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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>2018-01-15T15:40:55Z</responseDate> <request identifier=oai:HAL:hal-00413047v1 verb=GetRecord metadataPrefix=oai_dc>http://api.archives-ouvertes.fr/oai/hal/</request> <GetRecord> <record> <header> <identifier>oai:HAL:hal-00413047v1</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: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:B3ESTE</setSpec> <setSpec>collection:UNIV-MONTPELLIER</setSpec> </header> <metadata><dc> <publisher>HAL CCSD</publisher> <title lang=en>Rock magnetic and paleointensity results from Mesozoic baked contacts of Armenia</title> <creator>Shcherbakova, V. V.</creator> <creator>Perrin, Mireille</creator> <creator>Shcherbakov, V. P.</creator> <creator>Pavlov, V. E.</creator> <creator>Ayvaz'Yan, A.</creator> <creator>Zhidkov, G. V.</creator> <contributor>Borok Geophysical Observatory (BGO) ; Schmidt Institute of Physics of the Earth [Moscow] (IPE) ; Russian Academy of Sciences [Moscow] (RAS) - Russian Academy of Sciences [Moscow] (RAS)</contributor> <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>Schmidt Institute of Physics of the Earth [Moscow] (IPE) ; Russian Academy of Sciences [Moscow] (RAS)</contributor> <contributor>Yerevan State University, Departament of Geology ; Université du Québec</contributor> <description>International audience</description> <source>ISSN: 1343-8832</source> <source>Earth Planets and Space</source> <publisher>Springer/Terra Scientific Publishing Company</publisher> <identifier>hal-00413047</identifier> <identifier>https://hal.archives-ouvertes.fr/hal-00413047</identifier> <source>https://hal.archives-ouvertes.fr/hal-00413047</source> <source>Earth Planets and Space, Springer/Terra Scientific Publishing Company, 2009, 61 (1), pp.23-39</source> <language>en</language> <subject lang=en>Paleointensity</subject> <subject lang=en>Armenia</subject> <subject lang=en>Cretaceous</subject> <subject lang=en>baked contacts</subject> <subject lang=en>Thellier method</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>Samples were obtained from three baked contacts and one lava flow along the upper Turonian-lower Coniacian Tovuz section, two baked contacts along the upper Coniacian-lower Santonian Paravakar section in the northern part of Armenia, and three baked contacts along the Titonian-Valanginian Kafan section in southern Armenia. A total of 130 samples were studied. Updated mean paleomagnetic poles were calculated for the Upper Cretaceous Tovuz-Paravakar sections (65.6 degrees N, 162.2 degrees E, A(95) = 4.3, paleolatitude = 27.0 +/- 3.4 degrees) and the Upper Jurassic-Lower Cretaceous Kafan section (61.7 degrees N, 158.9 degrees E, A(95) = 4.8 degrees, paleolatitude = 24.7 +/- 3.8 degrees). Paleointensity determinations could be estimated from two of the upper Cretaceous and three of the Upper Jurassic-Lower Cretaceous baked contacts, corresponding to a 30% success rate. The mean virtual dipole moments obtained were low (1.7-5.5 x 10(22) A m(2)), which is in agreement with data published by Bol'shakov and Solodovnikov (1981a, 1983) for the same sections (3.0-4.4 x 10(22) A m(2)). Our results support the hypothesis of the Mesozoic Dipole Low, even though the overall data arc widely dispersed.</description> <date>2009</date> </dc> </metadata> </record> </GetRecord> </OAI-PMH>