335 |
|
.I \-i |
336 |
|
option so that light sources do not appear in the output. |
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 |
|
This may be desirable when used in combination with image sampling |
365 |
|
.TP |
366 |
|
.BR -bv |
367 |
|
Boolean switch for back face visibility. |
368 |
< |
With this switch off, back faces of opaque objects will be invisible |
369 |
< |
to all rays. |
368 |
> |
With this switch off, back faces of all objects will be invisible |
369 |
> |
to view rays. |
370 |
|
This is dangerous unless the model was constructed such that |
371 |
< |
all surface normals on opaque objects face outward. |
371 |
> |
all surface normals face outward. |
372 |
|
Although turning off back face visibility does not save much |
373 |
|
computation time under most circumstances, it may be useful as a |
374 |
|
tool for scene debugging, or for seeing through one-sided walls from |
375 |
|
the outside. |
376 |
– |
This option has no effect on transparent or translucent materials. |
376 |
|
.TP |
377 |
|
.BI -av " red grn blu" |
378 |
|
Set the ambient value to a radiance of |
405 |
|
.BI -ab \ N |
406 |
|
Set the number of ambient bounces to |
407 |
|
.I N. |
408 |
< |
This is the maximum number of diffuse bounces |
409 |
< |
computed by the indirect calculation. |
410 |
< |
A value of zero implies no indirect calculation. |
408 |
> |
This is the maximum number of diffuse bounces computed by the indirect |
409 |
> |
calculation. A value of zero implies no indirect calculation. |
410 |
> |
.IP |
411 |
> |
This value defaults to 1 in photon mapping mode (see |
412 |
> |
.I -ap |
413 |
> |
below), implying that global photon irradiance is always computed via |
414 |
> |
.I one |
415 |
> |
ambient bounce; this behaviour applies to any positive number of ambient |
416 |
> |
bounces, regardless of the actual value specified. A negative value enables |
417 |
> |
a preview mode that directly visualises the irradiance from the global |
418 |
> |
photon map without any ambient bounces. |
419 |
|
.TP |
420 |
|
.BI -ar \ res |
421 |
|
Set the ambient resolution to |
524 |
|
except read modifiers to be included from |
525 |
|
.I file. |
526 |
|
.TP |
527 |
+ |
.BI -ap " file [bwidth1 [bwidth2]]" |
528 |
+ |
Enable photon mapping mode. Loads a photon map generated with |
529 |
+ |
.I mkpmap(1) |
530 |
+ |
from |
531 |
+ |
.I file, |
532 |
+ |
and evaluates the indirect irradiance depending on the photon type |
533 |
+ |
(automagically detected) using density estimates with a bandwidth of |
534 |
+ |
.I bwidth1 |
535 |
+ |
photons, or the default bandwidth if none is specified (a warning will be |
536 |
+ |
issued in this case). |
537 |
+ |
.IP |
538 |
+ |
Global photon irradiance is evaluated as part of the ambient calculation (see |
539 |
+ |
.I \-ab |
540 |
+ |
above), caustic photon irradiance is evaluated at primary rays, and |
541 |
+ |
indirect inscattering in |
542 |
+ |
.I mist |
543 |
+ |
is accounted for by volume photons. Contribution photons are treated as |
544 |
+ |
global photons by |
545 |
+ |
.I rpict. |
546 |
+ |
.IP |
547 |
+ |
Additionally specifying |
548 |
+ |
.I bwidth2 |
549 |
+ |
enables bias compensation for the density estimates with a |
550 |
+ |
minimum and maximum bandwidth of |
551 |
+ |
.I bwidth1 |
552 |
+ |
and |
553 |
+ |
.I bwidth2, |
554 |
+ |
respectively. |
555 |
+ |
.IP |
556 |
+ |
Global photon irradiance may be optionally precomputed by |
557 |
+ |
.I mkpmap(1), |
558 |
+ |
in which case the bandwidth, if specified, is ignored, as the nearest photon |
559 |
+ |
is invariably looked up. |
560 |
+ |
.IP |
561 |
+ |
Using direct photons replaces the direct calculation with density estimates |
562 |
+ |
for debugging and validation of photon emission. |
563 |
+ |
.TP |
564 |
+ |
.BI -am " frac" |
565 |
+ |
Maximum search radius for photon map lookups. Without this option, an |
566 |
+ |
initial maximum search radius is estimated for each photon map from the |
567 |
+ |
average photon distance to the distribution's centre of gravity. It is then |
568 |
+ |
adapted to the photon density in subsequent lookups. This option imposes a |
569 |
+ |
global fixed maximum search radius for |
570 |
+ |
.I all |
571 |
+ |
photon maps, thus defeating the automatic adaptation. It is useful when |
572 |
+ |
multiple warnings about short photon lookups are issued. Note that this |
573 |
+ |
option does not conflict with the bandwidth specified with the |
574 |
+ |
.I \-ap |
575 |
+ |
option; the number of photons found will not exceed the latter, but may be |
576 |
+ |
lower if the maximum search radius contains fewer photons, thus resulting in |
577 |
+ |
short lookups. Setting this radius too large, on the other hand, may |
578 |
+ |
degrade performance. |
579 |
+ |
.TP |
580 |
+ |
.BI -ac " pagesize" |
581 |
+ |
Set the photon cache page size when using out-of-core photon mapping. The |
582 |
+ |
photon cache reduces disk I/O incurred by on-demand loading (paging) of |
583 |
+ |
photons, and thus increases performance. This |
584 |
+ |
is expressed as a (float) multiple of the density estimate bandwidth |
585 |
+ |
specified with |
586 |
+ |
.I \-ap |
587 |
+ |
under the assumption that photon lookups are local to a cache page. Cache |
588 |
+ |
performance is sensitive to this parameter: larger pagesizes will reduce the |
589 |
+ |
paging frequency at the expense of higher latency when paging does occur. |
590 |
+ |
Sensible values are in the range 4 (default) to 16. |
591 |
+ |
.TP |
592 |
+ |
.BI -aC " cachesize" |
593 |
+ |
Set the total number of photons cached when using out-of-core photon |
594 |
+ |
mapping, taking into account the pagesize specified by |
595 |
+ |
.I \-ac. |
596 |
+ |
Note that this is approximate as the number of cache pages is rounded to |
597 |
+ |
the nearest prime. This allows adapting the cache to the available physical |
598 |
+ |
memory. In conjunction with the |
599 |
+ |
.I \-n |
600 |
+ |
option, this is the cache size |
601 |
+ |
.I per parallel process. |
602 |
+ |
Cache performance is less sensitive to this parameter, |
603 |
+ |
and reasonable performance can obtained with as few as 10k photons. The |
604 |
+ |
default is 1M. This option recognises multiplier suffixes (k = 1e3, M = |
605 |
+ |
1e6), both in upper and lower case. |
606 |
+ |
.TP |
607 |
|
.BI -me " rext gext bext" |
608 |
|
Set the global medium extinction coefficient to the indicated color, |
609 |
|
in units of 1/distance (distance in world coordinates). |
653 |
|
.BR \-u |
654 |
|
Boolean switch to control uncorrelated random sampling. |
655 |
|
When "off", a low-discrepancy sequence is used, which reduces |
656 |
< |
variance but can result in a brushed appearance in specular highlights. |
656 |
> |
variance but can result in a dithered appearance in specular highlights. |
657 |
|
When "on", pure Monte Carlo sampling is used in all calculations. |
658 |
|
.TP |
659 |
|
.BI -lr \ N |
660 |
|
Limit reflections to a maximum of |
661 |
< |
.I N. |
661 |
> |
.I N, |
662 |
> |
if N is a positive integer. |
663 |
|
If |
664 |
|
.I N |
665 |
|
is zero, then Russian roulette is used for ray |
666 |
|
termination, and the |
667 |
|
.I -lw |
668 |
|
setting (below) must be positive. |
669 |
< |
If N is a negative integer, then this sets the upper limit |
670 |
< |
of reflections past which Russian roulette will not be used. |
669 |
> |
If N is a negative integer, then this limits the maximum |
670 |
> |
number of reflections even with Russian roulette. |
671 |
|
In scenes with dielectrics and total internal reflection, |
672 |
|
a setting of 0 (no limit) may cause a stack overflow. |
673 |
|
.TP |
884 |
|
The default is to print warnings, so the first appearance of |
885 |
|
this option turns them off. |
886 |
|
.SH EXAMPLE |
887 |
< |
rpict \-vp 10 5 3 \-vd 1 \-.5 0 scene.oct > scene.pic |
887 |
> |
rpict \-vp 10 5 3 \-vd 1 \-.5 0 scene.oct > scene.hdr |
888 |
|
.PP |
889 |
< |
rpict \-S 1 \-o frame%02d.pic scene.oct < keyframes.vf |
889 |
> |
rpict \-S 1 \-o frame%02d.hdr scene.oct < keyframes.vf |
890 |
> |
.PP |
891 |
> |
To render ambient illuminance in photon mapping mode from a global photon |
892 |
> |
map global.pm via one ambient bounce, and from a caustic photon map |
893 |
> |
caustic.pm: |
894 |
> |
.IP "" .2i |
895 |
> |
rpict -ab 1 -ap global.pm 50 -ap caustic.pm 50 -vf scene.vf scene.oct > |
896 |
> |
scene.hdr |
897 |
|
.SH ENVIRONMENT |
898 |
|
RAYPATH the directories to check for auxiliary files. |
899 |
|
.SH FILES |
913 |
|
.SH AUTHOR |
914 |
|
Greg Ward |
915 |
|
.SH "SEE ALSO" |
916 |
< |
getinfo(1), lookamb(1), oconv(1), pdfblur(1), pfilt(1), pinterp(1), pmblur(1), |
917 |
< |
printf(3), ra_rgbe(1), rad(1), rtrace(1), rvu(1) |
916 |
> |
getinfo(1), lookamb(1), mkpmap(1), oconv(1), pdfblur(1), pfilt(1), |
917 |
> |
pinterp(1), pmblur(1), printf(3), ra_rgbe(1), rad(1), rpiece(1), rtpict(1), rtrace(1), rvu(1) |