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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="data-paper">
  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESSD</journal-id><journal-title-group>
    <journal-title>Earth System Science Data</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESSD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Sci. Data</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1866-3516</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/essd-14-1233-2022</article-id><title-group><article-title>C<inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>ONTEXT: a Common Consensus on Convective OrgaNizaTion during the EUREC<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula>A eXperimenT</article-title><alt-title>C<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>ONTEXT: a Common Consensus on Convective OrgaNizaTion during the EUREC<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula>A eXperimenT</alt-title>
      </title-group><?xmltex \runningtitle{C${}^{{3}}$ONTEXT: a Common Consensus on Convective OrgaNizaTion during the EUREC${}^{4}$\!A eXperimenT}?><?xmltex \runningauthor{H. Schulz}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes">
          <name><surname>Schulz</surname><given-names>Hauke</given-names></name>
          <email>hauke.schulz@mpimet.mpg.de</email>
        <ext-link>https://orcid.org/0000-0001-5468-1137</ext-link></contrib>
        <aff id="aff1"><institution>The Atmosphere in the Earth System, Max Planck Institute for Meteorology, Hamburg, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Hauke Schulz (hauke.schulz@mpimet.mpg.de)</corresp></author-notes><pub-date><day>18</day><month>March</month><year>2022</year></pub-date>
      
      <volume>14</volume>
      <issue>3</issue>
      <fpage>1233</fpage><lpage>1256</lpage>
      <history>
        <date date-type="received"><day>26</day><month>November</month><year>2021</year></date>
           <date date-type="rev-request"><day>9</day><month>December</month><year>2021</year></date>
           <date date-type="rev-recd"><day>9</day><month>February</month><year>2022</year></date>
           <date date-type="accepted"><day>11</day><month>February</month><year>2022</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 Hauke Schulz</copyright-statement>
        <copyright-year>2022</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022.html">This article is available from https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022.html</self-uri><self-uri xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022.pdf">The full text article is available as a PDF file from https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e114">The C<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>ONTEXT (a Common Consensus on Convective OrgaNizaTion during the EUREC<inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A eXperimenT) dataset is presented as an overview of the mesoscale cloud patterns identified during the EUREC<inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A (Elucidating the role of clouds–circulation coupling in climate) field campaign in early 2020. Based on infrared and visible satellite images, 50 researchers of the EUREC<inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A science team manually identified the four prevailing mesoscale patterns of shallow convection observed by <xref ref-type="bibr" rid="bib1.bibx12" id="text.1"/>. The common consensus on the observed mesoscale cloud patterns emerging from these manual classifications is presented. It builds the basis for future studies and reduces the subjective nature of these visually defined cloud patterns. This consensus makes it possible to contextualize the measurements of the EUREC<inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A field campaign and interpret them in the mesoscale setting. Commonly used approaches to capture the mesoscale patterns are computed for comparison and show good agreement with the manual classifications. All four patterns as classified by <xref ref-type="bibr" rid="bib1.bibx12" id="text.2"/> were present in January–February 2020, although not all were dominant during the observing period of EUREC<inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A. Supplemental classifications of storm-resolving simulations suggest that the latter have a limited ability to replicate the observed cloud patterns and require further research.</p>

      <p id="d1e188">The full dataset including post-processed datasets for easier usage are openly available at the Zenodo archive at <ext-link xlink:href="https://doi.org/10.5281/zenodo.5979718" ext-link-type="DOI">10.5281/zenodo.5979718</ext-link> <xref ref-type="bibr" rid="bib1.bibx8" id="paren.3"/>.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e206">Clouds are often clustered. Examples of larger clusters are squall lines and the intertropical convergence zone. But also much smaller clouds like shallow trade wind cumuli are often seen clustered on a scale of several hundred kilometers. The understanding of these mesoscale patterns of shallow convection is still sparse. However, the ubiquity of these clouds and their reoccurring structure suggest that they play an important role in determining the radiative effects of the trade wind regimes <xref ref-type="bibr" rid="bib1.bibx1" id="paren.4"/>.
The EUREC<inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A (Elucidating the role of clouds–circulation coupling in climate) field campaign addresses among others, the question of which processes are at play that change the mesoscale appearance of shallow convection. Prior to the campaign, studies concentrated on the classification of mesoscale patterns based on satellite images by visual inspection <xref ref-type="bibr" rid="bib1.bibx12" id="paren.5"/>, rule-based algorithms <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx4" id="paren.6"/>, supervised neural networks <xref ref-type="bibr" rid="bib1.bibx6" id="paren.7"/> and unsupervised neural networks <xref ref-type="bibr" rid="bib1.bibx2" id="paren.8"/>. Most of these methods focus on four specific mesoscale cloud patterns that have been identified as commonly occurring in the North Atlantic downwind trades <xref ref-type="bibr" rid="bib1.bibx12" id="paren.9"/>. An overview of these four patterns which are named by their visual impressions as <italic>sugar</italic>, <italic>gravel</italic>, <italic>flowers</italic> and <italic>fish</italic> is given in Fig. <xref ref-type="fig" rid="Ch1.F1"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e256">Four classes of mesoscale patterns of shallow convection have been labeled by 50 scientists in satellite images of January and February 2020. An example of each of these classes is shown based on the reflectance measurements of the Moderate Resolution Imaging Spectroradiometer (MODIS) on board the Terra satellite (sugar and gravel) and the Visible Infrared Imaging Radiometer Suite (VIIRS) on board the Suomi National Polar-orbiting Partnership (NPP) satellite (flowers and fish). Example images provided by NASA Worldview.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f01.png"/>

      </fig>

      <p id="d1e265">These efforts show that the categorization of the mesoscale patterns is an elementary step in acquiring further knowledge about the cloud processes in the downstream trades; 50 scientists from 15 research institutes who were involved in the EUREC<inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A field campaign in January–February 2020 therefore participated in a joint online classification event. The results of this classification event are presented here. Due to the high attendance, the presented dataset can be interpreted as the common judgment of the EUREC<inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A science team on the mesoscale patterns of shallow convection in the wider trades during EUREC<inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A. The studied domain of 5–20<inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 62–40<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W contains the entire research area, including both the <italic>Tradewind Alley</italic> in the north (12.5–14.5<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N) and the <italic>Boulevard des Tourbillons</italic> close to the coast of South America <xref ref-type="bibr" rid="bib1.bibx13" id="paren.10"/>.  This dataset therefore allows for consistently communicating about the otherwise subjectively defined patterns and puts the measurements taken during EUREC<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A into their mesoscale context to advance the process understanding of shallow convection in the trades. The need for a better process understanding is highlighted by a supplemental classification of storm-resolving simulations covering the same time period.</p>
      <p id="d1e350">The paper is structured as follows: the dataset and its collection are described in Sect. <xref ref-type="sec" rid="Ch1.S2"/>. Potential use cases are described in Sect. <xref ref-type="sec" rid="Ch1.S3"/>. In Sect. <xref ref-type="sec" rid="Ch1.S4"/> additional classification methods that are able to detect the four mesoscale patterns are applied to the EUREC<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A time period and compared to the manual classifications described in this paper. We conclude with Sect. <xref ref-type="sec" rid="Ch1.S6"/>.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data description and development</title>
      <p id="d1e380">The manual classifications were gathered through the online platform <uri>https://www.zooniverse.org/</uri>  (last access: 1 July 2020), which has already been successfully used in an earlier project by <xref ref-type="bibr" rid="bib1.bibx6" id="text.11"/>. The platform makes it possible to crowdsource labels for, e.g., machine learning projects. Additional workflows can be defined to separate different image sources or to separate, for example, labels made during a practice run from those that belong to the actual classification. The former allowed everyone to familiarize themselves with the <?xmltex \hack{\mbox\bgroup}?><uri>https://www.zooniverse.org/</uri><?xmltex \hack{\egroup}?> platform without influencing the results.</p>
      <p id="d1e394"><?xmltex \hack{\newpage}?>For this dataset, we defined three workflows. Two workflows are based on satellite observations. The first one is based on the visible channels of both the GOES-16 (Geostationary Operational Environmental Satellite) ABI (Advanced Baseline Imager) and MODIS on board the Aqua and Terra satellites and is called EUREC<inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A VIS. The second one is based on the “clean” infrared channel (channel 13) of GOES-16 ABI only (EUREC<inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A IR).
To test how well storm-resolving simulations are able to reproduce the observed patterns, we included another workflow, EUREC<inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A ICON, which is based on ICON (ICOsahedral Nonhydrostatic) storm-resolving simulations covering the EUREC<inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A time period. The simulation has a grid spacing of  1.25 km and was initialized daily by the European Centre for Medium-Range Weather Forecasts Integrated Forecasting System (ECMWF IFS) and forced hourly. Each run is 48 h long. The first 24 h were discarded to allow for spin-up.</p>
      <p id="d1e442">To visualize the simulation output, we calculated a pseudo-albedo <inline-formula><mml:math id="M24" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> by following the approximation of <xref ref-type="bibr" rid="bib1.bibx18" id="text.12"/>:

              <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M25" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.19</mml:mn><mml:mo>⋅</mml:mo><mml:msup><mml:mi mathvariant="normal">LWP</mml:mi><mml:mfrac><mml:mn mathvariant="normal">5</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:mfrac></mml:msup><mml:mo>⋅</mml:mo><mml:msup><mml:mi>N</mml:mi><mml:mfrac><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:msup></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="italic">α</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">τ</mml:mi><mml:mrow><mml:mn mathvariant="normal">6.8</mml:mn><mml:mo>+</mml:mo><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math id="M26" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> is the optical depth, <inline-formula><mml:math id="M27" display="inline"><mml:mi mathvariant="normal">LWP</mml:mi></mml:math></inline-formula> is the liquid water vapor path and <inline-formula><mml:math id="M28" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> is an assumed cloud droplet number density. Here a number density of 70 cm<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> is used, which is at the lower end of the observed concentrations <xref ref-type="bibr" rid="bib1.bibx11" id="paren.13"/>.</p>
      <p id="d1e556">All workflows are further described in Table <xref ref-type="table" rid="Ch1.T1"/>.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e565">Description of data sources used to create the images of the classification workflows.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry namest="col2" nameend="col3" align="center">EUREC<inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A VIS </oasis:entry>
         <oasis:entry colname="col4">EUREC<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A IR</oasis:entry>
         <oasis:entry colname="col5">EUREC<inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A ICON</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry rowsep="1" colname="col2">MODIS (Terra/Aqua)</oasis:entry>
         <oasis:entry rowsep="1" colname="col3">ABI (GOES-16)</oasis:entry>
         <oasis:entry rowsep="1" colname="col4">ABI (GOES-16)</oasis:entry>
         <oasis:entry colname="col5"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Domain</oasis:entry>
         <oasis:entry namest="col2" nameend="col4" align="center">5–20<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 62–40<inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W </oasis:entry>
         <oasis:entry colname="col5">5–20<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 62–44<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Period</oasis:entry>
         <oasis:entry namest="col2" nameend="col4" align="center">7 Jan 2020–22 Feb 2020 </oasis:entry>
         <oasis:entry colname="col5">16 Jan 2020–20 Feb 2020</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Resolution</oasis:entry>
         <oasis:entry namest="col2" nameend="col4" align="center"><inline-formula><mml:math id="M37" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 km </oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M38" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula>2 km</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">(shown)</oasis:entry>
         <oasis:entry colname="col2">2-hourly, 12:00–20:00 UTC</oasis:entry>
         <oasis:entry namest="col3" nameend="col4" align="center">2-hourly </oasis:entry>
         <oasis:entry colname="col5">2-hourly</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Data source</oasis:entry>
         <oasis:entry colname="col2">Corrected reflectance</oasis:entry>
         <oasis:entry colname="col3">Channel 02 (red)</oasis:entry>
         <oasis:entry colname="col4">Channel 13 (IR)</oasis:entry>
         <oasis:entry colname="col5">Pseudo-albedo</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Number of scenes</oasis:entry>
         <oasis:entry colname="col2">94</oasis:entry>
         <oasis:entry colname="col3">234</oasis:entry>
         <oasis:entry colname="col4">562</oasis:entry>
         <oasis:entry colname="col5">425</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Remarks</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">Classified after</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">24 h spin-up</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e818">On 24 March 2020 the international, virtual classification event was hosted with 50 scientists from 15 institutes participating in the creation of the pattern classifications. For a full day the participants classified patterns of shallow trade wind convection by labeling, i.e., drawing rectangles of variable sizes around, the four common types: sugar,  gravel,  flowers and  fish <xref ref-type="bibr" rid="bib1.bibx12" id="paren.14"/>.</p>
      <p id="d1e824">In the end, over 12 500 labels were gathered. The observational workflows got the majority of the labels  (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>) because the identification of the patterns in the model simulation was too demanding. The cloud features in the simulations had too little similarity with those found in nature. By comparing the distribution of labels in the individual workflows, Fig. <xref ref-type="fig" rid="Ch1.F2"/> reveals that sugar was disproportionately rarely identified in the ICON simulations.
The largest feature, like fish, however, has been identified more often. This supports the assumption that larger features are better reproduced in storm-resolving simulations than features of smaller scales, like sugar.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e833">Distribution of labels by data source. The relative distribution is shown on the <inline-formula><mml:math id="M39" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis, while the absolute number of labels is indicated within each bar. The total number of labels per workflow is shown on the top of each bar.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f02.png"/>

      </fig>

      <p id="d1e849">Because all users have familiarity with the patterns either by previous work and/or being involved in the classification event of <xref ref-type="bibr" rid="bib1.bibx6" id="text.15"/>, it can be assumed that the labels are of high quality. In addition, they were trained immediately before starting the classification through an online presentation to get familiar with the labeling interface on <?xmltex \hack{\mbox\bgroup}?><uri>https://www.zooniverse.org/</uri><?xmltex \hack{\egroup}?> and to once more refresh the different mesoscale cloud pattern categories.
Compared to <xref ref-type="bibr" rid="bib1.bibx6" id="text.16"/>, where the focus has been to classify as many diverse cloud scenes as possible to capture nature's variability and thus serve as a better machine learning dataset, the aim for this dataset is to create a common classification dataset for the EUREC<inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A time period that participating scientists agree on and can directly be used in further studies. Therefore, the temporal frequency has been increased from daily cloud scenes to 2-hourly cloud scenes to reflect also the changes on the sub-daily scale such as those identified by <xref ref-type="bibr" rid="bib1.bibx15" id="text.17"/>. Due to this design difference, a single day is now on average classified 20 times in case of the visible workflow instead of just about 6 (3 per each daytime Aqua/Terra satellite overpass) as in <xref ref-type="bibr" rid="bib1.bibx6" id="text.18"/>. Each individual image is however still viewed about 3 times.</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="d1e884">Overview of processing levels of the datasets including the variable names used in the respective datasets.</p></caption>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f03.png"/>

      </fig>

      <p id="d1e893">After the joint classification event, over 12 500 labels were processed to make them more user friendly, especially because the raw data miss temporal and geospatial information. The processing steps with the intermediate products are illustrated in Fig. <xref ref-type="fig" rid="Ch1.F3"/> and described as follows:
<list list-type="bullet"><list-item>
      <p id="d1e900"><italic>Level 0.</italic>
The level 0 dataset consists of the raw data output and originates from the Zooniverse platform. It consists of CSV (comma-separated values) files that contain entries for each workflow, image (subject) and classification including technical details like the time spent on drawing a specific label. Labels are given by their origin (<inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:math></inline-formula>) and their height (<inline-formula><mml:math id="M42" display="inline"><mml:mi>h</mml:mi></mml:math></inline-formula>) and width (<inline-formula><mml:math id="M43" display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula>) given in pixel coordinates.</p></list-item><list-item>
      <p id="d1e932"><italic>Level 1.</italic>
The level 1 dataset is further processed and combines the information distributed over the level 0 dataset files. It contains each label as a separate entry and contains information about the classified object, the user, and the geographical and Cartesian coordinates of the label. This product is saved in a netCDF (Network Common Data Form) file.</p></list-item><list-item>
      <p id="d1e938"><italic>Level 2.</italic>
For the level 2 dataset, the data are merged by <monospace>classification_id</monospace>.</p>
      <p id="d1e946">The <monospace>classification_id</monospace> is a unique identifier of a classification, where a classification refers here to the process of labeling a single image by a single user. The user might use several labels of the same or a different kind to completely classify a scene. This process eliminates overlaps of same-user classifications for each pattern and turns the data into masks rather than coordinates (see Fig. <xref ref-type="fig" rid="Ch1.F3"/>). In cases where same-user classifications of different patterns overlap, the overlapping region is counted towards all classified patterns. This case is not handled specifically, as it shows the uncertainty a user had to classify a specific region as one or the other pattern. Masks have the advantage of being more easily queried whether a specific location is influenced by a mesoscale pattern or not. This product is saved in the Zarr format.</p></list-item><list-item>
      <p id="d1e955"><italic>Level 3.</italic>
To make working with the dataset easier, the percentage of agreement (<inline-formula><mml:math id="M44" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>) among users on a specific pattern on each location is calculated and saved as level 3 data for each workflow. It is calculated as follows:<disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M45" display="block"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>pattern</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mo>∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mi>U</mml:mi></mml:msubsup><mml:mi>c</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mi>U</mml:mi></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>where <inline-formula><mml:math id="M46" display="inline"><mml:mi>U</mml:mi></mml:math></inline-formula> is the number of users that have seen the particular image; <inline-formula><mml:math id="M47" display="inline"><mml:mi>c</mml:mi></mml:math></inline-formula> is the classification mask from the level 2 data; and <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi></mml:mrow></mml:math></inline-formula> is the geographic coordinates. Because the labels of users that attributed several classes to a single pixel are not removed, <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo>∑</mml:mo><mml:mi>p</mml:mi></mml:mrow></mml:math></inline-formula> can be greater than 100 %. An additional <italic>unclassified</italic> category is introduced to capture the agreement on unclassified regions, which is implicitly visible in, e.g., Fig. <xref ref-type="fig" rid="Ch1.F4"/>. Figure <xref ref-type="fig" rid="Ch1.F4"/> shows how participants agreed on the different patterns on 12 February depending on the workflow. This figure is continued in Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/>, where this overview of daily averaged classifications is given for each day to give an impression of the dataset and in particular the presence and distribution of mesoscale patterns during the EUREC<inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A field campaign. This product is saved in the Zarr format.</p></list-item></list></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e1075">Manual-classification examples for the three workflows (top to bottom: visible, infrared and simulation). The labels for each pattern (from left to right: sugar, flowers, fish and gravel) are shown next to the labeled image. Coastline of South America is marked in black. The circle marks the EUREC<inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A circle, one focus area of the EUREC<inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A field campaign and the main flight pattern of the participating research aircraft HALO (High Altitude and LOng Range Research Aircraft) <xref ref-type="bibr" rid="bib1.bibx5" id="paren.19"/>. Coastlines are based on GSHHG (Global Self-consistent, Hierarchical, High-resolution Shorelines) shapefiles <xref ref-type="bibr" rid="bib1.bibx16" id="paren.20"/>. Please note that the date format in this figure is year-month-day.</p></caption>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f04.png"/>

      </fig>

</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Potential dataset use and reuse</title>
      <p id="d1e1120">The EUREC<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A field campaign has been an international study with a wide range of research platforms and many minor objectives <xref ref-type="bibr" rid="bib1.bibx13" id="paren.21"/>. This dataset covers not only the core area of the experiment but also the wider area and time period. While the participating research airplanes and drones were mostly staying in the trade winds, some research vessels conducted measurements as far south as 6.5<inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N.</p>
      <p id="d1e1146">This dataset gives the opportunity to study all these measurements in the context of the mesoscale patterns observed in the downwind trades.
Due to the high subjectivity of these mesoscale cloud pattern definitions, it is of particular importance to discuss results based on a common consensus to keep studies comparable. The C<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>ONTEXT dataset can serve as such a reference for the period of the EUREC<inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A field campaign.</p>
      <p id="d1e1169">Figure <xref ref-type="fig" rid="Ch1.F5"/> shows the mesoscale context for three platforms participating in EUREC<inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A and representing different measurement strategies (see <xref ref-type="bibr" rid="bib1.bibx13" id="altparen.22"/>, for a complete list of platforms). Based on the classifications of the infrared workflow, the daily changes in the cloud patterns become apparent. The infrared workflow is preferred over the visible one because it covers both day and night and is therefore able to also capture the dial nature of the patterns <xref ref-type="bibr" rid="bib1.bibx15" id="paren.23"/>.
Before the intense observation period (IOP), 20 January to 20 February, the prevailing cloud pattern at the Barbados Cloud Observatory was gravel. With the start of the IOP, fish was detected most in the research area. After 24 January, patterns were much less widespread and well defined such that there was more disagreement on the patterns. This transition is independent of the location. Both the platforms in the north as well as R/V <italic>Atalante</italic>, which sailed further south in the Boulevard des Tourbillons (eddy boulevard), which is defined by <xref ref-type="bibr" rid="bib1.bibx13" id="text.24"/> as the area of the coastline of Brazil where the North Brazil Current (NBC) rings occur, were embedded in a similar transition. The reduced frequency of classifications towards the end of the IOP around 15 February are caused by mid-level clouds obscuring the view of shallow convection.</p>
      <p id="d1e1198">In Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/> the level 3 products are visualized for each studied day and can be used as a lookup table to quickly identify if a pattern has been identified at a specific time and place.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1206">Exemplary use case of level 3 data: mesoscale setting of research platforms during EUREC<inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A based on the EUREC<inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A IR workflow (<bold>a–c</bold>: Barbados Cloud Observatory (BCO), R/V <italic>Meteor</italic> and R/V <italic>Atalante</italic>). Please note that the date format in this figure is day.month.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f05.png"/>

      </fig>

</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Comparison with other classifications</title>
      <p id="d1e1254">Several methods have been developed to describe the mesoscale structure of shallow convection (<xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx6 bib1.bibx1 bib1.bibx2" id="altparen.25"/>). Here we focus on the comparison of the manual classifications with two other methods that specifically aim to detect the four mesoscale patterns of the downwind trades as defined by <xref ref-type="bibr" rid="bib1.bibx12" id="text.26"/> and shown in Fig. <xref ref-type="fig" rid="Ch1.F1"/>. <xref ref-type="bibr" rid="bib1.bibx1" id="text.27"/> combined a measure of organization (<inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <xref ref-type="bibr" rid="bib1.bibx14" id="altparen.28"/>) with the mean cluster size (<inline-formula><mml:math id="M61" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>), while <xref ref-type="bibr" rid="bib1.bibx6" id="text.29"/> developed a deep neural network to detect the patterns. Although <xref ref-type="bibr" rid="bib1.bibx4" id="text.30"/> show that different combinations of metrics, like cloud fraction and fractal dimension, better describe the variance in a cloud field, the pair of <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and mean cluster size has been widely used and is considered here for better comparison.</p>
      <p id="d1e1307">To assess the agreement between the different classification methods, we compare the method of <xref ref-type="bibr" rid="bib1.bibx1" id="text.31"/> and a deep neural network based on <xref ref-type="bibr" rid="bib1.bibx6" id="text.32"/> that detects the patterns in geostationary infrared images of GOES-16 ABI <xref ref-type="bibr" rid="bib1.bibx10" id="paren.33"/> instead of visible images taken on board the polar-orbiting satellites Terra and Aqua. It should be noted that this deep neural network has not been trained with the manual classifications presented here but with the manual classifications of <xref ref-type="bibr" rid="bib1.bibx6" id="text.34"/> which cover older years and included different geographical regions. The network is identical to the one used in <xref ref-type="bibr" rid="bib1.bibx10" id="text.35"/>.</p>
      <p id="d1e1325">Because the <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula> measure is sensitive to the domain size, we compute these metrics over a <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mn mathvariant="normal">10</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> sub-domain and consider only classifications within this domain for the comparison. Specifically, we focus on the region 10–20<inline-formula><mml:math id="M66" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 58–48<inline-formula><mml:math id="M67" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W. This domain size ensures that <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> describes the organization on the mesoscale and the cloud patterns we are interested in. The method has been successfully used in this domain in <xref ref-type="bibr" rid="bib1.bibx1" id="text.36"/> and applied accordingly. Brightness temperatures between 280 and 290 K are regarded as clouds. Days where the 25th percentile of brightness temperatures within any satellite image is lower than 285 K are discarded to avoid a bias by high clouds.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e1399">Comparison of the <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> versus mean cluster size (<inline-formula><mml:math id="M70" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>) classification method and the <bold>(a)</bold> <italic>manually</italic> classified patterns and <bold>(b)</bold> the neural network classifications. For each <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula> classification, the manually/automatically classified pattern area for each pattern is indicated as wedges of different sizes. Mean cluster size is given as a fraction of the domain size and multiplied by <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> to be consistent with <xref ref-type="bibr" rid="bib1.bibx1" id="text.37"/>. Grey areas indicate the middle terciles of <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M74" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> and are the bounds of the four pattern quadrants. All classifications are based on the GOES-16 ABI infrared images and are daily averages.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f06.png"/>

      </fig>

      <p id="d1e1483">Figure <xref ref-type="fig" rid="Ch1.F6"/> shows the comparison of the different methods. From the appearance of the patterns, we expect gravel and flowers to be rather regularly distributed and therefore to have a lower <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> compared to fish and sugar. It should be noted that <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is calculated based on a threshold in brightness temperature, and therefore only the deeper clouds in the sugar field are considered leading to a higher <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> value than one would expect from an otherwise rather randomly distributed cloud field. The mean cluster size should be small for sugar and gravel and larger for flowers and fish.</p>
      <p id="d1e1521">Indeed, the pattern area fraction maximizes for each pattern in the respective quadrant of the <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula> space independent of the classification method. Gravel classifications dominate the lower-left quadrant; sugar dominates the upper-left quadrant; and fish dominates the upper-right one. Flowers are harder to associate with a quadrant, as they are more centered. In general, the <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula> distribution has a large range of values for small mean cluster sizes and narrows with increasing mean cluster size.</p>
      <p id="d1e1554">This is also in alignment with <xref ref-type="bibr" rid="bib1.bibx1" id="text.38"/>, where the lower-right quadrant includes not only flowers but also about 35 % of the fish cases (their Fig. 1c). Flowers' cloud entities are generally smaller than those of the fish pattern and therefore cannot separate very well from the other patterns.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e1562">Time series of the area fraction covered by each pattern as identified in the workflows EUREC<inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A VIS (first bar), EUREC<inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A IR (second bar), EUREC<inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A ICON (third bar) and the deep neural network trained for the infrared classification of cloud patterns (fourth bar in <bold>a</bold>) within the area of 10–20<inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>N, 58–48<inline-formula><mml:math id="M84" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W. Thresholds of 0.1 <bold>(a)</bold> and 0.5 <bold>(b)</bold> have been applied to the percentage of agreement of the manual classifications and visualize that the overlap of different categories (cumulative area fractions above 1) is eliminated in the latter. Please note that the date format in this figure is year-month-day.</p></caption>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f07.png"/>

      </fig>

      <p id="d1e1633">Figure <xref ref-type="fig" rid="Ch1.F7"/> reveals the time series of the area fraction covered by the mesoscale patterns within the region of 10–20<inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 58–48<inline-formula><mml:math id="M86" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W and identified by the different classification approaches. For a better comparison with the EUREC<inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A VIS workflow, Fig. 7 is only based on daytime classifications (12:00–20:00 UTC).</p>
      <p id="d1e1667">To convert the agreement on patterns in the level 3 dataset into actual classifications, we applied a threshold of <inline-formula><mml:math id="M88" display="inline"><mml:mn mathvariant="normal">0.1</mml:mn></mml:math></inline-formula> to the percent agreement so that at least 10 % of participants who viewed a given scene must have agreed on a pattern. Agreement below this threshold is treated as an unclassified region. This threshold should be seen as a lower bound and is only used to reduce the noise of the classifications. For comparison, we also apply a stricter threshold of 0.5, which removes most of the overlap (Fig. <xref ref-type="fig" rid="Ch1.F7"/>b). The overall day-to-day changes remain robust.
Figure <xref ref-type="fig" rid="Ch1.F7"/> shows that in January–February 2020 all patterns were dominant at least once. It also shows that abrupt day-to-day changes of dominant patterns are rather rare, and a smooth transition from gravel to fish to sugar to flowers is observed.</p>
      <p id="d1e1681">Overall, the different classification methods agree well with each other, and no large discrepancies are found. This confirms that these methods are valid for further analysis of mesoscale patterns. While the <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula> metric is computationally cheap and can be easily applied to different regions, it is less suitable for short time periods because the terciles that attribute the <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">org</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula> pairs to specific quadrants are not robust for a small sample size. Terciles from other studies can only be used if the resolution of the dataset is the same. For short time periods, like those of typical campaigns where people are interested in specific days or even sub-daily variations, manual classifications are advantageous, as they do not require a large sample size. The neural network approach presents a good opportunity to extend the classifications to different time periods and regions by using manual classifications as a training set. Here, the manual classifications served as an additional independent validation dataset and proved once more the capabilities of the neural network which has been trained on the dataset of <xref ref-type="bibr" rid="bib1.bibx6" id="text.39"/>.</p>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Code and data availability</title>
      <p id="d1e1726">The C<inline-formula><mml:math id="M91" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>ONTEXT dataset including raw data is openly available on the Zenodo database (<xref ref-type="bibr" rid="bib1.bibx3" id="altparen.40"/>; <ext-link xlink:href="https://doi.org/10.5281/zenodo.5979718" ext-link-type="DOI">10.5281/zenodo.5979718</ext-link>, <xref ref-type="bibr" rid="bib1.bibx8" id="altparen.41"/>). The source code necessary to generate the dataset is available at <ext-link xlink:href="https://doi.org/10.5281/zenodo.5989155" ext-link-type="DOI">10.5281/zenodo.5989155</ext-link> <xref ref-type="bibr" rid="bib1.bibx9" id="paren.42"/> together with examples on how to process the data and retrieve the classifications for any platform as shown in, e.g., Fig. <xref ref-type="fig" rid="Ch1.F5"/>.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d1e1764">Mesoscale patterns of shallow convection are a main focus of the EUREC<inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A field campaign that took place in January and February 2020. To gain a better process understanding of shallow convection in the trades, the classifications of mesoscale patterns offer the opportunity to study the measurements in their mesoscale context and thereby split the observations into less complex pieces and disentangle otherwise superimposed processes. Here, we present C<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>ONTEXT, a dataset on the common consensus on the mesoscale patterns which occurred during the broader EUREC<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A time period and emerges from the manual classifications done by members of the EUREC<inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A science team.</p>
      <p id="d1e1809"><?xmltex \hack{\newpage}?>C<inline-formula><mml:math id="M96" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>ONTEXT reveals that all mesoscale cloud patterns are observed during the studied period of January and February 2020. However, in the intense observation period of the EUREC<inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="-0.125em"/></mml:mrow></mml:math></inline-formula>A field campaign, 20 January to 20 February, gravel was only sporadically identified and not prevalent in the study area. In contrast, a week before the intense observation period, gravel dominated in the research area. Instruments that were already running at this time, like those at the Barbados Cloud Observatory, were able to gain measurements under the mesoscale influence of gravel and complement the measurements from the IOP.</p>
      <p id="d1e1833">The difficulties of the participants to classify the patterns in the output of a storm-resolving simulation demands further investigation into how well simulations can capture the variability of mesoscale patterns of shallow convection in the trades.</p>
      <p id="d1e1836">A comparison of the manual-classification approach with other methods used in the literature to identify the four mesoscale patterns of shallow convection reveals a generally good agreement and confirms the validity of the different approaches. Nevertheless, the manual classifications are beneficial for limited temporal and spatial studies especially when the classifications are done by a group of several trained scientists. This presents a way to gain a consensus of subjectively defined cloud patterns without an additional layer of complexity from a neural network or any other algorithm.</p>
      <p id="d1e1840">In general, it has been shown that with little effort, classifications of the cloud field are possible and can be a huge benefit for the community, encouraging this approach for future studies.</p><?xmltex \hack{\clearpage}?>
</sec>

      
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<app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>Daily classification overview</title>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F8"><?xmltex \currentcnt{A1}?><?xmltex \def\figurename{Figure}?><label>Figure A1</label><caption><p id="d1e1857"> </p></caption>
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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F9"><?xmltex \currentcnt{A1}?><?xmltex \def\figurename{Figure}?><label>Figure A1</label><caption><p id="d1e1871"> </p></caption>
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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F10"><?xmltex \currentcnt{A1}?><?xmltex \def\figurename{Figure}?><label>Figure A1</label><caption><p id="d1e1886"> </p></caption>
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        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f08-part03.png"/>

      </fig>

<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F11"><?xmltex \currentcnt{A1}?><?xmltex \def\figurename{Figure}?><label>Figure A1</label><caption><p id="d1e1900"> </p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f08-part04.png"/>

      </fig>

<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F12"><?xmltex \currentcnt{A1}?><?xmltex \def\figurename{Figure}?><label>Figure A1</label><caption><p id="d1e1914">Heatmaps of manual classifications based on MODIS (Aqua and Terra) visible imagery. Left to right: visible imagery during an Aqua overpass and user agreement on sugar,  flowers,  fish and  gravel. The circle marks one focus area of the EUREC<inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup><mml:mspace width="-0.125em" linebreak="nobreak"/></mml:mrow></mml:math></inline-formula>A field campaign and the main flight pattern of the participating research aircraft HALO <xref ref-type="bibr" rid="bib1.bibx5" id="paren.43"/>. Coastlines are based on GSHHG shapefiles <xref ref-type="bibr" rid="bib1.bibx16" id="paren.44"/>. Please note that the date format in this figure is year-month-day.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f08-part05.png"/>

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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F13"><?xmltex \currentcnt{A2}?><?xmltex \def\figurename{Figure}?><label>Figure A2</label><caption><p id="d1e1946"> </p></caption>
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        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f09-part01.png"/>

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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F14"><?xmltex \currentcnt{A2}?><?xmltex \def\figurename{Figure}?><label>Figure A2</label><caption><p id="d1e1960"> </p></caption>
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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F15"><?xmltex \currentcnt{A2}?><?xmltex \def\figurename{Figure}?><label>Figure A2</label><caption><p id="d1e1974"> </p></caption>
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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F16"><?xmltex \currentcnt{A2}?><?xmltex \def\figurename{Figure}?><label>Figure A2</label><caption><p id="d1e1989"> </p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f09-part04.png"/>

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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F17"><?xmltex \currentcnt{A2}?><?xmltex \def\figurename{Figure}?><label>Figure A2</label><caption><p id="d1e2003">As Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F8"/> but for the infrared workflow. Images show the cloud field at 16:00 (except 11 February 2020 at 17:00). Please note that the date format in this figure is year-month-day.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f09-part05.png"/>

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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F18"><?xmltex \currentcnt{A3}?><?xmltex \def\figurename{Figure}?><label>Figure A3</label><caption><p id="d1e2019"> </p></caption>
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        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f10-part01.png"/>

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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F19"><?xmltex \currentcnt{A3}?><?xmltex \def\figurename{Figure}?><label>Figure A3</label><caption><p id="d1e2034"> </p></caption>
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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F20"><?xmltex \currentcnt{A3}?><?xmltex \def\figurename{Figure}?><label>Figure A3</label><caption><p id="d1e2048"> </p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f10-part03.png"/>

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<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F21"><?xmltex \currentcnt{A3}?><?xmltex \def\figurename{Figure}?><label>Figure A3</label><caption><p id="d1e2062">As Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F8"/> but for the ICON albedo workflow. Images show the cloud field at midnight. Please note that the date format in this figure is year-month-day.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/14/1233/2022/essd-14-1233-2022-f10-part04.png"/>

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  </app-group><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2079">The contact author has declared that there are no competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e2085">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e2091">This article is part of the special issue “Elucidating the role of clouds–circulation coupling in climate: datasets from the 2020 (EUREC<inline-formula><mml:math id="M99" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula>A) field campaign”. It is not associated with a conference.</p>
  </notes><?xmltex \hack{\newpage}?><?xmltex \hack{\vspace*{16.4cm}}?><ack><title>Acknowledgements</title><p id="d1e2108">The author thanks the participants of the international remote classification event for their time in labeling the cloud patterns. Daniel Klocke is thanked for conducting the ICON storm-resolving simulations. Geet George is thanked for helpful feedback on an earlier version of this paper. Leif Denby, Isabel L. McCoy and one additional anonymous reviewer are thanked for their valuable feedback that helped to improve the paper. We acknowledge the use of imagery from the NASA Worldview application (<uri>https://worldview.earthdata.nasa.gov</uri>, last access: 23 March 2020), part of the NASA Earth Observing System Data and Information System (EOSDIS). GOES-16 Advanced Baseline Imager data are available at <ext-link xlink:href="https://doi.org/10.7289/V5BV7DSR" ext-link-type="DOI">10.7289/V5BV7DSR</ext-link>. Its level 1b radiances were converted with <xref ref-type="bibr" rid="bib1.bibx7" id="text.45"/> to brightness temperatures. This publication uses data generated via the <uri>https://www.zooniverse.org/</uri>  platform, development of which is funded by generous support, including a Global Impact Award from Google and by a grant from the Alfred P. Sloan Foundation.</p></ack><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2126">This paper was edited by Gijs de Boer and reviewed by Leif Denby, Isabel L. McCoy, and one anonymous referee.</p>
  </notes><ref-list>
    <title>References</title>

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