is
shown in the upper panels of Figure
. FEAVA is
indicated by a vertical path of high energy in the middle of the image
and is clearly outlined by the FEAVA detector. Non-focused multiples
depart from Shuey's approximation too, but the resulting
FEAVA detector output is one order of magnitude smaller than that
caused by actual focusing. The lower panels of Figure
show the results of migrating with the correct
velocity model, albeit with a single reference velocity. The focusing
is no longer visible in the image. The
focusing-caused FEAVA detector output has fallen significantly, to the
level of power of surrounding multiples. The two FEAVA outputs
are displayed in the same intensity scale.
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FEAVA was clearly reduced by migration, but not entirely
eliminated. One natural question is whether significantly increasing
the number of reference velocities in migration will improve the
outcome. However, a migration with eight reference velocities which
produced the upper panels of Figure
, show
that this is not the case for this type of stratigraphic play. The improvements are
incremental, visible only by electronically displaying the two pictures in an
animated sequence.
Another potential limitation
stems from the fact that, due to the combination of depth/offset sampling Sava and Biondi (2001), the range of angles into
which offsets can be reliably transformed was limited to
, while the FEAVO detector works up to
. Would
energy from greater angles improve the situation? The bottom panels of
Figure
are produced with an offset sampling
four times smaller than before, resulting in reliable transformations
from offset to angle up to
. This does not bring
improvements either. On the contrary, multiples, highly curved at
large angles, create more noise in the FEAVA detector
output. The extra smoothness comes from having decreased the midpoint
sampling by a factor of four.