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Neotectonics and Mantle Earthquakes in the Pamir-Hindu Kush Region

机译:帕米尔-兴都库什地区的新构造和地幔地震

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摘要

Tectonic aspects of the formation of the Pamirs-Hindu Kush zone of intermediate earthquakes are discussed. A model of the regional late-collision (neoteclonic) evolution is developed based on the analysis of geologic data. The first stage of this evolution spans from the late Eocene to the beginning of the late Miocene; the second stage, from the late Miocene to the Holocene. These stages are characterized by different thermody-namic conditions and, correspondingly, by different geodynamic settings that determined a specific style of tectonic deformation. The early stage was marked by differentiated lateral displacements of the Earth's tectoni-cally delaminated crust. The heating of the crust that is reflected in intense granitic magmatism promoted delaminalion. At the late stage, the heating and delamination probably waned and were replaced by more homogeneous lateral motion of blocks and by regional uplift. Because of lateral displacements, the oceanic crust fragments of different age were overridden by blocks of the continental crust and submerged to a depth of 40-70 km. Their eclogitization might have lead to further submergence into the mantle. Mantle earthquakes in the Pamir-Hindu Kush zone are induced by relaxation of the stress that accumulates in submerging fragments.
机译:讨论了中地震帕米尔斯-兴都库什带形成的构造方面。基于地质数据分析,建立了区域晚期碰撞(新纪元)演化模型。演化的第一阶段是从始新世晚期到中新世晚期。第二阶段,从中新世晚期到全新世。这些阶段的特征是不同的热动力条件,并相应地具有不同的地球动力学背景,这些条件决定了特定的构造变形形式。早期的特征是地球构造-地壳分层地壳的横向位移有所不同。强烈的花岗岩岩浆作用所反映的地壳加热促进了层剥作用。在后期,加热和分层可能会减弱,并被更均匀的砌块横向运动和区域隆升所代替。由于横向位移,不同年龄的洋壳碎片被大陆壳块覆盖,并淹没到40-70 km的深度。它们的凝结可能导致其进一步浸入地幔中。帕米尔-兴都库什带的地幔地震是由水下碎片中积累的应力松弛引起的。

著录项

  • 来源
    《Geotectonics》 |2005年第1期|p.56-68|共13页
  • 作者

    T. P. Ivanova; V. G. Trifonov;

  • 作者单位

    Institute for Dynamics of Geospheres, Russian Academy of Sciences, Leninskii pr. 38, bldg. 6, Moscow, 117334 Russia;

  • 收录信息 美国《科学引文索引》(SCI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学、地球科学;
  • 关键词

  • 入库时间 2022-08-18 03:40:06

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