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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>2018-01-15T18:42:15Z</responseDate> <request identifier=oai:HAL:hal-00617518v1 verb=GetRecord metadataPrefix=oai_dc>http://api.archives-ouvertes.fr/oai/hal/</request> <GetRecord> <record> <header> <identifier>oai:HAL:hal-00617518v1</identifier> <datestamp>2018-01-11</datestamp> <setSpec>type:ART</setSpec> <setSpec>subject:sdu</setSpec> <setSpec>subject:sde</setSpec> <setSpec>collection:CNRS</setSpec> <setSpec>collection:UNIV-FCOMTE</setSpec> <setSpec>collection:SDE</setSpec> <setSpec>collection:GM</setSpec> <setSpec>collection:GIP-BE</setSpec> <setSpec>collection:AGROPOLIS</setSpec> <setSpec>collection:INSU</setSpec> <setSpec>collection:UNIV-AG</setSpec> <setSpec>collection:CHRONO-ENVIRONNEMENT</setSpec> <setSpec>collection:B3ESTE</setSpec> <setSpec>collection:UNIV-MONTPELLIER</setSpec> </header> <metadata><dc> <publisher>HAL CCSD</publisher> <title lang=en>Polyphase seismic faulting in the Ivrea zone (Italian Alps) revealed by Ar-40/Ar-39 dating of pseudotachylytes</title> <creator>Souquiere, Francois</creator> <creator>Monie, Patrick</creator> <creator>Fabbri, Olivier</creator> <creator>Chauvet, Alain</creator> <contributor>Laboratoire Chrono-environnement (LCE) ; Université Bourgogne Franche-Comté (UBFC) - Centre National de la Recherche Scientifique (CNRS) - Université de Franche-Comté (UFC)</contributor> <contributor>Dynamique de la Lithosphere ; 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>Bassins ; 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> <description>International audience</description> <source>ISSN: 0954-4879</source> <source>EISSN: 1365-3121</source> <source>Terra Nova</source> <publisher>Wiley-Blackwell</publisher> <identifier>hal-00617518</identifier> <identifier>https://hal.archives-ouvertes.fr/hal-00617518</identifier> <source>https://hal.archives-ouvertes.fr/hal-00617518</source> <source>Terra Nova, Wiley-Blackwell, 2011, 23 (3), pp.162-170. 〈10.1111/j.1365-3121.2011.00994.x〉</source> <identifier>DOI : 10.1111/j.1365-3121.2011.00994.x</identifier> <relation>info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-3121.2011.00994.x</relation> <language>en</language> <subject lang=en>DORA-MAIRA MASSIF</subject> <subject lang=en>VERBANO ZONE</subject> <subject lang=en>ULTRAMAFIC PSEUDOTACHYLYTES</subject> <subject lang=en>INSUBRIC LINE</subject> <subject lang=en>SOUTHERN ALPS</subject> <subject>[SDU.STU.GC] Sciences of the Universe [physics]/Earth Sciences/Geochemistry</subject> <subject>[SDE.MCG] Environmental Sciences/Global Changes</subject> <type>info:eu-repo/semantics/article</type> <type>Journal articles</type> <description lang=en>P>Most fault-related pseudotachylytes in the Val Sesia area, Ivrea zone, NW Italian Alps, occur in two areas: near the Canavese Line in the Kinzigite Formation paragneisses and in an elongate belt in the Mafic Complex gabbros away from the Canavese Line. Ar-40/Ar-39 dating indicates that pseudotachylytes from the Kinzigite Formation were formed in the late Eocene, likely during the early stages of the collision between the NW corner of the Adriatic indenter and the European margin. Pseudotachylytes from the Mafic Complex were formed under a transpressive strain regime, as suggested by kinematic indicators, and yield Early Cretaceous (Albian) Ar-40/Ar-39 ages. Their formation is possibly related to shortening during the inception of the tectonic inversion of the Adriatic passive margin.</description> <date>2011</date> </dc> </metadata> </record> </GetRecord> </OAI-PMH>