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Authordc.contributor.authorContreras Reyes, Eduardo 
Authordc.contributor.authorMaksymowicz, Andrei 
Authordc.contributor.authorLange, Dietrich 
Authordc.contributor.authorIngo, Grevemeyer 
Authordc.contributor.authorMuñoz Linford, Pamela Karina 
Authordc.contributor.authorAchu Moscoso, Eduardo Alberto 
Admission datedc.date.accessioned2018-06-11T17:36:33Z
Available datedc.date.available2018-06-11T17:36:33Z
Publication datedc.date.issued2017
Cita de ítemdc.identifier.citationEarth and Planetary Science Letters 478 (2017): 27–39es_ES
Identifierdc.identifier.otherhttp://dx.doi.org/10.1016/j.epsl.2017.08.028
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/148769
Abstractdc.description.abstractSubduction megathrust earthquakes show complex rupture behaviour and large lateral variations of slip. However, the factors controlling seismic slip are still under debate. Here, we present 2-D velocity-depth tomographic models across four trench-perpendicular wide angle seismic profiles complemented with high resolution bathymetric data in the area of maximum coseismic slip of the Mw8.8 Maule 2010 megathrust earthquake (central Chile, 34◦–36◦S). Results show an abrupt lateral velocity gradient in the trench-perpendicular direction (from 5.0 to 6.0 km/s) interpreted as the contact between the accretionary prism and continental framework rock whose superficial expression spatially correlates with the slope-shelf break. The accretionary prism is composed of two bodies: (1) an outer accretionary wedge (5–10km wide) characterized by low seismic velocities of 1.8–3.0 km/s interpreted as an outer frontal prism of poorly compacted and hydrated sediment, and (2) the middle wedge (∼50 km wide) with velocities of 3.0–5.0 km/s interpreted as a middle prism composed by compacted and lithified sediment. In addition, the maximum average coseismic slip of the 2010 megathrust event is fairly coincident with the region where the accretionary prism and continental slope are widest (50–60 km wide), and the continental slope angle is low (<5◦). We observe a similar relation along the rupture area of the largest instrumentally recorded Valdivia 1960 Mw9.5 megathrust earthquake. For the case of the Maule event, published differential multibeam bathymetric data confirms that coseismic slip must have propagated up to ∼6 km landwards of the deformation front and hence practically the entire base of the middle prism. Sediment dewatering and compaction processes might explain the competent rheology of the middle prism allowing shallow earthquake rupture. In contrast, the outer frontal prism made of poorly consolidated sediment has impeded the rupture up to the deformation front as high resolution seismic reflection and multibeam bathymetric data have not showed evidence for new deformation in the trench region.es_ES
Patrocinadordc.description.sponsorshipChilean National Science Foundation FONDECYT grant 1130004. Sonderforschungsbereich 574 (Special Research Area) FONDE-CYT grant 3150160es_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherElsevieres_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourceEarth and Planetary Science Letterses_ES
Keywordsdc.subjectSubduction zone earthquakees_ES
Keywordsdc.subjectChilees_ES
Keywordsdc.subjectConvergent margines_ES
Keywordsdc.subjectAccretionary prismes_ES
Keywordsdc.subjectMaule 2010 earthquakees_ES
Títulodc.titleOn the relationship between structure, morphology and large coseismic slip: a case study of the Mw 8.8 Maule, Chile 2010 earthquakees_ES
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadortjnes_ES
Indexationuchile.indexArtículo de publicación ISIes_ES


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