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Revision of the age of magnetization of the Montmartin red beds, Normandy, France

dc.contributor.authorPerroud, Herveen_US
dc.contributor.authorRobardet, M.en_US
dc.contributor.authorVoo, Rob Van deren_US
dc.contributor.authorBonhommet, Norberten_US
dc.contributor.authorParis, F.en_US
dc.date.accessioned2010-06-01T21:40:19Z
dc.date.available2010-06-01T21:40:19Z
dc.date.issued1985-02en_US
dc.identifier.citationPerroud, H.; Robardet, M.; Voo, R.; Bonhommet, N.; Paris, F. (1985). "Revision of the age of magnetization of the Montmartin red beds, Normandy, France." Geophysical Journal of the Royal Astronomical Society 80(2): 541-549. <http://hdl.handle.net/2027.42/74719>en_US
dc.identifier.issn0016-8009en_US
dc.identifier.issn1365-246Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/74719
dc.description.abstractA new roadcut has enabled us to sample the south-dipping limb of the Montmartin syncline for a palaeomagnetic reevaluation of an earlier result published by Jones, Van der Voo & Bonhommet. In combination with the results previously published in 1979 for the north-dipping beds of the syncline, a conclusively negative fold test is obtained. The resulting magnetization (declination/inclination =206°/-3°, Α 95 = 12°, palaeopole at 38°S, 325°E) is interpreted to be of Late Carboniferous age, not Late Devonian as thought earlier. Simultaneously, we have re-evaluated the age of the rocks, previously thought to be Late Devonian on the basis of Acritarchs, Chitinozoans and spores. It has not been possible to reconfirm these fossils, not even in the same samples as studied originally; in contrast, the regional presence of Early Palaeozoic fossils suggests to us an age similar to that of other red beds in the Arrnorican Massif, which have been dated as Early Ordovician. The geodynamic implications of our finding that the Montmartin rocks are completely remagnetized, however, are of no great consequence for the geodynamics of the Hercynian belt. Pre-folding magnetization obtained from Silurian and Devonian rocks in Spain and Germany argue for the same conclusion as reached erroneously in our earlier study, namely that the Armorican Massif and adjacent parts of Hercynian Europe were adjointed to North America, Great Britain, the Baltic Shield and the Russian Platform since at least Late Devonian time. If a Medio-European ocean existed during the Palaeozoic, it was virtually closed before the mid-Devonian and of insignificant width during Culm deposition in Early Carboniferoirs time.en_US
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dc.format.extent3109 bytes
dc.format.mimetypeapplication/pdf
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dc.publisherBlackwell Publishing Ltden_US
dc.rights1985 Royal Astronomical Societyen_US
dc.titleRevision of the age of magnetization of the Montmartin red beds, Normandy, Franceen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbsecondlevelGeology and Earth Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Geological Sciences, the University of Michigan, Ann Arbor, MI 48109, USA and Laboratoire de GÉophysique Interne (LP 4661 du CNRS), Institut de GÉologie, UniversitÉ de Rennes, Avenue du GÉnÉral-Leclerc, 35042 Rennes-CÉdex, Franceen_US
dc.contributor.affiliationumDepartment of Geological Sciences, the University of Michigan, Ann Arbor, MI 48109. USAen_US
dc.contributor.affiliationotherLaboratoire de PalÉonto1ogie et Stratigraphie (GRECO 130007 du CNRS), Institut de GÉologie, UniversitÉ de Rennes, 35042 Relines-CÉdex, Franceen_US
dc.contributor.affiliationotherLaboratoire de GÉophysique Interne (LP 4661 du CNRs), Institut de GÉologie, UniversitÉ de Rennes, Avenue du GÉnÉral-Leclerc, 35042 Rennes-CÉdex, Franceen_US
dc.contributor.affiliationotherLaboratoire de PalÉontologie ef Stratigraphie (GRECO 130007 du CNRS), Institut de GÉologie, UniversitÉ de Rennes, 35042 Rennes-CÉdex, Franceen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/74719/1/j.1365-246X.1985.tb05108.x.pdf
dc.identifier.doi10.1111/j.1365-246X.1985.tb05108.xen_US
dc.identifier.sourceGeophysical Journal of the Royal Astronomical Societyen_US
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dc.owningcollnameInterdisciplinary and Peer-Reviewed


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