The focus of this thesis is to determine the most accurate processes and operators to properly image PS data.
Converted-wave seismic data have intrinsic characteristics
that make their processing different than that of conventional
PP seismic data. For a simple horizontal layer embedded in a
constant-velocity medium the concept of Common Midpoint Gathers (CMP),
does not hold for PS data; therefore, each trace represents a different point
in the subsurface. For PS data, the most common representation
is known as Common Reflection/Conversion-point Gathers (CRP/CCP).
Figure
shows an schematic
representation for both the CMP and the CCP/CRP definition. The top panel represents the raypath
geometry for a converted-mode ray in a CMP distribution; because of
the difference between the P-velocity and the
S-velocity, each source-receiver ray illuminates a different point in the
subsurface. The bottom panels presents the raypath for the converted-mode
ray distribution in CRP/CCP geometry. The appropriate knowledge of the
P-wave velocity, the S-wave velocity, and the physics of wave propagation,
makes it possible to arrange each source-receiver ray
to illuminate the same point in the subsurface, this point is also
known as the image point.
CCP stacking is a processing technique for converted-wave data that approximates the correction from the CMP to the CCP domain; however, the final result is in the time domain and the knowledge of the P and S velocity models is required.
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Another characteristic of converted-wave data is that the polarity flips along
the reflection hyperbola.
This polarity change is an intrinsic property of the shear-wave displacement Danbom and Domenico (1988).
In a constant-velocity medium, the vector displacement field produces
opposite movements in the receivers at either side of the intersection
of the normal ray with the surface (Figure
).
This leads to the polarity flip along the same reflection.
Figure
presents a characteristic Common Shot
Gather (CSG) for the PS section of the 2-D OBS Mahogany data set
in the Gulf of Mexico. This is an example of the
polarity flip characteristic of converted-wave data.
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pflip
Figure 3 Polarity inversion in converted waves seismic data. +g and -g correspond to positive and negative polarity in a common shot gather. The vector displacement field produces opposite movements at either size of the intersection of the normal ray with the surface. | ![]() |
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shot-intro
Figure 4 PS Common Shot Gather (CSG) from the 2-D Mahogany data set in the Gulf of Mexico. Note the polarity flip along the same hyperbolas. | ![]() |
In a complex velocity medium, the normal ray
determines the location of the polarity flip.
For flat reflectors in v(z) media, and in areas with constant
P-to-S velocity ratio (
), the normal incidence ray emerges at
the surface at zero-offset.
However, in general, the P and S raypaths corresponding to
the normal-incidence (zero-amplitude) ray will not necessarily emerge
at the surface at the zero-offset point.
Figure
illustrates this for the case of a dipping
layer and a non-constant
.
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pflip2
Figure 5 Polarity flip problem for a dipping layer and a non-constant | ![]() |
For 3-D OBS data, the irregularity in the acquisition geometry
is an additional problem for the imaging of converted-wave data.
Irregular geometries are a serious impediment for
accurate subsurface imaging Beasley (1994); Chemingui (1996); Gardner and Canning (1994). Irregularly sampled
data affect the image with amplitude artifacts and phase
distortions if the missing data are assumed to be zero traces. Irregular geometry problems are more
acute in cases in which the amplitude information is one of the
main goals of study. Typical
OBS seismic data acquisition presents processing problems similar to those of
land data.
Gardner and Canning (1994) demonstrate some of the
effects of irregular sampling on 3-D prestack migration, through
synthetic examples using real 3-D land-acquisition geometry.
Figure
illustrates this problem. This figure
presents the source and receiver distribution for 3-D OBS data
set in the Alba oil field in the North Sea. The gap in the source
distribution, panel (a), is due to an oil production platform. These gaps in the data result
in artifacts in the final 3-D image.
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