2-D wavepath migration

Citation
H. Sun et Gt. Schuster, 2-D wavepath migration, GEOPHYSICS, 66(5), 2001, pp. 1528-1537
Citations number
11
Categorie Soggetti
Earth Sciences
Journal title
GEOPHYSICS
ISSN journal
00168033 → ACNP
Volume
66
Issue
5
Year of publication
2001
Pages
1528 - 1537
Database
ISI
SICI code
0016-8033(200109/10)66:5<1528:2WM>2.0.ZU;2-U
Abstract
Prestack Kirchhoff migration (KM) is computationally intensive for iterativ e velocity analysis. This is partly because each time sample in a trace mus t be smeared along a quasi-ellipsoid in the model. As a less costly alterna tive, we use the stationary phase approximation to the KM integral so that the time sample is smeared along a small Fresnel zone portion of the quasi- ellipsoid. This is equivalent to smearing the time samples in a trace over a 1.5-D fat ray (i.e., wavepath), so we call this "wavepath migration" (WM) . This compares to standard KM, which smears the energy in a trace along a 3-D volume of quasi-concentric ellipsoids. In principle, single trace migra tion with WM has a computational count of O(N-1.5) compared to KM, which ha s a computational count of O(N-3), where N is the number of grid points alo ng one side of a cubic velocity model. Our results with poststack data show that WM, produces an image that in some places contains fewer migration ar tifacts and is about as well resolved as the KM image. For a 2-D poststack migration example, the computation time of WM is less than one-third that o f KM. Our results with prestack data show that WM images contain fewer migr ation artifacts and can define the complex structure more accurately. It is also shown that WM can be significantly faster than KM if a slant stack te chnique is used in the migration. The drawback with WM is that it is someti mes less robust than KM because of its sensitivity to errors in estimating the incidence angles of the reflections.