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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>2018-01-15T15:39:44Z</responseDate> <request identifier=oai:HAL:hal-00475536v1 verb=GetRecord metadataPrefix=oai_dc>http://api.archives-ouvertes.fr/oai/hal/</request> <GetRecord> <record> <header> <identifier>oai:HAL:hal-00475536v1</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:B3ESTE</setSpec> <setSpec>collection:UNIV-AG</setSpec> <setSpec>collection:UNIV-MONTPELLIER</setSpec> </header> <metadata><dc> <publisher>HAL CCSD</publisher> <title lang=en>Kinematics of the southern Red Sea-Afar Triple Junction and implications for plate dynamics</title> <creator>Mcclusky, Simon</creator> <creator>Reilinger, Robert</creator> <creator>Ogubazghi, Ghebrebrhan</creator> <creator>Amleson, Aman</creator> <creator>Healeb, Biniam</creator> <creator>Vernant, Philippe</creator> <creator>Sholan, Jamal</creator> <creator>Fisseha, Shimelles</creator> <creator>Asfaw, Laike</creator> <creator>Bendick, Rebecca</creator> <creator>Kogan, Lewis</creator> <contributor>Department of Earth, Atmospheric and Planetary Sciences [MIT, Cambridge] (EAPS) ; Massachusetts Institute of Technology (MIT)</contributor> <contributor>Department of Earth Sciences, University of Asmara ; Université du Québec</contributor> <contributor>Department of Mines, Eritrea Geological Survey, Asmara ; Université du Québec</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>Yemen National Seismological Observatory Center, Dhamar ; Université du Québec</contributor> <contributor>Geophysical Observatory, Addis Ababa University ; Université du Québec</contributor> <contributor>Department of Geosciences, University of Montana, Missoula ; Université du Québec</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-00475536</identifier> <identifier>https://hal.archives-ouvertes.fr/hal-00475536</identifier> <source>https://hal.archives-ouvertes.fr/hal-00475536</source> <source>Geophysical Research Letters, American Geophysical Union, 2010, 37, pp.L05301. 〈10.1029/2009GL041127〉</source> <identifier>DOI : 10.1029/2009GL041127</identifier> <relation>info:eu-repo/semantics/altIdentifier/doi/10.1029/2009GL041127</relation> <language>en</language> <subject lang=id>Danakil</subject> <subject lang=id>Red Sea</subject> <subject lang=id>geodesy</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>GPS measurements adjacent to the southern Red Sea and Afar Triple Junction, indicate that the Red Sea Rift bifurcates south of 17 degrees N latitude with one branch following a continuation of the main Red Sea Rift (similar to 150 degrees Az.) and the other oriented more N-S, traversing the Danakil Depression. These two rift branches account for the full Arabia-Nubia relative motion. The partitioning of extension between rift branches varies approximately linearly along strike; north of similar to 16 degrees N latitude, extension (similar to 15 mm/yr) is all on the main Red Sea Rift while at similar to 13 degrees N, extension (similar to 20 mm/yr) has transferred completely to the Danakil Depression. The Danakil Block separates the two rifts and rotates in a counterclockwise sense with respect to Nubia at a present-day rate of 1.9 +/- 0.1 degrees/Myr around a pole located at 17.0 +/- 0.2 degrees N, 39.7 +/- 0.2 degrees E, accommodating extension along the rifts and developing the roughly triangular geometry of the Danakil Depression. Rotating the Danakil Block back in time to close the Danakil Depression, and assuming that the rotation rate with respect to Nubia has been roughly constant, the present width of the Danakil Depression is consistent with initiation of block rotation at 9.3 +/- 4 Ma, approximately coincident with the initiation of ocean spreading in the Gulf of Aden, and a concomitant similar to 70% increase in the rate of Nubia-Arabia relative motion.</description> <date>2010</date> </dc> </metadata> </record> </GetRecord> </OAI-PMH>