Ff. Pollitz, GLOBAL TOMOGRAPHY FROM RAYLEIGH AND LOVE WAVE-DISPERSION - EFFECT OF RAY-PATH BENDING, Geophysical journal international, 118(3), 1994, pp. 730-758
A large data set of fundamental-mode Rayleigh and Love wave phases has
been employed for global tomographic inversions. These data represent
observations of the first arriving surface waves R(1) and L(1) from a
pproximately 850 seismic events, with about 10 observations of dispers
ion per event. The inversion for laterally varying depth-dependent str
ucture is performed in several steps. At discrete periods from 111 s-2
50 s for Love waves, and from 111s-200 s for Rayleigh waves, we first
determine simultaneously the global distribution of phase-velocity ano
maly and the relocations of the seismic events. Each phase-velocity di
stribution is then corrected for laterally varying Moho depth and bath
ymetry, followed by inversion for 3-D earth structure in the depth ran
ge 0-240 km. In order to lie within the limits of ray theory we restri
ct all model perturbations to a degree 0-16 spherical-harmonic expansi
on. A second-order scattering (ray path) correction is included in the
inversions. The phase-velocity perturbations show a high correlation
with surface tectonics at shorter periods. Comparison of inversions sh
ows that those performed without the ray-path correction exhibit a com
plicated pattern of fast- and slow-velocity bias. The only common feat
ure in the patterns of bias (with respect to period or wave type) is t
hat fast velocity bias is concentrated in regions of large structural
gradient. The amplitude pattern of the depth-dependent model has prono
unced peaks in the intervals 0-70 km and 140-210 km. The deeper peak i
s associated with lateral variations in asthenosphere structure. We de
rive new estimates for the spherically averaged phase velocities of th
e fundamental-mode Rayleigh and Love waves. The spherically averaged p
hase velocities are decreased by about 0.1 per cent by including the r
ay-path correction. These phase-velocity dispersions can be simultaneo
usly fit well with an isotropic model either with or without the ray-p
ath correction, but particularly well when the ray-path correction is
included. In both cases a pronounced low-velocity zone of the global e
xtent is required in the depth range 120-190 km.