2017
DOI: 10.1007/s12549-017-0312-1
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Foraminiferal palaeobathymetry and depositional sequences of the subsurface Eocene Apollonia Formation in North Western Desert, Egypt

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Cited by 9 publications
(3 citation statements)
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“…(2006) recorded that, the LO of Hantkenina dumblei Weinzierl and Applin is high in the E9 Zone. Farouk et al. (2018) confirmed the same conclusion in the Eocene Apollonia Formation at the North Western Desert .…”
Section: Resultssupporting
confidence: 83%
“…(2006) recorded that, the LO of Hantkenina dumblei Weinzierl and Applin is high in the E9 Zone. Farouk et al. (2018) confirmed the same conclusion in the Eocene Apollonia Formation at the North Western Desert .…”
Section: Resultssupporting
confidence: 83%
“…Two most widely significant regional unconformities occur between the Khoman/Apollonia Formational boundary as a result of tectonic rising, which caused the missing of around 200 m (roughly 656 ft), while the second erosion event occurred near the top of the Dabaa Formation, which has an eroded thickness of 400 m (1312 ft) (Abdel‐Fattah et al, 2017; Farouk et al, 2018; Tawfik, Ondrak, et al, 2022; Tawfik, Winterleitner, & Mutti, 2022) (Table 3). Other erosion surfaces are lower in thickness and result from faulting in A/R ‘E’, A/R ‘G’ and Upper Bahariya.…”
Section: Resultsmentioning
confidence: 99%
“…The Paleo water depth (PWD) was estimated based on the interpreted depositional environments of different rock units from previous sedimentological and paleontological studies (e.g. El Beialy et al, 2011;Salem and Sehim, 2017;Tahoun et al, 2017;Farouk et al, 2018;Shehata et al, 2018aShehata et al, , 2019Ibrahim et al, 2020;Mahfouz et al, 2020). The Sediment-Water Interface Temperature (SWIT) was calculated using the global mean temperature at sea level for latitudes of 28° and 29°, Northern Africa, based on Wygrala (1989).…”
Section: Basin Modeling 431 Input Data and Boundary Conditionsmentioning
confidence: 99%