NAME
psvspec - Construct Vs/Vp spectra for P-S converted wave
data.
SYNOPSIS
psvspec [ -NInputFileName ] [ -OOutputFileName ] [ -Vpikvpik
] [ -tminstart ] [ -tmaxstop ] [ -nsStartTrace ] [
-neEndTrace ] [ -rsStartRecord ] [ -reEndRecord ] [
-nvsvpnvsvp ] [ -vsvp0vsvp0 ] [ -vsvp1vsvp1 ] [ -igtigt ] [
-dmuldmul ] [ -tmultmul ] [ -thldthld ] [ -V ] [ -? or -h
]
DESCRIPTION
psvspec constructs a Vs/Vp spectrum for P-S converted-wave
data. psvspec reads in P-S converted-wave seismic data in
SIS format along with corresponding P-wave velocity picks
from a separate file. The velocity picks can be in any of
the common pick-file formats: XSD pick file, Disco HANDVEL
velocity file, TDFN velocity card images, or "flat" file.
Using the P-velocity information from the pick file, psvspec
performs a non-hyperbolic Vs/Vp ratio coherency scan on
either CSP or CCP gathers. The output is an SIS-format
velocity-ratio analysis panel, showing coherency as a func-
tion of Vs/Vp ratio and two-way travel time (down P-wave, up
S-wave). This data can be viewed directly or used with the
program "cvd" to perform interactive Vs/Vp-ratio analysis.
Detailed theoretical development is descripbed in the report
"Nonhyperbolic Vonverted Wave Velocity Analysis and Normal
Moveout", F95D42.
Command line arguments
-N InputFileName [default: stdin]
Enter the input data file name. The input data can be a
Common Source Point (CSP), or a Common Conversion Point
(CCP), or a Common Depth Point (CDP) gathered dataset.
-O OutputFileName [default: stdout]
Enter the output data file name. The output is a
velocity-ratio analysis panel showing coherency as a
function os Vs/Vp ratio and two way travel time (down
P-wave, up S-wave).
-Vpik vpik [No default]
The corresponding P-wave velocity pick file. All of the
pick-file formats commonly in use at Amoco (XSD, TDFN,
Disco HANDVEL, USP) are supported by psvspec. The pick
file format is automatically detected.
-tmin start (default = 0, beginning of trace).
Starting time of traces in milliseconds.
-tmax stop (default = end of trace).
End time in each trace for analysis in milliseconds
-ns StartTrace [default: 1]
The start trace number.
-ne EndTrace [default: last trace of record]
The end trace number.
-rs StarRecord [default: 1]
Start record number.
-re EndRecord [default: last record]
End record number.
-nvvsvp nvsvp (default =101)
Maximum number of velocity ratios to use spaced between
vsvp0 and vsvp1
-vsvp0 vsvp0 (default = 0.3)
Minimum velocity ratio value input.
-vsvp1 vsvp1 (default = 0.8)
Maximum velocity ratio value input.
-igt igt (default = 8)
An integer value to give the time-gate window T cen-
tered at t at time t(0). The half-time gate T/2 is
related to igt by T/2=igt*dt, where dt is the sample
interval in ms.
-dmul dmul (default=1.0)
Multiply each distance, itr(117), by this factor. This
is useful when the header has different units than
expected.
-tmul tmul (default=1.0)
Multiply the sampling interval, dt, by this factor.
This is useful if the sampling interval is in different
units than expected.
-thld thresh
Semblance threshold: semblances less than this value
will be zeroed. Default = 0.0 (no thresholding). W
ith the -fI-A option (max semblances scaled to 1.0)
this represents a relative thresholding.
-V Enter the command line argument '-V' to get additional
printout.
-? or -h
Enter the command line argument '-?' or -h or -help
to get online help. The program terminates after the
help screen is printed.
BUGS
There probably are some bugs waiting to be found.
SEE ALSO
cvd(1), psnmo(1), ccpbin(1) , ccpstk(1)
AUTHOR
Yaohui Zhang
COPYRIGHT
copyright 2001, Amoco Production Company
All Rights Reserved
an affiliate of BP America Inc.
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