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The synthetic modeling results confirm the point that near surface velocity
variations create not only timing anomalies, but also focusing anomalies.
These focusing anomalies cannot be compensated for by static shift.
Near surface variations cause distinct trajectories in midpoint-offset plots
of trace power.
Preliminary results show that slant stack imaging based on these power plots
can be used to locate velocity perturbations. Once these perturbations
are located, the seismic wavefield can be extrapolated through the near
surface to iteratively estimate velocity.
Much work remains to be done in order to implement
and link these two steps, but the
results presented here are encouraging.
Next: REFERENCES
Up: Bevc: Near surface v(x,z)
Previous: Downward continuation
Stanford Exploration Project
11/16/1997