首页> 美国卫生研究院文献>Proceedings of the National Academy of Sciences of the United States of America >Greater India Basin hypothesis and a two-stage Cenozoic collision between India and Asia
【2h】

Greater India Basin hypothesis and a two-stage Cenozoic collision between India and Asia

机译:大印度盆地假说和印度与亚洲之间的两阶段新生代碰撞

代理获取
本网站仅为用户提供外文OA文献查询和代理获取服务,本网站没有原文。下单后我们将采用程序或人工为您竭诚获取高质量的原文,但由于OA文献来源多样且变更频繁,仍可能出现获取不到、文献不完整或与标题不符等情况,如果获取不到我们将提供退款服务。请知悉。

摘要

Cenozoic convergence between the Indian and Asian plates produced the archetypical continental collision zone comprising the Himalaya mountain belt and the Tibetan Plateau. How and where India–Asia convergence was accommodated after collision at or before 52 Ma remains a long-standing controversy. Since 52 Ma, the two plates have converged up to 3,600 ± 35 km, yet the upper crustal shortening documented from the geological record of Asia and the Himalaya is up to approximately 2,350-km less. Here we show that the discrepancy between the convergence and the shortening can be explained by subduction of highly extended continental and oceanic Indian lithosphere within the Himalaya between approximately 50 and 25 Ma. Paleomagnetic data show that this extended continental and oceanic “Greater India” promontory resulted from 2,675 ± 700 km of North–South extension between 120 and 70 Ma, accommodated between the Tibetan Himalaya and cratonic India. We suggest that the approximately 50 Ma “India”–Asia collision was a collision of a Tibetan-Himalayan microcontinent with Asia, followed by subduction of the largely oceanic Greater India Basin along a subduction zone at the location of the Greater Himalaya. The “hard” India–Asia collision with thicker and contiguous Indian continental lithosphere occurred around 25–20 Ma. This hard collision is coincident with far-field deformation in central Asia and rapid exhumation of Greater Himalaya crystalline rocks, and may be linked to intensification of the Asian monsoon system. This two-stage collision between India and Asia is also reflected in the deep mantle remnants of subduction imaged with seismic tomography.
机译:印度和亚洲板块之间的新生代汇合形成了典型的大陆碰撞带,包括喜马拉雅山带和青藏高原。在52 Ma或之前发生碰撞后,如何协调印度和亚洲的融合,以及在哪里融合仍然是一个长期存在的争议。自52 Ma以来,这两个板块的汇聚速度达到了3600±35 km,但亚洲和喜马拉雅山的地质记录中记录的上地壳缩短却缩短了约2350 km。在这里我们显示出收敛和缩短之间的差异可以通过在喜马拉雅山大约50到25 Ma之间俯冲高度扩展的大陆和海洋印度岩石圈来解释。古地磁数据表明,这种扩展的大陆和海洋``大印度''海角是由120到70 Ma之间的南北延伸2675±700 km所形成的,位于北印度洋喜马拉雅山和克拉通印度之间。我们建议大约50 Ma的“印度”-亚洲碰撞是西藏-喜马拉雅微大陆与亚洲的碰撞,然后是沿大喜马拉雅山俯冲带俯冲的大洋性大印度盆地的俯冲。印度-亚洲与较厚且连续的印度大陆岩石圈的“硬”碰撞发生在25-20 Ma左右。这种硬碰撞与中亚的远场变形和大喜马拉雅山晶体岩的快速发掘同时发生,并且可能与亚洲季风系统的加剧有关。印度和亚洲之间的这种两阶段碰撞也反映在地震层析成像成像中俯冲的深层地幔残留物中。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
代理获取

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号