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<publisher>HAL CCSD</publisher>
<title lang=en>The 2010 M-w 8.8 Maule Megathrust Earthquake of Central Chile, Monitored by GPS</title>
<creator>Vigny, C.</creator>
<creator>Socquet, A.</creator>
<creator>PEYRAT, Sophie</creator>
<creator>Ruegg, J-C</creator>
<creator>Metois, M.</creator>
<creator>Madariaga, R.</creator>
<creator>Morvan, S.</creator>
<creator>Lancieri, M.</creator>
<creator>Lacassin, R.</creator>
<creator>Campos, J.</creator>
<creator>Carrizo, D.</creator>
<creator>Bejar-Pizarro, M.</creator>
<creator>Barrientos, S.</creator>
<creator>Armijo, R.</creator>
<creator>Aranda, C.</creator>
<creator>Valderas-Bermejo, M-C</creator>
<creator>Ortega, I.</creator>
<creator>Bondoux, F.</creator>
<creator>Baize, S.</creator>
<creator>Lyon-Caen, H.</creator>
<creator>Pavez, A.</creator>
<creator>Vilotte, J. P.</creator>
<creator>Bevis, M.</creator>
<creator>Brooks, B.</creator>
<creator>Smalley, R.</creator>
<creator>Parra, H.</creator>
<creator>Baez, J-C</creator>
<creator>Blanco, M.</creator>
<creator>Cimbaro, S.</creator>
<creator>Kendrick, E.</creator>
<contributor>Laboratoire de géologie de l'ENS (LGE) ; École normale supérieure - Paris (ENS Paris) - 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>Risques ; 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) - 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>Departamento de Geofisica, Universidad de Chile, Santiago ; Université du Québec</contributor>
<description>International audience</description>
<source>ISSN: 0036-8075</source>
<source>EISSN: 1095-9203</source>
<source>Science</source>
<publisher>American Association for the Advancement of Science</publisher>
<identifier>hal-00783213</identifier>
<identifier>https://hal.archives-ouvertes.fr/hal-00783213</identifier>
<source>https://hal.archives-ouvertes.fr/hal-00783213</source>
<source>Science, American Association for the Advancement of Science, 2011, 332, pp.1417-1421. 〈10.1126/science.1204132〉</source>
<identifier>DOI : 10.1126/science.1204132</identifier>
<relation>info:eu-repo/semantics/altIdentifier/doi/10.1126/science.1204132</relation>
<language>en</language>
<subject lang=en>Chile</subject>
<subject lang=en>earthquake</subject>
<subject lang=en>GPS</subject>
<subject>[SDU.STU.GP] Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]</subject>
<subject>[PHYS.PHYS.PHYS-GEO-PH] Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]</subject>
<subject>[SDE.MCG] Environmental Sciences/Global Changes</subject>
<type>info:eu-repo/semantics/article</type>
<type>Journal articles</type>
<description lang=en>Large earthquakes produce crustal deformation that can be quantified by geodetic measurements, allowing for the determination of the slip distribution on the fault. We used data from Global Positioning System (GPS) networks in Central Chile to infer the static deformation and the kinematics of the 2010 moment magnitude (M-w) 8.8 Maule megathrust earthquake. From elastic modeling, we found a total rupture length of similar to 500 kilometers where slip (up to 15 meters) concentrated on two main asperities situated on both sides of the epicenter. We found that rupture reached shallow depths, probably extending up to the trench. Resolvable afterslip occurred in regions of low coseismic slip. The low-frequency hypocenter is relocated 40 kilometers southwest of initial estimates. Rupture propagated bilaterally at about 3.1 kilometers per second, with possible but not fully resolved velocity variations.</description>
<date>2011</date>
</dc>
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