在尼泊尔中部的喜马拉雅山脉,活跃的异序推力故障发生
Cameron Wobus1, Arjun Heimsath, Kelin Whipple
1Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA. cwobus@mit.edu
Nature
|April 23, 2005
概括
新证据揭示了尼泊尔中部的一个活跃的推力断层,挑战了主要的喜马拉雅推力 (MHT) 作为印度-欧亚融合的唯一住宿. 这一发现凸显了喜马拉雅山脉前线以北更深层的构造活动.
科学领域:
- 构造学和地球物理学的构造学.
- 喜马拉雅地质学的地质学
- 星际约会 星际约会 星际约会
背景情况:
- 印度-欧亚洲板块的融合主要归因于主要的喜马拉雅推力 (MHT).
- MHT的表面表达在尼泊尔的西瓦利克山脉,与地质学和地震数据一致.
- 一个替代模型表明北方断层的滑动,也适合现有数据.
研究的目的:
- 调查尼泊尔中部印度 - 欧亚大陆汇聚的构造性适应.
- 为了测试目前的变形模型,仅沿着主要的喜马拉雅推力 (MHT).
- 为了确定MHT已知的表面表达的北方的活跃断层.
主要方法:
- 在现场宇宙10Be约会以确定千年时间尺度的侵蚀率.
- 在尼泊尔中部岩石升起梯度的分析.
- 与现有的40Ar-39Ar热年代学数据的整合.
主要成果:
- 在尼泊尔中部短距离 (<2公里) 检测到侵蚀率增加了四倍.
- 这表明MHT表面轨迹以北约100公里的活跃推力断层.
- 岩石升起模式不仅仅是通过MHT坡道上的被动运输来解释的.
结论:
- 位于喜马拉雅高山脚下的深层,突破地表的结构正在积极挖掘岩石.
- 这些发现挑战了印度-欧亚大陆融合的单一MHT适应模式.
- 气候,侵蚀和构造学之间的强烈合可能维持了喜马拉雅山脉前线以北的变形.
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