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Comparing ray/doc/man/man1/rpict.1 (file contents):
Revision 1.5 by greg, Tue Jan 18 01:13:23 2005 UTC vs.
Revision 1.21 by rschregle, Wed May 18 12:45:55 2016 UTC

# Line 70 | Line 70 | A cylindrical panorma may be selected by setting
70   to the letter 'c'.
71   This view is like a standard perspective vertically, but projected
72   on a cylinder horizontally (like a soupcan's-eye view).
73 < Two fisheye views are provided as well; 'h' yields a hemispherical fisheye
74 < view and 'a' results in angular fisheye distortion.
73 > Three fisheye views are provided as well; 'h' yields a hemispherical fisheye
74 > view, 'a' results in angular fisheye distortion, and 's'
75 > results in a planisphere (stereographic) projection.
76   A hemispherical fisheye is a projection of the hemisphere onto a circle.
77   The maximum view angle for this type is 180 degrees.
78   An angular fisheye view is defined such that distance from the center of
79   the image is proportional to the angle from the central view direction.
80   An angular fisheye can display a full 360 degrees.
81 + A planisphere fisheye view maintains angular relationships between lines,
82 + and is commonly used for sun path analysis.
83 + This is more commonly known as a
84 + "stereographic projection," but we avoid the term here so as not to
85 + confuse it with a stereoscopic pair.
86 + A planisphere fisheye can display up to (but not including) 360 degrees,
87 + although distortion becomes extreme as this limit is approached.
88   Note that there is no space between the view type
89   option and its single letter argument.
90   .TP
# Line 152 | Line 160 | This is option is useful for generating skewed perspec
160   rendering an image a piece at a time.
161   A value of 1 means that the rendered image starts just to the right of
162   the normal view.
163 < A value of -1 would be to the left.
163 > A value of \-1 would be to the left.
164   Larger or fractional values are permitted as well.
165   .TP
166   .BI -vl \ val
# Line 263 | Line 271 | A warning about aiming failure will issued if
271   .I frac
272   is too large.
273   It is usually wise to turn off image sampling when using
274 < direct jitter by setting -ps to 1.
274 > direct jitter by setting \-ps to 1.
275   .TP
276   .BI -ds \ frac
277   Set the direct sampling ratio to
# Line 327 | 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 357 | 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.
368 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 398 | 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 472 | Line 487 | header of the ambient file.
487   .I Getinfo(1)
488   may be used to print out this information.
489   .TP
490 < .BI -ae \ mat
490 > .BI -ae \ mod
491   Append
492 < .I mat
492 > .I mod
493   to the ambient exclude list,
494   so that it will not be considered during the indirect calculation.
495   This is a hack for speeding the indirect computation by
496   ignoring certain objects.
497   Any object having
498 < .I mat
498 > .I mod
499   as its modifier will get the default ambient
500   level rather than a calculated value.
501 < Any number of excluded materials may be given, but each
501 > Any number of excluded modifiers may be given, but each
502   must appear in a separate option.
503   .TP
504 < .BI -ai \ mat
504 > .BI -ai \ mod
505   Add
506 < .I mat
506 > .I mod
507   to the ambient include list,
508   so that it will be considered during the indirect calculation.
509   The program can use either an include list or an exclude
# Line 497 | Line 512 | list, but not both.
512   .BI -aE \ file
513   Same as
514   .I \-ae,
515 < except read materials to be excluded from
515 > except read modifiers to be excluded from
516   .I file.
517   The RAYPATH environment variable determines which directories are
518   searched for this file.
519 < The material names are separated by white space in the file.
519 > The modifier names are separated by white space in the file.
520   .TP
521   .BI -aI \ file
522   Same as
523   .I \-ai,
524 < except read materials to be included from
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 -ac " pagesize"
579 + Set the photon cache page size when using out-of-core photon mapping. The
580 + photon cache reduces disk I/O incurred by on-demand loading (paging) of
581 + photons, and thus increases performance. This
582 + is expressed as a (float) multiple of the density estimate bandwidth
583 + specified with
584 + .I \-ap
585 + under the assumption that photon lookups are local to a cache page. Cache
586 + performance is sensitive to this parameter: larger pagesizes will reduce the
587 + paging frequency at the expense of higher latency when paging does occur.
588 + Sensible values are in the range 4 (default) to 16.
589 + .TP
590 + .BI -aC " cachesize"
591 + Set the total number of photons cached when using out-of-core photon
592 + mapping, taking into account the pagesize specified by
593 + .I \-ac.
594 + Note that this is approximate as the number of cache pages is rounded to
595 + the nearest prime. This allows adapting the cache to the available physical
596 + memory. In conjunction with the
597 + .I \-n
598 + option, this is the cache size
599 + .I per parallel process.
600 + Cache performance is less sensitive to this parameter,
601 + and reasonable performance can obtained with as few as 10k photons. The
602 + default is 1M. This option recognises multiplier suffixes (k = 1e3, M =
603 + 1e6), both in upper and lower case.
604 + .TP
605   .BI -me " rext gext bext"
606   Set the global medium extinction coefficient to the indicated color,
607   in units of 1/distance (distance in world coordinates).
# Line 555 | Line 648 | though the
648   .I \-dv
649   option (above) may be used to override this.
650   .TP
651 + .BR \-u
652 + Boolean switch to control uncorrelated random sampling.
653 + When "off", a low-discrepancy sequence is used, which reduces
654 + variance but can result in a dithered appearance in specular highlights.
655 + When "on", pure Monte Carlo sampling is used in all calculations.
656 + .TP
657   .BI -lr \ N
658   Limit reflections to a maximum of
659 < .I N.
659 > .I N,
660 > if N is a positive integer.
661 > If
662 > .I N
663 > is zero, then Russian roulette is used for ray
664 > termination, and the
665 > .I -lw
666 > setting (below) must be positive.
667 > If N is a negative integer, then this sets the upper limit
668 > of reflections past which Russian roulette will be used.
669 > In scenes with dielectrics and total internal reflection,
670 > a setting of 0 (no limit) may cause a stack overflow.
671   .TP
672   .BI -lw \ frac
673   Limit the weight of each ray to a minimum of
674   .I frac.
675 < During ray-tracing, a record is kept of the final contribution
676 < a ray would have to the image.
677 < If it is less then the specified minimum, the ray is not traced.
675 > During ray-tracing, a record is kept of the estimated contribution
676 > (weight) a ray would have in the image.
677 > If this weight is less than the specified minimum and the
678 > .I -lr
679 > setting (above) is positive, the ray is not traced.
680 > Otherwise, Russian roulette is used to
681 > continue rays with a probability equal to the ray weight
682 > divided by the given
683 > .I frac.
684   .TP
685   .BI -S \ seqstart
686   Instead of generating a single picture based only on the view
# Line 752 | Line 868 | Set the time between progress reports to
868   A progress report writes the number of rays traced, the percentage
869   completed, and the CPU usage to the standard error.
870   Reports are given either automatically after the specified interval,
871 < or when the process receives a continue (-CONT) signal (see
871 > or when the process receives a continue (\-CONT) signal (see
872   .I kill(1)).
873   A value of zero turns automatic reporting off.
874   .TP
# Line 766 | Line 882 | Boolean switch for warning messages.
882   The default is to print warnings, so the first appearance of
883   this option turns them off.
884   .SH EXAMPLE
885 < rpict -vp 10 5 3 -vd 1 -.5 0 scene.oct > scene.pic
885 > rpict \-vp 10 5 3 \-vd 1 \-.5 0 scene.oct > scene.hdr
886   .PP
887 < rpict -S 1 -o frame%02d.pic scene.oct < keyframes.vf
887 > rpict \-S 1 \-o frame%02d.hdr scene.oct < keyframes.vf
888 > .PP
889 > To render ambient illuminance in photon mapping mode from a global photon
890 > map global.pm via one ambient bounce, and from a caustic photon map
891 > caustic.pm:
892 > .IP "" .2i
893 > rpict -ab 1 -ap global.pm 50 -ap caustic.pm 50 -vf scene.vf scene.oct >
894 > scene.hdr
895   .SH ENVIRONMENT
896   RAYPATH         the directories to check for auxiliary files.
897   .SH FILES
898 < /usr/tmp/rtXXXXXX               common header information for picture sequence
898 > /tmp/rtXXXXXX           common header information for picture sequence
899   .br
900   rfXXXXXX                temporary name for recover file
901   .SH DIAGNOSTICS
# Line 788 | Line 911 | option.
911   .SH AUTHOR
912   Greg Ward
913   .SH "SEE ALSO"
914 < getinfo(1), lookamb(1), oconv(1), pdfblur(1), pfilt(1), pinterp(1), pmblur(1),
915 < printf(3), ra_rgbe(1), rad(1), rtrace(1), rvu(1)
914 > getinfo(1), lookamb(1), mkpmap(1), oconv(1), pdfblur(1), pfilt(1),
915 > pinterp(1), pmblur(1), printf(3), ra_rgbe(1), rad(1), rtrace(1), rvu(1)

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