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  <front>
    <journal-meta><journal-id journal-id-type="publisher">GMD</journal-id><journal-title-group>
    <journal-title>Geoscientific Model Development</journal-title>
    <abbrev-journal-title abbrev-type="publisher">GMD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Geosci. Model Dev.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1991-9603</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/gmd-14-3159-2021</article-id><title-group><article-title>Earth System Model Evaluation Tool (ESMValTool) v2.0 – diagnostics for
extreme events, regional and impact evaluation, and analysis of Earth system
models in CMIP</article-title><alt-title>ESMValTool v2.0</alt-title>
      </title-group><?xmltex \runningtitle{ESMValTool v2.0}?><?xmltex \runningauthor{K.~Weigel et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Weigel</surname><given-names>Katja</given-names></name>
          <email>weigel@iup.physik.uni-bremen.de</email>
        <ext-link>https://orcid.org/0000-0001-6133-7801</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Bock</surname><given-names>Lisa</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7058-5938</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Gier</surname><given-names>Bettina K.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2928-8664</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Lauer</surname><given-names>Axel</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9270-1044</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Righi</surname><given-names>Mattia</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3827-5950</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Schlund</surname><given-names>Manuel</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5251-0158</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Adeniyi</surname><given-names>Kemisola</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Andela</surname><given-names>Bouwe</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9005-8940</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4 aff5">
          <name><surname>Arnone</surname><given-names>Enrico</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6740-5051</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Berg</surname><given-names>Peter</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1469-2568</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Caron</surname><given-names>Louis-Philippe</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5221-0147</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Cionni</surname><given-names>Irene</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Corti</surname><given-names>Susanna</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4456-6682</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Drost</surname><given-names>Niels</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9795-7981</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Hunter</surname><given-names>Alasdair</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Lledó</surname><given-names>Llorenç</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8628-6876</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9 aff13">
          <name><surname>Mohr</surname><given-names>Christian Wilhelm</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2656-1802</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Paçal</surname><given-names>Aytaç</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1324-2389</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Pérez-Zanón</surname><given-names>Núria</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8568-3071</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff10">
          <name><surname>Predoi</surname><given-names>Valeriu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9">
          <name><surname>Sandstad</surname><given-names>Marit</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9">
          <name><surname>Sillmann</surname><given-names>Jana</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0219-5345</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff11">
          <name><surname>Sterl</surname><given-names>Andreas</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3457-0434</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Vegas-Regidor</surname><given-names>Javier</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0096-4291</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff12 aff4">
          <name><surname>von Hardenberg</surname><given-names>Jost</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5312-8070</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff1">
          <name><surname>Eyring</surname><given-names>Veronika</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6887-4885</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Institute of Environmental Physics (IUP), University of Bremen,
Bremen, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Deutsches Zentrum für Luft- und Raumfahrt (DLR), Institut für
Physik der Atmosphäre, Oberpfaffenhofen, Germany</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Netherlands eScience Center (NLeSC), Amsterdam, the Netherlands</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Institute of Atmospheric Sciences and Climate, Consiglio Nazionale
delle Ricerche (ISAC-CNR), Italy</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Physics, University of Torino, Italy</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Hydrology research unit, Swedish Meteorological and Hydrological
Institute (SMHI), Sweden</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Barcelona Supercomputing Center (BSC), Barcelona, Spain</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>Agenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo
economico sostenibile (ENEA), Rome, Italy</institution>
        </aff>
        <aff id="aff9"><label>9</label><institution>CICERO – Center for International Climate Research, Oslo, Norway</institution>
        </aff>
        <aff id="aff10"><label>10</label><institution>NCAS Computational Modelling Services (CMS), University of Reading,
Reading, UK</institution>
        </aff>
        <aff id="aff11"><label>11</label><institution>Royal Netherlands Meteorological Institute (KNMI), de Bilt, the
Netherlands</institution>
        </aff>
        <aff id="aff12"><label>12</label><institution>Department of Environment, Land and Infrastructure Engineering,
Politecnico di Torino, Turin, Italy</institution>
        </aff>
        <aff id="aff13"><label>a</label><institution>now at: Division for Forestry and Forest Resources, The Norwegian
Institute of Bioeconomy Research (NIBIO), Ås, Norway</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Katja Weigel (weigel@iup.physik.uni-bremen.de)</corresp></author-notes><pub-date><day>3</day><month>June</month><year>2021</year></pub-date>
      
      <volume>14</volume>
      <issue>6</issue>
      <fpage>3159</fpage><lpage>3184</lpage>
      <history>
        <date date-type="received"><day>24</day><month>July</month><year>2020</year></date>
           <date date-type="rev-request"><day>9</day><month>October</month><year>2020</year></date>
           <date date-type="rev-recd"><day>5</day><month>April</month><year>2021</year></date>
           <date date-type="accepted"><day>12</day><month>April</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 </copyright-statement>
        <copyright-year>2021</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://gmd.copernicus.org/articles/.html">This article is available from https://gmd.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://gmd.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://gmd.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e394">This paper complements a series of now four publications that
document the release of the Earth System Model Evaluation Tool (ESMValTool)
v2.0. It describes new diagnostics on the hydrological cycle, extreme
events, impact assessment, regional evaluations, and ensemble member
selection. The diagnostics are developed by a large community of scientists
aiming to facilitate the evaluation and comparison of Earth system models
(ESMs) which are participating in the Coupled Model Intercomparison Project
(CMIP). The second release of this tool aims to support the evaluation of
ESMs participating in CMIP Phase 6 (CMIP6). Furthermore, datasets from
other models and observations can be analysed. The diagnostics for the
hydrological cycle include several precipitation and drought indices, as
well as hydroclimatic intensity and indices from the Expert Team on Climate
Change Detection and Indices (ETCCDI). The latter are also used for
identification of extreme events, for impact assessment, and to project
and characterize the risks and impacts of climate change for natural and
socio-economic systems. Further impact assessment diagnostics are included
to compute daily temperature ranges and capacity factors for wind and solar
energy generation. Regional scales can be analysed with new diagnostics
implemented for selected regions and stochastic downscaling. ESMValTool v2.0
also includes diagnostics to analyse large multi-model ensembles including
grouping and selecting ensemble members by user-specified criteria. Here, we
present examples for their capabilities based on the well-established CMIP
Phase 5 (CMIP5) dataset.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<?pagebreak page3160?><sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e406">Climate change is affecting the Earth system in many different ways. To be
able to assess the impacts of climate change on society and to develop
strategies for mitigation and adaptation, detailed knowledge of the
climate system and the key processes driving climate change is necessary.
This is particularly the case for changes in the hydrological cycle and
climate extreme events, both having direct consequences on ecosystems and
society (Eyring et al., 2020). With rising greenhouse gas concentrations
the hydroclimatic regime is expected to change (Giorgi et al.,
2019). As the intensity and distribution of precipitation determine the
availability of fresh water in a certain region, they are also related to the
severity of hazardous events such as flooding or droughts. The impact of
extreme events on many socio-economic factors increases with their severity,
but the rare occurrence of these events makes an assessment of the effect of
climate change on such events challenging (Zhang et al., 2011).
Compound events, caused by a combination of processes on multiple
spatial and temporal scales, particularly lead to severe impacts (Zscheischler et al.,
2018).</p>
      <p id="d1e409">Changes in climate can alter both the strength and the probability of
extreme events (Seneviratne et al., 2012; IPCC, 2012). For various
extreme events an increase in severity and frequency was observed in the
past decades and is expected with rising temperatures, such as
warm temperature extremes (Alexander, 2016). With rising temperatures an
increase is also expected in the amount of precipitation. For wet
precipitation extremes this increase is expected to happen faster than for
the total wet-day (days with precipitation <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> mm) precipitation
(Sillmann et al., 2013b). Several studies project that
dry regions are becoming drier and wet regions wetter (Martin, 2018; Greve et
al., 2014), which is expected to result in an increase in both wet and dry
extreme events, depending on the region. This tendency was highlighted by a
general increase in the hydroclimatic intensity, which gives a joint measure
of dry and wet conditions in a warming climate (Giorgi et al., 2011).
Studies by Donat et al. (2019) and Pfahl et al. (2017) show an
increase in observed precipitation extremes in humid regions, whereas there
is no clear indication of the change in precipitation extreme events in arid
regions. The impact of different climate forcers such as greenhouse gases
and aerosols on droughts remains to be understood in more detail
(Marvel et al., 2019).</p>
      <p id="d1e422">Although the climate system is of global extent, its manifestations have
regional and local impacts (IPCC, 2014a).
Particularly for regional climate changes, robust projections require not only
an understanding of the underlying physics and internal variability but also
a reduction of model biases (Xie et al., 2015). If model
biases are corrected without considering the underlying physical processes,
however, downscaling of ESM results to regional scales can result in
unwanted artefacts (Maraun et al., 2017). Observed changes on the
regional scale depend to a large extent on atmospheric dynamics; therefore,
the signal of climate change is often smaller than the internal variability
(Deser et al., 2012), while large differences are found in the
modelled future scenarios (Shepherd, 2014). Stochastic downscaling of
precipitation can aid in this direction as the fields at regional scale are
derived from the spectral properties of the fields at large scale, with an
ability to reproduce extremes even over complex orography (Rebora
et al., 2006; D'Onofrio et al., 2014; Terzago et al., 2018). Model ensembles
can be used to quantify uncertainties in climate change projections due to
internal variability (Xie et al., 2015), and
clustering analysis can be used to intercompare and group ensemble members based on
similar characteristics and select the most representative ones, going
beyond the biases of individual models (Straus et al., 2007).</p>
      <p id="d1e425">The Earth System Model Evaluation Tool (ESMValTool) version 2.0 (v2.0)
includes diagnostics and performance metrics for the analysis and evaluation
of ESMs with observations. It is developed by a large community, which
involves more than 150 scientists from over 60 institutions. Figures and
other output produced by the tool include full provenance information to
allow for traceability and reproducibility of the results. The main focus is
on the analysis of ESM simulations from the Coupled Model Intercomparison
Project (CMIP) of the World Climate Research Programme (WCRP). CMIP started
in 1995 (Meehl et al., 2000) with the aim of providing scientists with
comparable coupled model runs based on standardized boundary conditions
(Covey et al., 2003). CMIP results from phase 5 (CMIP5)
(Taylor et al., 2012) are the basis for many assessments in the
IPCC's Fifth Assessment Report (AR5) (IPCC, 2013). Now, data from phase 6
(CMIP6) (Eyring et al., 2016) are available. With every phase of CMIP the
volume of data increases: for CMIP6 a total data volume of about 20 to 40 PB
is expected. This emphasizes the need for a fast and comprehensive tool like
the ESMValTool (v2.0) to evaluate these model results. In this work, the
diagnostics which focus on climate impacts are described, and their output
using the well-established CMIP5 data is shown.</p>
      <p id="d1e429">In this study we present diagnostics included in the ESMValTool specifically
for the analysis of the hydrological cycle, extreme events, climate impacts,
multi-model ensemble member sub-selection, and regional model evaluation.
This article completes a series of publications documenting ESMValTool v2.0:
Righi et al. (2020) describe the
technical aspects, Eyring et al. (2020) the new large-scale diagnostics,
and Lauer et al. (2020) emergent
constraints and diagnostics for future projections from ESMs in CMIP.</p>

<?xmltex \floatpos{p}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e435">Overview of recipes implemented in ESMValTool v2.0 along with the
section in which they are described, a brief description, the variables used, and the
diagnostic scripts included. For further details, we refer to the GitHub
repository and documentation at <uri>https://docs.esmvaltool.org/</uri> (last access: 1 June 2021).</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.85}[.85]?><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="2cm"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="4cm"/>
     <oasis:colspec colnum="4" colname="col4" align="justify" colwidth="2cm"/>
     <oasis:colspec colnum="5" colname="col5" align="justify" colwidth="5.5cm"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Recipe name</oasis:entry>
         <oasis:entry colname="col2">Section <?xmltex \hack{\hfill\break}?>(figures)</oasis:entry>
         <oasis:entry colname="col3">Description, references</oasis:entry>
         <oasis:entry colname="col4">Variables (observational datasets)</oasis:entry>
         <oasis:entry colname="col5">Diagnostic scripts</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col5">Section 3.1: Hydrological cycle </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_hyint.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.1.1 (Fig. 1)</oasis:entry>
         <oasis:entry colname="col3">Recipe for evaluating the intensity of the hydroclimatic cycle, calculating a set of six indices following Giorgi et al. (2011, 2014): simple precipitation intensity index (SDII), maximum dry spell length (DSL) and wet spell length (WSL), hydroclimatic intensity index (HY-INT), which is a measure of the overall behaviour of the hydroclimatic cycle, and precipitation area (PA), i.e. the area over which precipitation occurs on any given day</oasis:entry>
         <oasis:entry colname="col4">pr</oasis:entry>
         <oasis:entry colname="col5">hyint/hyint.R</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_hyint_extreme_events.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.1.1 (Fig. 2)</oasis:entry>
         <oasis:entry colname="col3">Multi-diagnostic version of hyint, which allows inclusion of ETCCDI results from the extreme_events diagnostics and performs joint analysis of indices for hydroclimatic intensity and extreme events; Giorgi et al. (2014, 2011), Sillmann et al. (2013a)</oasis:entry>
         <oasis:entry colname="col4">pr <?xmltex \hack{\hfill\break}?>tasmin <?xmltex \hack{\hfill\break}?>tasmax <?xmltex \hack{\hfill\break}?></oasis:entry>
         <oasis:entry colname="col5">hyint/hyint.R <?xmltex \hack{\hfill\break}?>extreme_events/extreme_events.R</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_consecdrydays.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.1.2</oasis:entry>
         <oasis:entry colname="col3">Dry-day definition (precip limit, mm per day) and drought duration (days) can be set by the user <?xmltex \hack{\hfill\break}?>Output as NetCDF files for each model possible; computed consistently with the CDO method “eca_cdd” in Schulzweida (2018)</oasis:entry>
         <oasis:entry colname="col4">pr</oasis:entry>
         <oasis:entry colname="col5">droughtindex/diag_cdd.py</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><italic>recipe_spei.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.1.2 <?xmltex \hack{\hfill\break}?>(Figs. 3, 4)</oasis:entry>
         <oasis:entry colname="col3">Global average histogram of SPI and SPEI as absolute values and as bias; calculations based on pr for both indices, but for SPEI with the additional use of ta to derive evapotranspiration using the Thornthwaite method; <?xmltex \hack{\hfill\break}?>requires a reference dataset and calculates a global cosine of latitude-weighted histogram for all valid grid points of the reference dataset; calculation of SPI and SPEI based on <?xmltex \hack{\hfill\break}?>Vicente-Serrano et al. (2010)</oasis:entry>
         <oasis:entry colname="col4">pr <?xmltex \hack{\hfill\break}?>(ERA-Interim) <?xmltex \hack{\hfill\break}?>ta <?xmltex \hack{\hfill\break}?>(CRUts4.01)</oasis:entry>
         <oasis:entry colname="col5">droughtindex/diag_spi.r <?xmltex \hack{\hfill\break}?>droughtindex/diag_spei.r</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

<?xmltex \floatpos{p}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e591">Continued.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.85}[.85]?><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="2cm"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="4cm"/>
     <oasis:colspec colnum="4" colname="col4" align="justify" colwidth="2cm"/>
     <oasis:colspec colnum="5" colname="col5" align="justify" colwidth="5.5cm"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Recipe name</oasis:entry>
         <oasis:entry colname="col2">Section <?xmltex \hack{\hfill\break}?>(figures)</oasis:entry>
         <oasis:entry colname="col3">Description, references</oasis:entry>
         <oasis:entry colname="col4">Variables (observational datasets)</oasis:entry>
         <oasis:entry colname="col5">Diagnostic scripts</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_martin18grl.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.1.2 (Fig. 5)</oasis:entry>
         <oasis:entry colname="col3">Computes a monthly time series of SPI based on diag_spi.r (distribution and representing timescale can be set by the user) and calculates drought events as consecutive number of months with SPI <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>; for each grid point the drought characteristics (frequency, average duration, and SPI as well as the severity index) based on <?xmltex \hack{\hfill\break}?>Martin (2018) are calculated; differences between individual models or a multi-model mean and observations or future scenarios and historical model runs are calculated</oasis:entry>
         <oasis:entry colname="col4">pr (CRU)</oasis:entry>
         <oasis:entry colname="col5">droughtindex/diag_save_spi.R <?xmltex \hack{\hfill\break}?>droughtindex/collect_drought_func.py <?xmltex \hack{\hfill\break}?>droughtindex/collect_drought_obs_multi.py <?xmltex \hack{\hfill\break}?>droughtindex/collect_drought_model.py</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col5">Section 3.2: Extreme events </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_extreme_events.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.2 <?xmltex \hack{\hfill\break}?>(Figs. 6, 7)</oasis:entry>
         <oasis:entry colname="col3">Calculates indices for monitoring changes in extremes (Sillmann et al., 2013a) based on daily temperature and precipitation data; produces Glecker and time series plots as shown in the IPCC AR5 report (Flato et al., 2013)</oasis:entry>
         <oasis:entry colname="col4">pr <?xmltex \hack{\hfill\break}?>tas <?xmltex \hack{\hfill\break}?>tasmin <?xmltex \hack{\hfill\break}?>tasmax <?xmltex \hack{\hfill\break}?>(ERA-Interim)</oasis:entry>
         <oasis:entry colname="col5">extreme_events/extreme_events.R</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col5">Section 3.3: Evaluation for impact assessments </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_heatwaves_coldwaves.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.3.1 <?xmltex \hack{\hfill\break}?>(Fig. 8)</oasis:entry>
         <oasis:entry colname="col3">MAGIC, time averages, differences between historical simulations and a future scenario; calculates the number of days exceeding a given quantile for a minimum number of consecutive days; <?xmltex \hack{\hfill\break}?>Watts et al. (2015)</oasis:entry>
         <oasis:entry colname="col4">Tasmin <?xmltex \hack{\hfill\break}?>Tasmax</oasis:entry>
         <oasis:entry colname="col5">magic_bsc/extreme_spells.r</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_extreme_index.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.3.2 <?xmltex \hack{\hfill\break}?>(Fig. 9)</oasis:entry>
         <oasis:entry colname="col3">MAGIC, computes time series of the number of several extreme events: heat wave, <?xmltex \hack{\hfill\break}?>cold wave, heavy precipitation, drought, and high wind; <?xmltex \hack{\hfill\break}?>Karl et al. (1996), Gleason et al. (2008), American Academy of Actuaries (2018)</oasis:entry>
         <oasis:entry colname="col4">Tasmin <?xmltex \hack{\hfill\break}?>tasmax <?xmltex \hack{\hfill\break}?>pr <?xmltex \hack{\hfill\break}?>scfWind</oasis:entry>
         <oasis:entry colname="col5">magic_bsc/extreme_index.r</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_diurnal_temperature_index.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.3.3 <?xmltex \hack{\hfill\break}?>(Fig. 10)</oasis:entry>
         <oasis:entry colname="col3">MAGIC, time averages, difference between historical and future scenario; computes the dates on which the DTR exceeds a threshold; <?xmltex \hack{\hfill\break}?>Déandreis et al. (2014)</oasis:entry>
         <oasis:entry colname="col4">tasmin <?xmltex \hack{\hfill\break}?>tasmax</oasis:entry>
         <oasis:entry colname="col5">magic_bsc/diurnal_temp_index.r</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_capacity_factor.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.3.4 <?xmltex \hack{\hfill\break}?>(Fig. 11)</oasis:entry>
         <oasis:entry colname="col3">MAGIC, calculates the wind power capacity factor; <?xmltex \hack{\hfill\break}?>Lledo et al. (2019)</oasis:entry>
         <oasis:entry colname="col4">scfWind</oasis:entry>
         <oasis:entry colname="col5">magic_bsc/capacity_factor.r</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><italic>recipe_pv_capacity_factor.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.3.4 <?xmltex \hack{\hfill\break}?>(Fig. 12)</oasis:entry>
         <oasis:entry colname="col3">Photovoltaic capacity factor</oasis:entry>
         <oasis:entry colname="col4">tasmax <?xmltex \hack{\hfill\break}?>rsds <?xmltex \hack{\hfill\break}?>(ERA-Interim)</oasis:entry>
         <oasis:entry colname="col5">pv_capacityfactor/pv_capacity_factor.R</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e849">Continued.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.85}[.85]?><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="2cm"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="4cm"/>
     <oasis:colspec colnum="4" colname="col4" align="justify" colwidth="2cm"/>
     <oasis:colspec colnum="5" colname="col5" align="justify" colwidth="5.5cm"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Recipe name</oasis:entry>
         <oasis:entry colname="col2">Section <?xmltex \hack{\hfill\break}?>(figures)</oasis:entry>
         <oasis:entry colname="col3">Description, references</oasis:entry>
         <oasis:entry colname="col4">Variables (observational datasets)</oasis:entry>
         <oasis:entry colname="col5">Diagnostic scripts</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col5">Section 3.4: Regional model evaluation </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_flato13ipcc.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.4.1 (Figs. 13, 14, 14, 16)</oasis:entry>
         <oasis:entry colname="col3">Figures similar to figures of the IPCC AR5 (Flato et al., 2013) <?xmltex \hack{\hfill\break}?>Fig. 13: Seasonal cycle over land within defined regions (like Fig. 9.38) <?xmltex \hack{\hfill\break}?>Fig. 14: Downscaling: Seasonal bias box plot within defined regions (like Fig. 9.39) <?xmltex \hack{\hfill\break}?>Fig. 15: Downscaling: Seasonal bias box plot within defined polar and ocean regions (like Fig. 9.40) <?xmltex \hack{\hfill\break}?>Fig. 16: Downscaling: Observations versus models within defined regions (like Fig. 9.41)</oasis:entry>
         <oasis:entry colname="col4">tas (ERA-Interim, CRU) <?xmltex \hack{\hfill\break}?>pr (CRU)</oasis:entry>
         <oasis:entry colname="col5">regional_downscaling/Figure9.38.ncl <?xmltex \hack{\hfill\break}?>regional_downscaling/Figure9.38.ncl <?xmltex \hack{\hfill\break}?>regional_downscaling/Figure9.38.ncl <?xmltex \hack{\hfill\break}?>regional_downscaling/Figure9.38.ncl <?xmltex \hack{\hfill\break}?></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><italic>recipe_rainfarm.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.4.2 (Fig. 17)</oasis:entry>
         <oasis:entry colname="col3">MAGIC, stochastic spatial downscaling of daily precipitation using the RainFARM method (Rebora et al., 2006; D'Onofrio et al., 2014); allows calculation of climatological weights to take into account the effect of orography following Terzago et al. (2018); produces ensembles of downscaled precipitation fields in NetCDF format – no plots are produced</oasis:entry>
         <oasis:entry colname="col4">pr</oasis:entry>
         <oasis:entry colname="col5">rainfarm/rainfarm.R</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col5">Section 3.5: Multi-model ensemble member sub-selection </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><italic>recipe_ensclus.yml</italic></oasis:entry>
         <oasis:entry colname="col2">3.5 (Fig. 18)</oasis:entry>
         <oasis:entry colname="col3">Cluster analysis tool for ensembles of climate model simulations: EnsClus groups ensemble members according to similar characteristics (based on the <inline-formula><mml:math id="M3" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-means algorithm) and selects the most representative member for each cluster (Straus et al., 2007)</oasis:entry>
         <oasis:entry colname="col4">Pr <?xmltex \hack{\hfill\break}?>tas</oasis:entry>
         <oasis:entry colname="col5">ensclus/ensclus.py</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <?pagebreak page3163?><p id="d1e990">This paper is organized as follows: Sect. 2 describes the model and
observation data used. Section 3 presents the ESMValTool recipes for the
analyses of hydroclimatic intensity, droughts, extreme events, model impact
evaluation, multi-model ensemble member sub-selection, and regional model
evaluation. It also describes use of the ESMValTool as a post-processing
tool for further downscaling applications. Section 4 closes with a summary.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Models and observations</title>
      <p id="d1e1001">ESMValTool v2.0 was developed particularly for the analysis of CMIP data
(Righi et al., 2020). This work mainly
presents results based on the well-established CMIP5 model ensemble, but
other model output and observational data, e.g. provided by observations for
the Model Intercomparison Project (obs4MIPs; Teixeira et al., 2014; Waliser
et al., 2020), can also be analysed. As in version v1.0 (Eyring et al.,
2016), ESMValTool v2.0 expects input data to be in a climate and forecast
(CF) metadata-compliant Network Common Data Format (NetCDF) following the
Climate Model Output Rewrite (CMOR) standard. The detailed requirements for
CMOR can be found in these tables (<uri>http://pcmdi.github.io/cmor-site/tables.html</uri>, last access: 1 June 2021). For the recipes described
here, European Centre for Medium-Range Weather Forecasts (ECMWF) ERA-Interim
and Climatic Research Unit (CRU) reanalysis data are used for the evaluation
of the model results. Table 1 lists these data in case they are used for a
recipe. These datasets should be seen as examples as they can easily be
replaced by other reanalysis or observational datasets. Reformatting scripts
with downloading instructions are provided with the ESMValTool v2.0 to
convert many observational datasets to the CMOR standard. A list of
observational datasets available can be found in
Righi et al. (2020) and in the user's
guide at
<uri>https://docs.esmvaltool.org/en/latest/input.html#supported-datasets</uri> (last access: 1 June 2021),
where it is updated for newly included datasets. For ECMWF ERA5
“cmorization on the fly” is<?pagebreak page3164?> implemented, which works on the ERA5 NetCDF
data directly and does not require prior reformatting.</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Overview of recipes included in ESMValTool v2.0</title>
      <p id="d1e1018">This section describes the new and extended ESMValTool v2.0 recipes for
analysis of extreme events and regional model output, as well as for applying ESM
output in assessments of the impact of climate change and
carrying out model ensemble sub-selection. In ESMValTool v2.0, a recipe is a
*.yml file used to define the diagnostics and performance metrics to apply
to the simulation output, as well as the datasets and variables used. The
ESMValTool is started from the command line using the following, for example.</p>
      <p id="d1e1021"><monospace>esmvaltool run esmvaltool/recipes/</monospace> <monospace>examples/recipe_python.yml</monospace></p>
      <p id="d1e1028">Here, <italic>esmvaltool/recipes/examples/recipe_python.yml</italic> is
one possible recipe. Instead of this example, any other recipe provided with
the ESMValTool or created by the user can be used. For more detailed
instructions on how to run the tool and modify or create recipes, see the
documentation at <uri>https://docs.esmvaltool.org/</uri> (last access: 1 June 2021).</p>
      <p id="d1e1037">In the following, the recipes are briefly described and illustrated with
example figures using CMIP5 data. All recipes presented in this work are
summarized in Table 1, which includes a short description, together with the
analysed variables used, the applied diagnostics and their purpose, and the references the diagnostics are based on. Because the online
documentation for the ESMValTool v2.0 at <uri>https://docs.esmvaltool.org/</uri> (last access: 1 June 2021) was written simultaneously with this paper by
the same authors, there is considerable overlap in this non-peer-reviewed
document.</p>
      <p id="d1e1044">Section 3.1 describes recipes for the hydrological cycle, including indices
for hydroclimatic intensity and drought detection. In Sect. 3.2 recipes
for other extreme events are presented. Recipes for model impact assessment
are described in Sect. 3.3 and recipes for regional model evaluation in
Sect. 3.4. Section 3.5 presents a recipe for the sub-selection of
multi-model ensemble members.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Hydrological cycle</title>
<sec id="Ch1.S3.SS1.SSS1">
  <label>3.1.1</label><title>Hydroclimatic intensity and related indices</title>
      <p id="d1e1061">The Earth's hydrological cycle is a key element of the climate system with
important impacts on society. For example, the intensity and
distribution of precipitation determine the abundance or scarcity of fresh
water in a certain region. They are also related to the severity of hazardous
events such as flooding or droughts. Several studies have shown an
acceleration of the hydrological cycle and an intensification of both dry
and wet extremes in a warming climate (IPCC, 2013). A simple investigation
of total precipitation-related quantities can hide some of the most relevant
aspects of the hydrological cycle and its extremes, which can be highlighted
through the joint use of the concept of hydroclimatic intensity and related
indices (e.g. Giorgi et al., 2014). The hydroclimatic
intensity (Giorgi et al., 2011), derived as the product of mean daily
precipitation and dry spell length normalized over a reference period,
offers a joint view of both dry and wet conditions, allowing for the unique
quantification of the response in the intensity of the hydrological cycle in a
changing climate. The <italic>hyint</italic> (hydroclimatic intensity) diagnostic was developed to calculate several indices
for hydroclimatic and climate extremes and allow a multi-index evaluation of
climate models.</p>
      <p id="d1e1067">The <italic>recipe_hyint.yml</italic> calculates six indices for evaluating the  global warming response of
the hydrological cycle including both wet and dry extremes. The indices are
selected according to Giorgi et al. (2014), including the simple
precipitation intensity index (SDII), the maximum dry spell length (DSL) and
wet spell length (WSL), the hydroclimatic intensity index (HY-INT,
calculated as normalized DSL times normalized SDII), which is a measure of
the intensity of the hydroclimatic cycle compared to a reference period
(Giorgi et al., 2011), and the precipitation area (PA), i.e. the area
over which precipitation occurs on any given day (Giorgi et al.,
2014). The <italic>recipe_hyint_extreme_events.yml</italic> can also ingest the 27 temperature- and precipitation-based
Expert Team on Climate Change Detection and Indices (ETCCDI) (Zhang et
al., 2011) calculated by the <italic>recipe_extreme_events.yml</italic> to produce a multi-index analysis (see Sect. 3.2 for further details). The diagnostics perform a subsequent analysis
calculating time series and trends of the selected indices for predefined
continental areas, normalized to a reference period. The linear model (lm)
function of R is used to calculate trends. Statistical significance is
tested based on a Student's <inline-formula><mml:math id="M4" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test under a non-null coefficients hypothesis.
Trend coefficients and their statistics, including standard error, <inline-formula><mml:math id="M5" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> value,
and precipitation above the 95th percentile of the reference distribution,
are stored. The recipe created several plots, including global and
regional maps, time series with spread, trend lines, and summary plots of
trend coefficients. Results are stored in NetCDF files, including relevant
information such as normalization functions and thresholds, and as figures.
Figures 1 and 2 show examples of an analysis performed with the <italic>hyint</italic>
diagnostic. A map of the HY-INT index (Fig. 1) calculated from EC-EARTH
model data shows the projected average HY-INT compared to the reference
period (1976–2005): hydroclimatic intensity is projected to greatly increase
in some regions (e.g. eastern South America, northern Africa, and the
Arabian peninsula) and to decrease over other regions (e.g. Antarctica,
Greenland, central and north-eastern Asia, central Africa, and western and
northern South America), with large areas showing only moderate changes.
Trends shown in Fig. 2 exhibit a relatively low inter-model spread for
HY-INT. The projected increase in HY-INT seen for all models with values
ranging around 10 % per century  (also reflected as large
geographical patterns) can also be seen in the precipitation intensity (SDI)
and heavy precipitation indices (R95),<?pagebreak page3165?> the latter with an increased spread
between 10 % and 30 % per century. Precipitation area (PA) is projected to
increase by most models, whereas for projected changes in the dry spell
length (DSL) and especially in the wet spell length (WSL), models do not
agree on the sign of the projected changes, which is also reflected in high
geographical variability (not shown).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e1099">Mean hydroclimatic intensity index (i.e. a combination of
precipitation intensity and dry spell length normalized compared to a
reference period) over the years 2006–2099, for the EC-EARTH model RCP8.5
projection. The historical years 1976–2005 were used as the reference
period. The figure is an example of a large number of different plots which
can be produced with <italic>recipe_hyint.yml</italic>, similar to (Giorgi et al., 2014). For
details see Sect. 3.1.1.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-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="d1e1114">Trend in selected indices for an ensemble of CMIP5 models
(historical <inline-formula><mml:math id="M6" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> RCP8.5 projection) over the time period 1976–2099. The
trends are calculated over the latitude band 60<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–60<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. Data were normalized to the historical 1976–2005 period. Indices include
the precipitation area (PA), hydroclimatic intensity (HY-INT), precipitation
intensity (SDII), heavy precipitation (R95), and wet and dry spell length (WSL
and DSL) following Giorgi et al. (2014). Error bars show the
geographical variability (standard deviation) within the region and colours the
statistical significance of the trend (90 % grey, 95 % blue). This is an
example of a large number of different plots which can be produced with
<italic>recipe_hyint.yml</italic>, similar to Giorgi et al. (2014). For details see Sect. 3.1.1.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f02.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS1.SSS2">
  <label>3.1.2</label><title>Droughts</title>
      <p id="d1e1159">Three main types of droughts can be separated: (i) meteorological, (ii) hydrological, and (iii) agricultural droughts. Any type of drought needs to
be defined in the context of local and seasonal characteristics, implying
that a drought should be identified as an anomalous condition rather than being based
on an absolute threshold.</p>
      <p id="d1e1162">Meteorological droughts are negative anomalies in precipitation. Depending
on the local characteristics, a drought can be defined as an extended period
of daily precipitation amounts below a given threshold. The threshold value
is defined as the minimum amount of precipitation that is needed to recharge
the soil moisture content. This approach requires good knowledge of the
local and seasonal characteristics of the soil moisture content. However, it
is a useful analysis to investigate climate models' distributions of wet and dry
periods, which are indicative of how well suited the model is to couple to
hydrological impact models. For example, CMIP5 models have been shown to generally
underestimate the number of consecutive dry days (Sillmann et al., 2013b;
Cheng et al., 2016). The standardized precipitation index (SPI;
McKee et al., 1993) describes local precipitation anomalies and is often
used to identify meteorological droughts. The SPI was developed as a
replacement for the commonly used Palmer drought indices
(Palmer, 1965) to better capture dry and wet anomalies. The SPI
is calculated using monthly mean precipitation. Therefore, it does not
account for the intensity of single precipitation events and the runoff
process. Furthermore, SPI does not account for evaporation from the surface.
This implies that one component of the water fluxes at the surface is
lacking, which makes SPI incompatible with the concept of hydrological
droughts. Evaluation of SPI from CMIP5 models shows large model biases
(Ukkola et al., 2018).</p>
      <p id="d1e1165">A hydrological drought occurs when low water supply effects streams,
reservoirs, and groundwater levels and is usually caused by extended periods
of meteorological droughts. These hydrological processes are usually not
simulated with sufficient detail in climate models. As a consequence,
agricultural droughts (i.e. when crops become affected by the hydrological
drought) also cannot be simulated properly by the models. Hydrological droughts
can, however, be estimated in climate models by accounting for
evapotranspiration. This allows for the estimation of surface water retention.
The standardized precipitation–evapotranspiration index (SPEI;
Vicente-Serrano et al., 2010) has been developed to take into account the
effect of evapotranspiration on surface water fluxes. Evapotranspiration is
typically not provided by CMIP models, so SPEI often takes other inputs to
estimate  it, e.g. with the Thornthwaite method based on temperature
(Thornthwaite, 1948), the Hargreaves method using the monthly mean of
daily minimum and maximum near-surface temperature (tasmin and tasmax)
(Hargreaves, 1994), or the Penman–Monteith method using minimum and
maximum temperature together with 2 m wind speed (Allen et al.,
1994), which is estimated from the surface wind (at 10 m). However, it has
been shown that the method used to derive the potential evapotranspiration
has little impact on the drought statistics (Burke et al., 2006).
In contrast to this finding, Shaw and Riha (2011) conclude that,
especially for future scenarios with rising temperatures, potential
evapotranspiration based on estimates considering temperature only can lead
to an overestimation of SPEI.</p>
      <p id="d1e1168">In order to assess the performance of drought characteristics in climate
models, three diagnostics have been implemented into the ESMValTool (v2.0):
consecutive dry days, SPI, and SPEI. The consecutive dry days diagnostic
(<italic>recipe_consecdrydays.yml</italic>) has been implemented consistently with the CDO method “eca_cdd” (Climate Data Operators, Schulzweida, 2018), and the SPI
and SPEI diagnostics (<italic>recipe_spei.yml</italic>) are based on the R package SPEI
(<uri>https://cran.r-project.org/web/packages/SPEI/SPEI.pdf</uri>, last access: 1 June 2021;
Vicente-Serrano et al., 2010). The recipe <italic>recipe_spei.yml</italic> computes the SPI and SPEI
quantities for each model and summarizes the statistics of both indices as
global averages in categories from “extremely dry” to “extremely wet”;
see Figs. 3 and 4. By including an estimate for evapotranspiration, the
model biases are reduced, particularly for the overly frequent “moderately
wet” category. For SPI (Fig. 3), the bias plot shows a clear
underestimation of dry and wet conditions, which are mainly compensated for<?pagebreak page3166?> by
overly frequent moderately and extremely wet conditions. For the neutral
condition category, the results differ depending on the models, with a
tendency towards overly frequent occurrence in most models. For SPEI (Fig. 4)
the bias plot indicates overly frequent neutral conditions at the expense of
mainly dry and wet conditions. Moderate and extreme wet conditions are
overestimated in practically all models, whereas moderately and extremely dry
conditions show the opposite behaviour.</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="d1e1186">Output from SPI diagnostic in <italic>recipe_spei.yml</italic> with globally averaged histograms
of SPI over land areas, weighted by the cosine of latitude for a selection
of CMIP5 models and using gridded observations from CRUts4.01. <bold>(a)</bold> Absolute values and <bold>(b)</bold> bias of all models compared to CRUts4.01; for
details see Sect. 3.1.2.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f03.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e1206">Output from the SPEI diagnostic in <italic>recipe_spei.yml</italic> with globally averaged
histograms of SPEI over land areas, weighted by the cosine of latitude for a
selection of CMIP5 models and using gridded observations from CRUts4.01.
<bold>(a)</bold> Absolute values and <bold>(b)</bold> bias of all models compared to CRUts4.01; for
details see Sect. 3.1.2.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f04.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1226">Difference in number <bold>(a)</bold>, duration <bold>(b)</bold>, average SPI <bold>(c)</bold>, and
severity index <bold>(d)</bold> of drought events between the RCP8.5 (2050–2100) and
historic (1950 to 2000) multi-model mean of 15 CMIP5 models. Here, a drought
event is defined as any number of consecutive months with an SPI <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>. For the SPI calculation a gamma distribution and a representative timescale of 6 months are used. The figure is similar to Fig. 3a–d of
Martin (2018) and produced with recipe_martin18grl.yml; for details see Sect. 3.1.2.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f05.png"/>

          </fig>

      <p id="d1e1259">Using the SPI calculation described above, a recipe analysing drought events
(<italic>recipe_martin18.yml</italic>) has been developed. Following Martin (2018), a drought event is
defined as any consecutive number of months with extremely dry
conditions (SPI <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>). The characteristics of these events from
historical and future scenario model runs (see Fig. 5) as well as from
observational data are then compared. The characteristics investigated are
frequency, length, average SPI, and the severity index following Peters
(2014), which is a measure combining the length and the SPI value of<?pagebreak page3167?> a
drought. Figure 5 shows an increase in the number of drought events, the
severity index, and to a lesser extent the duration of drought events in the
RCP8.5 scenario compared to the historical model runs, especially in
subtropical areas. The results support the finding that regions with
already dry conditions are much more likely to show a higher number of
drought events for the RCP8.5 scenario, known as the “dry gets drier and
the wet gets wetter” (DDWW) paradigm (Greve et al., 2014).</p>
</sec>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Extreme events</title>
      <p id="d1e1286">Changes in climate extremes are of utmost concern for society as the
consequences of climate change will be strongly<?pagebreak page3168?> manifested in the severe
impacts of extreme events, such as heat waves and extreme precipitation, on
human and natural systems. Some confidence in future projections of extreme
events can be gained by evaluating the models' performance in simulating
historical events against observational data and reanalysis datasets. The 27
core climate extremes indices defined by the ETCCDI (Zhang et al., 2011)
are able to capture different characteristics of temperature and
precipitation extremes and are suitable for monitoring observed climate
extremes, model evaluation, and analysis of changes in climate extremes in
future climate projections (e.g. Sillmann et al., 2013a, b; Donat et al., 2013). To calculate these indices, daily values of
total precipitation (pr), daily mean near-surface air temperature (tas),
daily minimum near-surface air temperature (tasmin), and daily maximum
near-surface air temperature (tasmax) are required.</p>
      <p id="d1e1289">The <italic>recipe_extreme_events.yml</italic> calculates climate extremes indices and produces diagnostic figures for
comparing model and observational extremes indices as presented in IPCC AR5
chapter 9 (Flato et al., 2013) and
Sillmann et al. (2013a).</p>
      <p id="d1e1295">The index computation is performed according to Zhang et al. (2005b). The indices are calculated from CMIP models as well as gridded
observational and reanalysis data. Calculating the indices can take several
hours to days depending on the number of models and observations, the length of
the time periods analysed, and the spatial resolution of the datasets as well as
the computational resources. If possible, it is recommended to run this
processing step on a parallel computing system, taking advantage of the
ESMValTool task-based parallelization feature
(Righi et al., 2020).</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="d1e1301">Time series plot of the annual percentage of days when the daily
maximum temperature is higher than the 90th percentile for the respective
calendar day. Percentile thresholds are calculated following
Zhang et al. (2005b) for the base period 1980–2004. The
shading indicates the interquartile ensemble spread (range between the 25th
and 75th quantiles). The CMIP5 ensemble mean (blue line, five models in this
example) averaged over all land grid boxes is compared with the reanalysis
datasets MERRA-2 (green dashed line) and ERA-Interim (red dashed line).
Similar to Fig. 9.37 e of IPCC AR5
(Flato et al., 2013) and produced
with <italic>recipe_extreme_events.yml</italic>; for details see Sect. 3.2.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f06.png"/>

        </fig>

      <p id="d1e1313">There are two types of diagnostic plots that can be produced together and
that reproduce the analysis shown in Fig. 9.37 of IPCC AR5
(Flato et al., 2013) for a given
reanalysis and model dataset. The first one (see Fig. 6) shows time series
providing a temporal comparison between the mean and spread (interquartile
range) of the CMIP5 model ensemble and the individual observations for a
single index. In Fig. 6, the agreement in trends between the CMIP5 models
and reanalyses can be captured very well due to the construction of the
percentile-threshold-based indices. Deviations from the nominal level of
10 % outside the base period<?pagebreak page3169?> are mainly due to differences in the
estimated trends in tasmin and tasmax of the individual models compared
to the respective reanalysis dataset. In Sillmann et al. (2014) an
alternative approach is described to evaluate percentile-threshold-based
indices accounting for potential model biases in the mean.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e1318">“Portrait” diagram showing relative spatially averaged
root mean square error (RMSE) in the 1980–2004 climatologies of 12
temperature and 3 precipitation indices (marked with a blue rectangle)
simulated by CMIP5 models (5 in this example along the <inline-formula><mml:math id="M11" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis) with respect to
the two reanalyses ERA-Interim (upper triangle) and MERRA-2 (lower triangle).
The RMSEs are spatially averaged over all land grid points. The top row
(RMSE<inline-formula><mml:math id="M12" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">all</mml:mi></mml:msub></mml:math></inline-formula>) indicates the mean relative RMSE across all indices for the
CMIP5 ensemble mean (first column) and median (second column) as well as each model
individually. Blue (red) indicates that a model performs better
(worse) than the median of all model results when compared to the respective
reanalysis dataset. The grey shaded column at the right-hand side indicates
the median RMSE normalized by the spatial standard deviation of the index
climatology in the reanalyses (RMSE<inline-formula><mml:math id="M13" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">std</mml:mi></mml:msub></mml:math></inline-formula>). The root mean square error is
shown in greyscale on the right. See Sillmann et
al. (2013a) for details. Similar to Fig. 9.37a of the IPCC AR5 report
(Flato et al., 2013) and produced
with <italic>recipe_extreme_events.yml</italic>; for details see Sect. 3.2.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f07.png"/>

        </fig>

      <p id="d1e1355">The second diagnostic plot (Fig. 7) shows performance metrics in a “portrait
diagram”, which compares multiple models with up to four different observations
for multiple indices. The root mean square error (RMSE) between each model
and each observational or reanalysis dataset is used as a measure for model
performance. Figure 7 shows that the magnitude of median RMSE normalized by
the spatial standard deviation of the index climatology
in the reanalyses (RMSEstd) is generally larger for precipitation indices
than for the absolute and percentile-threshold indices based on temperature,
with the exception of csdi and wsdi. For the temperature-based
percentile-threshold indices (i.e. tx90p, tx10p, tn90p, and tn10p), the
models generally perform well (except IPSL-CM5A-LR) due to their
construction. This results in good agreement for the ensemble mean and
medians compared to reanalysis data, whereas the root mean square error is
too large as it is dominated by the outlier model (IPSL-CM5A-LR).</p>
      <p id="d1e1358">Indices of climate extremes are a natural extension of those for the
hydrological cycle discussed in Sect. 3.1, and effort was made to make
them available within the same analysis tool. As mentioned before, the
ETCCDI computed by <italic>recipe_extreme_events.yml</italic> can be further processed by the recipe
<italic>recipe_hyint_extreme_events.yml</italic>. Analogous to the <italic>recipe_hyint.yml</italic> (see also Sect. 3.1.1), it computes maps and box-averaged
time series for pre-selected continental or user-defined regions, computing
trends and performing significance testing over the complete set of <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:mn mathvariant="normal">6</mml:mn><mml:mo>+</mml:mo><mml:mn mathvariant="normal">27</mml:mn></mml:mrow></mml:math></inline-formula>
indices. Depending on the specific objective, the user can select the needed
subset of indices. Significance testing is performed with a Student's <inline-formula><mml:math id="M15" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test
on the non-null coefficients hypothesis, and trend coefficients are stored
together with their statistics. The recipe produces a variety of plot types
for the indices, including maps and time series with their spread, trends,
and summary plots of trend coefficients.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Impacts of climate change</title>
<sec id="Ch1.S3.SS3.SSS1">
  <label>3.3.1</label><title>Heat wave and cold wave duration</title>
      <p id="d1e1404">Heat waves are expected to become one of the greatest threats to human
health in the 21st century due to projected increases in both frequency and
severity (IPCC, 2013; Ouzeau et al., 2016), while the duration, intensity,
and frequency of cold waves are expected to decrease. It is not clear yet,
however, what the impact of changes in heat waves and cold waves on related
mortality will be, since mortality due to heat waves and cold waves inferred
from historical simulations is typically overestimated. This is partly due
to challenges in the correct simulation of extremes (Wang et al.,
2016). In the case of heat waves in particular, models have been shown to
contain biases in the 90th and 10th percentiles over the historical period
(Pereira et al., 2017). However, by using a bias<?pagebreak page3170?> adjustment
method based on percentiles, climate models are able to produce output which
is consistent with events observed during the historical period
(Ouzeau et al., 2016).</p>
      <p id="d1e1407">The diagnostics of the <italic>recipe_heatwaves_coldwaves.yml</italic> uses the daily maximum or minimum temperatures to
estimate the relative change in heat wave and cold wave characteristics in
future climates compared to a reference period. The user selects the model,
emissions scenario, the region of interest, and the reference as well as the
projection periods and the percentile which will be used to compute the
threshold for exceedance or non-exceedance from the reference period (a
separate threshold is computed for each day of the selected season and grid
point using the quantile bootstrapping method described in
Zhang et al., 2005b). Further options which can be
selected include whether to compute the frequency of exceedances or
non-exceedances of extremely high or extremely low temperature events,
respectively. Additionally, the minimum duration of an event to be
classified as a heat wave or cold wave and the season of interest can be set. The
diagnostic calculates the number of consecutive days over which temperature
exceeds or does not exceed the given threshold in future climate
projections. The result is presented as annual time series of the total
number of heat wave or cold wave days for the selected season at each grid point,
and the average number of these days for the selected season in the future
climate projections is calculated; see Fig. 8.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e1415"><bold>(a)</bold> Average annual number of summer days during the time period
2060–2080 when the daily maximum near-surface air temperature exceeds the
80th percentile of the 1971–2000 reference period. The minimum duration
of a heat wave event can be chosen in the recipe and is set to 5 d here.
<bold>(b)</bold> Mean annual number of summer days when the daily maximum near-surface air
temperature exceeds the 80th percentile of the 1971–2000 reference
period averaged over the region shown in <bold>(a)</bold>. Results shown are for the RCP8.5 scenario simulated by BCC-CSM1-1 (see Sect. 3.3.1 for details on
<italic>recipe_heatwaves_coldwaves.yml</italic>).</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f08.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS3.SSS2">
  <label>3.3.2</label><title>Combined climate extreme index</title>
      <p id="d1e1443">High mortality rates, increases in hospital admissions, and major
economic losses are often associated with extreme events (Meehl et al.,
2000; Zhang et al., 2011; Fouillet et al., 2006; Whitman et al., 1997). This
emphasizes the need for monitoring and forecasting extreme events, in
particular since some studies suggest that extremes are increasing in both
frequency and severity with increasing anthropogenic greenhouse gases
(Alexander et al., 2006; Donat et al., 2013).</p>
      <p id="d1e1446">The recipe <italic>recipe_extreme_index.yml</italic> allows a user to compute the combined climate extreme index,
which is defined as a combination of different extreme values linked to
precipitation, surface temperature, and surface wind speed. This index is
similar to the climate extremes index (CEI; Karl et
al., 1996), the modified CEI (mCEI; Gleason et al.,
2008), and the actuaries climate index (ACI; American Academy of
Actuaries, 2018). In <italic>recipe_extreme_index.yml</italic>, the user defines the area, the reference period, the
period of interest, and the weights assigned for each individual component of
the index. The weights allow the user to put emphasis on the extremes
that are more relevant to them and/or completely exclude non-relevant ones.
Temperature and precipitation extremes are defined in a similar fashion as
in Donat et al. (2013) and are part of the larger set of extreme indices
compiled by the ETCCDI (Zhang et al., 2011). The different components of
the multi-metric index are the following:
<list list-type="bullet"><list-item>
      <p id="d1e1457"><italic>weight_t90p</italic> representing the number of days when the maximum temperature exceeds the 90th
percentile,</p></list-item><list-item>
      <p id="d1e1463"><italic>weight_t10p</italic> representing the number of days when the minimum temperature falls below the 10th
percentile,</p></list-item><list-item>
      <p id="d1e1469"><italic>weight_Wx</italic> representing the number of days when wind power (third power of wind speed) exceeds the
90th percentile,</p></list-item><list-item>
      <?pagebreak page3171?><p id="d1e1475"><italic>weight_cdd</italic> representing the maximum length of a dry spell (defined as the maximum number of
consecutive days when the daily precipitation is below 1 mm), and</p></list-item><list-item>
      <p id="d1e1481"><italic>weight_rx5day</italic> representing the maximum precipitation accumulated during 5 consecutive days.</p></list-item></list>
The thresholds are computed for each day in a season using a 5 d
running window as described in Zhang et al. (2005a). For the calculation
of the index a user-defined reference period is used for normalization and
computation of the threshold corresponding to the selected metric. This
recipe creates a plot containing the time average of the components listed
above for the period of interest (Fig. 9a–e). The recipe also computes
the area-weighted average of those components and combines them into a
single index using the weights and the running mean (<italic>running_mean</italic> parameter) defined by
the user. The output of the recipe consists of a NetCDF file of the
area-weighted and multi-model multi-metric index and a plot of the time
series of that index over the selected period.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e1492"><bold>(a–e)</bold> Average change in each of the components of the combined
climate extreme index for the time period 2020–2040 compared to the
1971–2000 reference period: <bold>(a)</bold> upper temperature percentile, <bold>(b)</bold> lower
temperature percentile, <bold>(c)</bold> wind, <bold>(d)</bold> drought, <bold>(e)</bold> maximum precipitation.
Panel <bold>(f)</bold> shows a time series for the combined index for 2020–2040. The
results are shown for the RCP8.5 scenario simulated by MPI-ESM-MR (see
Sect. 3.3.2 for details on <italic>recipe_extreme_index.yml</italic>).</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f09.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS3.SSS3">
  <label>3.3.3</label><title>Daily temperature range variation</title>
      <p id="d1e1533">The daily temperature range (DTR) corresponds to the difference between the
minimum and maximum temperature within a period of 24 h at a given
location. The usefulness of the global average DTR has been demonstrated using
both observations and climate model simulations (Braganza et al.,
2004). Changes in the mean and variability of the DTR have been shown to
have a wide range of impacts on society, for example on the transmission of
diseases (Lambrechts et al., 2011; Paaijmans et al., 2010) and energy
consumption (Déandreis et al., 2014).</p>
      <p id="d1e1536">In the energy sector, a vulnerability indicator based on the DTR has been
defined to identify locations which may experience increased diurnal
temperature variations in the future (Déandreis et al.,
2014). Increased diurnal temperature variations put additional stress on the
operational management of urban heating systems. A measure for increased
diurnal temperature variations is defined as the DTR exceeding the value of
the reference period by 5 K at a given location and for a given day of the
year. Projections of this measure are currently subject to large
uncertainties as projections of both daily maximum and minimum near-surface
temperature (tasmax and tasmin) in future climate projections are highly
uncertain.</p>
      <p id="d1e1539">The recipe <italic>recipe_diurnal_temperature_index.yml</italic> computes the mean DTR for a given reference period using
historical simulations and then the number of days on which the DTR in
future climate projections exceeds that of the reference period by 5 K or
more. The user can define both the reference and projection periods, as well as the
region to be analysed. The output produced by this recipe consists of a
four-panel plot showing the maps of the projected mean DTR indicator for
each season (see Fig. 10) and a NetCDF file containing the corresponding
data.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e1548">Average number of days per year exceeding the diurnal temperature
range (DTR) of the historical period (1961–1990) by 5 K during the
period 2030–2080. The example shown is calculated for the RCP8.5 scenario
simulated by MPI-ESM-MR (see Sect. 3.3.3 for details on
<italic>recipe_diurnal_temperature_index.yml</italic>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f10.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS3.SSS4">
  <label>3.3.4</label><title>Capacity factor</title>
      <p id="d1e1568">The energy sector is the largest contributor to greenhouse gas (GHG)
emissions (IPCC, 2014b). Therefore, many countries have
adopted mitigation strategies to increase the fraction of energy generated
from renewable sources in the forthcoming years. However, renewable energy
sources like wind power and solar power rely heavily on atmospheric
conditions to produce energy and are therefore exposed to risks from climate
variability and long-term change in the case that they lead to detrimental
atmospheric conditions. The relationship between wind speed and energy
production by wind turbines is highly non-linear because turbines are
designed to be efficient for a narrow band of wind speed conditions.
Therefore, changes in the wind speed distribution can impact<?pagebreak page3172?> electricity
generation and thus the revenues and economic viability of wind farms. The
capacity factor is a normalized indicator of the suitability of wind speed
conditions to produce electricity, irrespective of the size and number of
installed turbines. The factor is provided for wind turbines designed for
low, medium, and high wind speed conditions  grouped into three different
classes (IEC, 2005).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e1573">Wind capacity factor for five kinds of wind turbines: Enercon E70 <bold>(a)</bold>, Gamesa G80 <bold>(b)</bold>, Gamesa G87 <bold>(c)</bold>, Vestas V100 <bold>(d)</bold>, and Vestas V110 <bold>(e)</bold> using the IPSL-CM5A-MR
simulation for the RCP8.5 scenario during the period 2021–2050 (see Sect. 3.3.4 for details on <italic>recipe_capacity_factor.yml</italic>).</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f11.png"/>

          </fig>

      <p id="d1e1601">The recipe <italic>recipe_capacity_factor.yml</italic> computes the wind capacity factor for these three wind turbine
classes (see Fig. 11) by taking as input the daily instantaneous surface<?pagebreak page3173?> wind
speed and extrapolating to the wind speed at 100 m of height as described in
(Lledo et al., 2019). The user can select the region, period, and season
of interest. The result of the recipe is the capacity factor for each of the
three turbine classes saved as a NetCDF file.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e1610">Photovoltaic capacity factor during the DJF period 1980–2005
using ERA-Interim <bold>(a)</bold>, CMCC-CM <bold>(b)</bold>, CNRM-CM5 <bold>(c)</bold>, IPSL-CM5-MR <bold>(d)</bold>, MIROC5 <bold>(e)</bold>, and MRI-CGCM3 <bold>(f)</bold> (see Sect. 3.3.4 for details on
<italic>recipe_pv_capacity_factor.yml</italic>).</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f12.png"/>

          </fig>

      <p id="d1e1641">The output of solar photovoltaic (PV) systems depends on the time of the
day, season, and weather conditions. The PV capacity factor is a measure of
which fraction of the maximum possible energy is produced per grid cell. The
solar power generation of a PV system mainly depends on the amount of
incoming surface solar radiation but is also influenced by other atmospheric
variables that affect the efficiency of PV cells, which decreases as their
temperature increases. The <italic>recipe_pv_capacity_factor.yml</italic> computes the PV capacity factor using the daily
incoming surface solar radiation and the surface temperature with a method
described in Bett and Thornton (2016). The user can select
temporal range, season, and region of interest. An example is shown in
Fig. 12 for ERA-Interim and five CMIP5 models.</p>
</sec>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Applications for regional scales</title>
<sec id="Ch1.S3.SS4.SSS1">
  <label>3.4.1</label><title>Evaluation of global climate models for selected regions</title>
      <p id="d1e1663">Climate or Earth system models with a fully coupled ocean are important
tools to project the future evolution of the climate system in response to
anthropogenic forcings, such as the increase in GHG concentrations. Despite
their coarse horizontal resolutions (typically of the order of 100 km or less) these models can provide climate information at the
regional scale to allow for assessing the impacts of climate change.<?pagebreak page3174?> The
ability of these models to simulate regional climate is an important aspect
of model evaluation.</p>
      <p id="d1e1666">The recipe <italic>recipe_flato13ipcc.yml</italic> includes a subset of diagnostics and figures from the model
evaluation chapter of the IPCC AR5
(chapter 9, Flato et al., 2013),
which compares surface parameters (such as temperature and precipitation)
from models and observations at regional scales.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e1674">Difference of the mean seasonal cycle for the surface temperature
(tas) between 38 CMIP5 models and ERA-Interim data averaged for 1980–1999
over land in different regions: western North America (WNA), eastern North
America (ENA), Central America (CAM), tropical South America (TSA), southern
South America (SSA), Europe and the Mediterranean (EUM), North Africa (NAF),
central Africa (CAF), southern Africa (SAF), northern Asia (NAS), central Asia
(CAS), East Asia (EAS), South Asia (SAS), Southeast Asia (SEA), and
Australia (AUS). Similar to Fig. 9.38a of the IPCC AR5 report
(Flato et al., 2013) and produced
with <italic>recipe_flato13ipcc.yml</italic>; for details see Sect. 3.4.1.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f13.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><?xmltex \currentcnt{14}?><?xmltex \def\figurename{Figure}?><label>Figure 14</label><caption><p id="d1e1689">Box-and-whisker plots showing the 5th, 25th, 50th, 75th, and 95th
percentiles of the seasonal and annual mean biases for the surface
temperature (tas) between 34 CMIP5 models and ERA-Interim data. The regions
are as follows: Alaska and NW Canada (ALAs); eastern Canada, Greenland, and Iceland (CGIs);
western North America (WNAs); central North America (CNAs); eastern North
America (ENAs); Central America and Mexico (CAMs); the Amazon (AMZs); NE Brazil
(NEBs); the west coast of South America (WSAs); south-eastern South America (SSAs);
northern Europe (NEUs); central Europe (CEUs); southern Europe and the
Mediterranean (MEDs); the Sahara (SAHs); western Africa (WAFs); eastern Africa
(EAFs); southern Africa (SAFs); northern Asia (NASs); western Asia (WASs);
central Asia (CASs); the Tibetan Plateau (TIBs); eastern Asia (EASs); southern
Asia (SASs); Southeast Asia (SEAs); northern Australia (NASs); and southern
Australia and New Zealand (SAUs). The positions of these regions are shown on the
map; they differ from the ones in Fig. 12 and are defined following
Seneviratne et al. (2012).
Similar to Fig. 9.39a, c, and e of the IPCC AR5 report
(Flato et al., 2013) and produced
with <italic>recipe_flato13ipcc.yml</italic>; for details see Sect. 3.4.1.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f14.png"/>

          </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F15"><?xmltex \currentcnt{15}?><?xmltex \def\figurename{Figure}?><label>Figure 15</label><caption><p id="d1e1703">Box-and-whisker plots showing the 5th, 25th, 50th, 75th, and 95th
percentiles of the seasonal and annual mean biases for the precipitation
(pr) in oceanic and polar regions between 38 CMIP5 models and CRU data.
Similar to Fig. 9.40b, d, and f of the IPCC AR5 report
(Flato et al., 2013) and produced
with <italic>recipe_flato13ipcc.yml</italic>; for details see Sect. 3.4.1.</p></caption>
            <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f15.png"/>

          </fig>

      <p id="d1e1715">The mean seasonal cycle of precipitation and temperature is calculated over land
areas within selected regions for individual models, the multi-model mean,
and observation and/or reanalysis data (see Fig. 13). Regional biases, including
5th, 25th, 50th, 75th, and 95th percentiles of the biases, in seasonal and
annual mean temperature and precipitation are evaluated for several land,
polar, and oceanic regions (see Figs. 14 and 15). Diagnostics allow the
comparison of the multi-model mean for different projects (i.e. CMIP3,
CMIP5) including information on the amplitude of the root mean square error.
The regions used in this recipe can be irregular polygons and are defined
following the IPCC Special Report on Managing the Risks of Extreme Events
and Disasters to Advance Climate Change Adaptation (SREX) land regions
(Seneviratne et al., 2012). In
addition to the regions described here, the ESMValTool preprocessor can be
used to run many diagnostics on distinct regions defined by latitude and
longitude limits. We plan to also include regions with more complex
boundaries like the CORDEX (Coordinated Regional Downscaling Experiment)
regions (Gutowski et al., 2016).</p>
      <p id="d1e1718">Systematic biases in modelled projections (Boberg and Christensen,
2012) can be investigated by ranking models against observed monthly mean
temperature (see Fig. 16).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F16" specific-use="star"><?xmltex \currentcnt{16}?><?xmltex \def\figurename{Figure}?><label>Figure 16</label><caption><p id="d1e1723">Ranked modelled versus ERA-Interim mean temperature for 38 CMIP5
models in the Mediterranean region (defined as in Fig. 14) for the
1979–2000 period. Similar to Fig. 9.41b of the IPCC AR5 report
(Flato et al., 2013) and produced
with <italic>recipe_flato13ipcc.yml</italic>; for details see Sect. 3.4.1.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f16.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS4.SSS2">
  <label>3.4.2</label><title>Stochastic downscaling</title>
      <p id="d1e1743">The stochastic downscaling recipe is an example of how the ESMValTool
(including its pre-processing functionalities) can be used to create a
post-processing chain for further downscaling applications, but it is strictly
speaking not a diagnostic.</p>
      <p id="d1e1746">The application of climate model projections and forecasts to impact studies
at small scales, such as hydrological modelling or ecological modelling,
requires bridging the large gap between the spatial resolution of current
global and regional climate models and the scales required for a correct
representation of the spatial and temporal structure of precipitation at
fine scales as well as of the probability of extreme precipitation events. In
the absence of a dynamical, physically based representation, a possible approach
is the use of stochastic rainfall downscaling techniques. In particular, the
Rainfall Filtered AutoRegressive Model (RainFARM; Rebora et al., 2006;
D'Onofrio et al., 2014; Terzago et al., 2018) method is a weather generator
which has only<?pagebreak page3176?> one free parameter (which can be derived from large
scales) and which requires no further calibration. RainFARM can create
ensembles of high-resolution precipitation fields from coarse-scale climate
model data. This method also allows quantification of uncertainties and a
realistic representation of subgrid-scale variability of precipitation and
of precipitation extremes, which is a crucial prerequisite for impact
studies in the water sector.</p>
      <p id="d1e1749">The recipe <italic>recipe_rainfarm.yml</italic> allows running RainFARM within the ESMValTool. Downscaled output
can be produced directly from the climate model results read by the
ESMValTool and exploiting its input checking, validation, and pre-processing
features. The recipe produces ensembles of downscaled fields (see Fig. 17)
over selected regions in NetCDF format, which can then be used by users for
further analysis. Notice how the downscaled fields introduce fine-scale
precipitation structures while still maintaining on average the original
coarse-resolution precipitation. Different stochastic realizations are shown
to demonstrate how an ensemble of realizations can be used to reproduce
unresolved subgrid variability.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F17" specific-use="star"><?xmltex \currentcnt{17}?><?xmltex \def\figurename{Figure}?><label>Figure 17</label><caption><p id="d1e1758"><bold>(a)</bold> Example of daily accumulated precipitation from the
EC-EARTH CMIP5 model on a specific day (artificial date, not a real
precipitation event), downscaled using RainFARM from its original resolution
(1.125<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). <bold>(b, c)</bold> Two stochastic realizations
for increasing the spatial resolution by a factor of 8 to 0.14<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>;
a fixed spectral slope of <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mi>s</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.7</mml:mn></mml:mrow></mml:math></inline-formula> was used. The data were produced by
<italic>recipe_rainfarm.yml</italic>, but this plot was not produced by ESMValTool – the recipe output is NetCDF
only.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f17.png"/>

          </fig>

</sec>
</sec>
<?pagebreak page3177?><sec id="Ch1.S3.SS5">
  <label>3.5</label><title>Multi-model ensemble member sub-selection</title>
      <p id="d1e1814">Large multi-model ensembles are a way to assess model and scenario
uncertainties in future climate projections and other model experiments.
However, considering constraints in the availability of computer time and
human resources, not all available ensemble members can be included in most
detailed climate impact studies associated with a given future scenario.
Therefore, despite the importance of using an ensemble that is
representative for the region and process of interest covering their full
uncertainty range, one or a few ensemble members are often rather subjectively
selected depending on, for example, their availability and simplicity in
accessing the datasets. Using more specific information about the needs of the
impact study as guidance for the selection of simulations, the resulting
subset can be better suited for the purpose of climate change impact
research. Here, we present an efficient and flexible tool that makes better
use of the ensemble by reducing its size while maintaining important
ensemble characteristics.</p>
      <p id="d1e1817">To find an optimal subset of significantly different model projections for a
given emission scenario, a clustering algorithm is applied to the
multi-model ensemble for data reduction. This technique is already used to
characterize the most likely scenarios in an ensemble of weather forecasts
(Ferranti and Corti, 2011; Straus et al., 2017). Similar methodologies
also based on cluster analysis have been explored to select a subset from an
ensemble of climate simulations (Wilcke and<?pagebreak page3178?> Barring, 2016). This
approach, applied at a regional level, can also be used to identify the
subset of climate model ensemble members that best represent the full range
of results for further downscaling applications.</p>
      <p id="d1e1820">The choice of the ensemble members is made flexible in order to meet the
requirements of specific (regional) climate products and can be defined
according to region and user needs. The decision of which variables are
considered depends on the type and goals of the climate change impact
assessment. For example, a study on future hydrological floods would particularly require
changes in precipitation extreme quantiles, and a study on the
impact of climate change on the exploitation of ski slopes would require
information about changes in winter temperatures and precipitation.</p>
      <p id="d1e1823">EnsClus (recipe <italic>recipe_ensclus.yml</italic>) is a cluster analysis tool in written in Python for
ensembles of climate model simulations. The tool is based on the <inline-formula><mml:math id="M19" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-means
algorithm with the aim to group ensemble members by similar characteristics
and to select the most representative member for each cluster. The user
chooses which characteristic is used to group the ensemble members by the
clustering: maximum, a given percentile (75 % in the example below), mean,
standard deviation, or trend over the period. For each ensemble member this
value is computed at each grid point. This results in <inline-formula><mml:math id="M20" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> latitude–longitude
maps, with <inline-formula><mml:math id="M21" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> representing the number of ensemble members. The anomalies are computed
by subtracting the ensemble mean of these maps from each of the individual
maps. The anomalies are therefore not computed with respect to time but to
the ensemble members. An empirical orthogonal function (EOF) analysis is
performed on these anomaly maps. For the EOF analysis, the user can set
either how many principal components (PCs) should be calculated or the
minimum percentage of the explained variance which should be covered. After
reducing dimensionality via EOF analysis, the <inline-formula><mml:math id="M22" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-means algorithm is applied
using the selected PCs (the number <inline-formula><mml:math id="M23" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> of clusters needs to be defined prior
to the analysis). The output of the recipe is a classification by clusters,
i.e. which ensemble member belongs to which cluster and the most
representative ensemble member for each cluster, defined by the member being
closest to the cluster centroid. Additionally, output of the recipe includes
the statistics of clustering: in the PC space, the minimum and the maximum
distance between a member in a cluster and the cluster centroid (i.e. the
closest and the farthest member), as well as the intra-cluster standard deviation
for each cluster (i.e. compactness of the cluster). An example is shown in
Fig. 18. The figure shows a clustering based on the 75th percentile of
the historical summer (JJA) precipitation rate for 32 CMIP5 models for the
period 1900–2005. Based on the principal components explaining 80 % of the
variance, three clusters are computed. The green cluster is the most
populated with 16 ensemble members. It is mostly characterized by a positive
anomaly over central–northern Europe. The red cluster contains 12 ensemble
members. It exhibits a negative anomaly centred over southern Europe and in
a<?pagebreak page3179?> few cases (e.g. no. 12 and no. 23) extending north. The third cluster (blue)
includes only four models. It shows a north–south dipolar precipitation
anomaly, with a wetter than average Mediterranean counteracting drier
northern Europe. Ensemble members no. 9, no. 26, and no. 19 are the “specimen” of
each cluster, i.e. the model simulations that best represent the main
features of that cluster. These three ensemble members can eventually be
used as representative of all possible outcomes of the multi-model
ensemble distribution associated with the 32 CMIP5 historical integrations for
the summer precipitation rate 75th percentile over Europe. This reduces the
outcomes from 32 to 3 ensemble members. The number of ensemble members of
each cluster might provide a measure of the probability of occurrence of
each cluster. However, the final results are sensitive to models' bias and
to the metric used, as in any selection exercise.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F18" specific-use="star"><?xmltex \currentcnt{18}?><?xmltex \def\figurename{Figure}?><label>Figure 18</label><caption><p id="d1e1868">Clustering based on the 75th percentile of the historical summer
(JJA) daily precipitation rate for 32 CMIP5 models for the period 1900–2005.
The colour of the model number of each ensemble member indicates the cluster
to which they belong. The most representative members of each cluster are
marked with a coloured border. See Sect. 3.5 for details on
<italic>recipe_ensclus.yml</italic>.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/3159/2021/gmd-14-3159-2021-f18.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Summary</title>
      <p id="d1e1889">This paper summarizes the recipes available within the ESMValTool v2.0 for
the analysis of extreme events, droughts, model impact assessment,
sub-selection of multi-model ensemble members (e.g. for downscaling
applications), and model evaluation on regional scales. It complements
the series of papers that have been published on ESMValTool v2.0 by
Righi et al. (2020) describing the
technical aspects of ESMValTool v2.0, Eyring et al. (2020) presenting the
new large-scale diagnostics that have been included in v2.0 since<?pagebreak page3180?> the first
release in 2016 (Eyring et al., 2016), and
Lauer et al. (2020) covering emergent
constraints and diagnostics for the analysis of future projections from ESMs
in CMIP.</p>
      <p id="d1e1892">For droughts, recipes calculating the consecutive number of dry days, the
SPI, and the SPEI have been newly included in ESMValTool v2.0, as has a
recipe to analyse the frequency, length, and severity of drought events
based on the SPI.</p>
      <p id="d1e1895">For further analysis of extreme events, climate extreme indices of the
Expert Team on Climate Change Detection and Indices (ETCCDI) based on
Zhang et al. (2011) have been included. These indices are calculated
based on daily total precipitation and the mean, minimum, and maximum of the
near-surface air temperature. The indices can then be plotted, used as a
measure of model performance, and further processed to calculate index
trends and their significance.</p>
      <p id="d1e1898">For model impact assessments, recipes to analyse heat wave and cold wave
duration, diurnal temperature variations, and different extreme
indices are included in ESMValTool v2.0. Additional recipes compute capacity
factors to analyse the impact of climate change on  wind and solar energy
production.</p>
      <p id="d1e1902">For the analysis of ensembles of climate models, ESMValTool v2.0 provides a
cluster analysis based on a <inline-formula><mml:math id="M24" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-means algorithm whereby the ensemble members are
divided into clusters and can be plotted along with the properties of the
clusters and the most representative member of each cluster.</p>
      <p id="d1e1912">ESMValTool v2.0 also includes diagnostics for model evaluation on regional
scales. Surface parameters such as temperature and precipitation can be
evaluated for regions defined by polygons following the SPEX definitions of
land regions. Additionally, the ESMValTool output can be
processed further by tools for stochastic downscaling like RainFARM, which
is also implemented in v2.0.</p>
      <p id="d1e1915">Although the recipes here are presented using CMIP5 data, ESMValTool v2.0
can be run to perform the same analysis for CMIP6 data. As an open-source
project, the capabilities of the ESMValTool continue to grow, with
contributions from the scientific community highly welcome. Users can
analyse data using a wealth of existing recipes or join the ESMValTool
development team and add new recipes and diagnostics.</p>
</sec>

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

      <p id="d1e1923">ESMValTool v2.2 is released under the Apache
License version 2.0. The latest release of ESMValTool v2.2 is publicly
available on Zenodo at <ext-link xlink:href="https://doi.org/10.5281/zenodo.4562215" ext-link-type="DOI">10.5281/zenodo.4562215</ext-link>
(Andela et al., 2021a). The source code of the ESMValCore package, which
is installed as a dependency of the ESMValTool v2.2, is also publicly
available on Zenodo at <ext-link xlink:href="https://doi.org/10.5281/zenodo.4525749" ext-link-type="DOI">10.5281/zenodo.4525749</ext-link>
(Andela et al., 2021b). ESMValTool and ESMValCore are
developed on the<?pagebreak page3181?> GitHub repositories available at <uri>https://github.com/ESMValGroup</uri> (last access: 24 July 2020). CMIP5 data are
freely and publicly available from the Earth System Grid Federation.
Observations used in the evaluation are detailed in the various sections of
the paper and listed in Table 1. They are not distributed with ESMValTool,
which is restricted to the code as open-source software.<?xmltex \hack{\vspace*{-4mm}}?></p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1939">KW led the writing of the paper and, with the help of LB, BKG, AL, MR, MS, and
ND, coordinated the implementation of the diagnostics for this paper in
ESMValTool v2.0. VE coordinated the ESMValTool v2.0 release. All other
authors contributed to individual diagnostics for this release. All authors
contributed to the text.<?xmltex \hack{\vspace*{-4mm}}?></p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1946">The authors declare that they have no conflict of interest.<?xmltex \hack{\vspace*{-4mm}}?></p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1953">The diagnostic development of ESMValTool v2.0 for this paper was supported
by different projects with a different scientific focus, in particular by following: (1) Copernicus Climate Change Service (C3S) “Metrics and Access to Global
Indices for Climate Projections (C3S-MAGIC)” project C3S_34a
Lot 2; (2) the Horizon 2020 European Union Framework Programme for Research
and Innovation under grant agreement no. 641816, project CRESCENDO
(Coordinated Research in Earth Systems and Climate: Experiments, kNowledge,
Dissemination and Outreach); (3) the Helmholtz Society project “Advanced Earth
System Model Evaluation for CMIP (EVal4CMIP)”; and (4) the Federal Ministry of
Education and Research (BMBF) CMIP6-DICAD project. In addition, we received
technical support for the ESMValTool v2.0 development from the European
Union's Horizon 2020 Framework Programme for Research and Innovation
“Infrastructure for the European Network for Earth System Modelling
(IS-ENES3)” project under grant agreement no. 824084. We acknowledge the
World Climate Research Program's (WCRP's) Working Group on Coupled Modelling
(WGCM), which is responsible for CMIP, and we thank the climate modelling
groups for producing and making available their model output. This work used
JASMIN, the UK collaborative data analysis facility, and the DAS-5
(the Distributed ASCI Supercomputer 5) experimental supercomputer
(Bal et al., 2016). The computational resources of the
Deutsches Klimarechenzentrum (DKRZ, Germany) were also essential for
developing and testing this new version and are kindly acknowledged.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e1958">This research has been supported by the Copernicus Climate Change Service (C3S) (Metrics and Access to Global Indices for Climate Projections (C3S-MAGIC), C3S_34a Lot 2), the Helmholtz-Gemeinschaft (Advanced Earth System Model Evaluation for CMIP (grant no. EVal4CMIP)), the Horizon 2020 Framework Programme, H2020 Societal Challenges (CRESCENDO (grant no. 641816)), the Federal Ministry of Education and Research (BMBF) (grant no. CMIP6-DICAD), and the Horizon 2020 Framework Programme, H2020 Excellent Science (IS-ENES3 (grant no. 824084)).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>The article processing charges for this open-access<?xmltex \notforhtml{\newline}?> publication were covered by the University of Bremen.<?xmltex \hack{\vspace*{-4mm}}?></p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1970">This paper was edited by Carlos Sierra and reviewed by two anonymous referees.<?xmltex \hack{\vspace*{-5mm}}?></p>
  </notes><ref-list>
    <title>References</title>

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    <!--<article-title-html>Earth System Model Evaluation Tool (ESMValTool) v2.0 – diagnostics for extreme events, regional and impact evaluation, and analysis of Earth system models in CMIP</article-title-html>
<abstract-html><p>This paper complements a series of now four publications that
document the release of the Earth System Model Evaluation Tool (ESMValTool)
v2.0. It describes new diagnostics on the hydrological cycle, extreme
events, impact assessment, regional evaluations, and ensemble member
selection. The diagnostics are developed by a large community of scientists
aiming to facilitate the evaluation and comparison of Earth system models
(ESMs) which are participating in the Coupled Model Intercomparison Project
(CMIP). The second release of this tool aims to support the evaluation of
ESMs participating in CMIP Phase 6 (CMIP6). Furthermore, datasets from
other models and observations can be analysed. The diagnostics for the
hydrological cycle include several precipitation and drought indices, as
well as hydroclimatic intensity and indices from the Expert Team on Climate
Change Detection and Indices (ETCCDI). The latter are also used for
identification of extreme events, for impact assessment, and to project
and characterize the risks and impacts of climate change for natural and
socio-economic systems. Further impact assessment diagnostics are included
to compute daily temperature ranges and capacity factors for wind and solar
energy generation. Regional scales can be analysed with new diagnostics
implemented for selected regions and stochastic downscaling. ESMValTool v2.0
also includes diagnostics to analyse large multi-model ensembles including
grouping and selecting ensemble members by user-specified criteria. Here, we
present examples for their capabilities based on the well-established CMIP
Phase 5 (CMIP5) dataset.</p></abstract-html>
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