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<front>
<journal-meta>
<journal-id journal-id-type="publisher">EGUsphere</journal-id>
<journal-title-group>
<journal-title>EGUsphere</journal-title>
<abbrev-journal-title abbrev-type="publisher">EGUsphere</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">EGUsphere</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub"></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/egusphere-2026-2627</article-id>
<title-group>
<article-title>A unified closed-form collision kernel for warm-cloud coalescence in the gravity&amp;ndash;turbulence coupled regime and the origin of the rain-initiation bottleneck</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Chishtie</surname>
<given-names>Farrukh A.</given-names>
<ext-link>https://orcid.org/0000-0002-6392-6084</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Peaceful Society, Science and Innovation Foundation, Vancouver, Canada</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Department of Occupational Science and Occupational Therapy, University of British Columbia, Vancouver, Canada</addr-line>
</aff>
<pub-date pub-type="epub">
<day>01</day>
<month>07</month>
<year>2026</year>
</pub-date>
<volume>2026</volume>
<fpage>1</fpage>
<lpage>29</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2026 Farrukh A. Chishtie</copyright-statement>
<copyright-year>2026</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://egusphere.copernicus.org/preprints/2026/egusphere-2026-2627/">This article is available from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2627/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2627/egusphere-2026-2627.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2627/egusphere-2026-2627.pdf</self-uri>
<abstract>
<p>Warm rain forms faster in cloud observations than in standard microphysics models, with the discrepancy concentrated in the 15 to 40 &lt;em&gt;&amp;micro;&lt;/em&gt;m droplet-radius size gap where neither condensational growth nor gravitational differential settling is efficient. We present a closed-form unified collision kernel for warm-cloud coales-cence that interpolates continuously between the laminar and turbulent asymptotic regimes through a single dimensionless parameter, the turbulence-to-gravity ratio &lt;em&gt;&amp;xi;&lt;/em&gt; = &lt;em&gt;C&lt;/em&gt;₀&lt;em&gt;&amp;epsilon;&lt;/em&gt;&lt;sup&gt;1/3&lt;/sup&gt;&lt;span style=&quot;text-decoration: overline;&quot;&gt;&lt;em&gt;s&lt;/em&gt;&lt;/span&gt;&lt;sup&gt;1/3&lt;/sup&gt;/&lt;em&gt;A&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt;, where &lt;em&gt;A&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt; = &lt;em&gt;K&lt;/em&gt;&lt;sub&gt;St &lt;/sub&gt;(&lt;em&gt;R&lt;/em&gt;&lt;sup&gt;2&lt;/sup&gt;&lt;sub&gt;&lt;em&gt;k&lt;/em&gt;&lt;/sub&gt; &amp;minus; &lt;em&gt;R&lt;/em&gt;&lt;sup&gt;2&lt;/sup&gt;&lt;sub&gt;&lt;em&gt;k&lt;/em&gt;&amp;minus;1&lt;/sub&gt;) is the Stokes differential settling speed and &lt;span style=&quot;text-decoration: overline;&quot;&gt;&lt;em&gt;s&lt;/em&gt;&lt;/span&gt; is the mean inter-drop separation. The kernel takes the factored form&lt;/p&gt;
&lt;p&gt;&lt;em&gt;K &lt;/em&gt;(&lt;em&gt;R&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt;, &lt;em&gt;R&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt;&lt;sub&gt;&amp;minus;1&lt;/sub&gt;; &lt;em&gt;&amp;epsilon;&lt;/em&gt;) = &lt;em&gt;&amp;pi;&lt;/em&gt; (&lt;em&gt;R&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt; + &lt;em&gt;R&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt;&lt;sub&gt;&amp;minus;1&lt;/sub&gt;)&amp;sup2; |∆&lt;em&gt;v&lt;sub&gt;t&lt;/sub&gt;&lt;/em&gt;ᵉᶠᶠ | &lt;em&gt;E&lt;/em&gt;ᵉᶠᶠ , &lt;em&gt;E&lt;/em&gt;ᵉᶠᶠ = &lt;em&gt;E&lt;/em&gt;&lt;sub&gt;lam &lt;/sub&gt;(&lt;em&gt;R&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt;, &lt;em&gt;R&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt;&lt;sub&gt;&amp;minus;1&lt;/sub&gt;) &amp;middot; &lt;em&gt;&amp;eta;&lt;sub&gt;E&lt;/sub&gt;&lt;/em&gt;,&lt;/p&gt;
&lt;p&gt;with an effective approach velocity |∆&lt;em&gt;v&lt;sub&gt;t&lt;/sub&gt;&lt;/em&gt;ᵉᶠᶠ| = &lt;em&gt;A&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt; (1 + &lt;em&gt;&amp;xi; &lt;/em&gt;) and a turbulent efficiency enhancement &lt;em&gt;&amp;eta;&lt;sub&gt;E&lt;/sub&gt; &lt;/em&gt;(Stk, &lt;em&gt;&amp;xi; &lt;/em&gt;), both derived in closed form from the hierarchical fractional &lt;em&gt;N&lt;/em&gt;-body dynamics of Chishtie (2026). Three established results are recovered by construction rather than by fitting: the laminar limit &lt;em&gt;&amp;epsilon;&lt;/em&gt; &amp;rarr; 0 reproduces the Hall (1980) kernel with Pinsky et al. (2001) collision efficiency to within a &amp;plusmn;10 % band, the high-&lt;em&gt;&amp;epsilon;&lt;/em&gt; limit reproduces the classical Saffman&amp;ndash;Turner (1956) &lt;em&gt;&amp;epsilon;&lt;/em&gt;&lt;sup&gt;1/3&lt;/sup&gt; turbulent kinetic-theory scaling, and the monotonic ordering &lt;em&gt;&amp;eta;&lt;/em&gt;&lt;sub&gt;&lt;em&gt;E&lt;/em&gt;,2&lt;/sub&gt; &amp;gt; &lt;em&gt;&amp;eta;&lt;sub&gt;E&lt;/sub&gt;&lt;/em&gt;&lt;sub&gt;,3&lt;/sub&gt; &amp;gt; &lt;em&gt;&amp;eta;&lt;sub&gt;E&lt;/sub&gt;&lt;/em&gt;&lt;sub&gt;,4&lt;/sub&gt; with drop size matches the qualitative signature reported by Wang et al. (2005) and Chen et al. (2018) from DNS. Supporting the kernel construction, we also derive an effective Riesz fractional parameter &lt;em&gt;&amp;alpha;&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt;ᵉᶠᶠ = &lt;em&gt;&amp;xi;&lt;/em&gt; / [3(1 + &lt;em&gt;&amp;xi; &lt;/em&gt;)] + 2 &amp;minus; 2 / (&lt;em&gt;N&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt; + 1) that interpolates analytically between the gravity-only and turbulence-only limits, together with closed-form parametric trajectories &lt;em&gt;s&lt;sub&gt;k&lt;/sub&gt; &lt;/em&gt;(&lt;em&gt;&amp;theta;&lt;/em&gt;) = &lt;em&gt;s&lt;/em&gt;₀ sin&lt;sup&gt;&lt;em&gt;n&lt;/em&gt;&lt;/sup&gt; &lt;em&gt;&amp;theta;&lt;/em&gt; with &lt;em&gt;n&lt;/em&gt; = 2 / (&lt;em&gt;p&lt;sub&gt;k&lt;/sub&gt;&lt;/em&gt;ᵉᶠᶠ + 1) validated against RK45 integration to relative errors of 10&lt;sup&gt;&amp;minus;13&lt;/sup&gt;. The kernel is directly implementable in bin microphysics and large-eddy simulation super-droplet schemes and carries no free parameters.</p>
</abstract>
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