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dc.contributor.authorPisarevsky, Sergei
dc.contributor.authorGladkochub, D.
dc.contributor.authorKonstantinov, K.
dc.contributor.authorMazukabzov, A.
dc.contributor.authorStanevich, A.
dc.contributor.authorMurphy, J.
dc.contributor.authorTait, J.
dc.contributor.authorDonskaya, T.
dc.contributor.authorKonstantinov, I.
dc.date.accessioned2017-01-30T12:19:04Z
dc.date.available2017-01-30T12:19:04Z
dc.date.created2014-02-25T20:00:40Z
dc.date.issued2013
dc.identifier.citationPisarevsky, Sergei A. and Gladkochub, Dmitry P. and Konstantinov, Konstantine M. and Mazukabzov, Anatoly M. and Stanevich, Arkady M. and Murphy, J. Brendan and Tait, Jennifer A. and Donskaya, Tatiana V. and Konstantinov, Innokenty K. 2013. Paleomagnetism of Cryogenian Kitoi mafic dykes in South Siberia: Implications for Neoproterozoic paleogeography. Precambrian Research. 231: pp. 372-382.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/20414
dc.identifier.doi10.1016/j.precamres.2013.04.007
dc.description.abstract

We present a new paleomagnetic pole of 1.1°N, 22.4°E, A95 = 7.4° from the 760 Ma gabbro-dolerite Kitoi dykes located in the southern part of the Siberian Craton. The pole is supported by contact tests and suggests closer position of Siberia relative to Laurentia at 760 Ma than in Mesoproterozoic. We propose that this closer configuration was achieved by dextral transpressive motion of Siberia relative to Laurentia between 780 and 760 Ma. This motion was probably initiated at the first stage of the Rodinia breakup and is coeval with the 780 Ma Gunbarrel magmatic event of the western Canadian shield.

dc.publisherElsevier BV
dc.subjectPaleomagnetism
dc.subjectMafic dykes
dc.subjectRodinia
dc.subjectSiberian Craton
dc.subjectCryogenian
dc.subjectNeoproterozoic
dc.titlePaleomagnetism of Cryogenian Kitoi mafic dykes in South Siberia: Implications for Neoproterozoic paleogeography
dc.typeJournal Article
dcterms.source.volume231
dcterms.source.startPage372
dcterms.source.endPage382
dcterms.source.issn0301-9268
dcterms.source.titlePrecambrian Research
curtin.note

NOTICE: This is the author’s version of a work that was accepted for publication in Precambrian Research. Changes resulting from the publishing process, such as peer review, editing, corrections, structural formatting, and other quality control mechanisms may not be reflected in this document. Changes may have been made to this work since it was submitted for publication. A definitive version was subsequently published in Precambrian Research, Vol. 231 (2013). doi: 10.1016/j.precamres.2013.04.007

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curtin.accessStatusOpen access


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