We develop a tomographic inversion method that uses teleseismic P wave
polarization data to obtain velocity structure. Polarization inversio
n has some intrinsic advantages over travel Lime inversion: It is not
influenced by source location and origin time errors; it is not sensit
ive to deep mantle velocity structure and can be used iteratively to i
mprove the tomographic result. Polarization inversion is more sensitiv
e to near-station velocity structure and to velocity gradient and is c
omplementary to travel time inversion in this sense. The method is app
lied to California Institute of Technology-U.S. Geological Servey sout
hern California array data. The result is generally consistent with pr
evious work and also reveals that the high-velocity feature beneath th
e Transverse Ranges is bounded between 40 and 200 km depths and possib
ly has a second small piece at about 300 km depth. The slow velocity a
nomaly under the Salton Trough is limited to shallow depths, less than
about 60 km.