Bc. Zelt et al., INVERSION OF 3-DIMENSIONAL WIDE-ANGLE SEISMIC DATA FROM THE SOUTHWESTERN CANADIAN CORDILLERA, J GEO R-SOL, 101(B4), 1996, pp. 8503-8529
Seismic refraction/wide-angle reflection data were recorded on a trian
gular array in southwestern British Columbia centered on the boundary
between the Coast Belt to the southwest and the Intermontane Belt to t
he northeast. The experiment, part of the Lithoprobe Southern Cordille
ra transect, enabled determination of the three-dimensional (3-D) velo
city structure of the crust and upper mantle. An algorithm for the inv
ersion of wide-angle seismic data to determine 3-D velocity structure
and depth to reflecting interfaces is developed. The algorithm is base
d on existing procedures for the inversion and forward modeling of fir
st arrival travel times and forward modeling of reflection travel time
s, including (1) forward modeling using a 3-D finite difference algori
thm; and (2) a simple velocity model parameterization for the inversio
n which eliminates the need to solve a large system of equations. The
existing procedure is extended to allow (1) the inversion of reflectio
n times to solve for depth to a reflecting interface and/or velocity s
tructure; (2) the inversion of first arrival travel times to solve for
depth to a refracting interface; and (3) layer stripping. Application
of the algorithm to southern Cordillera data uses P-g to constrain up
per crustal velocity structure, PmP to constrain lower crustal velocit
y structure and depth to Moho, and P-n to constrain upper mantle veloc
ities and depth to Moho. The 3-D velocity model for the southwestern C
anadian Cordillera is characterized by (1) significant lateral velocit
y variations at all depths that do not, in general, correlate with sur
face geological features or gravity data; (2) a relatively high veloci
ty middle and lower,crust in the southwestern part of the study area w
hich correlates with a Strong relative gravity high and outlines the e
astern extent of lower Wrangellia, an accreted terrane forming the Ins
ular Belt to the west; (3) a narrow zone of slower velocity in the low
er crust and change in crustal thickness associated with the Fraser Fa
ult system, lending additional support to the view that it is a crusta
l penetrating fault; (4) an average upper mantle velocity of 7.85 km/s
; and (5) a depth to Moho of 33-36 lan in the Intermontane Belt and 36
-38 lan throughout most of the Coast Belt, decreasing in the west to 3
3 lan near the Insular-Coast contact. Horizontal velocity structure sl
ices and an interpreted cross section based on these and other results
show the complexity of crustal structure in the region.