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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>2018-01-17T12:16:01Z</responseDate> <request identifier=oai:HAL:hal-01685546v1 verb=GetRecord metadataPrefix=oai_dc>http://api.archives-ouvertes.fr/oai/hal/</request> <GetRecord> <record> <header> <identifier>oai:HAL:hal-01685546v1</identifier> <datestamp>2018-01-17</datestamp> <setSpec>type:ART</setSpec> <setSpec>subject:sdu</setSpec> <setSpec>subject:sde</setSpec> <setSpec>collection:CNRS</setSpec> <setSpec>collection:UNIV-AG</setSpec> <setSpec>collection:SDE</setSpec> <setSpec>collection:GM</setSpec> <setSpec>collection:AGROPOLIS</setSpec> <setSpec>collection:GIP-BE</setSpec> <setSpec>collection:B3ESTE</setSpec> <setSpec>collection:UNIV-MONTPELLIER</setSpec> <setSpec>collection:INSU</setSpec> </header> <metadata><dc> <publisher>HAL CCSD</publisher> <title lang=en>Control of asperities size and spacing on seismic behavior of subduction megathrusts</title> <creator>CORBI, Fabio</creator> <creator>Funiciello, Francesca</creator> <creator>Brizzi, Silvia</creator> <creator>LALLEMAND, Serge</creator> <creator>Rosenau, Matthias</creator> <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>Università degli Studi Roma Tre</contributor> <contributor>GeoForschungsZentrum - Helmholtz-Zentrum Potsdam (GFZ)</contributor> <description>International audience</description> <source>ISSN: 0094-8276</source> <source>EISSN: 1944-8007</source> <source>Geophysical Research Letters</source> <publisher>American Geophysical Union</publisher> <identifier>hal-01685546</identifier> <identifier>https://hal.archives-ouvertes.fr/hal-01685546</identifier> <identifier>https://hal.archives-ouvertes.fr/hal-01685546/document</identifier> <identifier>https://hal.archives-ouvertes.fr/hal-01685546/file/Corbi_et_al-2017-Geophysical_Research_Letters.pdf</identifier> <source>https://hal.archives-ouvertes.fr/hal-01685546</source> <source>Geophysical Research Letters, American Geophysical Union, 2017, 44 (16), pp.8227-8235. 〈10.1002/2017GL074182〉</source> <identifier>DOI : 10.1002/2017GL074182</identifier> <relation>info:eu-repo/semantics/altIdentifier/doi/10.1002/2017GL074182</relation> <language>en</language> <subject lang=en>Asperities</subject> <subject lang=en>megathrust earthquakes</subject> <subject lang=en>analog modelling</subject> <subject>[SDU.STU.TE] Sciences of the Universe [physics]/Earth Sciences/Tectonics</subject> <subject>[SDE.MCG] Environmental Sciences/Global Changes</subject> <type>info:eu-repo/semantics/article</type> <type>Journal articles</type> <description lang=en>The majority of the largest subduction megathrust earthquakes share the common characteristic of rupturing more than one asperity along strike of the margin. Understanding the factors that control coseismic failure of multiple asperities, and thus maximum magnitude, is central for seismic hazard assessment. To investigate the role of asperities size and spacing on maximum magnitude, seismicity rate, and percentage of synchronized ruptures, we use analog models simulating along-strike rupture behavior of megathrust earthquakes. We found negative correlations between the barrier-to-asperity length ratio Db/Da and maximum magnitude and seismicity rate. Db/Da also controls the process of asperities synchronization along the megathrust. A permanent barrier behavior is observed for Db/Da > 0.5. Comparing our experimental results to the Nankai Trough historical seismicity, we propose that the distribution of megathrust frictional heterogeneities likely explains the diversity of earthquakes which occurred there.</description> <date>2017</date> </dc> </metadata> </record> </GetRecord> </OAI-PMH>