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dc.date.accessioned2017-09-24T12:38:57Z
dc.date.available2017-09-24T12:38:57Z
dc.date.created2017-09-18T14:53:58Z
dc.date.issued2017
dc.identifier.citationShephard, Grace Elizabeth Matthews, Kara J. Hosseini, Kasra Domeier, Mathew . On the consistency of seismically imaged lower mantle slabs. Scientific Reports. 2017, 7
dc.identifier.urihttp://hdl.handle.net/10852/58513
dc.description.abstractThe geoscience community is increasingly utilizing seismic tomography to interpret mantle heterogeneity and its links to past tectonic and geodynamic processes. To assess the robustness and distribution of positive seismic anomalies, inferred as subducted slabs, we create a set of vote maps for the lower mantle with 14 global P-wave or S-wave tomography models. Based on a depth-dependent threshold metric, an average of 20% of any given tomography model depth is identified as a potential slab. However, upon combining the 14 models, the most consistent positive wavespeed features are identified by an increasing vote count. An overall peak in the most robust anomalies is found between 1000–1400 km depth, followed by a decline to a minimum around 2000 km. While this trend could reflect reduced tomographic resolution in the middle mantle, we show that it may alternatively relate to real changes in the time-dependent subduction flux and/or a mid-lower mantle viscosity increase. An apparent secondary peak in agreement below 2500 km depth may reflect the degree-two lower mantle slow seismic structures. Vote maps illustrate the potential shortcomings of using a limited number or type of tomography models and slab threshold criteria.en_US
dc.languageEN
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleOn the consistency of seismically imaged lower mantle slabsen_US
dc.typeJournal articleen_US
dc.creator.authorShephard, Grace Elizabeth
dc.creator.authorMatthews, Kara J.
dc.creator.authorHosseini, Kasra
dc.creator.authorDomeier, Mathew
cristin.unitcode185,15,22,40
cristin.unitnameSenter for Jordens utvikling og dynamikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1494896
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Scientific Reports&rft.volume=7&rft.spage=&rft.date=2017
dc.identifier.jtitleScientific Reports
dc.identifier.volume7
dc.identifier.doihttp://dx.doi.org/10.1038/s41598-017-11039-w
dc.identifier.urnURN:NBN:no-61230
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn2045-2322
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/58513/1/Shephard_etal_2017_slab_vote_maps_Scientific_Reports.pdf
dc.type.versionPublishedVersion
cristin.articleid10976


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