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Resistivity imaging of geothermal resources in northern Kenya rift by joint 1D inversion of MT and TEM data

机译:通过MT和TEM数据的一维反演对肯尼亚北部裂谷地热资源进行电阻率成像

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An extensive electromagnetic (EM) survey comprising over 400 sites on the Korosi, Paka and Silali volcanoes in the northern volcanic province in Kenya was conducted in order to assess the occurrence of geothermal resources in the context of the geophysics of the major volcanic centers of the north Kenyan East African Rift System (EARS). This area lies within the (EARS) where active extension is currently taking place. A joint inversion of magnetotelluric (MT) and co-located Transient electromagnetic (TEM) has revealed a resistivity pattern consistent with the existence of several geothermal systems within the study area. Each geothermal system is characterized by a relatively resistive 100 Omega m surficial layer overlying a similar to 10 Omega m low resistivity zone interpreted as the hydrothermally altered clay cap of the system. The cap overlies a higher resistivity zone of about 60 Omega m with a top at about 1000 m depth, interpreted as a potential high.temperature alteration zone. The trend of moderate high resistivity at the depth of the potential reservoir corresponds to the zone of intense faulting and fracturing as imaged on the surface. Similarly the moderate high resistivity at sea level mimics the trend of the rift with a break in between Paka and Silali volcanoes where the resistivity trend is offset to the west. This break and the accompanying offset maps a possible westward shift of the axis of the rift in the rift alignment between Paka and Silali volcanoes. Although the 1000-2000 m thick low resistivity zones imaged on the flanks of the Korosi, Paka and Silali volcanoes have been tentatively interpreted as volcanoclastic sediments, elsewhere in the Kenyan EARS, low resistivity zones adjacent to volcanoes have been interpreted differently. To address this ambiguity, these thick low resistivity zones will be further investigated, principally using gravity surveys. (C) 2017 Elsevier Ltd. All rights reserved.
机译:进行了广泛的电磁(EM)调查,包括肯尼亚北部火山省的科罗西,帕卡和西拉利火山的400多个站点,目的是在肯尼亚主要火山中心的地球物理学背景下评估地热资源的产生。肯尼亚北部的东非裂谷系统(EARS)。该区域位于(EARS)中,当前正在进行有效的扩展。大地电磁(MT)和并置的瞬态电磁(TEM)的联合反演揭示了与研究区域内若干地热系统的存在相符的电阻率模式。每个地热系统的特征是相对电阻100Ωm的表层,其上覆有类似于10Ωm的低电阻率带,该低电阻率带被解释为系统的水热蚀变粘土层。顶盖覆盖约60Ω的较高电阻率区,顶部约1000 m深度,被解释为潜在的高温变化区。在潜在储层深度处中等高电阻率的趋势对应于表面上成像的强烈断裂和破裂区域。同样,海平面适度的高电阻率模仿了裂谷的趋势,在Paka和Silali火山之间发生了断裂,电阻率趋势向西偏移。该断裂及其伴随的偏移量映射了帕卡火山和塞拉利火山之间裂谷走向中裂谷轴线的可能向西偏移。尽管科罗西火山,帕卡火山和西拉里火山两侧的1000-2000 m厚的低电阻率地区已被初步解释为火山碎屑沉积物,但在肯尼亚EARS的其他地方,与火山相邻的低电阻率地区却有不同的解释。为了解决这种模糊性,将主要使用重力测量法进一步研究这些厚的低电阻率区域。 (C)2017 Elsevier Ltd.保留所有权利。

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