<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "https://jats.nlm.nih.gov/nlm-dtd/publishing/3.0/journalpublishing3.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" specific-use="SMUR" dtd-version="3.0" xml:lang="en">
<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">1869-9537</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-2023-1295</article-id>
<title-group>
<article-title>Lahar events in the last 2,000 years from Vesuvius eruptions. Part 3: Hazard assessment over the Campanian Plain</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sandri</surname>
<given-names>Laura</given-names>
<ext-link>https://orcid.org/0000-0002-3254-2336</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>de' Michieli Vitturi</surname>
<given-names>Mattia</given-names>
<ext-link>https://orcid.org/0000-0002-6750-9245</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>Costa</surname>
<given-names>Antonio</given-names>
<ext-link>https://orcid.org/0000-0002-4987-6471</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>Di Vito</surname>
<given-names>Mauro Antonio</given-names>
<ext-link>https://orcid.org/0000-0002-7913-9149</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>Rucco</surname>
<given-names>Ilaria</given-names>
<ext-link>https://orcid.org/0000-0002-8497-494X</ext-link>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Doronzo</surname>
<given-names>Domenico Maria</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>Bisson</surname>
<given-names>Marina</given-names>
<ext-link>https://orcid.org/0000-0002-7104-9210</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>Gianardi</surname>
<given-names>Roberto</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>De Vita</surname>
<given-names>Sandro</given-names>
<ext-link>https://orcid.org/0000-0002-5337-7560</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>Sulpizio</surname>
<given-names>Roberto</given-names>
<ext-link>https://orcid.org/0000-0002-3930-5421</ext-link>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Bologna, Bologna, Italy</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Pisa, Pisa, Italy</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Vesuviano, Napoli, Italy</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>School of Engineering and Physical Sciences, Heriot-Watt University, Edinburgh, UK</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Dipartimento di Scienze della Terra e Geoambientali, University of Bari, Bari, Italy</addr-line>
</aff>
<pub-date pub-type="epub">
<day>18</day>
<month>07</month>
<year>2023</year>
</pub-date>
<volume>2023</volume>
<fpage>1</fpage>
<lpage>26</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2023 Laura Sandri et al.</copyright-statement>
<copyright-year>2023</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/2023/egusphere-2023-1295/">This article is available from https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1295/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1295/egusphere-2023-1295.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1295/egusphere-2023-1295.pdf</self-uri>
<abstract>
<p>&lt;p&gt;In this study we present a novel general methodology for Probabilistic Volcanic Hazard Assessment (PVHA) for lahars. We apply the methodology to perform a probabilistic assessment in the Campanian Plain (Southern Italy), focussing on syn-eruptive lahars from a reference-size eruption from Somma-Vesuvius. We take advantage of new field data relative to volcaniclastic flow deposits in the target region and recent improvements in modelling lahars. We explore the effect of uncertainty on the flow initial conditions on the invasion of lahar in the target area, by sampling coherent sets of values for the input model parameters and performing a large number of simulations. We analyse the simulation outputs to produce hazard curves, hazard maps and probability maps for the maximum flow thickness, and hazard surface and probability maps for joint thresholds in flow thickness and dynamic pressure. We believe the latter hazard products represent, on one hand, a novel product in PVHA for lahars, and, on the other hand, a useful means for impact assessment.&lt;/p&gt;</p>
</abstract>
<counts><page-count count="26"/></counts>
<funding-group>
<award-group id="gs1">
<funding-source>Istituto Nazionale di Geofisica e Vulcanologia</funding-source>
<award-id>-</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Dipartimento della Protezione Civile, Presidenza del Consiglio dei Ministri</funding-source>
<award-id>-</award-id>
</award-group>
</funding-group>
</article-meta>
</front>
<body/>
<back>
</back>
</article>