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#! /bin/sh # Clean.sh created data files rm -f *.bin *.su exit
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#! /bin/sh # PSdemo1 - simple example script for sufdmod1, PostScript graphics # N. Maercklin, Oct. 2006 # Output file names (velocity,density and seismogram): vfile=velocity.bin dfile=density.bin sufile=seismogram.su # Output PostScript file (three plots on one page): psfile=demo.ps # Velocity and density model: de...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling: part 1, the movie # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=10 WIDTHOFF2=500 HEIGHTOFF1=50 HEIGHTOFF2=530 n1=100 d1=5 f1=0.0 label1="Depth (km)" n2=100 d2=5 f2=0.0 label2="Distance (km)" xs=250 zs=300 hsz=50 vsx=250 verbo...
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#! /bin/sh # Clean.sh created data files rm -f *.out junk* *.eps *.ps density* velocity* *.pdf *.su exit
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling: part 1, the movie # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=50 WIDTHOFF2=530 HEIGHTOFF1=50 HEIGHTOFF2=530 n1=500 d1=5 f1=0.0 label1="Depth (km)" n2=500 d2=5 f2=0.0 label2="Distance (km)" xs=1250 zs=1250 hsz=1000 vsx=1000 ...
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#! /bin/sh # building a model with "unif2" hsfile=hsseis.out # build the file of velocities unif2 < model.unif2 nx=100 nz=500 dx=25 \ v00=5000,5500,6000,6500,7000,7500,8000 dz=10 > velocity.1 # build the file of densities unif2 < model.unif2 nx=100 nz=500 dx=25 \ v00=1.0,2.25,2.25,2.25,2.35,2.35,2.35 dz=10 > densi...
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#! /bin/sh # PSDemo --- example script for sufdmod2 # finite-difference modeling: display model and movie # Author: John Stockwell # Modified from various XDemos by Chris Liner 2/12/02 # Big changes... # 1. deleted (n1,n2) params to unif2 (unused) # note on use of (dx,dz) in unif2 hardwired model # added 2x2 s...
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#! /bin/sh # PSDemo3 --- example script for sufdmod2 # finite-difference modeling: display model and movie # Author: John Stockwell # modified from XDemo3 by Chris Liner 2/11/02 # (also added 2x2 smoothing to velocity model, # and uses ps2pdf to generate pdf output) n1=100 d1=5 f1=0.0 label1="Depth (km)" n2=100 d2=5 ...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling: Test of the PML transparent boundary conditions # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=50 WIDTHOFF2=530 HEIGHTOFF1=50 HEIGHTOFF2=530 n1=200 d1=5 f1=0.0 label1="Depth (km)" n2=200 d2=5 f2=0.0 label2="Distance (km)" xs=...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling: part 1, the movie # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=50 WIDTHOFF2=530 HEIGHTOFF1=50 HEIGHTOFF2=530 n1=500 d1=5 f1=0.0 label1="Depth (km)" n2=500 d2=5 f2=0.0 label2="Distance (km)" xs=1250 zs=125 hsz=300 vsx=1000 ve...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling: part 1, the movie # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=10 WIDTHOFF2=500 HEIGHTOFF1=50 HEIGHTOFF2=530 n1=100 d1=5 f1=0.0 label1="Depth (km)" n2=100 d2=5 f2=0.0 label2="Distance (km)" xs=250 zs=50 hsz=50 vsx=250 verbos...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling: part 1, the movie # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=10 WIDTHOFF2=500 HEIGHTOFF1=50 HEIGHTOFF2=530 n1=100 d1=5 f1=0.0 label1="Depth (km)" n2=100 d2=5 f2=0.0 label2="Distance (km)" xs=250 zs=300 hsz=50 vsx=250 verbo...
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#! /bin/sh # build velocity profiles with unif2 modelfile=syncline.unif2 velfile=syncline.bin n1=200 n2=400 d1=10 d2=10 unif2 <$modelfile method=$i ninf=2 nx=$n2 nz=$n1 v00=2000,4000 \ ninf=1 method=spline > $velfile ximage < $velfile wbox=400 hbox=200 n1=$n1 n2=$n2 d1=$d1 d2=$d2 \ wbox=800 hbox=400 legend=1 tit...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling # Author: John Stockwell n1=100 d1=5 f1=0.0 label1="Depth (km)" n2=100 d2=5 f2=0.0 label2="Distance (km)" xs=250 zs=250 hsz=250 vsx=250 verbose=2 vsfile="vseis.out" ssfile="sseis.out" hsfile="hseis.out" tmax=.5 mt=5 makevel nx=$n2 nz=$...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling, part 2 the output files # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=20 WIDTHOFF2=510 WIDTHOFF3=930 HEIGHTOFF1=50 HEIGHTOFF2=530 clip=.5 suwind <vseis.out j=3 | suxwigb clip=$clip \ title="Vertical line of seismograms" \ ...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling, part 2 the output files # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=50 WIDTHOFF2=530 HEIGHTOFF1=50 HEIGHTOFF2=530 suximage <vseis.out clip=1.0 \ title="Vertical line of seismograms" \ windowtitle="Vertical" \ label1="Tim...
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#! /bin/sh # building a model with "unif2" hsfile=hsseis.out # Use the Marmousi model zcat $CWPROOT/src/demos/Velocity_Profiles/Marmousi/marmhard.dat.gz | a2b n1=1 | unisam2 nx2=384 dx2=2 fx2=0 n2=768 d2=1 f2=0 nx1=122 dx1=4 fx1=0 n1=488 d1=1 f1=0 method=linear > velocity.1 # build the file of densities unif2 < mode...
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#! /bin/sh # building a model with "unif2" hsfile=hsseis.out # build the file of velocities unif2 < model.unif2 nx=100 nz=500 dx=25 \ v00=5000,5500,6000,6500,7000,7500,8000 dz=10 > velocity.1 # build the file of densities unif2 < model.unif2 nx=100 nz=500 dx=25 \ v00=1.0,2.25,2.25,2.25,2.35,2.35,2.35 dz=10 > densi...
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#! /bin/sh rm *susyn*
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#! /bin/sh ## use susynlv to make synthetic data susynlv nt=501 dt=0.004 ft=0.0 nxo=2 \ nxs=100 dxs=.025 dxo=.15 fxo=0.025 er=0 ob=0 \ v00=2.0 dvdz=0 dvdx=0 fpeak=30 smooth=1 \ ref="2:-.5,.45;3.,.45" \ ref="2:-.5,.75;3.,.75" \ ref="4:-.5,1.15;3.,1.15" \ ref="6:-.5,1.65;3.,1.65" \ sushw key=d2 a=.05 >susyn.out # ...
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#! /bin/sh WIDTH=320 HEIGHT=400 WIDTHOFF1=0 WIDTHOFF2=400 HEIGHTOFF1=50 HEIGHTOFF2=500 ## use susynlv to make synthetic data susynlv nt=501 dt=0.004 ft=0.0 nxo=2 \ nxs=100 dxs=.025 dxo=.15 fxo=0.025 er=0 ob=0 \ v00=2.0 dvdz=0 dvdx=0 fpeak=30 smooth=1 \ ref="2:-5.5,.45;7.,.45" \ ref="2:-5.5,.75;7.,.75" \ ref="4:-...
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#! /bin/sh # Clean - recursively call Clean in the demo directories # Test back-up dir first (at CWP must run on dobrin) DEMODIR=$CWPROOT/src/demos find . -name core -print -exec rm -f {} \; find . -name \.nfs\* -print -exec rm -f {} \; # Take care of subdirectories for i in `ls` do if [ -d $i ] then cd $i ...
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#! /bin/sh # Clean - recursively call Clean in the demo directories # Test back-up dir first (at CWP must run on dobrin) DEMODIR=$CWPROOT/src/demos/Velocity_Analysis find . -name core -print -exec rm -f {} \; find . -name \.nfs\* -print -exec rm -f {} \; # Take care of subdirectories for i in `ls` do if [ -d $i ...
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#! /bin/sh # LAS file location and name las=./las/well_logs.las # curve order in las file (p-sonic, s-sonic, density) pson=2 sson=3 den=4 # bacus averaging window length (in depth samples) # (note depth is in meters after las2su) navg=201 # output window geometry WIDTH=300 HEIGHT=400 WIDTHOFF1=0 WIDTHOFF2=315 WIDT...
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#! /bin/sh rm *.su
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#! /bin/sh rm *.asc *.su
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#! /bin/sh # run las2su on file in LAS format. las2su < test.las > las.su suxwigb < las.su title="well log in SU format" clip=100 & exit 0
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#! /bin/sh sustrip < data3d.su > data3d.bin # slices on top and back sides of cube # push right hand mouse button to see menu, select planes to view trip < data3d.bin verbose=1 n1=256 n2=32 n3=32 tbs=.2 \ cx=0 cy=0 cz=0 & exit 0
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#! /bin/sh rm -f data3d.* temp exit
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#! /bin/sh sustrip < data3d.su > data3d.bin # slices on bottom and back sides of cube # push right hand mouse button to see menu, select planes to view trip < data3d.bin verbose=1 n1=256 n2=32 n3=32 tbs=.2 \ cx=0 cy=0 cz=255 & exit 0
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#! /bin/sh sustrip < data3d.su > data3d.bin # slices centered through cube # push right hand mouse button to see menu, select planes to view trip < data3d.bin verbose=1 n1=256 n2=32 n3=32 tbs=.5 \ cx=16 cy=16 cz=128 & exit 0
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#! /bin/sh To run the 3D data viewing demo type names of the following shell scripts on the commandline. Make3Ddata --- generate 3D data file: data3d.su Trip1 --- planes pass through the center of data cube Trip2 --- planes on top and back sides of data cube Trip3 --- planes on bottom and back sides of...
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#! /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...
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#! /bin/sh sustrip < data3d.su > data3d.bin # slices on bottom and front sides of cube # push right hand mouse button to see menu, select planes to view trip < data3d.bin verbose=1 n1=256 n2=32 n3=32 tbs=.2 \ cx=31 cy=31 cz=255 & exit 0
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#! /bin/sh rm -f *.su temp *.bin exit
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#! /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...
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#! /bin/sh # Clean created data files rm -f vibrodata.* recon.* *.eps exit 0
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#! /bin/sh cd Demo* ; Clean
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#! /bin/sh rm *.dat reflection* junk* *.eps createf INSTALL *.2p *.ps
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#! /bin/sh p2=6 p1=6 size=64 infile=ffile.dat reconfile=recon.dat mrafile=mra.dat dfile=d.dat createf > $infile mrafxzwt verbose=1 order=4 p2=$p2 p1=$p1 \ mralevel2=3 mralevel1=3 \ reconfile=$reconfile n1=$size n2=$size\ dfile=$dfile recon=0 \ <$infile >$mrafile psimage n1=$size n2=$size title="Original Mod...
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#! /bin/sh p2=6 p1=6 size=64 infile=xy.dat unisam verbose=1 nout=$size xin=0,12,51,63 yin=0,0,0,0 \ nsint=1 amp=-0.3 isint=1 nwidth=4> x.dat farith verbose=1 in=x.dat n=$size op=cartprod in2=x.dat \ > $infile reconfile=recon.dat mrafile=mra.dat dfile=d.dat mrafxzwt verbose=1 order=4 p2=$p2 p1=$p1 \ n1=$s...
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#! /bin/sh S=. #the directory where your data is p1=9 p2=8 nc1=256 nc2=128 n1=750 n2=369 nt1=512 nt2=256 data=$S/model.su trimfile=$S/trimfile.2p infile=$S/model.2p mrafile=$S/mramodel.2p dfile=$S/dmodel.2p dmrafile=$S/dmramodel.2p reconfile=$S/reconmodel.2p reconmrafile=$S/reconmramodel.2p mraps=$S/mraMarmousi.ps di...
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#! /bin/sh WIDTH=420 HEIGHT=300 XOFF1=0 XOFF2=425 YOFF1=2 YOFF2=450 MARM=$CWPROOT/src/demos/Velocity_Profiles/Marmousi S=. zcat $MARM/marmhard.dat.gz | a2b n1=1 | unisam2 nx2=384 dx2=2.6667 fx2=0 n2=1024 d2=1 f2=0 nx1=122 \ dx1=4.1967 fx1=0 n1=512 d1=1 f1=0 method=linear | suaddhead ns=512 > model.su p1=9 p2=10 #n...
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#! /bin/sh WIDTH=300 HEIGHT=420 WIDTHOFF1=0 WIDTHOFF2=305 HEIGHTOFF1=2 HEIGHTOFF2=450 p2=6 p1=6 size=64 infile=ffile.dat reconfile=recon.dat mrafile=mra.dat dfile=d.dat make ./createf > $infile mrafxzwt verbose=1 order=4 p2=$p2 p1=$p1 \ mralevel2=3 mralevel1=3 reconfile=$reconfile \ dfile=$dfile recon=0 n1=$siz...
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#! /bin/sh WIDTH=300 HEIGHT=420 WIDTHOFF1=0 WIDTHOFF2=305 HEIGHTOFF1=2 HEIGHTOFF2=450 p2=6 p1=6 size=64 infile=xy.grid unisam verbose=1 nout=$size xin=0,12,51,63 yin=0,0,0,0 \ nsint=1 amp=-0.3 isint=1 nwidth=4> x.grid farith verbose=1 in=x.grid n=$size op=cartprod in2=x.grid \ > $infile reconfile=recon.da...
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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 $i if [ -f Clean.sh ] then Clean.sh fi rm -f *~ \#*\# .nfs* *.eps cd .. fi done # Take care of t...
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#! /bin/sh # shell for uniformly sampling velocity from a layered model set -v nz=51 dz=50 fz=0.0 labelz="Depth (m)" nx=201 dx=50 fx=0 labelx="Distance (m)" ninf=0 npmax=201 unif2 <input_datum >vfile_datum method=mono ninf=$ninf npmax=$npmax \ nz=$nz dz=$dz fz=$fz nx=$nx dx=$dx fx=$fx \ v00=2000\ dvdz=0 exit 0
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#! /bin/sh origdata=model.data data=shot_TOPO.data shot=4000 rec1=`expr $shot - 2000` rec2=`expr $shot + 2000` suwind<$data key=sx min=$shot max=$shot | suwind key=gx min=$rec1 max=$rec2 | suwind tmin=0 tmax=3.0 | suximage legend=1 f2=-2.0 d2=0.025 label1="Time (s)" label2="Offset (km)" \ title="Shot $shot with to...
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#! /bin/sh # shell for generating traveltimes by ray tracing set -v rayt2d <vfile_datum par=rayup.par exit
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#! /bin/sh rm *.eps data* *.data jpfile* tfile* vfile*
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#! /bin/sh data=shot_TOPO.data shot=4000 rec1=`expr $shot - 2000` rec2=`expr $shot + 2000` suwind<$data key=sx min=$shot max=$shot | suwind key=gx min=$rec1 max=$rec2 | suwind tmin=0 tmax=3.0 | supswigb f2=-2.0 d2=0.025 label1="Time (s)" label2="Offset (km)" \ title="Shot $1 from topography" perc=99.2 > data.eps ...
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#! /bin/sh # #set -x output=model.data nt=501 dt=0.008 ft=0.0 tmin=0.2 nxs=181 dxs=0.025 fxs=2.75 nxo=181 \ fxo=-2.25 dxo=0.025 fpeak=15 ls=1 dvdx=0.2 dvdz=0.6 \ x0=0.0 z0=0 v00=2 susynlv dt=$dt ft=$ft nxs=$nxs dxs=$dxs fxs=$fxs nxo=$nxo dxo=$dxo \ fxo=$fxo tmin=$tmin dvdx=$dvdx dvdz=$dvdz \ fpeak=$fpeak ls=$ls nt=$...
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#! /bin/sh # shell for Kirchhoff Wave Equation Datuming for pre-stack data #set -v data=model.data echo "This script will take a few minutes on a 2 ghz workstation." sudatumk2dr<$data par=kzup.par \ jpfile=jpfile.rec>kzshot.data susort<kzshot.data>receiv.data gx sx sudatumk2ds<receiv.data par=kzup.par \ jpfile=jpfi...
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#! /bin/sh # shell for uniformly sampling velocity from a layered model set -v nz=51 dz=50 fz=0.0 labelz="Depth (m)" nx=201 dx=50 fx=0 labelx="Distance (m)" ninf=0 npmax=500 unif2 <input_datum >vfile_datum method=mono ninf=$ninf npmax=$npmax \ nz=$nz dz=$dz fz=$fz nx=$nx dx=$dx fx=$fx \ v00=2000 \ dvdz=0 exit 0 ...
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#! /bin/sh flatdata=../Make_Data/model.data topodata=../Make_Data/shot_TOPO.data datumeddata=shot_DATUM.data shot=4000 rec1=`expr $shot - 2000` rec2=`expr $shot + 2000` # plot flat data suwind<$flatdata key=sx min=$shot max=$shot | suwind key=gx min=$rec1 max=$rec2 | suwind tmin=0 tmax=3.0 | suximage legend=1 f2=-2...
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#! /bin/sh rm *.eps data* *.data jpfile* tfile* vfile*
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#! /bin/sh data=shot_TOPO.data shot=4000 rec1=`expr $shot - 2000` rec2=`expr $shot + 2000` suwind<$data key=sx min=$shot max=$shot | suwind key=gx min=$rec1 max=$rec2 | suwind tmin=0 tmax=3.0 | supswigb f2=-2.0 d2=0.025 label1="Time (s)" label2="Offset (km)" \ title="Shot $1 from topography" perc=99.2 > data.eps ...
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#! /bin/sh # #set -x output=model.data nt=501 dt=0.008 ft=0.0 tmin=0.2 nxs=181 dxs=0.025 fxs=2.75 nxo=181 \ fxo=-2.25 dxo=0.025 fpeak=15 ls=1 dvdx=0.2 dvdz=0.6 \ x0=0.0 z0=0 v00=2 susynlv dt=$dt ft=$ft nxs=$nxs dxs=$dxs fxs=$fxs nxo=$nxo dxo=$dxo \ fxo=$fxo tmin=$tmin dvdx=$dvdx dvdz=$dvdz \ fpeak=$fpeak ls=$ls nt=$...
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#! /bin/sh # shell for generating traveltimes by ray tracing set -v rayt2d <vfile_datum par=ray_down.par exit
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#! /bin/sh # shell for Kirchhoff Wave Equation Datuming for pre-stack data #set -v data=../Make_Data/shot_TOPO.data echo "This script will take a few minutes on a 2 ghz workstation." sudatumk2dr<$data par=kz_down.par \ jpfile=jpfile.rec>kzshot.data susort<kzshot.data>receiv.data gx sx sudatumk2ds<receiv.data par=kz_...
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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 $i if [ -f Clean.sh ] then Clean.sh fi rm -f *~ \#*\# .nfs* *.eps cd .. fi done # Take care of t...
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#! /bin/sh # #------------Geometry Assignment & Sort----------------------------------- # input=mig_950.data suwind<$input key=offset min=950 max=950 | suwind tmax=4.0 |suwind key=tracr min=101 max=301 | suximage legend=1 label1="Depth (km)" label2="Midpoint (km)" d1=0.005 \ f2=2.5 d2=0.025 perc=99. \ title="Common-...
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#! /bin/sh # shell for smoothing a uniformly sampling velocity set -v n1=61 r1=150 dz=50 fz=-500 labelz="Depth (m)" n2=201 r2=150 dx=50 fx=0 labelx="Midpoint (m)" d1r=50 n1r=61 n2r=201 d2r=50 # smooth velocity and resample smooth3d<vfile_mig r1=$r1 r2=$r2 d1=$dz d2=$dx n1=$n1 n2=$n2 n3=1 \ verbose=1 iter=2 slowness...
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#! /bin/sh rm *.eps data* tfile* vfile* *.data jpfile*
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#! /bin/sh # #------------Geometry Assignment & Sort----------------------------------- # input=mig_950.data suwind<$input key=offset min=950 max=950 | suwind tmax=4.0 |suwind key=tracr min=101 max=301 | supsimage legend=1 label1="Depth (km)" label2="Midpoint (km)" d1=0.005 \ f2=2.5 d2=0.025 perc=99. \ title="Common...
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#! /bin/sh # shell for Kirchhoff migration from topography. #set -v set -x offset=950 input=../Make_Data/shot_TOPO.data output=mig_$offset.data suwind <$input key=offset min=$offset max=$offset > input.tmp sumigtopo2d par=kzmigtopo.par infile=input.tmp \ off0=$offset outfile=$output ...
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#! /bin/sh # shell for generating traveltimes by ray tracing set -v rayt2d <vfile_smooth par=rayvxz.par exit
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#! /bin/sh # shell for uniformly sampling velocity from a layered model set -v nz=61 dz=50 fz=-500.0 labelz="Depth (m)" nx=201 dx=50 fx=0 labelx="Distance (m)" ninf=1 npmax=2001 unif2 <input_mig >vfile_mig method=mono ninf=$ninf npmax=$npmax \ nz=$nz dz=$dz fz=$fz nx=$nx dx=$dx fx=$fx \ v00=2000,2000 \ x0=0.,0. ...
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#! /bin/sh # #------------Geometry Assignment & Sort----------------------------------- # input=mig_950.data suwind<$input key=offset min=950 max=950 | suwind tmax=4.0 |suwind key=tracr min=101 max=301 | supswigb label1="Depth (km)" label2="Midpoint (km)" d1=0.005 \ f2=2.5 d2=0.025 wbox=7 hbox=5 perc=99. \ title="Co...
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#! /bin/sh # clean the directory rm -f demo.su demo.su.ps demo*traces demo*plot demo*shot exit 0
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#! /bin/sh # Run CSHOT with CWP X Graphics # Zero-offset data corresponding to a model # with topography, base of weathering and # a reflector at depth demo=14 x1beg=-1000 x1end=4000 x2beg=0 x2end=18000 cp param1.1 param1 cshot1 | cshotplot >demo${demo}plot outpar=demo${demo}par xgraph <demo${demo}plot par=demo${d...
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#! /bin/sh # Run CSHOT with CWP X Graphics # Zero-offset data corresponding to a model # with topography, base of weathering and # a reflector at depth demo=14 x1beg=-1000 x1end=4000 x2beg=0 x2end=18000 cp param1.1 param1 cshot1 | cshotplot >demo${demo}plot outpar=demo${demo}par xgraph <demo${demo}plot par=demo${d...
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#! /bin/sh # clean the directory rm -f *.b rm -f demo.su* rm -f model.ps rm -f demo* cd MakeData ; Clean.sh cd .. cd VelocityFiles ; Clean.sh exit 0
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#! /bin/sh # use zero-velocity layer and wave-equation datuming # to datum data from topography to a horizontal surface #static shift data from topography to a horizontal surface above ################################################################### sustatic < demo.su > demo.su_zstat hdrs=2 sign=-1 sou_file=zsou.b ...
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#! /bin/sh # Display data before and after processing supsimage < demo.su f2=50 d2=50 label1="Time (s)" \ label2="Surface Location (ft)" title="Raw Data" > demo.su.ps supsimage < demo.su_zstat_dat f2=50 d2=50 label1="Time (s)" \ label2="Surface Location (ft)" \ title="After Wave-Equation Datuming" > demo.su_zstat_dat...
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#! /bin/sh # Display data before and after processing suximage < demo.su f2=50 d2=50 label1="Time (s)" \ xbox=20 ybox=20 wbox=400 hbox=300 \ label2="Surface Location (ft)" title="Raw Data" & suximage < demo.su_zstat_dat f2=50 d2=50 label1="Time (s)" \ xbox=450 ybox=20 wbox=400 hbox=300 \ label2="Surface Location (ft)...
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#! /bin/sh # 1) Zero-velocity layer statics are computed # 2) Thin-lens and diffraction term velocity # fields are created make modelstat a2b < zsou.dat n1=1 > zsou.b a2b < zrec.dat n1=1 > zrec.b a2b < vfp1.dat n1=1 > vfp1.b a2b < vfp2.dat n1=1 > vfp2.b cp *.b ../ rm -f *.dat exit 0
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#! /bin/sh # clean the directory make clean rm -f *.b exit 0
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#! /bin/sh # Set messages on set -x # Demo for suascii #------------------------------------------------- # Create a data set with suplane: # 32 traces # tracl=1-32 tracr=1-32 offset=400 ns=64 dt=4000 # The three dipping events cross on tracl=16 # Name temp data set temp=tempdata.bin #-----------------------...
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#! /bin/sh # Clean created data files rm -f binary_cdp temp* output* exit 0
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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) DEMODIR=$CWPROOT/src/demos/Filtering # Take care of subdirectories for i in `ls` do if [ -d $i ] then cd $i if [ -f Clean.sh ] then echo $i Clean.sh fi rm -f *~ \#*\...
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#! /bin/sh # Clean created data files rm -f binary_cdp temp* exit 0
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#! /bin/sh # Set messages on set -x # Demo for sudumptrace #------------------------------------------------- # Create a data set with suplane: # 32 traces # tracl=1-32 tracr=1-32 offset=400 ns=64 dt=4000 # The three dipping events cross on tracl=16 # Name temp data set temp=tempdata.bin #-------------------...
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#! /bin/sh # Clean created data files rm -f binary_cdp temp* exit 0
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#! /bin/sh # Set messages on ##set -x # Demo for sukeycount #------------------------------------------------- # Create a data set with suplane: # 32 traces # tracl=1-32 tracr=1-32 offset=400 ns=64 dt=4000 # The three dipping events cross on tracl=16 # Name temp data set 1 temp1=temp1.bin # Name temp data se...
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#! /bin/sh # Set messages on ##set -x # Demo for sukeycount #------------------------------------------------- # Create a data set with suplane: # 32 traces # tracl=1-32 tracr=1-32 offset=400 ns=64 dt=4000 # The three dipping events cross on tracl=16 # Name temp data set 1 temp1=temp1.bin # Name temp data se...
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#! /bin/sh # Clean created data files rm -f binary_cdp temp* exit 0
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#! /bin/sh # Making su data for big Endian machines if [ ! -f oz25.F -o ! -f oz25.H ] then echo "See the README file for accessing the required data" 1>&2; exit 1 fi # Add header and set fields # Set header fields for future processing convenience. # Notes: # n1 in graphics programs corresponds to SEG-Y field ns # ...
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#! /bin/sh # Clean created data files rm -f data.su *.eps oz* exit
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#! /bin/sh # Investigate data with sugabor to ascertain a time-varying filter # for sutvband WIDTH=600 HEIGHT=450 WIDTHOFF1=0 WIDTHOFF2=640 HEIGHTOFF1=50 HEIGHTOFF2=530 # Spectrum of raw data suspecfx <data.su | suxmovie \ title="FX spectrum" \ windowtitle="FX"\ label1="Freq (Hz)" label2="Offset (km)" \ -geometry...
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#! /bin/sh # Investigate data with sugabor to ascertain a time-varying filter # for sutvband # Takes too long to be practical demo=gabor # Spectrum of raw data suspecfx <data.su | supsimage \ title="FX spectrum"\ label1="Freq (Hz)" label2="Offset (km)" >${demo}.1.eps perc=90 suspecfx <data.su | supsimage perc=$pe...
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#! /bin/sh # Making su data for little Endian machines if [ ! -f oz25.F -o ! -f oz25.H ] then echo "See the README file for accessing the required data" 1>&2; exit 1 fi # Since we are on a "Little Endian" machine (PC), we must swap bytes # Add header and set header fields for future processing convenience. # Remar...
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#! /bin/sh # Best results starting with suspecfx and using some indicated sufilters demo=filt2 perc=90 # accept value in book tpow=3.2 # accept value in oz25.H f=0,10,15,20 amps=0.,0.,1.,1. sufilter <data.su f=$f amps=$amps | sugain tpow=$tpow | supsimage perc=$perc \ title="f=$f + gain"\ label1="Time (sec)" la...
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#! /bin/sh # Try some display gains on the muted, filtered data WIDTH=600 HEIGHT=450 WIDTHOFF1=0 WIDTHOFF2=640 HEIGHTOFF1=50 HEIGHTOFF2=530 perc=90 f=0,15,25,30 amps=0.,0.,1.,1. xmute=1,49,97 tmute=1.2,.2,1.2 ntaper=5 tpow=1 sufilter <data.su f=$f amps=$amps | sumute key=tracl xmute=$xmute tmute=$tmute ntaper=$ntap...
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#! /bin/sh # Use sumute to eliminate direct arrivals on the filtered data WIDTH=600 HEIGHT=450 WIDTHOFF1=0 WIDTHOFF2=640 HEIGHTOFF1=50 HEIGHTOFF2=530 perc=90 tpow=2 f=0,15,25,30 amps=0.,0.,1.,1. sufilter <data.su f=$f amps=$amps | sugain tpow=$tpow | suxmovie perc=$perc \ title="f=$f + gain" windowtitle="f=$f" \ ...
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#! /bin/sh # Making su data for big Endian machines if [ ! -f oz25.F -o ! -f oz25.H ] then echo "See the README file for accessing the required data" 1>&2; exit 1 fi # Add header and set header fields for future processing convenience. # Notes: # n1 in graphics programs corresponds to SEG-Y field ns # d1 in graphic...
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#! /bin/sh # Clean created data files rm -f data*.su *.eps oz* exit
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#! /bin/sh demo=look # Look at raw data using par file to supply all parameters # This would work even we did not use sushw in MakeDataBig/Little supsimage<data.su par=oz25.H >${demo}.1.eps # Repeat using SU headers and adding the suggested tpow in oz25.H tpow=3.191650 sugain <data.su tpow=$tpow | supsimage \ title=...
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#! /bin/sh # Try some display gains on the muted, filtered data demo=gain perc=90 f=0,15,25,30 amps=0.,0.,1.,1. xmute=1,49,97 tmute=1.2,.2,1.2 ntaper=5 tpow=1 sufilter <data.su f=$f amps=$amps | sumute key=tracl xmute=$xmute tmute=$tmute ntaper=$ntaper | sugain tpow=$tpow | supsimage perc=$perc \ title="filter, m...
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#! /bin/sh WIDTH=600 HEIGHT=450 WIDTHOFF1=0 WIDTHOFF2=640 HEIGHTOFF1=50 HEIGHTOFF2=530 # Look at raw data using par file to supply all parameters # This would work even we did not use sushw in MakeDataBig/Little suxmovie<data.su par=oz25.H windowtitle="Raw Data"\ -geometry ${WIDTH}x${HEIGHT}+${WIDTHOFF1}+${HEIGHTOFF1...
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