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In this Appendix I present the analytical expressions
for the derivatives of the VTI group slowness function
expressed in equation 6 in the main text.
These derivatives are necessary for the numerical computation
of the RMO functions.
The VTI slowness function can be approximated as
Fowler (2003):
| ![\begin{eqnarray}
S^2_{\rm VTI}\left(\theta\right)
&=&
\frac
{
{S_V}^2\cos^2 \the...
...ht)
+
{S_V}^2\left({S_N}^2-{S_H}^2\right)
\sin^2 2 \theta
}
}
{2},\end{eqnarray}](img100.gif) |
|
| (57) |
where
| ![\begin{displaymath}
S^2_{\rm Ell}\left(\theta\right)
=
{S_V}^2\cos^2 \theta+ {S_H}^2\sin^2 \theta\end{displaymath}](img101.gif) |
(58) |
is the elliptical component.
The derivatives are then written as:
| ![\begin{eqnarray}
\left.
\frac{\partial S_{\rm VTI}\left(\theta\right)}{\partial ...
...\right)
+
{S_V}^2\left({S_N}^2-{S_H}^2\right)
\sin^2 2 \theta
}
},\end{eqnarray}](img102.gif) |
(59) |
| (60) |
| (61) |
where the derivatives of the elliptical component with
respect to
and
are:
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Stanford Exploration Project
5/3/2005