1887

Abstract

The sedimentary Rosário do Sul Formation (southern Brasil), believed to be of Late Triassic age was sampled<br>for paleomagnetic study from the in Rio Grande do Sul State of. In most sites both thermal and alternating field<br>demagnetization in 12-17 steps revealed either a reversed or normal characteristic remanent magnetization<br>(ChRM). Combining results yield 11 reversed (RSF-R) and 4 normal (RSF-N) magnetized sites and the later was<br>interpreted as a secondary magnetization. This secondary magnetization was acquired during Early Cretaceous<br>due to reheating or/and chemical remagnetization by the overlying thick sequences of the Serra Geral flood<br>(SGF) basalt. The mean primary paleomagnetic direction calculated using only 11 reversed polarity sites (RFSR)<br>yields, Dec=166.3°, Inc=35° (α95=5.9° and k=61), implying in a ~14° counter clockwise rotation in the<br>declination and a shallow inclination. The mean inclination is shallow as expected due to compaction of the<br>sediments by the overlying SGF basalt. The associated virtual geomagnetic pole is located at 71°E and 74°S.<br>The rotated virtual geomagnetic pole of the primary magnetization (RSF-R*) do not match other South American<br>poles of Triassic age. However, the rotated paleomagnetic pole (79.9°S, 127.13°E) is close to Middle- Late<br>Jurassic VGP's calculated on volcanic deposits in South America.

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/content/papers/10.3997/2214-4609-pdb.215.sbgf217
1999-08-15
2024-04-27
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