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Comparing ray/doc/man/man1/rtpict.1 (file contents):
Revision 1.11 by greg, Mon Apr 11 04:03:36 2022 UTC vs.
Revision 1.15 by greg, Tue Dec 12 17:18:27 2023 UTC

# Line 1 | Line 1
1   .\" RCSid "$Id$"
2   .TH RTPICT 1 3/19/2018 RADIANCE
3   .SH NAME
4 < rtpict - generate a RADIANCE picture or layered image using rtrace
4 > rtpict - generate a RADIANCE picture, hyperspectral image, or layers using rtrace
5   .SH SYNOPSIS
6   .B rtpict
7   .B "-n nproc"
8   [
9 + .B -co
10 + ][
11   .B "-o[vrxlLRXnNsmM] out_dir"
12   ][
13   .B "-d ref_depth/unit"
# Line 19 | Line 21 | rtpict - generate a RADIANCE picture or layered image
21   .B octree
22   .SH DESCRIPTION
23   .I Rtpict
24 < is a script that generates a picture from the RADIANCE scene given in
24 > is a script that generates a picture or hyperspectral image
25 > from the RADIANCE scene given in
26   .I octree
27   and sends it to the standard output, or to a file specified with the
28   .I \-o
29   option.
30   Most options and defaults are the same as
31   .I rpict(1),
32 < although a few switches are silently ignored.
33 < Options incompatible with multi-processing can generate an error.
32 > although a few options are silently ignored, and the
33 > .I rtrace(1)
34 > .I \-co
35 > boolean switch is supported.
36 > Options incompatible with multi-processing may generate an error.
37   .PP
38   The
39 < .I rtrace(1)
39 > .I rtrace
40   tool is called with
41   .I vwrays(1)
42   to perform the actual work.
# Line 78 | Line 84 | M      material.idx
84   Different encodings are associated with different data types.
85   Color data (from the 'v', 'r', and 'x' types) will be converted to
86   a flat RGBE picture by
87 < .I pvalue(1).
87 > .I pvalue(1),
88 > unless the
89 > .I \-co+
90 > option is specified and
91 > .I \-cs
92 > is greater than 3.
93 > In this case, a hyperspectral image will be generated for each
94 > of the value types, converted by
95 > .I rcomb(1)
96 > and with its suffix set to ".hsr" rather than ".hdr".
97   Distances (from the 'l', 'L', 'R', and 'X' types) will be
98   converted to a 16-bit representation by
99   .I rcode_depth(1),
# Line 88 | Line 103 | option should be used to assign the reference (median)
103   units, which applies to the overall scene.
104   Surface normals (from the 'n' and 'N' types) will be converted
105   to a 32-bit representation by
106 < .I rcode_normal(1).
106 > .I rcode_norm(1).
107   Finally, identifiers (from the 's', 'm', and 'M' types) will be
108   converted to a 16-bit index format by
109   .I rcode_ident(1).
# Line 98 | Line 113 | If the
113   option is used to turn on irradiane output, then the picture associated
114   with the 'v' type will be renamed
115   .I "irradiance.hdr"
116 < and some other output types become irrelevant (i.e., 'r', 'x', 'R', and 'X').
116 > or
117 > .I "irradiance.hsr"
118 > and some other output types become irrelevant
119 > (i.e., 'r', 'x', 'R', and 'X').
120   If one or more of the associated output files already exists in the
121   destination directory, an error will be printed and the command will abort.
122   .SH EXAMPLES
# Line 109 | Line 127 | rtpict -n 4 -vf mypers.vf -ab 1 -af scene.amb scene.oc
127   To render radiance, first surface distance, and normals in a layered image:
128   .IP "" .2i
129   rtpict -n 8 -vf fish.vf @render.opt -ovLn fisholay scene.oct
130 + .PP
131 + To render a hyperspectral irradiance image with 18 spectral samples:
132 + .IP "" .2i
133 + rtpict -vf inside.vf -i+ -cs 18 -co+ scene.oct > scene_inside.hsr
134   .SH AUTHOR
135   Greg Ward
136   .SH "SEE ALSO"
137   getinfo(1), mkpmap(1), oconv(1), pfilt(1),
138 < pvalue(1), rad(1), rcode_depth(1), rcode_normal(1), rcode_ident(1),
139 < rcrop(1), rpiece(1), rpict(1), rsplit(1), rtrace(1), rvu(1), vwrays(1)
138 > pvalue(1), rad(1), rcode_depth(1), rcode_norm(1), rcode_ident(1),
139 > rcomb(1), rcrop(1), rmtxop(1),
140 > rpiece(1), rpict(1), rsplit(1), rtrace(1), rvu(1), vwrays(1)

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