Crustal Structure Beneath India and Tibet: New Constraints From Inversion of Receiver Functions

2017 ◽  
Vol 122 (10) ◽  
pp. 7839-7859 ◽  
Author(s):  
Arun Singh ◽  
M. Ravi Kumar ◽  
Debasis D. Mohanty ◽  
Chandrani Singh ◽  
Rahul Biswas ◽  
...  
2014 ◽  
Vol 96 ◽  
pp. 237-254 ◽  
Author(s):  
Sumer Chopra ◽  
Tao-Ming Chang ◽  
Sowrav Saikia ◽  
R.B.S. Yadav ◽  
Pallabee Choudhury ◽  
...  

2011 ◽  
Vol 187 (1) ◽  
pp. 303-326 ◽  
Author(s):  
Hrvoje Tkalčić ◽  
Youlin Chen ◽  
Ruifeng Liu ◽  
Huang Zhibin ◽  
Li Sun ◽  
...  

2016 ◽  
Vol 64 (6) ◽  
pp. 2020-2049 ◽  
Author(s):  
Syuhada Syuhada ◽  
Nugroho Dwi Hananto ◽  
Chalid I. Abdullah ◽  
Nanang T. Puspito ◽  
Titi Anggono ◽  
...  

2019 ◽  
Vol 751 ◽  
pp. 41-53 ◽  
Author(s):  
Carolina Buffoni ◽  
Martin Schimmel ◽  
Nora Cristina Sabbione ◽  
María Laura Rosa ◽  
Gerardo Connon

2016 ◽  
Vol 680 ◽  
pp. 99-112 ◽  
Author(s):  
Arun Singh ◽  
Kirti Bhushan ◽  
Chandrani Singh ◽  
Michael S. Steckler ◽  
S. Humayun Akhter ◽  
...  

2016 ◽  
Vol 121 (7) ◽  
pp. 5049-5067 ◽  
Author(s):  
A. Christian Stanciu ◽  
Raymond M. Russo ◽  
Victor I. Mocanu ◽  
Paul M. Bremner ◽  
Sutatcha Hongsresawat ◽  
...  

Geosphere ◽  
2019 ◽  
Vol 16 (1) ◽  
pp. 378-391 ◽  
Author(s):  
E.E. Rodriguez ◽  
R.M. Russo

Abstract Continental crustal structure is the product of those processes that operate typically during a long tectonic history. For the Patagonia composite terrane, these tectonic processes include its early Paleozoic accretion to the South America portion of Gondwana, Triassic rifting of Gondwana, and overriding of Pacific Basin oceanic lithosphere since the Mesozoic. To assess the crustal structure and glean insight into how these tectonic processes affected Patagonia, we combined data from two temporary seismic networks situated inboard of the Chile triple junction, with a combined total of 80 broadband seismic stations. Events suitable for analysis yielded 995 teleseismic receiver functions. We estimated crustal thicknesses using two methods, the H-k stacking method and common conversion point stacking. Crustal thicknesses vary between 30 and 55 km. The South American Moho lies at 28–35 km depth in forearc regions that have experienced ridge subduction, in contrast to crustal thicknesses ranging from 34 to 55 km beneath regions north of the Chile triple junction. Inboard, the prevailing Moho depth of ∼35 km shallows to ∼30 km along an E-W trend between 46.5°S and 47°S; we relate this structure to Paleozoic thrust emplacement of the Proterozoic Deseado Massif terrane above the thicker crust of the North Patagonian/Somún Cura terrane along a major south-dipping fault.


Sign in / Sign up

Export Citation Format

Share Document