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01.perturbation
Figure 5 Anomaly of 1222#222: linear and non-linear image
perturbations (left/right); zero offset section (top) and selected
angle-gathers (bottom) corresponding to the locations of the
vertical lines in the upper panel. Large differences between
the linear and non-linear image perturbations indicate
situations in which we violate the Born approximation.
01.inversion
Figure 6 Anomaly of 1222#222: inversion from the non-linear
image perturbation ( ) using the explicit (top),
bilinear (middle) and implicit (bottom) WEMVA operators.
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05.perturbation
Figure 7 Anomaly of 5222#222: linear and non-linear image
perturbations (left/right); zero offset section (top) and selected
angle-gathers (bottom) corresponding to the locations of the
vertical lines in the upper panel. Large differences between
the linear and non-linear image perturbations indicate
situations in which we violate the Born approximation.
05.inversion
Figure 8 Anomaly of 5222#222: inversion from the non-linear
image perturbation ( ) using the explicit (top),
bilinear (middle) and implicit (bottom) WEMVA operators.
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20.perturbation
Figure 9 Anomaly of 20222#222: linear and non-linear image
perturbations (left/right); zero offset section (top) and selected
angle-gathers (bottom) corresponding to the locations of the
vertical lines in the upper panel. Large differences between
the linear and non-linear image perturbations indicate
situations in which we violate the Born approximation.
20.inversion
Figure 10 Anomaly of 20222#222: inversion from the non-linear
image perturbation ( ) using the explicit (top),
bilinear (middle) and implicit (bottom) WEMVA operators.
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40.perturbation
Figure 11 Anomaly of 40222#222: linear and non-linear image
perturbations (left/right); zero offset section (top) and selected
angle-gathers (bottom) corresponding to the locations of the
vertical lines in the upper panel. Large differences between
the linear and non-linear image perturbations indicate
situations in which we violate the Born approximation.
40.inversion
Figure 12 Anomaly of 40222#222: inversion from the non-linear
image perturbation ( ) using the explicit (top),
bilinear (middle) and implicit (bottom) WEMVA operators.
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Short Note
Matching dips in velocity estimation
Robert G. Clapp
bob@sep.stanford.edu
Accurate velocity estimation is essential to obtain
a good migrated image and accurate resevoir attributes ().
The problem is that
tomographic velocity estimation is an underdetermined problem.
We can reduce the null space of the tomographic
process by adding additional constraints, or
more accurate goals, to the estimation.
In early work (, , , ) I discussed one such constraint:
encouraging velocity follows dip.
Often we have an added constraint; although we may
be unsure of reflector position
(due to anisotropy, etc.) or we may have a good estimate of
reflector dip (either
from well logs, geologic models, etc). By
incorporating this information into the
inversion we can better constrain the inversion process.
This method is tested on a fairly complicated synthetic dataset.
THEORY
Tomography is a non-linear problem that we linearize
around an initial slowness model. In this discussion I will
be talking about the specific case of ray based tomography but
most of the discussion is valid for other tomographic operators.
We can linearize the problem around an initial slowness model and
obtain a linear relation 223#223 between
the change in travel times 224#224 and
change in slowness 141#141 and reflector position 225#225. We
break up our tomography operator into its two parts, changes
due to slowness along the ray 226#226 and changes due to reflector movement
227#227:
Inverting for both 141#141 and 225#225 is an unstable process.
We can improve stability by introducing another operator 229#229 which maps slowness
changes to reflector changes,
We can approximate the change in travel time
due to a change in reflector movement by
where 232#232 is the velocity at the reflector,
5#5 is the reflector dip, and 4#4 is the
reflection angle ().
We can approximate the change in reflector
position due to a change in slowness by assuming
movement normal to the reflector and integrating
along the normal ray,
If we note that the travel time of the normal ray
is independent of velocity we can write
where t0 is the travel time in the initial model and
t1 is the travel time through the new model.
If we ignore the second order term,
The reason for this review is that our mapping of
slowness change to reflector movement leads to a
way to approximate reflector dip in the post-tomographic domain.
For simplicity let's concern ourselves with the 2-D problem, though
it's easily extendible to 3-D.
Imagine that 236#236 represents our a priori reflector dip, 110#110 is a
derivative operator, 237#237 is our final reflector dip,
238#238 is the initial reflector position,
and 225#225 is our change in reflector position. We can derive
a fairly simple fitting goal relating reflector dip
and 141#141,
If we combine this new fitting goal with our tomographic
fitting goal and our regularization fitting goal we get,
EXAMPLE
To test the methodology I decided to use a synthetic 2-D dataset generated
by BP based on a typical North Sea environment, Figure
.
To avoid tomography's problem with sharp velocity contrasts I
chose to assume an accurate knowledge of the velocity
structure down to 1.8 km. For the remaining initial velocity structure
I smoothed the correct velocity. Figure
shows
the initial velocity model and initial migration.
amoco-vel-cor
Figure 1 The left panel shows the correct
velocity model. The right panel shows the result of migrating
with this velocity model.
amoco-vel0
Figure 2 The left panel shows the initial
velocity model. The right panel shows the result of migrating
with this velocity model.
I then performed two different series of tomography loops.
In the first case I used a standard approach, without the
constraint on dip of the basement reflector at 4 km.
Figure
shows the initial migration with
my pick of the reflector position overlaid (238#238 in
fitting goals (
)). Figures
and
show the velocity and migration
result after a single non-linear iteration of tomography using
both approaches.
In the first iteration
the velocity structure looks somewhat more accurate without
the dip constraint.
The image tells a different story. Note
how the bottom reflector is much flatter using the dip constraint
condition (Figure
) and the overall image
positioning is a little better. After four iterations, we see a more
dramatic difference. Without the dip constraint condition (Figure
)
the velocity model is having trouble converging, especially along
the right edge. The bottom reflector is quite discontinuous and
misplaced. The overall image quality is disappointing. With the dip
constraining condition (Figure
)
the velocity model is correctly finding the salt boundaries. The
bottom reflector is fairly flat, consistent, and well positioned.
The overall image quality is better than the result without
the dip constraint.
picked
Figure 3 The initial migrated model
overlaid by the picked initial reflector position.
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amoco-vel1.steer
Figure 4 The left panel shows the
velocity model after one iteration of
`conventional' tomography. The right panel shows the result of migrating
with the velocity model in the left panel.
amoco-vel1.steer-ref
Figure 5 The left panel shows the
velocity model after one iteration of
tomography with a dip constraint. The right panel shows the result of migrating
with the velocity model in the left panel.
Note the more continuous nature of the bottom reflector (compared
to Figure
.
amoco-vel4.steer
Figure 6 The left panel shows the
velocity model after four iteration of
`conventional' tomography. The right panel shows the result of migrating
with the velocity model in the left panel.
amoco-vel4.steer-ref
Figure 7 The left panel shows the
velocity model after four iteration of
tomography with a dip constraint. The right panel shows the result of migrating
with the velocity model in the left panel.
Note the more continuous nature of the bottom reflector, better constraining
of the salt boundaries, and overall more accurate imaging focusing
and positioning compared to the result without the added constraint (Figure
.
Next: CONCLUSIONS
Up: Prucha and Biondi: STANFORD
Previous: Conclusions
Stanford Exploration Project
6/7/2002