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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-2026-1865</article-id>
<title-group>
<article-title>First deployment of active AirCore in a volcanic plume at Mount Etna</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Degen</surname>
<given-names>Johannes</given-names>
<ext-link>https://orcid.org/0009-0007-9376-4470</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>Bobrowski</surname>
<given-names>Nicole</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Bossard</surname>
<given-names>Mélisende M.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Boucher</surname>
<given-names>Lucie</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Chen</surname>
<given-names>Huilin</given-names>
<ext-link>https://orcid.org/0000-0002-1573-6673</ext-link>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Engel</surname>
<given-names>Andreas</given-names>
<ext-link>https://orcid.org/0000-0003-0557-3935</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>Geil</surname>
<given-names>Bastien H.</given-names>
</name>
<xref ref-type="aff" rid="aff8">
<sup>8</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Giuffrida</surname>
<given-names>Giovanni B.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>van Heuven</surname>
<given-names>Steven</given-names>
<ext-link>https://orcid.org/0000-0003-2001-8710</ext-link>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Hoffmann</surname>
<given-names>Thorsten</given-names>
<ext-link>https://orcid.org/0000-0003-0939-271X</ext-link>
</name>
<xref ref-type="aff" rid="aff8">
<sup>8</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Karbach</surname>
<given-names>Niklas</given-names>
</name>
<xref ref-type="aff" rid="aff8">
<sup>8</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ortenzi</surname>
<given-names>Gianluigi</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Schuck</surname>
<given-names>Tanja J.</given-names>
<ext-link>https://orcid.org/0000-0002-1380-3684</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Institute for Atmospheric and Environmental Sciences, Goethe University Frankfurt, Frankfurt, Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Institute of Environmental Physics, Heidelberg University, Heidelberg, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Etneo, Catania, Italy</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>École et Observatoire des Sciences de la Terre, Strasbourg University, Strasbourg, France</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>École Normale Supérieure de Paris, Paris Sciences et Lettres University, Paris, France</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>Centre for Isotope Research, University of Groningen, Groningen, the Netherlands</addr-line>
</aff>
<aff id="aff7">
<label>7</label>
<addr-line>School of Atmospheric Sciences, Nanjing University, Nanjing, China</addr-line>
</aff>
<aff id="aff8">
<label>8</label>
<addr-line>Department of Chemistry, Johannes Gutenberg-Universität Mainz, Mainz, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>21</day>
<month>05</month>
<year>2026</year>
</pub-date>
<volume>2026</volume>
<fpage>1</fpage>
<lpage>30</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2026 Johannes Degen 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-2026-1865/">This article is available from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1865/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1865/egusphere-2026-1865.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1865/egusphere-2026-1865.pdf</self-uri>
<abstract>
<p>Uncrewed Aerial Systems (UAS) are by now well established platforms for observations in volcanic plumes which are a challenging environment. Options for trace gas observations inside volcanic plumes still remain limited because sophisticated measurement techniques for high-precision observations of trace gases often require instrumentation that cannot be used on board UAS due to high weight and power consumption. UAS-borne sampling of air followed by post-flight analysis can &amp;nbsp;extend the number of observable trace gases as well as the measurement quality. Originally developed for stratospheric observations, AirCore sampling with long coiled tubes has proven to be a light-weight sampling technique to probe parts of the atmosphere that are otherwise difficult to access. Trace gas analysis of sampled air is done post-flight, most commonly with fast high-precision optical methods with continuous flow analysers, delivering high-quality and high-resolution trace gas mole fractions. While balloon-borne AirCore setups perform passive sampling making use of natural pressure differences, we used a UAS-deployable small active AirCore setup collecting air with a pump. In July 2024, this &amp;nbsp;setup was deployed on a UAS alongside electrochemical and optical gas sensors to probe the volcanic plumes of Mount Etna (Sicily, Italy), which was particularly active at the time. This was to our knowledge the first time that the AirCore sampling technique was used inside volcanic plumes. The air sample was successfully analysed with cavity-ring down spectroscopy for carbon monoxide (CO), carbon dioxide (CO&lt;sub&gt;2&lt;/sub&gt;) and methane (CH&lt;sub&gt;4&lt;/sub&gt;). While CO&lt;sub&gt;2&lt;/sub&gt; and often also CO mole fractions were markedly enhanced in the plume, no significant change of CH&lt;sub&gt;4&lt;/sub&gt; was observed. The ratio of CO and CO&lt;sub&gt;2&lt;/sub&gt; mole fraction enhancements was found to be rather low which might point at fast oxidation processes.</p>
</abstract>
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