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The impulse response of the AMO operator in homegeneous media
is a skewed saddle.
The shape of the saddle depends on the offset
vector of the input data
and on the offset vector of the desired output data
, where the unit vectors
and
point respectively in the in-line direction and the cross-line
direction.
The time shift to be applied to the data is a function of
the difference vector
between the midpoint of the input trace and the
midpoint of the output trace.
The analytical expression of the AMO saddle,
is
|  |
(41) |
The traveltimes t1 and t2 are respectively the traveltime of
the input data after NMO has been applied,
and the traveltime of the results before inverse NMO has been applied.
Figure
shows three AMO operators that correspond
to three different azimuth correction
angles in a homogeneous medium. From left to right, the azimuth corrections are 15, 30, and 45 degrees, respectively.
The input and output offset were the same and equal to 2 km.
Though the general shape of the AMO operator is practically
the same between the three operators, the size is very much
dependent on the amount of azimuth
correction; the larger the azimuth correction the
larger the AMO operator.
Clearly, for zero
azimuth correction the operator reduces to a point. The size dependence of the
operator on azimuth holds
regardless of the medium. The shape of the operator, however, is very much
independent of azimuth correction.
Amo-homo3
Figure 2 AMO operators for isotropic
homogeneous media for an input and output
offset of 2 km and correction to only the azimuth. The azimuth corrections from left
plot to right are 15, 30, and 45 degrees, respectively. The velocity of the homogeneous isotropic medium is
2 km/s, and the input NMO corrected time is 2 s. The x0 (inline) and y0 (crossline)
axis are in km and the t0 is in seconds.
This holds here and throughout. The circular lines are contours of equal ray parameter.
In Figure
and throughout, the contour curves plotted represent
lines of equal ray parameter.
It provides information on the distribution of dip angles,
as well as on the distribution of energy along the operator;
denser contour lines imply higher amplitude.
Next: Generating the Azimuth moveout
Up: Rickett, et al.: STANFORD
Previous: Introduction
Stanford Exploration Project
7/5/1998