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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-2026-3856</article-id>
<title-group>
<article-title>Vertical profiling and aerosol typing using fluorescence Raman and depolarization lidar measurements over Thessaloniki, Greece</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Peletidou</surname>
<given-names>Georgia</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>Voudouri</surname>
<given-names>Kalliopi A.</given-names>
<ext-link>https://orcid.org/0000-0001-8298-5103</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 contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Michailidis</surname>
<given-names>Konstantinos</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>Paschou</surname>
<given-names>Peristera</given-names>
<ext-link>https://orcid.org/0000-0001-9959-0247</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>Siomos</surname>
<given-names>Nikolaos</given-names>
<ext-link>https://orcid.org/0000-0001-7773-342X</ext-link>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Reichardt</surname>
<given-names>Jens</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Balis</surname>
<given-names>Dimitrios</given-names>
<ext-link>https://orcid.org/0000-0003-1161-7746</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Aristotle University of Thessaloniki, Department of Physics, 54124 Thessaloniki, Greece</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>National Observatory of Athens, Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing, 15236  Athens, Greece</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Chair of Experimental Meteorology, Faculty of Physics, Ludwig-Maximilians-Universität München, 80539 München,  Germany</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Richard-Aßmann-Observatorium, Deutscher Wetterdienst, Lindenberg, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>08</day>
<month>07</month>
<year>2026</year>
</pub-date>
<volume>2026</volume>
<fpage>1</fpage>
<lpage>27</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2026 Georgia Peletidou 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-2026-3856/">This article is available from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3856/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3856/egusphere-2026-3856.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3856/egusphere-2026-3856.pdf</self-uri>
<abstract>
<p>In this study, we present the first fluorescence lidar observations over Thessaloniki, Greece, (40.63&amp;deg; N, 22.96&amp;deg; E; 60 m a.s.l.) using a multiwavelength Raman and depolarization lidar with fluorescence capabilities. For the first time in the Eastern Mediterranean fluorescence backscattering coefficient and the spectral fluorescence capacity parameter are retrieved and combined with particle depolarization ratio, lidar ratios, and &amp;Aring;ngstr&amp;ouml;m exponents to characterize the aerosol load over Thessaloniki, a region influenced by diverse aerosol sources. Representative case studies of biomass-burning smoke, Saharan dust, and mixed pollen event showing distinct fluorescence properties are discussed in detail, while an extended dataset covering the period April 2024 &amp;ndash; December 2025 is further analysed, comprising 108 aerosol layers from 50 measurement cases. A sub-dataset is also compared with the EARLINET Mahalanobis distance&amp;ndash;based typing algorithm, highlighting the importance and complementarity of fluorescence lidar observations on the aerosol characterization in complex environments. Based on the spectral fluorescence capacity and the particle depolarization ratio, the identified layers are classified into smoke, dust, polluted continental, clean continental and mixed pollen. THELISYS retrievals show that the spectral fluorescence capacity depends on aerosol type, with smoke showing the highest values (3.5 &amp;times; 10&lt;sup&gt;&amp;minus;6&lt;/sup&gt; &amp;minus; 12.7 &amp;times; 10&lt;sup&gt;&amp;minus;6&lt;/sup&gt; 𝑛𝑚&lt;sup&gt;&amp;minus;1&lt;/sup&gt;), followed by mixed pollen (2.3 &amp;times; 10&lt;sup&gt;&amp;minus;6&lt;/sup&gt; &amp;minus; 4.8 &amp;times; 10&lt;sup&gt;&amp;minus;6&lt;/sup&gt; 𝑛𝑚&lt;sup&gt;&amp;minus;1&lt;/sup&gt;), polluted continental (1.0 &amp;times; 10&lt;sup&gt;&amp;minus;6&lt;/sup&gt; &amp;minus; 3.3 &amp;times; 10&lt;sup&gt;&amp;minus;6&lt;/sup&gt; 𝑛𝑚&lt;sup&gt;&amp;minus;1&lt;/sup&gt;), clean continental (0.3 &amp;times; 10&lt;sup&gt;&amp;minus;6&lt;/sup&gt; &amp;minus; 1.2 &amp;times; 10&lt;sup&gt;&amp;minus;6&lt;/sup&gt; 𝑛𝑚&lt;sup&gt;&amp;minus;1&lt;/sup&gt;) and dust (0.6 &amp;times; 10&lt;sup&gt;&amp;minus;6&lt;/sup&gt; &amp;minus; 1.3 &amp;times; 10&lt;sup&gt;&amp;minus;6&lt;/sup&gt; 𝑛𝑚&lt;sup&gt;&amp;minus;1&lt;/sup&gt;). The fluorescence capacity values observed for all aerosol types are comparable with other studies across central and northern Europe, however the linear particle depolarization ratio measurements attributed to pollen differ from those reported at more northern latitudes, possibly reflecting differences in pollen type.</p>
</abstract>
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