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References

 
l1
l1
Figure 6
Semblance computed along moveout trajectories for possible source locations in 3-D. Each panel corresponds to a different depth. The limits of each picture are the boundaries of the array. Data in the low-frequency range (10-60 Hz) were used, and not surprisingly noise from pumps on the surface dominates the results.
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gl1
Figure 7
Maximum value of semblance from Figure 6 as a function of depth. Verifies that surface sources dominate.
gl1
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l2
Figure 8
Same semblance computation in 3-D as Figure 6, but for record 2. Surface noise sources dominate again.
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gl2
Figure 9
Maximum value of semblance vs. depth for Figure 8. Surface sources are not as dominant as in record 1.
gl2
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h1
Figure 10
Semblance computation in 3-D for record 1, using the high frequency range (40-120 Hz) over which pump noise is less dominant. Unlike the low-frequency case (Figure 6), here there are large semblance values at depth.
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gh1
Figure 11
Maximum value of semblance as a function of depth for Figure 10. Note the increase at around 700 meters, suggesting that non-surface sources are present.
gh1
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h2
Figure 12
Same semblance computation as Figure 10, but for record 2.
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gh2
Figure 13
Maximum value of semblance vs. depth for Figure 12. Here also there is a semblance increase at depth.
gh2
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Next: About this document ... Up: Cole & Vanyan: An Previous: Acknowledgments
Stanford Exploration Project
1/13/1998