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Seismic wave extrapolation using lowrank symbol ... - Madagascar

Seismic wave extrapolation using lowrank symbol ... - Madagascar

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Fomel, Ying, & Song 2 Lowrank <strong>wave</strong> <strong>extrapolation</strong><br />

propagation, because it involves eigenfunctions rather than rows and columns of the<br />

original <strong>extrapolation</strong> matrix. Our algorithm can also be regarded as an extension<br />

of the <strong>wave</strong>field interpolation algorithm of Etgen and Brandsberg-Dahl (2009), with<br />

optimally selected reference velocities and weights. Another related method is the<br />

Fourier finite-difference (FFD) method proposed recently by Song and Fomel (2011).<br />

FFD may have an advantage in efficiency, because it uses only one pair of multidimensional<br />

forward and inverse FFTs (fast Fourier transforms) per time step. However, it<br />

does not offer flexible controls on the approximation accuracy.<br />

Our approach to <strong>wave</strong> <strong>extrapolation</strong> is general and can apply to different types of<br />

<strong>wave</strong>s, including both acoustic and elastic seismic <strong>wave</strong>s, as well as velocity continuation<br />

(Fomel 2003b), offset continuation (Fomel 2003a), prestack exploding reflector<br />

<strong>extrapolation</strong> (Alkhalifah and Fomel 2010), etc.<br />

The paper is organized as follows. We first present the theory behind the proposed<br />

algorithm, then describe the algorithm and test its accuracy on a number of synthetic<br />

benchmark examples of increasing complexity.<br />

WAVE EXTRAPOLATION<br />

Let P (x, t) be the seismic <strong>wave</strong>field at location x and time t. The <strong>wave</strong>field at the<br />

next time step t + ∆t can be approximated by the following mixed-domain operator<br />

(Wards et al. 2008)<br />

∫<br />

P (x, t + ∆t) = ̂P (k, t) e i φ(x,k,∆t) dk , (1)<br />

where ̂P (k, t) is the spatial Fourier transform of P (x, t)<br />

̂P (k, t) = 1 ∫<br />

P (x, t)e −i k·x dx , (2)<br />

(2 π) 3<br />

where k is the spatial <strong>wave</strong>number. To define the phase function φ(x, k, t), which<br />

appears in equation (1), one can substitute approximation (1) into the <strong>wave</strong> equation<br />

and extract the geometrical (high-frequency) asymptotic of it. In case of seismic <strong>wave</strong><br />

propagation, this leads to the eikonal-like equation<br />

∂φ<br />

∂t<br />

= ±V (x, k) |∇φ| , (3)<br />

where V (x, k) is the phase velocity, and the choice of the sign corresponds, in the<br />

case of a point source, to expanding or contracting <strong>wave</strong>s. In the isotropic case, V<br />

does not depend on k. The initial condition for equation (3) is<br />

φ(x, k, 0) = k · x , (4)<br />

which turns equation (1) into the simple inverse Fourier transform operation.

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