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首页> 外文期刊>Journal of applied sciences research >Palynology and palynofacies studies of the subsurface Aptian-Cenomanian sedimentsfrom the central North Western Desert, Egypt
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Palynology and palynofacies studies of the subsurface Aptian-Cenomanian sedimentsfrom the central North Western Desert, Egypt

机译:埃及西北沙漠中部阿普生-西诺曼尼亚表层沉积物的孢粉学和古相研究

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The lower Cretaceous sediments succession is composed of four formations in Northern Western Desert of Egypt. These formations are Alamein, Dahab, Kharita and Bahariya formations. They are considered as the main target of the oil and gas exploration in the Egyptian Western Desert. The present study investigated their thermal maturity and potentiality to generate the hydrocarbons. These were conducted by the study palynostratigraphy, palynofacies and spore coloration of samples from these formations in WD 19-2 borehole. The identified palynozones are Afropollis jardinus Acme Zone (late Albian – early Cenomanian), Araucariacites australis Acme Zone (middle Albian) and Murospora florida Acme zone (Aptian). The first zone is differentiated into two subzones, which are Elaterosporites klaszii Interval Subzone and Cretacaeiporites densimurus Interval Subzone. The palynofacies analysis revealed that the Alamein and Dahab formations are deposited in deltaic shallow marine dysoxic to anoxic environment. Kharita Formation was deposited in more proximal near shore marine environment under suboxic to oxic conditions. The Bahariya Formation was deposited in proximal near shore dysoxic to oxic marine conditions. The investigated kerogens from the Alamein and Dahab formations were gas prone type II and III, while in Kharita and Bahariya formations they were gas prone type II, III and IV. The spore color or thermal alteration index (TAI) observations indicated that the samples from Alamein and Dahab formations contain mature kerogens and can be a potential source yield hydrocarbons. The Kerogens of Kharita and Bahariya formations are immature to yield gas and are not effective hydrocarbon source.
机译:下白垩纪沉积层序由埃及北部西部沙漠的四个地层组成。这些地层是阿拉曼,达哈卜,卡里塔和巴哈里亚地层。它们被认为是埃及西部沙漠中油气勘探的主要目标。本研究调查了它们的热成熟度和产生碳氢化合物的潜力。这些是通过研究地层学,孢粉和WD 19-2井眼中这些地层样品的孢子着色进行的。识别出的油菜素地带为非洲紫花苜蓿Acme区(阿尔比晚期至西诺曼尼亚晚期),南洋南洋杉Acme区(阿尔比亚中部)和佛罗里达紫檀Acme区(Aptian)。第一个区域分为两个子区域,分别是Elaterosporites klaszii间隔子区域和Cretacaeiporites densimurus间隔子区域。孢粉分析表明,阿拉曼和达哈卜地层沉积在三角洲浅海低氧至缺氧的环境中。在低氧至有氧条件下,Kharita组沉积在更近的近岸海洋环境中。 Bahariya组沉积在近岸低氧至有氧海洋条件下。所研究的来自Alamein和Dahab地层的干酪根是易燃气体II和III型,而在Kharita和Bahariya地层中则是易燃气体II,III和IV型。孢子颜色或热变化指数(TAI)观察表明,来自Alamein和Dahab地层的样品含有成熟的干酪根,并且可能是潜在的烃源。 Kharita和Bahariya地层的干酪根尚不成熟,不会产生天然气,不是有效的烃源。

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