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dc.date.accessioned2018-04-11T14:18:40Z
dc.date.available2018-04-11T14:18:40Z
dc.date.created2017-12-12T11:19:42Z
dc.date.issued2017
dc.identifier.citationConrad, Clinton Phillips Selway, K. Hirschmann, M.M. Ballmer, M.D. Wessel, P. . Constraints on volumes and patterns of asthenospheric melt from the space-time distribution of seamounts. Geophysical Research Letters. 2017, 44(14), 7203-7210
dc.identifier.urihttp://hdl.handle.net/10852/61508
dc.description.abstractAlthough partial melt in the asthenosphere is important geodynamically, geophysical constraints on its abundance remain ambiguous. We use a database of seamounts detected using satellite altimetry to constrain the temporal history of erupted asthenospheric melt. We find that intraplate volcanism on young seafloor (<60 Ma) equates to a ~20 m thick layer spread across the seafloor. If these seamounts tap partial melt within a ~20 km thick layer beneath the ridge flanks, they indicate extraction of an average melt fraction of ~0.1%. If they source thinner layers or more laterally restricted domains, larger melt fractions are required. Increased seamount volumes for older lithosphere suggest either more active ridge flank volcanism during the Cretaceous or additional recent melt eruption on older seafloor. Pacific basin age constraints suggest that both processes are important. Our results indicate that small volumes of partial melt may be prevalent in the upper asthenosphere across ocean basins. This article was originally published in Geophysical Research Letters. © 2017 American Geophysical Unionen_US
dc.languageEN
dc.publisherAmerican Geophysical Union
dc.titleConstraints on volumes and patterns of asthenospheric melt from the space-time distribution of seamountsen_US
dc.typeJournal articleen_US
dc.creator.authorConrad, Clinton Phillips
dc.creator.authorSelway, K.
dc.creator.authorHirschmann, M.M.
dc.creator.authorBallmer, M.D.
dc.creator.authorWessel, P.
cristin.unitcode185,15,22,40
cristin.unitnameSenter for Jordens utvikling og dynamikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1526167
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Geophysical Research Letters&rft.volume=44&rft.spage=7203&rft.date=2017
dc.identifier.jtitleGeophysical Research Letters
dc.identifier.volume44
dc.identifier.issue14
dc.identifier.startpage7203
dc.identifier.endpage7210
dc.identifier.doihttp://dx.doi.org/10.1002/2017GL074098
dc.identifier.urnURN:NBN:no-64118
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0094-8276
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/61508/4/Conrad_et_al-2017-Geophysical_Research_Letters.pdf
dc.type.versionPublishedVersion
dc.relation.projectNFR/223272


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