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<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-13-7795-2013</article-id>
<title-group>
<article-title>Direct entrainment and detrainment rate distributions of individual shallow cumulus clouds in an LES</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Dawe</surname>
<given-names>J. T.</given-names>
<ext-link>https://orcid.org/0000-0002-4704-5404</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Austin</surname>
<given-names>P. H.</given-names>
<ext-link>https://orcid.org/0000-0001-8036-8152</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Department of Earth, Ocean, and Atmospheric Sciences, University of British Columbia, Room 2020, Earth Sciences Building, 2207 Main Mall, Vancouver, BC, V6T 1Z4, Canada</addr-line>
</aff>
<pub-date pub-type="epub">
<day>13</day>
<month>08</month>
<year>2013</year>
</pub-date>
<volume>13</volume>
<issue>15</issue>
<fpage>7795</fpage>
<lpage>7811</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2013 J. T. Dawe</copyright-statement>
<copyright-year>2013</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://acp.copernicus.org/articles/13/7795/2013/acp-13-7795-2013.html">This article is available from https://acp.copernicus.org/articles/13/7795/2013/acp-13-7795-2013.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/13/7795/2013/acp-13-7795-2013.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/13/7795/2013/acp-13-7795-2013.pdf</self-uri>
<abstract>
<p>Probability distribution functions of shallow cumulus cloud core
  entrainment and detrainment rates are calculated using 4362
  individual cumulus clouds isolated from LES (large eddy simulation) using a cloud tracking
  algorithm.  Calculation of the mutual information between fractional
  entrainment/detrainment and a variety of mean cloud core properties
  suggests that fractional entrainment rate is best predicted by the
  mean cloud buoyancy &lt;i&gt;B&lt;/i&gt; and the environmental buoyancy lapse rate
d&lt;span style=&quot;text-decoration: overline&quot;&gt;&amp;theta;&lt;sub&gt;&amp;rho;&lt;/sub&gt;&lt;/span&gt;/d&lt;i&gt;z&lt;/i&gt;
 at that level, while
  fractional detrainment is best predicted by the mean vertical
  velocity &lt;i&gt;w&lt;/i&gt; and the critical mixing fraction &amp;chi;&lt;sub&gt;c&lt;/sub&gt;.  Fractional
  entrainment and detrainment rates are relatively insensitive to
  cloud core horizontal area, and the perimeter of horizontal
  cloud core sections display an &lt;i&gt;a&lt;/i&gt;&lt;sup&gt;0.73&lt;/sup&gt; dependence. This implies
  that cloud core mass entrainment flux &lt;i&gt;E&lt;/i&gt; is proportional to cloud
  core cross-sectional area instead of cloud core surface area, as is
  generally assumed.  Empirical best-fit relations for &amp;epsilon;(&lt;i&gt;B&lt;/i&gt;,
 d&lt;span style=&quot;text-decoration: overline&quot;&gt;&amp;theta;&lt;sub&gt;&amp;rho;&lt;/sub&gt;&lt;/span&gt;/d&lt;i&gt;z&lt;/i&gt; and &amp;delta;(&lt;i&gt;w&lt;/i&gt;,
  &amp;chi;&lt;sub&gt;c&lt;/sub&gt;) are found for both individual shallow cumulus clouds and
  cloud ensembles.  It is found that clouds with high buoyancy in
  strong stratification experience low entrainment rates, while clouds
  with high vertical velocities and critical mixing fractions
  experience low detrainment rates.</p>
</abstract>
<counts><page-count count="17"/></counts>
</article-meta>
</front>
<body/>
<back>
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