根据尼日利亚西北部索科托盆地白垩纪和第三纪地层的潜在实地数据推断的深层地壳框架调查

Adamu Abubakar, Othniel Kamfani Likkason, Yunusa Abdulganiyu, Hadiza Umar Tsafe, Umar Mahmood, B. Balarabe, A. Yohanna
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引用次数: 0

摘要

索科托组的古新世沉积物(包括甘巴地层、丹格地层和卡兰贝纳地层)被里马组的马斯特里赫特沉积物所覆盖,里马组包括乌尔诺地层、杜卡马杰地层和塔洛卡地层。研究这些沉积物时使用了高分辨率航空磁力和卫星重力测量。上述地层与本研究区域的白垩纪和第三纪地层相对应,位于 Iullemmeden 盆地的东南部。我们的目的是利用整个区域的卫星重力和航空磁数据确定并解释密度和磁化的水平变化。利用二维(2D)径向平均功率谱分析对深层磁源和密度源进行了扫描,为研究区域下的莫霍、下部和上部岩石圈建立了东北至西南和东至西走向的模型。利用向上延续、导数分析以及二维重力和磁力模型对结果进行了进一步评估。根据电位场数据的垂直梯度,确定了许多重要的构造趋势(即 NE-SW、E-W 和 ENE-WSW)。光谱分析和欧拉解卷积法可用来计算下地幔和上地幔地壳边界的深度以及莫霍面的深度。定性分析结果表明,贡杜米地层和伊洛地层向东北方向侵入是引力和磁力相互作用显著的主要原因。在向上延伸 5 千米、7 千米、20 千米和 30 千米的异常图上,可以看到深层地壳结构和矿化异常体随深 度的差异。从数量上看,沿选定剖面(L1、L2、L4、L6 和 L7)的二维区域模型显示了 Gundumi 和 Illo Formation(Continental Intercalaire,CI)类型地壳的典型岩石地层演替,该地壳又分为下地幔地壳、上地幔地壳和莫霍面。按地表深度计算,沉积厚度在 4.06 千米至 23.31 千米之间。莫霍界面、下地幔壳、上地幔壳和磁性地壳的深度都在∼10.23 千米左右。索科托群北部和南部的基岩局部模型之间的距离分别约为∼6至∼8千米和∼4.5千米。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Investigation into a deep-rooted crustal framework deduced from potential field data in Cretaceous and Tertiary strata, Sokoto Basin NW, Nigeria
The Paleocene sediments from the Sokoto Group, which comprises of the Gamba, Dange, and Kalambaina formations, were covered by Maastrichtian sediments from the Rima Group, which includes the Wurno, Dukamaje, and Taloka formations. High-resolution aeromagnetic and satellite gravity measurements were used to study these sediments. The aforementioned strata correspond to the Cretaceous and Tertiary strata in this research area and are situated in the south-eastern part of the Iullemmeden Basin. Our aim is to determine and explain the horizontal variation in density and magnetization using the whole regional satellite gravity and aeromagnetic data. The deeper magnetic and density sources were scanned using a two-dimensional (2D) radially averaged power spectrum analysis to produce the NE to SW and E to W trending models for the Moho, lower, and upper lithosphere under the study area. The results were further assessed using upward continuation, derivative analysis, and two-dimensional gravity and magnetic modeling. Numerous important structural trends (i.e., NE-SW, E-W & ENE-WSW), have been identified as a result of the vertical gradients for the potential field data. Spectral analysis and Euler deconvolution can be used to calculate the depths to the lower and upper mantle crust boundaries as well as the depth to Moho. The findings of a qualitative analysis point to an intrusion of the Gundumi and Illo Formations that has a northeast orientation as the primary cause of the significant gravitational and magnetic interaction. The differences in the deep-seated crustal structures and mineralized anomalous bodies with depth were visible on anomaly maps with an upward continuation of 5 km, 7 km, 20 km, and 30 km. Quantitatively, the 2D regional models along the selected profiles (L1, L2, L4, L6 and L7) display a typical lithostratigraphic succession of the Gundumi and Illo Formation (Continental Intercalaire, CI) type of crust, which is subdivided into the lower and upper mantle crust as well as the Moho. The sediment thickness by surface depth ranges from ∼4.06 km and ∼23.31 km. The Moho interface, lower and upper mantle crusts, and magnetic crust are all located at depths of around ∼10.23 km. The distance between the local models of the foundation rocks to the north and south of the Sokoto Group was approximately ∼6 to ∼8 km and ∼4.5 km, respectively.
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