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<title lang=en>Earthquake supercycles in Central Italy, inferred from 36Cl exposure dating</title>
<creator>Schlagenhauf, Aloe</creator>
<creator>Manighetti, I.</creator>
<creator>Benedetti, L.</creator>
<creator>Gaudemer, Y.</creator>
<creator>Finkel, R.</creator>
<creator>Malavieille, Jacques</creator>
<creator>Pou, K.</creator>
<contributor>Institut des Sciences de la Terre (ISTerre) ; Université Joseph Fourier - Grenoble 1 (UJF) - Institut Français des Sciences et Technologies des Transports, de l'Aménagement et des Réseaux (IFSTTAR) - Institut national des sciences de l'Univers (INSU - CNRS) - Institut de recherche pour le développement [IRD] : UR219 - PRES Université de Grenoble - Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry]) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Géoazur (GEOAZUR) ; Université Pierre et Marie Curie - Paris 6 (UPMC) - Université Nice Sophia Antipolis (UNS) ; Université Côte d'Azur (UCA) - Université Côte d'Azur (UCA) - Institut national des sciences de l'Univers (INSU - CNRS) - Observatoire de la Côte d'Azur - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Centre européen de recherche et d'enseignement de géosciences de l'environnement (CEREGE) ; Institut de Recherche pour le Développement (IRD) - Aix Marseille Université (AMU) - Collège de France (CdF) - Institut national des sciences de l'Univers (INSU - CNRS) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Institut de Physique du Globe de Paris (IPGP) ; Université Pierre et Marie Curie - Paris 6 (UPMC) - Institut national des sciences de l'Univers (INSU - CNRS) - IPG PARIS - Université Paris Diderot - Paris 7 (UPD7) - Université de la Réunion (UR) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Earth and Planetary Science Department ; University of California [Berkeley]</contributor>
<contributor>Géosciences Montpellier ; Université des Antilles et de la Guyane (UAG) - Institut national des sciences de l'Univers (INSU - CNRS) - Université de Montpellier (UM) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Funded by the INSU-CNRS Dyeti program.</contributor>
<description>International audience</description>
<source>ISSN: 0012-821X</source>
<source>Earth and Planetary Science Letters</source>
<publisher>Elsevier</publisher>
<identifier>hal-00667280</identifier>
<identifier>https://hal.archives-ouvertes.fr/hal-00667280</identifier>
<source>https://hal.archives-ouvertes.fr/hal-00667280</source>
<source>Earth and Planetary Science Letters, Elsevier, 2011, 307 (3-4), pp.487-500. 〈10.1016/j.epsl.2011.05.022〉</source>
<identifier>DOI : 10.1016/j.epsl.2011.05.022</identifier>
<relation>info:eu-repo/semantics/altIdentifier/doi/10.1016/j.epsl.2011.05.022</relation>
<language>en</language>
<subject lang=en>past earthquakes</subject>
<subject lang=en>earthquake clustering</subject>
<subject lang=en>36Cl cosmogenic exposure dating</subject>
<subject lang=en>normal fault</subject>
<subject lang=en>Lazio-Abruzzo (Central Italy)</subject>
<subject>[SDU.STU] Sciences of the Universe [physics]/Earth Sciences</subject>
<type>info:eu-repo/semantics/article</type>
<type>Journal articles</type>
<description lang=en>We use 36Cl surface exposure dating to determine the slip release pattern over the last ~ 15 kyr for the Velino-Magnola fault, a major active normal fault in Central Italy. We sampled the fault at five well-separated sites along its length, and modeled the 36Cl concentrations measured in the 376 samples. We find that the fault broke in at least 9 large earthquakes that occurred in two 5-6 ka-long supercycles. Each cycle included a 4-5 ka-long phase of relative quiescence, followed by a cluster of at least 3 large earthquakes or earthquake sequences that released most of the accumulated strain in ~ 1 ka. All 9 identified events broke the entire fault and produced maximum surface slips of 2-3 m. Though the Velino-Magnola fault seems presently in a stage of relative quiescence, it may re-enter a phase of paroxysmal seismic activity in a few hundred of years</description>
<date>2011-07-15</date>
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