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Remagnetizations in late Permian and early triassic rocks from southern Africa and their implications for Pangea reconstructions

dc.contributor.authorBallard, Martha M.en_US
dc.contributor.authorVan der Voo, Roben_US
dc.contributor.authorHalbich, Ingo W.en_US
dc.date.accessioned2006-04-07T19:27:06Z
dc.date.available2006-04-07T19:27:06Z
dc.date.issued1986-09en_US
dc.identifier.citationBallard, Martha M., Van der Voo, Rob, Halbich, I. W. (1986/09)."Remagnetizations in late Permian and early triassic rocks from southern Africa and their implications for Pangea reconstructions." Earth and Planetary Science Letters 79(3-4): 412-418. <http://hdl.handle.net/2027.42/26063>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V61-4B4RR06-K/2/98e7c8943b959b35719dc9d622e5d2c1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/26063
dc.description.abstractA paleomagnetic study of late Paleozoic and early Mesozoic sedimentary rocks from southern Africa suggests wide-spread remagnetization of these rocks. Samples of the Mofdiahogolo Formation in Botswana and of the Lower Beaufort Group in South Africa were treated using thermal, alternating field and chemical demagnetization. The Mofdiahogolo redbeds show a univectoral decay of the remanence revealing a characteristic direction of D = 340[deg], I = -58[deg], K = 64, [alpha]95 = 12[deg]. The Lower Beaufort sandstones, using thermal and alternating field demagnetization, show a very similar direction of D = 337[deg], I = -63[deg], K = 91, [alpha]95 = 6[deg]. A fold test on the Beaufort rocks is negative indicating that this magnetization is secondary and acquired after the Permo-Triassic Cape Belt folding event. Previous studies have reported similar directions in the. Upper Beaufort redbeds as well as in the Kenyan Maji ya Chumvi Formation of Early Triassic age. The poles of these studies have been used in testing the validity of the various Pangea reconstructions for the Late Permian and the Early Triassic. Our results suggest that these poles may also be based on remagnetized data and that their use to document the position of Gondwana in Pangea reconstructions should be treated with caution.en_US
dc.format.extent622951 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleRemagnetizations in late Permian and early triassic rocks from southern Africa and their implications for Pangea reconstructionsen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelGeology and Earth Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Geological Sciences, University of Michigan, Ann Arbor, MI 48109, U.S.A.en_US
dc.contributor.affiliationumDepartment of Geological Sciences, University of Michigan, Ann Arbor, MI 48109, U.S.A.en_US
dc.contributor.affiliationotherDepartment of Geology, University of Stellenbosch, Stellenbosch,, Republic of South Africaen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/26063/1/0000137.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0012-821X(86)90196-2en_US
dc.identifier.sourceEarth and Planetary Science Lettersen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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