3 years ago

Magnetostratigraphy and mid‐palaeolatitude VGP dispersion during the Permo‐Carboniferous Superchron: results from Paraná Basin (Southern Brazil) rhythmites


A detailed magnetostratigraphic and rock‐magnetism study of two Late Palaeozoic rhythmite exposures (Itu and Rio do Sul) from the Itararé Group (Paraná Basin, Brazil) is presented in this paper. After stepwise alterning‐field procedures and thermal cleaning were performed, samples from both collections show reversed characteristic magnetization components, which is expected for Late Palaeozoic rocks. However, the Itu rocks presented an odd, flat inclination pattern that could not be corrected with mathematical methods based on the virtual geomagnetic pole (VGP) distributions. Correlation tests between the maximum anisotropy of the magnetic susceptibility axis (K1) and the magnetic declination indicated a possible mechanical influence on the remanence acquisition. The Rio do Sul sequence displayed medium to high inclinations and provided a high‐quality palaeomagnetic pole (after shallowing corrections of f = 0.8) of 347.5°E 63.2°S (N = 119; A95 = 3.3; K = 31), which is in accordance with the Palaeozoic apparent wander pole path of South America.

The angular dispersion (Sb) for the distribution of the VGPs calculated on the basis of both the 45° cut‐off angle and Vandamme method was compared to the best‐fit Model G for mid‐latitudes. Both of the Sb results are in reasonable agreement with the predicted (palaeo) latitudinal S‐λ relationship during the Cretaceous Normal Superchron (CNS), although the Sb value after the Vandamme cut‐off has been applied is a little lower than expected. This result, in addition to those for low palaeolatitudes during the Permo‐Carboniferous Reversed Superchron (PCRS) previously reported, indicates that the low secular variation regime for the geodynamo that has already been discovered in the CNS might have also been predominant during the PCRS.

Publisher URL: https://onlinelibrary.wiley.com/doi/abs/10.1111/j.1365-246X.2012.05670.x

DOI: 10.1111/j.1365-246X.2012.05670.x

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