man/man1/pvalue.1

.\" RCSid "$Id: pvalue.1,v 1.3 2003/12/09 15:59:06 greg Exp $"
.TH PVALUE 1 1/15/99 RADIANCE
.SH NAME
pvalue - convert RADIANCE picture to/from alternate formats
.SH SYNOPSIS
.B pvalue
[
.B options
]
[
.B file
]
.br
.B "pvalue -r"
[
.B options
]
[
.B file1
[
.B "file2 file3"
]
]
.SH DESCRIPTION
.I Pvalue
converts the pixels of a RADIANCE picture to or from another format.
In the default mode, pixels are sent to the
standard output, one per line, in the following ascii format:

        xpos    ypos    red     green   blue

If no
.I file
is given, the standard input is read.
.PP
The reverse conversion option
.I (-r)
may be used with a single input file or when reading from the
standard input, but if the second form is used with three separate
input files, the three primaries are presumed to be separated in
these files.
.TP 10n
.BR \-u
Print only unique values in the output, skipping runs of equal pixels.
Specifying
.I \+u
turns this option off, which is the default.
.TP
.BR \-o
Print original values, before exposure compensation.
Specifying
.I \+o
uses final values, which is the default.
.TP
.BR \-h
Do not print header.
Specifying
.I \+h
causes the header to be printed, which is the default.
.TP
.BI \-H
Do not print the resolution string.
(See also the
.I \-r
option below.)
Specifying an input resolution for reverse conversion also turns
this option off.
Specifying
.I \+H
causes the resolution string to be printed, which is the default.
.TP
.BI \-s \ nbytes
Skip the specified number of bytes on the input header.
This option is useful for skipping unintelligible headers in
foreign file formats.
(Does not work when reading from standard input.)
.TP
.BI \-e \ exposure
Adjust the exposure by the amount specified.
If the exposure is being given as a conversion factor, use
.I \+e
instead, so an EXPOSURE line will not be recorded in the header
(if any).
.TP
.BI \-g \ gamma
Set gamma correction for conversion.
When converting from a RADIANCE picture to another format,
the inverse gamma is applied to correct for monitor response.
When converting to a RADIANCE picture
.I (\-r
option), the gamma is applied directly to recover the linear values.
By default,
.I gamma
is set to 1.0, meaning no gamma correction is performed.
.TP
.BR \-d
Data only,
do not print x and y pixel position.
.TP
.BR \-da
Same as
.I \-d.
.TP
.BR \-di
Print ascii integer values from 0 to 255+.
If
.I \+di
is given, the integer values will be preceded by
the x and y pixel locations.
.TP
.BR \-db
Output binary byte values from 0 to 255.
.TP
.BR \-dw
Output binary 16-bit words from 0 to 65535.
.TP
.BR \-dW
Output binary 16-bit words from 0 to 65535, byte-swapped.
.TP
.BR \-df
Output binary float values.
.TP
.BR \-dF
Output byte-swapped binary float values.
.TP
.BR \-dd
Output binary double values.
.TP
.BR \-dD
Output byte-swapped binary double values.
.TP
.BR \-R
Reverse ordering of colors so that the output is blue then green
then red.
The default ordering (specified with
.I \+R)
is red then green then blue.
.TP
.BR \-n
The RGB values are non-interleaved, meaning that all the red, green
and blue data are stored together in separate chunks.
Interleaving may be turned on with the
.I \+n
option, which is the default.
.TP
.BR \-b
Print brightness values rather than RGB.
Specifying
.I \+b
turns this option off, which is the default.
.TP
.BI \-p P
Put out only the primary
.I P,
where
.I P
is one of upper or lower case 'R', 'G' or 'B' for red, green or
blue, respectively.
This option may be used to separate the Radiance primaries into
three files with three separate runs of
.I pvalue,
or only one file when only one primary is needed.
Note that there is no space between this option and its argument.
.TP
.BR \-r
Perform reverse conversion.
Input is in the format given by the other options.
The x and y resolution must be specified on the command line, unless
the image file contains a Radiance resolution string at the
beginning (see 
.I \-H
option above and
.I \-y
option below).
Specifying
.I \+r
converts from a Radiance picture to other values, which is the
default.
.TP
.BI -y \ res
Set the output y resolution to
.I res.
If
.I \+y
is specified, then the scanlines are assumed to be in
increasing order (ie. bottom to top).
The default value for this option is 0, which means
that the picture size and scanline order must appear
as the first line after the header (if any) in the
input file.
Either an upper or lower case 'Y' may be used for this option.
Since Radiance files always contain such a line, 
this option has no effect for forward conversions.
.TP
.BI +x \ res
Set the output x resolution to
.I res.
If
.I \-x
is specified, then the scanlines are assumed to be in
decreasing order (ie. right to left).
The ordering of the
.I \-y
and
.I \+x
options determines whether the scanlines are sorted along
x or along y.
Most Radiance pictures are sorted top to bottom, then left
to right.
This corresponds to a specification of the form "-y yres +x xres".
Either an upper or lower case 'X' may be used for this option.
Like the
.I \-y
option,
.I \-x
options have no effect for forward conversions.
.SH EXAMPLE
To look at the original, unique pixels in picture:
.IP "" .2i
pvalue -o -u picture | more
.PP
To convert from a 512x400 8-bit greyscale image in bottom to top,
left to right scanline ordering:
.IP "" .2i
pvalue -r -db -b -h +y 400 +x 512 input.im > flipped.pic
.br
pflip -v flipped.pic > final.pic
.SH AUTHOR
Greg Ward
.SH BUGS
The
.I \-r
option does not work with the
.I \-u
option.
Also, input pixel locations are ignored during a reverse
conversion, so this information is not used in determining
the scanline ordering or picture size.
.SH "SEE ALSO"
getinfo(1), pcompos(1), pfilt(1), pflip(1),
protate(1), rpict(1), rtrace(1), rvu(1)
Revision:	1.4
Committed:	Thu Jan 1 19:31:45 2004 UTC (21 years, 9 months ago) by greg
Branch:	MAIN
Changes since 1.3:	+2 -2 lines
Log Message:	Renamed rview, lam, calc, and neat to rvu, rlam, icalc, and neaten
#	User	Rev	Content
1	greg	1.4	.\" RCSid "$Id: pvalue.1,v 1.3 2003/12/09 15:59:06 greg Exp $"
2	greg	1.1	.TH PVALUE 1 1/15/99 RADIANCE
3			.SH NAME
4			pvalue - convert RADIANCE picture to/from alternate formats
5			.SH SYNOPSIS
6			.B pvalue
7			[
8			.B options
9			]
10			[
11			.B file
12			]
13			.br
14			.B "pvalue -r"
15			[
16			.B options
17			]
18			[
19			.B file1
20			[
21			.B "file2 file3"
22			]
23			]
24			.SH DESCRIPTION
25			.I Pvalue
26			converts the pixels of a RADIANCE picture to or from another format.
27			In the default mode, pixels are sent to the
28			standard output, one per line, in the following ascii format:
29
30			xpos ypos red green blue
31
32			If no
33			.I file
34			is given, the standard input is read.
35			.PP
36			The reverse conversion option
37			.I (-r)
38			may be used with a single input file or when reading from the
39			standard input, but if the second form is used with three separate
40			input files, the three primaries are presumed to be separated in
41			these files.
42			.TP 10n
43			.BR \-u
44			Print only unique values in the output, skipping runs of equal pixels.
45			Specifying
46			.I \+u
47			turns this option off, which is the default.
48			.TP
49			.BR \-o
50			Print original values, before exposure compensation.
51			Specifying
52			.I \+o
53			uses final values, which is the default.
54			.TP
55			.BR \-h
56			Do not print header.
57			Specifying
58			.I \+h
59			causes the header to be printed, which is the default.
60			.TP
61			.BI \-H
62			Do not print the resolution string.
63			(See also the
64			.I \-r
65			option below.)
66			Specifying an input resolution for reverse conversion also turns
67			this option off.
68			Specifying
69			.I \+H
70			causes the resolution string to be printed, which is the default.
71			.TP
72			.BI \-s \ nbytes
73			Skip the specified number of bytes on the input header.
74			This option is useful for skipping unintelligible headers in
75			foreign file formats.
76			(Does not work when reading from standard input.)
77			.TP
78			.BI \-e \ exposure
79			Adjust the exposure by the amount specified.
80			If the exposure is being given as a conversion factor, use
81			.I \+e
82			instead, so an EXPOSURE line will not be recorded in the header
83			(if any).
84			.TP
85			.BI \-g \ gamma
86			Set gamma correction for conversion.
87			When converting from a RADIANCE picture to another format,
88			the inverse gamma is applied to correct for monitor response.
89			When converting to a RADIANCE picture
90			.I (\-r
91			option), the gamma is applied directly to recover the linear values.
92			By default,
93			.I gamma
94			is set to 1.0, meaning no gamma correction is performed.
95			.TP
96			.BR \-d
97			Data only,
98			do not print x and y pixel position.
99			.TP
100			.BR \-da
101			Same as
102			.I \-d.
103			.TP
104			.BR \-di
105			Print ascii integer values from 0 to 255+.
106			If
107			.I \+di
108			is given, the integer values will be preceded by
109			the x and y pixel locations.
110			.TP
111			.BR \-db
112			Output binary byte values from 0 to 255.
113			.TP
114			.BR \-dw
115			Output binary 16-bit words from 0 to 65535.
116			.TP
117			.BR \-dW
118			Output binary 16-bit words from 0 to 65535, byte-swapped.
119			.TP
120			.BR \-df
121			Output binary float values.
122			.TP
123	greg	1.2	.BR \-dF
124			Output byte-swapped binary float values.
125			.TP
126	greg	1.1	.BR \-dd
127			Output binary double values.
128	greg	1.2	.TP
129			.BR \-dD
130			Output byte-swapped binary double values.
131	greg	1.1	.TP
132			.BR \-R
133			Reverse ordering of colors so that the output is blue then green
134			then red.
135			The default ordering (specified with
136			.I \+R)
137			is red then green then blue.
138			.TP
139			.BR \-n
140			The RGB values are non-interleaved, meaning that all the red, green
141			and blue data are stored together in separate chunks.
142			Interleaving may be turned on with the
143			.I \+n
144			option, which is the default.
145			.TP
146			.BR \-b
147			Print brightness values rather than RGB.
148			Specifying
149			.I \+b
150			turns this option off, which is the default.
151			.TP
152			.BI \-p P
153			Put out only the primary
154			.I P,
155			where
156			.I P
157			is one of upper or lower case 'R', 'G' or 'B' for red, green or
158			blue, respectively.
159			This option may be used to separate the Radiance primaries into
160			three files with three separate runs of
161			.I pvalue,
162			or only one file when only one primary is needed.
163			Note that there is no space between this option and its argument.
164			.TP
165			.BR \-r
166			Perform reverse conversion.
167			Input is in the format given by the other options.
168			The x and y resolution must be specified on the command line, unless
169			the image file contains a Radiance resolution string at the
170			beginning (see
171			.I \-H
172			option above and
173			.I \-y
174			option below).
175			Specifying
176			.I \+r
177			converts from a Radiance picture to other values, which is the
178			default.
179			.TP
180			.BI -y \ res
181			Set the output y resolution to
182			.I res.
183			If
184			.I \+y
185			is specified, then the scanlines are assumed to be in
186			increasing order (ie. bottom to top).
187			The default value for this option is 0, which means
188			that the picture size and scanline order must appear
189			as the first line after the header (if any) in the
190			input file.
191			Either an upper or lower case 'Y' may be used for this option.
192			Since Radiance files always contain such a line,
193			this option has no effect for forward conversions.
194			.TP
195			.BI +x \ res
196			Set the output x resolution to
197			.I res.
198			If
199			.I \-x
200			is specified, then the scanlines are assumed to be in
201			decreasing order (ie. right to left).
202			The ordering of the
203			.I \-y
204			and
205			.I \+x
206			options determines whether the scanlines are sorted along
207			x or along y.
208			Most Radiance pictures are sorted top to bottom, then left
209			to right.
210			This corresponds to a specification of the form "-y yres +x xres".
211			Either an upper or lower case 'X' may be used for this option.
212			Like the
213			.I \-y
214			option,
215			.I \-x
216			options have no effect for forward conversions.
217			.SH EXAMPLE
218			To look at the original, unique pixels in picture:
219			.IP "" .2i
220			pvalue -o -u picture \| more
221			.PP
222			To convert from a 512x400 8-bit greyscale image in bottom to top,
223			left to right scanline ordering:
224			.IP "" .2i
225			pvalue -r -db -b -h +y 400 +x 512 input.im > flipped.pic
226			.br
227			pflip -v flipped.pic > final.pic
228			.SH AUTHOR
229			Greg Ward
230			.SH BUGS
231			The
232			.I \-r
233			option does not work with the
234			.I \-u
235			option.
236			Also, input pixel locations are ignored during a reverse
237			conversion, so this information is not used in determining
238			the scanline ordering or picture size.
239			.SH "SEE ALSO"
240			getinfo(1), pcompos(1), pfilt(1), pflip(1),
241	greg	1.4	protate(1), rpict(1), rtrace(1), rvu(1)