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Elliptic Coordinates

The elliptic coordinate system (see figure 3) is defined by
$\displaystyle \left[ \begin{array}{c}
x_1\\
x_3
\end{array} \right] =
\left[ \...
...os} \,\xi_1\\
a\, {\rm sinh}\, \xi_3 \, {\rm sin} \,\xi_1
\end{array} \right].$     (20)

The transformation matrix is defined by
$\displaystyle \left[ \begin{array}{cc}
\frac{\partial x_1}{\partial \xi_1}& \fr...
...{\rm cos} \,\xi_1 & {\rm cosh} \,\xi_3 \, {\rm sin}
\,\xi_1
\end{array}\right],$     (21)

which leads to the following differential travel-time equations
$\displaystyle \left[ \begin{array}{c}
\frac{\partial t}{\partial h_{\xi_1}}\\
...
...gamma \,( a \, {\rm cosh} \, \xi_3 \, {\rm sin} \, \xi_1 )
\end{array} \right].$     (22)

The computation for the ADCIG in elliptic coordinates is given by

$\displaystyle {\rm tan}\,\gamma =- \frac{\partial \xi_3}{\partial h_{\xi_1}}.$ (23)

Thus, ADCIGs calculated in elliptic coordinates directly yield the reflection opening angle without any additional filtering.

EC
Figure 3.
Example of an elliptic coordinate system. [NR]
EC
[pdf] [png]


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Next: Numerical Examples Up: Canonical Examples Previous: Sheared Cartesian Coordinates

2009-04-13