📄 suinvco3d.3d.suinvco3d
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SUINVCO3D - Seismic INVersion of Common Offset data with V(X,Y,Z) velocity function in 3D suinvco3d <infile >outfile [optional parameters] Required Parameters: vfile= file containing velocity array v[nvy][nvx][nvz] nzv= number of z samples (1st dimension) in velocity nxm= number of midpoints of input traces nym= number of lines geo_type= geometry type 1 ---- general velocity distribution v(x,y,z) 2 ---- v(x,z) medium 3 ---- v(z) medium com_type= computation type, determines what tables are needed 1 ---- only needs traveltime, weight=1.0 2 ---- traveltime, propagation angles, weight=ctheta 3 ---- traveltime, angle and amplitude, weight=det/as/ag/(1+ctheta) nzt= number of z samples (1st dimension) in traveltime nxt= number of x samples (2nd dimension) in traveltime nyt= number of y samples (3rd dimension) in traveltime tfile file containing traveltime array t[nyt][nxt][nzt] ampfile file containing amplitude array amp[nyt][nxt][nzt] d21file file containing Beylkin determinant component array d22file file containing Beylkin determinant component array d23file file containing Beylkin determinant component array d31file file containing Beylkin determinant component array d32file file containing Beylkin determinant component array d33file file containing Beylkin determinant component array a1file file containing ray propagation angle (polar) array b1file file containing ray propagation angle (azimuth) array Optional Parameters: dt= or from header (dt) time sampling interval of input data offs= or from header (offset) source-receiver offset dxm= or from header (d2) x sampling interval of midpoints fxm=0 first midpoint in input trace dym=50.0 y sampling interval of midpoints fym=0 y-coordinate of first midpoint in input trace nxv= number of x samples (2nd dimension) in velocity nyv= number of y samples (3rd dimension) in velocity dxv=50.0 x sampling interval of velocity fxv=0.0 first x sample of velocity dyv=50.0 y sampling interval of velocity fyv=0.0 first y sample of velocity dzv=50.0 z sampling interval of velocity fzv=0.0 first z sample of velocity nxb=nx/2 band centered at midpoints (see note) fxo=0.0 x-coordinate of first output trace dxo=15.0 horizontal spacing of output trace nxo=101 number of output traces ", fyo=0.0 y-coordinate of first output trace dyo=15.0 y-coordinate spacing of output trace nyo=101 number of output traces in y-direction fzo=0.0 z-coordinate of first point in output trace dzo=15.0 vertical spacing of output trace nzo=101 number of points in output trace ", dxt=100.0 x-coordinate spacing of input tables(traveltime, etc) dyt=100.0 y-coordinate spacing of input tables(traveltime, etc) dzt=100.0 z-coordinate spacing of input tables(traveltime, etc) xt0=0.0 x-coordinate of first input tables xt1=0.0 x-coordinate of last input tables yt0=0.0 y-coordinate of first input tables yt1=0.0 y-coordinate of last input tables fmax=0.25/dt Maximum frequency set for operator antialiasing ang=180 Maximum dip angle allowed in the image apet=45 aperture open angle for summation alias=0 =1 to set the anti-aliasing filter verbose=1 =1 to print some useful information Notes: The information needed in the computation of the weighting factor in Kirchhoff inversion formula includes traveltime, amplitude, and Beylkin determinant at each grid point for each source/receiver point. For a 3-D nonzero common-offset inversion, the Beylkin determinant is computed from a 3x3 matrix with each element containing a sum of quantities from the source and the receiver. The nine elements in the Beylkin matrix for each source/receiver can be determined by eight quantities. These quantities can be computed by the dynamic ray tracer. Tables of traveltime, amplitude, and Beylkin matrix elements from each source and receiver are pre-computed and stored in files. For each trace, tables of traveltime, amplitude and Beylkin matrix at the source and receiver location are input or interpolated from neighboring tables. For the computation of weighting factor, linear interpolation is used to determine the weighting factor at each output grid point, and weighted diffraction summation is then applied. For each midpoint, the traveltimes and weight factors are calculated in the horizontal range of (xm-nxb*dx-z*tan(apet), xm+nxb*dx+z*tan(apet)). Offsets are signed - may be positive or negative. ", This algorithm is based on the inversion formulas in chaper 5 of _Mathematics of Multimensional Seismic Migration, Imaging and Inversion_ (Springer-Verlag, 2000), by Bleistein, N., Cohen, J.K. and Stockwell, Jr., J. W.
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