| 60 |
|
.IP "\fB\-apC \fIfile nphotons\fR" |
| 61 |
|
Generate a contribution photon map containing approximately |
| 62 |
|
\fInphotons\fR photons, and output to file \fIfile\fR. This may then be |
| 63 |
< |
used by \fIrcontrib(1)\fR to compute light source contributions. |
| 63 |
> |
used by \fIrcontrib(1)\fR to compute light source contributions. When used |
| 64 |
> |
with \fIrtrace(1)\fR or \fIrpict(1)\fR, contribution photon maps behave as |
| 65 |
> |
regular global photon maps and yield cumulative contributions from all light |
| 66 |
> |
sources. |
| 67 |
|
.IP |
| 68 |
|
With this option, \fImkpmap\fR uses a modified photon distribution |
| 69 |
|
algorithm that ensures all light sources contribute approximately the |
| 84 |
|
photon flux; the remaining photons are discarded as their contributions |
| 85 |
|
have been accounted for. |
| 86 |
|
.IP |
| 87 |
< |
This obviates the explicit irradiance |
| 88 |
< |
evaluation by \fIrpict(1), rtrace(1)\fR and \fIrvu(1)\fR, thus providing |
| 89 |
< |
a speedup at the expense of accuracy. The resulting error is tolerable |
| 90 |
< |
if the indirect illumination has a low gradient, as is usually the case |
| 88 |
< |
with diffuse illumination. |
| 87 |
> |
This obviates the explicit irradiance evaluation by \fIrpict(1), |
| 88 |
> |
rtrace(1)\fR and \fIrvu(1)\fR, thus providing a speedup at the expense of |
| 89 |
> |
accuracy. The resulting error is tolerable if the indirect illumination has |
| 90 |
> |
a low gradient, as is usually the case with diffuse illumination. |
| 91 |
|
|
| 92 |
|
.IP "\fB\-apD \fIpredistrib\fR" |
| 93 |
|
Photon predistribution factor; this is the fraction of \fInphotons\fR |
| 95 |
|
remaining number of photons to emit in the main pass to approximately |
| 96 |
|
yield a photon map of size \fInphotons\fR. |
| 97 |
|
.IP |
| 98 |
< |
Setting this too high may |
| 99 |
< |
yield more than \fInphotons\fR in the initial pass with highly |
| 100 |
< |
reflective geometry. Note that this value may exceed 1, which may be |
| 99 |
< |
useful if the resulting photon map size greatly deviates from |
| 98 |
> |
Setting this too high may yield more than \fInphotons\fR in the initial pass |
| 99 |
> |
with highly reflective geometry. Note that this value may exceed 1, which |
| 100 |
> |
may be useful if the resulting photon map size greatly deviates from |
| 101 |
|
\fInphotons\fR with a very low average reflectance. |
| 102 |
|
|
| 103 |
< |
.IP "\fB\-apP \fIprecomp\fR" |
| 104 |
< |
Fraction of global photons to precompute in the range ]0,1] when using the |
| 105 |
< |
\fB\-app\fR option. |
| 103 |
> |
.IP "\fB\-api \fIxmin ymin zmin xmax ymax zmax\fR" |
| 104 |
> |
Define a region of interest within which to store photons exclusively; |
| 105 |
> |
photons will only be stored within the volume bounded by the given minimum |
| 106 |
> |
and maximum coordinates. Multiple instances of this option may be specified |
| 107 |
> |
with cumulative effect to define compound regions of interest. This is |
| 108 |
> |
useful for constraining photons to only the relevant regions of a scene, but |
| 109 |
> |
may increase the photon distribution time. |
| 110 |
> |
.IP |
| 111 |
> |
\fBWARNING: this is an optimisation option for advanced users (an elite |
| 112 |
> |
group collectively known as \fIZe Ekspertz\fB) and may yield biased results. |
| 113 |
> |
Use with caution!\fR |
| 114 |
|
|
| 115 |
|
.IP "\fB\-apm \fImaxbounce\fR" |
| 116 |
< |
Maximum number of bounces (scattering events) along a photon path before |
| 117 |
< |
being considered "runaway" and terminated. Photons paths are normally |
| 109 |
< |
terminated via \fIRussian Roulette\fR, depending on their albedo. With |
| 110 |
< |
unrealistically high albedos, this is not guaranteed, and this options |
| 111 |
< |
imposes a hard limit to avoid an infinite loop. |
| 116 |
> |
Synonymous with \fB\-lr\fR for backwards compatibility. May be removed in |
| 117 |
> |
future releases. |
| 118 |
|
|
| 119 |
|
.IP "\fB\-apM \fImaxprepass\fR" |
| 120 |
|
Maximum number of iterations of the distribution prepass before terminating |
| 130 |
|
space which separates them from the emitting light source via an |
| 131 |
|
opening, or port. |
| 132 |
|
.IP |
| 133 |
< |
A typical application is daylight simulation, where a |
| 134 |
< |
fenestration acts as port to admit photons into an interior after |
| 135 |
< |
emission from an external light source. Multiple instances of this |
| 130 |
< |
option may be specified. |
| 133 |
> |
A typical application is daylight simulation, where a fenestration acts as |
| 134 |
> |
port to admit photons into an interior after emission from an external light |
| 135 |
> |
source. Multiple instances of this option may be specified. |
| 136 |
|
.IP |
| 137 |
|
Note that port objects must be defined with their surface normals |
| 138 |
|
pointing \fIinside\fR as per \fImkillum\fR convention. |
| 141 |
|
Read photon port modifiers from the file \fImodfile\fR as a more convenient |
| 142 |
|
alternative to multiple instances of \fB\-apo\fR. |
| 143 |
|
|
| 144 |
+ |
.IP "\fB\-apP \fIprecomp\fR" |
| 145 |
+ |
Fraction of global photons to precompute in the range ]0,1] when using the |
| 146 |
+ |
\fB\-app\fR option. |
| 147 |
+ |
|
| 148 |
|
.IP "\fB\-apr \fIseed\fR" |
| 149 |
< |
Seed for the random number generator. This is necessary for generating |
| 150 |
< |
different photon distributions for the same octree and photon map size. |
| 149 |
> |
Seed for the random number generator. This is useful for generating |
| 150 |
> |
different photon distributions for the same octree and photon map size, |
| 151 |
> |
notably in progressive applications. |
| 152 |
|
|
| 153 |
|
.IP "\fB\-aps \fImod\fR" |
| 154 |
|
Specifies a modifier \fImod\fR defined as \fIantimatter\fR material to act |
| 169 |
|
Read virtual receiver surface modifiers from the file \fImodfile\fR as a more |
| 170 |
|
convenient alternative to multiple instances of \fB\-aps\fR. |
| 171 |
|
|
| 172 |
+ |
.IP "\fB\-ae \fImod\fR" |
| 173 |
+ |
Add \fImod\fR to the ambient exclude list, so that it will be ignored by the |
| 174 |
+ |
photon map. Objects having \fImod\fR as their modifier will not have |
| 175 |
+ |
photons deposited on them. Multiple modifiers may be given, each as separate |
| 176 |
+ |
instances of this option. |
| 177 |
+ |
.IP |
| 178 |
+ |
\fBWARNING: this is an optimisation option for advanced users and may yield |
| 179 |
+ |
biased results. It may also significantly increase photon distribution |
| 180 |
+ |
times. Use with caution!\fR |
| 181 |
+ |
|
| 182 |
+ |
.IP "\fB\-aE \fIfile\fR" |
| 183 |
+ |
Same as \fI-ae\fR, except modifiers to be exluded are read from \fIfile\fR, |
| 184 |
+ |
separated by whitespace. The RAYPATH environment variable determines which |
| 185 |
+ |
directories are searched for this file. |
| 186 |
+ |
|
| 187 |
+ |
.IP "\fB\-ai \fImod\fR" |
| 188 |
+ |
Add \fImod\fR to the ambient include list, so that it will contribute to the |
| 189 |
+ |
photon map. Only objects having \fImod\fR as their modifier will have |
| 190 |
+ |
photons deposited on them. Multiple modifiers may be given, each as separate |
| 191 |
+ |
instances of this option. Note that the ambient include and exclude options |
| 192 |
+ |
are mutually exclusive. |
| 193 |
+ |
.IP |
| 194 |
+ |
\fBWARNING: this is an optimisation option for advanced users and may yield |
| 195 |
+ |
biased results. It may also significantly increase photon distribution |
| 196 |
+ |
times. Use with caution!\fR |
| 197 |
+ |
|
| 198 |
+ |
.IP "\fB\-aI \fIfile\fR" |
| 199 |
+ |
Same as \fI-ai\fR, except modifiers to be included are read from \fIfile\fR, |
| 200 |
+ |
separated by whitespace. The RAYPATH environment variable determines which |
| 201 |
+ |
directories are searched for this file. |
| 202 |
+ |
|
| 203 |
|
.IP "\fB\-bv\fR[\fB+\fR|\fB-\fR]" |
| 204 |
|
Toggles backface visibility; enabling this causes photons to be stored and |
| 205 |
|
possibly scattered if they strike the back of a surface, otherwise they |
| 231 |
|
inadvertently destroying the results of potentially lengthy photon |
| 232 |
|
mapping runs. |
| 233 |
|
|
| 234 |
+ |
.IP "\fB\-ld \fImaxdist\fR" |
| 235 |
+ |
Limit cumulative distance travelled by a photon along its path to |
| 236 |
+ |
\fImaxdist\fR. Photon hits within this distance will be stored, and the |
| 237 |
+ |
photon is terminated once its path length exceeds this limit. This is |
| 238 |
+ |
useful for setting radial regions of interest around emitting/reflecting |
| 239 |
+ |
geometry, but may increase the photon distribution time. |
| 240 |
+ |
.IP |
| 241 |
+ |
\fBWARNING: this is an optimisation option for advanced users (an elite |
| 242 |
+ |
group collectively known as \fIZe Ekspertz\fB) and may yield biased results. |
| 243 |
+ |
Use with caution!\fR |
| 244 |
+ |
|
| 245 |
+ |
.IP "\fB\-lr \fImaxbounce\fR" |
| 246 |
+ |
Limit number of bounces (scattering events) along a photon path to |
| 247 |
+ |
\fImaxbounce\fR before being considered "runaway" and terminated. Photons |
| 248 |
+ |
paths are normally terminated via \fIRussian Roulette\fR, depending on their |
| 249 |
+ |
albedo. With unrealistically high albedos, this is not guaranteed, and this |
| 250 |
+ |
option imposes a hard limit to avoid an infinite loop. |
| 251 |
+ |
.IP |
| 252 |
+ |
\fBWARNING: this is an optimisation option for advanced users (an elite |
| 253 |
+ |
group collectively known as \fIZe Ekspertz\fB) and may yield biased results. |
| 254 |
+ |
Use with caution!\fR |
| 255 |
+ |
|
| 256 |
|
.IP "\fB\-ma \fIralb galb balb\fR" |
| 257 |
|
Set the global scattering albedo for participating media in conjunction |
| 258 |
|
with the \fB\-apv\fR option. See \fIrpict(1)\fR for details. |
| 367 |
|
(SNF). |
| 368 |
|
|
| 369 |
|
.SH "SEE ALSO" |
| 370 |
< |
rpict(1), rtrace(1), rvu(1), rcontrib(1), |
| 371 |
< |
\fIThe RADIANCE Photon Map Manual\fR |
| 372 |
< |
|
| 370 |
> |
rpict(1), rtrace(1), rvu(1), rcontrib(1), \fIThe RADIANCE Photon Map |
| 371 |
> |
Manual\fR, \fIDevelopment and Integration of the RADIANCE Photon Map |
| 372 |
> |
Extension: Technical Report\fR |
