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Figure 3 shows the velocity as a function
of depth at one surface location in the area where the salt body
does not interfere with the fault reflections.
Although the velocity gradient of about is relatively mild in absolute terms,
it is the strongest within this salt model.
The effects of the vertical gradient on the moveouts
of the reflections after DMO and AMO are measurable,
but not too strong.
Figure 4 shows the moveouts
of the reflection from the fault at a typical
CMP location in the area.
As expected, the moveout after simple binning (a)
points upward with offset, because of the dip effect.
Also not surprisingly, the
moveout after DMO (c) points downward with offset.
Hale and Artley 1993,
and several others authors,
showed that
constant-velocity DMO overcorrects the moveouts
in a horizontally layered medium
with velocity increasing with depth.
In contrast, the moveout from the fault
reflection is approximately flat after AMO (b).
The simple explanation of these results is that
AMO is a residual operator and consequently
moves energy less than DMO does.
Therefore, it overcorrects the moveout less than
constant velocity DMO.
In some respects, it behaves similarly
to the ``squeezed DMO'' presented by
Hale and Artley 1993.
Next: NMO-velocity conflict
Up: Tests on the SEG/EAGE
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Stanford Exploration Project
7/5/1998