| 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 |
> |
In photon mapping mode (see |
| 412 |
> |
.I -ap |
| 413 |
> |
below), a positive value implies that global photon irradiance is |
| 414 |
> |
always computed via |
| 415 |
> |
.I one |
| 416 |
> |
ambient bounce. A negative value enables a preview mode that directly |
| 417 |
> |
visualises the irradiance from the global photon map without any ambient |
| 418 |
> |
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. |
| 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 |
+ |
Coefficient for maximum search radius for photon map lookups. The search |
| 564 |
+ |
radius is automatically determined based on the average photon distance to the |
| 565 |
+ |
distribution's centre of gravity, and scaled by this coefficient. Increase this |
| 566 |
+ |
value if multiple warnings about short photon lookups are issued. |
| 567 |
+ |
.TP |
| 568 |
|
.BI -me " rext gext bext" |
| 569 |
|
Set the global medium extinction coefficient to the indicated color, |
| 570 |
|
in units of 1/distance (distance in world coordinates). |
| 614 |
|
.BR \-u |
| 615 |
|
Boolean switch to control uncorrelated random sampling. |
| 616 |
|
When "off", a low-discrepancy sequence is used, which reduces |
| 617 |
< |
variance but can result in a brushed appearance in specular highlights. |
| 617 |
> |
variance but can result in a dithered appearance in specular highlights. |
| 618 |
|
When "on", pure Monte Carlo sampling is used in all calculations. |
| 619 |
|
.TP |
| 620 |
|
.BI -lr \ N |
| 621 |
|
Limit reflections to a maximum of |
| 622 |
< |
.I N. |
| 622 |
> |
.I N, |
| 623 |
> |
if N is a positive integer. |
| 624 |
|
If |
| 625 |
|
.I N |
| 626 |
|
is zero, then Russian roulette is used for ray |
| 628 |
|
.I -lw |
| 629 |
|
setting (below) must be positive. |
| 630 |
|
If N is a negative integer, then this sets the upper limit |
| 631 |
< |
of reflections past which Russian roulette will not be used. |
| 631 |
> |
of reflections past which Russian roulette will be used. |
| 632 |
|
In scenes with dielectrics and total internal reflection, |
| 633 |
|
a setting of 0 (no limit) may cause a stack overflow. |
| 634 |
|
.TP |
| 845 |
|
The default is to print warnings, so the first appearance of |
| 846 |
|
this option turns them off. |
| 847 |
|
.SH EXAMPLE |
| 848 |
< |
rpict \-vp 10 5 3 \-vd 1 \-.5 0 scene.oct > scene.pic |
| 848 |
> |
rpict \-vp 10 5 3 \-vd 1 \-.5 0 scene.oct > scene.hdr |
| 849 |
|
.PP |
| 850 |
< |
rpict \-S 1 \-o frame%02d.pic scene.oct < keyframes.vf |
| 850 |
> |
rpict \-S 1 \-o frame%02d.hdr scene.oct < keyframes.vf |
| 851 |
> |
.PP |
| 852 |
> |
To render ambient illuminance in photon mapping mode from a global photon |
| 853 |
> |
map global.pm via one ambient bounce, and from a caustic photon map |
| 854 |
> |
caustic.pm: |
| 855 |
> |
.IP "" .2i |
| 856 |
> |
rpict -ab 1 -ap global.pm 50 -ap caustic.pm 50 -vf scene.vf scene.oct > |
| 857 |
> |
scene.hdr |
| 858 |
|
.SH ENVIRONMENT |
| 859 |
|
RAYPATH the directories to check for auxiliary files. |
| 860 |
|
.SH FILES |
| 874 |
|
.SH AUTHOR |
| 875 |
|
Greg Ward |
| 876 |
|
.SH "SEE ALSO" |
| 877 |
< |
getinfo(1), lookamb(1), oconv(1), pdfblur(1), pfilt(1), pinterp(1), pmblur(1), |
| 878 |
< |
printf(3), ra_rgbe(1), rad(1), rtrace(1), rvu(1) |
| 877 |
> |
getinfo(1), lookamb(1), mkpmap(1), oconv(1), pdfblur(1), pfilt(1), |
| 878 |
> |
pinterp(1), pmblur(1), printf(3), ra_rgbe(1), rad(1), rtrace(1), rvu(1) |
| 879 |
> |
|
