1 |
.\" RCSid "$Id: rtpict.1,v 1.14 2023/12/12 16:31:45 greg Exp $" |
2 |
.TH RTPICT 1 3/19/2018 RADIANCE |
3 |
.SH NAME |
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" |
14 |
] |
15 |
[ |
16 |
.B "rpict options" |
17 |
] |
18 |
[ |
19 |
.B @file |
20 |
] |
21 |
.B octree |
22 |
.SH DESCRIPTION |
23 |
.I Rtpict |
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 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 |
40 |
tool is called with |
41 |
.I vwrays(1) |
42 |
to perform the actual work. |
43 |
This enables the |
44 |
.I \-n |
45 |
option for multiprocessing on platforms that support it. |
46 |
If the |
47 |
.I \-n |
48 |
option is not specified or is set to 1, then |
49 |
.I rpict |
50 |
is called directly. |
51 |
There is no benefit in setting the number of processes to anything |
52 |
greater than the number of virtual cores available on your machine. |
53 |
Also, it is very important to set the |
54 |
.I \-af |
55 |
option if an irradiance cache is being generated; |
56 |
otherwise, your speed-up will be far from linear. |
57 |
.PP |
58 |
If the |
59 |
.I \-o |
60 |
option has additional characters corresponding to output types from |
61 |
.I rtrace, |
62 |
it must be followed by the name of a directory that either exists or |
63 |
will be created to contain image layers, one per output type. |
64 |
The supported types are listed below, and do not include types that |
65 |
are useless or have no convenient representation. |
66 |
The table below shows the correspondence between output type and file name |
67 |
in the specified directory: |
68 |
.sp |
69 |
.nf |
70 |
v radiance.hdr |
71 |
r r_refl.hdr |
72 |
x r_unrefl.hdr |
73 |
l d_effective.dpt |
74 |
L d_firstsurf.dpt |
75 |
R d_refl.dpt |
76 |
X d_unrefl.dpt |
77 |
n perturbed.nrm |
78 |
N unperturbed.nrm |
79 |
s surface.idx |
80 |
m modifier.idx |
81 |
M material.idx |
82 |
.fi |
83 |
.sp |
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), |
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), |
100 |
and the |
101 |
.I \-d |
102 |
option should be used to assign the reference (median) depth and world |
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_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). |
110 |
.PP |
111 |
If the |
112 |
.I \-i |
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 |
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 |
123 |
To render a scene with four processes: |
124 |
.IP "" .2i |
125 |
rtpict -n 4 -vf mypers.vf -ab 1 -af scene.amb scene.oct > scene_pers.hdr |
126 |
.PP |
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_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) |