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dc.contributor.authorHuang, Wentao
dc.contributor.authorLippert, Peter C.
dc.contributor.authorJackson, Michael J.
dc.contributor.authorDekkers, Mark J.
dc.contributor.authorZhang, Yang
dc.contributor.authorLi, Juan
dc.contributor.authorGuo, Zhaojie
dc.contributor.authorKapp, Paul
dc.contributor.authorvan Hinsbergen, Douwe J. J.
dc.date.accessioned2017-04-07T00:58:45Z
dc.date.available2017-04-07T00:58:45Z
dc.date.issued2017-02
dc.identifier.citationRemagnetization of the Paleogene Tibetan Himalayan carbonate rocks in the Gamba area: Implications for reconstructing the lower plate in the India-Asia collision 2017, 122 (2):808 Journal of Geophysical Research: Solid Earthen
dc.identifier.issn21699313
dc.identifier.doi10.1002/2016JB013662
dc.identifier.urihttp://hdl.handle.net/10150/623053
dc.description.abstractThe characteristic remanent magnetization (ChRM) isolated from Paleogene carbonate rocks of the Zongpu Formation in Gamba (28.3 degrees N, 88.5 degrees(E) of southern Tibet has previously been interpreted to be primary. These data are pertinent for estimating the width of Greater India and dating the initiation of India-Asia collision. We have reanalyzed the published ChRM directions and completed thorough rock magnetic tests and petrographic observations on specimens collected throughout the previously investigated sections. Negative nonparametric fold tests demonstrate that the ChRM has a synfolding or postfolding origin. Rock magnetic analyses reveal that the dominant magnetic carrier is magnetite. "Wasp-waisted" hysteresis loops, suppressed Verwey transitions, high frequency-dependent in-phase magnetic susceptibility, and evidence that > 70% of the ferrimagnetic material is superparamagnetic at room temperature are consistent with the rock-magnetic fingerprint of remagnetized carbonate rocks. Scanning electron microscopy observations and energy-dispersive X-ray spectrometry analysis confirm that magnetite grains are authigenic. In summary, the carbonate rocks of the Zongpu Formation in Gamba have been chemically remagnetized. Thus, the early Paleogene latitude of the Tibetan Himalaya and size of Greater India have yet to be determined and the initiation of collision cannot yet be precisely dated by paleomagnetism. If collision began at 59 +/- 1 Ma at similar to 19 degrees N, as suggested by sedimentary records and paleomagnetic data from the Lhasa terrane, then a huge Greater India, as large as similar to 3500-3800 km, is required in the early Paleogene. This size, in sharp contrast to the few hundred kilometers estimated for the Early Cretaceous, implies an ever greater need for extension within Greater India during the Cretaceous.
dc.description.sponsorshipNetherlands Organization for Scientific Research (NWO) [825.15.016]; Institute for Rock Magnetism (IRM) at the University of Minnesota - Instruments and Facilities Program of NSFen
dc.language.isoenen
dc.publisherAMER GEOPHYSICAL UNIONen
dc.relation.urlhttp://doi.wiley.com/10.1002/2016JB013662en
dc.rights© 2017. American Geophysical Union. All Rights Reserved.en
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.titleRemagnetization of the Paleogene Tibetan Himalayan carbonate rocks in the Gamba area: Implications for reconstructing the lower plate in the India-Asia collisionen
dc.typeArticleen
dc.contributor.departmentUniv Arizona, Dept Geoscien
dc.identifier.journalJournal of Geophysical Research: Solid Earthen
dc.description.note6 month embargo; First published: 13 February 2017en
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en
dc.eprint.versionFinal published versionen
dc.contributor.institutionKey Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education, School of Earth and Space Sciences; Peking University; Beijing China
dc.contributor.institutionDepartment of Geology and Geophysics; University of Utah; Salt Lake City Utah USA
dc.contributor.institutionInstitute for Rock Magnetism, Department of Earth Sciences; University of Minnesota; Minneapolis Minnesota USA
dc.contributor.institutionDepartment of Earth Sciences; Utrecht University; Utrecht Netherlands
dc.contributor.institutionKey Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education, School of Earth and Space Sciences; Peking University; Beijing China
dc.contributor.institutionState Key Laboratory of Mineral Deposit Research, School of Earth Sciences and Engineering; Nanjing University; Nanjing China
dc.contributor.institutionKey Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education, School of Earth and Space Sciences; Peking University; Beijing China
dc.contributor.institutionDepartment of Geosciences; University of Arizona; Tucson Arizona USA
dc.contributor.institutionDepartment of Earth Sciences; Utrecht University; Utrecht Netherlands
refterms.dateFOA0017-08-14T00:00:00Z
html.description.abstractThe characteristic remanent magnetization (ChRM) isolated from Paleogene carbonate rocks of the Zongpu Formation in Gamba (28.3 degrees N, 88.5 degrees(E) of southern Tibet has previously been interpreted to be primary. These data are pertinent for estimating the width of Greater India and dating the initiation of India-Asia collision. We have reanalyzed the published ChRM directions and completed thorough rock magnetic tests and petrographic observations on specimens collected throughout the previously investigated sections. Negative nonparametric fold tests demonstrate that the ChRM has a synfolding or postfolding origin. Rock magnetic analyses reveal that the dominant magnetic carrier is magnetite. "Wasp-waisted" hysteresis loops, suppressed Verwey transitions, high frequency-dependent in-phase magnetic susceptibility, and evidence that > 70% of the ferrimagnetic material is superparamagnetic at room temperature are consistent with the rock-magnetic fingerprint of remagnetized carbonate rocks. Scanning electron microscopy observations and energy-dispersive X-ray spectrometry analysis confirm that magnetite grains are authigenic. In summary, the carbonate rocks of the Zongpu Formation in Gamba have been chemically remagnetized. Thus, the early Paleogene latitude of the Tibetan Himalaya and size of Greater India have yet to be determined and the initiation of collision cannot yet be precisely dated by paleomagnetism. If collision began at 59 +/- 1 Ma at similar to 19 degrees N, as suggested by sedimentary records and paleomagnetic data from the Lhasa terrane, then a huge Greater India, as large as similar to 3500-3800 km, is required in the early Paleogene. This size, in sharp contrast to the few hundred kilometers estimated for the Early Cretaceous, implies an ever greater need for extension within Greater India during the Cretaceous.


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