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Our work up to this point has concentrated on analysis of the 2-D synthetic
model. To analyze the finite-difference generated data we began by
constructing travel time maps using a fast-marching eikonal solver
(). The pre-stack Kirchhoff depth migrated
common-offset
sections obtained by this method can be seen in Figure
.
The depth migration code used was developed by us using Genkir3D, a package
designed to aid in the development of Kirchhoff imaging applications.
().
Figure
displays many interesting features. The only
processing that has been done is pre-stack Kirchhoff depth migration followed
by stacking the common offset sections. Comparing the stacked section to
the velocity model shows that we have done a good job of imaging even the
steeply dipping reflectors. However, there are fairly strong migration
artifacts and noise in the area beneath the edge of the salt. The most
interesting feature is on the reflector we wish to image almost directly
beneath the edge of the salt body. The strong reflector suddenly disappears
then reappears as a faint event. This corresponds with
Figure
which shows common reflector point (CRP) gathers
illustrating that away from the edge of the salt we did flatten the events
and the reflector is quite strong but near the salt our reflector becomes
practically non-existent. It is this intriguing behavior that we examine next.
overlay2.full
Figure 4 Raypaths through the synthetic model
impinging on the problem section of the reflector
stack.v
Figure 5 PSDM synthetic result using the eikonal
solver to find traveltimes
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Stanford Exploration Project
7/5/1998