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dc.date.accessioned2021-04-29T19:43:19Z
dc.date.available2021-04-29T19:43:19Z
dc.date.created2021-03-16T17:02:36Z
dc.date.issued2020
dc.identifier.citationXia, Bing Thybo, Hans Artemieva, Irina M. . Lithosphere Mantle Density of the North China Craton. Journal of Geophysical Research (JGR): Solid Earth. 2020, 125(9)
dc.identifier.urihttp://hdl.handle.net/10852/85739
dc.description.abstractWe constrain the lithospheric mantle density of the North China Craton (NCC) at both in situ and standard temperature‐pressure (STP) conditions from gravity data. The lithosphere‐asthenosphere boundary (LAB) depth is constrained by our new thermal model, which is based on a new regional heat flow data set and a recent regional crustal model NCcrust. The new thermal model shows that the thermal lithosphere thickness is <120 km in most of the NCC, except for the northern and southern parts with the maximum depth of 170 km. The gravity calculations reveal a highly heterogeneous density structure of the lithospheric mantle with in situ and STP values of 3.22–3.29 and 3.32–3.40 g/cm3, respectively. Thick and reduced‐density cratonic‐type lithosphere is preserved mostly in the southern NCC. Most of the Eastern Block has a thin (90–140 km) and high‐density lithospheric mantle. Most of the Western Block has a high‐density lithospheric mantle and a thin (80–110 km) lithosphere typical of Phanerozoic regions, which suggests that the Archean lithosphere is no longer present there. We conclude that in almost the entire NCC the lithosphere has lost its cratonic characteristics by geodynamic processes that include, but are not limited to, the Paleozoic closure of the Paleo‐Asian Ocean in the north, the Mesozoic Yangtze Craton flat subduction in the south, the Mesozoic Pacific subduction in the east, the Cenozoic remote response to the Indian‐Eurasian collision in the west, and the Cenozoic extensional tectonics (possibly associated with the slab roll‐back) in the center.
dc.languageEN
dc.titleLithosphere Mantle Density of the North China Craton
dc.typeJournal article
dc.creator.authorXia, Bing
dc.creator.authorThybo, Hans
dc.creator.authorArtemieva, Irina M.
cristin.unitcode185,15,22,40
cristin.unitnameSenter for Jordens utvikling og dynamikk
cristin.ispublishedtrue
cristin.fulltextpostprint
cristin.qualitycode2
dc.identifier.cristin1898453
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Journal of Geophysical Research (JGR): Solid Earth&rft.volume=125&rft.spage=&rft.date=2020
dc.identifier.jtitleJournal of Geophysical Research (JGR): Solid Earth
dc.identifier.volume125
dc.identifier.issue9
dc.identifier.pagecount23
dc.identifier.doihttps://doi.org/10.1029/2020JB020296
dc.identifier.urnURN:NBN:no-88403
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn2169-9313
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/85739/5/2020JB020296.pdf
dc.type.versionPublishedVersion
cristin.articleide2020JB020


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