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Comparing ray/doc/man/man1/mkillum.1 (file contents):
Revision 1.2 by greg, Tue Dec 9 15:59:06 2003 UTC vs.
Revision 1.12 by greg, Sun Aug 11 02:57:49 2013 UTC

# Line 5 | Line 5 | mkillum - compute illum sources for a RADIANCE scene
5   .SH SYNOPSIS
6   .B mkillum
7   [
8 + .B "\-n nprocs"
9 + ][
10   .B "rtrace options"
11   ]
12   .B octree
# Line 18 | Line 20 | light source distributions for each surface, replacing
20   secondary sources whose contributions can be computed more efficiently by
21   .I rpict(1)
22   and
23 < .I rview(1).
23 > .I rvu(1).
24   This type of optimization is most useful for windows and skylights which
25   represent concentrated sources of indirect illumination.
26   .I Mkillum
# Line 27 | Line 29 | directional distributions.
29   These are best handled respectively by the ambient calculation
30   and the secondary source types in RADIANCE.
31   .PP
32 < The arguments to
32 > If the
33 > .I \-n
34 > option is specified with a value greater than 1, multiple
35 > ray tracing processes will be used to accelerate computation on a shared
36 > memory machine.
37 > Note that there is no benefit to using more processes
38 > than there are local CPUs available to do the work.
39 > .PP
40 > Remaining arguments to
41   .I mkillum
42 < are passed directly to
42 > are interpreted as rendering options for
43   .I rtrace(1),
44 < which is used to compute the light distributions for the input surfaces.
44 > to compute the light distributions for the input surfaces.
45   These surfaces can be any combination of polygons, spheres and rings.
46   Other surfaces may be included, but
47   .I mkillum
# Line 46 | Line 56 | the file names.
56   (Note that this character must be escaped from most shells.)
57   This is necessary so
58   .I mkillum
59 < can tell where the arguments to
50 < .I rtrace(1)
59 > can tell where the rendering arguments
60   end and its own input files begin.
61   .SH VARIABLES
62   .I Mkillum
# Line 128 | Line 137 | Only produce secondary sources for surfaces modified b
137   .TP
138   .BR n
139   Do not produce any secondary sources.
140 < All input will be passed to the output unaffected.
140 > All input will be passed to the output unaffected, except any
141 > void surfaces will be removed.
142   .TP
143   .BI b =real
144   Do not produce a secondary source for a surface if its average
# Line 182 | Line 192 | will use the material type "illum" with the input surf
192   as its alternate material.
193   The default is
194   .I l-.
195 + .SH EXAMPLES
196 + The following command generates illum's corresponding to geometry
197 + in the files "it1.rad" and "it2.rad":
198 + .IP "" .3i
199 + mkillum \-ab 2 \-ad 1024 \-av .1 .1 .1 basic.oct "<" it1.rad it2.rad > illums.rad
200 + .PP
201 + The output file "illums.rad" would then be combined with the original
202 + scene geometry to create a more easily rendered composite.
203 + .SH ENVIRONMENT
204 + RAYPATH         the directories to check for auxiliary files.
205   .SH AUTHOR
206   Greg Ward
207   .SH ACKNOWLEDGEMENT
208   Work on this program was initiated and sponsored by the LESO
209   group at EPFL in Switzerland.
210   .SH "SEE ALSO"
211 < oconv(1), rad(1), rpict(1), rtrace(1), rview(1)
211 > genBSDF(1), oconv(1), rad(1), rpict(1), rtrace(1), rvu(1)

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