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Revision: 1.1
Committed: Thu Feb 25 04:48:19 2021 UTC (4 years, 3 months ago) by greg
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docs: added man page for pabopto2bsdf

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# Content
1 .\" RCSid "$Id: mgf2rad.1,v 1.3 2007/09/04 17:36:40 greg Exp $"
2 .TH PABOPTO2BSDF 1 2/24/2021 RADIANCE
3 .SH NAME
4 pabopto2bsdf - convert pab-opto BSDF measurements to scattering interpolant representation
5 .SH SYNOPSIS
6 .B pabopto2bsdf
7 [
8 .B \-t
9 ][
10 .B "\-n nproc"
11 ][
12 .B "\-s symmetry"
13 ]
14 .B "meas1 meas2 .."
15 .SH DESCRIPTION
16 .I Pabopto2bsdf
17 takes two or more pab-opto
18 .I Mountain
19 files, each corresponding
20 to a different incident beam angle, and produces a
21 Scattering Interpolant Representation (SIR)
22 on the standard output for further processing.
23 The binary SIR contains a Radial Basis Function fitting
24 each incident BSDF data file
25 and a "transport plan" between neighboring RBF
26 directions in a spherical Delaunay mesh.
27 .PP
28 The SIR provides a complete 4-dimensional
29 BSDF description that may be resampled for other
30 formats such as Klems and tensor tree.
31 However, a separate run of
32 .I pabopto2bsdf
33 is needed to produce an SIR for each
34 incident and scattered hemisphere pair.
35 At most, there will be 4 such hemisphere pairs for
36 front reflection, back reflection, front transmission,
37 and back transmission.
38 Theoretically, only one transmission direction is required,
39 but it is often safest to measure both if both directions
40 will be used in a simulation.
41 .PP
42 See
43 .I bsdf2klems(1)
44 and
45 .I bsdf2ttree(1)
46 for details.
47 The
48 .I bsdf2rad(1)
49 and
50 .I bsdfview(1)
51 tools are also useful for visualizaing SIR and XML files.
52 .PP
53 The
54 .I pabopto2bsdf
55 .I \-t
56 option reverses the assumed sample orientation front-to-back,
57 and is discussed below under the "#intheta" header entry.
58 Multi-processing may be used to accelerate the program
59 on systems that support it via the
60 .I \-n
61 option.
62 .PP
63 BSDF symmetry may be specified with the
64 .I \-s
65 option, which is one of "isotropic", "quadrilateral",
66 "bilateral", "up", or "anisotropic".
67 Any of these may be abbreviated with as little as a single
68 letter, and case is ignored.
69 .PP
70 Normally,
71 .I pabopto2bsdf
72 attempts to deduce BSDF symmetry from the incident phi angles
73 provided.
74 If every input data file uses the same incident phi angle, the
75 BSDF is assumed to be "isotropic", meaning rotationally symmetric.
76 If input phi angles only cover one quarter of the incident hemisphere,
77 then the sample is assumed to have quadrilateral symmetry.
78 Similarly, half-hemisphere coverage implies "bilateral" symmetry,
79 although it is also compatible with "up" symmetry, which must be specified
80 on the command line.
81 The difference is crucial.
82 Similar to quadrilateral symmetry, bilateral symmetry is "mirrored,"
83 meaning that the sample material looks identical when viewed in a mirror.
84 However, "up" symmetry means that the sample looks the same when
85 rotated by 180-degree (upside-down), but does not look the same in a mirror.
86 Although bilateral symmetry is a superset of "up" symmetry,
87 we assume the former when provided only half of the input hemisphere.
88 The "up" symmetry was a late addition, and involves rotating and copying the
89 input data, treating the result as anisotropic.
90 It is therefore less efficient, and should only be used when necessary.
91 Finally, if the incident hemisphere is fully covered, the BSDF is also anisotropic.
92 .PP
93 If a
94 .I \-s
95 symmetry option is specified and it does not agree with the input
96 data provided, an error message is issued and no output is produced.
97 Note that only the "up" and "bilateral" symmetry options have
98 identical input coverage, so this is the only time the
99 .I \-s
100 option must be specified if the default mirroring is inappropriate.
101 .PP
102 The
103 .I Mountain
104 software operates the pg2 goniophotometer to
105 capture BSDF scattering data in separate files for each incident
106 angle in a text file beginning with a header
107 whose lines each start with a pound sign ('#').
108 Some header settings require colons and others do not, as indicated below.
109 The
110 .i pabopto2bsdf
111 program understands the following lines from each header and ignores
112 the rest:
113 .TP
114 .BR #sample_name
115 A double-quoted string containing the name associated with this sample.
116 If input files contain different sample names, the one read
117 will be the sample name passed to the SIR output.
118 .TP
119 .BR #format:
120 The data format, typically one of "theta phi DSF" or "theta phi BSDF".
121 These differ only in their inclusion of a cosine factor.
122 The word "BRDF" or "BTDF" is accepted in place of "BSDF".
123 Any other specification or a format missing generates an error.
124 .TP
125 .BR #intheta
126 The incident theta (polar) angle in degrees, measured from the sample's
127 surface normal.
128 Theta values should be between 0 and 180, where values less than 90
129 are considered incident to the "front" side of the sample, and
130 theta values greater than 90 are incident to the "back" side in
131 the standard coordinate system.
132 Notions of sample "front" and "back" may be reversed using the
133 .I -t
134 option if desired.
135 .TP
136 .BR #inphi
137 The incident phi (azimuthal) angle in degrees counter-clockwise as
138 seen from the "front" side of the sample.
139 .TP
140 .BR #incident_angle
141 The incident theta and phi angles are each given in this header
142 line, offered as an alternative to separate "#intheta" and "#inphi"
143 angles.
144 The interpretation is the same as above.
145 .TP
146 .BR #upphi
147 If present, this phi angle that corresponds to
148 the sample "up" orientation.
149 By default, it is assumed to be 0 degrees, meaning that "up"
150 is phi=0.
151 To get the standard RADIANCE coordinates for BSDFs, "#upphi" should
152 be set to 90.
153 .TP
154 .BR #colorimetry:
155 Two colorimetry values are currently understood, "CIE-Y" and "CIE-XYZ".
156 The default colorimetry of "CIE-Y", which may be left unspecified,
157 takes each DSF or BSDF value as photometric.
158 If "CIE-XYZ" is specified, then the DSF or BSDF values must be triplets
159 corresponding to CIE XYZ values.
160 Such files are typically produced by the
161 .I pabopto2xyz(1)
162 tool rather than
163 .I Mountain,
164 directly.
165 .PP
166 The BSDF scattering data follows the header in unspecified order,
167 where each line in the file
168 contains the scattered theta and phi angles measured in the same
169 coordinate system as incident theta and phi, followed by the DSF
170 or BSDF value, which may either be a single photometric quantity
171 for "CIE-Y" colorimetry or a triplet if the colorimetry is "CIE-XYZ".
172 A minimal incident BSDF data file might contain:
173 .sp
174 .nf
175 #incident_angle 82.5 180
176 #format: theta phi DSF
177 84.968 125.790 0.009744
178 84.889 125.610 0.007737
179 84.805 125.427 0.008569
180 ...
181 .fi
182 .sp
183 The above header is equivalent to the more complete version below:
184 .sp
185 .nf
186 #format: theta phi DSF
187 #incident_angle 82.5 180
188 #intheta 82.5
189 #inphi 180
190 #upphi 0
191 #colorimetry: CIE-Y
192 84.968 125.790 0.009744
193 84.889 125.610 0.007737
194 84.805 125.427 0.008569
195 ...
196 .fi
197 .sp
198 The ordering of the header and data lines is unimportant,
199 but all header lines must precede all data lines in each input file.
200 .SH EXAMPLE
201 To generate an SIR file from a collection of transmission measurements
202 of a material with 180-degree symmetry using 4 processes:
203 .IP "" .2i
204 pabopto2bsdf -n 4 -s up f*_Tvis.txt > front_trans.sir
205 .PP
206 To combine this with front reflection measurements into a Klems BSDF file:
207 .IP "" .2i
208 pabopto2bsdf -n 4 -s up f*_Rvis.txt > front_refl.sir
209 .br
210 bsdf2klems front_trans.sir front_refl.sir > Klems_bsdf.xml
211 .SH AUTHOR
212 Greg Ward
213 .SH "SEE ALSO"
214 bsdf2klems(1), bsdf2rad(1), bsdf2ttree(1), bsdfview(1), pabopto2xyz(1)