NAME
sqavou - module to do Semi-Quantitative AVO
SYNOPSIS
sqavou [ -Nntap ] [ -Ootap ] [ -vardin ] [ -as ] [ -ai ] [
-rs ] [ -re ] [ -ws ] [ -we ] [ -to ] [ -dof ] [ -md ] [ -em
] [ -s ] [ -vpvs ] [ -dead ] [ -disco ] [ -cdp ] [ -? ]
DESCRIPTION
sqavou takes selected portions of trace data and does a hil-
bert transform or optionally computes the envelope for a
number of frequency bands.
Hilb gets both its data and its parameters from command line
arguments. These arguments specify the input, output, the
start and end times, the start and end traces, and the start
and end records. Internally, the program does angle-
dependent stacking on the input data file, in the same way
as program ANGST. Thus many of the specified parameters are
the same as those used for ANGST.
Command line arguments
-N ntap
Enter the input data set name or file immediately after
typing -N. This input file should include the complete
path name if the file resides in a different directory.
Example -N/b/vsp/dummy tells the program to look for
file 'dummy' in directory '/b/vsp'
-O otap
Enter the output data set name or file immediately
after typing -O. This output file is not required when
piping the output to another process. The output data
set also requires the full path name (see above).
-v cardin
Enter the TDFN card file name immediately after typing
-v. This file should contain the TDFN velocity card
images.
-as angbeg
Enter the start angle for the ANGST angle stack rou-
tine. The default is 0.
-ai anginc
Enter the angle increment for the ANGST angle stack
routine. The default is 15 degrees.
-rs irs
Enter the start record number. The default is the
first record. If spacial windowing is used, both rs and
re parameters should be supplied.
-re ire
Enter the ending record number. The default is the
last record. If spacial windowing is used, both rs and
re parameters should be supplied.
-ws ws
Enter the window start time used for spacial windowing.
The default is the beginning of the trace. If spacial
windowing is used, both rs and re parameters should be
supplied.
-we we
Enter the window end time used for spacial windowing.
The default is the end of the trace. If spacial window-
ing is used, both rs and re parameters should be sup-
plied.
-to to
Enter the desired output type (either 1 or 2). Type 1
(default) is for Delta Rock properties, type 2 is for
Bortfeld Coeffcients.
-dof dof
Enter the desired degree of fit (either 2 or 3). Dof of
2 will use the equations for a two parameter solution
while a dof of 3 (default) will use the three parameter
equations.
-md mode
Enter the desired solution mode (either 0, 1, or 2). A
mode of 0 will use straight ray approximations, a mode
of 1 will use curved ray approximations, and a mode of
2 will use perturbed curved ray approximations. No
default.
-em angl
Enter the desired angles flag (either 0 or 1). An
angles flag of 0 (default) uses incident angles, while
an angles flag of 1 uses emergent angles.
-s vscale
If present, velocity are multiplied by this constant.
Default is 1.0.
-vpvs vpvs
If present, this value for Vp/Vs ratio will be used in
the three parameter calculations. Default is 2.0.
-dead
If present, zero-valued stack traces are not flagged
"dead". Default is NO.
-disco
If present, velocity card images are in DISCO HANDVEL
format. Default is NO.
-cdp If present, velocity and angle functions are keyed to
CDP, not RI number. Default is NO.
-? Enter the command line argument '-?' to get on-line
help screen. The program stops after printing the
screen.
COPYRIGHT
copyright 2001, Amoco Production Company
All Rights Reserved
an affiliate of BP America Inc.
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