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This appendix details the computations associated with the
finite-difference solution
to the equation in a 2-D orthogonal Riemannian space.
The 3-D wave equation (22)
takes in two dimensions the simpler form:
| |
(38) |
If we substitute the Fourier-domain wavenumbers by their equivalent
space-domain partial derivatives, we obtain
| |
(39) |
A finite-difference implementation of equation (39)
involving the Crank-Nicolson method is
| |
|
| (40) |
If we make the notations
| |
|
| (41) |
we can write equation (40) as
| |
|
| (42) |
or, if we isolate the terms corresponding to the two extrapolation levels as:
| |
|
| (43) |
After grouping the terms, we obtain
which is a finite-difference representation of the solvable using
fast tridiagonal solvers.
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Up: Sava and Fomel: Riemannian
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Stanford Exploration Project
10/14/2003