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CONNECTION OF THE LINEARIZED EIKONAL EQUATION AND TRAVELTIME TOMOGRAPHY

The eikonal equation (1) can be rewritten in the form  
 \begin{displaymath}
\bold{n} \cdot \nabla \tau = n \;,\end{displaymath} (12)
where $\bold{n}$ is the unit vector, pointing in the traveltime gradient direction. The integral solution of equation (12) takes the form  
 \begin{displaymath}
\tau = \int_{\Gamma (\bold{n})} n dl\;,\end{displaymath} (13)
which states that the traveltime $\tau$ can be computed by integrating the slowness n along the ray $\Gamma (\bold{n})$,tangent at every point to the gradient direction $\bold{n}$ .

Similarly, we can rewrite the linearized eikonal equation (5) in the form  
 \begin{displaymath}
\bold{n_0} \cdot \nabla \tau_1 = n_1 \;,\end{displaymath} (14)
where $\bold{n_0}$ is the unit vector, pointing in gradient direction for the initial traveltime $\tau_0$. The integral solution of equation (14) takes the form  
 \begin{displaymath}
\tau_1 = \int_{\Gamma (\bold{n_0})} n_1 dl\;,\end{displaymath} (15)
which states that the traveltime perturbation $\tau_1$ can be computed by integrating the slowness perturbation n1 along the ray $\Gamma (\bold{n_0})$, defined by the initial slowness model n0 . This is exactly the basic principle of traveltime tomography.

I have borrowed this proof from Lavrentiev et al. (1970), who used linearization of the eikonal equation as the theoretical basis for traveltime inversion.


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Stanford Exploration Project
11/11/1997