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Whether an AGC window or a more careful geometric spreading correction
has been applied, two generations of seismic survey will, in general,
have different time-varying gain functions applied to them. If not
compensated for correctly, this may lead to a systematic leakage of
non-reservoir events into the difference section. Although an
amplitude correction may need to be time and space-varying, it should
be constrained to vary very slowly, so it is not influenced by changes
in the reservoir zone.
The simplest approach to amplitude balancing is to scale the data
based on the r.m.s. energy in the two surveys. However, this assumes
that the energy present in the noise fields are the same in both
datasets, or of much smaller magnitude than the signal energy.
As an illustration we can consider two normalized
datasets, and , to consist of some shared
signal, , and uncorrelated ``noise'' components,
and , which include the reservoir difference
anomaly we seek:
| |
(2) |
| (3) |
In order to rescale the signals to the same level, we need to apply a
scale factor, to , where
| |
(4) |
or again assuming the noise fields are weakly correlated with the
geological signal
| |
(5) |
where s1 and s2 are the signal-to-noise levels in the two
datasets. For high ( and ), or similar (), signal-to-noise levels reduces to unity, and the
equal energy condition is valid.
For the field examples in this paper, the equal energy condition was
used to balance the filter amplitudes. This is a reasonable assumption
for many examples, and does not require independent estimates of the
signal-to-noise ratio.
Next: Warping
Up: Rickett & Lumley: Cross-equalizing
Previous: Matched-filtering
Stanford Exploration Project
7/5/1998