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11: TRUE AMPLITUDE MIGRATION

Our task will be to choose a kernel $w({\bf r},r)$ that supplies the proportionality of image amplitude and reflection coefficient.

We shall neglect: 1) directional characteristics of the source, 2) refraction coefficients, 3) influence of the free boundary, and 4) variation of the density $\rho$. With these restrictions the amplitude of a wave on the surface $\Sigma$ is:  
 \begin{displaymath}
A_0 (r) = {{c \cdot R} \over {\sqrt{J(s,r)}}} \sqrt{{v(s)} \over {v(r)}}\end{displaymath} (116)
where s and r are the source and receiver locations, $\sqrt{J(s,r)}$describes the geometrical spreading of a wave propagating along the ray $s{\bf r}r$ (see Figure 1), and R is the reflection coefficient at the point ${\bf r}$.

Equation (116) is good for marine surveys. For land surveys we usually measure the vertical component

\begin{displaymath}
\stackrel{\sim}{A_0} (r) = A_0 (r) \cos \theta.\end{displaymath}



 
next up previous print clean
Next: CSP migration, 3D case Up: Goldin: Method of discontinuities Previous: 10: EXTREMAL VELOCITIES
Stanford Exploration Project
1/13/1998