1887

Abstract

Paraxial wave equations are a powerful way to approach seismic migration. They have been successfully used in both 2D (cf. Collino [2]) and in 3D (cf. Graves and Clayton [3]). Here we present a numerical method for the solution of these equations, which avoids the lateral splitting used in most in the 3D in methods used until now.

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/content/papers/10.3997/2214-4609.201410601
1992-06-01
2020-10-23
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http://instance.metastore.ingenta.com/content/papers/10.3997/2214-4609.201410601
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