HR: 1340h
AN: S53B-0224 [Abstracts]
TI: High-Resolution Tomography of the Kaapvaal Craton
AU: * Chevrot, S
EM: Sebastien.Chevrot@cnes.fr
AF: Observatoire Midi Pyrenees, 14 Avenue Edouard Belin, Toulouse, 31400
France
AU: Zhao, L
EM: zhaol@usc.edu
AF: Department of Earth Sciences, University of Southern California, Los Angeles, CA 90089-0740
United States
AB:
We present the results of a tomographic study using the broadband
waveforms recorded by the Kaapvaal Seismic Array deployed in
Southern Africa between 1997 and 1999. The Kaapvaal array is
composed of about 80 stations at an average spacing of ~100 km.
We accurately measure the phase delays between the
different stations using a waveform cross-correlation method.
For each event, we compute and subtract the average
of all the measurements to reduce the effect of structures
outside the array. The dataset is composed of phase delays of broadband {\it{SH}} waves
as well as narrowband Rayleigh waves at a number of frequencies
between 0.01 Hz and 0.04 Hz. A crustal correction is applied to
the phase-delay measurements before they are inverted using
an LSQR algorithm. We use a normal-mode coupling method to compute the Fr{\'{e}}chet
(sensitivity) kernels for the Rayleigh waves and
a normal-mode-ray-theory hybrid approach to compute
the kernels for the {\it{SH}} waves. This hybrid approach is
adopted to ensure both the efficiency of the calculations
with a 10-km grid spacing for the {\it{SH}} waves and the accuracy
of the kernels in the near and intermediate fields from the
seismic stations.
The resulting shear-wave speed model has similar patterns to
the shear-wave model for the Kaapvaal region (James et al. 2001)
but covers a broader area. The wave-speed anomalies show
good correlation with surface geology, in particular with the
limits of the cratonic blocks. The upper mantle beneath the Kaapvaal craton is characterized
by high wave speed reaching at least 300-km depth. One of the
interesting features of our model is a low-speed region
in the upper mantle to the east of the Kimberley Array
which coincides with the suture between the Witwatersrand and
the Kimberley blocks.
DE: 7218 Lithosphere and upper mantle
SC: Seismology [S]
MN: 2004 AGU Fall Meeting