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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-2026-1411</article-id>
<title-group>
<article-title>Explicit Numerical Simulations of Hailstorm Seeding with a Three&amp;ndash;Moment Microphysics Cloud&amp;ndash;Resolving Model: A Comparison of Two Operational Methodologies for Hail Suppression</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Savić</surname>
<given-names>Darko</given-names>
<ext-link>https://orcid.org/0000-0001-5043-6791</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>Vučković</surname>
<given-names>Vladan</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Vujović</surname>
<given-names>Dragana</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>University of Belgrade, Faculty of Physics, Belgrade, 11001, Serbia</addr-line>
</aff>
<pub-date pub-type="epub">
<day>08</day>
<month>04</month>
<year>2026</year>
</pub-date>
<volume>2026</volume>
<fpage>1</fpage>
<lpage>55</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2026 Darko Savić et al.</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-2026-1411/">This article is available from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1411/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1411/egusphere-2026-1411.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1411/egusphere-2026-1411.pdf</self-uri>
<abstract>
<p>The global trend of increasing economic losses due to hailstorms sustains the relevance of hail suppression as a weather modification technique. However, quantifying the physical effectiveness of operational cloud seeding remains a significant challenge due to the inherent nonlinearity and complexity of convective processes.&lt;/p&gt;
&lt;p&gt;In this study, we use a 3&amp;ndash;dimensional numerical model, ARPS (Advanced Regional Prediction System), featuring a three&amp;ndash;moment microphysical scheme to simulate the seeding of a supercell. The model is improved by implementing a two&amp;ndash;moment aerosol microphysics that accounts for all the known scavenging processes and parameterizations of all four ice&amp;ndash;nucleating modes. The prognostic equations for aerosol mixing ratio and number concentration in the air and in each hydrometeor category were calculated. Simulations were conducted at a high spatial resolution (500 m horizontal, 250 m vertical) over a 3&amp;ndash;hour evolution period. This approach allows for a very explicit simulation of processes associated with cloud seeding.&lt;/p&gt;
&lt;p&gt;Two operational seeding methodologies were investigated, RHSS (Republic Hydrometeorological Service of Serbia, 2023) and AB23 (Abshaev et al., 2023). The results indicate that both strategies effectively reduce hail&amp;ndash;induced crop damage. Total hail kinetic energy decreased by 27 % (RHSS) and 17.9 % (AB23). Notably, the surface area of moderate risk (KE&lt;sub&gt;flux&lt;/sub&gt; &amp;gt; 100 J m&lt;sup&gt;-2&lt;/sup&gt;) was reduced by 36.6 % and 38.6 %, while high&amp;ndash;risk areas (KE&lt;sub&gt;flux&lt;/sub&gt; &amp;gt; 300 J m&lt;sup&gt;-2&lt;/sup&gt;) saw a significant reduction of 66 % and 88 %, respectively.</p>
</abstract>
<counts><page-count count="55"/></counts>
<funding-group>
<award-group id="gs1">
<funding-source>Science Fund of the Republic of Serbia</funding-source>
<award-id>7389</award-id>
</award-group>
</funding-group>
</article-meta>
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