Paleomagnetism of the Carboniferous-Permian Patquía formation, Paganzo Basin, Argentina: Implications for the apparent polar wander path for South America and Gondwana during the late Palaeozoic

The magnetic properties of the Carboniferous-Permian red beds of the Patquía Formation at Punta del Viento, Sierra de Umango and some previously reported localities, all in the Paganzo Basin (Argentina) have been studied. Whereas all sites are characterized by hematite as the main magnetic carrier a...

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Autor principal: Geuna, S.E
Otros Autores: Escosteguy, L.D, Limarino, C.O
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Publicado: 2010
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100 1 |a Geuna, S.E. 
245 1 0 |a Paleomagnetism of the Carboniferous-Permian Patquía formation, Paganzo Basin, Argentina: Implications for the apparent polar wander path for South America and Gondwana during the late Palaeozoic 
260 |c 2010 
270 1 0 |m Geuna, S. E.; Departamento de Ciencias Geológicas, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires / CONICET, Ciudad Universitaria Pab. 2, C1428EHA, Ciudad de Buenos Aires, Argentina; email: geuna@gl.fcen.uba.ar 
506 |2 openaire  |e Política editorial 
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520 3 |a The magnetic properties of the Carboniferous-Permian red beds of the Patquía Formation at Punta del Viento, Sierra de Umango and some previously reported localities, all in the Paganzo Basin (Argentina) have been studied. Whereas all sites are characterized by hematite as the main magnetic carrier and a reversed-polarity magnetic remanence, we found a pattern of variation in magnetic properties along the integrated column for Patquía Formation. The Lower Member (Late Carboniferous) showed higher intensity of natural and saturation isothermal remanent magnetisation (NRM and SIRM, respectively) than the Permian Upper Member. The fall in NRM intensity from the Lower to Upper Member of the Patquía Formation may be related to a change in quantity and/ or grain-size of the hematite pigment, which may reflect the change in environmental and/or depositional setting. As for directional values of NRM, paleomagnetic poles reported for both sections are clearly different. The lower section provided a pole position coincident with Late Carboniferous poles for Gondwana, while the upper section poles are departed from the Early Permian position. We cannot decide whether the Upper Member pole is due to a primary magnetisation at 290 Ma or to a remagnetisation at ~260-270 Ma; even so, the obtained paleomagnetic pole is robust and indicates a rapid apparent polar wander in a ~30° counter clockwise rotation of the region, after deposition of the Late Carboniferous lower section, and in coincidence with the San Rafael Orogenic Phase.  |l eng 
593 |a Departamento de Ciencias Geológicas, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires / CONICET, Ciudad Universitaria Pab. 2, C1428EHA, Ciudad de Buenos Aires, Argentina 
593 |a Instituto de Geología y Recursos Minerales, Servicio Geológico Minero Argentino, Argentina 
690 1 0 |a APPARENT POLAR WANDER 
690 1 0 |a MAGNETIC REMANENCE 
690 1 0 |a PALEOMAGNETISM 
690 1 0 |a RED BEDS 
690 1 0 |a APPARENT POLAR WANDER PATH 
690 1 0 |a CARBONIFEROUS 
690 1 0 |a GONDWANA 
690 1 0 |a HEMATITE 
690 1 0 |a MAGNETIC REVERSAL 
690 1 0 |a PALEOMAGNETISM 
690 1 0 |a PERMIAN 
690 1 0 |a RED BED 
690 1 0 |a REMAGNETIZATION 
690 1 0 |a PAGANZO BASIN 
651 4 |a ARGENTINA 
700 1 |a Escosteguy, L.D. 
700 1 |a Limarino, C.O. 
773 0 |d 2010  |g v. 8  |h pp. 373-397  |k n. 4  |p Geol. Acta  |x 16956133  |w (AR-BaUEN)CENRE-8135  |t Geologica Acta 
856 4 1 |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-79551562902&doi=10.1344%2f105.000001578&partnerID=40&md5=8a98b4db29011baa6624e8d5fdf78a13  |y Registro en Scopus 
856 4 0 |u https://doi.org/10.1344/105.000001578  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_16956133_v8_n4_p373_Geuna  |y Handle 
856 4 0 |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_16956133_v8_n4_p373_Geuna  |y Registro en la Biblioteca Digital 
961 |a paper_16956133_v8_n4_p373_Geuna  |b paper  |c PE 
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999 |c 68359