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Hydrothermal convection in and around mineralized fault zones: insights from two- and three-dimensional numerical modeling applied to the Ashanti belt, Ghana

机译:矿化断层带及其周围的热液对流:从应用于加纳阿散蒂带的二维和三维数值模拟中获得的见解

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Among hydrogeological processes, free convection in faults has been cited as a possible cause of gold mineralization along major fault zones. Here, we investigate the effects of free convection to determine whether it can cause giant orogenic gold deposits and their regular spatial distribution along major fault/shear zones. The approach comprises: (i) coupled two- and three-dimensional numerical heat- and fluid-flow simulations of simplified geological models; and (ii) calculation of the rock alteration index (RAI) to delineate regions where precipitation/dissolution can occur. Then, comparing the deduced alteration patterns with temperature distribution, potential areas of gold mineralization, defined by T> 200℃ and RAI < 0, are predicted. The models are based on the orogenic Paleoproterozoic ore deposits of the Ashanti belt in western Africa. These deposits occur in the most permeable parts of the fault zone, where the lateral permeability contrast is the highest. For a simple geometry, with a fault zone adjacent to a sedimentary basin half as permeable, we note a transition from three-dimensional circulation within the fault to a two-dimensional convective pattern in the basin far from the fault. Moreover, whereas two-dimensional undulated isotherms dominate in the basin, three-dimensional corrugated isotherms result from the preferred convective pattern within the fault, thus enhancing a periodic distribution of thermal highs and lows. In our most elaborate three-dimensional model with an imposed lateral permeability gradient, the RAI distribution indicates that fluid circulation in fault zones gives rise to a spatial periodicity of alteration patterns consistent with field data.
机译:在水文地质过程中,断层中的自由对流被认为是主要断层带金矿化的可能原因。在这里,我们研究了自由对流的影响,以确定它是否会引起大型造山型金矿床及其沿主要断层/剪切带的规则空间分布。该方法包括:(i)简化地质模型的二维和三维数值热和流体流动耦合模拟; (ii)计算岩石蚀变指数(RAI)以描绘可能发生降水/溶解的区域。然后,将推论的蚀变模式与温度分布进行比较,预测了T> 200℃和RAI <0所定义的金矿化的潜在区域。这些模型基于西非阿散蒂带的造山古元古代矿石矿床。这些沉积物出现在断层带最易渗透的部分,那里的横向渗透率对比最高。对于简单的几何形状,断层带邻近沉积盆地的一半是可渗透的,我们注意到从断层内部的三维环流到盆地中远离断层的二维对流模式的过渡。此外,尽管二维波动等温线在盆地中占主导地位,但三维波纹状等温线是由断层内的首选对流模式产生的,从而增强了热量高低之间的周期性分布。在我们最精细的三维模型中,施加了侧向渗透率梯度,RAI分布表明断层带中的流体循环产生了与田间数据一致的蚀变模式的空间周期性。

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