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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-2026-2631</article-id>
<title-group>
<article-title>Raman source using a hollow-core fiber for ozone monitoring in the lower troposphere</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Weinzaepflen</surname>
<given-names>Joris</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<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>Ravetta</surname>
<given-names>François</given-names>
<ext-link>https://orcid.org/0000-0002-4264-6235</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>Victori</surname>
<given-names>Stéphane</given-names>
<ext-link>https://orcid.org/0000-0003-3045-2377</ext-link>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ancellet</surname>
<given-names>Gérard</given-names>
<ext-link>https://orcid.org/0000-0002-1542-6085</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>Cailteau-Fischbach</surname>
<given-names>Cristelle</given-names>
<ext-link>https://orcid.org/0009-0002-0549-6087</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</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>Mariage</surname>
<given-names>Vincent</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>Delahaye</surname>
<given-names>Frédéric</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Gérôme</surname>
<given-names>Frédéric</given-names>
<ext-link>https://orcid.org/0000-0001-9213-2876</ext-link>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Benabid</surname>
<given-names>Fetah</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Laboratoire Atmosphères et Observations Spatiales (LATMOS) / Institut Pierre-Simon Laplace (IPSL), Sorbonne Université,  Université Versailles Saint-Quentin, CNRS, 4 place Jussieu 75252 Paris, France</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>CIMEL Electronique, 172 rue de Charonne - 75011 Paris, France</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Université Paris-Saclay, Institut d’Optique Graduate School, CNRS, Laboratoire Charles Fabry, 2 Av. Augustin Fresnel 91127 Palaiseau, France</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Sorbonne Université, CNRS, UAR OMA Terra, Observatoire des Sciences de l’Univers Ecce Terra, Paris Cedex 5, France</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>GLOphotonics, 123 Avenue Albert Thomas, Limoges 87060, France</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>GPPMM Group Xlim, 123 Avenue Albert Thomas Limoges, 87060, France</addr-line>
</aff>
<pub-date pub-type="epub">
<day>04</day>
<month>08</month>
<year>2026</year>
</pub-date>
<volume>2026</volume>
<fpage>1</fpage>
<lpage>17</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2026 Joris Weinzaepflen 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-2026-2631/">This article is available from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2631/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2631/egusphere-2026-2631.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2631/egusphere-2026-2631.pdf</self-uri>
<abstract>
<p>The DIfferential Absorption microlidar for Boundary Layer Ozone (DIABLO) is designed for boundary-layer profiling. This instrument uses a diode-pumped, passively Q-switched Nd:YAG laser at 266 nm, coupled to a deuterium-filled hollow-core fiber (HCF) to generate the 289 nm Stokes wavelength via stimulated Raman scattering (SRS). The high Raman gain in the gas-filled HCF enables efficient UV conversion with significantly lower pump energy than required in traditional free-space Raman cells. At the output of the fiber, 1-ns pulses of 10 &lt;em&gt;&amp;mu;&lt;/em&gt;J at 266 nm and 7 &lt;em&gt;&amp;mu;&lt;/em&gt;J at 289 nm are obtained with a repetition rate of 1 kHz. First atmospheric measurements in central Paris provide ozone concentrations between 400 m and 1700 m. In contrast with existing UV DIAL ozone systems, which are typically bulky, complex, and operated in campaign-based research configurations, DIABLO targets a compact and low-energy architecture optimized for autonomous boundary-layer monitoring.</p>
</abstract>
<counts><page-count count="17"/></counts>
<funding-group>
<award-group id="gs1">
<funding-source>Association Nationale de la Recherche et de la Technologie</funding-source>
<award-id>2023/1612</award-id>
</award-group>
</funding-group>
</article-meta>
</front>
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