The fact that a correlation in the Fourier components of the wavefield is introduced by a perturbation to a translation invariant model can be seen from the Born approximation of the perturbed wavefield, . Rewriting Equation (30) in terms of Fourier coordinates gives
where summation is assumed over the repeated indices and , is the scattering location, and the Green’s functions and are defined in Section 3.3. The perturbations to the source function were ignored for the sake of simplicity. To obtain Equation (83) we used the fact that the operator , which describes the perturbation to the model at , is a linear operator. The equation shows that the perturbation to the model in general causes a response at wavevector and frequency to a source at and . This response is thus correlated with the unperturbed wave created by the same source. Notice that for a perturbation that depends both on space and time, the operator explicitly depends on and . Using Equation (83) the correlations of the wavefield in the Fourier domain can be approximated, to first order in the strength of the perturbation, as where the source covariances express the assumptions of stationarity and horizontal spatial homogeneity (the functions are equal to the functions within a multiplicative factor, see Section 3.2). In Equation (84) summation over the repeated indices, , , and , is assumed. This expression is accurate to first order in the strength of the perturbation to the background model, which appears in the operator .
Let us now connect the result of the previous section with the results of Woodard and Fan (2005). In real space, Woodard and Fan (2005) use
to model the effect of a flow . This approximation neglects any possible effect of the flow on the wave sources and wave damping. Woodard and Fan (2005) expand the velocity field in Fourier components, in the horizontal directions and time, and known functions of depth. For the sake of a relatively simple example, let us look at the special case of a vertical flow of the form where the vector is a horizontal wavevector and is a temporal frequency. Under these assumptions, we have Let us further assume that the sources are all located at a particular depth and that only the component of is nonzero, again only for the sake of simplicity. This is done here only to avoid carrying the integrals over and . Then Equation (84) becomes Equation (89) is already quite informative. First of all, note that a velocity field with horizontal wavenumber only correlates components of the wavefield whose horizontal wavenumbers differ by . This is sensible. Likewise, velocity fields with harmonic time dependence with frequency only couple components of the wavefield whose frequencies differ by . The above result can be reduced to the equations of Woodard and Fan (2005) by inserting the normal summation approximations for the Greens function’s (see Birch et al., 2004, and Section 3.3.2) into the above result.Woodard and Fan (2005) make the further approximation that oscillations of different radial orders are excited incoherently. This is certainly not the case in reality, as evidenced by the asymmetry in the power spectrum. It is not clear what effect this approximation will have on the final result, as most of the power is near the resonances, where lineasymmetry is not important.
Notice that we also need to compute the term as the final result that we wish to obtain is the first order change in introduced by a small change in the model. This second term can be computed in exactly the same manner as the term, which we have already done.
So far we have only addressed the forward problem. The other half of the directmodeling approach is the inverse problem, that is inferring the flows in the Sun from the Fourier domain correlations seen in the data. The inverse problem in direct modeling has been solved as a linear leastsquares problem (Woodard, 2002; Woodard and Fan, 2005). A crucial observation is that a flow with horizontal wavenumber only couples modes with wavenumbers and when . This is a result of the assumption that the background model is planeparallel and translation invariant. As a result the different wavenumber components of the flow can be inferred one at a time, in the spirit of the MCD inversion scheme (Jacobsen et al., 1999). The same argument applies in the time domain, and flows can be inferred one frequency component at a time.
Woodard (2002) tested his directmodeling approach on a quiet sun region using MDI data. The method was used to invert for nearsurface supergranularscale flow. Although many approximations were made in carrying out the inversion, general agreement (a correlation coefficient of 0.68) was found between the Doppler component of the seismically inferred flow in the photosphere and the directly observed surface Doppler signal (see Figure 29). Thus direct modelling appears to be a very promising technique.

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