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Comparing ray/doc/man/man1/rcontrib.1 (file contents):
Revision 1.17 by greg, Sat Mar 14 16:25:46 2020 UTC vs.
Revision 1.24 by greg, Wed Oct 23 23:51:20 2024 UTC

# Line 9 | Line 9 | rcontrib - compute contribution coefficients in a RADI
9   ][
10   .B \-V
11   ][
12 + .B "\-t secs"
13 + ][
14   .B "\-c count"
15   ][
16   .B \-fo
# Line 43 | Line 45 | rtrace options
45   .B octree
46   .br
47   .B "rcontrib [ options ] \-defaults"
48 + .br
49 + .B "rcontrib \-features [feat1 ..]"
50   .SH DESCRIPTION
51   .I Rcontrib
52   computes ray coefficients
# Line 119 | Line 123 | Note that output flushing via zero-direction rays is d
123   .I \-c
124   set to zero.
125   .PP
126 + Output flushing at fixed intervals may be enabled with the
127 + .I \-x
128 + option, which specifies the number of records
129 + (-c accumulations) before each flush.
130 + If the
131 + .I \-y
132 + option is also set, then periodic flushing is disabled and the
133 + output size for an RGB image is the taken from the x and y dimensions.
134 + In lieu of periodic flushing, a flush may be forced as mentioned above
135 + by sending a sample with a zero direction vector, although you
136 + must still send a full record of rays before output occurs.
137 + .PP
138 + If progress reports are desired, the
139 + .I \-t
140 + option specifies a time interval in seconds for reports sent to
141 + standard error.
142 + This requires that the number of input samples is known, meaning a
143 + .I \-y
144 + parameter has been specified.
145 + .PP
146   The output of
147   .I rcontrib
148   has many potential uses.
# Line 184 | Line 208 | and
208   .I \-o
209   options to the left of each
210   .I \-m
211 < setting are the ones used for that modifier.
211 > name are the ones used for that modifier.
212 > Any
213 > .I \-cs
214 > option changing the number of spectral color
215 > samples must appear before the first modifier.
216   The ordering of other options is unimportant, except for
217   .I \-x
218   and
# Line 302 | Line 330 | density estimates results in omitted contributions, th
330   is clamped accordingly and a warning is issued.
331   .SH EXAMPLES
332   To compute the proportional contributions from sources modified
333 < by "light1" vs. "light2" on a set of illuminance values:
333 > by "light1" vs. "light2" on a set of irradiance values:
334   .IP "" .2i
335   rcontrib \-I+ @render.opt \-o c_%s.dat \-m light1 \-m light2 scene.oct < test.dat
336   .PP
# Line 318 | Line 346 | of light1 and light2:
346   .IP "" .2i
347   pcomb \-c 100 90 75 c_light1.hdr \-c 50 55 57 c_light2.hdr > combined.hdr
348   .PP
349 < To compute an array of illuminance contributions according to a Tregenza sky:
349 > To compute an array of irradiance contributions according to a Tregenza sky:
350   .IP "" .2i
351   rcontrib \-I+ \-f tregenza.cal \-b tbin \-bn Ntbins \-o sky.dat \-m skyglow
352   \-b 0 \-o ground.dat \-m groundglow @render.opt scene.oct < test.dat
# Line 339 | Line 367 | is detected.
367   Greg Ward
368   .SH "SEE ALSO"
369   cnt(1), genklemsamp(1), getinfo(1), mkpmap(1), pcomb(1), pfilt(1),
370 < ra_rgbe(1), rcalc(1), rfluxmtx(1), rmtxop(1), rpict(1), rsensor(1),
371 < rtrace(1), total(1), vwrays(1), ximage(1)
370 > ra_rgbe(1), rcalc(1), rcomb(1), rfluxmtx(1), rmtxop(1), rpict(1),
371 > rsensor(1), rtrace(1), total(1), vwrays(1), ximage(1)
372  

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