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root/radiance/ray/doc/man/man1/falsecolor.1
Revision: 1.8
Committed: Tue Oct 5 01:07:16 2010 UTC (14 years, 8 months ago) by greg
Branch: MAIN
CVS Tags: rad4R1
Changes since 1.7: +2 -2 lines
Log Message:
Minor wording

File Contents

# User Rev Content
1 greg 1.8 .\" RCSid "$Id: falsecolor.1,v 1.7 2010/10/05 00:59:38 greg Exp $"
2 greg 1.1 .TH FALSECOLOR 1 11/15/93 RADIANCE
3     .SH NAME
4     falsecolor - make a false color RADIANCE picture
5     .SH SYNOPSIS
6     .B falsecolor
7     [
8     .B "\-i input"
9     ][
10     .B "\-p picture"
11     ][
12     .B "\-cb | \-cl"
13     ][
14     .B \-e
15     ][
16     .B "\-s scale"
17     ][
18     .B "\-l label"
19     ][
20     .B "\-n ndivs"
21     ][
22 greg 1.3 .B "\-lw lwidth"
23     ][
24     .B "\-lh lheight"
25     ][
26 greg 1.1 .B "\-log decades"
27     ][
28     .B "\-m mult"
29     ][
30 greg 1.7 .B "\-pal palette"
31 greg 1.4 ][
32 greg 1.1 .B "\-r redv"
33     ][
34     .B "\-g grnv"
35     ][
36     .B "\-b bluv"
37     ]
38     .SH DESCRIPTION
39     .I Falsecolor
40     produces a false color picture for lighting analysis.
41     Input is a rendered Radiance picture.
42     .PP
43     By default, luminance is displayed on a linear scale from 0 to 1000 nits, where
44     dark areas are blue and brighter areas move through the spectrum to red.
45     A different scale can be given with the
46     .I \-s
47     option.
48 greg 1.4 If the argument given to
49     .I \-s
50     begins with an "a" for "auto," then the maximum is used for scaling the result.
51 greg 1.1 The default multiplier is 179, which converts from radiance or irradiance
52     to luminance or illuminance, respectively.
53     A different multiplier can be given with
54     .I \-m
55     to get daylight factors or whatever.
56     For a logarithmic rather than a linear mapping, the
57     .I \-log
58     option can be used, where
59     .I decades
60     is the number of decades below the maximum scale desired.
61     .PP
62     A legend is produced for the new image with a label given by the
63     .I \-l
64     option.
65     The default label is "Nits", which is appropriate for standard Radiance
66     images.
67     If the
68     .I -i
69     option of
70     .I rpict(1)
71     was used to produce the image, then the appropriate label would be "Lux".
72     .PP
73     If contour lines are desired rather than just false color, the
74     .I \-cl
75     option can be used.
76     These lines can be placed over another Radiance picture using the
77     .I -p
78     option.
79     If the input picture is given with
80     .I \-ip
81     instead of
82     .I \-i,
83     then it will be used both as the source of values and as the picture
84     to overlay with contours.
85     The
86     .I \-cb
87     option produces contour bands instead of lines, where the thickness of
88     the bands is related to the rate of change in the image.
89     The
90     .I \-n
91     option can be used to change the number of contours (and corresponding
92     legend entries) from the default value of 8.
93 greg 1.3 The
94     .I \-lw
95     and
96     .I \-lh
97     options may be used to change the legend dimensions from the default width
98     and height of 100x200.
99     A value of zero in either eliminates the legend in the output.
100 greg 1.1 .PP
101     The
102     .I \-e
103     option causes extrema points to be printed on the brightest and
104     darkest pixels of the input picture.
105     .PP
106 greg 1.4 The
107 greg 1.7 .I "\-pal"
108     option provides different color palettes for
109 greg 1.4 .I falsecolor.
110 greg 1.7 The current choices are
111     .I spec
112     for the old spectral mapping,
113     .I hot
114 greg 1.8 for a thermal scale, and
115 greg 1.7 .I pm3d
116     for a variation of the default mapping,
117     .I def.
118 greg 1.1 The remaining options,
119     .I "\-r, \-g,"
120     and
121     .I \-b
122     are for changing the mapping of values to colors.
123     These are expressions of the variable
124     .I v,
125     where
126     .I v
127     varies from 0 to 1.
128     These options are not recommended for the casual user.
129     .PP
130     If no
131     .I \-i
132     or
133     .I \-ip
134     option is used, input is taken from the standard input.
135     The output image is always written to standard output, which should
136     be redirected.
137     .SH EXAMPLES
138     To create a false color image directly from
139     .I rpict(1):
140     .IP "" .2i
141 greg 1.6 rpict \-vf default.vp scene.oct | falsecolor > scene.hdr
142 greg 1.1 .PP
143     To create a logarithmic contour plot of illuminance values on a
144     Radiance image:
145     .IP "" .2i
146 greg 1.6 rpict \-i \-vf default.vp scene.oct > irrad.hdr
147 greg 1.1 .br
148 greg 1.6 rpict \-vf default.vp scene.oct > rad.hdr
149 greg 1.1 .br
150 greg 1.6 falsecolor \-i irrad.hdr \-p rad.hdr \-cl \-log 2 \-l Lux > lux.hdr
151 greg 1.1 .SH AUTHOR
152     Greg Ward
153 greg 1.7 .br
154     Axel Jacobs (Perl translation and -pal options)
155 greg 1.1 .SH ACKNOWLEDGEMENT
156     Work on this program was initiated and sponsored by the LESO
157     group at EPFL in Switzerland.
158     .SH "SEE ALSO"
159     getinfo(1), pcomb(1), pcompos(1), pextrem(1), pfilt(1), pflip(1), protate(1),
160     psign(1), rpict(1), ximage(1)