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The steering filter methodology has the most potential as a regularization
operator in large inversion problems. For our final example
we use inverse steering-filters in conjunction with another
operator, in this case a tomography operator, to improve the
inversion result.
For our tomography operator we chose Toldi's
interval to stacking velocity operatorToldi (1985).
Generally, Toldi1985 related perturbations in
interval slowness
to perturbations in stacking slowness
in simple slowness models.
We constructed a synthetic interval slowness perturbation model (Figure
toldi-steer, left panel) where the perturbations from zero follow a
sinusoidal path, and the anomalies go from positive to negative as you go
from left to right.
We used Toldi's forward operator to compute
stacking velocities at various depth levels (Figure toldi-stack,
left panel), in this case we simulating collecting stacking velocity at 10
evenly spaced depths (compared to 160 depth locations in our interval
slowness model), assuming a cable length of 2 km.
toldi-steer
Figure 10 Left, slowness perturbation model;
center, inversion result using Laplacian smoother; right, inversion result
using steering filters.
toldi-stack
Figure 11 Left, input stacking slowness;
right, calculated stacking slowness of steering filter inversion model.
We applied a fairly traditional inversion methodology to estimate
our interval velocity perturbations:
|  |
(20) |
| (21) |
Where
, is the Toldi operator;
, is a Laplacian smoother;
, is our interval slowness perturbation model; and
, is
our data, stacking slowness perturbations.
The center panel of Figure toldi-steer shows the inversion result.
We tried a variety of
values, selecting one that
created a rough
model, but did a fairly good job recovering the correct interval velocity
perturbations.
Next, we attempted to recover the interval slowness perturbations, starting
from the same stacking slowness perturbations, using the
steering filter
methodology.
We constructed our steering filters to follow the sinusoidal pattern of the
model and changed our fitting goal to:
|  |
(22) |
| (23) |
where
is our steering filter matrix. As the right panel of
Figure toldi-steer shows we did a substantially better job
following ``geology'', with the added benefit of better vertically
constraining the interval slowness perturbations.
Next: FUTURE WORK AND CONCLUSIONS
Up: Clapp, et al.: Steering
Previous: SHOT-GATHER BASED INTERPOLATION
Stanford Exploration Project
9/12/2000