The crustal structure of the Guayana Shield, Venezuela, from seismic refraction and gravity data

被引:25
|
作者
Schmitz, M
Chalbaud, D
Castillo, J
Izarra, C
机构
[1] FUNVISIS, Caracas, Venezuela
[2] Univ Simon Bolivar, Caracas, Venezuela
[3] Univ Liverpool, Liverpool L69 3BX, Merseyside, England
关键词
seismic refraction; crustal structure; Moho; gravity; Guayana shield;
D O I
10.1016/S0040-1951(01)00208-6
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
We present results from a seismic refraction experiment on the northern margin of the Guayana Shield performed during June 1998, along nine profiles of up to 320 km length, using the daily blasts of the Cerro Bolivar mines as energy source, as well as from gravimetric measurements. Clear Moho arrivals can be observed on the main E-W profile on the shield, whereas the profiles entering the Oriental Basin to the north are more noisy. The crustal thickness of the shield is unusually high with up to 46 km on the Archean segment in the west and 43 km on the Proterozoic segment in the east. A 20 km thick upper crust with P-wave velocities between 6.0 and 6.3 km/s can be separated from a lower crust with velocities ranging from 6.5 to 7.2 km/s. A lower crustal low velocity zone with a velocity reduction to 6.3 km/s is observed between 25 and 25 km depth. The average crustal velocity is 6.5 km/s. The changes in the Bouguer Anomaly, positive (30 mGal) in the west and negative (-20 mGal) in the east, cannot be explained by the observed seismic crustal features alone. Lateral variations in the crust or in the upper mantle must be responsible for these observations. (C) 2002 Elsevier Science B.V. All rights reserved.
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页码:103 / 118
页数:16
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