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Linearized Inversion

We pose the imaging problem as an inversion problem by linearizing the wave-equation with respect to our model ( $ m ({\mathbf x})$ ). Assuming that the earth behaves as a constant-density acoustic isotropic medium, we linearize the wave equation and apply the first-order Born approximation to get the following forward modeling equation:

$\displaystyle d^{mod}({\mathbf x_r},{\mathbf x_s},\omega) = \sum_{{\mathbf x}} ...
...({\mathbf x_s},{\mathbf x},\omega) m({\mathbf x}) G({\mathbf x},{\mathbf x_r}),$ (1)

where $ d^{mod}$ represents the forward modeled data, $ \omega$ is the temporal frequency, $ m ({\mathbf x})$ represents the reflectivity at image point $ {\mathbf x}$ , $ f_s(\omega)$ is the source waveform, and $ G({\mathbf x_s},{\mathbf x})$ is the Green's function of the two-way acoustic constant-density wave equation. Note that $ G$ is actually $ \omega$ dependent. It is important to point out that the adjoint of the forward modeling operator is the migration operator:


$\displaystyle {\mathbf m_{mig}} ({\mathbf x}) = \sum_{{\mathbf x_r},{\mathbf x_...
...},\omega) G^*({\mathbf x},{\mathbf x_r}) d({\mathbf x_r},{\mathbf x_s},\omega).$     (2)

The inversion problem is defined by minimizing the least-squares difference between the synthetic and the recorded data: One can use various types of propagators to formulate the Green's function. In our study, we use the two-way propagator. In this case, the migration operator is equivalent to reverse time migration (RTM). The inverted image ( $ m ({\mathbf x})$ ) is better than the migration image in the sense that its forward-modeled data fits the recorded data. Next, we discuss how to apply linearized inversion to jointly image with streamer and OBN data.


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Next: Joint imaging Up: Theory Previous: Theory

2012-05-10