运动学

IF 1 Q3 GEOCHEMISTRY & GEOPHYSICS
Natalia Radkovets, Yuriy Koltun
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引用次数: 0

摘要

本文研究了喀尔巴阡前深Pokuttya-Bukovyna部分台地基底的上阿尔—下塞诺曼尼亚质杂岩,该杂岩是洛普什纳油田的主要储层之一。方法。研究工作包括测井资料对比、岩心材料的岩性研究、岩石的矿物学和岩石学分析以及沉积盆地的古地理研究。结果。在对所有现有井进行分析的基础上,确定了在Pokuttya-Bukovyna喀尔巴阡人的整个本土范围内,晚alian -早Cenomanian时代的沉积物主要以砂岩为代表。它们由石英(50-80%)、长石(1-5%)、白云母(0.1-3%)、黄铁矿(0.1-3%)和辅助矿物锆石、绿帘石组成。砂岩的很大一部分由自生矿物组成-海绿石(10-15%,有时高达45%)和磷酸盐(1-3 - 10%)。岩石中的基质主要为多孔性和接触多孔性(占岩石体积的10-15%),具有良好的储层性质。在古地理重建的基础上,认为在阿尔比世晚期-塞诺曼世早期,整个中特提斯喀尔巴阡支陆架盆地内普遍存在陆源沉积作用,形成了厚砂岩地层。喀尔巴阡褶皱带的逆冲作用影响了岩石的埋藏史和沉积后演化。这导致了上阿尔比—下塞诺曼尼亚层序储集岩和圈闭的形成。研究区油气运移的特殊性表明,在Pokuttya-Bukovyna喀尔巴阡山脉本土群中发现新矿床的可能性很大。创意。应用岩性、地质-地球物理和古地理研究的复合体,可以研究阿尔及利亚-塞诺曼尼亚沙砾岩复合体的横向和剖面分布特征、矿物学和岩石学特征、沉积环境。研究层的沉积后演化和油气运移特征是由喀尔巴阡复理带逆冲至东欧地台边缘的动力学作用引起的。现实意义。结果表明,Lopushna油田的上alian -下Cenomanian砂岩在厚度和矿物组成上都代表了整个Pokuttya-Bukovyna喀尔巴阡山脉的潜在储层。由于Pokuttya断裂可能是喀尔巴阡复理石层向台地基底地层运移的一条通道,因此在Pokuttya- bukovyna喀尔巴阡原土的地震研究中,很有可能在类似Lopushna的构造中发现新的油气藏。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
GEODYNAMICS
The purpose of this work is to study the Upper Albian-Lower Cenomanian psammitic complex of the platform basement of the Pokuttya-Bukovyna part of the Carpathian Foredeep, which is one of the main reservoir strata of the Lopushna oil field. Methodology. The complex of investigations includes correlation of the well-log data, lithological studies of core material, mineralogical and petrographic analysis of rocks, and paleogeographic studies of the sedimentary basin. Results. On the basis of the analysis of all existing wells, it was established that the deposits of the Late Albian-Early Cenomanian age within the entire territory of the autochthon of the Pokuttya-Bukovyna Carpathians are mostly represented by sandstones. They are composed of quartz (50-80%), feldspar (1–5%), muscovite (0.1-3%), pyrite (0.1-3%) and accessory minerals – zircon and epidote. A significant part of sandstone is compoed of the authigenic minerals – glauconite (10-15%, sometimes up to 45%) and phosphate (1–3 up to 10%). The matrix in the rocks is mainly porous and contact-porous (10-15% of the rock volume), which provides these psammites with good reservoir properties. On the basis of paleogeographic reconstructions, it was established that in the Late Albian-Early Cenomanian, terrigenous sedimentation prevailed within the entire shelf basin of the Carpathian branch of the Meso-Tethys, which caused the accumulation of the thick sandstones’ strata. The burial history and post-sedimentary evolution of rocks took place under the influence of the thrusting of the Carpathian Fold Belt. This resulted in the formation of reservoir rocks and traps in the Upper Albian-Lower Cenomanian sequence. The peculiarities of hydrocarbon migration in the studied region indicate a high probability of discovering new deposits in the autochthon of the Pokuttya-Bukovyna Carpathians. Originality. The applied complex of lithological, geological-geophysical and paleogeographical studies made it possible to investigate the features of distribution of the Albian-Cenomanian psammite complex of rocks, both laterally and in section, their mineralogical and petrographic characteristics, sedimentary environments. The post-sedimentary evolution of the study strata and features of hydrocarbon migration were caused by the dynamics of the Carpathian Flysch Belt thrusting over the margin of the East-European platform. Practical significance. The obtained results show that the Upper Albian-Lower Cenomanian sandstones, which are oil and gas-bearing in the Lopushna field, represent the potential reservoirs in terms of both thickness and mineral composition within the entire autochthon of the Pokuttya-Bukovyna Carpathians. Since the Pokuttya fault could serve as a migration path for the hydrocarbons from the Carpathian flysch sequence into the platform basement strata, there is a high probability of the discovery of new accumulations in the structures similar to the Lopushna, revealed by seismic studies in the autochthon of the Pokuttya-Bukovyna Carpathians.
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来源期刊
Geodynamics
Geodynamics GEOCHEMISTRY & GEOPHYSICS-
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