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The main problem with the complex Fourier migration algorithm described above is that it is computationally expensive.
However, by looking at the zero-offset section in Figure 5, we see that simple poststack migration will not
be satisfactory. Since the salt body is present, a depth migration will help to restore the salt to its
correct thickness. Also, with a more complex velocity function, there is a better chance of stacking out a majority of
the multiple energy, which is very dominant in the CMP stack. In poststack migration, the object is to collapse
diffractions, steepen dips, and uncross bow ties.
Using a poststack phase-shift operator, we can put the dips of the synclinal
structure into the correct position, and the bow ties can be uncrossed. However, that is only a very small
part of the image. Moreover, the times of those events are
unlikely to be correct, especially under the salt. After migration it is still
impossible to see under the salt, where the fault blocks are. Therefore, a complex prestack algorithm, though computationally
expensive, becomes necessary in this type of complex geologic setting.
Next: Prestack Migration with P-Wave
Up: Gratwick: Imaging using 2-D
Previous: Migration Algorithm
Stanford Exploration Project
4/27/2000