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dc.contributor.authorBeasley, C.
dc.contributor.authorKender, S.
dc.contributor.authorGiosan, L.
dc.contributor.authorBolton, C.T.
dc.contributor.authorAnand, P.
dc.contributor.authorLeng, M.J.
dc.contributor.authorNilsson-Kerr, Katrina
dc.contributor.authorUllmann, Clemens V.
dc.contributor.authorHesselbo, Stephen P.
dc.contributor.authorLittler, Kate
dc.date.accessioned2022-04-04T11:42:14Z
dc.date.available2022-04-04T11:42:14Z
dc.date.created2022-02-03T15:33:03Z
dc.date.issued2021
dc.identifier.issn2572-4517
dc.identifier.urihttps://hdl.handle.net/11250/2989590
dc.description.abstractThe geological history of the South Asian monsoon (SAM) before the Pleistocene is not well-constrained, primarily due to a lack of available continuous sediment archives. Previous studies have noted an intensification of SAM precipitation and atmospheric circulation during the middle Miocene (∼14 Ma), but no records are available to test how the monsoon changed prior to this. In order to improve our understanding of monsoonal evolution, geochemical and sedimentological data were generated for the Oligocene-early Miocene (30–20 Ma) from Indian National Gas Hydrate Expedition 01 Site NGHP-01-01A in the eastern Arabian Sea, at 2,674 m water depth. We find the initial glaciation phase (23.7–23.0 Ma) of the Oligocene-Miocene transition (OMT) to be associated with an increase in water column ventilation and water mass mixing, suggesting an increase in winter monsoon type atmospheric circulation, possibly driven by a relative southward shift of the intertropical convergence zone. During the latter part of the OMT, or “deglaciation” phase (23.0–22.7 Ma), a long-term decrease in Mn (suggestive of deoxygenation), increase in Ti/Ca and dissolution of the biogenic carbonate fraction suggest an intensification of a proto-summer SAM system, characterized by the formation of an oxygen minimum zone in the eastern Arabian Sea and a relative increase of terrigenous material delivered by runoff to the site. With no evidence at this site for an active SAM prior to the OMT we suggest that changes in orbital parameters, as well as possibly changing Tethyan/Himalayan tectonics, caused this step change in the proto-monsoon system at this intermediate-depth site.en_US
dc.language.isoengen_US
dc.publisherWileyen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleEvidence of a South Asian Proto-Monsoon During the Oligocene-Miocene Transitionen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2021. The Authorsen_US
dc.source.articlenumbere2021PA004278en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.doi10.1029/2021PA004278
dc.identifier.cristin1997488
dc.source.journalPaleoceanography and Paleoclimatologyen_US
dc.identifier.citationPaleoceanography and Paleoclimatology. 2021, 36 (9), e2021PA004278.en_US
dc.source.volume36en_US
dc.source.issue9en_US


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Navngivelse 4.0 Internasjonal
Except where otherwise noted, this item's license is described as Navngivelse 4.0 Internasjonal