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首页> 外文期刊>Journal of African Earth Sciences >Paleoproterozoic structural frame of the Yetti domain (Eglab shield, Algeria): Emplacement conditions of the Tinguicht late pluton from magnetic fabric study
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Paleoproterozoic structural frame of the Yetti domain (Eglab shield, Algeria): Emplacement conditions of the Tinguicht late pluton from magnetic fabric study

机译:Yetti域(阿尔及利亚Eglab盾构)的古元古代构造框架:Tinguicht晚期岩体的磁性条件研究

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摘要

The Tinguicht pluton is part of the similar to 2.07 Ga post-collisional magmatic suites that intruded the Yetti Paleoproterozoic volcano-sedimentary series of the western part of the Eglab Shield (West African Craton). It represents one of the most recent units of these suites. This pluton, with a NW SE elliptic shape, is unfoliated, and its deformational structures are practically restricted to fracturing and faulting. New structural, microstructural and aeromagnetic data are presented in order to analyze in particular the relationship between the Tinguicht pluton emplacement and the related NNW-SSE major mega-shear zone, separating the Yetti and Eglab domains. To constrain the context of the regional post-collisional evolution of the Eglab shield, a structural analysis was performed by mapping the magnetic structures (foliation and lineation) using AMS. The combination of the results of all the used approaches leads to a new and enriched image of this granitic pluton and of its tectonic emplacement context. The elliptic shape of the granitic body and the AMS strain pattern are consistent with the presence of a NNW-SSE major structure. NNW-SSE is also one of the major directions highlighted by the aeromagnetic data. This study thus evidences the role of the pre-existing major shear zones in controlling emplacement of post-collisional Paleoproterozoic plutons like Tinguicht, as shown for Drissa pluton in the Eglab domain earlier. (C) 2015 Elsevier Ltd. All rights reserved.
机译:Tinguicht岩体是类似于2.07 Ga碰撞后岩浆套件的一部分,该套件侵入了Eglab Shield(西非克拉通)西部的Yetti古元古生代火山沉积系列。它代表了这些套房的最新单元之一。此NW SE椭圆形的子体未成叶,其变形结构实际上仅限于破裂和断层。提出了新的结构,微观结构和航空磁学数据,以便特别分析Tinguicht岩体位置和相关的NNW-SSE主要巨型剪切带之间的关系,从而将Yetti和Eglab域分开。为了限制Eglab盾的区域碰撞后演化的背景,通过使用AMS绘制磁性结构(叶面和线条)进行了结构分析。所有使用的方法的结果的结合产生了这种花岗岩岩体及其构造背景的新的丰富图像。花岗岩体的椭圆形状和AMS应变模式与NNW-SSE主结构的存在一致。 NNW-SSE也是航磁数据突出显示的主要方向之一。因此,这项研究证明了先前存在的主要剪切带在控制诸如Tinguicht之类的碰撞后古元古代小体的位置中的作用,如先前在Eglab域中的Drissa pluton所示。 (C)2015 Elsevier Ltd.保留所有权利。

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