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#! /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 $i
if
[ -f Clean.sh ]
then
Clean.sh
fi
rm -f *~ \#*\# .nfs* *.eps
cd ..
fi
done
# Take care of top... | Shell |
#! /bin/sh
# display impulse responses
suximage < data.su wbox=300 hbox=300 xbox=10 ybox=10 \
title="Test impulse data" &
suximage < mig.split wbox=300 hbox=300 xbox=330 ybox=10 \
title="Split Step" &
suximage < mig.ffd wbox=300 hbox=300 xbox=630 ybox=10 \
title="Fourier Finite Difference" &
suximage < mig.f... | Shell |
#! /bin/sh
# Clean created data files
rm -f data.su *.eps *.su mig.* vfile*
exit
| Shell |
#! /bin/sh
set -x
# make spike data and set headers
suspike nt=256 ntr=512 nspk=1 it1=128 ix1=256 |
sushw key=dt,d2,cdp a=4000,4,1 b=0,0,1 >data.su
# make background velocity profile
makevel nx=512 nz=256 dvdx=0.0 dvdz=0.0 v000=2500 >vfile.temp
# transpose background wavespeed profile
# for sumigsplit, sumigfd, s... | Shell |
#! /bin/sh
# shell for uniformly sampling velocity from a layered model
set -v
nz=251 dz=10 fz=.0 labelz="Depth (m)"
nx=161 dx=25 fx=0000.0 labelx="Distance (m)"
ninf=5 npmax=201
unif2 <input >data.v ninf=$ninf npmax=$npmax \
nz=$nz dz=$dz fz=$fz nx=$nx dx=$dx fx=$fx \
v00=2000,1500,1000,1000,3500,4000 \
dvdz... | Shell |
#! /bin/sh
WIDTH=550
HEIGHT=400
XOFF1=100
YOFF1=550
XOFF2=700
YOFF2=700
# Plot Synthetic common offset data
nt=501 dt=0.004 ft=0.0 nx=201 dx=0.015 fx=0.5 offset=0.1
suximage < data perc=99\
label1="Time (sec)" label2="Midpoint (km)" \
wbox=$WIDTH hbox=$HEIGHT xbox=$XOFF1 ybox=$YOFF1 \
title="Common Offset ... | Shell |
#! /bin/sh
# shell for smoothing a uniformly sampling velocity and for generating a
# slowness perturbation
set -v
n1=251 r1=200 dz=10 fz=0 labelz="Depth (m)"
n2=161 r2=200 dx=25 fx=0 labelx="Midpoint (m)"
d1r=50 n1r=51 n2r=81 d2r=50
# smooth velocity and resample
smooth3d<data.v r1=$r1 r2=$r2 d1=$dz d2=$dx n1=$n1... | Shell |
#! /bin/sh
# shell for plotting the original and smoothed v(x,z) model
#set -v
nz=251 dz=10 fz=.0 labelz="Depth (m)"
nx=161 dx=25 fx=0000.0 labelx="Distance (m)"
ninf=5 npmax=201
psimage <data.v style=seismic \
n1=$nz d1=$dz f1=$fz grid1=dot label1="$labelz" \
n2=$nx d2=$dx f2=$fx grid2=dot label2="$labelx" \
... | Shell |
#! /bin/sh
# Clean up residue from runs
rm -f data* *.eps vpfile vsfile
| Shell |
#! /bin/sh
# shell for plotting synthetic data
nt=501 fxm=0.5 dt=0.004 dxm=0.015
supsimage<data n1=$nt f2=$fxm d1=$dt d2=$dxm perc=99\
label1="Time (s)" label2="Midpoint (km)" \
ybox=4 hbox=4 \
d1num=1 d2num=1 \
title="Common Offset Data (Offset=100 m)" > syndata.eps
# Plotting inverted data
n1=251 f2=0 d2=0.015... | Shell |
#! /bin/sh
# shell for Kirchhoff inversion
set -x
input=data
output=data.inv
fxm=500 nxm=201 dxm=15 nxd=5
nx=81 nz=51 dx=50 dz=50 fx=0 nxb=40 vfile=vsfile
dxo=15 nxo=267 fxo=0 fzo=0 dzo=10 nzo=251
fmax=50 ls=1 verbose=1 pert=1 vpfile=vpfile
sufrac phasefac=0.25<$input |
suinvvxzco nxm=$nxm dxm=$dxm fxm=$fxm nx... | Shell |
#! /bin/sh
# shell for Kirchhoff integral modeling
set -x
output=data
nt=501 dt=0.004 ft=0.0 tmin=0.2
nxm=201 dxm=15 fxm=500 nxd=5 dxo=200 nxo=1 fxo=100
nx=81 nz=51 dx=50 dz=50 fx=0 nxb=50
fpeak=30 ls=1 pert=1 vpfile=vpfile
susynvxz< vsfile nt=$nt dt=$dt ft=$ft tmin=$tmin \
nxm=$nxm dxm=$dxm fxm=$fxm nxd=$nxd ... | Shell |
#! /bin/sh
# shell for plotting the original and smoothed v(x,z) model
#set -v
nz=251 dz=10 fz=.0 labelz="Depth (m)"
nx=161 dx=25 fx=0000.0 labelx="Distance (m)"
ninf=5 npmax=201
xmovie <data.v \
n1=$nz d1=$dz f1=$fz label1="$labelz" \
n2=$nx d2=$dx f2=$fx label2="$labelx" \
-geometry 550x400+100+10 \
title=... | Shell |
#! /bin/sh
# shell for plotting the original and smoothed v(x,z) model
#set -v
WIDTH=400
HEIGHT=600
WIDTHOFF1=10
WIDTHOFF2=430
WIDTHOFF3=860
HEIGHTOFF1=20
# Plot Synthetic data
nt=501 dt=0.004 ft=0.0 nx=121 dx=25 fx=0
suximage < data d1=$dt f1=$ft d2=$dx f2=$fx perc=99.5\
label1="Time (sec)" label2="Midpoint (... | Shell |
#! /bin/sh
# Clean up residue from runs
rm -f *data data* tfile *.eps vfile jp* *.su
| Shell |
#! /bin/sh
# shell for plotting synthetic data and migrated data
supsimage<data perc=99.5\
label1="Time (s)" label2="Midpoint (m)" \
ybox=4 hbox=4 \
title="Synthetic Data" > syndata.eps
# Plotting migrated data
supsimage<data.stolt perc=99.5\
label1="Depth (km)" label2="Midpoint (km)" \
ybox=4 hbox=4 \
title... | Shell |
#! /bin/sh
# shell for Kirchhoff modeling for linear v(x,z)
set -x
nt=725 dt=0.004 ft=0.0 tmin=0.2 nxs=121 dxs=0.02 fxs=0.05
fxo=0.1 dxo=0.025 nxo=60
fpeak=30 er=0 ls=1 v00=1.5 dvdx=0 dvdz=0
susynlv nt=$nt dt=$dt ft=$ft nxs=$nxs dxs=$dxs fxs=$fxs fxo=$fxo\
dxo=$dxo nxo=$nxo tmin=$tmin v00=$v00 dvdx=$dvdx dvdz=$d... | Shell |
#! /bin/sh
cdpmin=1 cdpmax=121 dxcdp=20 verbose=1
vmig=1500 tmig=0.0
sustolt < data noffmix=1 cdpmin=$cdpmin cdpmax=$cdpmax \
vmig=$vmig tmig=$tmig \
verbose=$verbose dxcdp=$dxcdp > data.stolt
| Shell |
#! /bin/sh
cd Suinvco3d
./Clean.sh
| 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 $i
if
[ -f Clean.sh ]
then
Clean.sh
fi
rm -f *~ \#*\# .nfs* *.eps
cd ..
fi
done
# Take care of to... | Shell |
#! /bin/sh
# shell for running unif2 --- uniformly sampled Cshot model
# data is smoothed with smo2d
set -v
nx=1 dx=80 fx=1000 labelx="Distance (m)"
nz=101 dz=80 fz=.0 labelz="Depth (m)"
ninf=5 npmax=201
xsmoothing=0 zsmoothing=0
unif2 <interface ninf=$ninf npmax=$npmax \
nz=$nz dz=$dz fz=$fz nx=$nx dx=$dx fx=$f... | Shell |
#! /bin/sh
#set -v
WIDTH=250
HEIGHT=250
XOFF=0
YOFF=0
XOFF1=300
YOFF1=300
XOFF2=600
YOFF2=600
data=data3d.su
output=inv.su
nzo=101 nxo=32 nyo=32
echo "inline view"
suxmovie <$data loop=1 n1=$nzo n2=$nxo n3=$nyo mode=0 \
-geometry ${WIDTH}x${HEIGHT}+${XOFF}+${YOFF} \
title="Point Scatterer data (inline view)" &... | Shell |
#! /bin/sh
rm *.su junk* vfile* *.ps
| Shell |
#! /bin/sh
# Create a 3D data set for Bill Wingle's block program--the
# name should end with ".su"
#
# This data set consists of one shot per line: the
# shotpoints move orthogonal to the receiver line
# with the scattering point below the midpoint of
# surface array.
#
# The data set consists of 32 receiver lines and... | Shell |
#! /bin/sh
j=0
k=0
jmax=32
while [ "$j" -ne "$jmax" ]
do
suwind < inv.su key=cdp min=$j count=1 | suxwigb
j=`expr $j + 1 `
done
exit 0
| Shell |
#! /bin/sh
set -x
input=./data3d.su
vfile=./vfile
output=inv.su
dt=0.01 i=1 doff=0 n=1 offs=0 dfxm=0 fxm=0. ny=32
nxm=32 dxm=100 dxo=100 nxo=32 dyo=100 nyo=32 fxo=0. fyo=0. dzo=20 nzo=101
fzo=0. nz=101 dy=100 dz=20 fx=0. nxb=5 ang=10
sufrac<$input dt=$dt phase=0.5|
suinvzco3d dt=$dt offs=$offs ny=$ny nxm=$nxm... | Shell |
#! /bin/sh
#set -v
data=data3d.su
output=inv.su
psout1=data3d.ps
psout2=inversion.ps
nzo=101 nxo=32 nyo=32
sustrip<$data |pscube n1=$nzo n2=$nxo n3=$nyo > $psout1
nzo=32 nxo=32 nyo=32
sustrip<$output|pscube n1=$nzo n2=$nxo n3=$nyo > $psout2
echo
echo "You may view the files $psout1 and $psout2 with your PostScrip... | Shell |
#! /bin/sh
# shell for running unif2 --- uniformly sampled Cshot model
# data is smoothed with smo2d
set -v
nx=1 dx=0.1 fx=0. labelx="Distance (m)"
nz=101 dz=0.1 fz=.0 labelz="Depth (m)"
ninf=3 npmax=201
xsmoothing=0 zsmoothing=0
unif2 <interface ninf=$ninf npmax=$npmax \
nz=$nz dz=$dz fz=$fz nx=$nx dx=$dx fx=... | Shell |
#! /bin/sh
#set -v
output=inv.su
psout=inversion.ps
nzo=20 nxo=20 nyo=20
suxmovie <$output loop=1 mode=0 n1=$nzo n2=$nxo n3=$nyo \
title="Impulse Response 3D inline view " &
suxmovie <$output loop=1 mode=1 n1=$nzo n2=$nxo n3=$nyo \
title="Impulse Response 3D crossline view " &
suxmovie <$output loop=1 mode=2 n1=$n... | Shell |
#! /bin/sh
set -x
output=data.su
nt=101 dt=0.1 ntr=121 offset=0 nspk=1 ix1=61 it1=51
suspike nt=$nt dt=$dt ntr=$ntr nspk=$nspk offset=$offset \
ix1=$ix1 it1=$it1 >$output
supsimage<$output > sudata.ps
exit
| Shell |
#! /bin/sh
rm *.su junk* vfile* *.ps
| Shell |
#! /bin/sh
set -x
input=data.su
output=inv.su
vfile=vfile
dt=0.15 offs=0. i=1 doff=0 n=1 dfxm=0 fxm=0 ny=11
nxm=11 dxm=1 dxo=0.5 nxo=20 dyo=0.5 nyo=20 fxo=0 fyo=0. dzo=0.5
nzo=20
fzo=0. nz=101 dy=1 dz=0.1 fx=0. nxb=70 na=100
sufrac<$input dt=$dt phase=0.5 |
suinvzco3d dt=$dt offs=$offs ny=$ny nxm=$nxm dxm=$dxm \... | Shell |
#! /bin/sh
#set -v
output=inv.su
psout=inversion.ps
nzo=20 nxo=20 nyo=20
sustrip<$output|pscube n1=$nzo n2=$nxo n3=$nyo > $psout
echo
echo "You may view the file $psout with your PostScript previewer"
echo
exit 0
| Shell |
#! /bin/sh
rm -rf vfile* *.su *.ps
exit
| Shell |
#! /bin/sh
#
set -x
nt=300 dt=0.004 ft=0.0 nxm=150 dxm=0.01 fxm=0.0 dxo=0 nxo=1 fxo=0.0
fpeak=20 ls=0 dvdx=0.2 dvdz=0.5 ndpfz=5 v00=2.0
pert=0 ob=1 er=0
DIR=.
output=$DIR/rawdataffd.su
migdata=$DIR/datamigffd.su
vfile=$DIR/vfile
susynlv nt=$nt dt=$dt ft=$ft fpeak=$fpeak ls=1 verbose=1 smooth=0\
nxm=$nxm dxm=$dxm ... | Shell |
#! /bin/sh
#
#set -x
nt=300 dt=0.004 ft=0.0 nxm=100 dxm=0.01 fxm=0.0 dxo=0 nxo=1 fxo=0.0
fpeak=20 ls=0 dvdx=0.5 dvdz=0.5 ndpfz=5 v00=2.0
pert=0 ob=1 er=0
DIR=.
output=$DIR/rawdataffd.su
migdata=$DIR/datamigffd.su
migps=$DIR/migffd.ps
vfile=$DIR/vfile
T1=$DIR/ffd1.ps
T2=$DIR/ffd2.ps
susynlv nt=$nt dt=$dt ft=$ft fpe... | Shell |
#! /bin/sh
rm -rf vfile* *.su *.ps
exit
| Shell |
#! /bin/sh
#
set -x
nt=300 dt=0.004 ft=0.0 nxm=150 dxm=0.01 fxm=0.0 dxo=0 nxo=1 fxo=0.0
fpeak=20 ls=0 dvdx=0.2 dvdz=0.5 ndpfz=5 v00=2.0
pert=0 ob=1 er=0
DIR=.
output=$DIR/rawdatafd.su
migdata=$DIR/datamigfd.su
vfile=$DIR/vfile
susynlv nt=$nt dt=$dt ft=$ft fpeak=$fpeak ls=1 verbose=1 smooth=0\
nxm=$nxm dxm=$dxm fx... | Shell |
#! /bin/sh
#
#echo off
#set -x
nt=300 dt=0.004 ft=0.0 nxm=100 dxm=0.01 fxm=0.0 dxo=0 nxo=1 fxo=0.0
fpeak=20 ls=0 dvdx=0.5 dvdz=0.5 ndpfz=5 v00=2.0
pert=0 ob=1 er=0
DIR=.
output=$DIR/rawdatafd.su
migdata=$DIR/datamigfd.su
migps=$DIR/migfd.ps
vfile=$DIR/vfile
T1=$DIR/fd1.ps
T2=$DIR/fd2.ps
susynlv nt=$nt dt=$dt ft=$f... | Shell |
#! /bin/sh
for i in *
do
if [ -d $i ]
then
cd $i
Clean.sh
cd ..
fi
done
| Shell |
#! /bin/sh
demo=decon1
tpow=1 # gain power before examining autocorrelations
# tpow=2 might be better for field data
###PURPOSE###
# We make some simple data: 8 traces with 2-way reverberations and
# a weak tilting reflector hidden underneath the reverberations. The
# spike data is convolved with the minimum phas... | Shell |
#! /bin/sh
#set -x
demo=decon3
deconparams=deconparams3
fold=8
space=3 # 3 null traces between panels
tpow=1 # gain power before examining autocorrelations
# tpow=2 would often be better for field data
###PURPOSE###
# We use the same data described in the first demo. But here
# we illustrate how to set up a serie... | Shell |
#! /bin/sh
# Clean created data files
rm -f modeldata deconpanel *.eps junk* *.ps traces INSTALL
exit
| Shell |
#! /bin/sh
WIDTH=420
HEIGHT=400
WIDTHOFF1=0
WIDTHOFF2=430
WIDTHOFF3=860
HEIGHTOFF1=50
HEIGHTOFF2=500
tpow=1 # gain power before examining autocorrelations
# tpow=2 might be better for field data
mix=1,1,1
###PURPOSE###
# Same as in demo1, except here gapped decon comes before
# spiking decon. Again, you are to as... | Shell |
#! /bin/sh
WIDTH=420
HEIGHT=400
WIDTHOFF1=0
WIDTHOFF2=430
WIDTHOFF3=860
HEIGHTOFF1=50
HEIGHTOFF2=500
tpow=1 # gain power before examining autocorrelations
# tpow=2 might be better for field data
###PURPOSE###
# We make some simple data: 8 traces with 2-way reverberations and
# a weak tilting reflector hidden under... | Shell |
#! /bin/sh
WIDTH=420
HEIGHT=400
HEIGHT2=900
WIDTHOFF1=0
WIDTHOFF2=430
WIDTHOFF3=860
HEIGHTOFF1=50
HEIGHTOFF2=500
###PURPOSE###
# We make some simple data: 8 traces with 2-way reverberations and
# a weak tilting reflector hidden underneath the reverberations. The
# spike data is convolved with the minimum phase wavel... | Shell |
#! /bin/sh
#set -x
demo=decon4
deconparams=deconparams4
fold=8
space=3 # 3 null traces between panels
tpow=1 # gain power before examining autocorrelations
# tpow=2 would often be better for field data
###PURPOSE###
# We use the same data described in the first demo. But here
# we illustrate how to set up a ser... | Shell |
#! /bin/sh
WIDTH=600
HEIGHT=400
WIDTHOFF1=0
WIDTHOFF2=640
HEIGHTOFF1=50
HEIGHTOFF2=530
deconparams=deconparams4
fold=8
space=3 # 3 null traces between panels
tpow=1 # gain power before examining autocorrelations
# tpow=2 would often be better for field data
mix=1,1,1
pnoise=.0005
###PURPOSE###
# We use the same d... | Shell |
#! /bin/sh
demo=decon2
tpow=1 # gain power before examining autocorrelations
# tpow=2 would often be better for field data
###PURPOSE###
# Same as in demo1, except here gapped decon comes before
# spiking decon. Again, you are to assume that the decon
# parameters are estimated from the autocorrelation shown in
#... | Shell |
#! /bin/sh
WIDTH=600
HEIGHT=400
WIDTHOFF1=0
WIDTHOFF2=640
HEIGHTOFF1=50
HEIGHTOFF2=530
deconparams=deconparams3
fold=8
space=3 # 3 null traces between panels
tpow=1 # gain power before examining autocorrelations
# tpow=2 would often be better for field data
mix=1,1,1
pnoise=.0005
###PURPOSE###
# We use the same d... | Shell |
#! /bin/sh
WIDTH=4
HEIGHT=4
HEIGHT2=9
###PURPOSE###
# We make some simple data: 8 traces with 2-way reverberations and
# a weak tilting reflector hidden underneath the reverberations. The
# spike data is convolved with the minimum phase wavelet specified below.
# The purpose of this demo is to create and apply a wa... | Shell |
#! /bin/sh
## use susynlv to make synthetic data
susynlv nt=201 dt=0.004 ft=0.0 nxo=1 \
nxs=100 dxs=.025 fxs=0.0 er=0 ob=0 \
v00=2.0 dvdz=0 dvdx=0 fpeak=30 smooth=1 \
ref="1:-1.,.1;7.,.5" \
ref="1:-1.,.5;7.,.2" \
ref="2:-1.,.5;7.,.9" |
sushw key=d2 a=.05 >susyn1.out
sufilter <susyn1.out >susyn1.flt
suaddnoise < s... | Shell |
#! /bin/sh
WIDTH=320
HEIGHT=400
WIDTHOFF1=0
WIDTHOFF2=400
WIDTHOFF3=800
HEIGHTOFF1=50
HEIGHTOFF2=500
## use susynlv to make synthetic data
susynlv nt=201 dt=0.004 ft=0.0 nxo=1 \
nxs=100 dxs=.025 fxs=0.0 er=0 ob=0 \
v00=2.0 dvdz=0 dvdx=0 fpeak=30 smooth=1 \
ref="1:-1.,.1;7.,.5" \
ref="1:-1.,.5;7.,.2" \
ref="2:-1.... | Shell |
#! /bin/sh
rm *.ps susyn1* core
| Shell |
#! /bin/sh
# clean up files made by NMO demo
# deliberately leave stkvel.p in place in case Xvelocity not run
rm -f junk*
rm -f *.bin
rm -f *.eps *.ps
exit
| Shell |
#! /bin/sh
kaperture both=1 fmin=50 fmax=125 x0=0 y0=1000 nfreq=100 dgx=10 \
ngeo=1000 nstep=0 |
xy2z nx1=200 nx2=200 npairs=200000 > junk1.bin
psimage < junk1.bin n1=200 n2=200 wbox=4 hbox=4 style=normal > junk.ps
| Shell |
#! /bin/sh
kaperture both=1 fmin=50 fmax=125 x0=500 y0=1000 nfreq=100 dsx=10 \
ngeo=1000 nstep=0 |
xgraph title="common shot (500,1000)" n=200000,100 \
mark=1,0 marksize=1,0 linewidth=0,1 style=normal &
kaperture both=1 fmin=50 fmax=125 x0=1000 y0=1000 nfreq=100 dsx=10 \
ngeo=1000 nstep=0 |
xgraph title="common sho... | 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 -x
# Demos shell 2 for supickamp
# Andreas Rueger, Feb 18,1997
#------------------------------------
# Create an su Data set with :
#
# 32 traces in input file
# tracl=32 tracr=32 offset=400 ns=64 dt=4000
#
#------------------------------------
temp=pickdata.bin
#-------- create data set -----... | Shell |
#! /bin/sh
# set -x
# Clean-up shell for supickamp demos
# Andreas Rueger, Feb 18,1997
temp=pickdata.bin
mouse=window.data
rm $temp $mouse pick.info
| Shell |
#! /bin/sh
# set -x
# Demos shell for supickamp
# Andreas Rueger, Feb 18,1997
#------------------------------------
# Create an su Data set with :
#
# 32 traces in input file
# tracl=32 tracr=32 offset=400 ns=64 dt=4000
#
#------------------------------------
temp=pickdata.bin
#-------- create data set -------... | Shell |
#! /bin/sh
# Set messages on
set -x
# Demo for supickamp: "verbose=2"
# Modification of Demo "PickData2"
#------------------------------------
# Create an su Data set with :
#
# 32 traces in input file
# tracl=32 tracr=32 offset=400 ns=64 dt=4000
#
#------------------------------------
temp=pickdata.bin
#-----... | Shell |
#! /bin/sh
# set -x
# Demos shell 3 for supickamp
# Andreas Rueger, Feb 18,1997
#------------------------------------
# Create an su Data set with :
#
# 32 traces in input file
# tracl=32 tracr=32 offset=400 ns=64 dt=4000
#
#------------------------------------
temp=pickdata.bin
mouse=window.data
#-------- cre... | Shell |
#! /bin/sh
for i in *
do
if [ -d $i ]
then
cd $i
Clean.sh
cd ..
fi
done
| Shell |
#! /bin/sh
rm *.su data line
| Shell |
#! /bin/sh
DATA=.
n1=501
n2=24
file=$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
# 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
rm *.su
| Shell |
#! /bin/sh
# make synthetic data with suplane
suplane ntr=60 | sushw key=trid a=1 b=1 s=3 > temp.su
# suxwigb xbox=50 title="Synthetic data" < temp.su &
# make a ricker wavelet with suwaveform
suwaveform type=ricker1 fpeak=20 > ricker.su
# suxwigb xbox=250 title="ricker wavelet" < ricker.su &
# convolve the ricke... | Shell |
#! /bin/sh
sualford \
inS11=S11.su \
inS12=S12.su \
inS21=S21.su \
inS22=S22.su \
outS11=S11out.su \
outS12=S12out.su \
outS21=S21out.su \
outS22=S22out.su \
suxwigb < S11out.su xbox=50 ybox=50 hbox=500 wbox=500 title="S11 out" clip=1 &
suxwigb < S12out.su xbox=550 ybox=50 hbox=500 wbox=500 title="S12 out" c... | Shell |
#! /bin/sh
# Supofilt - Demo shell script for SUPOFILT
# Author: Nils Maercklin, GFZ Potsdam, Germany, 2001
# PostScript flag (set to 1 to generate PS output instead of X display):
POSTSCRIPT=0
# X window sizes and positions:
WIDTH=400
HEIGHT=500
WIDTHOFF1=0
WIDTHOFF2=410
HEIGHTOFF1=50
HEIGHTOFF2=100
HEIGHTOFF3=150
... | Shell |
#! /bin/sh
# MakeData - Generate a three-component dataset for demo scripts
# Supolar, Supofilt, and Sueipofi
# Author: Nils Maercklin, GFZ Potsdam, Germany, 2001
#
# Notes:
# It is not necessary to run this script prior to one of the demo scripts
# named above. It will be called automatically, if it is ... | Shell |
#! /bin/sh
# Sueipofi - Demo shell script for SUEIPOFI
# Author: Nils Maercklin, GFZ Potsdam, Germany, 2001
# PostScript flag (set to 1 to generate PS output instead of X display):
POSTSCRIPT=0
# X window sizes and positions:
WIDTH=400
HEIGHT=500
WIDTHOFF1=0
WIDTHOFF2=410
HEIGHTOFF1=50
HEIGHTOFF2=100
HEIGHTOFF3=150
... | Shell |
#! /bin/sh
# Clean.sh - Clean up after running demos
rm -f temp.su indata.su data3c.su pofi3c.su polar.* rotated.su core
rm -f supolar?.eps supofilt??.eps sueipofi??.eps suhrot.eps
rm -f data.*.eps polar.*.eps data3c.eps pofi3c.eps plot?.eps
rm -f a.asc x.asc x.bin a.bin
exit 0
| Shell |
#! /bin/sh
# Suhrot - Demo shell script for SUHROT
# Author: Nils Maercklin, GFZ Potsdam, Germany, 2001
# PostScript flag (set to 1 to generate PS output instead of X display):
POSTSCRIPT=0
# X window sizes and positions:
WIDTH=400
HEIGHT=600
WIDTHOFF1=0
WIDTHOFF2=410
HEIGHTOFF=50
# Create a three-component file:
... | Shell |
#! /bin/sh
# Supolar - Demo shell script for SUPOLAR
# Author: Nils Maercklin, GFZ Potsdam, Germany, 2001
# PostScript flag (set to 1 to generate PS output instead of X display):
POSTSCRIPT=0
# X window sizes and positions:
WIDTH=200
HEIGHT=300
WIDTHOFF1=0
WIDTHOFF2=200
WIDTHOFF3=400
WIDTHOFF4=600
HEIGHTOFF1=0
HEIGH... | Shell |
#! /bin/sh
# SU must be installed with the XDR flag set
inputdata=3stomp_test.segd
outfile=temp.su
segdread tape=$inputdata verbose=1 ptmax=2 buff=0 aux=1 use_stdio=1 |
suoldtonew > $outfile
surange < $outfile
# Sercel test
# note, there appear to be NANs on the output, but the result of
# filtering through "sunan... | Shell |
#! /bin/sh
# Clean created data files
rm -f *.su
exit
| Shell |
#! /bin/sh
for i in *
do
if [ -d $i ]
then
cd $i
Clean.sh
cd ..
fi
done
| Shell |
#! /bin/sh
# Clean created data files
rm -f *.su
exit
| Shell |
#! /bin/sh
suplane > junk.su
segyhdrs < junk.su
segywrite tape=junk.sgy verbose=1 < junk.su
segyread tape=junk.sgy bfile=junk1.bin hfile=junk1.h verbose=1 | segyclean > junk1.su
exit 0
| Shell |
#! /bin/sh
cd ./Sucommand ; Clean.sh
| Shell |
#! /bin/sh
# make data for NMO demo, goes into file: modeldata
# Note that since dsx=dgx, full fold is at most 32 (NOT 64),
# but in this quick demo we have only 12 shots, so fold is at most 12
######Work in kft instead of km (synlv puts 10^3 in header fields)######
# ref="1:1,2;4,2" reflector(s): "amplitude:x... | Shell |
#! /bin/sh
# clean up files made by NMO demo
# deliberately leave stkvel.p in place in case Xvelocity not run
rm -f modeldata junk*
exit
| Shell |
#! /bin/sh
echo "running sugain < modeldata scale=10 > junk.su"
echo
echo
time sugain < modeldata scale=10 > /dev/null
echo
echo
echo "Compare the above times with the same program run with"
echo "sucommand, with pipes initiated by change in fldr header field"
echo
echo
time sucommand < modeldata key=fldr... | Shell |
#! /bin/sh
# Zero offset sections
# Flat model and data
nx=101 fx=0 dx=0.05
nz=101 fz=0 dz=0.04
unif2 <model00deg ninf=2 nx=$nx nz=$nz dx=$dx dz=$dz \
v00=1.0,1.0 method=linear |
psimage perc=99 title="Flat Model"\
label1="Depth (km)" label2="Distance (km)" \
n1=$nz f1=$fz d1=$dz n2=$nx f2=$fx d2=$dx >zmodel00.e... | Shell |
#! /bin/sh
# Zero offset sections
WIDTH=300
HEIGHT=400
XOFF1=0
XOFF2=315
XOFF3=630
XOFF4=945
YOFF1=50
YOFF2=500
# Flat model and data
nx=101 fx=0 dx=0.05
nz=101 fz=0 dz=0.04
unif2 <model00deg ninf=2 nx=$nx nz=$nz dx=$dx dz=$dz \
v00=1.0,1.0 method=linear |
ximage perc=99 title="Flat Model" windowtitle="Flat Model"\... | Shell |
#! /bin/sh
# Clean created data files
rm -f *.eps
exit
| Shell |
#! /bin/sh
# Make some zero offset data to examine plot defaults in slow direction
WIDTH=540
HEIGHT=800
XOFF1=0
XOFF2=535
XOFF3=1070
YOFF=150
WIDTH=420
HEIGHT=700
XOFF1=0
XOFF2=430
XOFF3=860
YOFF=150
###########################################################################
# Here set fxm = dxm (not equal 0), then su... | Shell |
#! /bin/sh
# Non-zero offset sections
WIDTH=300
HEIGHT=400
XOFF1=0
XOFF2=315
XOFF3=630
XOFF4=945
YOFF1=50
YOFF2=500
# Flat model and data
nx=101 fx=0 dx=0.05
nz=101 fz=0 dz=0.04
unif2 <model00deg ninf=2 nx=$nx nz=$nz dx=$dx dz=$dz \
v00=1.0,1.0 method=linear |
ximage perc=99 title="Flat Model" windowtitle="Flat Mod... | Shell |
#! /bin/sh
# Non-zero offset sections
# Flat model and data
nx=101 fx=0 dx=0.05
nz=101 fz=0 dz=0.04
unif2 <model00deg ninf=2 nx=$nx nz=$nz dx=$dx dz=$dz \
v00=1.0,1.0 method=linear |
psimage perc=99 title="Flat Model"\
label1="Depth (km)" label2="Distance (km)" \
n1=$nz f1=$fz d1=$dz n2=$nx f2=$fx d2=$dx >model0... | Shell |
#! /bin/sh
# Make some zero offset data to examine headers
######Work in km (synlv puts 10^3 in header fields)######
# ref="1:1,2;4,2" reflector(s): "amplitude:x1,z1;x2,z2;x3,z3;..."
REF="1.0:0.0,1.0;5.0,1.0"
nt=750 ft=0.0 dt=0.008 # time information: number, first, spacing
nxm=100 fxm=0.05 dxm=0.05 # mid... | Shell |
#! /bin/sh
# Make some zero offset data to examine plot defaults in slow direction
###########################################################################
# Here set fxm = dxm (not equal 0), then susynlv takes care of the x-plot
# settings.
REF="1.0:0.0,1.0;5.0,1.0"
nt=751 ft=0.0 dt=0.008 # time information: ... | Shell |
#! /bin/sh
# Make some shot data to check headers
######Work in km (synlv puts 10^3 in header fields)######
# ref="1:1,2;4,2" reflector(s): "amplitude:x1,z1;x2,z2;x3,z3;..."
REF="1.0:0.0,1.0;5.0,1.0"
n1=750 ft=0.0 dt=0.008 # time information: number, first, spacing
nxs=2 fxs=0.025 dxs=0.025 # shot informa... | Shell |
#! /bin/sh
# Clean created data files
rm -f *.eps
exit
| Shell |
#! /bin/sh
# Examples of producing single shot records with susynlv
# Flat model and data
nx=101 fx=0 dx=0.05
nz=101 fz=0 dz=0.04
unif2 <model00deg ninf=2 nx=$nx nz=$nz dx=$dx dz=$dz \
v00=1.0,1.0 method=linear |
psimage perc=99 title="Flat Model"\
label1="Depth (km)" label2="Distance (km)" \
n1=$nz f1=$fz d1=$dz... | Shell |
#! /bin/sh
# Examples of producing single shot records with susynlv
WIDTH=300
HEIGHT=400
XOFF1=0
XOFF2=315
XOFF3=630
XOFF4=945
YOFF1=50
YOFF2=500
# Flat model and data
nx=101 fx=0 dx=0.05
nz=101 fz=0 dz=0.04
unif2 <model00deg ninf=2 nx=$nx nz=$nz dx=$dx dz=$dz \
v00=1.0,1.0 method=linear |
ximage perc=99 title="Fla... | Shell |
#! /bin/sh
# Make some shot data to examine plot defaults in slow direction
WIDTH=540
HEIGHT=800
XOFF1=0
XOFF2=535
XOFF3=1070
YOFF=150
###########################################################################
# Here set fxo = dxo (not equal 0), then susynlv takes care of the x-plot
# settings.
REF="1.0:0.0,1.0;5.0... | Shell |
#! /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.
WIDTH1=300
... | Shell |
#! /bin/sh
# Make some shot data to examine plot defaults in slow direction
###########################################################################
# Here set fxo = dxo (not equal 0), then susynlv takes care of the x-plot
# settings.
REF="1.0:0.0,1.0;5.0,1.0"
nt=751 ft=0.0 dt=0.008 # time information: number,... | Shell |
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