NAME

     radonf  - generalized Discrete Radon Transform from (t,x) to
     $( tau ,p)$, $ ( omega ,p)$ or $ ( omega ,k) $ space.


SYNOPSIS

     radonf [  -Nfile_in  ]  [  -Ofile_out  ]  [  -mminmmin  ]  [
     -mmaxmmax ] [ -npnp ] [ -sist ] [ -eiend ] [ -f1f1 ] [ -f2f2
     ] [ -f3f3 ] [ -f4f4 ] [ -tsemb1tsemb1 ] [ -tsemb2tsemb2 ]  [
     -tsemb3tsemb3  ] [ -tsemb4tsemb4 ] [ -xmaxxmax ] [ -zrefzref
     ] [ -ipwpw ] [ -alphaalpha ] [ -prewwhite ] [  -sigma1sigma1
     ]  [  -sigma2sigma2  ] [ -sembwxsembwx ] [ -sembwtsembwt ] [
     -nyquist ] [ -L ] [ -P ] [ -H ] [ -K ] [ -taup ] [ -time ] [
     -omega  ]  [  -livenlive  ]  [  -nxtapernxtaper  ]  [ -ntta-
     pernttaper ] [ -Mamaxmem ] [ -V ] [ -? ]


DESCRIPTION

     radonf takes irregularly sampled seismic (t,x)  gathers  and
     forward  transforms  them into the generalized $( tau ,p), (
     omega , p)$ or $( omega , k)$ domain. The  user  models  the
     seismic  data  with a series of np linear, parabolic, hyper-
     bolic curves (or for  the  least  squares  discrete  Fourier
     transform,  with  sines  and  cosines)  which are fit to the
     data in a least squares sense.


     When coupled with other programs,  radonf  can  be  used  to
     enhance  coherent signal or attenuate coherent noise such as
     linear noise  trains  and  multiple  reflections.  The  flow
     radonf|polymute|radonr   produces  results  identical to the
     modeled output of routine  rmmult  except that the  user  is
     allowed  to interact with the intermediate results in the $(
     tau ,p)  $  domain.  Typically,  input  to  the  process  is
     unstacked  common  shot, common receiver, common midpoint or
     common reflection point gathers. For multiple rejection, the
     primary  reflections  should  be  flattened or overcorrected
     using an appropriate NMO routine.  Stacked or common  offset
     data may be processed by breaking the data into running win-
     dows              using               the               flow
     rwindow|radonf|pred|polymute|radonr|rwindow -R.

     Like conventional  dip  filtering,  quadrant  chopping,  and
     other $( omega ,k)$ techniques, this technique allows effec-
     tive separation of coincident primaries and multiples in the
     transform  domain.  With  proper  parameterization,  one can
     remove well separated multiples while minimizing any  ampli-
     tude  effects  on  the  primaries,  including  at the inside
     traces.

     By using semblance weighting, one can deal effectively  with
     spatially aliased data.


     radonf  gets both its data and its parameters  from  command
     line  arguments.  These arguments specify the input, output,
     the temporal design window, the type of transformation to be
     used,  the  minimum  and  maximum moveout to be modeled, the
     number of parameters/curves to fit,  tapers,  and  semblance
     weighting if desired.

  Command line arguments
     -N file_in
          Enter the input data set name or file immediately after
          typing -N unless the input is from a pipe in which case
          the -N entry must be omitted.  This input  file  should
          include the complete path name if the file resides in a
          different              directory.               Example
          -N/export/data2/china/cdp.gather  tells  the program to
          look    for    file    'cdp.gather'    in     directory
          '/export/data2/china'.

     -O file_out
          Enter the output data  set  name  or  file  immediately
          after typing -O.  This output file is not required when
          piping the output to another process.  The output  data
          set also requires the full path name (see above).

     -s ist
          Window Start Time (msec).  This  window  specifies  the
          region  on  the  input  data  after which noise will be
          suppressed. (default = first sample).

     -e iend
          Window  End  Time  (msec).  End  of  window  for  noise
          suppression. (default = last sample)

     -f1 f1
          Frequency (Hz) at which we begin roll in of  a  Hamming
          zero phase band pass filter (default = 5Hz)

     -f2 f2
          Frequency (Hz) at which we end roll  in  of  a  Hamming
          zero phase band pass filter (default =  f1).

     -f3 f3
          Frequency (Hz) at which we begin roll out of a  Hamming
          zero phase band pass filter (default =  f4).

     -f4 f4
          Frequency (Hz) at which we end roll out  of  a  Hamming
          zero  phase  band pass filter . The cost increases with
          the value of f4. (default = Nyquist)

     -mmin mmin
          Minimum value of  differential  moveout  (msec)  to  be
          modeled,  measured  at distance xmax. If the primary is
          NMO-corrected to be flat,  it  is  recommended  to  set
          $mmin<=-200msec$ for a value of f1=5Hz , thereby allow-
          ing the algorithm to model subtle AVO effects at 5Hz in
          the wavelet. No default.

     -mmax mmax
          Maximum value of  differential  moveout  (msec)  to  be
          modeled,  measured  at distance xmax. This value should
          be slightly greater than the largest moveout  the  user
          wishes to reject. No default.

     -np np
          Number of parameters or  curves.  About  each  record's
          (actual  or  nonexisting)  zero  -offset trace a set of
          linear, parabolic,  hyperbolic  curves  (or  sines  and
          cosines for the -K option)  are used to model the data.
          The moveout range for these curves is specified in  the
          -mmin,  -mmax  entries above. This parameter determines
          how many curves are used to span that range.  The  cost
          goes  up  linearly with the value of np. (Default: np =
          $n sub trace$, where $n sub trace $ is  the  number  of
          traces  in the gather, guaranteeing enough locations to
          carry  trace  headers  from  forward  back  to  inverse
          transformation. see the -nyquist option below).

     -nyquist
          If present, np = 2*f4*.001*(mmax-mmin)+1 or two  points
          per  wavelength  at  the farthest offset, as in routine
          rmmult. (Default, use np=$ n sub trace $)

     -xmax xmax
          Maximum trace distance (ft  or  m)  in  the  data.  The
          moveout  entered  after  the   -mmin, -mmax options are
          referenced to this value of xmax.  For  linear  moveout
          (-L  option),  the  minimum slowness $p sub min = m sub
          min /x sub max = 1/v sub max $, while the maximum slow-
          ness  $p sub max = m sub max /x sub max = 1/v sub min $
          . No default.

     -prew white
          Percent  prewhitening  used  to  stabilize  the  least-
          squares  inversion  in the presence of noise. Default =
          5%

     -nttaper nttaper
          Temporal taper length (msec). This taper is applied  to
          both  the beginning and the end of the analysis window.
          Smooth tapers are imperative in obtaining artifact free
          Radon transforms! (default=100 msec)


     -nxtaper nxtaper
          Spatial taper length (traces). This taper is applied to
          both  the  start  and  the  end of the analysis window.
          Smooth tapers are imperative in obtaining artifact free
          Radon transforms! (default=5 traces)

     -live minlive
          Enter the minimum number of live traces accepted  in  a
          gather.  Gathers having less than this many live traces
          will be zeroed out and flagged dead. (default = 3).


     -M amaxmem
          Enter the maximum memory allowed  for  the  program  in
          Megawords.  The program will try to store as many radon
          transform matrices, $[R(  omega  ,x  sub  j  ,p)]$,  in
          memory  as  will  fit,  thereby eliminating the need to
          recompute them for the  repeated  source-receiver  dis-
          tances  in  subsequent  gathers.  (Default:  amaxmem=16
          Megawords on the  Crays,  amaxmem=4  Megawords  on  the
          Sparcs and HPs).

     -L   Enter the command line  argument  '-L'  to  use  linear
          curves in the data model (No default. Other options are
          -P, -H and -K).

     -P   Enter the command line argument '-P' to use   parabolic
          curves  in  the  data model. (No default. Other options
          are -L, -H and -K).

     -H   Enter the command  line  argument  '-H'  to  use   time
          invariant   hyperbolic  curves  in  the  data model (No
          default. Other options are -L, -P and -K).

     -K   Enter the command line argument '-K' to perform a least
          square  $  (  omega ,k) $ transform. (No default. Other
          options are -L, -P and -H).

     -zref zref
          Reference depth for time invariant hyperbolic curves if
          -H  option  selected.  Hyperbolae defined as in  Foster
          and Mosher, Geophysics, 1992 . Default: zref=xmax).

     -ipw pw
          Weight the input (t,x) data using inverse power weight-
          ing  in  the  conventional $( tau ,p)$ transform before
          normalization/orthogonalization.  This  weighting  will
          suppress high amplitude spurious events, including edge
          effects.  Maximum weight will be 1./pw times  the  mean
          square  energy of the current seismic gather to be pro-
          cessed. (Default if ipw is entered, is  0.1,  otherwise
          the  forward  transform  is  performed  without inverse
          power weighting).

     -alpha alpha
          If present, form the forward $(  tau  ,p)  $  transform
          using  an $alpha$ trim mean vs. conventional sum before
          normalization/orthogonalization.  This  weighting  will
          suppress high amplitude spurious events, including edge
          effects. $alpha$ = 1.0 will produce a conventional sum.
          $alpha$   =  .5  will  sum  half  the  data.  (Default,
          $alpha$=1.0, such that conventional summation is used).

     -sigma1 sigma1
          If present, reject data whose  time  average  semblance
          $sigma  bar  <=  sigma  sub  1 = sigma1$. See algorithm
          description  below.   This  weighting  will  accentuate
          coherent/continuous   events  and  suppress  incoherent
          events. (Default: NO semblance  weighting.  Suggestion:
          sigma1 = 0.05)

     -sigma2 sigma2
          If present, pass  data  whose  time  average  semblance
          $sigma  bar  >=  sigma  sub  2 = sigma1$. See algorithm
          description  below.   This  weighting  will  accentuate
          coherent/continuous   events  and  suppress  incoherent
          events.    (Default:    NO     semblance     weighting.
          Suggestion:sigma2 = 0.20)

     -sembwx sembwx
          Half width, $ n sub x $, in traces, of the running sem-
          blance calculation window which is triggered by supply-
          ing a non-zero value. See algorithm description  below.
          A reasonable number is sembwx = 5.

     -sembwt sembwt
          Half length, $w sub t =Kdt$ in  msec,  of  the  running
          semblance  calculation  window. (Used only if -sigma1,-
          sigma2 options invoked above. If so, default: sembwt  =
          24 msec)

     -tsemb1 tsemb1
          Time (msec) at which we  begin  roll  in  of  semblance
          weighting (Default = first sample).

     -tsemb2 tsemb2
          Time (msec) at  which  we  end  roll  in  of  semblance
          weighting (Default = tsemb2)

     -tsemb3 tsemb3
          Time (msec) at which  we  end  roll  off  of  semblance
          weighting (Default = tsemb4)


     -tsemb4 tsemb4
          Frequency (Hz) at which we end roll out  of  a  Hamming
          zero phase band pass filter (Default = last sample).

     -taup
          Output the conventional $( tau ,p)$ transform ( vs. the
          discrete  Radon  transform).  This option allows one to
          compare the subtle differences between  discrete  Radon
          and  coventional  $(  tau ,p) $ transforms. The conven-
          tional $( tau ,p) $ transform is significantly  cheaper
          than the discrete Radon transformand sometimes accurate
          results can be acheived for the -L option.

     -time
          If present, calculate the $( tau ,p) $  transform  part
          of  the  calculation in the time (vs. frequency) domain
          by resampling the traces using a 6 point  interpolator.
          (Default  if  -sigma1, -sigma2, -ipw, or -alpha options
          are used, otherwise the more efficient frequency domain
          transform is used).

     -omega
          If present, output the results in the $( omega ,p)$ vs.
          the $( tau ,p) $ domain (no matter how they were calcu-
          lated). The results are packed with the first  half  of
          the  samples  in  each  constant p trace containing the
          amplitude, the second containing the phase. This option
          is  useful  for examining aliasing effects and possible
          match filtering applications.  This  option  is  forced
          when using the -K option described above).

     -V   Enter the command line argument '-V' to get  additional
          printout.

     -?   Enter the command line  argument  '-?'  to  get  online
          help.   The program terminates after the help screen is
          printed.


The Reverse 2D Radon Transform:

     We define the reverse Radon transform (implemented  in  pro-
     gram radonr) for irregularly spaced data to be :

     ${u}=[R] {U}$,


     where

     $U sub m = U(  omega  ,p sub m  )$,

     $u sub j  = u( omega , x sub j  )$

     $R sub {mj}   = e sup { +i omega [p sub m theta (x sub  j  )
     ] }$,

     $omega =$ the temporal frequency in radians/sec,

     $p sub m = $ the mth apparent moveout in the x direction,

     $x sub j = $ the position of the jth trace ,

     $theta (x sub j ) = {x sub j } $ for a linear transform,

     $theta (x sub j ) = {x sub j }  sup  2  $  for  a  parabolic
     transform,

     $theta (x sub j ) = [{x sub j } sup 2 + {z sub ref } sup 2 ]
     sup 1/2 $ for a hyperbolic trans form, and

     $ z sub ref $ = an appropriate reference depth.




The Forward 2D Discrete Radon Transform:

     We define the forward DRT such that when when it is followed
     by the above reverse transform we can reconstruct the origi-
     nal data, $u( omega , x sub j )$ in a least squares sense:


     ${U}=([R] sup * [R] + epsilon [I] )  sup  {-1}   [R]  sup  *
     {u}$,

     where

     $R sub {mj} sup *   = e sup { -i omega [p sub m theta (x sub
     j )  ] }$,

     $[I]$ = the identity matrix, and

     $epsilon $ = a prewhitening factor.





The Conventional 2d Forward (tau,p) Transform:

     The conventional $( tau , p )$ algorithm  when  followed  by
     above  defined  reverse  transform will approximately recon-
     struct the original data when using linear moveout  (the  -L
     option below)
      on equally sampled trace spacing. This algorithm should not
     be  used for nonlinear moveouts and sparse, irregularly sam-
     pled data as encountered in 3D CMP gathers.

     First define the unscaled $( tau ,p )$ transform in the time
     (t,x) domain:
     $U bar ( tau ,p) =  sum from j=1 to J { u( tau -px sub j , x
     sub j )} $

     Next, transform from $( tau ,p)$ to $( omega ,p)$ and  scale
     with the so-called $ rho $ factor
      :

     $U ( omega , p) = rho ( omega ) U bar ( omega , p) $, where

     $rho ( omega ) = sqrt {omega / 2 pi }  $.




The least square Fourier (omega,k) Transform:

     The  conventional  Fast  Fourier  Transform  (FFT)   assumes
     equally  spaced  seismic  traces, in which case the discrete
     Fourier transform (DFT) as  implemented  in  program  fft2da
     becomes  orthogonal.  In  addition, the equal spacing allows
     one to exploit a certain  spatial  invariance  of  the  data
     resulting  in  the  'fast'  part of the FFT. For irregularly
     sampled data, the inverse DFT as implemented in  program  fk
     is  non  orthogonal. The least square DFT is closely related
     to the least square DRT:


     We define the reverse DFT (implemented  in  program  radonr)
     for irregularly spaced data to be :


     ${u}=[F] {U}$,

     or

     $u ( omega , x sub j ) = sum from {m= k sub min } to {m =  k
     sub max } F sub mj U sub m $,

     where

     $F sub {mj}   = e sup { +i omega [k sub m x sub j  ] }$,

     $k sub m = $ the mth wavenumber component in  the  x  direc-
     tion,

     $k sub min = 2 pi f sub 4 m sub min / x sub max $, and

     $k sub max = 2 pi f sub 4 m sub max / x sub max $

     We define the forward DFT such that when when it is followed by the above reverse transform we can reconstruct the original data, $u( omega , x sub j )$ in a least squares sense:


     ${U}=([F] sup * [F] + epsilon [I] )  sup  {-1}   [F]  sup  *
     {u}$,
     where

     $F sub {mj} sup *   = e sup { -i omega [k sub m x sub j    ]
     }$.




The Semblance weighted Forward (tau,p) Transform:

     For gathers comprised of only a few ( < 20 ) traces,  it  is
     useful  to  consider weighting/windo wing the output conven-
     tional $( tau ,p) $ transform $U ( tau , p)$  by weights  $w
     ( tau
      ,p) $ proportional to the time averaged semblance along the
     same  (linear)  summation curves to obtain $ U hat ( tau ,p)
     $:

     $ U hat ( tau , p) = w( sigma bar  ( tau ,p) U bar (  tau  ,
     p) $,

     where

     $w ( sigma bar  ) = 0.$ if $ sigma bar  <= sigma bar  sub  1
     $,


     $w ( sigma bar  ) =  1 over 2 [ 1 + cos({ sigma bar  - sigma
     bar   sub 1 } over {sigma bar  su b 2 - sigma bar  sub 1} pi
     )]$, if $ sigma bar  sub 1 < sigma bar  < sigma bar   sub  2
     $,

     $w ( sigma bar ) = 1.$ if $ sigma bar  >= sigma bar   sub  2
     $, and

     $ sigma bar  ( tau ,p)={ sum from k=-w/dt to k=+w/dt  [  sum
     from  j=1  to j=J u ( tau -px sub j ,x sub j )] sup 2 } over
     {J sum  from k=-w/dt to k=+w/dt sum from j=1 to j=J [u ( tau
     -px sub
      j , x sub j )] sup 2 }$




The Running Window Semblance Weighted

     Forward (tau,p) Transform:

     For gathers comprised of many ( > 20 ) traces, it is  useful
     to  consider weighting the  input data u(t,x)  by weights $w
     ( tau ,p, x sub j ) $ proportional to the time averaged semb
     lance in a running window ranging from $-n sub x$ to $+n sub
     x$ along the same (linear) summation curves used  to  calcu-
     late $U ( tau ,p)  $:

     $ U tilde ( tau , p) = sum from j=1 to j=J w[ sigma  bar   (
     tau-px sub j )] u( tau -px sub j )
        $,

     where

     $w ( sigma bar  )$ is defined as above, and

     $ sigma bar  ( tau - px  sub  j  )={  sum  from  k=-w/dt  to
     k=+w/dt  [  sum from {n=-n sub x } to {n= +n sub x } u ( tau
     -px sub j+n ,x sub j+n )] sup 2 } over {J  sum   from  {n=-n
     sub x } to {n=+n
      sub x } sum from j=1 to j=J [u ( tau -px sub j+n  ,  x  sub
     j+n )] sup 2 }$






NOTE 1:

     The flows  radonf|polymute|radonr, radonf|taupred|radonr and
     radonf|polymute|taupred|radonr  can  be  quite  effective in
     eliminating  coherent  noise  and/or  multiples.  The   flow
     radonf|radonr  by itself can be used to generate data and/or
     interpolate dead traces on a regular surface grid.


NOTE 2:

     Inverse  velocity  multiple  rejection  in  common  shot  or
     receiver  domain  can  be  difficult since the apices of the
     parabolae/hyperbolae are not centered about x=0.  Many  more
     parameters   are   needed  to  express  these  off  centered
     parabolae/hyperbolae    than     those     than     centered
     parabolae/hyperbolae  in the CMP domain. In general, filter-
     ing of common shot, receiver of offset domain should be done
     only with the -L or -F options. The -P and -H options show a
     clean separation of signal and noise only in the common mid-
     point  and  common  reflection  point  (MBS) domains. (P. J.
     Singer).


NOTE 3:

     Considerable care  must  be  taken  in  applying  the  radon
     transform,  yet  preserving  subtle AVO effects. Even if the
     desired events are flat, the p=0 moveout coefficient is only
     able  to model a constant amplitude component of this event.
     Other positive and/or negative p coefficients are needed  to
     model  the observed AVO variation. Rejecting these essential
     components of AVO in a  multiple  elimination  process  will
     also  wipe out the desired AVO effect! Thus, even if primary
     events are flattened in CMP or CRP data, it is necessary  to
     model  negative  moveouts  by  setting  $mmin<=-T$,  where T
     =1/f1. For example, if f1=5Hz, set $mmin<=-200msec$.  (N. C.
     Allegar).


NOTE 4:

     The flow  rwindow -ntr1 -npad5 |radonf -semb |radonr|rwindow
     -R   can  be used to significantly increase the coherency of
     post stack data.


NOTE 5:

     The       flow         rwindow        -ntr200        -npad21
     |radonf|taupred|radonr|rwindow -R  can be used in post stack
     suppression of dipping multiples.


NOTE 6 STOLEN HEADERS:

     In order to apply the discrete radon transform filtering  to
     3D post stack data, several trace headers need to be stolen.
     Considerable care was  taken  not  to  steal  commonly  used
     header words. Nevertheless, certain collisions may occur for
     unforseen flows. Future plans call for using the dds system,
     which will ameliorate the line header problem.

     Line header words stolen by radonf and radonr for transform in the inline direction
     (including normal shot gather, receiver gather and cmp gather transforms):

     Header keyword           variable

     Crew00                   't'
     Crew01                   'p'
     Crew02                   moveout ('L','P',or 'H')
     MnUHTm                   ntr (number of input traces)
     MxUHTm                   nfft (length of FFT)
     TmMsFS                   f1
     MutVel                   f4
     NmSpMi                   df
     MxRSEL                   zref
     MnGrEl                   mmin
     MxGrEl                   mmax
     MxTrOf                   xmax
     MxTrSt                   ist

     Trace header words stolen by radonf and radonr for transform in the inline direction:

     RedVel                   apparent velocity in ms/m (ms/ft).
     DstUsg                   p*dt*1.e+07 (for use in routine taupred)
     TVPT20 and TVPV20        p (as a floating point for use in routine mute3D)
     TVPT19                   x (inline distance as found in input word DstSgn)
     MulSkw                   muteend (first non-zero sample of input data used to restore early mute)
     StaCor                   dead trace flag 30000 changed to 30001
                              transform of dead trace flag 30001 changed to 30002
                              this allows pred and taupred to work
                              operation reversed on inverse transform

     Line header words stolen by radonf and radonr for transform in the crossline direction
     invoked by using the -Y option above:

     Header keyword           variable

     Crew00                   't'
     Crew03                   'q'
     Crew04                   moveout ('L','P',or 'H')
     MnShDp                   ntr (number of input traces)
     MxShDp                   nfft (length of FFT)
     TmMsSl                   f1*1.e+06
     TmSlIn                   f4*1.e+06
     AERcPr                   df*1.e+06
     IndAdj                   zref
     MnSPEl                   mmin
     MxSPEl                   mmax
     MnTrOf                   xmax
     MnTrSt                   ist

     Trace header words stolen by radonf and radonr for transform in the crossline direction:

     DstUsg                   q*dt*1.e+07 (for use in routine taupred)
     TVPtsemb21 and TVPV21        q (as a floating point for use in routine mute3D)
     TVPV19                   y (crossline distance as found in input word DstSgn)
     PREPIn                   muteend (first non-zero sample of input data used to restore early mute)
     StaCor                   dead trace flag 30000 changed to 30001
                              transform of dead trace flag 30001 changed to 30002
                              this allows pred and taupred to work
                              operation reversed on inverse transform

     Line header words stolen by rwindow in generating running window in the inline direction
     (default mode in rwindow):

     Header keyword           variable

     RATFld                   npad
     OpGrFl                   nline (number of lines in the inline direction)
     OrNREC                   nrec_inline (number of inline windowed records)
     OrNTRC                   ntrpline (number of inline traces of original unwindowed line)
     RATTrc                   ntrcumpads (ntr+2*npad)

     Line header words stolen by rwindow in generating running window in the
     Icrossline direction
     (invoked by using the -Y option in rwindow):

     Header keyword           variable

     FrstSP                   npad
     DpN1SP                   nline (number of lines in the crossline direction)
     NmDpIn                   nrec_inline (number of crossline windowed records)
     NTrLnS                   ntrpline (number of crossline traces of original unwindowed line)
     StWdFl                   ntrcumpads (ntr+2*npad)




NOTE 7:

     Weighting/Muting the results of the transform  according  to
     the semblance.  To weight (mute) the transformed data by the
     semblance along the entire moveout curves, simply supply the
     -sigma1  and  -sigma2 values.  See Marfurt and Cottle (1994)
     for examples.



NOTE 8:

     Weighting the transform with running semblance  To  apply  a
     running  semblance  weight  to  the  data  as  it  is  being
     transformed, supply the -sembwx and -sembwt options as  well
     as  the -sigma1 and -sigma2 values above. To avoid articacts
     that may arise, the user should  compare  the  results  with
     those  obtained  by  the conventional $( tau ,p) $ transform
     obtaining by invoking the -taup option. See Marfurt and Vas-
     siliou (1994) for examples.



REFERENCES

     Marfurt, K. J., Schneider, R. V. and Mueller, M.  C.,  1994,
     Challenges  in  seismic  processing  of irregularly sampled,
     finte aperture aliased data using discrete Radon $( tau  ,p)
     $ transforms: APR Geos. Res. Bul. F94-G-14.

     Marfurt, K. J. and Cottle,  D.  A.  1994,  A  comparison  of
     coherency  weighted  $(  tau ,p) $ filtering: Application to
     poststack and common offset data:  APR Geos. Res. Bul.  F94-
     G-16.

     Marfurt, K. J. and Vassiliou, A. A., 1994, in press.

     Yilmaz, O. and Tanner, T. 1994, Discrete plane wave decompo-
     sition by least-squares method, Geophysics: 59, 973-982.

     Stoffa, P. L., Buhl, P. Diebold, J. and  Wenzel,  F.,  1981,
     Direct  mapping  of  seismic data to the domain of intercept
     time and ray parameter - A plane-wave decomposition: Geophy-
     sics, 46, 255-267.



BUGS

     No bugs known at present.


SEE ALSO

     radonr,polymute,taupred,rmmult,rwindow,radon3d,swfilt3d,taupf,taupr,slstkf,slstkr



AUTHORS

     Kurt J. Marfurt. Original parabolic  moveout  version  built
     upon  earlier work in routine rmmult (1992). Alpha trim mean
     option added 6/93 by K. D. Crawford. 2D  by  2D  post  stack
     processing   features   added   12/93.  Semblance  weighting
     features added 3/94. Least square DFT option added 5/94.


COPYRIGHT

     copyright 2001, Amoco Production Company
               All Rights Reserved
          an affiliate of BP America Inc.














































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