Abdelbaset M Abudeif, Zakaria Hamimi, Gaber M Gaber, Adel Kotb, Nasir Alarifi, Stefano Bellucci, Marwa M Masoud
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Euler Deconvolution effectively delineates structural discontinuities and fault systems, while the Source Parameter Imaging (SPI) method improves depth accuracy through wavenumber analysis. The Analytical Signal method enhances resolution, providing detailed depth variations. Across these methods, the estimated depth ranges from 300 to 5000 m, with an average depth of approximately 2380 m, offering critical insights into the subsurface geological framework. Two-dimensional (2.5D) modeling was conducted on two selected gravity and magnetic profiles to estimate the depth, dip, density, and magnetic susceptibility of the source bodies. Additionally, three-dimensional (3D) modeling was applied to Bouguer gravity and Reduced-to-the-Pole (RTP) magnetic profiles, providing a detailed representation of the causative source structures. 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引用次数: 0
摘要
本研究的主要目的是全面了解埃及红海Esh El Mellaha地区及其周边地区的地下地质资料。这包括确定该区域下方基底面的深度和构造特征,以及识别沉积盖层内的其他重力和磁源和潜在构造。为了实现这一目标,对布格重力和航磁数据进行了利用、处理和分析。各种深度估计技术用于分析地下结构,每种技术都有其独特的优势。欧拉反褶积(Euler Deconvolution)可以有效地描述结构不连续面和断层系统,而源参数成像(SPI)方法通过波数分析提高了深度精度。分析信号方法提高了分辨率,提供了详细的深度变化。在这些方法中,估计深度范围为300至5000米,平均深度约为2380米,为了解地下地质框架提供了关键的见解。选取两条重磁剖面进行二维(2.5D)建模,估算震源体的深度、倾角、密度和磁化率。此外,三维(3D)建模应用于布格重力和降极(RTP)磁剖面,提供了诱发源结构的详细表示。重磁资料三维反演结果揭示了地下密度和磁化率的分布,有助于识别主要地质构造。剖面图和3D模型显示了地下地层的垂直和水平变化,突出了可能对应断层和岩性变化的明显异常带。结果表明,沉积演替厚度在1.0 ~ 2.2 km之间,与钻孔资料一致。在这些模型中发现的积极的构造特征表明了潜在油气藏的有希望的目标。
Modeling of potential field data for detecting structural and tectonic framework of Esh El Mellaha area, Red Sea, Egypt.
The main objective of this research is to get a comprehensive view on the subsurface geological data on the Esh El Mellaha area and environs, Red Sea, Egypt. This includes determining the depth and structural characteristics of the basement surface beneath the region, as well as identifying additional gravity and magnetic sources and potential structures within the sedimentary cover. To achieve this goal, Bouguer gravity and aeromagnetic data were used, processed and analyzed. Various depth estimation techniques were employed to analyze subsurface structures, each offering distinct advantages. Euler Deconvolution effectively delineates structural discontinuities and fault systems, while the Source Parameter Imaging (SPI) method improves depth accuracy through wavenumber analysis. The Analytical Signal method enhances resolution, providing detailed depth variations. Across these methods, the estimated depth ranges from 300 to 5000 m, with an average depth of approximately 2380 m, offering critical insights into the subsurface geological framework. Two-dimensional (2.5D) modeling was conducted on two selected gravity and magnetic profiles to estimate the depth, dip, density, and magnetic susceptibility of the source bodies. Additionally, three-dimensional (3D) modeling was applied to Bouguer gravity and Reduced-to-the-Pole (RTP) magnetic profiles, providing a detailed representation of the causative source structures. The results of the 3D inversion of gravity and magnetic data reveal the subsurface distribution of density and magnetic susceptibility, aiding in the identification of major geological structures. The sectional maps and 3D models illustrate the vertical and horizontal variations in subsurface formations, highlighting distinct anomaly zones that may correspond to faults and lithological changes. The obtained results indicate that the sedimentary succession thickness is ranging from 1.0 to 2.2 km, a finding corroborated by the borehole data. Positive structural features identified in these models suggest promising targets for potential hydrocarbon reservoirs.
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