Earthquake genesis in Nepal Himalaya: A perspective from imaging of the 25th April 2015 Mw 7.8 earthquake source zone

被引:4
|
作者
Pandey, Anand K. [1 ]
Saikia, Dipankar [2 ]
Kumar, M. Ravi [1 ,3 ]
机构
[1] CSIR Natl Geophys Res Inst, Hyderabad, Andhra Pradesh, India
[2] Indian Natl Ctr Ocean Informat Serv, Hyderabad, Andhra Pradesh, India
[3] Inst Seismol Res, Gandhinagar, India
关键词
Mw 7.8 Nepal Earthquake; Receiver functions; Crustal structure; Mid-crustal ramp; RECEIVER FUNCTIONS; COLLISION ZONE; BENEATH;
D O I
10.1016/j.jseaes.2016.12.039
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The Mw 7.8 earthquake in Central Nepal nucleated in the mid-crustal ramp zone of the Main Himalayan decollement Thrust (MHT) and propagated eastward for >140 km where the largest triggered event of Mw 7.3 occurred without any surface rupture. Although it is advocated that the slip and rupture dynamics are controlled by the structural configuration of the MHT and the upper crust, precise correlation between the seismic structure and seismogenesis is hitherto scarce in the Himalaya. To address the issue, we imaged the crustal structure along three profiles covering the earthquake source region using receiver function analysis of the seismic data from the HiCL1MB and HIMNT seismic networks to understand the lateral variability. A 5 km thick, low velocity layer is observed at the mid-crustal level, that steepens in the MHT ramp zone. The bulk of the seismicity including large shocks after the 2015 Nepal earthquake lies in the vicinity of this low velocity layer. Correlation of the seismic structure and aftershock distribution with the published crustal structure clearly suggests that the rupture involves a thicker zone extending for >40 km to the south of the source zone in the MHT ramp. We refined the structure of the MHT zone incorporating published coseismic slip and ground deformation to suggest that the rupture terminated at the footwall imbricate (horse) on the floor thrust below the zone of maximum coseismic uplift and there was a two stage rupture towards the eastern margin of the rupture zone. (C) 2016 Elsevier Ltd. All rights reserved.
引用
收藏
页码:259 / 267
页数:9
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