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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>
<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-2026-6431</article-id>
<title-group>
<article-title>Disentangling Atmospheric Turbulence from Hydrometeor Aerodynamics: Radar Spectrum Width Peaks and Microphysical Signatures within Dendritic Growth Zones</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Suh</surname>
<given-names>Sung-Ho</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Flight Safety Technology Division, NARO Space Center, Korea Aerospace Research Institute (KARI), 508 Haban-ro, Bongrae-myeon, Goheung-gun, Jeollanam-do, Republic of Korea</addr-line>
</aff>
<pub-date pub-type="epub">
<day>09</day>
<month>11</month>
<year>2026</year>
</pub-date>
<volume>2026</volume>
<fpage>1</fpage>
<lpage>31</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2026 Sung-Ho Suh</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-2026-6431/">This article is available from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6431/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6431/egusphere-2026-6431.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6431/egusphere-2026-6431.pdf</self-uri>
<abstract>
<p>The Doppler velocity spectrum width (&lt;em&gt;&amp;sigma;&lt;/em&gt;&lt;sub&gt;v&lt;/sub&gt;) observed by dual-polarization weather radar is widely used as a proxy for atmospheric turbulence, including convectively induced turbulence (CIT) hazardous to aviation. However, &lt;em&gt;&amp;sigma;&lt;/em&gt;&lt;sub&gt;v&lt;/sub&gt; also responds to the aerodynamic behavior of frozen hydrometeors, so its interpretation within the dendritic growth zone (DGZ) remains ambiguous. This study combines a spheroidal aerodynamic response model with quasi-vertical profile (QVP) observations from eight precipitation cases recorded by the S-band dual-polarization radar at the Yongin testbed. Simulations show that particle geometry governs how efficiently a wind perturbation is converted into radial-velocity variance: the whole plane-crystal series, from plates to dendrites, responds far more strongly than columnar or rimed habits. A quantitative procedure identified a &lt;em&gt;&amp;sigma;&lt;/em&gt;&lt;sub&gt;v&lt;/sub&gt; peak zone in five cases, all stratiform. In four of them &lt;em&gt;&amp;sigma;&lt;/em&gt;&lt;sub&gt;v&lt;/sub&gt; showed no systematic relationship with vertical wind shear (&lt;em&gt;VWS&lt;/em&gt;) but a temperature-dependent negative relationship with differential reflectivity (&lt;em&gt;Z&lt;/em&gt;&lt;sub&gt;DR&lt;/sub&gt;); static stability and near-vertical radial-velocity observations argue against a thermally driven origin, while the ice-relative vapor density excess (&lt;em&gt;&amp;Delta;&amp;rho;&lt;/em&gt;&lt;sub&gt;v&lt;/sub&gt;) maximum was positively related to, and vertically adjacent to, the &lt;em&gt;&amp;sigma;&lt;/em&gt;&lt;sub&gt;v&lt;/sub&gt; maximum. Beneath the peak, an aggregation index derived from &lt;em&gt;Z&lt;/em&gt;&lt;sub&gt;H&lt;/sub&gt;, &lt;em&gt;Z&lt;/em&gt;&lt;sub&gt;DR&lt;/sub&gt;, and &lt;em&gt;K&lt;/em&gt;&lt;sub&gt;DP&lt;/sub&gt; increased with &lt;em&gt;&amp;sigma;&lt;/em&gt;&lt;sub&gt;v&lt;/sub&gt; magnitude, whereas a counterpart index for vapor-depositional growth did not. The cases separate into weak plate-dominated growth, strong dendritic growth, and one shear-driven peak unrelated to the DGZ. These results suggest that &lt;em&gt;&amp;sigma;&lt;/em&gt;&lt;sub&gt;v&lt;/sub&gt; within growth layers is partly determined by the hydrometeors observed, so estimating turbulence inside precipitating systems requires knowledge of the microphysical state and hydrometeor type.</p>
</abstract>
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