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We pose the imaging problem as an inversion problem by linearizing the wave-equation with respect to our model (
). 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:
 |
(1) |
where
represents the forward modeled data,
is the temporal frequency,
represents the reflectivity at image point
,
is the source waveform, and
is the Green's function of the two-way acoustic constant-density wave equation. Note that
is actually
dependent. It is important to point out that the adjoint of the forward modeling operator is the migration operator:
 |
|
|
(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 (
) 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
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Previous: Theory
2012-05-10