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Velocity picking

For many kinds of data analysis, we need to know the velocity of the earth as a function of depth. To derive such information we begin from Figure 4.8 and draw a line through the maxima. In practice this is often a tedious manual process, and it needs to be done everywhere we go. There is no universally accepted way to automate this procedure, but we will consider one that is simple enough that it can be fully described here, and which works well enough for these demonstrations. (I plan to do a better job later.)

Theoretically we can define the velocity or slowness as a function of traveltime depth by the moment function. Take the absolute value of the data scans and smooth them a little on the time axis to make something like an unnormalized probability function, say $p(\tau ,s)>0$. Then the slowness $s(\tau )$ could be defined by the moment function, i.e.,

\begin{displaymath}
s(\tau ) \eq { \sum_s  s p(\tau ,s) \over \sum_s  p(\tau ,s) }
\end{displaymath} (12)

The problem with defining slowness $s(\tau )$ by the moment is that it is strongly influenced by noises away from the peaks, particularly water velocity noises. Thus, better results can be obtained if the sums in equation (4.12) are limited to a range about the likely solution. To begin with, we can take the likely solution to be defined by universal or regional experience. It is sensible to begin from a one-parameter equation for velocity increasing with depth where the form of the equation allows a ray tracing solution such as equation ([*]). Experience with Gulf of Mexico data shows that $\alpha\approx 1/2 {\rm sec}^{-1}$ is reasonable there for equation ([*]).

Experience with moments, equation (4.12), shows they are reasonable when the desired result is near the guessed center of the range. Otherwise, the moment is biased towards the initial guess. This bias can be reduced in stages. At each stage we shrink the width of the zone used to compute the moment.

A more customary way to view velocity space is to square the velocity scans and normalize them by the sum of the squares of the signals. This has the advantage that the remaining information represents velocity spectra and removes variation due to seismic amplitudes. Since in practice, reliability seems somehow proportional to amplitude the disadvantage of normalization is that reliability becomes more veiled.

fit
Figure 9.
Slowness scans. Overlaying is the line of slowness picks.
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[pdf] [png] [scons]


next up previous [pdf]

Next: Stabilizing RMS velocity Up: VELOCITY SPECTRA Previous: VELOCITY SPECTRA

2009-03-16