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Comparing ray/doc/man/man1/mkillum.1 (file contents):
Revision 1.1 by greg, Tue Mar 11 19:20:21 2003 UTC vs.
Revision 1.4 by greg, Fri Sep 17 21:43:49 2004 UTC

# Line 1 | Line 1
1 < .\" RCSid "$Id"
1 > .\" RCSid "$Id$"
2   .TH MKILLUM 1 10/6/95 RADIANCE
3   .SH NAME
4   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 > .I rtrace(1)
36 > processes will be used to accelerate computation on a shared
37 > memory machine.
38 > Note that there is no benefit to using more processes
39 > than there are local CPUs available to do the work.
40 > .PP
41 > Remaining arguments to
42   .I mkillum
43   are passed directly to
44   .I rtrace(1),
# Line 188 | Line 199 | Greg Ward
199   Work on this program was initiated and sponsored by the LESO
200   group at EPFL in Switzerland.
201   .SH "SEE ALSO"
202 < oconv(1), rad(1), rpict(1), rtrace(1), rview(1)
202 > oconv(1), rad(1), rpict(1), rtrace(1), rvu(1)

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