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首页> 外文期刊>Tectonics >Deep Structure of the Eastern Himalayan Collision Zone: Evidence for Underthrusting and Delamination in the Postcollisional Stage
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Deep Structure of the Eastern Himalayan Collision Zone: Evidence for Underthrusting and Delamination in the Postcollisional Stage

机译:喜马拉雅东部碰撞带的深层结构:碰撞后阶段的下冲和分层证据

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Based on broadband seismic data from 102 stations in the eastern Himalayan collision zone, the crustal thickness and Poisson's ratio were determined by using the H-kappa stacking analysis of teleseismic P wave receiver functions. The Moho topography rapidly deepens northward in the northern Lhasa terrane, inferring the northern limit of the Indian plate underthrusting beneath Tibetan Plateau. Our seismic images show that steep subduction of the Indian plate occurs to the west of the Eastern Himalayan Syntaxis while gentle subduction to the east. The variation of subduction geometry of the Indian plate may be one of the causes for the formation of the eastern Himalayan Syntaxis. The 2-D crustal density modeling of the gravity measurements shows that the average crustal density in the eastern Himalayan collision zone is less dense than the global average continental crust, and our preferred model has 5- to 10-km-thick, high density layer (2,970-3,000 kg/m(3)) in the lower crust beneath the eastern Lhasa terrane, consistent with mafic underplating. The attributes of a thickened crust with northward deepening Moho and low-to-normal Poisson's ratio might be the geophysical signature of delamination beneath the Lhasa terrane and underthrusting of Indian plate. We hypothesize that the orogenic root of the Lhasa terrane was removed by convective-driven delamination, followed by northward subduction of the Indian plate. Thus, delamination and continental subduction are the dominant deep processes in the postcollisional stage in the eastern Himalayan collision zone.
机译:根据喜马拉雅东部碰撞带102个台站的宽带地震数据,通过远震P波接收器函数的H-kappa叠加分析确定了地壳厚度和泊松比。 Moho地形在拉萨北部的北部迅速向北加深,推断出印度板块的北界在青藏高原以下发生了逆冲作用。我们的地震图像显示,印度板块的俯冲俯冲发生在东部喜马拉雅山脉的西部,而俯冲俯冲在东部。印度板块俯冲几何的变化可能是形成东部喜马拉雅句法的原因之一。重力测量的二维地壳密度模型显示,喜马拉雅东部碰撞带的平均地壳密度不及全球平均大陆壳低,我们首选的模型具有5至10公里厚的高密度层(2,970-3,000 kg / m(3))位于东部拉萨地体下方的下地壳中,与镁铁质的基底层一致。地壳增厚,莫霍面向北加深和泊松比低至正常的属性可能是拉萨地层下的分层和印度板块下冲的地球物理特征。我们假设拉萨地体的造山根系由对流驱动的分层作用除去,然后向北俯冲印度板块。因此,分层和大陆俯冲是东部喜马拉雅碰撞带碰撞后阶段的主要深部过程。

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