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.TH PMAPDUMP 1 "$Date$ $Revision$" RADIANCE |
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.SH NAME |
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pmapdump - generate RADIANCE scene description of photon map distribution |
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pmapdump - generate RADIANCE scene description or point list representing |
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photon positions and (optionally) flux |
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.SH SYNOPSIS |
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pmapdump [\fB-n\fR \fInspheres1\fR] [\fB-r\fR \fIradscale1\fR] |
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[\fB-c\fR \fIrcol1\fR \fIgcol1\fR \fIbcol1\fR] \fIpmap1\fR |
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[\fB-n\fR \fInspheres2\fR] [\fB-r\fR \fIradscale2\fR] |
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[\fB-c\fR \fIrcol2\fR \fIgcol2\fR \fIbcol2\fR] \fIpmap2\fR ... |
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pmapdump [\fB-a\fR] [\fB-n\fR \fInum1\fR] [\fB-r\fR \fIradscale1\fR] |
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[\fB-f\fR | \fB-c\fR \fIrcol1\fR \fIgcol1\fR \fIbcol1\fR] |
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\fIpmap1\fR |
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[\fB-a\fR] [\fB-n\fR \fInum2\fR] [\fB-r\fR \fIradscale2\fR] |
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[\fB-f\fR | \fB-c\fR \fIrcol2\fR \fIgcol2\fR \fIbcol2\fR] |
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\fIpmap2\fR ... |
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.SH DESCRIPTION |
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\fIpmapdump\fR takes one or more photon map files generated with |
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\fImkpmap(1)\fR as input and sends a RADIANCE scene description of their |
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photon distributions to the standard output. This can be visualised with |
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e.g. \fIobjview(1)\fR, \fIrpict(1)\fR, or \fIrvu(1)\fR to assess the |
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location and local density of photons in relation to the scene geometry. |
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\fImkpmap(1)\fR as input and, by default, sends a RADIANCE scene description |
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of their photon distributions to the standard output. Photons are |
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represented as spheres of material type \fIglow\fR. These can be |
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visualised with e.g. \fIobjview(1)\fR, \fIrpict(1)\fR, or \fIrvu(1)\fR to |
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assess the location and local density of photons in relation to the scene |
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geometry. No additional light sources are necessary, as the spheres |
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representing the photons are self-luminous. |
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.PP |
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Alternatively, photons can also be output as an ASCII point list, where |
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each line contains a photon's position and colour. |
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This point list can be imported in a 3D point cloud processor/viewer |
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to interactively explore the photon map. |
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.PP |
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An arbitrary number of photon maps can be specified on the command line and |
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the respective photon type is determined automagically. The different |
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photon types are visualised as colour coded spheres according to the |
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following default schema: |
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the respective photon type is determined automagically. Per default, the |
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different photon types are visualised as colour coded spheres/points |
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according to the following default schema: |
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.IP |
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\fIBlue\fR: global photons |
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.br |
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\fIYellow\fR: contribution photons |
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.PP |
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These colours can be overridden for individual photon maps with the \fB-c\fR |
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option (see below). |
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option (see below). Alternatively, photons can be individually coloured |
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according to their actual RGB flux with the \fB-f\fR option (see below); |
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while this makes it difficult to discern photon types, it can be used to |
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quantitatively analyse colour bleeding effects, for example. |
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.SH OPTIONS |
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Options are effective for the photon map file immediately following on the |
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command line, and are reset to their defaults after completion of each dump. |
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As such they may be set individually for each photon map. |
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As such they must be set individually for each photon map. |
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.IP "\fB-n \fInspheres\fR" |
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Specifies the number of spheres to dump for the next photon map. The dump |
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is performed by random sampling with \fInspheres\fR as target count, hence |
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the number actually output will be approximate. \fINspheres\fR may be |
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followed by a multiplier suffix for convenience, where \fIk\fR = 10^3 and |
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\fIm\fR = 10^6, although the latter may lead to problems when processing the |
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output geometry with \fIoconv(1)\fR. The default number of spheres is 10k. |
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.IP "\fB-a\fR" |
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Boolean switch to output photons as a point list in ASCII (text) format |
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instead of a RADIANCE scene. |
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Each output line consists of 6 tab-separated floating point values: the |
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X, Y, Z coordinates of the photon's position, and the R, G, B colour |
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channels of its flux. These values. notably the flux, are expressed in |
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scientific notation if necessary to accommodate their high dynamic range. |
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.IP |
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As \fIpmapdump\fR groups its options per photon map, this option must be |
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specified per photon map for consistent output. This prevents erroneously |
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dumping RADIANCE scene descriptions along with point lists, which will |
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fail to load in the 3D point cloud processor/viewer. |
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.IP "\fB-c\fR \fIrcol\fR \fIgcol\fR \fIbcol\fR" |
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Specifies a custom sphere/point colour for the next photon map. The colour |
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is specified as an RGB triplet, with each component in the range (0..1]. |
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Without this option, the default colour for the corresponding photon type |
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is used. This option is mutually exclusive with \fB-f\fR. |
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.IP "\fB-f\fR" |
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Boolean switch to colour each sphere/point according to the corresponding |
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photon's RGB flux instead of a constant colour. The flux is adjusted for |
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the fraction of dumped photons to maintain the total flux contained in the |
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dumped photon map. Note that no exposure is applied, and as such the |
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resulting colours can span several orders of magnitude and may require tone |
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mapping with \fIpcond(1)\fR for visualisation. This option is mutually |
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exclusive with \fB-c\fR. |
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.IP "\fB-n \fInum\fR" |
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Specifies the number of spheres or points to dump for the next photon map. |
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The dump is performed by random sampling with \fInum\fR as target count, |
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hence the number actually output will be approximate. \fINum\fR may be |
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suffixed by a case-insensitive multiplier for convenience, where |
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\fIk\fR = 10^3 and \fIm\fR = 10^6, although the latter may lead to problems |
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when processing the output geometry with \fIoconv(1)\fR. The default number |
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is 10k. |
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.IP "\fB-r \fIradscale\fR" |
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Specifies a relative scale factor \fIradscale\fR for the sphere radius. The |
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sphere radius is determined automatically from an estimated average distance |
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between spheres so as to reduce clustering, assuming a uniform distribution. |
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In cases where the distribution is substantially nonuniform (e.g. highly |
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In cases where the distribution is substantially nonuniform (e.g. highly |
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localised caustics) the radius can be manually corrected with this option. |
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The default value is 1.0. |
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The default value is 1.0. This option is ignored for point list output |
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in conjuction with \fB-a\fR. |
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.IP "\fB-c\fR \fIrcol\fR \fIgcol\fR \fIbcol\fR" |
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Specifies a custom sphere colour for the next photon map. The colour is |
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specified as an RGB triplet, with each component in the range (0..1]. |
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Without this option, the default colour for the corresponding photon type |
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is used. |
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.SH NOTES |
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The output may contain many overlapping spheres in areas with high photon |
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density, particularly in caustics. This results in inefficient and slow |
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octree generation with \fIoconv(1)\fR. Generally this can be improved by |
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reducing \fInspheres\fR and/or \fIradscale\fR. |
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The RADIANCE scene output may contain many overlapping spheres in areas with |
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high photon density, particularly in caustics. This results in inefficient |
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and slow octree generation with \fIoconv(1)\fR. Generally this can be |
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improved by reducing \fInum\fR and/or \fIradscale\fR. |
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.SH EXAMPLES |
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To visualise the distribution of global and caustic photons superimposed |
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Visualise the distribution of global and caustic photons superimposed |
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on the scene geometry with 5000 pale red and 10000 pale blue spheres, |
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respectively: |
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.IP |
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pmapdump -n 5k -c 1 0.4 0.4 global.pm -n 10k -c 0.4 0.4 1 caustic.pm | |
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oconv - scene.rad > scene_pmdump.oct |
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oconv - scene.rad > scene_pm.oct |
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.PP |
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Alternatively, the dump may be viewed on its own by piping the output of |
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\fIpmapdump\fR directly into \fIobjview(1)\fR (using the default number of |
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spheres in this example): |
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Visualise the caustic photon distribution superimposed on the scene geometry |
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with 10000 spheres coloured according to the photons' respective RGB flux: |
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.IP |
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pmapdump -n 10k -f caustic.pm | oconv - scene.rad > scene_pm.oct |
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.PP |
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But Capt. B wants 'em bigger: |
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.IP |
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pmapdump -r 4.0 bonzo.pm > bonzo_bigballz.rad |
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.PP |
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RADIANCE scene dumps may also be viewed on their own by simply piping the |
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output of \fIpmapdump\fR directly into \fIobjview(1)\fR (using the default |
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number of spheres in this example): |
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.IP |
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pmapdump zombo.pm | objview |
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.PP |
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Instead of a RADIANCE scene, dump photons as a (really long) point list to |
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an ASCII file for import into a 3D point cloud processor/viewer: |
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.IP |
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pmapdump -a -f -n 1m lotsa.pm > lotsa_pointz.txt |
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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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(c) Fraunhofer Institute for Solar Energy Systems, |
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.br |
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(c) Lucerne University of Applied Sciences and Arts, |
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(c) Tokyo University of Science. |
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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 ACKNOWLEDGEMENTS |
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Development of the RADIANCE photon mapping extension was supported by: |
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.RS |
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\fIFraunhofer Institute for Solar Energy Systems\fR |
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funded by |
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the German Research Foundation (\fIDFG LU204/10-2\fR, "Fassadenintegrierte |
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Regelsysteme (FARESYS)"), |
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\fILucerne University of Applied Sciences and Arts\fR |
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funded by |
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the Swiss National Science Foundation (\fISNSF 147053\fR, "Daylight redirecting components"), |
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\fITokyo University of Science\fR |
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funded by the JSPS Grants-in-Aid for Scientific |
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Research Programme (\fIKAKENHI JP19KK0115\fR, "Three-dimensional light flow"). |
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.RE |
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Many thanks also to the many individuals who tested the code and provided |
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valuable feedback. Special greetz to Don Gregorio, PAB and Capt.\~B! |
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.SH "SEE ALSO" |
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mkpmap(1), objview(1), oconv(1), rpict(1), rvu(1), |
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\fIThe RADIANCE Photon Map Manual\fR |
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.br |
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\fIThe RADIANCE Photon Map Manual\fR, |
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.br |
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\fIDevelopment and Integration of the RADIANCE Photon Map Extension: |
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Technical Report\fR, |
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.br |
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\fIThe RADIANCE Out-of-Core Photon Map: Technical Report\fR, |
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.br |
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\fIBonzo Daylighting Tool a.k.a. EvilDRC [TM]\fR |
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