1999
DOI: 10.1016/s0301-9268(99)00024-8
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The metamorphic evolution of the Paleoproterozoic (Birimian) volcanic Ashanti belt (Ghana, West Africa)

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Cited by 99 publications
(72 citation statements)
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References 33 publications
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“…These values are also comparable to a Belt-type granite sample reported in John et al (1999), with 3.59 wt% CaO, 4.58 wt% Na 2 O, 1.89 wt% K 2 O, and 50 ppm Rb. The published CaO content of this Belt-type sample is, thus, far higher than the CaO contents of the samples analyzed here.…”
Section: Granite Classification and Provenancesupporting
confidence: 86%
“…These values are also comparable to a Belt-type granite sample reported in John et al (1999), with 3.59 wt% CaO, 4.58 wt% Na 2 O, 1.89 wt% K 2 O, and 50 ppm Rb. The published CaO content of this Belt-type sample is, thus, far higher than the CaO contents of the samples analyzed here.…”
Section: Granite Classification and Provenancesupporting
confidence: 86%
“…These are too small in size to have been the major source of supply for such a large basin as the LGB protolith. Larger occurrences of silicic igneous rocks as well as signs of high-grade metamorphism of this age group are found elsewhere on the Earth, especially in South America in the Transamazonian belts and related belts in Western and Central Africa (Dada, 1998;Feybesse et al, 1998;Hartmann et al, 1999;John et al, 1999;Norcross et al, 2000;Plá Cid et al, 2000;Nomade et al, 2002). Also, larger occurrences of this age group are found in Eastern Asia in Korea and the North China Craton (Cheong et al, 2000;Zhao et al, 2000).…”
Section: Tectonic Consequences and Correlationmentioning
confidence: 91%
“…The terranes were accreted and cratonised during the Eburnean orogeny, a period of SE to NW directed crustal shortening, metamorphism and magmatic accretion (Oberthür et al, 1998;Feybesse et al, 2006). Peak metamorphic conditions are widely reported as amphibolite facies (500-600°C; 4-6 kbar; John et al, 1999;White et al, 2013), with a retrograde greenschist facies overprint (Hirdes et al, 1996). The Birimian terranes formed over a period of ~180 Ma (Perrouty et al, 2012;White et al, 2014 and references therein;Parra-Avila et al, 2015).…”
Section: Geological Settingmentioning
confidence: 99%
“…This period is divided into two phases. Though there is regional variation, broadly the Eoeburnean (also known as Eburnean I or the Tangaean; 2266-2150 Ma) precedes the Eburnean (2216-1980 (Taylor et al, 1992;Dia et al, 1997;Loh et al, 1999;Allibone et al, 2002;Gueye et al, 2007;Tshibubudze et al, 2009;Hein, 2010;de Kock et al, 2011). The Eoeburnean consists of volcanism, granitoid emplacement and fold, thrust tectonics, and is interpreted by Tshibubudze et al, (2015) to be a single diachronous event across the Birimian.…”
Section: Geological Settingmentioning
confidence: 99%