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Comparing ray/doc/man/man1/rpict.1 (file contents):
Revision 1.12 by greg, Tue Mar 11 02:21:45 2008 UTC vs.
Revision 1.24 by greg, Fri Jan 11 21:12:24 2019 UTC

# Line 335 | Line 335 | This option may be desirable in conjunction with the
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
# Line 365 | Line 365 | accuracy and rendering time.
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
# Line 406 | Line 405 | indirect contributions, such as when both indoor and o
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
# Line 517 | Line 524 | Same as
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).
# Line 566 | Line 653 | option (above) may be used to override this.
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
# Line 796 | Line 884 | Boolean switch for warning messages.
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
# Line 818 | Line 913 | option.
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)

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