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- W3205362069 endingPage "464" @default.
- W3205362069 startingPage "445" @default.
- W3205362069 abstract "Congo and São Francisco cratons are made of several Archean and Paleoproterozoic nuclei welded together by Paleoproterozoic belts. The pair is considered to be a stable lithospheric entity by ~2.0 Ga and hosts fissural mafic magmatism at 2.7–2.6, 1.71, 1.50, and 0.92 Ga; magmatic events at 1.38 and 1.10 Ga are restricted to Africa. Some of these dike swarms and also younger sedimentary units have been targeted for paleomagnetic studies, but the paleomagnetic data for the Congo−São Francisco craton is still scarce. Here we review the available data for both cratons. A total of 21 paleomagnetic poles was selected for paleogeographic reconstructions, 11 of them with Q-index higher than 4. Segments of apparent wander paths were drawn for 1.1–0.92, 0.79–0.74, and 0.57–0.52 Ga. Tentative reconstructions are proposed to place Congo−São Francisco into the context of supercontinents Columbia, Rodinia, and Gondwana." @default.
- W3205362069 created "2021-10-25" @default.
- W3205362069 creator A5013480617 @default.
- W3205362069 creator A5013974971 @default.
- W3205362069 creator A5062852745 @default.
- W3205362069 creator A5069923836 @default.
- W3205362069 date "2021-01-01" @default.
- W3205362069 modified "2023-10-18" @default.
- W3205362069 title "The Precambrian drift history and paleogeography of Congo−São Francisco craton" @default.
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