibr" rid="bib1.bibx58" id="altparen.32"/>) 1-2.6, 2-4.5 and 5-8.5. The magnitudes
2.6, 4.5 and 8.5 (in <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) represent the 2100 global radiative forcing in comparison to the pre-industrial era. However, even if the
radiative forcing at the end of the century is the same in both RCPs and SSPs, the path to reach it can differ substantially, leading to differences
in the projected climate <xref ref-type="bibr" rid="bib1.bibx78" id="paren.33"/>. One of the main differences between the SSPs and RCPs is that the former have a compatible socioeconomic
scenario associated with each forcing scenario, SSP1 being based on sustainability, inclusive development and inequality reduction, SSP2 representing a
middle-of-the-road scenario, where slow progress is made in achieving sustainable development goals and with a mild decline in resource and energy
use and being SSP5 based on fossil-fuelled development, rapid technological progress and economic growth <xref ref-type="bibr" rid="bib1.bibx58 bib1.bibx53" id="paren.34"/>. The results from
CMIP5 and CMIP6 sharing the same 2100 radiative forcing will be displayed together for simplicity, but the reader should always bear in mind that the
evolution of GHG concentrations differs between them. They are not entirely comparable as RCPs and SSPs defined with the same radiative forcing at the
end of the century do not share the same progression of aerosol and GHG concentrations throughout the 21st century. HighResMIP is only available for the
scenario SSP5-8.5 for future projections.</p>
      <p id="d1e601">Many of the models have more than one member, meaning that the model runs have been started with different initial conditions, leading to diverging
climate trajectories. The aim of having multiple members is to sample the uncertainty that arises from internal variability <xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx19" id="paren.35"/>. Having multi-member models means that the multi-model ensembles are super-ensembles. A summary of the simulations performed by each
model used and for every scenario can be found in Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/>.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Observational data</title>
      <p id="d1e617">We use observational references to compare the model experiments to the observed past and to derive performance weights of ensemble members. Multiple
observational products are used including both reanalysis (ERA5 and JRA55) and gridded observations (GPCC, CRU, BerkeleyEarth and HadSLP2) to account
for observational uncertainty. A summary of the observational datasets used is found in Table <xref ref-type="table" rid="Ch1.T1"/>. JRA55 will not be displayed in the
time series plots as it overestimates the precipitation over the Mediterranean during the period 1958–1978 <xref ref-type="bibr" rid="bib1.bibx68" id="paren.36"/>.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Methods</title>
      <p id="d1e634">All datasets are regridded to a 1<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M15" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid using a conservative interpolation method to allow comparison between
different models and observational references. After regridding, the dataset's original orography will differ from that of the
1<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <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> grid. Therefore, the TAS values obtained for a specific altitude might suffer a shift in altitude, which needs to be
corrected by means of the 6.49 <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> standard lapse rate <xref ref-type="bibr" rid="bib1.bibx77 bib1.bibx18" id="paren.37"/>. This is only necessary when absolute
climatologies are used, as computing the change in TAS climatology from one period to the other cancels out this height shift.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e711">Summary of each diagnostic's use and time period.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Diagnostic</oasis:entry>
         <oasis:entry colname="col2">Period(s)</oasis:entry>
         <oasis:entry colname="col3">Use</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M21" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">2021–2040/2061–2080/2081–2100 against 1986–2005</oasis:entry>
         <oasis:entry colname="col3">weighted and unweighted projection results</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">DIFF</oasis:entry>
         <oasis:entry colname="col2">1980–2014</oasis:entry>
         <oasis:entry colname="col3">performance weight</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">STD</oasis:entry>
         <oasis:entry colname="col2">1980–2014</oasis:entry>
         <oasis:entry colname="col3">performance weight</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">TREND</oasis:entry>
         <oasis:entry colname="col2">1980–2014</oasis:entry>
         <oasis:entry colname="col3">performance weight and verification</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CLIM</oasis:entry>
         <oasis:entry colname="col2">1980–2014</oasis:entry>
         <oasis:entry colname="col3">independence weighting</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e808">To assess the seasonal dependence of climate change over the Mediterranean region, results are computed for the winter months December–January–February
(DJF), spring months March–April–May (MAM), summer months June–July–August (JJA) and autumn months September–October–November (SON). A summary
of the time periods used and the applications of the different diagnostics can be found in Table <xref ref-type="table" rid="Ch1.T2"/>.</p>
      <p id="d1e814">All calculations have been performed using the Earth System Model Evaluation Tool (ESMValTool). ESMValTool is a community framework that facilitates
the processing of generic climate datasets, allowing for reproducibility of results <xref ref-type="bibr" rid="bib1.bibx59" id="paren.38"/>.</p>
      <p id="d1e820">Mediterranean TAS and PR are assessed over land to highlight the impact of climate change over populated regions. This avoids values over sea
influencing results over land when regridding is performed, i.e. TAS behaves differently over land than over sea due to differences in surface
thermodynamic properties, while PR over sea should not have an impact on freshwater resources over land.</p>
<sec id="Ch1.S2.SS3.SSS1">
  <label>2.3.1</label><title>Projections verification</title>
      <p id="d1e830">To verify the projection ensembles used, we compare the linear trend (TREND) distributions of the observational products against the multi-model
ensembles. This is computed by applying the linear ordinary least square regression fit with time as an independent variable. The 35-year period
1980–2014 has been used to calculate trends in each model and observational dataset, as a period with shorter span would be too dependent on the
effect of internal variability from the climate system <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx57" id="paren.39"/>. Note that CMIP5 years 2006–2014 are taken from the
corresponding scenario simulation. The results are gathered in the respective OBS, CMIP5, CMIP6 and HighResMIP distributions (displayed as box plots),
and we perform a qualitative assessment on the differences between observed and simulated historical trends.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS2">
  <label>2.3.2</label><title>Mediterranean hotspot evaluation</title>
      <?pagebreak page324?><p id="d1e844">A climate change hotspot is defined as a region whose climate is especially responsive to global change <xref ref-type="bibr" rid="bib1.bibx27" id="paren.40"/>. To characterize the
hotspot, we compare the TAS and PR behaviours in the Mediterranean against the global and latitudinal band responses respectively. The first step is
to calculate the change in the variables' magnitude between the reference period (1986–2005, from <xref ref-type="bibr" rid="bib1.bibx13" id="altparen.41"/>) climatology (CLIM) and a
future period CLIM (this diagnostic is referred to as <inline-formula><mml:math id="M22" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula> in this text). To evaluate the TAS hotspot, we compute the differences between the
multi-model Mediterranean land-only <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> and the global land–ocean <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> means <xref ref-type="bibr" rid="bib1.bibx43" id="paren.42"/>. For PR the land–ocean
latitudinal belt 30–45<inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N mean is used instead of the global mean <xref ref-type="bibr" rid="bib1.bibx43" id="paren.43"/>.  To highlight the difference in the impact of the
hotspot within the Mediterranean region, we plot the hotspot maps using the near-term and long-term <inline-formula><mml:math id="M26" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>, which refer to the future periods
2041–2060 and 2081–2100 respectively. Additionally, to assess the evolution of the hotspot, we calculate the projected area-averaged 10-year
rolling windows of the Mediterranean <inline-formula><mml:math id="M27" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula> and the large-scale <inline-formula><mml:math id="M28" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula> for both TAS and PR. For precipitation, the area aggregations are computed
using absolute values and then the relative change with respect to the reference is calculated (displayed in percentage).</p>
</sec>
<sec id="Ch1.S2.SS3.SSS3">
  <label>2.3.3</label><title>Mediterranean projected changes quantification</title>
      <p id="d1e925">To quantify the projected magnitudes of Mediterranean region climate change, we compute <inline-formula><mml:math id="M29" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula> between the reference period 1985–2005 and
the future periods: near term (2021–2040), mid-term (2041–2060) and long term (2081–2100). We use 20-year baseline and future periods following
the guidelines from <xref ref-type="bibr" rid="bib1.bibx36" id="text.44"/>. Additionally, as CMIP5 historical simulations end in 2005, the reference period 1986–2005 from IPCC's AR5
<xref ref-type="bibr" rid="bib1.bibx13" id="paren.45"/> is chosen to avoid overlapping historical and scenario experiments when extracting projection results. Note that only the
near-term period is available for HighResMIP as the future experiment ends in 2050. The advantage of using <inline-formula><mml:math id="M30" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula> instead of future CLIMs is that
the GCMs' mean-state systematic biases are removed, and we obtain a more easily interpretable comparison of the responses among models and between models
and observations <xref ref-type="bibr" rid="bib1.bibx26" id="paren.46"/>.</p>
      <p id="d1e951">With the aim to sample the inherent uncertainty of the multi-model ensemble, we compute the inter-model spread from the 5th and 95th percentiles of
the ensemble distribution. To take into account the scenario uncertainty, we display the distribution of <inline-formula><mml:math id="M31" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula> from the three different
scenarios that we have used for each ensemble side by side (RCP2.6, RCP4.5 and RCP8.5 for CMIP5 and SSP1-2.6, SSP2-4.5 and SSP5-8.5 for CMIP6).</p>
      <p id="d1e961">The statistical significance of TAS and PR mean changes and the degree of agreement between the models are used to assess the uncertainty and robustness
of the multi-model ensemble results. A climate change signal is considered robust when at least 80 % of the models agree on the projected sign of
the <inline-formula><mml:math id="M32" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>s <xref ref-type="bibr" rid="bib1.bibx13" id="paren.47"/>. A change in the multi-model mean is considered significant when it is beyond the threshold of a two-tailed paired
<inline-formula><mml:math id="M33" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test <xref ref-type="bibr" rid="bib1.bibx71" id="paren.48"/> at the 95 % confidence level. The paired <inline-formula><mml:math id="M34" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test is chosen because it is invariant to differences in the sample's
variability.<?pagebreak page325?> We consider that the null hypothesis is met when there is no difference between the multi-model distribution in the reference and future
periods. To compute the <inline-formula><mml:math id="M35" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> statistic, first, each model's mean is computed from its members, and secondly, the multi-model ensemble mean and standard
deviation are calculated.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS4">
  <label>2.3.4</label><title>Weighting method</title>
      <p id="d1e1007">It has been argued that more robust projections could be obtained by giving more weight to members with good performance
<xref ref-type="bibr" rid="bib1.bibx39" id="paren.49"/>. Therefore, we compare historical simulations against the observational ensemble mean and more weight is given to those members
that better reproduce the observed climate, i.e. weighting them by performance. Another aspect that can be taken into account when weighting a
multi-model ensemble is the independence between members. Giving equal weight to all members (one model one vote) is not a fair approach as some share
model formulations (either because their runs belong to the same model or because their models share similarities), and would be overrepresented in
the ensemble. An independence weighting method is applied to correct this issue.</p>
      <p id="d1e1013">Using the approach developed in <xref ref-type="bibr" rid="bib1.bibx45" id="text.50"/>, <xref ref-type="bibr" rid="bib1.bibx12" id="text.51"/> and <xref ref-type="bibr" rid="bib1.bibx51" id="text.52"/>, we use Eq. (1) to give a weight <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to each
member <inline-formula><mml:math id="M37" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> in the projections ensemble. The distances (measured with the root mean squared error, RMSE) <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> between member <inline-formula><mml:math id="M39" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> and the observational
reference inform the performance weight, and the distance <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> between member <inline-formula><mml:math id="M41" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> and every other member <inline-formula><mml:math id="M42" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> from the multi-model ensemble informs
the independence weight. The amount of <inline-formula><mml:math id="M43" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> members is represented by <inline-formula><mml:math id="M44" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>, which is the total number of members minus one. <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the independence and performance shape parameters respectively. The mean of the observational ensemble is used as the
observational reference.
              <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M47" display="block"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:mfrac><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msup></mml:mrow><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>j</mml:mi><mml:mo>≠</mml:mo><mml:mi>i</mml:mi></mml:mrow><mml:mi>m</mml:mi></mml:msubsup><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:mfrac><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msup></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula></p>
      <p id="d1e1208">The weighting method distances account for different performance and independence diagnostics (trends, differences, variabilities and climatologies) to avoid weighting members that could match the performance and independence criteria of a single diagnostic just by chance. The diagnostics <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msub><mml:mi>s</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, respectively used to evaluate the distances <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, are different, as <xref ref-type="bibr" rid="bib1.bibx51" id="text.53"/> suggests. The aim when evaluating performance is to give more weight to members that resemble the observed past in a more faithful way. Differently, the aim of weighting for independence is to clearly identify members that behave in a similar way. All the diagnostics are computed over the period 1980–2014
<xref ref-type="bibr" rid="bib1.bibx12" id="paren.54"/>. The variables used to compute the diagnostics are TAS and PSL <xref ref-type="bibr" rid="bib1.bibx51" id="paren.55"/>. The performance diagnostics are the surface
temperature 1980–2014 CLIM minus its area average (TAS-DIFF), the surface temperature interannual standard deviation (TAS-STD), the surface
temperature linear trend (TAS-TREND), the sea-level pressure 1980–2014 CLIM minus its area-average (PSL-DIFF) and the sea-level pressure interannual
standard deviation (PSL-STD). The independence diagnostics are the 1980–2014 PSL and TAS climatologies (PSL-CLIM and TAS-CLIM).</p>
      <p id="d1e1271">The distances between member-observations for each of the diagnostics are aggregated as in Eq. (<xref ref-type="disp-formula" rid="Ch1.E2"/>) where <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represents the distance for
each diagnostic <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mi>d</mml:mi></mml:msup><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mtext>TAS-TREND</mml:mtext><mml:mo>,</mml:mo><mml:mtext>TAS-DIFF</mml:mtext><mml:mo>,</mml:mo><mml:mtext>TAS-STD</mml:mtext><mml:mo>,</mml:mo><mml:mtext>PSL-DIFF</mml:mtext><mml:mo>,</mml:mo><mml:mtext>PSL-STD</mml:mtext><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Equation (<xref ref-type="disp-formula" rid="Ch1.E3"/>) shows how to
compute the distances between models and observations, where <inline-formula><mml:math id="M54" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> refers to each grid cell and <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represents its area weight. To find
<inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> the same method is followed but using <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mi>s</mml:mi></mml:msup><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mtext>TAS-CLIM</mml:mtext><mml:mo>,</mml:mo><mml:mtext>PSL-CLIM</mml:mtext><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and comparing members against each other instead of
observations.

                  <disp-formula specific-use="align" content-type="numbered"><mml:math id="M58" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mi>d</mml:mi></mml:msup></mml:mrow></mml:munder><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi>d</mml:mi><mml:mi>i</mml:mi><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mi>d</mml:mi></mml:msup></mml:mrow></mml:msubsup></mml:mrow><mml:mrow><mml:msub><mml:mtext>MEDIAN</mml:mtext><mml:mi>i</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:msubsup><mml:mi>d</mml:mi><mml:mi>i</mml:mi><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mi>d</mml:mi></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd><mml:mtext>3</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msubsup><mml:mi>d</mml:mi><mml:mi>i</mml:mi><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mi>d</mml:mi></mml:msup></mml:mrow></mml:msubsup><mml:mo>=</mml:mo><mml:msqrt><mml:mrow><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mi>g</mml:mi></mml:munder><mml:msub><mml:mi>w</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub><mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>i</mml:mi><mml:mi>d</mml:mi></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">obs</mml:mi><mml:mi>d</mml:mi></mml:msubsup></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msqrt></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d1e1500">The shape parameters are constant values that determine if the member-observations or the member–member distances are enough to downweight a member
(<inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) or if they are close enough to determine some dependency between members (<inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) respectively. Each ensemble
(CMIP5 and CMIP6), season and scenario has its own associated shape parameters. Appendix <xref ref-type="sec" rid="App1.Ch1.S2"/> explains in further detail the meaning of
the shape parameters, the methods used to compute them and the diagnostics used to determine performance and independence.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
      <p id="d1e1537">Apart from the figures displayed in this section and the Supplement, additional ones generated during the study can be found in a shiny
app in the following link <uri>https://earth.bsc.es/shiny/medprojections-shiny_app/</uri> (last access: December 2021).</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Verification</title>
      <p id="d1e1550">We compare CMIP and HighResMIP ensemble TAS and PR trends to the observational ensemble trends between 1980 and 2014 as an indication of model
performance over the Mediterranean. PR and TAS trends in the observational ensemble fall within the range of the multi-model ensembles in all seasons
(see Fig. 1 for DJF and JJA results; MAM and SON not shown). The historical multi-model ensemble spread of temperature trends is notably larger<?pagebreak page326?> than
that of the observational ensemble. CMIP6 past warming trends are generally larger than CMIP5. The inter-model spread for the precipitation
projections is large for all ensembles and usually has both negative and positive trends (e.g. DJF CMIP5 precipitation trends range from <inline-formula><mml:math id="M61" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.092 to
0.097 <inline-formula><mml:math id="M62" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">d</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">decade</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> for the 5th and 95th percentiles respectively). HighResMIP TAS trends are contained within the CMIP6 ensemble,
but some of the high-resolution (HR) models exhibit trends outside the CMIP6 range for PR in JJA (Fig. <xref ref-type="fig" rid="Ch1.F1"/>d). The agreement between the
different observational products in past warming trends is shown in Fig. S7 (columns 1 and 5). While the general warming patterns
are similar, there are some notable differences over the Balkans and western Asia. The figure also highlights the need to consider multiple
observational sources, as historical trends differ both in magnitudes and spatial patterns.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e1590">Historical trends for DJF <bold>(a, b)</bold> and JJA <bold>(c, d)</bold> temperature <bold>(a, c)</bold> and precipitation <bold>(b, d)</bold> of the observational, CMIP5, CMIP6 and HighResMIP ensembles. The observational distribution is composed of the different values obtained from each of the observational products. In the box plots, the black horizontal line represents the median and the black dot is the mean. The interquartilic range (IQR) and whiskers are defined by the 25th–75th and 5th–95th percentiles respectively. HighResMIP models  are displayed as markers, enabling a comparison of the HR (green) and LR (orange) models within the experiment. The same markers are used for two different resolution runs of the same model (see Table S1 in the Supplement).</p></caption>
          <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://esd.copernicus.org/articles/13/321/2022/esd-13-321-2022-f01.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1613">Mediterranean region TAS (upper rows) and PR (lower rows) change differences with respect to the mean global temperature change and the mean 30–45<inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N latitudinal belt precipitation change respectively. The changes for the periods 2041–2060 (first and third row) and 2081–2100 (second and fourth row) are evaluated against the 1986–2005 mean. The differences are shown for the CMIP5 (left) and CMIP6 (right) DJF, JJA and annual mean projections (columns) under the high emission scenario RCP8.5 and SSP5-8.5 respectively. N indicates the number of models included in the ensemble mean.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://esd.copernicus.org/articles/13/321/2022/esd-13-321-2022-f02.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>The Mediterranean as a climate change hotspot</title>
      <p id="d1e1641">Figure <xref ref-type="fig" rid="Ch1.F2"/> shows CMIP5 and CMIP6 high radiative forcing scenario differences of <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> over the Mediterranean against the
1986–2005 global-mean <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> (for DJF, JJA and the annual means). The Mediterranean <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>PR</mml:mtext></mml:mrow></mml:math></inline-formula> is compared to the
30–45<inline-formula><mml:math id="M67" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N latitudinal belt <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>PR</mml:mtext></mml:mrow></mml:math></inline-formula> mean.</p>
      <p id="d1e1696">The Mediterranean region shows a higher annual temperature increase than the global mean. When accounting for seasonal differences, the highest
amplifications are visible for JJA over the Iberian Peninsula and the Balkans. CMIP5 and CMIP6 agree on the regions showing the highest amplified
warming, but the latter projects larger amplification magnitudes. There is agreement between both CMIPs in the distribution and magnitude of the DJF
warming amplification, which is small and even negative in the north-west part of the domain. While projections agree on a precipitation increase in
the 30–45<inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N latitudinal belt for the long-term period <xref ref-type="bibr" rid="bib1.bibx43" id="paren.56"/>, the Mediterranean region shows a decline in precipitation. The largest amplified drying shifts latitudinally from the south of the Mediterranean region in DJF to the north in JJA. The most affected region in JJA is projected to be the south-west of the Iberian Peninsula. Both CMIPs agree on the precipitation patterns of change, but CMIP6 dries more and faster in the amplified drying regions, and projects larger precipitation increases in regions where the hotspot has a negative sign such as the south-east of the domain (probably enhanced by using relative precipitation changes).</p>
      <p id="d1e1711">TAS and PR differences increase in magnitude from the mid- to the long term, while the spatial pattern remains the same, indicating that the climate in the Mediterranean changes faster than the global average when forced by the 8.5 <inline-formula><mml:math id="M70" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> scenarios. The low emission scenario, instead, shows a hotspot weakening from the mid- to the long term as the warming amplification is reduced and the precipitation differences are maintained (see Fig. S1 in the Supplement). The weakening of the hotspot under the low emission scenario will be further explored below.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1734">Mediterranean region warming against global warming for the three scenarios (columns) shown in DJF <bold>(a–c)</bold> and JJA <bold>(d–f)</bold> for the CMIP5 and CMIP6 ensemble means. Each dot represents a 10 year mean change beginning from 1960–1969 (light colouring) until 2091–2100 (opaque colouring). The changes are computed with 1986–2005 as baseline. An ordinary least squares linear regression is computed and the slope and <inline-formula><mml:math id="M71" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> values are shown. <inline-formula><mml:math id="M72" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> indicates the number of models included in the ensemble mean.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://esd.copernicus.org/articles/13/321/2022/esd-13-321-2022-f03.png"/>

        </fig>

      <p id="d1e1763">Even though CMIP6 projects a larger warming and drying amplification than CMIP5, Fig. <xref ref-type="fig" rid="Ch1.F3"/> shows that CMIP5 and CMIP6 agree on the
relation between global and local warming (slopes drawn in the figures). This indicates that CMIP6 does not enhance the hotspot with respect to
CMIP5, but rather the higher amplified warming in the Mediterranean is the result of a globally warmer multi-model ensemble. For DJF, additional
warming over the Mediterranean is almost zero with respect to the global mean. Contrastingly for JJA, additional warming over the Mediterranean is
about 1.6 times higher than the global-mean warming. This relationship appears to be linearly maintained for higher global warming levels,
i.e. with time and GHG concentrations.</p>
      <?pagebreak page328?><p id="d1e1768">In spite of this strong agreement in the relationship between global and local warming, CMIP5 and CMIP6 have slight differences in the projected
precipitation over the Mediterranean in comparison to the 30–45<inline-formula><mml:math id="M73" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N latitudinal belt (see Fig. S2). CMIP5 generally shows
more negative slopes than CMIP6, meaning that the former is projecting a larger amplification of the precipitation hotspot as the relative
precipitation loss in the Mediterranean (ordinate) for the same amount of precipitation increase in the larger-scale region (abscissa) is
larger. While this is true for all seasons and scenarios, the difference between CMIP5 and CMIP6 is more noticeable during DJF and especially for the
low emission scenario. Figure S3 highlights more extreme relative CMIP6 precipitation changes in the latitudinal band and increases
of over 30 % in Asia and over the Pacific as opposed to CMIP5. Therefore, conclusions must be drawn carefully from comparing area-averaged values
of these regions. Nevertheless, there is agreement between both ensembles on the spatial distribution of PR changes.</p>
      <p id="d1e1780">We tried following a second approach to assess the trend differences of the precipitation hotspot between the CMIPs. Figure S4 shows
changes in precipitation for the Mediterranean region against the global-mean warming, and the ensemble that dries faster for the same magnitude of
global warming is CMIP5. This is more noticeable during the DJF season. The results from Fig. S4, together with Fig. S2, give evidence supporting
that CMIP5 projects a larger precipitation hotspot (relative to its own large-scale climate response) than CMIP6.</p>
      <p id="d1e1783">Coming back to the hotspot weakening, the low emission scenario panels (Figs. S2a and d and S4a and d) show more clearly how a recovery of the
precipitation decline is projected following mitigation. For the rest of the scenarios, the projected amplified warming, combined with an anomalous
precipitation decline, makes the Mediterranean a climate change hotspot <xref ref-type="bibr" rid="bib1.bibx43" id="paren.57"/>.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Unweighted projections</title>
<sec id="Ch1.S3.SS3.SSS1">
  <label>3.3.1</label><title>Temperature</title>
      <p id="d1e1804">Figure <xref ref-type="fig" rid="Ch1.F4"/>a shows projected multi-model ensemble JJA and DJF TAS changes under three scenarios and three time horizons over the
Mediterranean. The CMIP6 ensemble always shows larger <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> than CMIP5. The inter-model spread for the end of the century is larger for CMIP6
than CMIP5. CMIP6 projects JJA temperatures to increase by over 7.4 <inline-formula><mml:math id="M75" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> (90 % inter-model spread within 5.6 to
9.1 <inline-formula><mml:math id="M76" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) by the end of the century under the high emission scenario and 2.3 <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> (90 % within 1.2 to
3.3 <inline-formula><mml:math id="M78" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) under the low emission scenario (Fig. <xref ref-type="fig" rid="Ch1.F4"/>). CMIP5 shows a mean JJA warming of 5.9 <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> by the end of
the century (90 % within 4.1 to 7.7 <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) under RCP8.5 and 1.6 <inline-formula><mml:math id="M81" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> (90 % within 0.3 to 2.5 <inline-formula><mml:math id="M82" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>)
under RCP2.6. In DJF the warming is always lower, and 90 % of CMIP6 models for the high emission scenario project a <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> within 3.3
to 6.8 <inline-formula><mml:math id="M84" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> (CMIP5: 2.7 to 5.0 <inline-formula><mml:math id="M85" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>). For the remaining seasons (MAM and SON), CMIP6 shows a larger warming and larger
intermodel spread than CMIP5 (not shown). HighResMIP HR and low-resolution (LR) projections are contained within the CMIP5 and CMIP6 distributions
(only near term; see Fig. S5c). No specific relation between the LR and HR model outputs can be found, and due to the small size of
the HighResMIP ensemble, further conclusions cannot be drawn. Finally, from the area-averaged distributions of <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F4"/>a)
we can see that the largest source of uncertainty for the mid- and long term is the forcing scenario, and the inter-model spread for the near term.</p>
      <p id="d1e1965">The inter-model spread grows larger with emissions both for TAS and PR (Fig. <xref ref-type="fig" rid="Ch1.F4"/>a and c). To check the influence of the equilibrium climate
sensitivity (ECS) on the increasing inter-model spread, the same plot is computed with a subset of CMIP5 and CMIP6 models with ECSs constrained
between 2.6 and 3.3 <inline-formula><mml:math id="M87" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> (rather than the original 2.1 to 4.7 <inline-formula><mml:math id="M88" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ECS range from CMIP5, <xref ref-type="bibr" rid="bib1.bibx49" id="altparen.58"/> and the 1.8 to 5.6 <inline-formula><mml:math id="M89" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ECS range from CMIP6, <xref ref-type="bibr" rid="bib1.bibx32" id="altparen.59"/>). From Fig. S6 it can be seen that ensembles with narrower ECS ranges show a reduction in inter-model spread
growth over time for the high emission scenarios.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e2015">CMIP5 and CMIP6 JJA and DJF projections for the near-, mid- and long-term periods with respect to the baseline period considering the 2.6, 4.5 and 8.5 <inline-formula><mml:math id="M90" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> RCP and SSP radiative forcing scenarios for <bold>(a)</bold> unweighted <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula>, <bold>(b)</bold> weighted <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> and <bold>(c)</bold> unweighted <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>PR</mml:mtext></mml:mrow></mml:math></inline-formula>. The black horizontal line in the boxes represents the median and the black dot is the mean. The interquartile range (IQR) and whiskers are defined by the 25th–75th and 5th–95th percentiles respectively. The number of members in the boxplot distributions is represented by <inline-formula><mml:math id="M94" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> in the legend.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://esd.copernicus.org/articles/13/321/2022/esd-13-321-2022-f04.png"/>

          </fig>

      <p id="d1e2089">Figure <xref ref-type="fig" rid="Ch1.F5"/> shows the spatial distribution of the projected JJA warming in the high emission scenario for CMIP5, CMIP6 and HighResMIP in the
three future reference periods. JJA warming is significant and robust for the three future periods in the Mediterranean region (see
Fig. <xref ref-type="fig" rid="Ch1.F5"/>). As seen before, CMIP6 warms more than CMIP5 and at a faster rate. Nevertheless, there is good spatial agreement between the
warming projected by the CMIP experiments over the Mediterranean region. The Iberian Peninsula, the Balkans and Eastern Europe are the regions with
the largest mean JJA warming, with values reaching over 8 <inline-formula><mml:math id="M95" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d1e2108">The remaining scenarios also project robust and significant warming for JJA throughout the century with a tendency of smaller positive trends by 2050
(not shown). CMIP6 systematically projects higher warming than CMIP5 again with a similar spatial warming pattern. The regions with larger warming are
the Iberian Peninsula and the Balkans.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e2113">JJA <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> according to CMIP5, CMIP6 and HighResMIP ensemble means (columns) for the three relevant future periods (rows), under the RCP8.5 and SSP5-8.5 scenarios. The time series plot shows the anomalies in the Mediterranean region with respect to the period 1986–2005 for the multi-model ensembles and  the observational references. A solid line indicates the one-member-per-model ensemble mean and the shaded region indicates the 5th–95th percentiles range. The CRU trend for the period 1980–2014 is shown along with the dashed line, which bounds the Mediterranean region.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://esd.copernicus.org/articles/13/321/2022/esd-13-321-2022-f05.png"/>

          </fig>

      <p id="d1e2132">The temperature spatial changes during DJF for the high emission scenario are shown in Fig. S8. The north-eastern Mediterranean
shows the largest projected warming in DJF (4.5 <inline-formula><mml:math id="M97" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> according to CMIP5 and 6 <inline-formula><mml:math id="M98" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> to CMIP6). For the near term,
HighResMIP shows a slightly larger TAS increase than CMIP6 in eastern Europe. The rest of scenarios agree with the spatial distribution of changes but
with lower warming magnitudes (not shown).</p>
</sec>
<sec id="Ch1.S3.SS3.SSS2">
  <label>3.3.2</label><title>Precipitation</title>
      <?pagebreak page329?><p id="d1e2167">In contrast to temperature, CMIP5 and CMIP6 show the same mean JJA <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>PR</mml:mtext></mml:mrow></mml:math></inline-formula> declines of <inline-formula><mml:math id="M100" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>33 % by the end of the century under the high
emission scenario (Fig. <xref ref-type="fig" rid="Ch1.F4"/>c). CMIP6 has a wider inter-model 90 % range than CMIP5. The former spans <inline-formula><mml:math id="M101" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>63 % to <inline-formula><mml:math id="M102" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4 % and
the latter <inline-formula><mml:math id="M103" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>56 % to <inline-formula><mml:math id="M104" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>11 %. For the low emission scenario CMIP6 mean JJA precipitation declines by <inline-formula><mml:math id="M105" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7 % (90 % within
<inline-formula><mml:math id="M106" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>23 % to +17 %) and CMIP5 by <inline-formula><mml:math id="M107" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4 % (90 % within <inline-formula><mml:math id="M108" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>19 % to +16 %). In DJF and by the end of the century, CMIP6
precipitation declines by <inline-formula><mml:math id="M109" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8 % (90 % within <inline-formula><mml:math id="M110" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20 % to +5 %) and CMIP5 by <inline-formula><mml:math id="M111" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9 % (90 % within <inline-formula><mml:math id="M112" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>31 % to +4 %)
under the high emission scenario. For the low emission scenario in DJF, CMIP6 shows a mean +2 % precipitation increase (90 % within
<inline-formula><mml:math id="M113" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>11 % to +18 %) and CMIP5 a <inline-formula><mml:math id="M114" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1 % decline (90 % within <inline-formula><mml:math id="M115" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 % to 9 %). Seasons JJA, DJF (Fig. <xref ref-type="fig" rid="Ch1.F4"/>c), MAM and SON
(not shown) for all scenarios generally project mean <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>PR</mml:mtext></mml:mrow></mml:math></inline-formula> declines beginning from the mid-term period onwards. Nevertheless, there is an
exception in DJF under the low emission scenario, where a slight increase in mean DJF precipitation is projected. HighResMIP near-term projections of
PR change are contained within the CMIP6 ensemble (Fig. S5b and d). Generally, the signal is considerable, but the inter-model spread is wide for all
multi-model ensembles; therefore, we will later present the statistical robustness and significance of changes. Finally, from the area-averaged
distributions of <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>PR</mml:mtext></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F4"/>c), we see that the largest source of uncertainty is the forcing scenario for long-term JJA
projections, and the inter-model spread for DJF and near and mid-term JJA.</p>
      <p id="d1e2321">Precipitation spatial changes in the Mediterranean region only become more robust and significant with time (see Fig. <xref ref-type="fig" rid="Ch1.F6"/>). <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>PR</mml:mtext></mml:mrow></mml:math></inline-formula>
projected for the long term during JJA, and under the 8.5 <inline-formula><mml:math id="M119" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> scenarios, indicate significant and robust decline for most of the
region. The mid-term 8.5 <inline-formula><mml:math id="M120" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and the long-term 4.5 <inline-formula><mml:math id="M121" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> scenarios show locally robust and significant changes in the
Iberian Peninsula and north of the Pyrenees. Both CMIPs agree on the south-western Iberian Peninsula having the strongest precipitation decline, with
long-term CMIP6 changes ranging from <inline-formula><mml:math id="M122" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>50 % to <inline-formula><mml:math id="M123" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>60 % and CMIP5 from <inline-formula><mml:math id="M124" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>30 % to <inline-formula><mml:math id="M125" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>40 % for the high emission scenario. Despite lower
forcing scenarios projecting less robust and significant changes (except the western Mediterranean for long-term SSP2-4.5), the results agree on a
general precipitation decline throughout the region with patterns similar to high emission scenario projections (not shown). The HighResMIP
projections agree with CMIP6 mean magnitudes and spatial pattern for most of the seasons in the near-term<?pagebreak page330?> period (the large amount of non-robust and
non-significant grid points must be noted).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e2418">Same as Fig. <xref ref-type="fig" rid="Ch1.F5"/> for JJA precipitation and showing CRU in the top left panel.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://esd.copernicus.org/articles/13/321/2022/esd-13-321-2022-f06.png"/>

          </fig>

      <p id="d1e2430"><inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>PR</mml:mtext></mml:mrow></mml:math></inline-formula>s in DJF are different from those in JJA (see Fig. S9). The southern part of the domain is expected to see a
significant and robust precipitation decline in the long term of up to <inline-formula><mml:math id="M127" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20 % to <inline-formula><mml:math id="M128" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>40 % over northern Africa. The north of the Mediterranean
is located in a transition zone, as precipitation in areas north of the Pyrenees, Alps and Balkan Peninsula is projected to increase and in areas under
38<inline-formula><mml:math id="M129" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N is projected to decrease, causing changes for the Iberian, Italian and Balkan peninsulas to remain uncertain. In comparison to CMIP5,
CMIP6 shows a wider 5th–95th percentile spread over the Mediterranean region for all the scenarios considered (2.6 and 4.5 <inline-formula><mml:math id="M130" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> scenarios
are not shown). As a final remark, the observed DJF precipitation variability in the time series falls outside the simulated 90 % inter-model
spread (5th-95th percentiles shown in shading in Fig. <xref ref-type="fig" rid="Ch1.F6"/>).</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Weighted projections</title>
      <p id="d1e2495">The models of CMIP ensembles perform very differently depending on the computed diagnostic, and some models share similarities. Section 1 of the
Supplement explains in further detail how differently models represent the observed climate over the Mediterranean region, justifying the
need to constrain the projection ensembles.</p>
      <p id="d1e2498">We obtain new projections from applying the performance and independence weighting method to TAS projections from the CMIP5 and CMIP6 ensembles. Figure <xref ref-type="fig" rid="Ch1.F4"/>b shows the distribution of <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> in the weighted ensembles for the three emission scenarios and the three
future periods. The weighting increases the CMIP5 mean and median projections while at the same time decreasing the CMIP6 mean and median projections,
bringing the two ensemble means closer together: before weighting, the CMIP5 and CMIP6 medians differed by 1.32 <inline-formula><mml:math id="M132" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> and after weighting the
difference is 0.68 <inline-formula><mml:math id="M133" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> (for the highest emission scenario in JJA).<?pagebreak page331?> Generally, the high emission scenario means are those that see larger reductions in the CMIP6 ensemble; e.g. differences between the unweighted and weighted ensemble means are around <inline-formula><mml:math id="M134" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.3, <inline-formula><mml:math id="M135" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.2 and <inline-formula><mml:math id="M136" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.1 <inline-formula><mml:math id="M137" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> in JJA and DJF for SSPs 5-8.5, 2-4.5 and 1-2.6 respectively. The IQRs are generally narrowed for all seasons and scenarios
except for the mid- and long-term JJA SSP2-4.5, SSP1-2.6 and RCP2.6 scenarios. The 90 % spreads are slightly reduced or maintained; exceptions are the CMIP6 DJF long-term distributions and the CMIP6 JJA low and middle emission scenarios for the mid-term. The 75th–95th percentile range in the weighted CMIP6 ensemble increases while the 5th–25th percentile range decreases, generating a skewed weighted CMIP6 distribution towards smaller warming. Weighting the CMIP5 ensemble leads to a more constrained distribution.</p>
      <p id="d1e2571">The weighted <inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>TAS</mml:mtext></mml:mrow></mml:math></inline-formula> projections in DJF show similar responses as in JJA: the mean signal in CMIP6 decreases while it increases in CMIP5,
making the differences between both mean distributions smaller. In some cases the weighting did not lead to large alterations of the projected
inter-model spread, suggesting that uncertainties in the temperature changes are well sampled by the original ensembles. In contrast, the large IQR of
CMIP6 model projections in the long term is reduced by half, and the CMIP5 90 % inter-model spread narrows by up to 1 <inline-formula><mml:math id="M139" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, after
weighting. Nevertheless, even though the weighting approach reduces the probability of the most extreme warming values, they remain possible in the
weighted ensemble. Generally speaking, the 90 % inter-model spreads are maintained while the IQRs narrow.</p>
      <p id="d1e2596">To assess the contribution of the performance and independence weights in the resulting distribution, we have plotted the distribution of performance
and full weights, and compared the raw ensemble long-term warming distribution with the performance-weighted and the fully weighted warmings (Fig. S12). JJA performance shifts both CMIP ensembles to larger warmings, while the addition of independence weights shifts the CMIP6 median to
lower warmings than the raw<?pagebreak page332?> ensemble. DJF performance weights do not have an effect on the warming medians but they the narrow CMIP5 spread. The addition
of DJF independence weighting shifts the CMIP6 median warming and broadens its inter-model spread. The CMIP5 median remains unchanged but its spread grows
toward the raw distribution without reaching it.</p>
      <p id="d1e2600">Note that precipitation-weighted projections are not shown as there is no evidence that the diagnostics used to assess temperature
<xref ref-type="bibr" rid="bib1.bibx51" id="paren.60"/> are relevant to the precipitation response of the models.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e2615">Projections obtained from climate multi-model ensembles contain various sources of uncertainties. Different modelling methods and emission scenarios
(e.g. land use, GHG emissions) lead to different results <xref ref-type="bibr" rid="bib1.bibx66" id="paren.61"/>. We use different multi-model ensembles and radiative forcing
scenarios to consider as many factors as possible contributing to the uncertainty of the Mediterranean climate change projections. Additionally, a
weighting method constraining the projections has been applied to reduce uncertainty in the projections.</p>
      <p id="d1e2621">We have shown that average Mediterranean temperature changes were larger than the global-mean average during JJA, but close to it during DJF, for all
scenarios, time periods and model ensembles. This hotspot is projected to enhance over the 21st century under the scenarios RCP8.5, SSP5-8.5, RCP4.5
and SSP2-4.5, and to diminish from the mid- to long term under the RCP2.6 or SSP1-2.6 scenarios. Interestingly, the multi-model ensemble mean
projections of the low emission scenario show a recovery of the precipitation decline towards the end of the century, suggesting that precipitation
could be restored to historical values relatively fast in the Mediterranean region if strict mitigation policies are applied. Previous studies also
have identified the Mediterranean warming amplification <xref ref-type="bibr" rid="bib1.bibx43 bib1.bibx80" id="paren.62"/>, but it must be stressed that this enhanced warming does not
apply to the DJF season.</p>
      <p id="d1e2627">We argue that the different results obtained from CMIP5 and CMIP6 for the Mediterranean hotspot and the unweighted projections are largely due to the
global response from each multi-model ensemble. Figures <xref ref-type="fig" rid="Ch1.F3"/>, S2 and S4 show how the regional changes relative to the larger scale are similar
for both CMIPs, indicating that CMIP6 is not producing a regional enhancement of climate change, but it rather follows a larger global change. This
behaviour is most evident in JJA than in DJF, as the relative changes with respect to larger scales are more similar for the two multi-model
ensembles. To further support this statement, we look at the spatial distribution of changes within the Mediterranean region in
Figs. <xref ref-type="fig" rid="Ch1.F5"/>, <xref ref-type="fig" rid="Ch1.F6"/>, S3, S8 and S9. The figures generally agree on the spatial distribution of changes even if the magnitudes
differ. Therefore, we can argue that the main difference in TAS and PR output from the older (CMIP5) and newer generation (CMIP6) multi-model
ensembles is an enhancement of the global change, while its relation with the Mediterranean region response has been maintained. The work of
<xref ref-type="bibr" rid="bib1.bibx55" id="text.63"/> arrives at a similar conclusion for the European region.</p>
      <p id="d1e2639">The drivers of the projected Mediterranean climate change has been studied by <xref ref-type="bibr" rid="bib1.bibx9" id="text.64"/>, <xref ref-type="bibr" rid="bib1.bibx10" id="text.65"/> and <xref ref-type="bibr" rid="bib1.bibx69" id="text.66"/>. They have
found that the mechanisms projected to drive the Mediterranean climate are large-scale upper-tropospheric flow changes (PR in DJF), reduction in the
regional land–sea temperature gradient (PR in DJF and JJA) and changes in the north–south lapse rate contrast (PR in JJA, TAS in DJF and JJA). While
these drivers have been deeply studied for CMIP5, affirming that the same mechanisms remain valid for the CMIP6 ensemble would be speculative.</p>
      <p id="d1e2652">Consistent with basic radiative forcing theory <xref ref-type="bibr" rid="bib1.bibx75" id="paren.67"/>, temperature projections have shown that the warming over the 21st century is
larger when stronger radiative forcing scenarios are applied. There is confidence in a precipitation decline for the high emission scenario over the
whole Mediterranean region in JJA and only in the south during DJF. Conclusions should be drawn carefully from precipitation as there is a large
inter-model spread. For other seasons and scenarios, precipitation declines are projected, although results are uncertain due to the large spread and low
significance and robustness over most of the region. Regarding HighResMIP, the HR near-term precipitation and temperature changes generally fall
within the CMIP6 ensemble distribution and no clear improvement could be seen from the increased resolution in the historical trends, probably due to
the small number of HighResMIP models available for the assessment, and the focus on larger-scale changes and temporal resolutions.</p>
      <p id="d1e2658">The largest source of uncertainty in determining the warming and precipitation changes over the mid- and long-term periods is the emission scenario (as seen
in Fig. <xref ref-type="fig" rid="Ch1.F4"/>). To illustrate scenario uncertainty, let us take the range between the 5th and 95th percentile of the low (high) and high
(low) emission scenario distributions for temperature (precipitation) changes. CMIP6 shows a range from 1 to 9 <inline-formula><mml:math id="M140" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> warming and
<inline-formula><mml:math id="M141" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>62 % to 19 % precipitation long-term changes in JJA. CMIP5 ranges from 0.1 to 7.5 <inline-formula><mml:math id="M142" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> warming and <inline-formula><mml:math id="M143" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>54 % to
18 %. This broad spectrum of possible futures has various possible associated outcomes. The inter-model spread grows at faster rates throughout the
21st century with higher radiative forcing, in part due to the differing climate sensitivities of the models inside the ensemble (see Fig. S6);
i.e. the differences between a low and a high climate sensitivity model will become amplified with larger radiative forcing.</p>
      <?pagebreak page333?><p id="d1e2701">The implications of an 8.5 <inline-formula><mml:math id="M144" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> increase in radiative forcing from preindustrial times by the end of the century could pose severe
strains on human health, due to heat-related illnesses <xref ref-type="bibr" rid="bib1.bibx46" id="paren.68"/> and altered transmission of infectious diseases <xref ref-type="bibr" rid="bib1.bibx56" id="paren.69"/>; food
security due to crop pests and diseases <xref ref-type="bibr" rid="bib1.bibx52" id="paren.70"/> and productivity declines in many countries whose economies depend on agriculture
<xref ref-type="bibr" rid="bib1.bibx20" id="paren.71"/>; water insecurity due to droughts <xref ref-type="bibr" rid="bib1.bibx20" id="paren.72"/> and changing rainfall patterns in vulnerable regions
<xref ref-type="bibr" rid="bib1.bibx63" id="paren.73"/>. Note that the three climate change-induced impacts defined above are closely intertwined and may increase existing scarcities.</p>
      <p id="d1e2740">In face of the very pessimistic future projected by the high emission scenario, some studies argue that 8.5 <inline-formula><mml:math id="M145" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> forcing is highly
unlikely as it is based on an expansion of coal use throughout the 21st century instead of on a reduction <xref ref-type="bibr" rid="bib1.bibx60" id="paren.74"/>. In the context of energy
transition and decreasing demand for coal, the high emission scenario has often been criticized <xref ref-type="bibr" rid="bib1.bibx61" id="paren.75"/>. Nevertheless, studies on the carbon cycle
discuss that <inline-formula><mml:math id="M146" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> feedbacks might be underestimated in the GHG concentration scenarios <xref ref-type="bibr" rid="bib1.bibx6" id="paren.76"/>, and thus we have considered keeping
the 8.5 scenarios as an extreme yet possible future.</p>
      <p id="d1e2780">The CMIP6 ensemble is known to have models with notably higher climate sensitivity than CMIP5; i.e. radiative forcing generates stronger changes and
at a faster rate <xref ref-type="bibr" rid="bib1.bibx32" id="paren.77"/>. The higher sensitivity could be due to model design or the definition of the radiative forcing scenario. Even if
SSP and RCP scenarios are labelled after the radiative forcing (in <inline-formula><mml:math id="M147" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) by the end of the century, the transient GHG concentrations are
different <xref ref-type="bibr" rid="bib1.bibx50 bib1.bibx58" id="paren.78"/>. Wyser et al. (2020) suggests that running the same model with equal 2100 GHG concentrations from SSP and
RCP (2.6, 4.5 and 8.5 <inline-formula><mml:math id="M148" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) leads to larger temperature changes when forcing the model with the former. It has been argued that
improvements in the formulation of clouds and aerosols in CMIP6 are major contributors to larger climate sensitivities with respect to CMIP5
<xref ref-type="bibr" rid="bib1.bibx49 bib1.bibx32" id="paren.79"/>. Even if there is higher sensitivity to radiative forcing in some CMIP6 models, this behaviour is not reproduced by
all of them, resulting in a larger inter-model spread compared to CMIP5.</p>
      <p id="d1e2826">In terms of which multi-model ensemble performs better, some studies argue that the CMIP6 ensemble shows improvements in simulating the climate of historical references in China <xref ref-type="bibr" rid="bib1.bibx79" id="paren.80"/>, Turkey <xref ref-type="bibr" rid="bib1.bibx2" id="paren.81"/>, the Tibetan plateau <xref ref-type="bibr" rid="bib1.bibx47" id="paren.82"/> and the global mean <xref ref-type="bibr" rid="bib1.bibx25" id="paren.83"/>. Nevertheless, as no performance studies have been made specifically for the Mediterranean region, we cannot speculate as to which ensemble performs better. Therefore, this would be a topic of interest for further study.</p>
      <p id="d1e2842">Assessing the weighted temperature ensemble, we found that the CMIP6 distribution shifts to lower changes, meaning that models showing larger TAS
changes have been down-weighted, reducing the differences between CMIP6 and CMIP5 experiment medians and means. To find the reason behind this shift
we plotted the ensemble warming distribution for the long term after applying only the performance weights (numerator of equation <xref ref-type="disp-formula" rid="Ch1.E1"/>) and
compared it to the raw and fully weighted ensembles (see Fig. S12). We found that the independence weights are those shifting the CMIP6 ensemble to
lower warmings rather than the performance. In this regard, CMIP5's median is unaltered by independence and its effect can only be seen in
inter-model spread changes. JJA performance weights shift CMIP5 and CMIP6 to larger warmings, suggesting that a number of the members projecting
larger changes do a better job at representing the historical climate. A last remark that can be extracted from Fig. S12 is that both independence and
performance weighting play an important role, which changes between seasons and ensembles. Therefore, there is not a straightforward interpretation of
the general behaviour of the weights.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d1e2856">This study aims to analyse the projected temperature and precipitation changes by the CMIP5 and CMIP6 multi-model ensembles in the Mediterranean
region. Different scenarios and seasons have been assessed to tackle the uncertainties inherent to ensemble projections. To complement the traditional
information provided, a weighting method that accounts for historical performance and inter-independence of the models has been applied to offer an
alternative view of the temperature projections.</p>
      <p id="d1e2859">The Mediterranean is a climate-change hotspot due to amplified warming and drying when compared to the large-scale climate behaviour. The
amplified warming of the Mediterranean is found in JJA and not in DJF. Comparing the Mediterranean hotspot in CMIP5 and CMIP6, we found that the ratio
of warming amplification is similar for both multi-model means, meaning that no enhanced regional warming is projected by the CMIP6 ensemble, but it
is rather the consequence of a globally warmer ensemble.</p>
      <p id="d1e2862">Conclusions must be drawn carefully from multi-model ensembles as the single models perform very differently and might share dependencies with each
other. Model agreement gives high confidence in significant and robust warming affecting the entire Mediterranean region throughout the 21st century caused
by anthropogenic emissions. The Balkan Peninsula during DJF and the Balkan and Iberian peninsulas during JJA are expected to be the most affected
regions. Precipitation changes are less robust and significant and show greater spatial heterogeneity than the warming. Significant and robust
declines in precipitation are expected to affect the Mediterranean in JJA and the southern part in winter by the end of the 21st century if high
emission scenarios are considered. The warming combined with a precipitation decline could put the whole region under strain, especially the south,
which has fewer resources to adapt to the changing climate. The biggest source of uncertainty to determine the magnitude of TAS and PR changes is the
emission scenario, which<?pagebreak page334?> will depend on the future policies and measures for mitigation followed. Considering three scenarios, the
long-term projected warming (given by the 50 % inter-model spread) spans 1.83–8.49 <inline-formula><mml:math id="M149" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> according to CMIP6 and
1.22–6.63 <inline-formula><mml:math id="M150" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> according to CMIP5 in JJA. For precipitation, the decline ranges from <inline-formula><mml:math id="M151" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>49 % to <inline-formula><mml:math id="M152" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>16 % in CMIP6 and from
<inline-formula><mml:math id="M153" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>47 % to <inline-formula><mml:math id="M154" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22 % in CMIP5. It has also been concluded that part of the increasing warming inter-model spread with time is related to the
wide range of ECS values among the ensemble members.</p>
      <p id="d1e2918">A weighting method has been applied to reduce the uncertainty caused by models that poorly represent key aspects of the historical climate and by the
high dependence of the results provided by families of models (that might be overrepresented in the multi-model ensemble). Based on the constrained
projections, we conclude that CMIP6 overestimates warming in the Mediterranean and its 25th to 50th percentile inter-model spread. The shift to lower warming seen by the weighted CMIP6 ensemble is driven by the independence weighting. CMIP5 slightly underestimates warming and generally overestimates the IQR inter-model spread. The weighted projections are relevant because they help to reconcile the conclusions extracted from the last two CMIP phases, reducing future climate change uncertainties. The fact that CMIP6's 90 % spread range is unaltered shows that the climate uncertainty might have been underestimated in previous, less physically advanced, CMIP exercises, which displayed smaller inter-model spread when constrained.</p>
      <p id="d1e2922">Further work is required for the weighting method to identify the most relevant diagnostics that best assess historical precipitation model
performance. As spatial heterogeneities can be seen in the Mediterranean region, we suggest considering subregions for the Mediterranean in order to extract more user-relevant information from the constrained projections. Furthermore, it would be of great interest for the community to update studies on the physical mechanisms and the performance of the CMIP6 multi-model ensemble in the Mediterranean region.</p>
</sec>

      
      </body>
    <back><app-group>

<app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>Model data summary</title>
      <p id="d1e2936">A summary of all the initial-condition runs from the multi-model ensembles CMIP5, CMIP6 and HighResMIP for the three radiative scenarios used in this
study can be found in Table <xref ref-type="table" rid="App1.Ch1.S1.T3"/>.</p>

<?xmltex \floatpos{p}?><table-wrap id="App1.Ch1.S1.T3" specific-use="star" orientation="landscape"><?xmltex \currentcnt{A1}?><label>Table A1</label><caption><p id="d1e2944">Summary of the members used in this study from CMIP5, CMIP6 and HighResMIP. The columns display the emission scenarios.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.70}[.70]?><oasis:tgroup cols="10">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left" colsep="1"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:colspec colnum="7" colname="col7" align="left"/>
     <oasis:colspec colnum="8" colname="col8" align="left"/>
     <oasis:colspec colnum="9" colname="col9" align="left"/>
     <oasis:colspec colnum="10" colname="col10" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CMIP5</oasis:entry>
         <oasis:entry colname="col2">lat <inline-formula><mml:math id="M155" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> lon</oasis:entry>
         <oasis:entry colname="col3">RCP2.6</oasis:entry>
         <oasis:entry colname="col4">RCP4.5</oasis:entry>
         <oasis:entry colname="col5">RCP8.5</oasis:entry>
         <oasis:entry colname="col6">CMIP6</oasis:entry>
         <oasis:entry colname="col7">lat <inline-formula><mml:math id="M156" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> lon</oasis:entry>
         <oasis:entry colname="col8">SSP1-2.6</oasis:entry>
         <oasis:entry colname="col9">SSP2-4.5</oasis:entry>
         <oasis:entry colname="col10">SSP5-8.5</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">ACCESS1-0</oasis:entry>
         <oasis:entry colname="col2">1.25<inline-formula><mml:math id="M157" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M158" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M159" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">ACCESS-CM2</oasis:entry>
         <oasis:entry colname="col7">1.25<inline-formula><mml:math id="M160" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M161" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M162" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-2)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">ACCESS1-3</oasis:entry>
         <oasis:entry colname="col2">1.25<inline-formula><mml:math id="M163" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M164" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M165" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">ACCESS-ESM1-5</oasis:entry>
         <oasis:entry colname="col7">1.25<inline-formula><mml:math id="M166" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M167" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M168" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-3)i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-10)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r(1-3)i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">BCC-CSM1-1</oasis:entry>
         <oasis:entry colname="col2">2.8125<inline-formula><mml:math id="M169" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M170" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.8125<inline-formula><mml:math id="M171" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">AWI-CM-1-1-MR</oasis:entry>
         <oasis:entry colname="col7">0.9375<inline-formula><mml:math id="M172" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M173" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.9375<inline-formula><mml:math id="M174" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">BCC-CSM1-1-M</oasis:entry>
         <oasis:entry colname="col2">1.125<inline-formula><mml:math id="M175" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M176" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.125<inline-formula><mml:math id="M177" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">BCC-CSM2-MR</oasis:entry>
         <oasis:entry colname="col7">1.125<inline-formula><mml:math id="M178" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M179" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.125<inline-formula><mml:math id="M180" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">BNU-ESM</oasis:entry>
         <oasis:entry colname="col2">2.8125<inline-formula><mml:math id="M181" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M182" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.8125<inline-formula><mml:math id="M183" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">CanESM5</oasis:entry>
         <oasis:entry colname="col7">2.8125<inline-formula><mml:math id="M184" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M185" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.8125<inline-formula><mml:math id="M186" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-10)i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-10)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r(1-10)i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CanESM2</oasis:entry>
         <oasis:entry colname="col2">2.8125<inline-formula><mml:math id="M187" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M188" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.8125<inline-formula><mml:math id="M189" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r(1-5)i1p1</oasis:entry>
         <oasis:entry colname="col4">r(1-5)i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1-5)i1p1</oasis:entry>
         <oasis:entry colname="col6">CanESM5-CanOE</oasis:entry>
         <oasis:entry colname="col7">2.8125<inline-formula><mml:math id="M190" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M191" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.8125<inline-formula><mml:math id="M192" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-3)i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-3)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r(1-3)i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CCSM4</oasis:entry>
         <oasis:entry colname="col2">0.942406<inline-formula><mml:math id="M193" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M194" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M195" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r(1-5)i1p1</oasis:entry>
         <oasis:entry colname="col4">r(1-5)i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1-5)i1p1</oasis:entry>
         <oasis:entry colname="col6">CAS-ESM2-0</oasis:entry>
         <oasis:entry colname="col7">1.40625<inline-formula><mml:math id="M196" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M197" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.40625<inline-formula><mml:math id="M198" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">–</oasis:entry>
         <oasis:entry colname="col9">r(1,3)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1-BGC</oasis:entry>
         <oasis:entry colname="col2">0.942406<inline-formula><mml:math id="M199" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M200" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M201" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">CESM2</oasis:entry>
         <oasis:entry colname="col7">0.9375<inline-formula><mml:math id="M202" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M203" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M204" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1,4,10-11)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r(1,2)i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1-CAM5</oasis:entry>
         <oasis:entry colname="col2">0.942406<inline-formula><mml:math id="M205" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M206" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M207" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r(1-3)i1p1</oasis:entry>
         <oasis:entry colname="col4">r(1-3)i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1-3)i1p1</oasis:entry>
         <oasis:entry colname="col6">CESM2-WACCM</oasis:entry>
         <oasis:entry colname="col7">0.9375<inline-formula><mml:math id="M208" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M209" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M210" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-3)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CMCC-CESM</oasis:entry>
         <oasis:entry colname="col2">3.75<inline-formula><mml:math id="M211" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M212" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.75<inline-formula><mml:math id="M213" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">CIESM</oasis:entry>
         <oasis:entry colname="col7">0.9375<inline-formula><mml:math id="M214" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M215" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M216" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">–</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CMCC-CM</oasis:entry>
         <oasis:entry colname="col2">0.75<inline-formula><mml:math id="M217" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M218" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.75<inline-formula><mml:math id="M219" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">CMCC-CM2-SR5</oasis:entry>
         <oasis:entry colname="col7">0.9375<inline-formula><mml:math id="M220" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M221" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M222" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CMCC-CMS</oasis:entry>
         <oasis:entry colname="col2">1.875<inline-formula><mml:math id="M223" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M224" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M225" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">CNRM-CM6-1</oasis:entry>
         <oasis:entry colname="col7">1.40625<inline-formula><mml:math id="M226" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M227" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.40625<inline-formula><mml:math id="M228" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-6)i1p1f2</oasis:entry>
         <oasis:entry colname="col9">r(1-6)i1p1f2</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-CM5</oasis:entry>
         <oasis:entry colname="col2">1.40625<inline-formula><mml:math id="M229" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M230" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.40625<inline-formula><mml:math id="M231" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
         <oasis:entry colname="col5">r(1-2,4,6,10)i1p1</oasis:entry>
         <oasis:entry colname="col6">CNRM-CM6-1-HR</oasis:entry>
         <oasis:entry colname="col7">0.5<inline-formula><mml:math id="M232" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M233" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.5<inline-formula><mml:math id="M234" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f2</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f2</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CSIRO-Mk3-6-0</oasis:entry>
         <oasis:entry colname="col2">1.875<inline-formula><mml:math id="M235" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M236" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M237" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r(1-10)i1p1</oasis:entry>
         <oasis:entry colname="col4">r(1-10)i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1-10)i1p1</oasis:entry>
         <oasis:entry colname="col6">CNRM-ESM2-1</oasis:entry>
         <oasis:entry colname="col7">1.40625<inline-formula><mml:math id="M238" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M239" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.40625<inline-formula><mml:math id="M240" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-5)i1p1f2</oasis:entry>
         <oasis:entry colname="col9">r(1-5)i1p1f2</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">EC-Earth</oasis:entry>
         <oasis:entry colname="col2">1.125<inline-formula><mml:math id="M241" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M242" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.125<inline-formula><mml:math id="M243" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r(8,12)i1p1</oasis:entry>
         <oasis:entry colname="col4">r(2,6-9,12-14)i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1,2,6,8,9,12,13)i1p1</oasis:entry>
         <oasis:entry colname="col6">EC-Earth3</oasis:entry>
         <oasis:entry colname="col7">0.703125<inline-formula><mml:math id="M244" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M245" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.703125<inline-formula><mml:math id="M246" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(4,6,9,11,13,15)i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(2,7,18-24)i1p1f2</oasis:entry>
         <oasis:entry colname="col10">r(4,6,9,11,13,15)i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">FGOALS-s2</oasis:entry>
         <oasis:entry colname="col2">1.6667<inline-formula><mml:math id="M247" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M248" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.8125<inline-formula><mml:math id="M249" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1-3)i1p1</oasis:entry>
         <oasis:entry colname="col6">FGOALS-g3</oasis:entry>
         <oasis:entry colname="col7">2.25<inline-formula><mml:math id="M250" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M251" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2<inline-formula><mml:math id="M252" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-4)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">FIO-ESM</oasis:entry>
         <oasis:entry colname="col2">2.8125<inline-formula><mml:math id="M253" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M254" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.8125<inline-formula><mml:math id="M255" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r(1:3)i1p1</oasis:entry>
         <oasis:entry colname="col4">r(1-3)i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1-3)i1p1</oasis:entry>
         <oasis:entry colname="col6">FGOALS-f3-L</oasis:entry>
         <oasis:entry colname="col7">1.0<inline-formula><mml:math id="M256" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M257" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M258" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GFDL-CM3</oasis:entry>
         <oasis:entry colname="col2">2.0<inline-formula><mml:math id="M259" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M260" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M261" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">FIO-ESM-2-0</oasis:entry>
         <oasis:entry colname="col7">0.942408<inline-formula><mml:math id="M262" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M263" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M264" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-3)i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-3)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r(1-3)i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GFDL-ESM2G</oasis:entry>
         <oasis:entry colname="col2">2.0<inline-formula><mml:math id="M265" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M266" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M267" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">GFDL-ESM4</oasis:entry>
         <oasis:entry colname="col7">1.0<inline-formula><mml:math id="M268" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M269" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M270" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GFDL-ESM2M</oasis:entry>
         <oasis:entry colname="col2">2.0<inline-formula><mml:math id="M271" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M272" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M273" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">GISS-E2-1-G</oasis:entry>
         <oasis:entry colname="col7">2.0<inline-formula><mml:math id="M274" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M275" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M276" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p3f1</oasis:entry>
         <oasis:entry colname="col9">–</oasis:entry>
         <oasis:entry colname="col10">r1i1p3f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-H</oasis:entry>
         <oasis:entry colname="col2">2.0<inline-formula><mml:math id="M277" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M278" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M279" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r(1-3,5)i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1-2)i1p1</oasis:entry>
         <oasis:entry colname="col6">HadGEM3-GC31-LL</oasis:entry>
         <oasis:entry colname="col7">1.25<inline-formula><mml:math id="M280" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M281" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M282" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f3</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f3</oasis:entry>
         <oasis:entry colname="col10">r(1-3)i1p1f3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-H-CC</oasis:entry>
         <oasis:entry colname="col2">2.0<inline-formula><mml:math id="M283" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M284" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M285" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">INM-CM4-8</oasis:entry>
         <oasis:entry colname="col7">1.5<inline-formula><mml:math id="M286" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M287" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.0<inline-formula><mml:math id="M288" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">2.0<inline-formula><mml:math id="M289" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M290" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M291" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r(2,6)1i1p3</oasis:entry>
         <oasis:entry colname="col5">r(1-2)i1p1</oasis:entry>
         <oasis:entry colname="col6">INM-CM5-0</oasis:entry>
         <oasis:entry colname="col7">1.5<inline-formula><mml:math id="M292" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M293" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.0<inline-formula><mml:math id="M294" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R-CC</oasis:entry>
         <oasis:entry colname="col2">2.0<inline-formula><mml:math id="M295" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M296" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M297" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">IPSL-CM6A-LR</oasis:entry>
         <oasis:entry colname="col7">1.25<inline-formula><mml:math id="M298" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M299" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M300" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-4,6)i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-6,10,11,14,22,25)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadGEM2-AO</oasis:entry>
         <oasis:entry colname="col2">1.25<inline-formula><mml:math id="M301" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M302" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M303" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">KACE-1-0-G</oasis:entry>
         <oasis:entry colname="col7">1.25<inline-formula><mml:math id="M304" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M305" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M306" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-2)i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1,3)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadGEM2-ES</oasis:entry>
         <oasis:entry colname="col2">1.25<inline-formula><mml:math id="M307" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M308" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M309" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r(1-4)i1p1</oasis:entry>
         <oasis:entry colname="col4">r(1-4)i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1-4)i1p1</oasis:entry>
         <oasis:entry colname="col6">KIOST-ESM</oasis:entry>
         <oasis:entry colname="col7">1.875<inline-formula><mml:math id="M310" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M311" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M312" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">–</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">INMCM4</oasis:entry>
         <oasis:entry colname="col2">1.5<inline-formula><mml:math id="M313" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M314" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.0<inline-formula><mml:math id="M315" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">MCM-UA-1-0</oasis:entry>
         <oasis:entry colname="col7">2.25<inline-formula><mml:math id="M316" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M317" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.75<inline-formula><mml:math id="M318" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IPSL-CM5A-LR</oasis:entry>
         <oasis:entry colname="col2">1.875<inline-formula><mml:math id="M319" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M320" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.75<inline-formula><mml:math id="M321" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r(1-4)i1p1</oasis:entry>
         <oasis:entry colname="col4">r3i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1-4)i1p1</oasis:entry>
         <oasis:entry colname="col6">MIROC6</oasis:entry>
         <oasis:entry colname="col7">1.40625<inline-formula><mml:math id="M322" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M323" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.40625<inline-formula><mml:math id="M324" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-3)i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-3)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r(1-3)i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IPSL-CM5A-MR</oasis:entry>
         <oasis:entry colname="col2">1.26761<inline-formula><mml:math id="M325" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M326" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M327" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">MIROC-ES2L</oasis:entry>
         <oasis:entry colname="col7">2.8125<inline-formula><mml:math id="M328" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M329" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.8125<inline-formula><mml:math id="M330" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f2</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f2</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IPSL-CM5B-LR</oasis:entry>
         <oasis:entry colname="col2">1.875<inline-formula><mml:math id="M331" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M332" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.75<inline-formula><mml:math id="M333" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">MPI-ESM1-2-HR</oasis:entry>
         <oasis:entry colname="col7">0.9375<inline-formula><mml:math id="M334" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M335" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.9375<inline-formula><mml:math id="M336" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MIROC-ESM</oasis:entry>
         <oasis:entry colname="col2">2.8125<inline-formula><mml:math id="M337" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M338" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.8125<inline-formula><mml:math id="M339" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">MPI-ESM1-2-LR</oasis:entry>
         <oasis:entry colname="col7">1.875<inline-formula><mml:math id="M340" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M341" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M342" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-10)i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-10)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r(1-10)i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MIROC-ESM-CHEM</oasis:entry>
         <oasis:entry colname="col2">2.8125<inline-formula><mml:math id="M343" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M344" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.8125<inline-formula><mml:math id="M345" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">MRI-ESM2-0</oasis:entry>
         <oasis:entry colname="col7">1.125<inline-formula><mml:math id="M346" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M347" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.125<inline-formula><mml:math id="M348" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MIROC5</oasis:entry>
         <oasis:entry colname="col2">1.40625<inline-formula><mml:math id="M349" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M350" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.40625<inline-formula><mml:math id="M351" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r(2-3)1i1p1</oasis:entry>
         <oasis:entry colname="col4">r(2-3)i1p1</oasis:entry>
         <oasis:entry colname="col5">r(2-3)i1p1</oasis:entry>
         <oasis:entry colname="col6">NESM3</oasis:entry>
         <oasis:entry colname="col7">1.875<inline-formula><mml:math id="M352" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M353" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M354" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-2)i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-2)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r(1-2)i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-LR</oasis:entry>
         <oasis:entry colname="col2">1.875<inline-formula><mml:math id="M355" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M356" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M357" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r(1-3)i1p1</oasis:entry>
         <oasis:entry colname="col4">r(1-3)i1p1</oasis:entry>
         <oasis:entry colname="col5">r(1-3)i1p1</oasis:entry>
         <oasis:entry colname="col6">NorESM2-LM</oasis:entry>
         <oasis:entry colname="col7">1.25<inline-formula><mml:math id="M358" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M359" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.75<inline-formula><mml:math id="M360" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r(1-3)i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-MR</oasis:entry>
         <oasis:entry colname="col2">1.875<inline-formula><mml:math id="M361" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M362" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M363" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r(1-3)i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">NorESM2-MM</oasis:entry>
         <oasis:entry colname="col7">0.9375<inline-formula><mml:math id="M364" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M365" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M366" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col9">r1i1p1f1</oasis:entry>
         <oasis:entry colname="col10">r1i1p1f1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MRI-CGCM3</oasis:entry>
         <oasis:entry colname="col2">1.125<inline-formula><mml:math id="M367" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M368" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.125<inline-formula><mml:math id="M369" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6">UKESM1-0-LL</oasis:entry>
         <oasis:entry colname="col7">1.25<inline-formula><mml:math id="M370" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M371" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.875<inline-formula><mml:math id="M372" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">r(1-4,8)i1p1f2</oasis:entry>
         <oasis:entry colname="col9">r(1-4,8)i1p1f2</oasis:entry>
         <oasis:entry colname="col10">r(1-4,8)i1p1f2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MRI-ESM1</oasis:entry>
         <oasis:entry colname="col2">1.125<inline-formula><mml:math id="M373" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M374" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.125<inline-formula><mml:math id="M375" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8"/>
         <oasis:entry colname="col9"/>
         <oasis:entry colname="col10"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">NorESM1-M</oasis:entry>
         <oasis:entry colname="col2">1.875<inline-formula><mml:math id="M376" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M377" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M378" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1</oasis:entry>
         <oasis:entry colname="col4">r1i1p1</oasis:entry>
         <oasis:entry colname="col5">r1i1p1</oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8"/>
         <oasis:entry colname="col9"/>
         <oasis:entry colname="col10"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry rowsep="1" colname="col1">HighResMIP</oasis:entry>
         <oasis:entry rowsep="1" colname="col2">lat <inline-formula><mml:math id="M379" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> lon</oasis:entry>
         <oasis:entry rowsep="1" colname="col3">SSP5-8.5</oasis:entry>
         <oasis:entry namest="col4" nameend="col10" align="center">  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CMCC-CM2-HR4</oasis:entry>
         <oasis:entry colname="col2">0.942408<inline-formula><mml:math id="M380" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M381" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.25<inline-formula><mml:math id="M382" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1f1</oasis:entry>
         <oasis:entry namest="col4" nameend="col10" align="center">  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-CM6-1-HR</oasis:entry>
         <oasis:entry colname="col2">0.5<inline-formula><mml:math id="M383" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M384" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.5<inline-formula><mml:math id="M385" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1f1</oasis:entry>
         <oasis:entry namest="col4" nameend="col10" align="center">  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadGEMGE3-GC31-HM</oasis:entry>
         <oasis:entry colname="col2">0.234375<inline-formula><mml:math id="M386" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M387" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.351562<inline-formula><mml:math id="M388" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1f1</oasis:entry>
         <oasis:entry namest="col4" nameend="col10" align="center">  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CMCC-CM2-VHR4</oasis:entry>
         <oasis:entry colname="col2">0.234681<inline-formula><mml:math id="M389" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M390" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M391" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1f1</oasis:entry>
         <oasis:entry namest="col4" nameend="col10" align="center">  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">EC-Earth3P</oasis:entry>
         <oasis:entry colname="col2">0.703125<inline-formula><mml:math id="M392" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M393" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.703125<inline-formula><mml:math id="M394" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r3i1p2f1</oasis:entry>
         <oasis:entry namest="col4" nameend="col10" align="center">  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadGEMGE3-GC31-MM</oasis:entry>
         <oasis:entry colname="col2">0.555557<inline-formula><mml:math id="M395" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M396" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.833333<inline-formula><mml:math id="M397" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1f1</oasis:entry>
         <oasis:entry namest="col4" nameend="col10" align="center">  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-CM6-1</oasis:entry>
         <oasis:entry colname="col2">1.40625<inline-formula><mml:math id="M398" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M399" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.40625<inline-formula><mml:math id="M400" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r1i1p1f1</oasis:entry>
         <oasis:entry namest="col4" nameend="col10" align="center">  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">EC-Earth3P-HR</oasis:entry>
         <oasis:entry colname="col2">0.3515625<inline-formula><mml:math id="M401" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M402" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3515625<inline-formula><mml:math id="M403" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">r2i1p2f1</oasis:entry>
         <oasis:entry namest="col4" nameend="col10" align="center">  </oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

</app>

<app id="App1.Ch1.S2">
  <?xmltex \currentcnt{B}?><label>Appendix B</label><?xmltex \opttitle{Diagnostics, $\sigma _{{\mathrm{d}}}$ and $\sigma _{{\mathrm{s}}}$ of the weighting method}?><title>Diagnostics, <inline-formula><mml:math id="M404" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M405" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of the weighting method</title>
      <p id="d1e6458">This Appendix aims to describe the methodology behind the performance and independence weighting. First, we will explain the diagnostics chosen to
compute the distances and secondly how to obtain the two constant shape parameters from Eq. (1).</p>
      <p id="d1e6461">As the aim is to obtain weighted projections from a multi-model ensemble, the diagnostics to assess performance and independence must be relevant for
the used variable. The weighting is going to be optimized for temperature projections and therefore variables TAS and PSL from the historical period
(1980–2014) will be used, as these variables are relevant for the projected temperature <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx12" id="paren.84"/>. In order for CMIP5 to comply with the historical reference period, the diagnostics will include the first years of the scenario experiments (2006–2014). As there is a unique ensemble of members for each project, scenario and season, each ensemble will have its own set of weights.</p>
      <p id="d1e6467">The diagnostics used are differences, climatologies, trends and variability. According to <xref ref-type="bibr" rid="bib1.bibx66" id="text.85"/>, TAS historical trends have an evident
physical link and high correlation with future projected warming. The trend is defined by the linear ordinary least square regression fit for each
grid point with time as the independent variable during the reference period (TREND); the climatologies are computed as the time mean of each grid point
over the reference period (CLIM); the differences are computed by subtracting the area-averaged climatology to each grid point's reference period
climatology (DIFF) and the variability is obtained with the mean inter-annual standard deviation for each grid point (STD). As the trend is not
relevant for PSL, it is not computed <xref ref-type="bibr" rid="bib1.bibx51" id="paren.86"/>.</p>
      <p id="d1e6477">When assessing performance, the aim is to identify the models that more faithfully represent the historical climate. As all our results are computed
as differences from the historical period, model biases in the climatology should not be relevant. That is why the diagnostics used for performance
weighting are TAS-TREND, TAS-DIFF, TAS-STD, PSL-DIFF and PSL-DIFF. Differently, the aim of weighting for independence is to identify members that have
similar traits. Biases in models should be similar for dependent models <xref ref-type="bibr" rid="bib1.bibx51" id="paren.87"/>; therefore, we use CLIM for temperature and sea-level
pressure (TAS-CLIM and PSL-CLIM) to compute the distances <inline-formula><mml:math id="M406" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> from Eq. (1). Computing the climatology over relatively long periods is a good
approach as the internal variability becomes minimized and, ideally, it is the main attribute distinguishing two members of the same model
<xref ref-type="bibr" rid="bib1.bibx33" id="paren.88"/>.</p>
      <p id="d1e6500">Finally, to compute the actual values of <inline-formula><mml:math id="M407" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M408" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> the single diagnostic distances (e.g. TAS-TREND, TAS-DIFF, PSL-DIFF) must be combined. This is done by normalizing the single diagnostics with the median over all members and then averaging them.</p>
      <?pagebreak page336?><p id="d1e6528">The shape parameters are constant thresholds that inform how large or small distances should be to determine performance (<inline-formula><mml:math id="M409" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and independence
(<inline-formula><mml:math id="M410" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>). If <inline-formula><mml:math id="M411" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is overconstrained (small value), it will generate a very strict performance weighting as only members with very
low values of <inline-formula><mml:math id="M412" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> will receive any weight. Contrarily, if high values of <inline-formula><mml:math id="M413" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are used, models with large distances will receive
performance weight, leading to too-permissive constraints. The independence shape parameter does not work in such a straightforward way: small values
of <inline-formula><mml:math id="M414" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> could weight all models as being independent, as the distance to consider two members dependent would have to be too
small. This could result in models receiving similar weights. A similar thing could happen but for the opposite reason if a large
<inline-formula><mml:math id="M415" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> was used, i.e. most models would seem dependent as large distances between members would be considered small enough. We therefore
must find an optimal <inline-formula><mml:math id="M416" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> that is neither too small nor too large <xref ref-type="bibr" rid="bib1.bibx39" id="paren.89"/>.</p>
      <p id="d1e6626">The ensemble gives the necessary information to make a best guess of both shape parameters. Regarding the performance parameter, <xref ref-type="bibr" rid="bib1.bibx39" id="text.90"/>
suggests applying perfect model tests for a range of <inline-formula><mml:math id="M417" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> candidates to obtain the optimal magnitude. The candidates are values
between 10 % and 200 % of the median <inline-formula><mml:math id="M418" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> distance. Consecutively, all members in the ensemble are once taken as the reference while the
rest are weighted following equation (1), with <inline-formula><mml:math id="M419" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> being the distance between the perfect member and the member <inline-formula><mml:math id="M420" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>. The <inline-formula><mml:math id="M421" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
candidates are iteratively tested for all perfect model tests until the smallest <inline-formula><mml:math id="M422" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> that makes 80 % of the perfect models fall
in between the 10th and 90th percentiles of their respective weighted ensembles is found. The diagnostics used in the test are the same as those
used to weight performance but computed for the future periods (2041–2060 and 2081–2100) as we want <inline-formula><mml:math id="M423" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to be based on the
uncertainties of the future projection ensemble. The average <inline-formula><mml:math id="M424" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> between both periods is used for its corresponding season, scenario
and CMIP ensemble.</p>
      <p id="d1e6717">The parameter <inline-formula><mml:math id="M425" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is informed by models with more than one initial-condition run. Ideally, members from the same model should be
considered completely dependent as their modelling assumptions are the same, even though internal variability makes the runs differ. The independence
weighting should identify when initial-condition runs from the same model are added or subtracted from an ensemble. If the independence weights (Eq. 1
denominator) are calculated for an ensemble with one member per model (<inline-formula><mml:math id="M426" display="inline"><mml:mrow><mml:msubsup><mml:mi>w</mml:mi><mml:mi>j</mml:mi><mml:mtext>ind</mml:mtext></mml:msubsup></mml:mrow></mml:math></inline-formula>) and then all the available members of a model <inline-formula><mml:math id="M427" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> are added
to the ensemble (<inline-formula><mml:math id="M428" display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represents the amount of members added), the average independence weights of model <inline-formula><mml:math id="M429" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> (<inline-formula><mml:math id="M430" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mi>j</mml:mi><mml:mtext>ind</mml:mtext></mml:msubsup></mml:mrow></mml:math></inline-formula>) are
expected to decrease by a ratio <inline-formula><mml:math id="M431" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:msub><mml:mi>E</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Additionally, including members of a model <inline-formula><mml:math id="M432" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> to the ensemble should have a minimal effect on the
independence weights of the rest of the models <inline-formula><mml:math id="M433" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> represented by only one member in the ensemble.</p>
      <p id="d1e6815">The optimal <inline-formula><mml:math id="M434" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is found via an iterative process for a range of <inline-formula><mml:math id="M435" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> candidates, looking for the one that
minimizes the sum <inline-formula><mml:math id="M436" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M437" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M438" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are defined as <xref ref-type="bibr" rid="bib1.bibx11" id="paren.91"/>

              <disp-formula specific-use="align"><mml:math id="M439" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mtext>mean</mml:mtext><mml:mi>j</mml:mi></mml:msub><mml:msup><mml:mfenced close="]" open="["><mml:mrow><mml:msubsup><mml:mi>w</mml:mi><mml:mi>j</mml:mi><mml:mtext>ind</mml:mtext></mml:msubsup><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi>E</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mi>j</mml:mi><mml:mtext>ind</mml:mtext></mml:msubsup><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mtext>mean</mml:mtext><mml:mi>j</mml:mi></mml:msub><mml:mfenced close="}" open="{"><mml:mrow><mml:msub><mml:mtext>mean</mml:mtext><mml:mi>i</mml:mi></mml:msub><mml:msup><mml:mfenced close="]" open="["><mml:mrow><mml:msubsup><mml:mi>w</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>≠</mml:mo><mml:mi>j</mml:mi></mml:mrow><mml:mtext>ind</mml:mtext></mml:msubsup><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mrow><mml:mi>i</mml:mi><mml:mo>≠</mml:mo><mml:mi>j</mml:mi></mml:mrow><mml:mtext>ind</mml:mtext></mml:msubsup><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mo>∀</mml:mo><mml:mi>j</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p><?xmltex \hack{\newpage}?>
</app>
  </app-group><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e7045">The tool used for the diagnostics is ESMValTool (the version used is available at <ext-link xlink:href="https://doi.org/10.5281/zenodo.4562215" ext-link-type="DOI">10.5281/zenodo.4562215</ext-link>) <xref ref-type="bibr" rid="bib1.bibx7" id="paren.92"/> and its core modules are from ESMValCore (the version used is available at <ext-link xlink:href="https://doi.org/10.5281/zenodo.4947127" ext-link-type="DOI">10.5281/zenodo.4947127</ext-link>) <xref ref-type="bibr" rid="bib1.bibx8" id="paren.93"/>. The observational data used GPCC (<ext-link xlink:href="https://doi.org/10.5676/DWD_GPCC/FD_M_V2020_025" ext-link-type="DOI">10.5676/DWD_GPCC/FD_M_V2020_025</ext-link>; <xref ref-type="bibr" rid="bib1.bibx21" id="altparen.94"/>), CRU (<uri>https://crudata.uea.ac.uk/cru/data/hrg/cru_ts_4.04/cruts.2004151855.v4.04/</uri>, <ext-link xlink:href="https://doi.org/10.1038/s41597-020-0453-3" ext-link-type="DOI">10.1038/s41597-020-0453-3</ext-link>; <xref ref-type="bibr" rid="bib1.bibx70" id="altparen.95"/>), JRA55 (<uri>https://jra.kishou.go.jp/JRA-55/index_en.html#reanalysis</uri>; <xref ref-type="bibr" rid="bib1.bibx38" id="altparen.96"/>), ERA5 (<ext-link xlink:href="https://doi.org/10.1002/qj.3803" ext-link-type="DOI">10.1002/qj.3803</ext-link>; <xref ref-type="bibr" rid="bib1.bibx22" id="altparen.97"/>), BerkeleyEarth (<uri>http://berkeleyearth.lbl.gov/auto/Global/Gridded/Complete_TAVG_LatLong1.nc</uri>; <xref ref-type="bibr" rid="bib1.bibx4" id="altparen.98"/>) and HadSLP (<ext-link xlink:href="https://doi.org/10.1175/JCLI3937.1" ext-link-type="DOI">10.1175/JCLI3937.1</ext-link>; <xref ref-type="bibr" rid="bib1.bibx72" id="altparen.99"/>). CMIP data: all CMIP5 and 6 datasets were downloaded from the Earth System Grid Federation available at <uri>https://esg-dn1.nsc.liu.se/projects/esgf-liu/</uri> <xref ref-type="bibr" rid="bib1.bibx23" id="paren.100"/>. The models used are listed in Table A1.</p>

      <p id="d1e7108">The ESMValTool recipes and the code for the diagnostics can be found at <uri>https://doi.org/10.23728/b2share.01b483fa953241b2b2d8f5242cae6e8c</uri> <xref ref-type="bibr" rid="bib1.bibx14" id="paren.101"/>.</p>

      <p id="d1e7117">Additional figures not shown in the main text or the Supplement can be found in the figure repository built with a shiny app following the link <uri>https://earth.bsc.es/shiny/medprojections-shiny_app/</uri> <xref ref-type="bibr" rid="bib1.bibx15" id="paren.102"/>.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e7126">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/esd-13-321-2022-supplement" xlink:title="pdf">https://doi.org/10.5194/esd-13-321-2022-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e7135">JC, FD and MJ designed the study. JC developed and ran the diagnostics, and wrote the initial manuscript. MJ helped in figure production. MJ, FD, RM and JC contributed to the interpretation of the results and the improvement of the manuscript. PB and MS contributed to downloading and fixing the datasets used in this study.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e7141">The contact author has declared that neither they nor their co-authors have any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e7147">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e7153">We acknowledge the World Climate Research Programme, which, through its Working Group on Coupled Modelling, coordinated and promoted CMIP5 and CMIP6. We thank the climate modelling groups for producing and making available their model output, the Earth System Grid Federation (ESGF) for archiving the data and providing access and the multiple funding agencies who support CMIP5, CMIP6 and ESGF. We also thank the European Centre for Medium-Range Weather Forecasts (ECMWF), the Japan Meteorological Agency (JMA), the University of East Anglia (UEA), the Deutscher Wetterdienst (DWD), Berkeley Earth and<?pagebreak page337?> the Met Office (UKMO) for providing ERA5, JRA55, CRU, GPCC, BerkeleyEarth and  HadSLP2 reanalysis/observational data respectively. We acknowledge the Earth System Evaluation Tool (ESMValTool) community for the development and distribution of the tool, and we sincerely thank Saskia Loosveldt-Tomas and Javier Vegas-Regidor (BSC-CNS) for technical support with the tool.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e7158">The work in this paper was partly supported by the European Commission H2020 project EUCP (grant no. 776613).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e7164">This paper was edited by Gabriele Messori and reviewed by three anonymous referees.</p>
  </notes><ref-list>
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