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The DSR equation in midpoint-offset space

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

$\displaystyle y     $ $\textstyle =$ $\displaystyle     { g  + s \over 2 }$ (15)
$\displaystyle h     $ $\textstyle =$ $\displaystyle     { g  - s \over 2 }$ (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:
$\displaystyle {\partial t \over \partial g}     $ $\textstyle =$ $\displaystyle    \
{\partial t \over \partial y}  {\partial y \over \parti...
...( {\partial t \over \partial y}  +\
{\partial t \over \partial h }   \right)$ (17)
$\displaystyle {\partial t \over \partial s}     $ $\textstyle =$ $\displaystyle    \
{\partial t \over \partial y}  {\partial y \over \parti...
...( {\partial t \over \partial y}  -\
{\partial t \over \partial h }   \right)$ (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 (9.15) and (9.16) and then Fourier transformed to $ ( k_y , k_h ) $-space. The question is then, what form would the double-square-root equation (9.13) take in terms of the spatial frequencies $ ( k_y , k_h ) $? Define the seismic data field in either coordinate system as

\begin{displaymath}
U ( s, g ) \eq  U' ( y , h )
\end{displaymath} (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 (9.19) gives
$\displaystyle { \partial U \over \partial s}     $ $\textstyle =$ $\displaystyle    \
{ \partial y \over \partial s}  { \partial U' \over \pa...
...y  }  +\
{ \partial h \over \partial s}  { \partial U' \over \partial h  }$ (20)
$\displaystyle { \partial U \over \partial g}    $ $\textstyle =$ $\displaystyle    \
{ \partial y \over \partial g}  { \partial U' \over \pa...
...l y  } +\
{ \partial h \over \partial g} { \partial U' \over \partial h  }$ (21)

and utilizing (9.15) and (9.16) gives
$\displaystyle { \partial U \over \partial s}     $ $\textstyle =$ $\displaystyle    \
{1 \over 2 } \left( { \partial U' \over \partial y   } -\
{ \partial U' \over \partial h   }   \right)$ (22)
$\displaystyle { \partial U \over \partial g}    $ $\textstyle =$ $\displaystyle    \
{1 \over 2 } \left( { \partial U' \over \partial y   } +\
{ \partial U' \over \partial h   }   \right)$ (23)

In Fourier transform space where $ \partial / \partial x $ transforms to $ i k_x $, equations (9.22) and (9.23), when $i$ and $U = U' $ are cancelled, become
$\displaystyle k_s    $ $\textstyle =$ $\displaystyle     {1 \over 2 } ( k_y - k_h )$ (24)
$\displaystyle k_g    $ $\textstyle =$ $\displaystyle     {1 \over 2 } ( k_y + k_h )$ (25)

Equations (9.24) and (9.25) are Fourier representations of (9.22) and (9.23). Substituting (9.24) and (9.25) into (9.13) 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} (26)

Equation (9.26) is the takeoff point for many kinds of common-midpoint seismogram analyses. Some convenient definitions that simplify its appearance are

$\displaystyle G    $ $\textstyle =$ $\displaystyle     { v k_g \over \omega }$ (27)
$\displaystyle S    $ $\textstyle =$ $\displaystyle     { v k_s \over \omega }$ (28)
$\displaystyle Y    $ $\textstyle =$ $\displaystyle     { v k_y \over 2 \omega }$ (29)
$\displaystyle H    $ $\textstyle =$ $\displaystyle     { v k_h \over 2 \omega }$ (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 $ \pm 1 $ 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 (9.26) becomes slightly less cluttered:
\begin{displaymath}
\begin{tabular}{\vert c\vert} \hline
 $\displaystyle {\st...
... +
\sqrt{1-(Y-H)^2}  \right) U$ \\
 \hline
\end{tabular}\end{displaymath} (31)

EXERCISES:

  1. Adapt equation (9.26) to allow for a difference in velocity between the shot and the geophone.
  2. Adapt equation (9.26) to allow for downgoing pressure waves and upcoming shear waves.


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Next: THE MEANING OF THE Up: SURVEY SINKING WITH THE Previous: The DSR equation in

2009-03-16