Early cretaceous absolute geomagnetic paleointensities from Cordoba Province (Argentina)

We present here new paleointensity and geochronology results from Early Cretaceous volcanic rocks of Sierra Chica de Cordoba (Argentina). The new K-Ar isotopic ages of 5 samples range from 136 to 122 Ma. Twenty five samples from 7 individual flows yielded acceptable paleointensity estimates. The mea...

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Detalles Bibliográficos
Autores: Ruiz, RC, Goguitchaichvili, A, Geuna, SE, Alva-Valdivia, LM, Sole, J, Morales, J
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2006
País:México
Institución:Universidad Nacional Autónoma de México
Repositorio:Sistema de Información de la Facultad de Ciencias, UNAM
OAI Identifier:oai:repositorio.fciencias.unam.mx:11154/2315
Acceso en línea:http://hdl.handle.net/11154/2315
Access Level:acceso abierto
Palabra clave:Geosciences, Multidisciplinary
paleointensity
rock-magnetism
Early Cretaceous
South America
Descripción
Sumario:We present here new paleointensity and geochronology results from Early Cretaceous volcanic rocks of Sierra Chica de Cordoba (Argentina). The new K-Ar isotopic ages of 5 samples range from 136 to 122 Ma. Twenty five samples from 7 individual flows yielded acceptable paleointensity estimates. The mean paleointensity values per flow are ranging from 53.0 +/- 1.9 to 25.4 +/- 2.6 mu T and the corresponding Virtual Dipole Moments (VDMs) are ranging, from 9.3 +/- 1.3 to 4.6 +/- 0.5 (10(22) Am-2). This corresponds to the mean value of 7.3 +/- 1.7 x 10(22) Am-2, which is compatible to the present geomagnetic axial dipole. Currently available selected paleointensity data from 80 to 130 Ma suggest that geomagnetic field strength frequently fluctuated before and during the Cretaceous Normal Superchron while the magnetic polarity maintained stable. The mean paleointensities derived from Cordoba lavas agree remarkably well with those obtained from the Parana Magmatic Province (133-132 Ma). This reinforces the hypothesis about the unreliability of 'Mesozoic Dipole Low'.