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Revision 1.18 by greg, Wed Sep 9 21:28:19 2020 UTC vs.
Revision 1.21 by greg, Wed Oct 19 21:25:20 2022 UTC

# Line 45 | 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 121 | 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
# Line 309 | Line 326 | density estimates results in omitted contributions, th
326   is clamped accordingly and a warning is issued.
327   .SH EXAMPLES
328   To compute the proportional contributions from sources modified
329 < by "light1" vs. "light2" on a set of illuminance values:
329 > by "light1" vs. "light2" on a set of irradiance values:
330   .IP "" .2i
331   rcontrib \-I+ @render.opt \-o c_%s.dat \-m light1 \-m light2 scene.oct < test.dat
332   .PP
# Line 325 | Line 342 | of light1 and light2:
342   .IP "" .2i
343   pcomb \-c 100 90 75 c_light1.hdr \-c 50 55 57 c_light2.hdr > combined.hdr
344   .PP
345 < To compute an array of illuminance contributions according to a Tregenza sky:
345 > To compute an array of irradiance contributions according to a Tregenza sky:
346   .IP "" .2i
347   rcontrib \-I+ \-f tregenza.cal \-b tbin \-bn Ntbins \-o sky.dat \-m skyglow
348   \-b 0 \-o ground.dat \-m groundglow @render.opt scene.oct < test.dat

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