The customary numerical solution to the x-domain forms of the equations
in Tables .3 and
.4 is arrived at by splitting.
That is, you march forward a small
-step alternately
with the two extrapolators
![]() |
(18) | |
(19) |
![]() |
(20) |
Migrations that include the lens equation are called depth migrations. The term is often omitted, giving a time migration.
Observe that the diffraction parts of Tables .3 and
.4 are the same.
Let us use them and equation (19) to
define a table of diffraction equations.
Substitute
for i kx and
clear
from the denominators to
get Table
.5.