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By converting the DSR equation to midpoint-offset space
we will be able to identify the familiar zero-offset migration part
along with corrections for offset.
The transformation between (g,s) recording parameters
and (y,h) interpretation parameters is
| ![\begin{eqnarray}
y \ \ \ \ &=&\ \ \ \ { g \ +\ s \over 2 }
\\ h \ \ \ \ &=&\ \ \ \ { g \ -\ s \over 2 }\end{eqnarray}](img28.gif) |
(15) |
| (16) |
Travel time t may be parameterized in (g,s)-space or (y,h)-space.
Differential relations for this
conversion are given by the chain rule for derivatives:
| ![\begin{eqnarray}
{\partial t \over \partial g} \ \ \ \ &=&\ \ \ \
{\partial t \...
... \over \partial y} \ -\
{\partial t \over \partial h } \, \right)\end{eqnarray}](img29.gif) |
(17) |
| (18) |
Having seen how stepouts transform from shot-geophone space
to midpoint-offset space,
let us next see that spatial frequencies transform in much the same way.
Clearly, data could be transformed from (s,g)-space
to (y,h)-space with (15) and (16)
and then Fourier transformed to ( ky , kh )-space.
The question is then,
what form would the double-square-root equation (13)
take in terms of the spatial frequencies ( ky , kh )?
Define the seismic data field in either coordinate system as
| ![\begin{displaymath}
U ( s, g )\ \eq \ U' ( y , h )\end{displaymath}](img30.gif) |
(19) |
This introduces a new mathematical function U' with the same
physical meaning as U but,
like a computer subroutine or function call,
with a different subscript look-up procedure
for (y,h) than for (s,g).
Applying the chain rule for partial differentiation to (19) gives
| ![\begin{eqnarray}
{ \partial U \over \partial s} \ \ \ \ &=&\ \ \ \
{ \partial y...
...{ \partial h \over \partial g}\ { \partial U' \over \partial h \ }\end{eqnarray}](img31.gif) |
(20) |
| (21) |
and utilizing (15) and (16) gives
| ![\begin{eqnarray}
{ \partial U \over \partial s }\ \ \ \ &=&\ \ \ \
{1 \over 2 }...
...partial y \, }\ +\
{ \partial U' \over \partial h \, } \, \right)\end{eqnarray}](img32.gif) |
(22) |
| (23) |
In Fourier transform space
where
transforms to i kx,
equations (22) and (23),
when i and U = U' are cancelled, become
| ![\begin{eqnarray}
k_s\ \ \ \ &=&\ \ \ \ {1 \over 2 }\ ( k_y\ -\ k_h )
\\ k_g\ \ \ \ &=&\ \ \ \ {1 \over 2 }\ ( k_y\ +\ k_h )\end{eqnarray}](img33.gif) |
(24) |
| (25) |
Equations (24)
and (25)
are Fourier representations of (22) and (23).
Substituting (24) and (25)
into (13) achieves the main purpose of this section,
which is to get the double-square-root migration equation
into midpoint-offset coordinates:
| ![\begin{displaymath}
{\partial\ \over \partial z} \ U\ \ =\ \ -\,i \,
{\omega \o...
..._y \,-\, v k_h \over 2\,\omega } \, \right)^2
\ } \ \right] \ U\end{displaymath}](img34.gif) |
(26) |
Equation (26) is the takeoff point
for many kinds of common-midpoint seismogram analyses.
Some convenient definitions that simplify its appearance are
| ![\begin{eqnarray}
G\ \ \ \ &=&\ \ \ \ { v\ k_g \over \omega }
\\ S\ \ \ \ &=&\ \ ...
...over 2\ \omega }
\\ H\ \ \ \ &=&\ \ \ \ { v\ k_h \over 2\ \omega }\end{eqnarray}](img35.gif) |
(27) |
| (28) |
| (29) |
| (30) |
The new definitions S and G are the sines
of the takeoff angle and of the arrival angle of a ray.
When these sines are at their limits of
they refer
to the steepest possible slopes in (s,t)- or (g,t)-space.
Likewise, Y may be interpreted as the dip of the data as seen
on a seismic section.
The quantity H refers to stepout observed on a common-midpoint gather.
With these definitions (26) becomes slightly less cluttered:
| ![\begin{displaymath}
\begin{tabular}
{\vert c\vert} \hline
\\ $\displaystyle {\...
...\sqrt{1-(Y-H)^2} \ \right) U$\space \\ \\ \hline\end{tabular}\end{displaymath}](img37.gif) |
(31) |
EXERCISES:
-
Adapt equation (26) to allow for a difference in velocity
between the shot and the geophone.
-
Adapt equation (26) to allow for downgoing pressure waves
and upcoming shear waves.
Next: THE MEANING OF THE
Up: SURVEY SINKING WITH THE
Previous: The DSR equation in
Stanford Exploration Project
12/26/2000