| 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 (0.78-0.0 Ma) age, and thus assign it to the Matuyama Chron (2.58-0.78 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.
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											Authors
												Th.E. Wong, R. de Kramer, P.L. de Boer, C. Langereis, J. Sew-A-Tjon, 
											