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NAME

       cpx2ps - Produce various eps codes from complex data files.

DESCRIPTION

       cpx2ps v2.1, FMR software, Bert Kampes, (c)1999-2000 \n

       +++ WARNING: infile missing

              SYNOPSIS:

              cpx2ps -w width [-f format==cr4] [-q out==mag] [-e exp==1.0] [-s sc==1.0]

              [-l  1]  [-L alllines] [-p 1] [-P width] [-M1/1 | -F1/1] [-m mirror] [-T title] [-c
              cptname==gray] [-z size==16] [-o epsfile] [-G grdfile] [-C cptfile]  [-gKSUVZ]  [-h
              elp] [--] cpxfile

              cpxfiddle options:

       -w width
              of complexfile in complex pixels

       -f format
              of  complex  input file.  ci2|cr4|cr8 (cr4 is default) r4 now also possible, though
              it limites other options.  do not use subsampling, mirroring etc, file is cat-ed.

       -q output
              what is to be computed mag|phase|real|imag|normal (mag is default)

       -e exp compute scale*output^exp

       -s scale
              compute scale*output^exp

       -l firstline
              cut out complexfile from firstline

       -L lastline
              cut out complexfile up to lastline

       -p firstpixel cut out complexfile from firstpixel

       -P lastpixel
              cut out complexfile up to lastpixel

       -m X Y XY
              mirror option.

       -M 1/1 multilook factor in X/Y direction

       -F 1/1 subsample Factor in X/Y direction

              GMT options:

       -T title
              title to plot (one word only for now) default no title

       -c colortable name of color table (see grd2cpt)
              if -q mag then gray table is default if -q other then gray table is default

       -S     add a scale bar (psscale)

       -Z     continuous color table (grd2cpt)

       -K     Leave postscript file open after last call to GMT

       -z cm  largest size of paper

       -U     Place UNIX time stamp and filename in output

              General options:

       -g     Do not call gv to view result.

       -o     output postscript file, default=23812.eps (pid)

       -G     output grd file, default=23812.eps (pid) If specified, file is not removed  at  end
              If file exists, prompted for reuse.

       -C     output  cpt  file, default=23812.cpt (pid) If specified, file is not removed at end
              If file exists, prompted for reuse.

       -V erbose
              give verbose information

       -h elp this help

       complexfile
              inputfile, major row order pixel interleaved

              EXAMPLES:

              Generate a postscript file with phase of complex interferogram in  file  cpxint.raw
              (complex 2x4B floats) that has 998 range pixels:

              cpx2ps -w 998 -qphase -fcr4 -- cpxint.raw

              The same but with a scale bar, timestamp, and no title:

              cpx2ps -w 998 -qphase -fcr4 -Tnone -U -S -- cpxint.raw

              To  plot  the  magnitude  to  the  power  0.3 of a file in the format complex short
              integers (2x2B) use:

              cpx2ps -w 998 -qmag -fci2 -e0.3 -- cpxint.raw

              To see a large file it is convenient to set a large size (-z).  This file cannot be
              printed, but viewing it with gv is nice:

              cpx2ps -w 998 -qphase -z200 -- cpxint.raw

              To  plot the phase of a hgt file, first create a tmp file with the program hgt2file
              (hgtfile infile linelength tmpfile [ampflag]) Next,  run  cpx2ps  with  appropriate
              flags for a float file, e.g.  (Note that this limits some options in scaling etc.):

              cpx2ps -w 998 -crainbow -fr4 -- tmpfile

              BUGS:

              When mirroring and multilooking/subsampling sometimes the number of lines/pixels of
              the output is computed incorrectly. Simply don't use multilooking/subsampling...

              Please mail bugs/comments to kampes@geo.tudelft.nl

              SEE ALSO:

              cpxfiddle, GMT

       +++ WARNING: infile missing

              PROGRAM: cpx2ps -- Produce various eps codes from complex data files.

              SYNOPSIS:

              cpx2ps -w width [-f format==cr4] [-q out==mag] [-e exp==1.0] [-s sc==1.0]

              [-l 1] [-L alllines] [-p 1] [-P width] [-M1/1 | -F1/1] [-m mirror] [-T  title]  [-c
              cptname==gray]  [-z  size==16] [-o epsfile] [-G grdfile] [-C cptfile] [-gKSUVZ] [-h
              elp] [--] cpxfile

              cpxfiddle options:

       -w width
              of complexfile in complex pixels

       -f format
              of complex input file.  ci2|cr4|cr8 (cr4 is default) r4 now also  possible,  though
              it limites other options.  do not use subsampling, mirroring etc, file is cat-ed.

       -q output
              what is to be computed mag|phase|real|imag|normal (mag is default)

       -e exp compute scale*output^exp

       -s scale
              compute scale*output^exp

       -l firstline
              cut out complexfile from firstline

       -L lastline
              cut out complexfile up to lastline

       -p firstpixel cut out complexfile from firstpixel

       -P lastpixel
              cut out complexfile up to lastpixel

       -m X Y XY
              mirror option.

       -M 1/1 multilook factor in X/Y direction

       -F 1/1 subsample Factor in X/Y direction

              GMT options:

       -T title
              title to plot (one word only for now) default no title

       -c colortable name of color table (see grd2cpt)
              if -q mag then gray table is default if -q other then gray table is default

       -S     add a scale bar (psscale)

       -Z     continuous color table (grd2cpt)

       -K     Leave postscript file open after last call to GMT

       -z cm  largest size of paper

       -U     Place UNIX time stamp and filename in output

              General options:

       -g     Do not call gv to view result.

       -o     output postscript file, default=23819.eps (pid)

       -G     output  grd  file, default=23819.eps (pid) If specified, file is not removed at end
              If file exists, prompted for reuse.

       -C     output cpt file, default=23819.cpt (pid) If specified, file is not removed  at  end
              If file exists, prompted for reuse.

       -V erbose
              give verbose information

       -h elp this help

       complexfile
              inputfile, major row order pixel interleaved

              EXAMPLES:

              Generate  a  postscript file with phase of complex interferogram in file cpxint.raw
              (complex 2x4B floats) that has 998 range pixels:

              cpx2ps -w 998 -qphase -fcr4 -- cpxint.raw

              The same but with a scale bar, timestamp, and no title:

              cpx2ps -w 998 -qphase -fcr4 -Tnone -U -S -- cpxint.raw

              To plot the magnitude to the power 0.3 of  a  file  in  the  format  complex  short
              integers (2x2B) use:

              cpx2ps -w 998 -qmag -fci2 -e0.3 -- cpxint.raw

              To see a large file it is convenient to set a large size (-z).  This file cannot be
              printed, but viewing it with gv is nice:

              cpx2ps -w 998 -qphase -z200 -- cpxint.raw

              To plot the phase of a hgt file, first create a tmp file with the program  hgt2file
              (hgtfile  infile  linelength  tmpfile  [ampflag]) Next, run cpx2ps with appropriate
              flags for a float file, e.g.  (Note that this limits some options in scaling etc.):

              cpx2ps -w 998 -crainbow -fr4 -- tmpfile

              BUGS:

              When mirroring and multilooking/subsampling sometimes the number of lines/pixels of
              the output is computed incorrectly. Simply don't use multilooking/subsampling...

              Please mail bugs/comments to kampes@geo.tudelft.nl

              SEE ALSO:

              cpxfiddle, GMT

SEE ALSO

       The  full  documentation  for  cpx2ps  is maintained as a Texinfo manual.  If the info and
       cpx2ps programs are properly installed at your site, the command

              info cpx2ps

       should give you access to the complete manual.

cpx2ps v2.1, FMR software, Bert Kampes, (cSeptember02017                                CPX2PS(1)