Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
4690481 | Sedimentary Geology | 2009 | 13 Pages |
Abstract
Palaeomagnetic data indicate a dominantly reversed magnetic polarity in the Para Member, whereas the Lelydorp Member shows a normal magnetic polarity with a minor reversed polarity overprint. The reversed polarities of the Para Member exclude a Brunhes Chron (0.78-0.0Â Ma) age, and thus assign it to the Matuyama Chron (2.58-0.78Â Ma). This implies that the Coropina Formation is much older than hitherto assumed, and that one or more (long-term) hiatuses are not recognizable in the lithological succession.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Earth-Surface Processes
Authors
Th.E. Wong, R. de Kramer, P.L. de Boer, C. Langereis, J. Sew-A-Tjon,