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Comparing ray/doc/man/man1/rtrace.1 (file contents):
Revision 1.12 by greg, Mon Jun 13 20:07:55 2005 UTC vs.
Revision 1.25 by greg, Sat Jan 25 18:27:39 2014 UTC

# Line 30 | Line 30 | Input for each ray is:
30   If the direction vector is (0,0,0), a bogus record
31   is printed and the output is flushed if the
32   .I -x
33 < value is unset or zero.
33 > value is one or zero.
34   (See the notes on this option below.)\0
35   This may be useful for programs that run
36   .I rtrace
# Line 87 | Line 87 | d      direction (normalized)
87   .IP
88   v       value (radiance)
89   .IP
90 + V       contribution (radiance)
91 + .IP
92   w       weight
93   .IP
94   W       color coefficient
# Line 178 | Line 180 | option (below) may be used to override this.
180   This option is especially useful in
181   conjunction with ximage(1) for computing illuminance at scene points.
182   .TP
183 < .BR \-R
184 < Boolean switch to control random sampling.
183 > .BR \-u
184 > Boolean switch to control uncorrelated random sampling.
185   When "off", a low-discrepancy sequence is used, which reduces
186   variance but can result in a brushed appearance in specular highlights.
187   When "on", pure Monte Carlo sampling is used in all calculations.
# Line 197 | Line 199 | Set the x resolution to
199   .I res.
200   The output will be flushed after every
201   .I res
202 < input rays.
202 > input rays if
203 > .I \-y
204 > is set to zero.
205 > A value of one means that every ray will be flushed, whatever
206 > the setting of
207 > .I \-y.
208   A value of zero means that no output flushing will take place.
209   .TP
210   .BI -y \ res
# Line 228 | Line 235 | format.
235   .I \-f
236   option, above.)
237   .TP
238 + .BI -n \ nproc
239 + Execute in parallel on
240 + .I nproc
241 + local processes.
242 + This option is incompatible with the
243 + .I \-P
244 + and
245 + .I \-PP,
246 + options.
247 + Multiple processes also do not work properly with ray tree output
248 + using any of the
249 + .I \-o*t*
250 + options.
251 + There is no benefit from specifying more processes than there are
252 + cores available on the system or the
253 + .I \-x
254 + setting, which forces a wait at each flush.
255 + .TP
256   .BI -dj \ frac
257   Set the direct jittering to
258   .I frac.
# Line 310 | Line 335 | may also be desirable in conjunction with the
335   .I \-i
336   option.
337   .TP
338 < .BI -sj \ frac
339 < Set the specular sampling jitter to
340 < .I frac.
341 < This is the degree to which the highlights are sampled
342 < for rough specular materials.
343 < A value of one means that all highlights will be fully sampled
344 < using distributed ray tracing.
338 > .BI -ss \ samp
339 > Set the specular sampling to
340 > .I samp.
341 > For values less than 1, this is the degree to which the highlights
342 > are sampled for rough specular materials.
343 > A value greater than one causes multiple ray samples to be sent
344 > to reduce noise at a commmesurate cost.
345   A value of zero means that no jittering will take place, and all
346   reflections will appear sharp even when they should be diffuse.
347   .TP
# Line 336 | Line 361 | accuracy and rendering time.
361   .TP
362   .BR -bv
363   Boolean switch for back face visibility.
364 < With this switch off, back faces of opaque objects will be invisible
365 < to all rays.
364 > With this switch off, back faces of all objects will be invisible
365 > to view rays.
366   This is dangerous unless the model was constructed such that
367 < all surface normals on opaque objects face outward.
367 > all surface normals face outward.
368   Although turning off back face visibility does not save much
369   computation time under most circumstances, it may be useful as a
370   tool for scene debugging, or for seeing through one-sided walls from
371   the outside.
347 This option has no effect on transparent or translucent materials.
372   .TP
373   .BI -av " red grn blu"
374   Set the ambient value to a radiance of
# Line 523 | Line 547 | source within a given scattering volume.
547   .TP
548   .BI -lr \ N
549   Limit reflections to a maximum of
550 < .I N.
550 > .I N,
551 > if N is a positive integer.
552   If
553   .I N
554   is zero or negative, then Russian roulette is used for ray
# Line 531 | Line 556 | termination, and the
556   .I -lw
557   setting (below) must be positive.
558   If N is a negative integer, then this sets the upper limit
559 < of reflections past which Russian roulette will not be used.
559 > of reflections past which Russian roulette will be used.
560   In scenes with dielectrics and total internal reflection,
561   a setting of 0 (no limit) may cause a stack overflow.
562   .TP
# Line 610 | Line 635 | system call will share memory on a copy-on-write basis
635   .SH EXAMPLES
636   To compute radiance values for the rays listed in samples.inp:
637   .IP "" .2i
638 < rtrace -ov scene.oct < samples.inp > radiance.out
638 > rtrace \-ov scene.oct < samples.inp > radiance.out
639   .PP
640   To compute illuminance values at locations selected with the 't'
641   command of
642   .I ximage(1):
643   .IP "" .2i
644 < ximage scene.pic | rtrace -h -x 1 -i scene.oct | rcalc -e '$1=47.4*$1+120*$2+11.6*$3'
644 > ximage scene.hdr | rtrace \-h \-x 1 \-i scene.oct | rcalc \-e '$1=47.4*$1+120*$2+11.6*$3'
645   .PP
646   To record the object identifier corresponding to each pixel in an image:
647   .IP "" .2i
648 < vwrays -fd scene.pic | rtrace -fda `vwrays -d scene.pic` -os scene.oct
648 > vwrays \-fd scene.hdr | rtrace \-fda `vwrays \-d scene.hdr` \-os scene.oct
649   .PP
650   To compute an image with an unusual view mapping:
651   .IP "" .2i
652 < cnt 640 480 | rcalc -e 'xr:640;yr:480' -f unusual_view.cal | rtrace
653 < -x 640 -y 480 -fac scene.oct > unusual.pic
652 > cnt 480 640 | rcalc \-e 'xr:640;yr:480' \-f unusual_view.cal | rtrace
653 > \-x 640 \-y 480 \-fac scene.oct > unusual.hdr
654   .SH ENVIRONMENT
655   RAYPATH         the directories to check for auxiliary files.
656   .SH FILES
# Line 644 | Line 669 | option.
669   Greg Ward
670   .SH "SEE ALSO"
671   getinfo(1), lookamb(1), oconv(1), pfilt(1), pinterp(1),
672 < pvalue(1), rpict(1), rtcontrib(1), rvu(1), vwrays(1), ximage(1)
672 > pvalue(1), rpict(1), rcontrib(1), rvu(1), vwrays(1), ximage(1)

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