| 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 |
| 87 |
|
.IP |
| 88 |
|
v value (radiance) |
| 89 |
|
.IP |
| 90 |
+ |
V contribution (radiance) |
| 91 |
+ |
.IP |
| 92 |
|
w weight |
| 93 |
|
.IP |
| 94 |
|
W color coefficient |
| 180 |
|
This option is especially useful in |
| 181 |
|
conjunction with ximage(1) for computing illuminance at scene points. |
| 182 |
|
.TP |
| 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. |
| 188 |
+ |
.TP |
| 189 |
|
.BR \-I |
| 190 |
|
Boolean switch to compute irradiance rather than radiance, |
| 191 |
|
with the input origin and direction interpreted instead |
| 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 |
| 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. |
| 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 |
| 548 |
|
.TP |
| 549 |
|
.BI -lr \ N |
| 550 |
|
Limit reflections to a maximum of |
| 551 |
< |
.I N. |
| 551 |
> |
.I N, |
| 552 |
> |
if N is a positive integer. |
| 553 |
|
If |
| 554 |
|
.I N |
| 555 |
|
is zero or negative, then Russian roulette is used for ray |
| 557 |
|
.I -lw |
| 558 |
|
setting (below) must be positive. |
| 559 |
|
If N is a negative integer, then this sets the upper limit |
| 560 |
< |
of reflections past which Russian roulette will not be used. |
| 560 |
> |
of reflections past which Russian roulette will be used. |
| 561 |
|
In scenes with dielectrics and total internal reflection, |
| 562 |
|
a setting of 0 (no limit) may cause a stack overflow. |
| 563 |
|
.TP |
| 636 |
|
.SH EXAMPLES |
| 637 |
|
To compute radiance values for the rays listed in samples.inp: |
| 638 |
|
.IP "" .2i |
| 639 |
< |
rtrace -ov scene.oct < samples.inp > radiance.out |
| 639 |
> |
rtrace \-ov scene.oct < samples.inp > radiance.out |
| 640 |
|
.PP |
| 641 |
|
To compute illuminance values at locations selected with the 't' |
| 642 |
|
command of |
| 643 |
|
.I ximage(1): |
| 644 |
|
.IP "" .2i |
| 645 |
< |
ximage scene.pic | rtrace -h -x 1 -i scene.oct | rcalc -e '$1=47.4*$1+120*$2+11.6*$3' |
| 645 |
> |
ximage scene.hdr | rtrace \-h \-x 1 \-i scene.oct | rcalc \-e '$1=47.4*$1+120*$2+11.6*$3' |
| 646 |
|
.PP |
| 647 |
|
To record the object identifier corresponding to each pixel in an image: |
| 648 |
|
.IP "" .2i |
| 649 |
< |
vwrays -fd scene.pic | rtrace -fda `vwrays -d scene.pic` -os scene.oct |
| 649 |
> |
vwrays \-fd scene.hdr | rtrace \-fda `vwrays \-d scene.hdr` \-os scene.oct |
| 650 |
|
.PP |
| 651 |
|
To compute an image with an unusual view mapping: |
| 652 |
|
.IP "" .2i |
| 653 |
< |
cnt 640 480 | rcalc -e 'xr:640;yr:480' -f unusual_view.cal | rtrace |
| 654 |
< |
-x 640 -y 480 -fac scene.oct > unusual.pic |
| 653 |
> |
cnt 480 640 | rcalc \-e 'xr:640;yr:480' \-f unusual_view.cal | rtrace |
| 654 |
> |
\-x 640 \-y 480 \-fac scene.oct > unusual.hdr |
| 655 |
|
.SH ENVIRONMENT |
| 656 |
|
RAYPATH the directories to check for auxiliary files. |
| 657 |
|
.SH FILES |
| 670 |
|
Greg Ward |
| 671 |
|
.SH "SEE ALSO" |
| 672 |
|
getinfo(1), lookamb(1), oconv(1), pfilt(1), pinterp(1), |
| 673 |
< |
pvalue(1), rpict(1), rtcontrib(1), rvu(1), vwrays(1), ximage(1) |
| 673 |
> |
pvalue(1), rpict(1), rcontrib(1), rvu(1), vwrays(1), ximage(1) |
