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PROVENANCE, DIAGENESIS AND RESERVOIR QUALITY OF THE LOWER CRETACEOUS SANDSTONE OF THE ORANGE BASIN, SOUTH AFRICA

机译:南非橙色盆地下白垩统砂岩的物源,成岩作用和储层质量

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摘要

The Orange Basin, offshore South Africa, formed as a result of Gondwana break-up and rifting during the late Jurassic to early Cretaceous periods followed by drifting apart of the African and South American plates. A number of wells have been drilled over the last three decades in the Orange Basin, focussed primarily in water depths of less than 500m with gas/condensate and one oil discovery in the syn-rift succession illustrating a working petroleum system. Lower Cretaceous (Albian age) sandstones of the Orange Basin conformably overlie Aptian age sedimentary rocks including potential source rocks for Albian reservoirs, although well testing has yet to demonstrate commercial volumes of hydrocarbons. This work examines sandstones sampled from well A-W1 and attempts to clarify sediment provenance and post-depositional diagenetic modification of these potential reservoir sands through a combination of analytical techniques including thin section petrographic characterization, X-ray diffractometry (XRD), X-ray fluorescence (XRF) analyses (major element analysis after Al-Harbi and Khan, 2008), high-resolution transmission electron microscopy (HR-TEM) and scanning electron microscopy (SEM). The data generated from these analytical techniques have been utilized to interpret the diagenetic and geochemical variation and development of the Albian sands of this well as characteristic of the potential play area. Albian age sandstones have a detrital mineralogy dominated by quartz, K-feldspar and mica and range from greywacke to litharenites. Diagenetic modifications include feldspar and lithic fragment dissolution, compaction and reduction of the depositional porosity through grain rearrangements, rotation and fragmentation of grains and cementation (primarily quartz and carbonate). Relatively early formation of authigenic chlorite, followed quartz cementation occurred in an environment where the movement of formation waters was relatively unrestricted.
机译:南非近海的奥兰治盆地是由于侏罗纪晚期至白垩纪早期冈瓦纳断裂和裂谷而形成的,随后又在非洲和南美板块中漂移开来。在过去的三十年中,在奥兰治盆地钻了许多井,主要集中在小于500m的水深中,其中有天然气/凝析油,并且在同分立裂隙演替中发现了一个石油,说明了一个有效的石油系统。奥兰治盆地的下白垩统(阿尔比时代)砂岩覆盖在阿普特时代的沉积岩上,包括阿尔比亚储层的潜在烃源岩,尽管试井尚未显示出一定数量的碳氢化合物。这项工作检查了从A-W1井采样的砂岩,并试图通过结合包括薄片岩相表征,X射线衍射法(XRD),X射线在内的分析技术来阐明这些潜在储层砂的沉积物来源和沉积后的成岩作用。荧光(XRF)分析(Al-Harbi和Khan之后的主要元素分析,2008年),高分辨率透射电子显微镜(HR-TEM)和扫描电子显微镜(SEM)。这些分析技术所产生的数据已被用来解释该地区的阿尔比亚砂岩的成岩作用和地球化学变化以及发育以及潜在游动区的特征。阿拉伯时代的砂岩具有碎屑矿物学特征,主要由石英,钾长石和云母组成,范围从格雷瓦克岩到锂辉石。成岩作用包括长石和碎屑的溶解,通过晶粒重排的压实和沉积孔隙的减少,晶粒的旋转和破碎以及胶结作用(主要是石英和碳酸盐)。自生亚氯酸盐的形成相对较早,随后在地层水流动相对不受限制的环境中发生了石英胶结作用。

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