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Flattening by predictive painting

As shown in Table 1, Fowler's is the only set of equations that do not require an explicit use of the curvature $ Q$ . The dependence on the curvature is absorbed by the $ \tau _0$ function. The other two sets of equations, Dix and stripping formulas, as well as the equations for effective parameters, do need curvature. The curvature computation can be problematic when the data are contaminated by noise. This makes these three methods (effective, stripping, and Dix) less practical when applied to real data with poor SNR. However, Fowler's rules represent a way to circumvent the problem. In fact, if we can find an algorithm that estimates the $ \tau _0$ mapping function directly from the data, all the curvature issues will get solved.

The desired algorithm exists and is known as seismic image flattening. The idea of using local slopes for automatic flattening was introduced by Bienati and Spagnolini (2001) and Lomask et al. (2006). Flattening by predictive painting (appendix A) uses the local-slope field to construct a recursive prediction operator (equation A-4) that spreads a traveltime reference trace in the image and predicts the reflecting surfaces which are then unwrapped until the image is flattened.

We propose bypassing the issue of estimating the zero-slope time $ \tau _{0}$ field by using the predictive painting approach. Let us discuss how it works on the previously shown synthetic data in Figure 7a. Figure 7b shows local event slope $ R$ measured from the data using the PWD algorithm. Figure 7c shows how predictive painting spreads a zero-slope time $ \tau _{0}$ reference trace along local data slopes to predict the zero-slope time $ \tau _{0}$ mapping field and hence the geometry of the traveltime reflection curves along $ \tau $ -$ p$  CMP gather. Because this procedure does not involve curvature computations, it represents a much more robust way of obtaining the $ \tau _{0}$ field that is needed by the inversion formulas in equations 27 and 28. After $ \tau _{0}$ has been found, we also have what we need to perform gather flattening (Burnett and Fomel, 2009a,b). Unshifting each trace (Figure 7d) automatically flattens the data, thus performing a velocity-independent $ \tau $ -$ p$  NMO correction. As expected, all events are perfectly aligned, and the correction does not suffer from instabilities of curvature estimation. Moreover, predictive painting is automatic and does not require any prior assumptions about the moveout shape.

dataPsynthwidth=Synthetic CMP $ \tau $ -$ p$ transformed gather (a), estimated local slopes (b), zero slope time $ \tau _0$ obtained by predictive painting (c), and the gather flattened (d).

Now, given the slope field $ R$ and its zero-slope time field $ \tau _{0}$ , we retrieve interval parameters using equations 27 and 28. In Figure 8, the estimated NMO (a) horizontal velocities (b) and the anellipticity (c) parameter are mapped to the appropriate zero-slope time using the painted zero-slope time $ \tau _{0}$ field (Figure 7c). The exact interval profiles (yellow lines) are recovered nearly perfectly although the resolution slightly worsens with respect to the effective profiles (Figure 6). The main reason is the instability of the additional numerical differentiation along the $ \tau $ direction that all the approaches require.

intPmasksynth
intPmasksynth
Figure 7.
Fowler's equation based inversion to interval normal moveout (a) horizontal velocity (b) and anellipticity parameter $ \eta $ (c). The yellow lines represent the exact values used for generating the synthetic dataset in figure 3 (a).
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next up previous [pdf]

Next: Field data example Up: Casasanta & Fomel: Velocity-independent Previous: Fowler's equations

2011-06-25