Thickness estimates of the upper-mantle transition zone from bootstrapped velocity spectrum stacks of receiver functions

被引:52
作者
Gurrola, H [1 ]
Minster, JB
机构
[1] Texas Tech Univ, Dept Geosci, Lubbock, TX 79409 USA
[2] Univ Calif San Diego, Inst Geophys & Planetary Phys, La Jolla, CA 92093 USA
关键词
receiver functions; transition zone; upper mantle; velocity spectrum stacking;
D O I
10.1046/j.1365-246X.1998.1331470.x
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 modify the receiver-functions stacking technique known as velocity spectrum stacking (VSS) so as to estimate combinations of velocity model (V-P and V-S) and depth that stack the Ps conversion from upper-mantle discontinuities most coherently. We find that by estimating the differences in the depths to the 660 and 410 km discontinuities using velocities that maximize the slacked amplitudes of P410s and P660s phases we can estimate the thickness of the transition zone more accurately than the depths to either of these discontinuities. We present two examples indicating that the transition zone beneath Obninsk, Russia, is 252+/-6 km thick and that beneath Pasadena, California, is only 220+/-6 km thick.
引用
收藏
页码:31 / 43
页数:13
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