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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>2018-01-15T18:21:00Z</responseDate> <request identifier=oai:HAL:hal-01389118v1 verb=GetRecord metadataPrefix=oai_dc>http://api.archives-ouvertes.fr/oai/hal/</request> <GetRecord> <record> <header> <identifier>oai:HAL:hal-01389118v1</identifier> <datestamp>2018-01-11</datestamp> <setSpec>type:ART</setSpec> <setSpec>subject:sdu</setSpec> <setSpec>collection:UNIV-REUNION</setSpec> <setSpec>collection:CNRS</setSpec> <setSpec>collection:UNIV-AG</setSpec> <setSpec>collection:GM</setSpec> <setSpec>collection:AGROPOLIS</setSpec> <setSpec>collection:UNIV-TLSE3</setSpec> <setSpec>collection:INSU</setSpec> <setSpec>collection:B3ESTE</setSpec> <setSpec>collection:UNIV-MONTPELLIER</setSpec> <setSpec>collection:OMP</setSpec> <setSpec>collection:OMP-LMTG</setSpec> <setSpec>collection:OMP-GET</setSpec> <setSpec>collection:IRD</setSpec> </header> <metadata><dc> <publisher>HAL CCSD</publisher> <title lang=en>Anisotropy beneath the Pyrenees Range from teleseismic shear wave splitting: Results from a test experiment</title> <creator>Barruol, Guilhem</creator> <creator>Souriau, Annie</creator> <contributor>Laboratoire de Tectonophysique (Tectonophysique) ; Université Montpellier 2 - Sciences et Techniques (UM2) - Institut national des sciences de l'Univers (INSU - CNRS) - Centre National de la Recherche Scientifique (CNRS)</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>Géosciences Environnement Toulouse (GET) ; Institut de Recherche pour le Développement (IRD) - Université Paul Sabatier - Toulouse 3 (UPS) - Observatoire Midi-Pyrénées (OMP) - Centre National de la Recherche Scientifique (CNRS)</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-01389118</identifier> <identifier>http://hal.univ-reunion.fr/hal-01389118</identifier> <identifier>http://hal.univ-reunion.fr/hal-01389118/document</identifier> <identifier>http://hal.univ-reunion.fr/hal-01389118/file/barruol_pyr_GRL1995.pdf</identifier> <source>http://hal.univ-reunion.fr/hal-01389118</source> <source>Geophysical Research Letters, American Geophysical Union, 1995, 22 (4), pp.493-496. 〈10.1029/94GL03225〉</source> <identifier>DOI : 10.1029/94GL03225</identifier> <relation>info:eu-repo/semantics/altIdentifier/doi/10.1029/94GL03225</relation> <language>en</language> <subject>[SDU.STU.GP] Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]</subject> <type>info:eu-repo/semantics/article</type> <type>Journal articles</type> <description lang=en>We have investigated the seismic anisotropy from SKS and SKKS wave splitting along a N-S profile perpendicular to the Pyrenean mountain belt. The line crossed the North Pyrenean Fault (NPF), which probably represents the plate boundary between the European and the Iberian plates. We observed large delay times δt (1.3 to 1.5 s) and uniform fast polarization directions ϕ (N100E) at three stations located on the Iberian plate. On the other hand, δt are smaller (0.5–1.0 s) and the ϕ scattered at stations located north of the NPF. The small scale variability, the relation with surface geology and the correlation of the δt with lithospheric thickness suggest that the anisotropy could be predominantly of lithospheric origin. However, an asthenospheric contribution cannot be ruled out. In the North Pyrenean Zone, an important thermal event before the Pyrenean compression has likely erased the former mantle fabric. The observed anisotropy is then likely related to the Pyrenean orogeny. On the Iberian plate, our splitting parameters are similar to those obtained at two stations located on Hercynian structures in Central Spain. This suggests that two contributions are likely superposed to that of the Pyrenean built up: one related to the Hercynian orogeny and the other one related to the rotation of the Iberian plate.</description> <date>1995</date> </dc> </metadata> </record> </GetRecord> </OAI-PMH>