Paleomagnetism of Upper Triassic rocks in the Los Colorados hill section, Mendoza province, Argentina

Different authors have highlighted a systematic disagreement between Late Carboniferous-Triassic paleomagnetic poles (PPs) for Gondwanaland and Laurasia when they are repositioned in a classical reconstruction prior to the breakup of Pangea A. This disagreement has been interpreted in geodynamic ter...

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Autor principal: Vizán, H.
Otros Autores: Ixer, R., Turner, P., Cortés, J.M, Cladera, G.
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Publicado: 2004
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100 1 |a Vizán, H. 
245 1 0 |a Paleomagnetism of Upper Triassic rocks in the Los Colorados hill section, Mendoza province, Argentina 
260 |c 2004 
270 1 0 |m Vizán, H.; CONICET, Departamento de Ciencias Geologicas, Universidad de Buenos Aires, Pabellón 2, Buenos Aires 1428, Argentina; email: haroldo@gl.fcen.uba.ar 
506 |2 openaire  |e Política editorial 
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520 3 |a Different authors have highlighted a systematic disagreement between Late Carboniferous-Triassic paleomagnetic poles (PPs) for Gondwanaland and Laurasia when they are repositioned in a classical reconstruction prior to the breakup of Pangea A. This disagreement has been interpreted in geodynamic terms or as an evidence of non-dipole components of the geomagnetic field. Such analyses have been made using data on South American PPs published approximately 25 years ago and obtained using outdated methodologies. In this article, the authors present new Late Triassic paleomagnetic data from rocks that crop out in the Pre-Andean ranges (Precordillera) of Mendoza province (Argentina). Samples of different lithologies were taken from two limbs of a doubly plunging syncline, and several field tests of paleomagnetic stability were applied. The results indicate primary site mean directions that yield a PP with geographic coordinates and statistical parameters as follows: Lat.=76°S, Lon.=280°E, N=12, R=11.63, α95=8°, K=30.2. This PP agrees with mean PPs of Laurasia of similar ages in different models of Pangea A, indicating that the hypothesis of a dipolar paleomagnetic field could be valid for the Late Triassic. © 2004 Elsevier Ltd. All rights reserved.  |l eng 
536 |a Detalles de la financiación: Universidad de Buenos Aires 
536 |a Detalles de la financiación: Consejo Nacional de Investigaciones Científicas y Técnicas 
536 |a Detalles de la financiación: University of Birmingham 
536 |a Detalles de la financiación: We thank the Universidad de Buenos Aires, the University of Birmingham and CONICET (Consejo Nacional de Investigaciones Científicas y Técnicas) for financial support of the research. Dr J. Genise helped us during the fieldwork. Special thanks to Drs R. Somoza, S.E. Geuna, C. Marcicano (U.B.A.) for help with a revision of a prevous version of this paper. H.V. is in debt to the research staff of the ‘old'School of Earth Sciences of the University of Birmingham. The careful reviews by Drs D. Tarling and A. Rapalini, are appreciated. 
593 |a CONICET, Departamento de Ciencias Geologicas, Universidad de Buenos Aires, Pabellón 2, Buenos Aires 1428, Argentina 
593 |a School of Earth Sciences, The University of Birmingham, Edgbaston, Birmingham B15 2TT, United Kingdom 
593 |a CONICET, Museo Paleontologico Egidio Feruglio, Avenida Fontana 140, 9100 Trelew, Chubut, Argentina 
651 4 |a ARGENTINA 
651 4 |a ARGENTINA 
651 4 |a MENDOZA 
651 4 |a SOUTH AMERICA 
690 1 0 |a LATE TRIASSIC 
690 1 0 |a PALEOMAGNETISM 
690 1 0 |a PANGEA 
690 1 0 |a PRECORDILLERA 
690 1 0 |a PALEOMAGNETISM 
690 1 0 |a PANGAEA 
690 1 0 |a POLAR WANDERING 
690 1 0 |a TRIASSIC 
690 1 0 |a PRECORDILLERA 
690 1 0 |a WESTERN HEMISPHERE 
690 1 0 |a WORLD 
700 1 |a Ixer, R. 
700 1 |a Turner, P. 
700 1 |a Cortés, J.M. 
700 1 |a Cladera, G. 
773 0 |d 2004  |g v. 18  |h pp. 41-59  |k n. 1  |p J. South Am. Earth Sci.  |x 08959811  |w (AR-BaUEN)CENRE-1080  |t Journal of South American Earth Sciences 
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