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Comparing ray/doc/man/man1/rpict.1 (file contents):
Revision 1.16 by greg, Sat Jan 25 18:27:39 2014 UTC vs.
Revision 1.20 by rschregle, Fri Jun 5 08:49:01 2015 UTC

# Line 405 | 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 516 | 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.
544 + .IP
545 + Additionally specifying
546 + .I bwidth2
547 + enables bias compensation for the density estimates with a
548 + minimum and maximum bandwidth of
549 + .I bwidth1
550 + and
551 + .I bwidth2,
552 + respectively.
553 + .IP
554 + Global photon irradiance may be optionally precomputed by
555 + .I mkpmap(1),
556 + in which case the bandwidth, if specified, is ignored, as the nearest photon
557 + is invariably looked up.
558 + .IP
559 + Using direct photons replaces the direct calculation with density estimates
560 + for debugging and validation of photon emission.      
561 + .TP
562 + .BI -am " frac"
563 + Maximum search radius for photon map lookups.  Without this option, an
564 + initial maximum search radius is estimated for each photon map from the
565 + average photon distance to the distribution's centre of gravity.  It is then
566 + adapted to the photon density in subsequent lookups.  This option imposes a
567 + global fixed maximum search radius for
568 + .I all
569 + photon maps, thus defeating the automatic adaptation.  It is useful when
570 + multiple warnings about short photon lookups are issued.  Note that this
571 + option does not conflict with the bandwidth specified with the
572 + .I \-ap
573 + option; the number of photons found will not exceed the latter, but may be
574 + lower if the maximum search radius contains fewer photons, thus resulting in
575 + short lookups.  Setting this radius too large, on the other hand, may
576 + degrade performance.
577 + .TP
578   .BI -me " rext gext bext"
579   Set the global medium extinction coefficient to the indicated color,
580   in units of 1/distance (distance in world coordinates).
# Line 565 | Line 624 | option (above) may be used to override this.
624   .BR \-u
625   Boolean switch to control uncorrelated random sampling.
626   When "off", a low-discrepancy sequence is used, which reduces
627 < variance but can result in a brushed appearance in specular highlights.
627 > variance but can result in a dithered appearance in specular highlights.
628   When "on", pure Monte Carlo sampling is used in all calculations.
629   .TP
630   .BI -lr \ N
# Line 799 | Line 858 | this option turns them off.
858   rpict \-vp 10 5 3 \-vd 1 \-.5 0 scene.oct > scene.hdr
859   .PP
860   rpict \-S 1 \-o frame%02d.hdr scene.oct < keyframes.vf
861 + .PP
862 + To render ambient illuminance in photon mapping mode from a global photon
863 + map global.pm via one ambient bounce, and from a caustic photon map
864 + caustic.pm:
865 + .IP "" .2i
866 + rpict -ab 1 -ap global.pm 50 -ap caustic.pm 50 -vf scene.vf scene.oct >
867 + scene.hdr
868   .SH ENVIRONMENT
869   RAYPATH         the directories to check for auxiliary files.
870   .SH FILES
# Line 818 | Line 884 | option.
884   .SH AUTHOR
885   Greg Ward
886   .SH "SEE ALSO"
887 < getinfo(1), lookamb(1), oconv(1), pdfblur(1), pfilt(1), pinterp(1), pmblur(1),
888 < printf(3), ra_rgbe(1), rad(1), rtrace(1), rvu(1)
887 > getinfo(1), lookamb(1), mkpmap(1), oconv(1), pdfblur(1), pfilt(1),
888 > pinterp(1), pmblur(1), printf(3), ra_rgbe(1), rad(1), rtrace(1), rvu(1)

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