scholarly journals Crust and upper mantle velocity structure of the Yellowstone hot spot and surroundings

2008 ◽  
Vol 113 (B3) ◽  
Author(s):  
Derek L. Schutt ◽  
Ken Dueker ◽  
Huaiyu Yuan
Keyword(s):  
Upper Mantle ◽  
Velocity Structure ◽  
Hot Spot ◽  
Crust And Upper Mantle ◽  
Mantle Velocity

scholarly journals Crust and upper mantle velocity structure of the northwestern Indian Peninsular Shield from inter-station phase velocities of Rayleigh and Love waves

2015 ◽  
Vol 58 (2) ◽  
Author(s):  
Gaddale Suresh ◽  
Sankar N. Bhattacharya ◽  
Satbir S. Teotia
Keyword(s):  
Upper Mantle ◽  
Rayleigh Waves ◽  
Velocity Structure ◽  
Love Waves ◽  
Upper Crust ◽  
Crust And Upper Mantle ◽  
Phase Velocities ◽  
South Indian ◽  
Mantle Velocity ◽  
Peninsular Shield

<p>We measure the inter-station Rayleigh and Love wave phase velocities across the northwestern Indian Peninsular shield (NW-IP) through cross-correlation and invert these velocities to evaluate the underneath crust and upper mantle velocity structure down to 400 km. We consider a cluster of three stations in the northern tip of the Peninsula and another cluster of eight stations in the south. We measure phase velocities along 28 paths for Rayleigh waves and 17 paths for Love waves joining two stations with one from each cluster and using broadband records of earthquakes which lie nearly on the great circle joining the pair of stations. The phase velocities are in the period range of 10 to 275 s for Rayleigh waves and of 10 to 120 s for Love waves. The isotropic model obtained through inversion of the phase velocities indicates 199.1 km thick lithosphere with 3-layered crust of thickness 36.3 km; the top two layers have nearly same velocities and both constitute the upper crust with thickness of 12.6 km. The upper crust is mafic, whereas the lower crust is felsic. In the mantle lid, velocities increase with depth. The velocities of mantle lid beneath NW-IP is lower than those beneath south Indian Peninsula showing the former is hotter than the later perhaps due to large Phanerozoic impact on NW-IP. The significant upper mantle low velocity zone beneath NW-IP indicates high temperature which could be attributed to the past existence of a broad plume head at the west-central part of the Peninsula.</p>

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