scholarly journals Crustal velocity structure of the Deccan Volcanic Province, Indian Peninsula, from observed surface wave dispersion

2014 ◽  
Vol 57 (4) ◽  
Author(s):  
Gaddale Suresh ◽  
Satbir S. Teotia ◽  
Sankar N. Bhattacharya
Keyword(s):  
Wave Velocity ◽  
Rayleigh Waves ◽  
Velocity Structure ◽  
Crustal Thickness ◽  
P Wave ◽  
Upper Crust ◽  
S Wave ◽  
Deccan Volcanic Province ◽  
Epicentral Zone ◽  
Volcanic Province

<p>Through inversion of fundamental mode group velocities of Love and Rayleigh waves, we study the crustal and subcrustal structure across the central Deccan Volcanic Province (DVP), which is one of the world’s largest terrestrial flood basalts. Our analysis is based on broadband seismograms recorded at seismological station Bhopal (BHPL) in the central India from earthquakes located near west coast of India, with an average epicentral distance about 768 km. The recording station and epicentral zone are situated respectively on the northern and southern edges of DVP with wave paths across central DVP. The period of group velocity data ranges from 5 to 60 s for Rayleigh waves and 5 to 45 s for Love waves. Using the genetic algorithm, the observed data have been inverted to obtain the crust and subcrustal velocity structure along the wavepaths. Using this procedure, a similar velocity structure was also obtained earlier for the northwestern DVP, which is in the west of the present study region. Comparison of results show that the crustal thickness decreases westward from central DVP (39.6 km) to northwestern DVP (37.8 km) along with the decrease of thickness of upper crust; while the thickness of lower crust remains nearly same. From east to west S-wave velocity in the upper crust decreases by 2 to 3 per cent, while P-wave velocity in the whole crust and subcrust decreases by 3 to 6 per cent. The P- and S-wave velocities are positively correlated with crustal thickness and negatively correlated with earth’s heat flow. It appears that the elevated crustal and subcrustal temperature in the western side is the main factor for low velocities on this side.</p>

Mapping crustal structure of the Nechako–Chilcotin plateau using teleseismic receiver function analysis,

2014 ◽  
Vol 51 (4) ◽  
pp. 407-417 ◽  
Author(s):  
H.S. Kim ◽  
J.F. Cassidy ◽  
S.E. Dosso ◽  
H. Kao
Keyword(s):  
Wave Velocity ◽  
Crustal Structure ◽  
Velocity Structure ◽  
Receiver Function ◽  
Function Analysis ◽  
Crustal Thickness ◽  
Receiver Functions ◽  
S Wave ◽  
Low Velocity ◽  
Velocity Models

This paper presents results of a passive-source seismic mapping study in the Nechako–Chilcotin plateau of central British Columbia, with the ultimate goal of contributing to assessments of hydrocarbon and mineral potential of the region. For the present study, an array of nine seismic stations was deployed in 2006–2007 to sample a wide area of the Nechako–Chilcotin plateau. The specific goal was to map the thickness of the sediments and volcanic cover, and the overall crustal thickness and structural geometry beneath the study area. This study utilizes recordings of about 40 distant earthquakes from 2006 to 2008 to calculate receiver functions, and constructs S-wave velocity models for each station using the Neighbourhood Algorithm inversion. The surface sediments are found to range in thickness from about 0.8 to 2.7 km, and the underlying volcanic layer from 1.8 to 4.7 km. Both sediments and volcanic cover are thickest in the central portion of the study area. The crustal thickness ranges from 22 to 36 km, with an average crustal thickness of about 30–34 km. A consistent feature observed in this study is a low-velocity zone at the base of the crust. This study complements other recent studies in this area, including active-source seismic studies and magnetotelluric measurements, by providing site-specific images of the crustal structure down to the Moho and detailed constraints on the S-wave velocity structure.

S-Wave Velocity Structure of the Middle and Upper Crust Beneath the Yunnan Region

2004 ◽  
Vol 47 (5) ◽  
pp. 946-953 ◽  
Author(s):  
Zheng-Qin HE ◽  
Tai-Lan YE ◽  
Wei SU
Keyword(s):  
Wave Velocity ◽  
Velocity Structure ◽  
Upper Crust ◽  
S Wave ◽  
Yunnan Region

Crustal Structure of Eastern North Carolina: Piedmont and Coastal Plain

2019 ◽  
Vol 109 (6) ◽  
pp. 2288-2304 ◽  
Author(s):  
Shuai Zhao ◽  
Wenbin Guo
Keyword(s):  
North Carolina ◽  
Wave Velocity ◽  
Coastal Plain ◽  
Lower Crust ◽  
Thin Layers ◽  
P Wave ◽  
Upper Crust ◽  
S Wave ◽  
The West ◽  
Atlantic Margin

Abstract We present the results from an onshore seismic refraction and wide‐angle reflection profile, conducted in 2015, across the coastal plain and eastern Piedmont provinces of North Carolina. We use forward modeling to create 1D synthetic seismogram models and then invert first break picks to create 2D P‐ and S‐wave velocity models. The crustal thickness is 38 km beneath the Piedmont and central coastal plain, but it thins to 32 km at the coastline. The average thickness of the upper crust is 11 km with an average P‐wave velocity (VP) of 6.0  km/s and S‐wave velocity (VS) of 3.5  km/s. A prominent seismic low‐velocity zone (LVZ) (VP<6.0 and VS<3.6  km/s) exists between the depths of 6 and 11 km, beneath the western third of the seismic profile. The middle crust varies greatly in thickness, increasing from 3 km in the west (eastern Piedmont) to 13 km in the east (coastal plain), with seismic velocities of 6.5  km/s for VP and 3.8  km/s for VS. The lower crust thins significantly toward the rifted Atlantic margin, decreasing from 24 km thick in the west (Piedmont) to 8 km at the coastline, with velocities of approximately 6.9  km/s for VP and 3.9  km/s for VS. We estimate the composition of the crust by comparing the measured values of VP and Poisson’s ratio with laboratory measurements. The upper and middle crusts are in agreement with a felsic composition, while the lower crustal composition is predominately felsic to intermediate. The LVZ in the upper crust is associated with thin layers of the mylonitic rocks involved in the top and the bottom of thrusting, and the top of the lower crust could be the master detachment fault during the thin‐skinned Alleghanian orogeny. The eastward thinning of the lower crust is consistent with crustal extension during the Mesozoic rifting of the Atlantic margin.

Joint inversion of receiver functions and apparent incidence angles to investigate the crustal structure of Mars

2021 ◽  
Author(s):  
Rakshit Joshi ◽  
Brigitte Knapmeyer-Endrun ◽  
Klaus Mosegaard ◽  
Felix Bissig ◽  
Amir Khan ◽  
...  
Keyword(s):  
Wave Velocity ◽  
Crustal Structure ◽  
Joint Inversion ◽  
Landing Site ◽  
Crustal Thickness ◽  
Receiver Functions ◽  
P Wave ◽  
S Wave ◽  
Data Set ◽  
Insight Mission

&lt;p&gt;Since InSight (the Interior Exploration using Geodesy and Heat Transport) landed 26 months ago and deployed an ultra sensitive broadband seismometer(SEIS) on the surface of Mars, around 500 seismic events of diverse variety have been detected, making it possible to directly analyze the subsurface properties of Mars for the very first time. One of the primary goals of the mission is to retrieve the crustal structure below the landing site. Current estimates differ by more than 100% for the average crustal thickness. Since data from orbital gravity measurementsprovide information on relative variations of crustal thickness but not absolute values, this landing site measurement could serve as a tie point to retrieve global crustal structure models. To do so, we propose using a joint inversion of receiver functions and apparent incidence angles, which contain information on absolute S-wave velocities of the subsurface. Since receiver function inversions suffer from a velocity depth trade-off, we in addition exploit a simple relation which defines apparent S-wave velocity as a function of observed apparent P-wave incidence angles to constrain the parameter space. Finally we use the Neighbourhood Algorithm for the inversion of a suitable joint objective function. The resulting ensemble of models is then used to derive the full uncertainty estimates for each model parameter. Before its application on data from InSight mission, we successfully tested the method on Mars synthetics and terrestrial data from various geological settings using both single and multiple events. Using the same method, we have previously been able to constrain the S-wave velocity and depth for the first inter-crustal layer of Mars between 1.7 to 2.1 km/s and 8 to 11 km, respectively. Here we present the results of applying this technique on our selected data set from the InSight mission. Results show that the data can be explained equally well by models with 2 or 3 crustal layers with constant velocities. Due to the limited data set it is difficult to resolve the ambiguity of this bi-modal solution. We therefore investigate information theoretic statistical tests as a model selection criteria and discuss their relevance and implications in seismological framework.&lt;/p&gt;&lt;div&gt;&lt;/div&gt;&lt;div&gt;&lt;/div&gt;&lt;div&gt;&lt;/div&gt;

UPPER MANTLE STRUCTURE IN CANADA FROM SEISMIC OBSERVATIONS USING CHEMICAL EXPLOSIONS

1967 ◽  
Vol 4 (5) ◽  
pp. 961-975 ◽  
Author(s):  
K. G. Barr
Keyword(s):  
Wave Velocity ◽  
Upper Mantle ◽  
Velocity Structure ◽  
P Wave ◽  
Hudson Bay ◽  
S Wave ◽  
Low Velocity ◽  
P Wave Velocity ◽  
Upper Mantle Structure ◽  
Chemical Explosions

Long-range seismic observations at the standard Canadian seismic stations, from chemical explosions in Hudson Bay and Lake Superior, are used to derive a P-wave velocity structure for the upper mantle. The coordinates of observed cusps are used to define the structural discontinuities. These discontinuities are at depths of 126 and 366 km, which agree closely with the depths of the S-wave velocity discontinuities deduced from surface-wave observations. The observations do not require a low velocity layer in the upper mantle.

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