code stringlengths 1 1.96M | language stringclasses 1
value |
|---|---|
#! /bin/sh
# Examples of producing multiple shot records with susynlv
# Note that we label by shot record and since there are 50 offsets,
# use d2=0.02 (1/50). We add some noise to make data a bit more
# realistic, in particular, velocity analyses (with suvelan) seem very
# "blocky" without a little noise.
# Flat mo... | Shell |
#! /bin/sh
# Clean.sh - recursively call Clean.sh in the demo directories
# Test back-up dir first (at CWP must run on NeXT-net)
# Take care of subdirectories
for i in `ls`
do
if
[ -d $i ]
then
cd $i
if
[ -f Clean.sh ]
then
Clean.sh
fi
rm -f *~ \#*\# .nfs* *.eps
cd ..
fi
done
# Take care of t... | Shell |
#! /bin/sh
cd Tetramod ; Clean.sh
exit 0
| Shell |
#! /bin/sh
S=.
viewer3 verbose=1 \
< $S/hzfile3.grid \
rayfile=$S/rayfile3.grid \
sttfile=$S/sttfile3.grid \
wffile=$S/wffile3.grid
exit 0
| Shell |
#! /bin/sh
rm hzfile* tetrafile*
| Shell |
#! /bin/sh
Hz=.
nxhz=3
nyhz=3
nhz=1
tetrafile=$Hz/tetrafile3.tetra
hzfile=$Hz/hzfile3.grid
tetramod verbose=1 nhz=$nhz \
nxhz=$nxhz nyhz=$nyhz \
z00=0 \
z01=0 \
z10=0 \
z11=0 \
v00=2 \
v01=2 \
v10=2 \
v11=2 \
dvdz00=1.0 \
dvdz01=1.0 \
dvdz10=1.0 \
dvdz11=1.0 \
hzfile=$hzfile > $tetrafile
exit 0
| Shell |
#! /bin/sh
# multiple suppressed prestack data
data=radon.data.pbal.gain.jon=1.cdp.su
# data after nmo
nmodata=nmo.$data
parfile=nmovel.par
sunmo < $data par=$parfile > $nmodata
exit 0
| Shell |
#! /bin/sh
suttoz nz=1500 dz=3 par=suttoz.par \
< stolt.seis.su > stolt.depth.seis.su
exit 0
| Shell |
#! /bin/sh
# break up the data in to subsets
data=gain.jon=1.cdp.su
suwind key=cdp min=1 max=500 < $data > junk.cdp=1-500.su
suwind key=cdp min=501 max=1000 < $data > junk.cdp=501-1000.su
suwind key=cdp min=1001 max=1500 < $data > junk.cdp=1001-1500.su
suwind key=cdp min=1501 < $data > junk.cdp=1501-2142.su
exit ... | Shell |
#! /bin/sh
vnmo=
tnmo=
data=
pmula=0
pmulb=0
## view nmo corrected data in the Radon domain
sunmo vnmo=$vnmo tnmo=$tnmo < $data |
suradon offref=-3237 interoff=-262 pmin=-2000 \
pmax=2000 dp=16 choose=0 igopt=2 \
depthref=1000 | suximage perc=99 &
## nmo->radon-> inverse NMO: for multiple suppression
sunmo vnmo=$... | Shell |
#! /bin/sh
# Velocity analyses for the cmp gathers
# Authors: Dave Hale, Jack K. Cohen, with modifications by John Stockwell
# NOTE: Comment lines preceeding user input start with ##
#set -x
## Set parameters
datadir=.
velpanel=gain.spike.mute.pbal.cdp.su # gained data sorted in cdps
vpicks=radonnmovel.par #... | Shell |
#! /bin/sh
#set -x
# set parameters here
method=mono # interpolation method
r1=10
r2=10
unifpar=unif2.par
unif2 < unif2.ascii par=$unifpar method=$method |
smooth2 par=$unifpar r1=$r1 r2=$r2 > junk.bin
cp junk.bin unewvelzx.bin
transp par=$unifpar < unewvelzx.bin > unewvelxz.bin
echo "Writin... | Shell |
#! /bin/sh
vnmo=1500
interoff=-262
offref=-3237
depthref=1000
pmin=-2000
pmax=2000
dp=8
igopt=2
pmula=-800
pmulb=47
data=gain.jon=1.cdp.su
# view gather in the radon transform domain
choose=0 # =1 use suradon as a radon domain filter
#sunmo vnmo=$vnmo < $data |
#suradon offref=$offref depthr... | Shell |
#! /bin/sh
# put the data back together
file1=
file2=
file3=
file4=
newfile=
cat $file1 $file2 $file3 $file4 > temp.su
sushw key=tracl a=1 b=1 < temp.su > $newfile
exit 0
| Shell |
#! /bin/sh
data=data.pbal.gain.jon=1.cdp.su
radondata=radon.$data
# the tnmo= and vnmo= values go in a text file called "radonnmovel.par"
parfile=radonnmovel.par
interoff=-262
offref=-3237
depthref=1000
pmin=-2000
pmax=2000
dp=8
igopt=2
# you might consider making these values 10, or something
# we rely on... | Shell |
#! /bin/sh
data=radon.pmula=-1250.pmula=20.gain.jon=1.cdp.su
outdata=stack.radon.su
sunmo < $data par=stkvel.p1 |
sustack > $outdata
exit 0
| Shell |
#! /bin/sh
# convert a single RMS velocity to Interval velocity.
# put your values of tnmo= and vnmo= here.
tnmo=
vnmo=
#output file
outfile=suttoz.par
suintvel t0=$tnmo vs=$vnmo outpar=$outfile
echo t=$tnmo >> $outfile
echo "use v= and t= values for suttoz "
echo " result output in $outfile"
exit 0
| Shell |
#! /bin/sh
WIDTH=300
WIDTHOFF=50
WIDTHOFF2=50
HEIGHT=600
HEIGHTOFF=50
HEIGHTOFF2=250
HEIGHTOFF3=500
HEIGHT2=200
WIDTH2=600
WIDTHOFF3=100
WIDTH3=800
HEIGHT3=300
vrmst=vrmst.bin
vintt=vintt.bin
vinttav=vinttav.bin
vintzav=vintzav.bin
rmspar=vrmst.par
intpar=vintt.par
vinttplot=vinttplot.par
vintzplot=vintzplot.par
uni... | Shell |
#! /bin/sh
# Velocity analyses for the cmp gathers
# Authors: Dave Hale, Jack K. Cohen, with modifications by John Stockwell
# NOTE: Comment lines preceeding user input start with ##
#set -x
## Set parameters
datadir=.
velpanel=your_data_cdp.su # data sorted in cdps, multiple-suppressed
vpicks=nmovel.par # ou... | Shell |
#! /bin/sh
set -x
## The assumption is that source and receiver strengths are
## the only quantities that can influence the RMS power
## of a source or output channel gather
##
## The possible source of error in this approach is that we have
## not corrected for the response of the geology.
## correcting for souce ... | Shell |
#! /bin/sh
vnmo=1500,1757,2510
tnmo=0.0,1.5,3.38
data=gain.jon\=1.cdp\=265.su
# view nmo corrected data in the Radon domain
sunmo vnmo=$vnmo tnmo=$tnmo < $data |
suradon offref=-3237 interoff=-287 pmin=-2000 \
pmax=2000 dp=8 choose=0 igopt=2 \
depthref=1000 | suximage perc=99 &
exit 0
# nmo->radon-> inverse NMO:... | Shell |
#! /bin/sh
# Velocity analyses for the cmp gathers
# Authors: Dave Hale, Jack K. Cohen, with modifications by John Stockwell
# NOTE: Comment lines preceeding user input start with ##
#set -x
## Set parameters
velpanel=radon.gain.cdp=265.su # gained and deconvolved seismic data,
... | Shell |
#! /bin/sh
#set -x
# set parameters here
dmi=your_depth_section_here.su # depth migrated image
dz=3 # depth sampling interval
dx=1 # width sampling interval
perc=90
method=linear # interpolation method
parfile=unif2.par # ... | Shell |
#! /bin/sh
# Gaussian Beam
#set -x
# use a v(z,x) velocity profile here
vfile=hunewvelzx.bin
stacked=put_your_stacked_data_here
# vary the values of dz and nz as a test before running the full model
sumiggbzo < $stacked dx=12.5 dz=3 nz=1500 \
verbose=1 vfile=$vfile > gb.seismic.su
exit 0
| Shell |
#! /bin/sh
sustolt < stack.nmo.myradon.gain.jon=1.su \
par=stolt.par cdpmin=1 cdpmax=2142 taper=30 \
dxcdp=12.5 > stolt.seis.su
exit 0
| Shell |
#! /bin/sh
# fake data no multiples
sunull nt=1500 ntr=60 dt=.004 |
sushw key=gx,offset a=3300,-3237 b=25,50 c=1,1 |
suchw key1=sx key2=gx key3=offset a=0 b=1 c=1 |
suaddevent type=nmo nt=1500 t0=.5 dt=.004 vel=1500 |
suaddevent type=nmo nt=1500 t0=.6 dt=.004 vel=1525 |
suaddevent type=nmo nt=1500 t0=.7 dt=.004 ve... | Shell |
#! /bin/sh
sukdmig2d infile=simple.su outfile=kdmig.simple.su ttfile=tfile.simple \
ft=0 fzt=0 nzt=501 dzt=4.00 angmax=80.0 nxo=80 dxo=40 nzo=150 dzo=12 \
fxt=0 nxt=80 dxt=40 fs=0 ns=80 ds=40 \
dxm=40 v0=2000 noff=1 off0=0 doff=0
| Shell |
#! /bin/sh
rayt2d vfile=vel.kdmig.simple \
dt=.004 nt=501 fa=-80 na=80 \
fz=0 nz=501 dz=4 \
fx=0 nx=80 dx=40 ek=0 \
nxs=80 fxs=0 dxs=40 ms=1 \
tfile=tfile.simple
xmovie < tfile.simple clip=3 n1=501 n2=80 loop=1 title="%g traveltime table" &
| Shell |
#! /bin/sh
# Shell script to build velocity profiles with unif2
# input parameters
modelfile=syncline.unif2
velfile=syncline.bin
n1=200
n2=400
d1=10
d2=10
# use unif2 to build the velocity profile
unif2 <$modelfile method=$i ninf=2 nx=$n2 nz=$n1 v00=2000,3000 \
ninf=1 method=spline > $velfile
# view the velocity pr... | Shell |
#! /bin/sh
# Gaussian Beam
set -x
# Gaussian beam migration
sumiggbzo < seismic3.su dx=12.5 dz=3 nz=1500 vfile=newvelzx.bin verbose=1 > gb.seismic.su
suximage < gb.seismic.su wbox=750 hbox=550 perc=99 title="GB Migration" f2=0 &
supsimage < gb.seismic.su width=7.5 hbox=5.5 perc=99 title="GB Migration" f2=0 > gb.... | Shell |
#! /bin/sh
set -x
# fourier finite difference
# note dz*nz=4500 to get to the bottom of the model
# vary the values of dz and nz as a test before running the full model
sumigffd < seismic3.su dx=12.5 dz=3 nz=1500 vfile=newvelxz.bin > ffd.seismic.su
suximage < ffd.seismic.su wbox=750 hbox=550 perc=99 title="FFD Mig... | Shell |
#! /bin/sh
set -x
# split step
# note dz*nz=4500 to get to the bottom of the model
# vary the values of dz and nz as a test before running the full model
sumigsplit < seismic3.su dx=12.5 dz=3 nz=1500 vfile=newvelxz.bin > split.seismic.su
suximage < split.seismic.su wbox=750 hbox=550 perc=99 title="SPLIT Migration... | Shell |
#! /bin/sh
set -x
# Phase shift plus interpolation
# note dz*nz=4500 to get to the bottom of the model
# vary the values of dz and nz as a test before running the full model
sumigpspi < seismic3.su dx=12.5 dz=3 nz=1500 vfile=newvelxz.bin > pspi.seismic.su
suximage < pspi.seismic.su wbox=750 hbox=550 perc=99 title=... | Shell |
#! /bin/sh
# generate screen images and PostScript Hardcopy files
# Finite difference migration
suximage < fd.seismic.su wbox=750 hbox=550 perc=99 title="FD Migration" f2=0 &
supsimage < fd.seismic.su width=7.5 hbox=5.5 perc=99 title="FD Migration" f2=0 > fd.seismic.ps
# Fourier finite difference
suximage < ffd.sei... | Shell |
#! /bin/sh
set -x
# finite difference
# note dz*nz=4500 to get to the bottom of the model
# vary the values of dz and nz as a test before running the full model
sumigfd < seismic3.su dx=12.5 dz=3 nz=1500 vfile=newvelxz.bin > fd.seismic.su
suximage < fd.seismic.su wbox=750 hbox=550 perc=99 title="FD Migration" f2=0... | Shell |
#! /bin/sh
suxmovie < /cwpscratch/Data3/timemovie.su perc=98 n1=1500 n2=2142 loop=1 title="time section frame %g" &
| Shell |
#! /bin/sh
suttoz nz=1500 dz=3 < ps.seis.su \
t=0.0,1.0,2.5,3.45,4.36,5.1,5.45,5.95 \
v=1500,2000,3738.45,3338,3876.32,3678.11,5706.7,4156.17 \
> ps.depth.seis.su
exit 0
exit 0
| Shell |
#! /bin/sh
suxmovie < /cwpscratch/Data3/depthmovie.su perc=98 n1=1500 n2=2142 loop=1 title="depth section frame %g" &
| Shell |
#! /bin/sh
vel=1400
dvel=100
rm timemovie.su depthmovie.su
while [ "$vel" -lt 5000 ]
do
sustolt < seismic3.su cdpmin=1 cdpmax=2142 vmig=$vel dxcdp=12.5 > tmp.su
cat tmp.su >> timemovie.su
suttoz < tmp.su v=$vel dz=3 nz=1500 >> depthmovie.su
echo $vel
vel=`expr $vel + $dvel`
done
#suxmovie < movie.su perc=9... | Shell |
#! /bin/sh
sumigps < seismic3.su \
tmig=0.0,1.0,2.5,3.45,4.36,5.1,5.45,5.95 \
vmig=1500,2000,3738.45,3338,3876.32,3678.11,5706.7,4156.17 \
dx=12.5 > ps.seis.su
exit 0
| Shell |
#! /bin/sh
suttoz nz=1500 dz=3 < stolt.seis.su \
t=0.0,1.0,2.5,3.45,4.36,5.1,5.45,5.95 \
v=1500,2000,3738.45,3338,3876.32,3678.11,5706.7,4156.17 \
> stolt.depth.seis.su
exit 0
| Shell |
#! /bin/sh
sustolt < seismic3.su cdpmin=1 cdpmax=2142 \
tmig=0.0,1.0,2.5,3.45,4.36,5.1,5.45,5.95 \
vmig=1500,2000,3160,3210,3360,3408,3600,3650 \
dxcdp=12.5 > stolt.seis.su
exit 0
| Shell |
#! /bin/sh
cd Demos ; Clean
exit 0
| Shell |
#! /bin/sh
set -x
model=model10LayersInitial
data=gatherZR.su
scale=1
corrData=
prior=0
datacov=0
impedance=0
p=1
s=1
r=0
verbose=1
corrVP=
corrVS=
corrRHO=
orientation=Z
dz=0.01
targetbeg=1.00
targetend=1.08
r1=0.0
nr=48
dr=0.025
zs=0.005
F1=0
F2=0
F3=1
receiverfile=
u1=0.0
u2=2.0
directwave=0
nu=300
f1=2
f2=50
dt=0... | Shell |
#! /bin/sh
#demo for SUDREFSVMASTER
out=gatherZR.su
model=model10Layers
nr=48
dr=0.025
r1=0.
zs=.005
u1=0.0
u2=2.0
nu=300
f1=2
f2=50
dt=0.004
tmax=4
directwave=0
F1=0
F2=0
F3=1
wu=10
ww=25
fr=1
hanning=1
tau=7.07
nproc=1
nfreqproc=
verbose=1
recfile=
set -x
rm -f $file
sudrefsvmaster model=$mod... | Shell |
#! /bin/sh
#DEMO for logBlock
set -x
logLAS=logExample
lmedian=30
mincontrast=5
ncols=5
columns=1,2,5,3
verbose=0
output=blockedLog
logBlock logLAS=$logLAS \
lmedian=$lmedian \
mincontrast=$mincontrast \
ncols=$ncols \
columns=$columns \
verbose=$verbose > $output
| Shell |
#! /bin/sh
#DEMO for program covAdap
set -x
model=model10Layers
trend=model10LayersInitial
mode=C
dz=0.01
targetbeg=1.00
targetend=1.08
window=0.08
verbose=1
time covAdap \
model=$model \
trend=$trend \
mode=$mode \
dz=$dz \
targetbeg=$targetbeg \
targetend=$targetend \
window=$window \
ver... | Shell |
#! /bin/sh
#DEMO for dataCovar
set -x
#creating realizations
suplane nt=251 ntr=32 | suaddnoise sn=1 > data1
suplane nt=251 ntr=32 > data2
sudiff data1 data2 > noise
rm -f data1 data2
realizations=noise
nreal=32
t1=0
t2=1
scale=1
exponential=1
window=0
verbose=1
inverse=1
cov=covar
invcov=invcovar
dataCovar \
... | Shell |
#! /bin/sh
#DEMO for gaussSampling
#set -x
#setting number of realizations
number=10
i=1
covariance=alpha
mean=model10LayersInitial
exponential=1
impedance=0
p=1
s=0
r=0
targetbeg=1.00
targetend=1.08
dz=0.01
verbose=1
output=realizations
>$output
while [ $i -le $number ]
do
gaussSampling \
covariance=$... | Shell |
#! /bin/sh
cd lib ; rm libdga.a
cd ..
cd Demo ; Clean
| Shell |
#! /bin/sh
#Cleaning purposes
rm *demo*
rm xcor
rm *log*
| Shell |
#! /bin/sh
data=/u/elbert/wgouveia/summer/dga/demo
input=$data/datademo.su
xcor=$data/xcor
path=/u/elbert/wgouveia/pvm/RIOS
dt=.004
$path/sustapply sources=20 receivers=43 maxfold=20 cmps=62 \
datafile=$input \
staticsfile=$data/answer.demo.4 \
verbose=1 |
sustatic hdrs=1 sign=-1 |
sustack |
suxwigb f1=0 d1=$dt d... | Shell |
#! /bin/sh
DATA=.
n1=501
n2=24
file=$DATA/data
seismic_data_file=$DATA/line
dataheader=$DATA/DemoCDP.su
finaldata=$DATA/datademo.su
#use susynlv to make synthetic data
susynlv nt=$n1 dt=.004 ft=0.0 \
nxo=$n2 dxo=.0 fxo=0.0 fxs=0. er=0 ob=1 \
nxs=1 v00=2.0 dvdz=0 dvdx=0 smooth=1 fpeak=25 \
ref="0.,1.;5.,1." > $fil... | Shell |
#! /bin/sh
# check to see if the CWPROOT environment variable is set
# this shell is part of the general CWP installing and maintenence environment
# John Stockwell 9 Dec 1992 -- Center for Wave Phenomena
PATH=/bin:/usr/bin:/usr/ucb:/usr/bsd
CMD=`basename $0`
if test "${CWPROOT}" = ""
then
echo "CWPROOT environment... | Shell |
#! /bin/sh
# make directories for CWP/SU codes installation
B=$CWPROOT/bin
I=$CWPROOT/include
L=$CWPROOT/lib
mkdir $CWPROOT
mkdir $B $L $I
mkdir $I/Xtcwp $L/X11 $L/X11/app-defaults $I/Xmcwp
mkdir $I/Triangles
mkdir $I/Wpc
mkdir $I/MGL
mkdir $I/Reflect
exit 0
| Shell |
# This shell script attempts to find the actual lexical spelling
# of the following objects:
# _iob : the traditional name of the stdio FILE structure
# _filbuf: the traditional name of the function to fill a FILE buffer
# _flsbuf: the traditional name of the function to flush a FILE buffer
#
# _uflow: _filbuf on Linux... | Shell |
if test "`cat Make.state`" != "$1"
then rm *.o Stdio_b/*.o Stdio_s/*.o Sfio_f/*.o
fi >/dev/null 2>&1
echo "$1" > Make.state
exit 0
| Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# THIS_YEAR - print the current year
#
# Usage: this_year
#
# NOTES - useful for building dated filenames, etc.
#
# /**************** end self doc ********************************/
# Author: John Stockwell, Jun 1993
date | awk '{ print $... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# COPYRIGHT - insert CSM COPYRIGHT lines at top of files in working directory
#
# Usage: copyright file(s)
#
# /**************** end self doc ********************************/
# $Author: john $
# $Source: /NeXTMount_3.1b/usr/local/cwp/src... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# OVERWRITE - copy stdin to stdout after EOF
#
# This shell is called from the shell script: replace
#
# /**************** end self doc ********************************/
# Kernighan and Pike - page 154
opath=$PATH
PATH=/bin:/usr/bin:... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# USERNAMES - get list of all login names
#
# Usage: usernames
#
# /**************** end self doc ********************************/
PATH=/bin:/usr/bin:/usr/ucb
awk -F: '{print $1 ": " $5}' /etc/passwd |
sed '
/The Super-user/d
/switch ... | Shell |
#! /bin/sh
# locks - list rcs files that are locked
# Usage: locks
# Jack K. Cohen, 1987
PATH=/bin:/usr/bin:/usr/ucb
for i in RCS/*,v
do
LINE=`head -5 $i | awk 'NR==5 {print $2}'`
if [ "$LINE" = "strict;" ]
then
echo $i: $LINE
fi
done
exit 0
| Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# VARLIST - list variables used in a Fortran program
#
# Usage: varlist file.f ...
#
# Output is in the file: vars.file
#
# /**************** end self doc ********************************/
# Jack K. Cohen, 1985
BIN=${CWPROOT}/bin
PATH=... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# CPALL , RCPALL - for local and remote directory tree/file transfer
#
# Usage: cpall sourcedir destinationdir
# Caveat: destinationdir must exist and be writeable by the user
#
# Usage: rcpall sourcedir remotemachine destinationdir
#
... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# CWPFIND - look for files with patterns in CWPROOT/src/cwp/lib
#
# Usage: cwpfind pattern_fragment
# cwpfind -e exact_pattern
#
# /**************** end self doc ********************************/
# Copyright 1985 by Jack K. Cohen
... | Shell |
#! /bin/sh
#/*********************** self documentation **********************/
# ARGV - give examples of dereferencing char **argv
#
# Usage: argv
#
#/**************** end self doc ********************************/
# Jack K. Cohen, 1985
PATH=/bin:/usr/bin:/usr/ucb
exec cat << 'END'
char *argv[] = char **argv
argv ... | Shell |
#! /bin/sh
# why - obscure joke
PATH=/bin:/usr/bin:/usr/ucb
exec echo "Because life is a transient"
| Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# ZAP - kill processes by name
#
# Typical usages:
# zap ximage
# zap 'xmovie|xgraph'
#
# Zap accepts full pattern matching for the process names
#
# Caveat: zap assumes that the FIRST field produced by the
# Unix "ps" command is the pid (... | Shell |
#! /bin/sh
#/*********************** self documentation **********************/
# WEEKDAY - prints today's WEEKDAY designation
#
# Usage: weekday
#
# Note: Useful for building dated filenames
#
# /**************** end self doc ********************************/
# Author: John Stockwell, 28 May 1993
PATH=/bin:/usr/bin:... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# FILETYPE - list all files of given type
#
# Usage: filetype string_from_file_output
#
# Examples:
# filetype text - list printable files
# filetype stripped - list unstripped files
# /**************** end self doc ***********... | Shell |
#! /bin/sh
#/*********************** self documentation **********************/
# TODAYS_DATE - prints today's date in ZULU format with no spaces
#
# Usage: todays_date
#
# Note: Useful for building dated filenames
#
# /**************** end self doc ********************************/
# Author: John Stockwell, 28 May 1... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# REPLACE - REPLACE string1 with string2 in files
#
# Usage: replace string1 string2 files
#
#/**************** end self doc ********************************/
# Kernighan and Pike - page 155
BIN=${CWPROOT}/bin
PATH=/bin:/usr/bin:/usr/u... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# NEWCASE - Changes the case of all the filenames in a directory, dir
#
# Usage: newcase -l dir change all filenames to lower case
# -u dir change all filenames to upper case
#
# Notes: Useful for files downloaded from VA... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# DIRTREE - show DIRectory TREE
#
# Usage: dirtree
#
# /**************** end self doc ********************************/
# John Stockwell May 1992
# (based loosely on a shell of the same name by Jack K. Cohen, 1988)
ROOT=${CWPROOT}
BIN=$... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# Grep - recursively call egrep in pwd
#
# Usage: Grep [-egrep_options] pattern
#
# Caution: Do NOT redirect into file in pwd, either use something
# like >../Grep.out or perhaps pipe output into mail to yourself.
#
# Author: Jack, 7/95... | Shell |
#! /bin/sh
#/*********************** self documentation **********************/
# TIME_NOW - prints time in ZULU format with no spaces
#
# Usage: time_now
#
# Note: Useful for building dated filenames
#
# /**************** end self doc ********************************/
# Author: John Stockwell, 28 May 1993
PATH=/bin... | Shell |
#! /bin/sh
#/*********************** self documentation **********************/
# PRECEDENCE - give table of C precedences from Kernighan and Ritchie
#
# Usage: precedence
#
#/**************** end self doc ********************************/
PATH=/bin:/usr/bin:/usr/ucb
exec cat <<'END'
TABLE of PREC... | Shell |
#! /bin/sh
# Clean.sh - recursively call Clean.sh in the demo directories
# Test back-up dir first (at CWP must run on NeXT-net)
# Take care of subdirectories
for i in `ls`
do
if
[ -d $i ]
then
cd $i
if
[ -f Clean.sh ]
then
Clean.sh
fi
rm -f *~ \#*\# .nfs* *.eps
cd ..
fi
done
# Take care of t... | Shell |
#! /bin/sh
set -v
in1=t.a
in2=amp.a
in3=d21.a
in4=d22.a
in5=d23.a
in6=d31.a
in7=d32.a
in8=d33.a
in9=a1.a
in10=b1.a
out1=t
out2=amp
out3=d21
out4=d22
out5=d23
out6=d31
out7=d32
out8=d33
out9=a1
out10=b1
tableq
a2b<$in1 n1=1>$out1
a2b<$in2 n1=1>$out2
a2b<$in3 n1=1>$out3
a2b<$in4 n1=1>$out4
a2b<$in5 n1=1>$out5
a2b<$in... | Shell |
#! /bin/sh
# shell for running unif2 --- uniformly sampled Cshot model
set -v
nx=1 nz=101 dz=15 fz=.0
ninf=3 npmax=201
unif2 <flatmodel ninf=$ninf npmax=$npmax \
nz=$nz dz=$dz fz=$fz nx=$nx \
v00=2000,3000,5000,7500 >vfile
out=vfiles.a
tmp1=tmp1
tmp2=tmp2
tmp3=tmp3
n1=101 d1=15 r1=75
n2=3 ... | Shell |
#! /bin/sh
#set -v
ximage<vfile n1=101 \
d1=0.015 d2=4.0 f2=1 label1="Depth (km)" label2="X (km)"\
title="Velocity"\
d1num=0.4 d2num=1 whbox=700 hbox=400\
titlesize=30 labelsize=24\
x2beg=0 x2end=4&
suximage<flat3lay500off.su \
d1=0.002 d2=0.01 f2=0.0 label1="Traveltime (s)" label2="X (km)... | Shell |
#! /bin/sh
# Clean up residue from runs
rm -f vfile*
rm -f t amp a1 b1 d21 d22 d23 d31 d32 d33
rm -f data* *.su *.ps junk* test*
| Shell |
#! /bin/sh
#set -v
psimage<vfile n1=101 \
d1=0.015 d2=4.0 f2=1 label1="Depth (km)" label2="X (km)"\
title="Velocity"\
d1num=0.4 d2num=1 width=7.0 height=4.0\
titlesize=30 labelsize=24\
x2beg=0 x2end=4>vfile.ps
supsimage<flat3lay500off.su \
d1=0.002 d2=0.01 f2=0.0 label1="Traveltime (s)" l... | Shell |
#! /bin/sh
set -v
input=flat3lay500off.su
vfile=vfile
tfile=t
ampfile=amp
d21file=d21
d22file=d22
d23file=d23
d31file=d31
d32file=d32
d33file=d33
a1file=a1
b1file=b1
output=inv500offw3.su
output1=inv500offw3.ps
geo_type=3
com_type=3
fxt=0.0 dxt=50.0 nxt=81
fyt=0.0 dyt=50.0 nyt=81
fzt=0.0 dzt=25.0 nzt=61
dt=0.002... | Shell |
#! /bin/sh
# Run CSHOT with CWP PostScript Graphics
model=1
cshot1 >/dev/null
cshot2
suaddhead <comodel${model}traces ftn=1 ns=701 |
sushw key=dt a=2000 >flat3lay500off.su
rm -f comodel1*
rm -f junk.su
exit 0
| Shell |
#! /bin/sh
# clean up
cd ./Demo
Clean.sh
exit 0
| Shell |
#! /bin/sh
cd lib
rm *.a
cd ../main
rm INSTALL *.o
| Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# UPDATEDOC - put self-docs in ../doc/Stripped and ../doc/Headers
#
# Usage: updatedoc path
#
# Notes:
# Paths include: cwp/main cwp/lib cwp/shell par/main par/lib par/shell
# xplot/main xplot/lib psplot/main psplot/lib psplot/shell
#... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# UPDATEDOCALL - put self-docs in ../doc/Stripped
#
# Usage: updatedocall
#
# Note: this shell uses updatedoc to update the database used by
# suname and gendocs
#
# /**************** end self doc ********************************... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# STRIPTOTXT - put files from $CWPROOT/src/doc/Stripped into a new
# directory in the form $CWPROOT/src/TXT/NAME.txt
#
# Usage: striptotxt
#
# Author: John Stockwell, Sept 2001
# /**************** end self doc *************... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# UPDATEHEAD - update ../doc/Headers/Headers.all
#
# Usage: updatehead
#
# Notes:
#
# This file builds the database used by suname
# /**************** end self doc ********************************/
##################$############... | Shell |
#! /bin/sh
# /*********************** self documentation **********************/
# GENDOCS - generate complete list of selfdocs in latex form
#
# Usage: gendocs -o output filename is: selfdocs.tex
#
# /**************** end self doc ********************************/
# Author: John Stockwell -- 5 Jan 1992
PATH=/bin:/... | Shell |
#! /bin/sh
rm *.o
| Shell |
#! /bin/sh
# Clean - master clean for this directory and ALL the Demo subdirectories
for i in Demo*
do
cd $i
Clean
cd ..
done
| Shell |
#! /bin/sh
# Clean up residue from runs
demo=1
rm -f demo${demo}plot demo${demo}par demo${demo}psfile[1-6] cshot1plot \
demo${demo}traces demo${demo}shot junk*
| Shell |
#! /bin/sh
# Run CSHOT with CWP PS Graphics
demo=1
MACHINE=keller
USER="-l jkc" # don't need if usernames the same on both machines
x1beg=0 x1end=10000 x2beg=0 x2end=10000
cshot1 |
cshotplot >demo${demo}plot outpar=demo${demo}par
psgraph <demo${demo}plot par=demo${demo}par style=seismic \
title="Dome " \
... | Shell |
#! /bin/sh
# Run CSHOT with CWP X Graphics
demo=1
x1beg=0 x1end=10000 x2beg=0 x2end=10000
cshot1 |
cshotplot >demo${demo}plot outpar=demo${demo}par
xgraph <demo${demo}plot par=demo${demo}par \
title="Dome " \
-geometry 600x600+650-70 \
label1="Depth (ft)" label2="Range (ft)" \
x1beg=$x1beg x1end=$x1end x2beg... | Shell |
#! /bin/sh
# Clean up residue from runs
rm -f record
(cd model.dir; Clean)
(cd inversion.dir; Clean)
| Shell |
#! /bin/sh
# Clean up residue from runs
demo=5
rm -f demo${demo}plot demo${demo}par demo${demo}psfile[1-6] cshot1plot \
demo${demo}traces demo${demo}shot
| Shell |
#! /bin/sh
# Run CSHOT with CWP PS Graphics
set -x
demo=5
x1beg=0 x1end=12000 x2beg=0 x2end=24000
cshot1>cshot1plot
cshotplot <cshot1plot >demo${demo}plot outpar=demo${demo}par
psgraph <demo${demo}plot par=demo${demo}par style=seismic \
title=" Ray Plot" \
ybox=3.5 hbox=4 grid1=dash grid2=dash \
label1=... | Shell |
Subsets and Splits
No community queries yet
The top public SQL queries from the community will appear here once available.