--- ray/doc/man/man1/rtcontrib.1 2005/06/02 04:47:26 1.7 +++ ray/doc/man/man1/rtcontrib.1 2006/02/05 22:22:20 1.15 @@ -1,4 +1,4 @@ -.\" RCSid "$Id: rtcontrib.1,v 1.7 2005/06/02 04:47:26 greg Exp $" +.\" RCSid "$Id: rtcontrib.1,v 1.15 2006/02/05 22:22:20 greg Exp $" .TH RTCONTRIB 1 5/25/05 RADIANCE .SH NAME rtcontrib - compute contribution coefficients in a RADIANCE scene @@ -7,6 +7,12 @@ rtcontrib - compute contribution coefficients in a RAD [ .B "\-n nprocs" ][ +.B \-V +][ +.B \-fo +| +.B \-r +][ .B "\-e expr" ][ .B "\-f source" @@ -14,8 +20,13 @@ rtcontrib - compute contribution coefficients in a RAD .B "\-o ospec" ][ .B "\-b binv" +][ +.B "\-bn nbins" ] -.B "\-m mod .." +{ +.B "\-m mod | \-M file" +} +.. [ .B $EVAR ] @@ -30,13 +41,49 @@ rtrace options .B "rtcontrib [ options ] \-defaults" .SH DESCRIPTION .I Rtcontrib -computes ray contributions (i.e., color coefficients) +computes ray coefficients for objects whose modifiers are named in one or more .I \-m settings. These modifiers are usually materials associated with light sources or sky domes, and must directly modify some geometric primitives to be considered in the output. +A modifier list may also be read from a file using the +.I \-M +option. +The RAYPATH environment variable determines directories to search for +this file. +(No search takes place if a file name begins with a '.', '/' or '~' +character.)\0 +.PP +By setting the boolean +.I \-V +option, you may instruct +.I rtcontrib +to report the contribution from each material rather than the ray +coefficient. +This is particularly useful for light sources with directional output +distributions, whose value would otherwise be lost in the shuffle. +With the default +.I -V- +setting, the output of rtcontrib is a coefficient that must be multiplied +by the radiance of each material to arrive at a final contribution. +This is more convenient for computing daylight coefficeints, or cases +where the actual radiance is not desired. +Use the +.I -V+ +setting when you wish to simply sum together contributions +(with possible adjustment factors) to obtain a final radiance value. +Combined with the +.I \-i +or +.I \-I +option, irradiance contributions are reported by +.I \-V+ +rather than radiance, and +.I \-V- +coefficients contain an additonal factor of PI. +.PP The output of .I rtcontrib has many potential uses. @@ -51,7 +98,7 @@ systems, such as luminaires, light pipes, and shading .I Rtcontrib calls .I rtrace(1) -with the -oTW option to calculate the daughter ray +with the -oTW (or -oTV) option to calculate the daughter ray contributions for each input ray, and the output tallies are sent to one or more destinations according to the given .I \-o @@ -59,7 +106,12 @@ specification. If a destination begins with an exclamation mark ('!'), then a pipe is opened to a command and data is sent to its standard input. Otherwise, the destination is treated as a file. -(An existing file of the same name is clobbered.)\0 +An existing file of the same name will not be clobbered, unless the +.I \-fo +option is given. +If instead the +.I \-r +option is specified, data recovery is attempted on existing files. If an output specification contains a "%s" format, this will be replaced by the modifier name. The @@ -70,8 +122,16 @@ this will be applied to a "%d" format in the output fi specification if present. The actual bin number is computed at run time based on ray direction and surface intersection, as described below. +If the number of bins is known in advance, it should be specified with the +.I \-bn +option, and this is critical for output files containing multiple values +per record. +Since bin numbers start from 0, the bin count is always equal to +the last bin plus 1. +Set the this value to 0 if the bin count is unknown (the default). The most recent -.I \-b +.I \-b, +.I \-bn and .I \-o options to the left of each @@ -109,8 +169,6 @@ Unlike will search the RADIANCE library directories for each file given in a .I \-f option. -(No search takes place if a file name begins with a '.', '/' or '~' -character.)\0 .PP If no .I \-o @@ -191,10 +249,10 @@ pcomb -c 100 90 75 c_light1.pic -c 50 55 57 c_light2.p .PP To compute an array of illuminance contributions according to a Tregenza sky: .IP "" .2i -rtcontrib -b tbin -o sky.dat -m skyglow -b 0 -o ground.dat -m groundglow +rtcontrib -I+ -b tbin -o sky.dat -m skyglow -b 0 -o ground.dat -m groundglow @render.opt -f tregenza.cal scene.oct < test.dat .SH ENVIRONMENT -RAYPATH path to search for -f files +RAYPATH path to search for -f and -M files .SH AUTHOR Greg Ward .SH "SEE ALSO"