Inspection of the stationary-phase results
[equation (7) and equation (9)]
shows that in a horizontally stratified medium the
cross-line ray parameters for the source and receiver
rays change across boundaries between layers with different velocities.
This result contradicts
Snell's law that states that the horizontal
ray parameters must be constant when the velocity
varies only vertically.
In common-azimuth downward continuation, by imposing the constraint that the
source and receiver ray must lie on the same plane,
we force the source and receiver rays to bend across interfaces
in a way that may not be consistent with Snell's law.
In particular, the ray bending determined by
common-azimuth continuation is incorrect when
the velocity variations would prescribe
the source ray to bend differently
than the receiver ray along the cross-line direction.
This error in the ray bending can be analyzed by
evaluating the difference between the values of
across an interface where the upper layer has
velocity *V _{1}* and the lower layer has velocity

(10) |

(11) | ||

(12) | ||

(13) |

The previous analysis shows that common-azimuth
downward continuation introduces an error in the ray bending
across velocity interfaces.
However, this consideration does not necessarily
leads to the conclusion that common-azimuth continuation
is inaccurate.
On the contrary, we argue that
the error in the ray bending
causes only second order errors in the continuation results.
This claim can be simply verified by recognizing that
for downward continuing common-azimuth data we evaluate
the phase function [equation (3)]
at its stationary point [equation (7)]
with respect to the cross-line offset wavenumber *k*_{hy}.
Since the phase function is stationary at the first order term of its Taylor expansion as a
function of *k*_{hy} around is equal to zero.
Therefore, an error in *k*_{hy} has only a second order effect
on the evaluation
of the phase function [equation (6)].
In other words,
the error introduced by the incorrect ray bending
has second order effects on the continuation results,
and consequently on the migration results.
This conclusion is supported by the accuracy
of the migrated images shown in the next section.

When the velocity field varies laterally, the previous analysis becomes more complex because the incorrect ray bending causes errors in the evaluation of the phase function not only through errors in the cross-line offset wavenumber ,but also through errors in the horizontal locations where the velocity function is evaluated. The arguments that support the conclusion that the errors in the phase function caused by error in are of second order are still valid for the general case of lateral velocity variations. However, the magnitude of the error introduced by the mispositioning of sources and receivers at depth when evaluating the velocity function cannot be neglected in principle. These errors are dependent on the spatial variability of the velocity function, and cannot be readily analyzed analytically. In the following section we show accurate migration results obtained over a velocity function varying both laterally and vertically. These results are encouraging and suggest that the range of application of common-azimuth migration to depth migration problems is fairly large.

Figure 2

MIGRATION RESULTS We tested common-azimuth migration by imaging two synthetic data sets generated by a modeling program based on the Kirchhoff integral. The Green functions are computed analytically assuming velocity functions with a constant spatial gradient. In both cases the velocity at the origin of the spatial coordinates is equal to .The first data set is generated assuming a vertical gradient of while the second data set is generated assuming a gradient with the horizontal component equal to and the vertical component equal to . The horizontal component of the gradient is oriented at an angle of 45 degrees with respect to the offset azimuth (in-line direction) of the acquisition geometry. The reflectivity model is a constant reflectivity function positioned along a half-spherical dome superimposed onto a horizontal planar reflector.

The acquisition geometry has 128 midpoint along both the in-line and cross-line directions; with midpoint spacing of in both directions. Each midpoint gather has 64 offsets, spaced every ; the nearest offset traces are actually recorded at zero offset. The offset-azimuth of the data is aligned with the in-line direction. Figure and show two in-line zero-offset sections extracted from respectively the vertical gradient data set and the oblique gradient data set. The effects of the lateral component of the velocity gradient are evident in both the tilting of the horizontal reflector, and in the asymmetry of the quasi-hyperbolic reflections from the dome.

Figures and show an in-line section and a depth slice of the results of migrating the vertical gradient data set. The in-line section (Figure ) is taken across the middle of the dome, while the depth slice (Figure ) is taken across the base of the dome .Common-azimuth migration has accurately imaged the data; both the in-line section and the depth slice show a perfect focusing of the reflectors. To visually verify the isotropic response of common-azimuth migration we overlaid a circle onto the depth slice. The migrated dome is perfectly circular, notwithstanding the ray bending caused by the strong vertical velocity gradient.

Figures and show the result of migrating the oblique gradient data set. The in-line section (Figure ) shows that common-azimuth migration has correctly positioned the reflectors. The planar reflector has been flattened, and the spherical dome has been properly focused. A spatial variability in both the frequency content and the amplitude of the migrated reflector is noticeable in the depth slice. The frequency variability is expected, and it is caused by the widening of the spatial wavelength of the wavefield caused by higher propagation velocities. The wavelet is narrower closer to the origin (upper-left corner) where velocity is lower and it is wider where the velocity is higher (lower-right corner). The amplitude variations cannot be readily explained, and further analysis is needed to determine whether they are artifacts of common-azimuth migration. The combined frequency and amplitude effects creates an ``anisotropic'' appearance to the migrated image. However, by overlaying a circle onto the plot of the seismic data we see that the migrated dome, though not perfectly circular, it is very close to circular. The comparison of these results with the results from the vertical gradient data set confirm the accuracy of common-azimuth migration even in the presence of strong lateral velocity gradients.

Figure 3

Figure 4

Figure 5

Figure 6

Figure 7

Figure 8

CONCLUSIONS We have shown that common-azimuth migration () can be successfully applied to imaging 3-D prestack data with laterally varying velocity. This important generalization of common-azimuth migration was made possible by two theoretical insights. The first one led us to recast common-azimuth migration as a recursive application of a new common-azimuth downward continuation operator. The second one is a ray-theoretical interpretation of common-azimuth downward continuation that enables us to analyze the errors in presence of ray bending caused by velocity inhomogeneities.

We implemented common-azimuth depth migration by downward continuation in mixed space-wavenumber domain using a split-step scheme. The application of our depth migration algorithm to a data set with a strong horizontal component of the velocity gradient resulted in an accurate imaging of the reflectors. ACKNOWLEDGEMENTS We thank Arnaud Berlioux for helping to generate the dome model using GOCAD. Biondo Biondi would like to thank Norm Bleistein for a short conversation that motivated him to better understand the errors involved in the stationary-phase derivation of common-azimuth migration.

[SEP,res]

A The purpose of this Appendix is to demonstrate the equivalence of the stationary phase derivation of the common-azimuth downward continuation operator [equation (7) in the main text] and the constraint on the propagation directions of the source rays and receiver rays expressed in equation (8).

We start by showing that equation (8)
is directly derived by imposing the condition that the
source ray and the receiver ray lie on the same plane.
For this condition to be fulfilled, the components of the two
rays in the direction of the cross-line axis *y* must be equal.
From elementary geometry, these components are

(14) |

(15) |

The second step is to eliminate *p*_{sz} and *p*_{rz} from
equation (A-2) by using the following
relationships among the ray parameters

(16) |

(17) |

To derive equation (7) from equation (A-4) it is sufficient to substitute for the ray parameters by applying the relationships

5/9/2001