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Travel-time relations

In a homogeneous medium, the seismic energy generated by a shot propagates along the straight rays that connect the shot position xs, reflector position (x,z), and receiver position xr. The total travel-time of this propagation can be formulated as  
 \begin{displaymath}
t={1 \over 2} \left[ \sqrt{t^2_0+{4(x-x_s)^2 \over v^2}}+
\sqrt{t^2_0+{4(x-x_r)^2 \over v^2}} \right],\end{displaymath} (1)
where v is the velocity of the medium, and

\begin{displaymath}
t_0={2z \over v}\end{displaymath}

is the vertical two-way travel time. We can solve equation (1) for t0,  
 \begin{displaymath}
t_0={1 \over t} \sqrt{t^2-{(x_r-x_s)^2 \over v^2}}
\sqrt{t^2-{(2x-x_r-x_s)^2 \over v^2}}.\end{displaymath} (2)

Equations (1) and (2) define the relations between two travel times and are the key equations of kinematic operators for imaging.


next up previous print clean
Next: Kinematic operators Up: PRINCIPLES OF THE ALGORITHM Previous: PRINCIPLES OF THE ALGORITHM
Stanford Exploration Project
1/13/1998