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01.perturbation
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.
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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.
01.inversion
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05.perturbation
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.
[*] view burn build edit restore

 
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.
05.inversion
[*] view burn build edit restore

 
20.perturbation
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.
[*] view burn build edit restore

 
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.
20.inversion
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40.perturbation
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.
[*] view burn build edit restore

 
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.
40.inversion
[*] view burn build edit restore

 

 

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:
228#228 (98)
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,
230#230 (99)
We can approximate the change in travel time due to a change in reflector movement by
231#231 (100)
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,
233#233 (101)
If we note that the travel time of the normal ray is independent of velocity we can write
234#234 (102)
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,
235#235 (103)
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,
239#239
(104)
If we combine this new fitting goal with our tomographic fitting goal and our regularization fitting goal we get,
   240#240
(105)

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
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.
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amoco-vel0
amoco-vel0
Figure 2
The left panel shows the initial velocity model. The right panel shows the result of migrating with this velocity model.
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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.
picked
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amoco-vel1.steer
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.
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amoco-vel1.steer-ref
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 [*].
[*] view burn build edit restore

 
amoco-vel4.steer
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.
[*] view burn build edit restore

 
amoco-vel4.steer-ref
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 [*].
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Next: CONCLUSIONS Up: Prucha and Biondi: STANFORD Previous: Conclusions
Stanford Exploration Project
6/7/2002