Born-approximate modeling formula

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Revision as of 21:39, 30 December 2020 by JohnWStockwellJr (talk | contribs) (Perturbation theory)
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It is often useful to construct integral equations as modeling formulas. One method of creating such an integral equation representation is the application of Green's theorem to a wave equation. A general integral equation formalism may be obtained using the notion of Scattering theory. That is, we assume that the medium may be decomposed into a known background wavespeed profile plus a perturbation called the scatterer. The wavefield, similarly may be decomposed into an background wavefield, also called the reference or the incident field, plus a perturbation field also called the scatterer.

The scatterer may be thought of as a volume scatter, or a surface scatterer. In this formalism we will consider the perturbation in the wavespeed profile to be a volume scatterer. We will also consider wave propagation to be governed by the scalar wave equation.

The scalar wave equation and the scalar Helmholtz equation

The scalar wave equation is given by


Here, is general position in the medium, is the source position, is general time , is the time history of the source, , is the wavespeed of the medium, and is the wavefield due to a source located at initiated at time .

Applying the forward Fourier transform in time to the scalar wave equation yields the scalar Helmholtz equation


We will consider the Helmholtz equation to be the governing equation of our problem. Because we are interested in recording at a specific position, there is a second Helmholtz equation that is of interest


Here is the Green's function of the medium. The superscript indicates that these are formally the adjoint operator and respective Green's function. In this case we have a self-adjoint problem.

Perturbation theory

We assume that the medium consists of a volume enclosed in a surface . For an unbounded medium we will allow this boundary surface to be at infinity. We further consider that the medium suggests of a background or incident model, represented by the velocity function , plus a scatterer, represented by a perturbation which is a deviation from the background velocity model.

One way of representing this that preserves the form of the Helmholtz equation is

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Correspondingly, we consider that the wavefield is similarly decomposable into an incident wavefield , which is the field in the absence of the scatterer, plus the scattered field , such that


In the absence of the scatterer, the incident or background wavefield is represented by