A Born-WKBJ Inversion Method For Acoustic Reflection Data , by Robert W. Clayton and Robert H. Stolt

A method is presented for determining density and bulk-modulus variations in the earth from standard reflection surveys. Explicit formulas are given which utilize the amplitude-versus offset infrormation present in the observed wave fields. The method automatically accounts for dipping reflectors, but since it is based on a Born approximation of the scattering equation, it is restricted to subcritical reflections. For the inversion, the medium is considered to be composed of a known low-spatial frequency variation (the background) plus an unknown high-spatial frequency variation in bulk modulus and density (the reflectivity). The division between the background and the reflectivity depends on the frequency content of the source. For constant background parameters, the computations are done in the Fourier domain, where the first part of the algorithm includes a frequency shift identical to than in an F-K migration. The modulus and density variations are then determined by observing in a least-squares sense amplitude verses offset wavenumber. For a spatially variable background WKBJ Green's operators that model the direct wave medium with a smoothly varying background are used. A downward continuation with these operators removes the effects of the variable velocity from the problem, and consequencly the remainder of the inversion essentially proceeds as if the background were constant. If the background is strictly depth dependent, then the WKBJ's Green's operators are analytic, and consequently the inversion can be expressed in closed form.


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