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From theory to practice

I found that squaring the semblance values ${\rm semb}(\gamma)$ produced a better result than the semblance values themselves. My resulting cdf $a_{\rm cdf}(\gamma_i)$ function was then  
 \begin{displaymath}
a_{\rm cdf}(\gamma_i)= \frac{ 
\sum_{\gamma_0}^{\gamma^i} {\...
 ...^2(\gamma)}
{\sum_{\gamma_0}^{\gamma^n} {\rm semb}^2(\gamma)}
.\end{displaymath} (11)
In addition, I need to account for the fact that I am not scanning over all possible $\gamma$ values. I introduced a constant parameter gmax that scaled my $\bf c$ values so that that one standard deviation of $\bf c$might correspond to 2-5 standard deviations $\bf a$.

Finally, we are going to a precondition the model Fomel et al. (1997) with the inverse of $\bf A$ and solve the problems in terms of the variable $\bf p= \bf A\bf m$,
   \begin{eqnarray}
\bf n &\approx&\bf A^{-1}\bf p\nonumber \\ \bf 0&\approx&\epsilon \bf p
.\end{eqnarray}
(12)


next up previous print clean
Next: Limitations Up: THEORY Previous: THEORY
Stanford Exploration Project
5/23/2004