首页> 外文期刊>Journal of Asian earth sciences >Moho depth variations over the Maldive Ridge and adjoining Arabian and Central Indian Basins, Western Indian Ocean, from three dimensional inversion of gravity anomalies
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Moho depth variations over the Maldive Ridge and adjoining Arabian and Central Indian Basins, Western Indian Ocean, from three dimensional inversion of gravity anomalies

机译:重力异常的三维反演,马尔代夫海岭及毗邻的阿拉伯盆地和中部印度洋盆地,西印度洋的莫霍面深度变化

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Analysis of high resolution satellite derived free air gravity data has been undertaken in the Greater Maldive Ridge (GMR) (Maldive Ridge, Deep Sea Channel, northern limit of Chagos Bank) segment of the Chagos Laccadive Ridge and the adjoining Arabian and Central Indian Basins. A Complete Bouguer Anomaly (CBA) map was generated from the Indian Ocean Geoidal Low removed Free Air Gravity (hereinafter referred to as "FAG-IOGL") data by incorporating Bullard A, B and C corrections. Using the Parker method, Moho topography was initially computed by inverting the CBA data. From the CBA the Mantle Residual Gravity Anomalies (MRGA) were computed by incorporating gravity effects of sediments and lithospheric temperature and pressure induced anomalies. Further, the MRGA was inverted to get Moho undulations from which the crustal thickness was also estimated. It was found that incorporating the lithospheric thermal and pressure anomaly correction has provided substantial improvement in the computed Moho depths especially in the oceanic areas. But along the GMR, there was not much variation in the Moho thickness computed with and without the thermal and pressure gravity correction implying that the crustal thickness of the ridge does not depend on the oceanic isochrones used for the thermal corrections. The estimated Moho depths in the study area ranges from 7 km to 28 km and the crustal thickness from 2 km to 27 km. The Moho depths are shallower in regions closer to Central Indian Ridge in the Arabian Basin i.e., the region to the west of the GMR is thinner compared to the region in the east (Central Indian Basin). The thickest crust and the deepest Moho are found below the N-S trending GMR segment of the Chagos-Laccadive Ridge. Along the GMR the crustal thickness decreases from north to south with thickness of 27 km below the Maldives Ridge reducing to similar to 9 km at 3 degrees S and further increasing towards Chagos Bank. Even though there are similarities in crustal thickness between Maldive Ridge and other regions like Mascarene Plateau which was recently interpreted as underlain by continental crust, much more geoscientific work including drilling has to be undertaken to finally confirm the exact nature of the ridge.
机译:在Chagos Laccadive Ridge的大马尔代夫海岭(GMR)(马尔代夫海脊,深海航道,Chagos银行北界)段以及毗连的阿拉伯和中部印度盆地进行了高分辨率卫星衍生的自由重力数据分析。通过合并Bullard A,B和C校正,从印度洋大地水准面低空游离重力(以下称为“ FAG-IOGL”)数据生成了完整的布格异常(CBA)图。使用Parker方法,首先通过反转CBA数据来计算Moho地形。通过CBA,通过结合沉积物的重力效应以及岩石圈温度和压力引起的异常来计算地幔残余重力异常(MRGA)。此外,将MRGA倒置以获得Moho波动,从中也可以估算出地壳厚度。已经发现,结合岩石圈热力和压力异常校正,尤其是在海洋地区,已大大提高了计算出的莫霍面深度。但是沿着GMR,在有和没有热力和压力重力校正的情况下,计算出的Moho厚度没有太大变化,这意味着洋脊的地壳厚度不取决于用于热校正的海洋等时线。研究区估计的莫霍面深度范围为7 km至28 km,地壳厚度为2 km至27 km。在靠近阿拉伯盆地中部印度洋脊的地区,莫霍面深度较浅,即,与东部(中部印度盆地)相比,GMR西侧的区域更薄。在Chagos-Laccadive山脊的N-S趋势GMR段之下发现了最厚的地壳和最深的莫霍面。沿着GMR,地壳厚度从北向南减小,在马尔代夫山脊以下27 km处,在南纬3度时减小到大约9 km,并向Chagos Bank进一步增加。即使马尔代夫海岭和其他地区如马斯卡林高原之间的地壳厚度相似(最近被解释为大陆地壳下垫),但仍需进行更多的地质工作,包括钻探,才能最终确定海岭的确切性质。

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