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To handle faults, I will have to leave the Fourier domain behind. The Fourier based method will estimate erroneous dips across faults. It will then try to honor these erroneous dips creating a result that behaves erratically. However, in the time-space domain, I should be able to handle all faults that have at least one half of the fault tip-line within the data cube. My approach is to create a masking operator (
) that will throw out dip estimates along faults. The method will try to remove all deformation except at the faults where it will allow complete slippage.
I want to find the time shifts,
, such that their gradient (
) is the dip,
. This sums across time-slices and is similar to equation (5). A time-space equivalent of equation (7) has also been implemented. I assume the dip,
, is not a function of the unknown
and write the fitting goal:
|  |
(8) |
This is multiplied by the masking operator (
) to throw out fitting equations at the faults as:
|  |
(9) |
The time shifts (
) can be found in a least-squares sense with:
|  |
(10) |
Next: Faulted model - test
Up: Lomask: Flattening 3-D data
Previous: Integrating dips in the
Stanford Exploration Project
7/8/2003