Provided by: radiance_4R1+20120125-1.1_amd64 bug

NAME

       pcond - condition a RADIANCE picture for output

SYNOPSIS

       pcond [ options ] input [ output ]

DESCRIPTION

       Pcond conditions a Radiance picture for output to a display or hard copy device.  If the dynamic range of
       the scene exceeds that of the display (as is usually the case), pcond will compress the dynamic range  of
       the  picture  such  that  both  dark and bright regions are visible.  In addition, certain limitations in
       human vision may be mimicked in order to provide an appearance similar to the experience one  might  have
       in the actual scene.

       Command line switches turn flags off and on, changing program behavior.  A switch given by itself toggles
       the flag from off to on or on to off depending on its previous state.  A switch followed by a  '+'  turns
       the  option on explicitly.  A switch followed by a '-' turns the option off.  The default is all switches
       off.  Other options specify output device parameters in order to get more accurate color and contrast.

       -h[+-]    Mimic human visual response in the output.  The goal of this process is to produce output  that
                 correlates  strongly with a person's subjective impression of a scene.  This switch is a bundle
                 of the -a, -v, -s and -c options.

       -a[+-]    Defocus darker regions of the image to simulate human visual acuity loss.  This option will not
                 affect well-lit scenes.

       -v[+-]    Add  veiling glare due to very bright regions in the image.  This simulates internal scattering
                 in the human eye, which results in a loss of visible contrast near bright sources.

       -s[+-]    Use the human contrast sensitivity function in determining  the  exposure  for  the  image.   A
                 darker scene will have relatively lower exposure with lower contrast than a well-lit scene.

       -c[+-]    If  parts  of the image are in the mesopic or scotopic range where the cone photoreceptors lose
                 their efficiency, this switch will cause a corresponding loss of color visibility in the output
                 and a shift to a scotopic (blue-dominant) response function.

       -w[+-]    Use  a  center-weighted average for the exposure rather than the default uniform average.  This
                 may improve the exposure for scenes with high or low peripheral brightness.

       -i fixfrac
                 Set the relative importance of fixation points to fixfrac, which is a value between  0  and  1.
                 If  fixfrac is zero (the default), then no fixation points are used in determining the local or
                 global adaptation.  If fixfrac is greater than zero, then a list of  fixation  points  is  read
                 from  the  standard  input.  These points are given as tab-separated (x,y) picture coordinates,
                 such as those produced by the -op option of ximage(1).  The foveal samples about these fixation
                 points  will then be weighted together with the global averaging scheme such that the fixations
                 receive fixfrac of the total weight.  If fixfrac is one, then  only  the  fixation  points  are
                 considered for adaptation.

       -I[+-]    Rather  than  computing  a  histogram  of  foveal  samples  from  the  source  picture, use the
                 precomputed histogram provided on the standard input.  This data should be given  in  pairs  of
                 the  base-10  logarithm  of  world  luminance  and  a count for each bin in ascending order, as
                 computed by the phisto(1) script.  This option is useful for producing identical  exposures  of
                 multiple  pictures  (as  in  an  animation),  and  provides  greater control over the histogram
                 computation.

       -l[+-]    Use a linear response function rather than the standard dynamic  range  compression  algorithm.
                 This will prevent the loss of usable physical values in the output picture, although some parts
                 of the resulting image may be too dark or too bright to see.

       -e expval Set the exposure adjustment for the picture to expval.  This may either be a  real  multiplier,
                 or  a  (fractional)  number of f-stops preceeded by a '+' or '-'.  This option implies a linear
                 response (see the -l option above).

       -u Ldmax  Specifies the top of the luminance range for the target output device.  That is, the  luminance
                 (in  candelas/m^2)  for  an  output  pixel  value of (R,G,B)=(1,1,1).  The default value is 100
                 cd/m^2.

       -d Lddyn  Specifies the dynamic range for the target output device, which is the ratio of the maximum and
                 minimum usable display luminances.  The default value is 32.

       -p xr yr xg yg xb yb xw yw
                 Specifies  the  RGB  primaries  for  the  target  output  device.  These are the 1931 CIE (x,y)
                 chromaticity values for red, green, blue and white, respectively.

       -f macbeth.cal
                 Use the given output file from macbethcal(1) to precorrect  the  color  and  contrast  for  the
                 target output device.  This does a more thorough job than a simple primary correction using the
                 -p option.  Only one of -f or -p may be given.

       -x mapfile
                 Put out the final mapping from world luminance to display luminance to mapfile.  This file will
                 contain  values from the minimum usable world luminance to the maximum (in candelas/m^2) in one
                 column, and their corresponding display luminance values (also in candelas/m^2) in  the  second
                 column.   This file may be used for debugging purposes, or to plot the mapping function created
                 by pcond.

EXAMPLES

       To display an image as a person might perceive it in the actual scene:

         pcond -h final.hdr > display.hdr
         ximage display.hdr ; rm display.hdr &

       To do the same on a 24-bit display with known primary values:

         setenv DISPLAY_PRIMARIES ".580 .340 .281 .570 .153 .079 .333 .333"
         pcond -h -p $DISPLAY_PRIMARIES final.hdr | ximage &

       To prepare a picture to be sent to a film recorder destined eventually  for  a  slide  projector  with  a
       minimum and maximum screen luminance of 1.5 and 125 candelas/m^2, respectively:

         pcond -d 83 -u 125 final.hdr > film.hdr

       To  do  the  same  if  the  output  colors of the standard image "ray/lib/lib/macbeth_spec.hdr" have been
       measured:

         macbethcal -c mbfilm.xyY > film.cal
         pcond -d 83 -u 125 -f film.cal final.hdr > film.hdr

       To further tweak the exposure to bring out certain areas indicated by dragging  the  right  mouse  button
       over them in ximage:

         ximage -op -t 75 final.hdr | pcond -i .5 -d 83 -u 125 -f film.cal final.hdr > film.hdr

       To use a histogram computed on every 10th animation frame:

         phisto frame*0.hdr > global.hist
         pcond -I -s -c frame0352.hdr < global.hist | ra_tiff - frame0352.tif

REFERENCE

       Greg  Ward  Larson, Holly Rushmeier, Christine Piatko, ``A Visibility Matching Tone Reproduction Operator
       for High Dynamic Range Scenes,'' IEEE Transactions on Visualization  and  Computer  Graphics  ,  December
       1997.

       http://www.sgi.com/Technology/pixformat/Larsonetal.html

AUTHOR

       Greg Ward Larson

SEE ALSO

       getinfo(1),   macbethcal(1),   normtiff(1),   pcompos(1),  pflip(1),  phisto(1),  pinterp(1),  pvalue(1),
       protate(1), ra_xyze(1), rad(1), rpict(1), ximage(1)