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Given the kinematic equivalence between the water-bottom multiple and a primary
from a reflector dipping at twice the dip angle, we can express the image space
coordinates of the water-bottom multiple in terms of the data space coordinates
by solving the system of equations presented by Fomel and Prucha
1999:
| ![\begin{eqnarray}
t_m&=&\frac{2\hat{Z}_\xi}{V}\frac{\cos\hat{\varphi}\cos\hat{\ga...
...varphi}\cos\hat{\varphi}}{\cos^2\hat{\varphi}-\sin^2\hat{\gamma}},\end{eqnarray}](img22.gif) |
(13) |
| (14) |
| (15) |
where
are the image space coordinates of the
primary that is kinematically equivalent to the first order water-bottom multiple as
mentioned n the previous section and
. The formal solution of
these equations, for the image space coordinates is:
| ![\begin{eqnarray}
\sin\hat{\gamma}&=&\frac{2h_D\cos 2\varphi}{Vt_m}\longrightarro...
...rac{V^2t_m^2\sin(2\varphi)}{2\sqrt{V^2t_m^2-4h_D^2\cos^2\varphi}}.\end{eqnarray}](img25.gif) |
(16) |
| (17) |
| (18) |
These equations allow the computation of the impulse response of the
water-bottom multiples in image space as a function of the aperture angle. More
importantly, they are the starting
point for understanding the kinematics of the data in 3D ADCIGs Tisserant and Biondi (2004),
still a subject of research.
Next: 2D Synthetic data example
Up: Alvarez: Kinematics of multiples
Previous: Diffracted multiples
Stanford Exploration Project
5/3/2005