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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0">
  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</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/acp-19-9241-2019</article-id><title-group><article-title>The sensitivity of oceanic precipitation to sea surface temperature</article-title><alt-title>Sensitivity of oceanic precipitation to sea surface temperature</alt-title>
      </title-group><?xmltex \runningtitle{Sensitivity of oceanic precipitation to sea surface temperature}?><?xmltex \runningauthor{J. Burdanowitz et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Burdanowitz</surname><given-names>Jörg</given-names></name>
          <email>joerg.burdanowitz@uni-hamburg.de</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Buehler</surname><given-names>Stefan A.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6389-1160</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Bakan</surname><given-names>Stephan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Klepp</surname><given-names>Christian</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Max Planck Institute for Meteorology Hamburg, Bundesstr. 53, 20146 Hamburg, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Meteorological Institute, Center for Earth System Research and Sustainability, Universität Hamburg, Bundesstr. 55,<?xmltex \hack{\break}?> 20146 Hamburg, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Jörg Burdanowitz (joerg.burdanowitz@uni-hamburg.de)</corresp></author-notes><pub-date><day>19</day><month>July</month><year>2019</year></pub-date>
      
      <volume>19</volume>
      <issue>14</issue>
      <fpage>9241</fpage><lpage>9252</lpage>
      <history>
        <date date-type="received"><day>11</day><month>February</month><year>2019</year></date>
           <date date-type="rev-request"><day>4</day><month>March</month><year>2019</year></date>
           <date date-type="rev-recd"><day>17</day><month>June</month><year>2019</year></date>
           <date date-type="accepted"><day>4</day><month>July</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 </copyright-statement>
        <copyright-year>2019</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e115">Our study forms the oceanic counterpart to numerous observational studies over land concerning the sensitivity of extreme precipitation to a change in air temperature. We explore the sensitivity of oceanic precipitation to changing sea surface temperature (SST) by exploiting two novel datasets at high resolution.
First, we use the Ocean Rainfall And Ice-phase precipitation measurement Network (OceanRAIN) as an observational along-track shipboard dataset at 1 min resolution. Second, we exploit the most recent European Reanalysis version 5 (ERA5) at hourly resolution on a 31 km grid. Matched with each other, ERA5 vertical velocity allows the constraint of the OceanRAIN precipitation.
Despite the inhomogeneous sampling along ship tracks, OceanRAIN agrees with ERA5 on the average latitudinal distribution of precipitation with fairly good seasonal sampling.
However, the 99th percentile of OceanRAIN precipitation follows a super Clausius–Clapeyron scaling with a SST that exceeds 8.5 % K<inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> while ERA5 precipitation scales with 4.5 % K<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>.
The sensitivity decreases towards lower precipitation percentiles, while OceanRAIN keeps an almost constant offset to ERA5 due to higher spatial resolution and temporal sampling. Unlike over land, we find no evidence for a decreasing precipitation event duration with increasing SST.
ERA5 precipitation reaches a local minimum at about 26 <inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C that vanishes when constraining vertical velocity to strongly rising motion and excluding areas of weak correlation between precipitation and vertical velocity. This indicates that instead of moisture limitations as over land, circulation dynamics rather limit precipitation formation over the ocean.
For the strongest rising motion, precipitation scaling converges to a constant value at all precipitation percentiles.
Overall, high resolutions in observations and climate models are key to understanding and predicting the sensitivity of oceanic precipitation extremes to a change in SST.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e160">The equilibrium water vapor pressure increases with temperature, as described by the Clausius–Clapeyron (CC) equation, by about 7 % K<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx14" id="paren.1"><named-content content-type="pre">e.g.,</named-content></xref>. The same CC scaling of a 7 % K<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> atmospheric moisture increase has also been found in modeling studies <xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx1" id="paren.2"/> and observations <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx32 bib1.bibx26" id="paren.3"/>. <xref ref-type="bibr" rid="bib1.bibx41" id="text.4"/> report a global change of 7.3 % K<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for global humidity observations from 1973 to 1999.
As more atmospheric moisture can lead to stronger precipitation events, a similar scaling relation for precipitation is expected; however, the actual rate of change in precipitation with warming is still uncertain, and this is what this study addresses over the ocean.</p>
      <?pagebreak page9242?><p id="d1e214">Despite being studied for some years, the uncertainty in the rate of change for precipitation exceeds that of the atmospheric moisture content because radiative constraints rather than moisture availability limit precipitation. Estimates for the change in global mean precipitation range between 1 and 3 % K<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx3 bib1.bibx1" id="paren.5"/>. Over the global land area, there is medium confidence that precipitation increased during the second half of the 20th century, while high confidence is found for the Northern Hemisphere midlatitudes <xref ref-type="bibr" rid="bib1.bibx16" id="paren.6"/>. At regional scales and for sub-daily precipitation estimates, some studies find changes strongly exceed 10 % K<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx23" id="paren.7"/>. How widespread such cases of super CC scaling occur is under debate <xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx24" id="paren.8"/>.
<xref ref-type="bibr" rid="bib1.bibx13" id="text.9"/> find a positive scaling for sub-hourly precipitation rates over Australia between 20 and 26 <inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, while they find a negative scaling above 26 <inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C due to moisture limitations. <xref ref-type="bibr" rid="bib1.bibx37" id="text.10"/> reveal latitudinal differences of CC scaling as well as marked differences between daily and sub-daily to sub-hourly precipitation rates. Accordingly, resolution plays a crucial role in the scaling of precipitation over land with surface temperature.</p>
      <p id="d1e278">Unlike over land, it remains widely unknown how precipitation scales with sea surface temperature (SST) over the ocean, particularly at sub-daily resolution, though the ocean covers more than 70 % of the Earth's surface and receives 77 % of its precipitation <xref ref-type="bibr" rid="bib1.bibx29" id="paren.11"/>. As a consequence, no long-term records of precipitation exist over the ocean <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx25" id="paren.12"/>. The few existing shorter datasets are often limited by measurement quality, sparse data coverage and low temporal resolution.</p>
      <p id="d1e287">Under the challenging oceanic conditions with high wind speeds of varying direction and sea state, optical disdrometers have been recommended as a reference in situ instrument to measure precipitation <xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx38" id="paren.13"/>. Since 2010, the Ocean Rainfall And Ice-phase precipitation measurement Network <xref ref-type="bibr" rid="bib1.bibx20" id="paren.14"><named-content content-type="pre">OceanRAIN;</named-content></xref> has provided high-quality in situ oceanic precipitation data from optical disdrometers at 1 min resolution. We use this dataset in combination with the most recent European Re-Analysis version 5 (ERA5) of the European Centre for Medium-Range Weather Forecasts (ECMWF) to investigate the sensitivity of oceanic precipitation to changing SSTs.</p>
      <p id="d1e299">In addition to thermodynamic drivers such as SST, dynamic drivers as part of the general atmospheric circulation strongly control if and how much precipitation is formed in the atmospheric column. <xref ref-type="bibr" rid="bib1.bibx10" id="text.15"/> find an overall increase in mean and extreme precipitation, mainly due to thermodynamic changes while dynamics tend to diminish precipitation, particularly in the subtropics. Changes in extreme precipitation are particularly important as they account for most of the accumulation. To shed light on observed changes in extreme precipitation with SST we constrain extreme precipitation from OceanRAIN by the circulation regime using vertical velocities from ERA5.</p>
      <p id="d1e305">The paper starts by introducing the datasets and the methods used. First, we investigate the OceanRAIN sampling and how precipitation intensities change with latitude. Second, we consider the change of different precipitation percentiles with respect to a change in SST. Third, we investigate the distribution of vertical velocity in ERA5 and use it to exclude regions of low correlation between precipitation and vertical velocity. We also compare OceanRAIN with ERA5 for the same vertical-velocity regime (lifting air mass). Fourth, we consider how the precipitation event duration changes with SST. The last chapter summarizes our findings and presents some concluding thoughts and next steps.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Data</title>
<sec id="Ch1.S2.SS1.SSSx1" specific-use="unnumbered">
  <title>OceanRAIN</title>
      <p id="d1e328">The Ocean Rainfall And Ice-phase precipitation measurement Network <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx4 bib1.bibx20" id="paren.16"><named-content content-type="pre">OceanRAIN;</named-content></xref> provides water-cycle-related and energy-cycle-related parameters from June 2010 to April 2017 over the global ocean, collected onboard eight research vessels (RVs). In OceanRAIN version 1.0 <xref ref-type="bibr" rid="bib1.bibx19" id="paren.17"><named-content content-type="pre">OceanRAIN-W;</named-content></xref>, the RVs include the German RVs <italic>Polarstern</italic> (since June 2010), <italic>Meteor</italic> (since March 2014), <italic>Maria S. Merian</italic> (October 2012 to June 2014) and <italic>Sonne</italic> (September to October 2012) as well as its successor <italic>Sonne II</italic> (since November 2014). The Australian RV <italic>Investigator</italic> (January to February 2016) and the American RV <italic>Roger Revelle</italic> (August to September 2016) contributed temporarily to OceanRAIN. <xref ref-type="bibr" rid="bib1.bibx20" id="text.18"/> describe the post-processing and quality-checking of the OceanRAIN data in detail.
OceanRAIN is publicly available free of charge: more information can be accessed at <uri>https://oceanrain.cen.uni-hamburg.de/index.php?id=2752</uri> (last access: 17 July 2019).</p>
      <p id="d1e369">Precipitation as rain, snow or mixed-phase precipitation is derived from particle size distributions recorded by the optical disdrometer ODM470, manufactured by the German company Eigenbrodt GmbH &amp; Co. KG. In the ODM470, a photodiode receiver detects the signal reduction of a near-infrared diode within the cross-sectional area of the optical measuring volume caused by falling hydrometeors <xref ref-type="bibr" rid="bib1.bibx21" id="paren.19"/>. The ODM470 was specifically designed to measure precipitation over the ocean: its cylindrically shaped measuring volume and its wind vane attached on a pivotable axis ensure high-quality precipitation measurements even under rough oceanic conditions with strong and highly varying wind speed and sea state. In addition, the typical mounting height of <inline-formula><mml:math id="M11" display="inline"><mml:mn mathvariant="normal">30</mml:mn></mml:math></inline-formula> to <inline-formula><mml:math id="M12" display="inline"><mml:mn mathvariant="normal">45</mml:mn></mml:math></inline-formula> m reduces unwanted influences by wave water and sea spray.</p>
      <p id="d1e389">The SST in OceanRAIN has been interpolated from the bulk water temperature that is measured in sea water inlets of the respective RV at a 2 to 7 m depth. The interpolation uses the cool skin parametrization from <xref ref-type="bibr" rid="bib1.bibx8" id="text.20"/>. The warm-layer effect is currently neglected. However, according to the OceanRAIN warm-layer flag <xref ref-type="bibr" rid="bib1.bibx20" id="paren.21"/>, less than 9 % of all cases with precipitation could be affected by a warm layer.</p>
</sec>
<sec id="Ch1.S2.SS1.SSSx2" specific-use="unnumbered">
  <title>ERA5</title>
      <p id="d1e404">The European Centre for Medium-Range Weather Forecasts (ECMWF) Reanalysis version 5 (ERA5) has been developed through the Copernicus Climate Change Service (C3S; <xref ref-type="bibr" rid="bib1.bibx7" id="altparen.22"/>). The ERA5 data assimilation system uses the current<?pagebreak page9243?> Integrated Forecasting System (IFS) version 41r2. Released in July 2017, the data contained hourly analyses and forecast fields at a spatial resolution of globally 31 km for the period of 2010 to 2016, which has been extended backward to 1979 and forward to three months from now <xref ref-type="bibr" rid="bib1.bibx15" id="paren.23"/>. We use the following parameters from ERA5: vertical velocity (<inline-formula><mml:math id="M13" display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula>) at the 500 hPa pressure level, sea surface temperature (sst) and total precipitation (tp) at the surface level. The data have been downloaded via the ECMWF Web API from the ECMWF data archive (MARS).</p>
</sec>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Methods</title>
      <p id="d1e429">A standard way to calculate the sensitivity of precipitation to a change in SST is to divide the precipitation rate (<inline-formula><mml:math id="M14" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>) into SST bins <xref ref-type="bibr" rid="bib1.bibx22" id="paren.24"><named-content content-type="pre">e.g., </named-content></xref>. For each of the 1 <inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C bins, percentiles of precipitation rate can be calculated. We consider the 25th, 50th, 75th, 90th and 99th percentiles to mainly reflect the sensitivity of high precipitation rates for which the 99th percentile represents heavy precipitation (see Table <xref ref-type="table" rid="Ch1.T1"/> for all names). Second, for each of the percentiles, we calculate the slope using two linear regression methods in order to derive the precipitation scaling (<inline-formula><mml:math id="M16" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e465">Quantitative (mm h<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and qualitative intensities for each of the five percentiles of OceanRAIN precipitation rate for <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.396</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.473</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> precipitating) minutes from June 2010 to April 2017.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Percentile</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M20" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> (mm h<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col3">Intensity</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">25th, <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mn mathvariant="normal">25</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M23" display="inline"><mml:mn mathvariant="normal">0.05</mml:mn></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">weak</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">50th, <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mn mathvariant="normal">50</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M25" display="inline"><mml:mn mathvariant="normal">0.18</mml:mn></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">light</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">75th, <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mn mathvariant="normal">75</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M27" display="inline"><mml:mn mathvariant="normal">0.80</mml:mn></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">medium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">90th, <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mn mathvariant="normal">90</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M29" display="inline"><mml:mn mathvariant="normal">2.64</mml:mn></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">strong</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">99th, <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mn mathvariant="normal">99</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M31" display="inline"><mml:mn mathvariant="normal">14.74</mml:mn></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">heavy</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e692">Since the widely used linear regression method of ordinary least squares (OLS) has some major weaknesses when it comes to outliers and skewed distributions, we also use the Theil–Sen estimator (TSE) <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx31" id="paren.25"/> as a more robust method. TSE is much less susceptible to outliers <xref ref-type="bibr" rid="bib1.bibx40" id="paren.26"/>, which is particularly needed for the much smaller sample of OceanRAIN data compared to ERA5. In addition, we simulate the robustness of the fit by bootstrapping. By these means, we get a more complete picture of how susceptible precipitation is to a change in SST.</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Is the OceanRAIN sampling sufficient to study the precipitation scaling with SST?</title>
      <p id="d1e718">Oceanic precipitation is driven by the global atmospheric circulation systems. The atmospheric circulation follows seasonal insolation changes. Sufficient seasonal sampling of precipitation is therefore needed from all climate zones for our attempt to investigate the precipitation sensitivity to SST changes. The global-ocean operation of RVs used in OceanRAIN (<inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.396</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> min in total; <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.473</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> min with precipitation) suggests sufficient spatial sampling is possible. Most oceanic regions are well sampled during all seasons (dark-blue boxes in Fig. <xref ref-type="fig" rid="Ch1.F1"/>a).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e755"><bold>(a)</bold> Two-dimensional histogram of OceanRAIN (June 2010 to April 2017) precipitating minutes, <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, per month as a function of latitude. Zero values (yellow boxes) indicate no precipitation sampling. White boxes indicate no sampling at all. <bold>(b)</bold> Five percentiles of OceanRAIN precipitation (mm h<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) as a function of 1<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude bands with relative occurrence (%) shown in color. <bold>(c)</bold> As with <bold>(b)</bold> but for ERA5 (June 2010 to December 2016).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/9241/2019/acp-19-9241-2019-f01.png"/>

        </fig>

      <p id="d1e815">Some measurement gaps exist during winter of the respective high-latitude regions towards both poles due to drifting ice and rough weather conditions. The Southern Ocean around 30<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S is sparsely sampled during late boreal summer as are the northern midlatitude regions from 50 to 70<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N during late boreal winter (light-blue boxes). In some subtropical regions, no precipitation was observed during times of OceanRAIN sampling (yellow boxes). Nevertheless, we find no pronounced gaps of seasonal sampling that would introduce seasonal biases with respect to latitude in OceanRAIN.</p>
      <p id="d1e837">Without obvious seasonal biases, we expect OceanRAIN to reflect the mean latitudinal precipitation distribution according to the atmospheric circulation patterns. In particular for strong-to-heavy precipitation (see Table <xref ref-type="table" rid="Ch1.T1"/> for classification), the highest precipitation rates occur at or close to the Equator while for weak-to-medium precipitation the highest precipitation rates also occur around 30<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S (Fig. <xref ref-type="fig" rid="Ch1.F1"/>b). Minimum precipitation rates at all intensities are found at both poles and in the subtropics at about 30<inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and 15<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, respectively. The exact positions of latitudinal precipitation minima and maxima vary with intensity and are likely related to sparse sampling, e.g., in the dry subtropics (purple colors in Fig. <xref ref-type="fig" rid="Ch1.F1"/>b). Nevertheless, the OceanRAIN time period of June 2010 to April 2017 reflects the expected mean precipitation distribution with respect to latitude.</p>
      <p id="d1e874">Comparing the latitudinal distribution of precipitation rates from OceanRAIN to that of ERA5 reveals an overall good agreement on the main climatological patterns and also some major differences (Fig. <xref ref-type="fig" rid="Ch1.F1"/>c). One of them – the much lower amplitude of precipitation rates from ERA5 – can be explained by the lower spatial and temporal resolution of ERA5 compared to OceanRAIN. The reduced variability for heavy precipitation in ERA5 compared to medium intensities marks a second distinction between OceanRAIN and ERA5. This is likely related to recurrence times of extreme precipitation events that exceed the typical OceanRAIN sampling of about 1000 min of precipitation per box mainly in the subtropics (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a). Building on these results, a further exploration of both datasets seems plausible to investigate the sensitivity of precipitation to SST changes.</p>
</sec>
<?pagebreak page9244?><sec id="Ch1.S3.SS2">
  <label>3.2</label><title>How does precipitation change with SST?</title>
      <p id="d1e889">Despite a pronounced variability, precipitation shows a clear trend of increasing SST at all five <inline-formula><mml:math id="M42" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> percentiles over the global ocean in OceanRAIN (Fig. <xref ref-type="fig" rid="Ch1.F2"/>a). The sensitivity of precipitation to SST increases for higher precipitation intensities. While weak precipitation increases by 4.5 % K<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and light-to-medium precipitation increases by more than 6 % K<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, heavy precipitation increases by almost 9 % K<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> according to TSE (Sect. <xref ref-type="sec" rid="Ch1.S2"/>). Here, the less robust OLS method leads to significantly lower sensitivities of 2.5 (weak) to 6 % K<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (heavy), considering the median of data of a randomly chosen 50 % of the binned intensities which were resampled 100 times.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e954">Five percentiles of <bold>(a)</bold> OceanRAIN (June 2010–April 2017) and <bold>(b)</bold> ERA5 (June 2010–December 2016) precipitation rate <inline-formula><mml:math id="M47" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> (mm h<inline-formula><mml:math id="M48" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) as a function of bin-wise SST (<inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) shown with linear regressions from TSE calculation.  Gray lines indicate 7 % K<inline-formula><mml:math id="M50" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> slope. <bold>(c, d)</bold> Histograms illustrate number of cases <inline-formula><mml:math id="M51" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> (per bin) for all in <bold>(a)</bold> and per month in <bold>(b)</bold>. <bold>(e, f)</bold> Slopes from TSE regressions (% K<inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) in <bold>(a)</bold> and <bold>(b)</bold> are indicated by markers as a function of percentile. Boxes (5th–95th percentile) refer to the OLS method as a comparison, which uses the halved dataset resampled 100 times.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/9241/2019/acp-19-9241-2019-f02.png"/>

        </fig>

      <p id="d1e1048">The interquartile spread of 1 to 2 % K<inline-formula><mml:math id="M53" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (50 % of the sensitivity) and data samples of much less than 10 000 min for some of the bins (Fig. <xref ref-type="fig" rid="Ch1.F2"/>c) indicate a high variability, which is why we put more trust in the sensitivities calculated by the more robust TSE.</p>
      <?pagebreak page9245?><p id="d1e1066">Precipitation in ERA5 reveals a local minimum at about 26 <inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, which we will discuss later. Altogether, ERA5 shows a much lower <inline-formula><mml:math id="M55" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling compared to OceanRAIN with values of about 0.3 to 3.1 % K<inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for weak-to-strong and of 4.5 % K<inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for heavy precipitation with TSE (Fig. <xref ref-type="fig" rid="Ch1.F2"/>b, f). As these numbers rely on global ocean coverage, even the average monthly data sampling density of <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> per bin (Fig. <xref ref-type="fig" rid="Ch1.F2"/>d) strongly exceeds that of OceanRAIN, resulting in a smoother trend of the <inline-formula><mml:math id="M59" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling and a lower interquartile spread of 0.4 to 0.8 % K<inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. As a consequence, the TSE always lies within the uncertainty of the OLS method (5th–95th percentile). Nevertheless, the question arises as to whether only resolution differences cause the systematically lower <inline-formula><mml:math id="M61" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling in ERA5 compared to OceanRAIN.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Can vertical velocity help to understand the precipitation scaling with SST?</title>
      <p id="d1e1159">To enhance our understanding of different <inline-formula><mml:math id="M62" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scalings over the ocean, we consider vertical velocity at 500 hPa from ERA5 to select cases that favor precipitation formation. As an indicator, we use the temporal correlation <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> at each grid point between hourly precipitation (<inline-formula><mml:math id="M64" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>) and hourly 500 hPa vertical velocity (<inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) from ERA5. As in <xref ref-type="bibr" rid="bib1.bibx10" id="text.27"/>, we use <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> as a threshold (note that we define positive vertical velocity as subsiding motion). The resulting areas of weak or even positive <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> for a month (bluish colors in Fig. <xref ref-type="fig" rid="Ch1.F3"/>a) mainly comprise, but are not limited
to, areas of subsidence and relatively low SSTs and amount to 5 % of the global ocean precipitation (see Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F8"/> for influence on ERA5). Unlike earlier studies, note that we use hourly instead of daily (e.g., <xref ref-type="bibr" rid="bib1.bibx10" id="altparen.28"/>) or monthly time steps (e.g., <xref ref-type="bibr" rid="bib1.bibx27" id="altparen.29"/>) for correlation, but correlations are calculated per month. The high seasonal variability of <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> leaves only small areas with a constantly weak <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> over a whole year (e.g., minimum for each month of 2010 in Fig. <xref ref-type="fig" rid="Ch1.F3"/>b). While the size of the areas varies slightly, the southeast Pacific and southeast Atlantic areas of constantly weak correlation stay the same for the years 2010–2016 while elsewhere <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> remains mostly below <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> (not shown).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e1348">Maps of temporal correlation <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> for each ERA5 grid box for <bold>(a)</bold> July 2010 and <bold>(b)</bold> the minimum monthly correlation for the year 2010. Blue colored areas are weakly or positively correlated and are excluded from further analysis (<inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>&gt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula>; <xref ref-type="bibr" rid="bib1.bibx10" id="altparen.30"/>).</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/9241/2019/acp-19-9241-2019-f03.jpg"/>

        </fig>

      <p id="d1e1401">In order to use <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to constrain OceanRAIN precipitation, we match each minute of OceanRAIN precipitation with the closest hourly <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> of ERA5. Negative <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> values correspond to rising motion. Almost two-thirds of the global-ocean ERA5 time steps during July 2010, as an example, have absolute vertical velocities <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mo>|</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>|</mml:mo></mml:mrow></mml:math></inline-formula> below 100 hPa d<inline-formula><mml:math id="M78" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F4"/>a).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e1470">Histograms of relative frequencies for <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (blue: rising motion; red: subsiding motion) of <bold>(a, b)</bold> all ERA5 grid boxes and <bold>(c, d)</bold> for OceanRAIN–ERA5 co-located ERA5 grid boxes with <bold>(a, c)</bold> linear ordinates and <bold>(b, d)</bold> logarithmic ordinates for strong motion.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/9241/2019/acp-19-9241-2019-f04.png"/>

        </fig>

      <p id="d1e1502">The slightly left-skewed distribution of <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <?xmltex \hack{\mbox\bgroup}?>(<inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mi mathvariant="italic">γ</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.44</mml:mn></mml:mrow></mml:math></inline-formula>)<?xmltex \hack{\egroup}?> has a 1st percentile of <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">692</mml:mn></mml:mrow></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, a 99th percentile of <inline-formula><mml:math id="M84" display="inline"><mml:mn mathvariant="normal">410</mml:mn></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, a mean of <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.1</mml:mn></mml:mrow></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M87" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and a median of <inline-formula><mml:math id="M88" display="inline"><mml:mn mathvariant="normal">15.5</mml:mn></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M89" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F4"/>b). When being matched to OceanRAIN, the <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> distribution of ERA5 loses its extremes (1st percentile, <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">602</mml:mn></mml:mrow></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M92" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>; 99th percentile, <inline-formula><mml:math id="M93" display="inline"><mml:mn mathvariant="normal">385</mml:mn></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M94" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>; Fig. <xref ref-type="fig" rid="Ch1.F4"/>c and d with log <inline-formula><mml:math id="M95" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis) while the left-skewness slightly reduces (<inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mi mathvariant="italic">γ</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.03</mml:mn></mml:mrow></mml:math></inline-formula>). Nevertheless, the <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> distribution of OceanRAIN–ERA5-matched time steps is very similar to the overall ERA5 distribution of July 2010 (Fig. <xref ref-type="fig" rid="Ch1.F4"/>a and c).</p>
      <?pagebreak page9246?><p id="d1e1709">The OceanRAIN–ERA5-matched time steps enable a direct comparison between both datasets for the <inline-formula><mml:math id="M98" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling. We define a range of <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1500</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M100" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> that, first, selects upward motion that generally fosters precipitation to form and that, second, provides sufficient matches per SST bin to allow the highest percentiles to be calculated (Fig. <xref ref-type="fig" rid="Ch1.F5"/>c, d).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e1758">As Fig. <xref ref-type="fig" rid="Ch1.F2"/> but for all OceanRAIN–ERA5-matched time steps for OceanRAIN  <bold>(a, c, e)</bold> and for ERA5 <bold>(b, d, f)</bold>, both for rising motion (<inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1500</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M102" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and excluding regions of <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>&gt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> from Fig. <xref ref-type="fig" rid="Ch1.F3"/>. Orange lines in <bold>(c)</bold> and <bold>(d)</bold> mark the lowest <inline-formula><mml:math id="M104" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> for which <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mn mathvariant="normal">99</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> can be calculated.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/9241/2019/acp-19-9241-2019-f05.png"/>

        </fig>

      <p id="d1e1864">This range represents a good compromise between a clear signal of rising motion and a sufficiently large size of remaining OceanRAIN samples. Third, we exclude grid boxes with a temporal correlation of <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>&gt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> per month that are mainly associated with dry areas of subsidence (see Fig. <xref ref-type="fig" rid="Ch1.F3"/>). The influence of these weakly correlated areas on the whole ERA5 dataset is shown in Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/> (see Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F8"/>). Also note that we use OceanRAIN SSTs for both datasets as the usage of ERA5 SSTs would reduce the total number of usable time steps (437 000 without <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> constraint) by 6.6 % (not shown). The resulting subsample of matched time steps for ERA5 (hourly) and OceanRAIN (every minute) comprises about 110 000 time steps. The relatively low number of remaining time steps limits the statistical robustness of the sample for some of the 1 <inline-formula><mml:math id="M108" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C SST bins that contain fewer than 1000 precipitation values (Fig. <xref ref-type="fig" rid="Ch1.F5"/>c, d). The data sparsity results in a quite scattered sensitivity distribution (Fig. <xref ref-type="fig" rid="Ch1.F5"/>a, b). First, compared to the larger sample of OceanRAIN measurements and ERA5 data (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>), particularly the weak-to-medium precipitation rates increase at a much higher rate with constrained <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Second, all OceanRAIN precipitation percentiles scale with 7.5 to 10 % K<inline-formula><mml:math id="M110" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (ERA5: 3 to 5.5 % K<inline-formula><mml:math id="M111" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) according to TSE (Fig. <xref ref-type="fig" rid="Ch1.F5"/>e, f). This means an approximate constant sensitivity of precipitation to a change in SST, for OceanRAIN even at super CC scaling, while the sensitivity difference remains between ERA5 and OceanRAIN.</p>
      <p id="d1e1966">To understand whether this uniform sensitivity at all precipitation percentiles results from the <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> constraint, from the data sparsity or is a feature of the matched subsample of data, we consider ERA5 with the same constraint of <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1500</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M114" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> but globally for the full ERA5 period, which leads to more than 1000 times more data (monthly <inline-formula><mml:math id="M115" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> in Fig. <xref ref-type="fig" rid="Ch1.F6"/>c).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e2026">As with Fig. <xref ref-type="fig" rid="Ch1.F5"/> but for the complete ERA5 period. Panels <bold>(a)</bold>, <bold>(c)</bold> and <bold>(e)</bold> are constrained by <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1500</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M117" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and panels <bold>(b)</bold>, <bold>(d)</bold> and <bold>(f)</bold> by <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5000</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1500</mml:mn></mml:mrow></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M119" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/9241/2019/acp-19-9241-2019-f06.png"/>

        </fig>

      <p id="d1e2126">Compared to OceanRAIN, the <inline-formula><mml:math id="M120" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling smoothens for all precipitation percentiles (Fig. <xref ref-type="fig" rid="Ch1.F6"/>a) while the interquartile spread reduces (Fig. <xref ref-type="fig" rid="Ch1.F6"/>e). Compared to Fig. <xref ref-type="fig" rid="Ch1.F5"/>f, mainly the <inline-formula><mml:math id="M121" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling of weak precipitation decreases below 2 % K<inline-formula><mml:math id="M122" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, and for medium-to-heavy precipitation it remains between 3 and 5 % K<inline-formula><mml:math id="M123" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. Compared to Fig. <xref ref-type="fig" rid="Ch1.F2"/>e, the <inline-formula><mml:math id="M124" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling increases more steeply for weak precipitation and reaches a plateau for medium-to-strong intensities before it increases again for heavy precipitation. Accordingly, the sensitivity in Fig. <xref ref-type="fig" rid="Ch1.F5"/>f points at the slightly increased sensitivities for low precipitation rates for the <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> constraint while the picture is mainly blurred due to the small sample size.</p>
      <p id="d1e2196">Constraining <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to rising motion strongly reduces the local minimum at about 26 <inline-formula><mml:math id="M127" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in Fig. <xref ref-type="fig" rid="Ch1.F2"/>b (see Fig. <xref ref-type="fig" rid="Ch1.F6"/>a). From this and areas of weak or positive correlation between SST and precipitation (Figs. <xref ref-type="fig" rid="Ch1.F3"/> and <xref ref-type="fig" rid="App1.Ch1.S1.F8"/>), we suppose that atmospheric conditions of weak <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> contribute to the local minimum at 26 <inline-formula><mml:math id="M129" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in ERA5. It might therefore seem natural that suppressed dynamical drivers of precipitation, predominantly in the subtropics, could generate this local minimum<?pagebreak page9247?> in precipitation intensity. Proving this assumption, however, goes beyond the scope of this work.</p>
      <p id="d1e2248">To further investigate the influence of a constraining <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, we consider stronger rising motion between <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5000</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1500</mml:mn></mml:mrow></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M133" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F6"/>b). Compared to somewhat weaker rising motion in <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, the weak precipitation rates increase by about 1 order of magnitude, while heavy precipitation rates are higher by a factor of 2. The change in the <inline-formula><mml:math id="M135" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling with SST smoothens while it tends towards a constant slope at all percentiles (Fig. <xref ref-type="fig" rid="Ch1.F6"/>f). This constant slope marks a linear increase and saturates for strongest rising motions at approximately 6 % K<inline-formula><mml:math id="M136" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in ERA5 (not shown). Accordingly, the shift of the range of <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> toward lower values (rising motion) tends to equalize the <inline-formula><mml:math id="M138" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling at different <inline-formula><mml:math id="M139" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> percentiles. This mainly results from an increase in <inline-formula><mml:math id="M140" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling at lower percentiles, while the <inline-formula><mml:math id="M141" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling remains approximately constant for high percentiles.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Does a change in precipitation event duration with SST affect the precipitation scaling?</title>
      <p id="d1e2377">Over land, previous studies state a decrease in precipitation event duration with increasing air temperature that explains the drop-off in precipitation scaling at high temperatures found for hourly to daily sampling rates (<xref ref-type="bibr" rid="bib1.bibx12" id="altparen.31"/>; <xref ref-type="bibr" rid="bib1.bibx37" id="altparen.32"/>). <xref ref-type="bibr" rid="bib1.bibx11" id="text.33"/> explain the decreasing event duration with a shift toward more convective precipitation events at high temperatures. To check whether this holds over the ocean, we calculated the OceanRAIN precipitation event duration by counting uninterrupted periods of continuous precipitation at 1 min sampling. The average precipitation event lasts between 6 and 11 min with an uncertainty of 1 to 2 min obtained from bootstrapping (Fig. <xref ref-type="fig" rid="Ch1.F7"/>a).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e2393">Two-dimensional histograms as a function of precipitation event duration <inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi mathvariant="normal">E</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (min) and OceanRAIN SST (<inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) for <bold>(a)</bold> linear and <bold>(b)</bold> logarithmic ordinate. Colors indicate relative occurrence (%) per SST bin. Markers in <bold>(a)</bold> show mean per SST bin surrounded by minimum and maximum from resampling 100 times as a measure of uncertainty. Markers in <bold>(b)</bold> show percentiles 50, 75, 90, 99 and 99.9 of <inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi mathvariant="normal">E</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Panel <bold>(c)</bold> shows the number <inline-formula><mml:math id="M145" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> of events per SST bin.</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/9241/2019/acp-19-9241-2019-f07.png"/>

        </fig>

      <p id="d1e2456">The shortest mean precipitation event duration occurs at 15 <inline-formula><mml:math id="M146" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, while the longest mean precipitation event duration occurs around 2 <inline-formula><mml:math id="M147" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and above 28 <inline-formula><mml:math id="M148" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. The mean is mainly driven by the highest percentiles (99th to 99.9th exceeding 2 h) that mainly cause the minimum at 15 <inline-formula><mml:math id="M149" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, but it is less pronounced for the 50th to 75th percentile where precipitation event duration remains constant (Fig. <xref ref-type="fig" rid="Ch1.F7"/>b). Although the precipitation event duration tends to decrease between 2 and 16 <inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C as over land (<xref ref-type="bibr" rid="bib1.bibx12" id="altparen.34"/>; <xref ref-type="bibr" rid="bib1.bibx37" id="altparen.35"/>), we find no systematic decrease over the whole SST range.</p>
      <p id="d1e2514">The precipitation event duration as a function of temperature can be influenced by several factors. First, the heterogeneous sampling in OceanRAIN can influence the event duration. Exceeding 2000 samples per bin, the sampling density per SST bin seems fairly good for most of the SST range; below 12 <inline-formula><mml:math id="M151" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C it even exceeds 4000 samples per bin (Fig. <xref ref-type="fig" rid="Ch1.F7"/>c). Nevertheless, heterogeneous spatial sampling by the ships can lead to a biased picture (see Fig. 3 in <xref ref-type="bibr" rid="bib1.bibx5" id="altparen.36"/>); e.g., the eastern Atlantic has been more densely sampled compared to the western Atlantic, which might have an effect on the occurrence of very long-lasting precipitation events. Second, the ship movement relative to cloud movement can affect the retrieved event duration. However, this effect cancels out over almost 40 000 events sampled from OceanRAIN (not shown). Overall, influences by the heterogeneity of OceanRAIN on the precipitation event duration cannot be ruled out but seem rather limited according to our investigations.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Summary and concluding remarks</title>
      <p id="d1e2540">This study forms the oceanic counterpart to numerous observational studies over land concerning the sensitivity of extreme precipitation to a change in air temperature. Unlike earlier studies with mainly hourly to daily sampling calling for higher resolution (e.g., <xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx9" id="altparen.37"/>), we consider precipitation rate and SST at a very high sampling rate of 1 min from OceanRAIN optical disdrometer measurements aboard global-ocean research vessels. In addition, hourly measurements of the new ERA5<?pagebreak page9248?> reanalysis serve to compare and, additionally, constrain precipitation by large-scale vertical velocity.</p>
      <p id="d1e2546">OceanRAIN challenges the user with its non-uniform sampling and variable spatial resolution along ship tracks. However, at the same time, it offers a unique opportunity to study oceanic precipitation at high quality with global-ocean sampling at 1 min temporal resolution. Additionally, we show that differences in seasonal and latitudinal sampling are small, which could otherwise affect the precipitation scaling <xref ref-type="bibr" rid="bib1.bibx30" id="paren.38"/>. Furthermore, the OceanRAIN average precipitation distribution with latitude looks similar to that in ERA5 with its homogeneous global-ocean coverage.</p>
      <p id="d1e2552">For OceanRAIN, the 99th percentile of 1 min precipitation rates shows a super CC scaling of almost 9 % K<inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in line with studies over land (e.g., <xref ref-type="bibr" rid="bib1.bibx6 bib1.bibx30" id="altparen.39"/>), while for ERA5 the 99th percentile of the hourly ERA5 precipitation rates increases by only 4.5 % K<inline-formula><mml:math id="M153" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (linear regression using Theil–Sen estimator). The tendency of a stronger scaling with higher temporal sampling confirms findings by <xref ref-type="bibr" rid="bib1.bibx37" id="text.40"/> and <xref ref-type="bibr" rid="bib1.bibx9" id="text.41"/>. This difference in CC scaling ranges between 4 and 6 % K<inline-formula><mml:math id="M154" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for the weak-to-strong precipitation rates between OceanRAIN and ERA5. For both datasets, precipitation increases with SST at all the percentiles considered. In contrast to studies over land, we find no “hook shape” <xref ref-type="bibr" rid="bib1.bibx9" id="paren.42"/> or clear drop-off <xref ref-type="bibr" rid="bib1.bibx13" id="paren.43"/> of precipitation over the ocean towards high SSTs. <xref ref-type="bibr" rid="bib1.bibx9" id="text.44"/> explain the “hook shape” by the lifted level of condensation under higher surface temperatures in a dry environment. Instead, despite the variability in OceanRAIN, we find a continuous increase in OceanRAIN precipitation with increasing SST, including the highest SSTs.</p>
      <p id="d1e2610">Nevertheless, the ERA5 precipitation rates reveal a local minimum at about 26 <inline-formula><mml:math id="M155" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. When excluding areas of weak temporal correlation of 500 hPa vertical velocity with precipitation rate, the local minimum in precipitation scaling becomes weaker. Despite the fact that the hourly vertical velocity might not necessarily be the best indicator of large-scale subsidence, the minimum vanishes when constraining precipitation to rising motion below <inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1500</mml:mn></mml:mrow></mml:math></inline-formula> hPa d<inline-formula><mml:math id="M157" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. From this, we infer that dynamical drivers such as subtropical large-scale subsidence inhibit precipitation formation and cause the local precipitation minimum at 26 <inline-formula><mml:math id="M158" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. However, it remains open whether this minimum reveals a deficiency in ERA5 – e.g., by suppressing precipitation formation too strongly in the subtropics – or whether this minimum has not yet become visible in OceanRAIN due to limited sampling.</p>
      <p id="d1e2654">The data sampling density plays a crucial role in precipitation-sparse regions that would need the longest sampling to be well represented. Generally, the non-uniform sampling by ships in OceanRAIN results in a more variable precipitation distribution with respect to SST. Therefore, we mainly rely on the Theil–Sen estimator (TSE) as linear regression method, which is less susceptible to outliers <xref ref-type="bibr" rid="bib1.bibx40" id="paren.45"/>, instead of only trusting the widely known ordinary least squares (OLS) method.</p>
      <p id="d1e2660">Although we find a more steady precipitation scaling in OceanRAIN compared to ERA5 at high SSTs, there is no evidence that this is caused by a decreasing duration of precipitation events with temperature as indicated by studies over land (<xref ref-type="bibr" rid="bib1.bibx12" id="altparen.46"/>; <xref ref-type="bibr" rid="bib1.bibx37" id="altparen.47"/>). Instead, we find a minimum average precipitation event duration in OceanRAIN of 7 min at about 15 <inline-formula><mml:math id="M159" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C that rises beyond 10 min above 28 <inline-formula><mml:math id="M160" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. This temperature dependence remains the same for higher percentiles corresponding to longer events. As most of the precipitation events last only a few minutes, this confirms our decision to use a high-temporal-sampling rate of 1 min to exclude resolution artifacts from the precipitation scaling. At 1 min resolution, we find no evidence of generally decreasing precipitation event duration with temperature.</p>
      <p id="d1e2687">For the OceanRAIN–ERA5-matched time steps, we find a high uncertainty for the reduced data sample using vertical velocity in 500 hPa from ERA5 to constrain precipitation rates. The OceanRAIN precipitation scales with super CC behavior at all precipitation percentiles (8 to 10 % K<inline-formula><mml:math id="M161" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) while ERA5 precipitation scales with 3 to 6 % K<inline-formula><mml:math id="M162" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, confirming the offset that we found between both unconstrained datasets. The offset in precipitation scaling is therefore likely attributable to the marked difference in spatial resolution that confronts the OceanRAIN along-track data with the areal ERA5 data of 31 km grid boxes. Furthermore, constraining precipitation towards strongly rising air masses leads to a precipitation scaling that converges towards 6 % K<inline-formula><mml:math id="M163" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for all precipitation rates in ERA5. For OceanRAIN, the too small data sample for precipitation in lifting air masses does not allow us to derive a number for the scaling, but the offset to ERA5 and the scaling with the OceanRAIN–ERA5-matched data both suggest super CC scaling for OceanRAIN.</p>
      <p id="d1e2726">Two aspects should be kept in mind when interpreting our results. First, the average precipitation scaling should not be directly translated into an increase in local precipitation per degree of warming, as locally dynamic processes can strongly alter the precipitation–SST relationship. Second, in light of the projected rising global mean temperature by anthropogenic climate change, large-scale circulation changes and other side effects in the Earth system could contribute or counteract the diagnosed precipitation sensitivity to a change in SST. Therefore, care needs to be taken when interpreting our results that are valid under the present climatic conditions.</p>
      <p id="d1e2729">The next steps would include more local analyses at 1 min resolutions once data sampling allows the highest precipitation intensities to be resolved globally. Furthermore, higher resolutions are needed in global climate models to project the hydrological sensitivity of extremes in a warming climate and its feedbacks.</p>
</sec>

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

      <?pagebreak page9249?><p id="d1e2737">The OceanRAIN data are available through the Climate and Environmental Retrieval and Archive (CERA) of World Data Center for Climate (WDCC) via (<ext-link xlink:href="https://doi.org/10.1594/wdcc/oceanrain-w" ext-link-type="DOI">10.1594/wdcc/oceanrain-w</ext-link>; <xref ref-type="bibr" rid="bib1.bibx19" id="altparen.48"/>). The ERA5 data are available through the Climate Data Store (CDS) Application Program Interface (API) via the Copernicus Climate Change Service (<ext-link xlink:href="https://cds.climate.copernicus.eu/cdsapp#/home">https://cds.climate.copernicus.eu/cdsapp#/home</ext-link>; <xref ref-type="bibr" rid="bib1.bibx7" id="altparen.49"/>).</p>
  </notes><?xmltex \hack{\clearpage}?><app-group>

<?pagebreak page9250?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>How circulation dynamics impact the precipitation scaling in ERA5</title>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F8"><?xmltex \currentcnt{A1}?><label>Figure A1</label><caption><p id="d1e2765">Panels <bold>(a)</bold>, <bold>(c)</bold> and <bold>(e)</bold> are the same as right panel of Fig. <xref ref-type="fig" rid="Ch1.F2"/>. Panels <bold>(b)</bold>, <bold>(d)</bold> and <bold>(f)</bold> exclude regions of <inline-formula><mml:math id="M164" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>&gt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> from Fig. <xref ref-type="fig" rid="Ch1.F3"/> for the complete ERA5 period.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/9241/2019/acp-19-9241-2019-f08.png"/>

      </fig>

      <p id="d1e2824">To shed light on the influence of circulation dynamics on the <inline-formula><mml:math id="M165" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling of ERA5, we consider the temporal correlation <inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>(</mml:mo><mml:mi>P</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. According to <xref ref-type="bibr" rid="bib1.bibx10" id="text.50"/>, we exclude all precipitation time steps with <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>&gt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> diminishing the influence of precipitation from very shallow convection and large-scale subsidence. The resulting precipitation distribution with respect to SST reveals a less pronounced minimum at about 26 <inline-formula><mml:math id="M168" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F8"/>b).</p>
      <p id="d1e2884">This leads to a slight increase in the <inline-formula><mml:math id="M169" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> scaling at all intensities (Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F8"/>e–f). Accordingly, <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> itself can better explain the  minimum at 26 <inline-formula><mml:math id="M171" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C compared to areas of low correlation between <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M173" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>.</p><?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2940">JB analyzed the data, made the figures and wrote the paper. SB, CK and SAB gave scientific advice and helped improve the paper.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2946">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2952">We thank the crews of all ships involved in the OceanRAIN project for their support, which made it possible to collect unique precipitation data over the ocean.  We thank the two anonymous referees for their help in improving the paper.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2957">Jörg Burdanowitz has been supported by the Deutsche Forschungsgemeinschaft (grant no. BU2253/1-2). Stefan A. Buehler was partially supported by the Cluster of Excellence CliSAP (EXC177), Universität Hamburg, was funded through the DFG, by the German Federal Ministry of Education and Research within the framework program “Research for Sustainable Development (FONA)” under project HD(CP)<inline-formula><mml:math id="M174" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (grant nos. O1LK1502B and O1LK1505D), and was also funded by the DFG HALO research program (grant no. BU2253/3-1).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2972">This paper was edited by Christopher Hoyle and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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    <!--<article-title-html>The sensitivity of oceanic precipitation to sea surface temperature</article-title-html>
<abstract-html><p>Our study forms the oceanic counterpart to numerous observational studies over land concerning the sensitivity of extreme precipitation to a change in air temperature. We explore the sensitivity of oceanic precipitation to changing sea surface temperature (SST) by exploiting two novel datasets at high resolution.
First, we use the Ocean Rainfall And Ice-phase precipitation measurement Network (OceanRAIN) as an observational along-track shipboard dataset at 1&thinsp;min resolution. Second, we exploit the most recent European Reanalysis version 5 (ERA5) at hourly resolution on a 31&thinsp;km grid. Matched with each other, ERA5 vertical velocity allows the constraint of the OceanRAIN precipitation.
Despite the inhomogeneous sampling along ship tracks, OceanRAIN agrees with ERA5 on the average latitudinal distribution of precipitation with fairly good seasonal sampling.
However, the 99th percentile of OceanRAIN precipitation follows a super Clausius–Clapeyron scaling with a SST that exceeds 8.5&thinsp;%&thinsp;K<sup>−1</sup> while ERA5 precipitation scales with 4.5&thinsp;%&thinsp;K<sup>−1</sup>.
The sensitivity decreases towards lower precipitation percentiles, while OceanRAIN keeps an almost constant offset to ERA5 due to higher spatial resolution and temporal sampling. Unlike over land, we find no evidence for a decreasing precipitation event duration with increasing SST.
ERA5 precipitation reaches a local minimum at about 26&thinsp;°C that vanishes when constraining vertical velocity to strongly rising motion and excluding areas of weak correlation between precipitation and vertical velocity. This indicates that instead of moisture limitations as over land, circulation dynamics rather limit precipitation formation over the ocean.
For the strongest rising motion, precipitation scaling converges to a constant value at all precipitation percentiles.
Overall, high resolutions in observations and climate models are key to understanding and predicting the sensitivity of oceanic precipitation extremes to a change in SST.</p></abstract-html>
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