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The missing data problem is probably the simplest to understand and
interpret. Following the methodology of Claerbout (1999) we solve
the
problem in its preconditioned form using
| ![\begin{eqnarray}
\bf d&\approx& \bf J \bf A^{-1}\bf p\ \nonumber
\bf 0&\approx& \bf I\bf p
,\end{eqnarray}](img8.gif) |
(3) |
| |
where:
- is a binned version of our known points
- is the known data selector
- is the preconditioning operator (in this case equation (2))
- p
- is our preconditioned variable.
To test the interpolation I used the `qdome' dataset (Figure 4).
I began by zeroing 95%
of the original data (Figure 5)
in vertical sections (somewhat simulating well logs).
To obtain the pxz and pyz dip field I used the same methodology
as Fomel (1999) estimating the dip field
from the known data using a non-linear estimation scheme.
mod-orig
Figure 4 3-D qdome model from Claerbout (1999).
mod-in
Figure 5 Decimated qdome model.
95%
of the original traces (Figure 4) have been thrown away.
Using the calculated dip field I then constructed
and
and
iterated 50 times using fitting goals (4).
Figure 6 shows the resulting interpolation. In general
the 3-D steering filters did an excellent job recovering the original data. There is some
lower frequency behavior around the fault boundaries but the fault
position is still quite obvious.
mod-out
Figure 6 Interpolated qdome model starting
from the data in Figure 5. Note how it is a little lower
frequency than Figure 4 but otherwise a near perfect
interpolation result.
Next: Conclusions
Up: Clapp: 3-D steering filters
Previous: 3-D extension
Stanford Exploration Project
9/5/2000