2020
DOI: 10.1007/978-3-030-49771-2_13
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Petrogenetic Evolution of the Neoproterozoic Igneous Rocks of Egypt

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Cited by 12 publications
(5 citation statements)
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“…The evolution of the ANS took place over 350 million years, from 870 Ma until about 520 Ma, when the great peneplain was cut and thick Cambro-Ordovician sandstones were deposited (Azer and Asimow, 2021). The ANS evolved through a series of stages that can be characterized as (1) supercontinent rift and drift (1000-900 Ma), (2) subduction and consumption of intervening ocean basins (870-750 Ma), (3) continental collision and orogeny (750-630 Ma), and (4) postorogenic extension and collapse (620-580 Ma plus minor later activity extending to 520 Ma).…”
Section: Discussionmentioning
confidence: 99%
“…The evolution of the ANS took place over 350 million years, from 870 Ma until about 520 Ma, when the great peneplain was cut and thick Cambro-Ordovician sandstones were deposited (Azer and Asimow, 2021). The ANS evolved through a series of stages that can be characterized as (1) supercontinent rift and drift (1000-900 Ma), (2) subduction and consumption of intervening ocean basins (870-750 Ma), (3) continental collision and orogeny (750-630 Ma), and (4) postorogenic extension and collapse (620-580 Ma plus minor later activity extending to 520 Ma).…”
Section: Discussionmentioning
confidence: 99%
“…The geodynamic model of the Igla Ahmr granites is shown in Figure 15. The Igla Ahmr tonalites are old granitic phases in the studied area, and show characteristic features of I-Type (Figures 12e, 13b and 14c); these tonalites originated from mantle-derived melts and contaminated with crustal materials (~670-630 Ma; [79]) during the syn-collisional stage (Figure 15a). Then, there is a transitional stage and a change in the tectonic style from the compressional setting and formation of syn-collisional granites (e.g., I-type tonalites, Figure 4a,b) to the extensional setting and formation of post-collisional granites (e.g., A-type syenogranites and alkali feldspar granites, Figure 4c-f).…”
Section: Geodynamic Evolution and Development Of The Ced Juvenile Crustmentioning
confidence: 99%
“…The formation of igneous rocks due to the cooling of magma (Azer & Asimow, 2021;Gill & Fitton, 2022). Rocks are solid aggregates formed by minerals that have solidified from natural processes (El Alami et al, 2020;Sultoni et al, 2019).…”
Section: The Process Of Rock Formation At Bukit Cintamentioning
confidence: 99%