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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>2018-01-15T18:31:49Z</responseDate> <request identifier=oai:HAL:hal-00941025v1 verb=GetRecord metadataPrefix=oai_dc>http://api.archives-ouvertes.fr/oai/hal/</request> <GetRecord> <record> <header> <identifier>oai:HAL:hal-00941025v1</identifier> <datestamp>2018-01-12</datestamp> <setSpec>type:ART</setSpec> <setSpec>subject:sdu</setSpec> <setSpec>subject:sde</setSpec> <setSpec>collection:CNRS</setSpec> <setSpec>collection:SDE</setSpec> <setSpec>collection:GM</setSpec> <setSpec>collection:GIP-BE</setSpec> <setSpec>collection:UNIV-ST-ETIENNE</setSpec> <setSpec>collection:INSU</setSpec> <setSpec>collection:UNIV-BPCLERMONT</setSpec> <setSpec>collection:LMV</setSpec> <setSpec>collection:AGROPOLIS</setSpec> <setSpec>collection:PRES_CLERMONT</setSpec> <setSpec>collection:B3ESTE</setSpec> <setSpec>collection:UNIV-AG</setSpec> <setSpec>collection:UNIV-MONTPELLIER</setSpec> <setSpec>collection:OPGC</setSpec> </header> <metadata><dc> <publisher>HAL CCSD</publisher> <title lang=en>Nickel and helium evidence for melt above the core-mantle boundary</title> <creator>Herzberg, Claude</creator> <creator>Asimow, Paul D.</creator> <creator>IONOV, Dmitri</creator> <creator>Vidito, Chris</creator> <creator>Jackson, Matthew G.</creator> <creator>Geist, Dennis</creator> <contributor>Department of Earth and Planetary Sciences [Piscataway] ; Rutgers, The State University of New Jersey [New Brunswick] (RUTGERS)</contributor> <contributor>California Institute of Technology (CALTECH)</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>Laboratoire Magmas et Volcans (LMV) ; Université Blaise Pascal - Clermont-Ferrand 2 (UBP) - Institut national des sciences de l'Univers (INSU - CNRS) - Université Jean Monnet [Saint-Étienne] (UJM) - Centre National de la Recherche Scientifique (CNRS)</contributor> <contributor>Department of Earth and Environment, Boston University ; Boston University [Boston] (BU)</contributor> <contributor>Department of Geological Sciences, University of Idaho ; Université du Québec</contributor> <description>International audience</description> <source>ISSN: 0028-0836</source> <source>EISSN: 1476-4679</source> <source>Nature</source> <publisher>Nature Publishing Group</publisher> <identifier>hal-00941025</identifier> <identifier>https://hal.archives-ouvertes.fr/hal-00941025</identifier> <source>https://hal.archives-ouvertes.fr/hal-00941025</source> <source>Nature, Nature Publishing Group, 2013, 493 (7432), pp.393-U134. 〈10.1038/nature11771〉</source> <identifier>DOI : 10.1038/nature11771</identifier> <relation>info:eu-repo/semantics/altIdentifier/doi/10.1038/nature11771</relation> <language>en</language> <subject lang=it>petrology</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>High 3He/4He ratios in some basalts have generally been interpreted as originating in an incompletely degassed lower-mantle source1, 2, 3, 4, 5, 6, 7, 8, 9. This helium source may have been isolated at the core-mantle boundary region since Earth's accretion4, 5, 6. Alternatively, it may have taken part in whole-mantle convection and crust production over the age of the Earth7, 8, 9; if so, it is now either a primitive refugium at the core-mantle boundary8 or is distributed throughout the lower mantle7, 9. Here we constrain the problem using lavas from Baffin Island, West Greenland, the Ontong Java Plateau, Isla Gorgona and Fernandina (Galapagos). Olivine phenocryst compositions show that these lavas originated from a peridotite source that was about 20 per cent higher in nickel content than in the modern mid-ocean-ridge basalt source. Where data are available, these lavas also have high 3He/4He. We propose that a less-degassed nickel-rich source formed by core-mantle interaction during the crystallization of a melt-rich layer or basal magma ocean5, 6, and that this source continues to be sampled by mantle plumes. The spatial distribution of this source may be constrained by nickel partitioning experiments at the pressures of the core-mantle boundary.</description> <date>2013-01-17</date> </dc> </metadata> </record> </GetRecord> </OAI-PMH>