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<OAI-PMH schemaLocation=http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd> <responseDate>2018-01-15T18:31:47Z</responseDate> <request identifier=oai:HAL:hal-00941279v1 verb=GetRecord metadataPrefix=oai_dc>http://api.archives-ouvertes.fr/oai/hal/</request> <GetRecord> <record> <header> <identifier>oai:HAL:hal-00941279v1</identifier> <datestamp>2018-01-11</datestamp> <setSpec>type:ART</setSpec> <setSpec>subject:sdu</setSpec> <setSpec>subject:phys</setSpec> <setSpec>subject:sde</setSpec> <setSpec>collection:CNRS</setSpec> <setSpec>collection:UNIV-GRENOBLE1</setSpec> <setSpec>collection:UNIV-SAVOIE</setSpec> <setSpec>collection:UNIV-PARIS7</setSpec> <setSpec>collection:INSU</setSpec> <setSpec>collection:OSUG</setSpec> <setSpec>collection:UGA</setSpec> <setSpec>collection:SDE</setSpec> <setSpec>collection:GM</setSpec> <setSpec>collection:UPMC</setSpec> <setSpec>collection:GIP-BE</setSpec> <setSpec>collection:AFRIQ</setSpec> <setSpec>collection:IFSTTAR</setSpec> <setSpec>collection:ISTERRE</setSpec> <setSpec>collection:ENS-PARIS</setSpec> <setSpec>collection:AGROPOLIS</setSpec> <setSpec>collection:PSL</setSpec> <setSpec>collection:IPGP</setSpec> <setSpec>collection:USPC</setSpec> <setSpec>collection:UNIV-AG</setSpec> <setSpec>collection:B3ESTE</setSpec> <setSpec>collection:UNIV-MONTPELLIER</setSpec> </header> <metadata><dc> <publisher>HAL CCSD</publisher> <title lang=en>Revisiting the North Chile seismic gap segmentation using GPS-derived interseismic coupling</title> <creator>Metois, M.</creator> <creator>Socquet, A.</creator> <creator>Vigny, C.</creator> <creator>Carrizo, D.</creator> <creator>PEYRAT, Sophie</creator> <creator>Delorme, A.</creator> <creator>Maureira, E.</creator> <creator>Valderas-Bermejo, M. -C.</creator> <creator>Ortega, I.</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 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>Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile, Santiago ; Universidad de Santiago de Chile [Santiago] (USACH)</contributor> <contributor>Ris ; 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>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>Servicio Sismologico Nacional, Universidad de Chile, Santiago ; Université du Québec</contributor> <description>International audience</description> <source>ISSN: 0956-540X</source> <source>EISSN: 1365-246X</source> <source>Geophysical Journal International</source> <publisher>Oxford University Press (OUP)</publisher> <identifier>hal-00941279</identifier> <identifier>https://hal.archives-ouvertes.fr/hal-00941279</identifier> <source>https://hal.archives-ouvertes.fr/hal-00941279</source> <source>Geophysical Journal International, Oxford University Press (OUP), 2013, 194 (3), pp.1283-1294. 〈10.1093/gji/ggt183〉</source> <identifier>DOI : 10.1093/gji/ggt183</identifier> <relation>info:eu-repo/semantics/altIdentifier/doi/10.1093/gji/ggt183</relation> <language>en</language> <subject lang=en>Satellite geodesy</subject> <subject lang=en>Seismic cycle</subject> <subject lang=en>Earthquake interaction</subject> <subject lang=en>forecasting</subject> <subject lang=en>and prediction</subject> <subject lang=en>Subduction zone processes</subject> <subject lang=en>South America</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>No major earthquake occurred in North Chile since the 1877 Mw 8.6 subduction earthquake that produced a huge tsunami. However, geodetic measurements conducted over the last decade in this area show that the upper plate is actually deforming, which reveals some degree of locking on the subduction interface. This accumulation of elastic deformation is likely to be released in a future earthquake. Because of the long elapsed time since 1877 and the rapid accumulation of deformation (thought to be 6-7 cm yr−1), many consider this area is a mature seismic gap where a major earthquake is due and seismic hazard is high. We present a new Global Positioning System (GPS) velocity field, acquired between 2008 and 2012, that describes in some detail the interseismic deformation between 18°S and 24°S. We invert for coupling distribution on the Nazca-South America subduction interface using elastic modelling. Our measurements require that, at these latitudes, 10 to 12 mm yr−1 (i.e. 15 per cent of the whole convergence rate) are accommodated by the clockwise rotation of an Andean block bounded to the East by the subandean fold-and-thrust belt. This reduces the accumulation rate on the subduction interface to 56 mm yr−1 in this area. Coupling variations on the subduction interface both along-strike and along-dip are described. We find that the North Chile seismic gap is segmented in at least two highly locked segments bounded by narrow areas of weak coupling. This coupling segmentation is consistent with our knowledge of the historical ruptures and of the instrumental seismicity of the region. Intersegment zones (Iquique, Mejillones) correlate with high background seismic rate and local tectonic complexities on the upper or downgoing plates. The rupture of either the Paranal or the Loa segment alone could easily produce a Mw 8.0-8.3 rupture, and we propose that the Loa segment (from 22.5°S to 20.8°S) may be the one that ruptured in 1877.</description> <date>2013-09</date> </dc> </metadata> </record> </GetRecord> </OAI-PMH>