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#! /bin/sh # Model 3: Simple 4 media model # model number model=3 # data directory (optional, if not set data will go into current directory datadir=../datadir/ psfile=${datadir}model${model}.eps datafile=${datadir}model${model}.data ##### Build 4 media model #### model shown in Figure 4 of the GBmod-paper ##...
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#! /bin/sh # Model 5: Salt dome model set +x # model number model=5 # data directory (optional, if not set data will go into current directory) datadir=../datadir/ datafile=${datadir}model${model}.data ##### Build the dome salt model. ##### Note how sedge is used to generate a continuous velocity field trimodel xmin...
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#! /bin/sh # Model 2 : two constant sloth media in contact with a syncline/anticline # boundary # model number model=2 #data directory (optional, if not set data will go into current directory) datadir=../datadir/ psfile=${datadir}model${model}.eps datafile=${datadir}model${model}.data ##### Build two media,...
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#! /bin/sh # Model 5: Salt dome model # model number model=5 # data directory (optional, if not set data will go into current directory) datadir=../datadir/ psfile=${datadir}model${model}.eps datafile=${datadir}model${model}.data ##### Build the dome salt model. ##### Note how sedge is used to generate a continuous...
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#! /bin/sh rm *.eps *.data junk*
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#! /bin/sh # Model 4: Cerveny (multi layer model with a lens and fault) # model number model=4 # data directory (optional, if not set data will go into current directory) datadir=../datadir/ datafile=${datadir}model${model}.data ##### Built the Cerveny model ##### note: this is the model that appears in figure 1 o...
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#! /bin/sh # Model 2 : two constant sloth media in contact with a syncline/anticline # boundary # model number model=2 #data directory (optional, if not set data will go into current directory) datadir=../datadir/ datafile=${datadir}model${model}.data ##### Build two media, syncline/anticline model ### note: ...
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#! /bin/sh # Model 1 - constant sloth (and hence constant wavespeed) medium # model number model=1 # data directory (optional, if unset put datafiles in current directory) datadir=../datadir/ datafile=${datadir}model${model}.data ##### Constant Sloth model trimodel xmin=0 zmin=0 xmax=1.0 zmax=1 \ 1 xedge=0,1 \ z...
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#! /bin/sh # Model 1 - constant sloth (and hence constant wavespeed) medium # model number model=1 # data directory (optional, if unset put datafiles in current directory) datadir=../datadir/ psfile=${datadir}model${model}.eps datafile=${datadir}model${model}.data ##### Constant Sloth model trimodel xmin=0 zmin=0...
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#! /bin/sh # Model 3: Simple 4 media model # model number model=3 # data directory (optional, if not set data will go into current directory datadir=../datadir/ datafile=${datadir}model${model}.data ##### Build 4 media model #### model shown in Figure 4 of the GBmod-paper ##### trimodel xmin=0 zmin=0 xmax=2.0...
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#! /bin/sh # Model 4: Cerveny (multi layer model with a lens and fault) # model number model=4 # data directory (optional, if not set data will go into current directory) datadir=../datadir/ psfile=${datadir}model${model}.eps datafile=${datadir}model${model}.data ##### Built the Cerveny model ##### note: this is t...
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#! /bin/sh cd datadir rm * cd .. for i in * do if test -d $i then cd $i Clean.sh cd .. fi done exit 0
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#! /bin/sh #### Run GBmod with Xwindow Graphics # model model=3 # data directory datadir=../datadir/ #### aux files modelfile=${datadir}model${model}.data rayendsfile=${datadir}rayend.data rayfile=${datadir}ray.data wavefile=${datadir}wave.data wavefilet=${datadir}wavet.data nangle=150 nxz=201 fangle=-45 langle=45...
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#! /bin/sh #### Run GBmod with Xwindow Graphics #### Create Figure 8 in the GBmod paper # model=4 #### find the right directory datadir=../datadir/ #### aux files modelfile=${datadir}model${model}.data rayendsfile=${datadir}rayend.data rayfile=${datadir}ray.data fresnelfile=${datadir}fresnel.data nangle=2 nxz=201...
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#! /bin/sh rm *.eps *.data junk* outpar
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#! /bin/sh if test "$PSPREVIEWER" = "" then echo "Environment variable PSPREVIEWER not set" ; exit 1 fi # model number model=3 #### find the right directory datadir=../datadir/ #### aux files modelfile=${datadir}model${model}.data modelpsfile=${datadir}model${model}.eps rayendsfile=${datadir}rayend.data rayfile=$...
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#! /bin/sh #### Run GBmod with CWP PostScript Graphics if test "$PSPREVIEWER" = "" then echo "Environment variable PSPREVIEWER not set" ; exit 1 fi # model number model=3 # data directory datadir=../datadir/ modelfile=${datadir}model${model}.data modelpsfile=${datadir}model${model}.eps rayendsfile=${datadir}rayend....
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#! /bin/sh #### Run GBmod with CWP PostScript Graphics #### Create Figure 7 in the GBmod paper if test "$PSPREVIEWER" = "" then echo "Environment variable PSPREVIEWER not set" ; exit 1 fi # model number model=4 #### find the right directory datadir=../datadir/ #### aux files modelfile=${datadir}model${model}.data...
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#! /bin/sh #### Run GBmod with Xwindow Graphics #### Create Figure 7 in the GBmod paper # model number model=4 # datadir directory datadir=../datadir/ #### aux files modelfile=${datadir}model${model}.data rayendsfile=${datadir}rayend.data rayfile=${datadir}ray.data nangle=150 nxz=201 fangle=-45 langle=45 target=5...
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#! /bin/sh #### Run GBmod with CWP PostScript Graphics #### Create Figure 6 in the GBmod paper if test "$PSPREVIEWER" = "" then echo "Environment variable PSPREVIEWER not set" ; exit 1 fi # model number model=3 #### find the right directory datadir=../datadir/ #### aux files modelfile=${datadir}model${model}.dat...
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#! /bin/sh #### Run GBmod with Xwindow Graphics #### Create Figure 8 in the GBmod paper # model number model=3 #### find the right directory datadir=../datadir/ #### aux files modelfile=${datadir}model${model}.data rayendsfile=${datadir}rayend.data rayfile=${datadir}ray.data nangle=20 nxz=201 nt=20 fangle=-17 lan...
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#! /bin/sh #### Run GBmod with Xwindow Graphics # model number model=3 datadir=../datadir/ rayendsfile=${datadir}rayend.data rayfile=${datadir}ray.data modelfile=${datadir}model${model}.data nangle=50 nxz=301 fangle=30 langle=45 #### generate modelfile #../Models/Xmodel${model} #### shoot the rays triray <$mod...
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#! /bin/sh #### Run GBmod with CWP PostScript Graphics #### Create Figure 8 in the GBmod paper if test "$PSPREVIEWER" = "" then echo "Environment variable PSPREVIEWER not set" ; exit 1 fi # model number model=4 #### find the right directory datadir=../datadir/ #### aux files modelfile=${datadir}model${model}.data...
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#! /bin/sh #### Run GBmod with CWP PostScript Graphics #### Create Figure 5 in the GBmod paper # model number model=3 #### find the right directory datadir=../datadir/ #### aux files modelfile=${datadir}model${model}.data rayendsfile=${datadir}rayend.data rayfile=${datadir}ray.data wavefile=${datadir}wave.data wav...
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#! /bin/sh #### Run GBmod with CWP PostScript Graphics #### Create Figure 8 in the GBmod paper if test "$PSPREVIEWER" = "" then echo "Environment variable PSPREVIEWER not set" ; exit 1 fi # model model=3 #### find the right directory datadir=../datadir/ #### aux files modelfile=${datadir}model${model}.data modelp...
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#! /bin/sh # Run GBmod with Xwindow Graphics #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir/ datafile=${datadir}model.data ##### Build syncline model (Figure 14) trimodel xmin=-1 zmin=0 xmax=5.0 zmax=...
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#! /bin/sh #### Shoot rays (Figure 14) #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data rayendsfile=${datadir}rayends.data rayfile=${datadir}rays.data nangle=130 fangle=-6...
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#! /bin/sh #### Control shell to #### 1. create syncline model #### 2. plot ray paths #### 3. generate a common shot record Model Rays Beams exit
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#! /bin/sh #### Create Figure 15 in the GBmod-paper #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir rayendsfile=${datadir}/rayends.data #### generate and plot commom shot record gbbeam<$rayendsfile \ ...
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#! /bin/sh # Run GBmod with Xwindow Graphics #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir/ datafile=${datadir}model.data ##### Built salt dome model (Figure 3) trimodel xmin=0 zmin=0 xmax=8 zmax=4 m...
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#! /bin/sh #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data rayendsfile=${datadir}rayends.data rayfile=${datadir}rays.data nxz=201 nangle=130 #### shoot the rays trira...
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#! /bin/sh #### Control shell to #### 1. create salt dome model #### 2. plot raypaths #### 3. generate common shot data Model Rays Beams exit 0
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#! /bin/sh #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ data=../../datadir rayendsfile=${data}/rayends.data #### generate and plot common shot record gbbeam<$rayendsfile \ bw=0 xg=0,8 zg=0,0 ng=101 lscale=0.8 \ ...
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#! /bin/sh # Run GBmod with PSwindow graphics datadir=../../datadir/ modelfile=${datadir}model.data trimodel xmin=-1 zmin=0 xmax=5.0 zmax=3.0 maxangle=10 \ 1 xedge=-1,0,1,2,3,4,5 \ zedge=0,0,0,0,0,0,0 \ sedge=0,0,0,0,0,0,0 \ 2 xedge=-1.,0.0,0.50,1.0,1.5,1.8,2.0,2.5,3.0,3.5,4.0,5 \ zedge=0.3,0.3,0.31,0.3,.37,...
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#! /bin/sh #### Shoot rays (Figure 20) #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data rayendsfile=${datadir}rayends.data rayfile=${datadir}rays.data nangle=260 fangle=-6...
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#! /bin/sh #### Control shell to #### 1. create syncline model #### 2. plot ray paths (all reflected rays) #### 3. generate common shot record Model Rays Beams exit 0
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#! /bin/sh #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data rayendsfile=${datadir}rayends.data ##### Generate Common-shot section nt=151 dt=0.025 bw=0 ft=0.0 ng=101 lsca...
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#! /bin/sh #### Create Figure 16 in the GBmod documentation #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data ##### Generate Zero-offset section nangle=130 nxz=401 fangle=...
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#! /bin/sh # Run GBmod with Xwindow Graphics #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ data=../../datadir/ datafile=${data}model.data ##### Built syncline model (Figure 14) trimodel xmin=-1 zmin=0 xmax=5.0 zmax=2.0 ma...
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#! /bin/sh #### Create Figure 17 in the GBmod documentation #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data ##### Generate Finite-Offset section fg=0.6 nangle=130 nxz=40...
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#! /bin/sh #### Control shell to #### 1. create syncline model #### 2. generate Zero-offset section #### 3. generate Finite-offset section Model Zero Finite exit 0
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#! /bin/sh rm */outpar
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#! /bin/sh #### Create Figure 16 in the GBmod documentation #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data ##### Generate Zero-offset section nangle=130 nxz=401 fangle...
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#! /bin/sh # Run GBmod with Xwindow Graphics #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ datadir=../../datadir/ datafile=${datadir}model.data ##### Build syncline model (Figure 14) trimodel xmin=-1 zmin=0 xmax=5.0 zmax...
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#! /bin/sh #### Create Figure 17 in the GBmod documentation #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data ##### Generate Finite-Offset section fg=0.6 nangle=130 nxz=4...
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#! /bin/sh #### Control shell to #### 1. create syncline model #### 2. generate Zero-offset section #### 3. generate Finite-offset section Model Zero Finite exit 0
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#! /bin/sh #### Create Figure 21 in the GBmod documentation #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ data=../../datadir/ modelfile=${data}model.data ##### Generate Zero-offset section nangle=260 fangle=-65 langle=65...
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#! /bin/sh # Run GBmod with Xwindow graphics datadir=../../datadir/ modelfile=${datadir}model.data trimodel xmin=-1 zmin=0 xmax=5.0 zmax=3.0 maxangle=10 \ 1 xedge=-1,0,1,2,3,4,5 \ zedge=0,0,0,0,0,0,0 \ sedge=0,0,0,0,0,0,0 \ 2 xedge=-1.,0.0,0.50,1.0,1.5,1.8,2.0,2.5,3.0,3.5,4.0,5 \ zedge=0.3,0.3,0.31,0.3,.37,....
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#! /bin/sh #### Create Figure 19 in the GBmod documentation #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ data=../../datadir/ modelfile=${data}model.data ##### Generate Zero-offset section nangle=131 fangle=-65 langle=65...
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#! /bin/sh #### Create Figure 21 in the GBmod documentation #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ data=../../datadir/ modelfile=${data}model.data ##### Generate Zero-offset section nangle=131 fangle=-65 langle=65...
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#! /bin/sh #### Control shell to #### 1. create syncline model #### 2. generate zero-offset data including all rays #### 3. generate zero-offset data including only reflected rays #### 4. as (3), but higher ray coverage Model Seis1 Seis2 Seis3 exit 0
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#! /bin/sh #### Create Figure 21 in the GBmod documentation #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ data=../../datadir/ modelfile=${data}model.data ##### Generate Zero-offset section nangle=260 fangle=-65 langle=65 ...
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#! /bin/sh # Run GBmod with Xwindow graphics data=../../datadir/ datafile=${data}model.data trimodel xmin=-1 zmin=0 xmax=5.0 zmax=3.0 maxangle=10 \ 1 xedge=-1,0,1,2,3,4,5 \ zedge=0,0,0,0,0,0,0 \ sedge=0,0,0,0,0,0,0 \ 2 xedge=-1.,0.0,0.50,1.0,1.5,1.8,2.0,2.5,3.0,3.5,4.0,5 \ zedge=0.3,0.3,0.31,0.3,.37,.68,.63,...
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#! /bin/sh #### Create Figure 19 in the GBmod documentation #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ data=../../datadir/ modelfile=${data}model.data ##### Generate Zero-offset section nangle=131 fangle=-65 langle=65 ...
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#! /bin/sh #### Create Figure 21 in the GBmod documentation #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ data=../../datadir/ modelfile=${data}model.data ##### Generate Zero-offset section nangle=131 fangle=-65 langle=65 ...
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#! /bin/sh #### Control shell to #### 1. create syncline model #### 2. generate zero-offset data including all rays #### 3. generate zero-offset data including only reflected rays #### 4. as (3), but higher ray coverage Model Seis1 Seis2 Seis3 exit 0
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#! /bin/sh # Run GBmod with Xwindow Graphics #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ datadir=../../datadir/ datafile=${datadir}model.data ##### Build syncline model (Figure 14) trimodel xmin=-1 zmin=0 xmax=5.0 zmax...
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#! /bin/sh #### Shoot rays (Figure 14) #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data rayendsfile=${datadir}rayends.data rayfile=${datadir}rays.data nangle=130 fangle=-...
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#! /bin/sh #### Control shell to #### 1. create syncline model #### 2. plot ray paths #### 3. generate a common shot record Model Rays Beams exit
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#! /bin/sh #### Create Figure 15 in the GBmod-paper #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ datadir=../../datadir rayendsfile=${datadir}/rayends.data #### generate and plot commom shot record gbbeam<$rayendsfile \ ...
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#! /bin/sh # Run GBmod with Xwindow Graphics #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir/ datafile=${datadir}model.data ##### Built salt dome model (Figure 3) trimodel xmin=0 zmin=0 xmax=8 zmax=4 m...
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#! /bin/sh #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data rayendsfile=${datadir}rayends.data rayfile=${datadir}rays.data nxz=201 nangle=130 #### shoot the rays trira...
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#! /bin/sh #### Control shell to #### 1. create salt dome model #### 2. plot raypaths #### 3. generate common shot data Model Rays Beams exit 0
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#! /bin/sh #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL PSdemo #------------------------------------------------ data=../../datadir rayendsfile=${data}/rayends.data #### generate and plot common shot record gbbeam<$rayendsfile \ bw=0 xg=0,8 zg=0,0 ng=101 lscale=0.8 \ ...
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#! /bin/sh # Run GBmod with Xwindow graphics datadir=../../datadir/ modelfile=${datadir}model.data trimodel xmin=-1 zmin=0 xmax=5.0 zmax=3.0 maxangle=10 \ 1 xedge=-1,0,1,2,3,4,5 \ zedge=0,0,0,0,0,0,0 \ sedge=0,0,0,0,0,0,0 \ 2 xedge=-1.,0.0,0.50,1.0,1.5,1.8,2.0,2.5,3.0,3.5,4.0,5 \ zedge=0.3,0.3,0.31,0.3,.37,....
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#! /bin/sh #### Shoot rays (Figure 20) #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data rayendsfile=${datadir}rayends.data rayfile=${datadir}rays.data nangle=260 fangle=-65...
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#! /bin/sh #### Control shell to #### 1. create syncline model #### 2. plot ray paths (all reflected rays) #### 3. generate common shot record Model Rays Beams exit 0
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#! /bin/sh #------------------------------------------------ # RUN THIS SHELL WITH MASTER SHELL Xdemo #------------------------------------------------ datadir=../../datadir/ modelfile=${datadir}model.data rayendsfile=${datadir}rayends.data ##### Generate Common-shot section nt=151 dt=0.025 bw=0 ft=0.0 ng=101 lscal...
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#! /bin/sh # Clean created data files rm -f *.eps exit
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#! /bin/sh # suimp2d, suimp3d --- impulsive seismic data over a point scatterer 2D,3D WIDTH=420 HEIGHT=700 XOFF1=0 XOFF2=430 XOFF3=860 YOFF=150 echo "The third of three windows in this demo takes some time to come up" echo ## Example 1: default -- one record zero offset above a point scatterer ## one shot at (0,0) #...
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#! /bin/sh # suimp2d, suimp3d --- impulsive seismic data over a point scatterer 2D,3D # Author: John Stockwell, 7 Jun 1993 demo=spike ## Example 1: default -- one record zero offset above a point scatterer ## one shot at (0,0) ## one receiver at (0,0) ## scatterer at (1000,1000) suimp2d x0=0 | supswigp title="Sing...
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#! /bin/sh # Clean.sh created data files rm -f *.out junk* *.dir *.data *.eps *.ps density* velocity* *reflection* exit
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#! /bin/sh set -x # # This script produces a velocity model for the modelling # # To view the model type: # ximage < velocity.dir n1=100 # # # Stig-Kyrre Foss, 29.Oct 2001 ninf=1 nx=100 nz=100 dx=5 dz=5 fx=0.0 fz=0.0 v00=1500.,2500. dvdx=0.0 npmax=100 dvdz=0.0,0.0 unif2 < boundaries > vpsmtest.dir nx=$nx nz=$nz ni...
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#! /bin/sh nt=250 indexdt=0 dt=0.001 time=0.25 ## THE MODEL: nx=100 nz=100 dx=5.0 dz=5.0 ## THE SOURCE: fpeak=30 sx=50 sz=10 # source=1 means that it is a point source source=1 # Source information (index=direction of source) indexux=0 indexuy=0 indexuz=1 wavelet=2 # impulse is 1 is a single source impu...
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#! /bin/sh nt=250 indexdt=0 dt=0.001 time=0.25 ## THE MODEL: nx=100 nz=100 dx=5.0 dz=5.0 ## THE SOURCE: fpeak=30 sx=50 sz=10 # source=1 means that it is a point source source=1 # Source information (index=direction of source) indexux=0 indexuy=0 indexuz=1 wavelet=2 # impulse is 1 is a single source impu...
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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 # modelfile=model11.unif # input model file for unif2aniso ninf=4 # number of interfaces (surface counts) x0=0,0,0,0 # x-position(s) for vp00,vs00,rho00, etc. z0=0,150,156 # z-position(s) for vp00,vs00,rho00, etc. nz=400 # ...
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#! /bin/sh rm *out* *.su* tmp *.ps *_file *.eps
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#! /bin/sh # waveguide - smoothed boundaries between waveguide and media modelfile=model7.unif # input model file for unif2aniso ninf=2 # number of interfaces (surface counts) x0=0,0,0 # x-position(s) for vp00,vs00,rho00, etc. z0=0,1000,1100 # z-position(s)...
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#! /bin/sh # This input file reproduces the output in Juhlin (1995) Figure 6a. # Note that the source in Table 1 in Juhlin (1995) is given as g(t), but should be f(t) # be f(t), i.e. the derivative of the Gaussian (dg) # Since the dg source waveform is defined by its avg frequency content # favg should be set to 24.15 ...
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#! /bin/sh # This input file reproduces the output in Juhlin (1995) Figure 6a. # Note that the source in Table 1 in Juhlin (1995) is given as g(t), but should be f(t) # be f(t), i.e. the derivative of the Gaussian (dg) # Since the dg source waveform is defined by its avg frequency content # favg should be set to 24.15 ...
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#! /bin/sh # This input file reproduces the output in Juhlin (1995) Figure 6a. # Note that the source in Table 1 in Juhlin (1995) is given as g(t), but should be f(t) # be f(t), i.e. the derivative of the Gaussian (dg) # Since the dg source waveform is defined by its avg frequency content # favg should be set to 24.15 ...
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#! /bin/sh # This input file reproduces the output in Juhlin (1995) Figure 8b. # Note that the source in Table 1 in Juhlin (1995) is given as g(t), but should be f(t) # be f(t), i.e. the derivative of the Gaussian (dg) # Since the dg source waveform is defined by its avg frequency content # favg should be set to 17.077...
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#! /bin/sh # modelfile=model10.unif # input model file for unif2aniso ninf=3 # number of interfaces (surface counts) x0=0,0 # x-position(s) for vp00,vs00,rho00, etc. z0=0,1800 # z-position(s) for vp00,vs00,rho00, etc. nz=600 # size o...
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#! /bin/sh # This input file reproduces the output in Juhlin (1995) Figure 8b. # Note that the source in Table 1 in Juhlin (1995) is given as g(t), but should be f(t) # be f(t), i.e. the derivative of the Gaussian (dg) # Since the dg source waveform is defined by its avg frequency content # favg should be set to 17.077...
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#! /bin/sh # This input file reproduces the output in Juhlin (1995) Figure 6b. # Note that the source in Table 1 in Juhlin (1995) is given as g(t), but should be f(t) # be f(t), i.e. the derivative of the Gaussian (dg) # Since the dg source waveform is defined by its avg frequency content # favg should be set to 24.15 ...
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#! /bin/sh # modelfile=model6.unif # input model file for unif2aniso ninf=4 # number of interfaces (surface counts) x0=0,0,0,0 # x-position(s) for vp00,vs00,rho00, etc. z0=0,150,156 # z-position(s) for vp00,vs00,rho00, etc. nz=200 # s...
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#! /bin/sh # modelfile=model6.unif # input model file for unif2aniso ninf=4 # number of interfaces (surface counts) x0=0,0,0,0 # x-position(s) for vp00,vs00,rho00, etc. z0=0,150,156 # z-position(s) for vp00,vs00,rho00, etc. nz=400 # s...
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#! /bin/sh # waveguide - sharp boundaries between layer and surrounding media modelfile=model7.unif # input model file for unif2aniso ninf=2 # number of interfaces (surface counts) x0=0,0,0 # x-position(s) for vp00,vs00,rho00, etc. z0=0,1000,1100 # z-positi...
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#! /bin/sh # Clean.sh created data files rm -f *.out junk* *.eps *.ps density* velocity* snaps* 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.pml.out pml=1 pml_thick=20 n1=500 n2=2000 d2=25 d1=25 # build the file of velocities unif2 < model.unif2 ninf=2 nx=$n2 nz=$n1 dz=$d1 dx=$d2 \ v00=5000,4700,5000 > velocity.1 # build the file of densities unif2 < model.unif2 ninf=6 nx=100 nz=500 dx=25 \ v0...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling: Test of the PML transparent boundary conditions # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=50 WIDTHOFF2=530 HEIGHTOFF1=50 HEIGHTOFF2=530 n1=100 d1=5 f1=0.0 label1="Depth (km)" n2=100 d2=5 f2=0.0 label2="Distance (km)" xs=...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling: part 1, the movie # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=50 WIDTHOFF2=530 HEIGHTOFF1=50 HEIGHTOFF2=530 n1=500 d1=5 f1=0.0 label1="Depth (km)" n2=500 d2=5 f2=0.0 label2="Distance (km)" xs=1250 zs=125 hsz=300 vsx=1000 ve...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2_pml # finite-difference modeling: part 1, the movie # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=10 WIDTHOFF2=500 HEIGHTOFF1=50 HEIGHTOFF2=530 n1=100 d1=5 f1=0.0 label1="Depth (km)" n2=100 d2=5 f2=0.0 label2="Distance (km)" xs=250 zs=50 hsz=50 vsx=250 ve...
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#! /bin/sh # Sufdmod2 --- example script for sufdmod2 # finite-difference modeling, part 2 the output files # Author: John Stockwell WIDTH=450 HEIGHT=450 WIDTHOFF1=20 WIDTHOFF2=510 WIDTHOFF3=930 HEIGHTOFF1=50 HEIGHTOFF2=530 clip=.5 suwind <vseis.pml.out j=3 | suxwigb clip=$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.pml.out clip=1.0 \ title="Vertical line of seismograms" \ windowtitle="Vertical" \ label1=...
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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 | smooth2 n1=122 n2=384 r1=5 r2=5 > velocity.1 # build the file of densities unif2 < model.unif2 ninf=6 nx=384 nz=122 dx=10 \ v00=1.0,2.25,2.25,2.25,2....
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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 # Xdemo1 - simple example script for sufdmod1, X window graphics # N. Maercklin, Oct. 2006 # Output file names (velocity,density and seismogram): vfile=velocity.bin dfile=density.bin sufile=seismogram.su # Velocity and density model: depth=0,600,601,1200,1201,1500,1501,2000 velo=2000,2000,3000,3000,2600,26...
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