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sfopoti3d (4.0)		index
user/junyan/Mopoti3d.c
\n Modeling of pure acoustic wave in 3-D transversely isotropic meida using optimized pseudo-Laplacian operator \n

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\n Synopsis
       sfopoti3d > out.rsf vel=vel.rsf sigma=fsigma.rsf delta=fdelta.rsf seta=fseta.rsf phi=fphi.rsf < source.rsf Gxxl=Gxxl.rsf Gxxr=Gxxr.rsf Gyyl=Gyyl.rsf Gyyr=Gyyr.rsf Gzzl=Gzzl.rsf Gzzr=Gzzr.rsf Gxyl=Gxyl.rsf Gxyr=Gxyr.rsf Gxzl=Gxzl.rsf Gxzr=Gxzr.rsf Gyzl=Gyzl.rsf Gyzr=Gyzr.rsf Gxxxxl=Gxxxxl.rsf Gxxxxr=Gxxxxr.rsf Gyyyyl=Gyyyyl.rsf Gyyyyr=Gyyyyr.rsf Gzzzzl=Gzzzzl.rsf Gzzzzr=Gzzzzr.rsf Gxxxyl=Gxxxyl.rsf Gxxxyr=Gxxxyr.rsf Gxxxzl=Gxxxzl.rsf Gxxxzr=Gxxxzr.rsf Gxyyyl=Gxyyyl.rsf Gxyyyr=Gxyyyr.rsf Gyyyzl=Gyyyzl.rsf Gyyyzr=Gyyyzr.rsf Gxzzzl=Gxzzzl.rsf Gxzzzr=Gxzzzr.rsf Gyzzzl=Gyzzzl.rsf Gyzzzr=Gyzzzr.rsf Gxxyyl=Gxxyyl.rsf Gxxyyr=Gxxyyr.rsf Gxxzzl=Gxxzzl.rsf Gxxzzr=Gxxzzr.rsf Gyyzzl=Gyyzzl.rsf Gyyzzr=Gyyzzr.rsf Gxxyzl=Gxxyzl.rsf Gxxyzr=Gxxyzr.rsf Gxyyzl=Gxyyzl.rsf Gxyyzr=Gxyyzr.rsf Gxyzzl=Gxyzzl.rsf Gxyzzr=Gxyzzr.rsf opt=1 dt= nt= isx= isy= isz= nbt=30 nbb=30 nxl=30 nxr=30 nyl=30 nyr=30 czt=0.01 czb=0.01 cxl=0.01 cxr=0.01 cmplx=n pad1=1 snap=1
\n

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\n Parameters
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file Gxxl= 		\tauxiliary input file name
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file Gxxr= 		\tauxiliary input file name
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file Gxxxxl= 		\tauxiliary input file name
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file Gxxxxr= 		\tauxiliary input file name
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file Gxxxyl= 		\tauxiliary input file name
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file Gxxxyr= 		\tauxiliary input file name
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file Gxxxzl= 		\tauxiliary input file name
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file Gxxxzr= 		\tauxiliary input file name
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file Gxxyyl= 		\tauxiliary input file name
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file Gxxyyr= 		\tauxiliary input file name
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file Gxxyzl= 		\tauxiliary input file name
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file Gxxyzr= 		\tauxiliary input file name
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file Gxxzzl= 		\tauxiliary input file name
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file Gxxzzr= 		\tauxiliary input file name
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file Gxyl= 		\tauxiliary input file name
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file Gxyr= 		\tauxiliary input file name
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file Gxyyyl= 		\tauxiliary input file name
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file Gxyyyr= 		\tauxiliary input file name
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file Gxyyzl= 		\tauxiliary input file name
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file Gxyyzr= 		\tauxiliary input file name
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file Gxyzzl= 		\tauxiliary input file name
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file Gxyzzr= 		\tauxiliary input file name
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file Gxzl= 		\tauxiliary input file name
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file Gxzr= 		\tauxiliary input file name
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file Gxzzzl= 		\tauxiliary input file name
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file Gxzzzr= 		\tauxiliary input file name
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file Gyyl= 		\tauxiliary input file name
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file Gyyr= 		\tauxiliary input file name
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file Gyyyyl= 		\tauxiliary input file name
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file Gyyyyr= 		\tauxiliary input file name
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file Gyyyzl= 		\tauxiliary input file name
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file Gyyyzr= 		\tauxiliary input file name
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file Gyyzzl= 		\tauxiliary input file name
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file Gyyzzr= 		\tauxiliary input file name
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file Gyzl= 		\tauxiliary input file name
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file Gyzr= 		\tauxiliary input file name
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file Gyzzzl= 		\tauxiliary input file name
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file Gyzzzr= 		\tauxiliary input file name
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file Gzzl= 		\tauxiliary input file name
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file Gzzr= 		\tauxiliary input file name
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file Gzzzzl= 		\tauxiliary input file name
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file Gzzzzr= 		\tauxiliary input file name
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bool cmplx=n [y/n]		\tuse complex FFT
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float cxl=0.01 		\tdecaying parameter
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float cxr=0.01 		\tdecaying parameter
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float czb=0.01 		\tdecaying parameter
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float czt=0.01 		\tdecaying parameter
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file delta= 		\tauxiliary input file name
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float dt= 		\t
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int isx= 		\t
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int isy= 		\t
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int isz= 		\t
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int nbb=30 		\t
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int nbt=30 		\t
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int nt= 		\t
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int nxl=30 		\t
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int nxr=30 		\t
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int nyl=30 		\t
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int nyr=30 		\tassume ABC pars are the same
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int opt=1 		\tif y, determine optimal size for efficiency
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int pad1=1 		\tpadding factor on the first axis
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file phi= 		\tauxiliary input file name
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file seta= 		\tauxiliary input file name
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file sigma= 		\tauxiliary input file name
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int snap=1 		\t
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file vel= 		\tauxiliary input file name
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