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Velocity, path-length and travel time changes

Depletion-related strain and velocity changes will perturb the travel path and length of a normally-incident ray. The distance $ dz$ travelled by the ray in time $ dt$ at velocity $ v$ is given by

$\displaystyle dz = v dt.$ (1)

For small perturbations $ \delta z\ll dz$ , $ \delta v\ll dv$ and $ \delta t\ll dt$ , we can write

$\displaystyle \frac {d(\delta z)}{dz} = \frac{\delta v}{v} + \frac {d(\delta t)}{dt},$ (2)

where, $ d(\delta z)/dz=\epsilon_{zz}$ is the vertical ``depth'' strain and $ d(\delta t)/dt=\epsilon_{tt}$ is the apparent ``time'' strain. The $ R$ -factor (Hatchell and Bourne, 2005a) relates the fractional change in velocity $ {\delta v}/{v}$ to the depth strain $ \epsilon_{zz}$ and time strain $ \epsilon_{tt}$ :

$\displaystyle \frac{\delta v}{v} = -R \epsilon_{zz} = -\frac{R}{1+R} \epsilon_{tt}.$ (3)

The $ R$ -factor can be measured from core samples in the laboratory (Hatchell and Bourne, 2005a; Bathija et al., 2009), derived from the estimated time-shifts (Hawkins et al., 2007), or derived from other production-related data (Hodgson et al., 2007). For most reservoir rocks, $ R$ values of $ 4$ to $ 6$ have been shown to be reasonable (Hodgson et al., 2007; Hatchell and Bourne, 2005b). In this paper, a constant $ R$ value of $ 5$ is assumed.
Figure: Apparent displacements by cyclic 1D search
\begin{figure}\begin{algorithm}[H]% enter the algorithm environment
% give the ...
... interpolation of $b$\ with displacements $a$\ \\
\end{algorithm}
\end{figure}

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2010-05-19