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Figure
(top) shows stacked section after prestack time-migration. Overall, the migrated section
seems well focused, and since the vertical axis is given in time, the position of the reflectors is
affected by the velocity model. The reflectors appear more shaky under areas of complex velocity structure. The
conversion of this data from time to depth will remove such
artificial complexity. Figure
shows common CMP gathers after prestack time migration. Stacking such gathers produces for us the image shown in Figure
(top).
At all times, the moveout is
well aligned, ready to be stacked. Some misalignment appears at CMP location 5000 and 6000 m,
but this is expected considering the complexity of the Marmousi Model.
The confirmation of the accuracy of the migration will allow
its use for velocity estimation, since non-alignment of the moveout cannot be blamed on the migration, and will be only attributed to velocity inaccuracies.
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(top).
Figure
(bottom) shows the stacked section after prestack time migration,
but in depth rather than time. Using the Marmousi
velocity model for the conversion has rendered more accurate reflector positioning than
that in the time domain. In imaging the reservoir anticline, some fault-like breaks appeared
in the depth image. This can be attributed to the complexity of the model
directly above this region, which might have negatively affected the time-to-depth
conversion. For prestack migration velocity
analysis we have yet to see which domain (depth or time) will result in better convergence
and stability. However, some
preliminary indications favor the time domain (),
simply because horizontal
reflectors are nearly stationary
in such a domain, and moveout from horizontal reflectors provides the majority
of the velocity information in the subsurface.