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首页> 外文期刊>Tectonophysics: International Journal of Geotectonics and the Geology and Physics of the Interior of the Earth >Three-dimensional lithospheric mapping of the eastern Indian shield: A multi-parametric inversion approach
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Three-dimensional lithospheric mapping of the eastern Indian shield: A multi-parametric inversion approach

机译:东印度盾构的岩石圈三维三维制图:多参数反演方法

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摘要

We analyzed satellite gravity and geoid anomaly and topography data to determine the 3D lithospheric density structure of the Singhbhum Protocontinent. Our density model shows that distinct vertical density heterogeneities exist throughout the lithosphere beneath the Singhbhum Protocontinent The crustal structure identified includes a lateral average crustal density variation from 2800 to 2890 kg/m(3) as well as a relatively flat Moho at 35-40 km depth in Singhbhum Protocontinent and Bastar Craton. A similar Moho depth range is found for the Mahanadi, Damodar, and Bengal basins. In the northern part of the area, Moho undulates between more than 40 km under the confluence of Mahanadi-Damodar Gondwana basins and the Ganga foreland basin, and 3632 km under the Eastern Ghats Mobile belt and finally reaches 24 km in the Bay of Bengal. The lithosphere-asthenosphere boundary (LAB) across the Singhbhum Protocontinent is at a depth of about 130-140 km. In the regions of Bastar Craton and Bengal Basin, the LAB dips to about 155 5 km depth. The confluence of Mahanadi and Damodar Gondwana basins toward the north-west and the foreland Ganga Basin toward the north are characterized by a deeper LAB lying at a depth of over 170 and 200 km, respectively. In the Bay of Bengal, the LAB is at a shallower depth of about 100-130 km except over the 85 E-0 ridge (150 km), and off the Kolkata coast (155 km). Significant density variation as well as an almost flat crust-mantle boundary indicates the effect of significant crustal reworking. The thin (135-140 km) lithosphere provides compelling evidence of lithospheric modification in the Singhbhum Protocontinent Similarities between the lithospheric structures of the Singhbhum Craton, Chhotanagpur Gneiss Complex, and Northern Singhbhum Mobile Belt confirm that the repeated thermal perturbation controlled continental lithospheric modification in the Singhbhum Protocontinent. (C) 2015 Elsevier BM. All rights reserved.
机译:我们分析了卫星重力,大地水准面异常和地形数据,以确定Singhbhum Protocontinent的3D岩石圈密度结构。我们的密度模型显示,整个Singhbhum原大陆下面的岩石圈存在着明显的垂直密度异质性。确定的地壳结构包括横向平均地壳密度变化范围为2800至2890 kg / m(3),以及35-40 km处相对平坦的莫霍面Singhbhum Protocontinent和Bastar Craton的深度。在Mahanadi,Damodar和Bengal盆地也发现了类似的Moho深度范围。在该地区的北部,在Mahanadi-Damodar Gondwana盆地和Ganga前陆盆地的交汇处,Moho起伏超过40公里,在East Ghats Mobile带之下起3632 km,最后到达孟加拉湾24 km。跨越辛格普托原始大陆的岩石圈-软流圈边界(LAB)的深度约为130-140 km。在巴斯塔尔·克雷顿(Bastar Craton)和孟加拉邦盆地(Bengal Basin)地区,LAB下降至大约155 5 km深。 Mahanadi和Damodar Gondwana盆地向西北汇合,前陆Ganga盆地向北汇合,其特征是更深的LAB位于分别超过170和200 km的深度。在孟加拉湾,LAB的浅层深度约为100-130 km,除了85 E-0山脊(150 km)和加尔各答海岸(155 km)以外。显着的密度变化以及几乎平坦的壳幔边界表明了地壳返工的效果。薄薄的岩石圈(135-140公里)提供了令人信服的Singhbhum原始岩石圈变质的证据。SinghbhumCraton,Chhotanagpur Gneiss复杂区和北部Singhbhum移动带岩石圈结构之间的相似性证实了反复的热扰动控制了大陆岩石圈的变质。 Singhbhum原始大陆。 (C)2015 Elsevier BM。版权所有。

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