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.\" RCSid "$Id: mkpmap.1,v 1.5 2017/03/30 11:58:17 rschregle Exp $" |
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.TH MKPMAP 1 "$Date: 2017/03/30 11:58:17 $ $Revision: 1.5 $" RADIANCE |
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greg |
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.SH NAME |
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mkpmap - generate RADIANCE photon map |
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.SH SYNOPSIS |
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mkpmap \fB\-apg\fR|\fB\-apc\fR|\fB\-apv\fR|\fB\-apd\fR|\fB\-app\fR|\fB\-apC\fR |
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\fIfile nphotons\fR [\fIbwidth\fR] ... |
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[options] \fIoctree\fR |
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.SH DESCRIPTION |
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\fIMkpmap\fR takes a RADIANCE scene description as an octree and |
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performs Monte Carlo forward path tracing from the light sources, |
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depositing indirect ray hitpoints along with their energy (flux) as |
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"photons". The resulting localised energy distribution represents a |
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global illumination solution which is written to a file for subsequent |
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evaluation by \fIrpict(1), rtrace(1)\fR and \fIrvu(1)\fR in a backward |
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raytracing pass. The photon map(s) can be reused for multiple viewpoints |
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and sensor locations as long as the geometry remains unchanged. |
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.SH OPTIONS |
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\fIMkpmap\fR can generate different types of photon maps depending on |
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the materials present in the scene. In most cases, these can be |
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specified independently or in combination on the command line. If |
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multiple photon maps of the same type are specified, the last instance |
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takes precedence. |
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.IP "\fB\-apg \fIfile nphotons\fR" |
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Generate a global photon map containing approximately \fInphotons\fR |
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photons, and output to \fIfile\fR. This accounts for all |
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indirect illumination, from both specular and diffuse scattering, on |
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surfaces with a diffuse component. This is the most general type of |
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photon map and replaces the ambient calculation in \fIrpict(1), |
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rtrace(1)\fR and \fIrvu(1)\fR. |
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.IP "\fB\-apc \fIfile nphotons\fR" |
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Generate a separate caustic photon map containing approximately |
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\fInphotons\fR photons, and output to file \fIfile\fR. This is a |
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subset of the global photon map intended for direct visualisation at |
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primary rays, This accounts for all indirect illumination on diffuse |
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surfaces from specular scattering, which usually exhibits a large |
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gradient and requires a higher resolution than the global photon map, |
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typically containing the tenfold number of photons. |
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.IP "\fB\-apv \fIfile nphotons\fR" |
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Generate a volume photon map containing approximately \fInphotons\fR |
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photons, and output to file \fIfile\fR. These account for indirect |
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inscattering in participating media such as \fBmist\fR and complement |
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the direct inscattering computed by \fIrpict(1), rtrace(1)\fR and |
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\fIrvu(1)\fR. See also the \fB\-me\fR, \fB\-ma\fR and \fB\-mg\fR options |
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below. |
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.IP "\fB\-apd \fIfile nphotons\fR" |
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Generate a direct photon map containing approximately \fInphotons\fR |
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photons, and output to file \fIfile\fR. This only accounts for direct |
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illumination and is intended for debugging and validation of photon emission |
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from the light sources, as the quality is too low for actual rendering. |
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rschregle |
1.4 |
.IP "\fB\-apC \fIfile nphotons\fR" |
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greg |
1.1 |
Generate a contribution photon map containing approximately |
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\fInphotons\fR photons, and output to file \fIfile\fR. This may then be |
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used by \fIrcontrib(1)\fR to compute light source contributions. |
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.IP |
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With this option, \fImkpmap\fR uses a modified photon distribution |
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algorithm that ensures all light sources contribute approximately the |
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same number of photons. Each photon indexes a primary hitpoint, incident |
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direction, and emitting light source which can be used to bin |
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contributions per light source and direction. |
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.IP |
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\fIMkpmap\fR cannot generate a contribution photon map in combination with |
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others in a single run, as it uses a different distribution algorithm. Other |
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photon maps specified on the command line will be ignored. |
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.IP "\fB\-app \fIfile nphotons bwidth\fR" |
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Generate a precomputed global photon map containing a fraction of |
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\fInphotons\fR photons (specified with the \fB\-apP\fR option, see |
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below), and output to file \fIfile\fR. This is a special case of the |
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global photon map where the irradiance is evaluated for a fraction of |
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the photon positions using \fIbwidth\fR nearest photons, and stored as |
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photon flux; the remaining photons are discarded as their contributions |
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have been accounted for. |
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.IP |
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This obviates the explicit irradiance |
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evaluation by \fIrpict(1), rtrace(1)\fR and \fIrvu(1)\fR, thus providing |
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a speedup at the expense of accuracy. The resulting error is tolerable |
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if the indirect illumination has a low gradient, as is usually the case |
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with diffuse illumination. |
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.IP "\fB\-apD \fIpredistrib\fR" |
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Photon predistribution factor; this is the fraction of \fInphotons\fR |
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which are emitted in a distribution prepass in order to estimate the |
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remaining number of photons to emit in the main pass to approximately |
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yield a photon map of size \fInphotons\fR. |
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.IP |
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Setting this too high may |
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yield more than \fInphotons\fR in the initial pass with highly |
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reflective geometry. Note that this value may exceed 1, which may be |
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useful if the resulting photon map size greatly deviates from |
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\fInphotons\fR with a very low average reflectance. |
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.IP "\fB\-apP \fIprecomp\fR" |
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Fraction of global photons to precompute in the range ]0,1] when using the |
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\fB\-app\fR option. |
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.IP "\fB\-apm \fImaxbounce\fR" |
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Maximum number of bounces (scattering events) along a photon path before |
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being considered "runaway" and terminated. Photons paths are normally |
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terminated via \fIRussian Roulette\fR, depending on their albedo. With |
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unrealistically high albedos, this is not guaranteed, and this options |
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imposes a hard limit to avoid an infinite loop. |
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.IP "\fB\-apM \fImaxprepass\fR" |
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Maximum number of iterations of the distribution prepass before terminating |
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if some photon maps are still empty. This option is rarely needed as a |
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an aborted prepass indicates an anomaly in the geometry or an |
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incompatibility with the specified photon map types (see \fBNOTES\fR below). |
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.IP "\fB\-apo \fImod\fR" |
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Specifies a modifier \fImod\fR to act as a \fIphoton port\fR. All |
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objects using this modifier will emit photons directly in lieu of any |
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light sources defined with the \fIsource\fR material. This greatly |
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accelerates photon distribution in scenes where photons have to enter a |
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space which separates them from the emitting light source via an |
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opening, or port. |
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.IP |
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A typical application is daylight simulation, where a |
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fenestration acts as port to admit photons into an interior after |
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emission from an external light source. Multiple instances of this |
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option may be specified. |
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.IP |
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Note that port objects must be defined with their surface normals |
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pointing \fIinside\fR as per \fImkillum\fR convention. |
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.IP "\fB\-apO \fImodfile\fR" |
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Read photon port modifiers from the file \fImodfile\fR as a more convenient |
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alternative to multiple instances of \fB\-apo\fR. |
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.IP "\fB\-apr \fIseed\fR" |
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Seed for the random number generator. This is necessary for generating |
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different photon distributions for the same octree and photon map size. |
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.IP "\fB\-aps \fImod\fR" |
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Specifies a modifier \fImod\fR defined as \fIantimatter\fR material to act |
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rschregle |
1.2 |
as a virtual (i.e. invisible) receiver surface. Photons will be deposited on |
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greg |
1.1 |
all surfaces using this modifier, just like regular materials, but will then |
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be transferred through the surface without undergoing scattering; the |
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surface therefore does not affect the light transport and simply acts as an |
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invisible photon receiver. This is useful when photon irradiance is to be |
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evaluated at points which do not lie on regular geometry, e.g. at workplane |
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greg |
1.6 |
height with \fIrtrace\fR's \fB-I\fR option. Without this workaround, |
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greg |
1.1 |
photons would be collected from parallel but distant planes, leading to |
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underestimation. Note that photons are only deposited when incident from |
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the front side of the sensor surface, i.e. when entering the |
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\fIantimatter\fR, thus the surface normal is relevant. \fIMkpmap\fR reports |
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an error if the specified modifier is not an \fIantimatter\fR material. |
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.IP "\fB\-apS \fImodfile\fR" |
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rschregle |
1.2 |
Read virtual receiver surface modifiers from the file \fImodfile\fR as a more |
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greg |
1.1 |
convenient alternative to multiple instances of \fB\-aps\fR. |
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.IP "\fB\-bv\fR[\fB+\fR|\fB-\fR]" |
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Toggles backface visibility; enabling this causes photons to be stored and |
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possibly scattered if they strike the back of a surface, otherwise they |
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are unconditionally absorbed and discarded. |
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.IP "\fB\-dp \fIsampleres\fR" |
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Resolution for sampling the spatial emission distribution of a modified |
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light source (e.g. via \fIbrightfunc\fR), in samples per steradian. This |
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is required for numerically integrating the flux emitted by the light |
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source and for constructing a probability density function for photon |
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emission. The accuracy of photon emission from modified sources |
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therefore depends on this parameter. This parameter may need increasing |
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with complex emission distributions in combination with caustics. |
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.IP "\fB\-ds \fIpartsize\fR" |
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Light source partition size ratio; a light source object is spatially |
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partitioned to distribute the photon emission over its surface. This |
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parameter specifies the ratio of the size (per dimension) of each |
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partition to the scene cube, and may need increasing for modified light |
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sources (e.g. via \fIbrightfunc\fR) with high spatial variation. |
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.IP "\fB\-e \fIfile\fR" |
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Redirect diagnostics and progress reports to \fIfile\fR instead of the |
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console. |
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.IP "\fB\-fo\fR[\fB+\fR|\fB-\fR]" |
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Toggles overwriting of output files. By default, \fImkpmap\fR will not |
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overwrite an already existing photon map file. This is to prevent |
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inadvertently destroying the results of potentially lengthy photon |
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mapping runs. |
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.IP "\fB\-i \fIinc\fR" |
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Photon heap size increment; the photon heap is enlarged by this amount |
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when storage overflows during photon distribution. No need to fiddle |
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with this under ordinary circumstances. |
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.IP "\fB\-ma \fIralb galb balb\fR" |
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Set the global scattering albedo for participating media in conjunction |
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with the \fB\-apv\fR option. See \fIrpict(1)\fR for details. |
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.IP "\fB\-me \fIrext gext bext\fR" |
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Set the global extinction coefficient for participating media in conjunction |
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with the \fB\-apv\fR option. See \fIrpict(1)\fR for details. |
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.IP "\fB\-mg \fIgecc\fR" |
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Set the global scattering eccentricity for participating media in conjunction |
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with the \fB\-apv\fR option. See \fIrpict(1)\fR for details. |
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rschregle |
1.3 |
.IP "\fB\-n \fInproc\fR" |
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Use \fInproc\fR processes for parallel photon distribution. There is no |
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benefit in specifying more than the number of physical CPU cores available. |
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rschregle |
1.5 |
This option is currently not available on Windows. |
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rschregle |
1.3 |
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greg |
1.1 |
.IP "\fB\-t \fIinterval\fR" |
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Output a progress report every \fIinterval\fR seconds. This includes |
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statistics about the currently emitting light source (including number of |
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partitions), the total number of photons emitted, the number of each type |
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stored, the percentage of the completed pass (pre or main), and the elapsed |
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time. |
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.SH NOTES |
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.SS Parametrisation |
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\fIMkpmap\fR recognises multiplier suffixes (k = 1000, m = 1000000) to |
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facilitate the specification of \fInphotons\fR, both in upper and lower |
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case. |
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.PP |
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.SS Distribution Algorithm |
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The photon distribution algorithm estimates the number of required |
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photons to emit to arrive at the specified target count \fInphotons\fR |
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per photon map using a distribution prepass followed by a main pass. |
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As a result, \fImkpmap\fR generates the \fBapproximate\fR number of photons |
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specified, which can vary by up to 10% for typical scenes, but can be |
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higher for scenes with unusually high or low reflectance. In this case, |
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the predistribution factor \fB\-apD\fR should be increased for scenes |
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with low reflectance, and reduced for those with high reflectance. |
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.PP |
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There are situations which may prevent certain (or any) |
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photon types from being generated, depending on the light source and material |
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configuration. This typically occurs when attempting to generate a caustic |
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photon map without specular materials present in the scene, or a volume |
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photon map without participating media. Ill-configured light sources may also |
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prevent indirect rays from reaching a surface, and thus no photons being |
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deposited. In these cases, \fImkpmap\fR will make a number of distribution |
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attempts before terminating with an error. This can be adjusted with the |
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\fB\-apM\fR option. |
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.SS Material Support |
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The \fIplasfunc\fR, \fImetfunc\fR, \fItransfunc\fR, \fIbrtdfunc\fR, |
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\fIplasdata\fR, \fImetdata\fR and \fItransdata\fR materials are not |
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supported by the photon mapping extension. Use the newer \fIbsdf\fR material |
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instead. |
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.PP |
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Virtual light sources (normally enabled with the \fImirror\fR material) are |
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disabled with the photon map, as the resulting caustics are already accounted |
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for. |
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rschregle |
1.2 |
.SS Virtual Receiver Surfaces |
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greg |
1.1 |
Since photons are surface bound, the density estimate is only asymptotically |
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correct when performed at points which lie on the scene geometry. The |
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irradiance is underestimated for arbitrarily placed points when photons are |
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collected from distant surfaces. \fIMkpmap\fR offers a workaround with a |
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rschregle |
1.2 |
virtual receiver surface using the \fIantimatter\fR material; see the \fB-aps\fR |
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greg |
1.1 |
and \fB-apS\fR options for details. |
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.SH EXAMPLES |
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The following command generates a global photon map \fIbonzo.gpm\fR and a |
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caustic photon map \fIbonzo.cpm\fR containing approximately 10000 and 100000 |
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photons, respectively, with progress report every 5 seconds: |
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.IP |
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mkpmap \-apg bonzo.gpm 10k \-apc bonzo.cpm 100k -t 5 bonzo.oct |
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.PP |
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Generate a global photon map containing 80000 photons, then precompute the |
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diffuse irradiance for 1/4 of these with a bandwidth of 40 photons: |
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.IP |
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mkpmap \-app bonzo-precomp.gpm 80k 40 \-apP 0.25 bonzo.oct |
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.PP |
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Generate 1 million global photons by emitting them from external light |
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sources of type \fIsource\fR into a reference room via a fenestration |
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with modifier \fIglazingMat\fR: |
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.IP |
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mkpmap \-apg refRoom.gpm 1m \-apo glazingMat refRoom.oct |
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.PP |
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Generate a contribution photon map containing 200000 photons suitable for |
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obtaining light source contributions with \fIrcontrib(1)\fR: |
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.IP |
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rschregle |
1.4 |
mkpmap \-apC bonzo-contrib.gpm 200k bonzo.oct |
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greg |
1.1 |
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.SH BUGS |
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The focus of a spotlight source, as defined by the length of its direction |
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vector, is ignored by the photon map; photons are unconditionally emitted |
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from the light source surface, which can lead to deviations from standard |
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RADIANCE. |
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.PP |
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Light sources simply absorb incoming photons. |
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.SH AUTHOR |
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Roland Schregle (roland.schregle@{hslu.ch,gmail.com}) |
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.SH COPYRIGHT |
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(c) Fraunhofer Institute for Solar Energy Systems, Lucerne University of |
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Applied Sciences and Arts. |
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.SH ACKNOWLEDGEMENT |
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Development of the RADIANCE photon mapping extension was sponsored by the |
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German Research Foundation (DFG) and the Swiss National Science Foundation |
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(SNF). |
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.SH "SEE ALSO" |
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rpict(1), rtrace(1), rvu(1), rcontrib(1), |
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