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Revision 1.2 by greg, Sat Sep 13 15:24:13 2003 UTC vs.
Revision 1.11 by greg, Thu Jul 18 14:45:59 2019 UTC

# Line 1 | Line 1
1 < .\" RCSid "$Id"
1 > .\" RCSid "$Id$"
2   .TH PVALUE 1 1/15/99 RADIANCE
3   .SH NAME
4   pvalue - convert RADIANCE picture to/from alternate formats
# Line 42 | Line 42 | these files.
42   .TP 10n
43   .BR \-u
44   Print only unique values in the output, skipping runs of equal pixels.
45 + For reverse conversions, the
46 + .I \-u
47 + option writes uncompressed output rather than the standard run-length RGBE
48 + encoding.
49   Specifying
50   .I \+u
51   turns this option off, which is the default.
52   .TP
53   .BR \-o
54   Print original values, before exposure compensation.
55 + If the input file is in XYZE format, the Y (green) channel
56 + will correspond to units of candelas/meter^2.
57 + Otherwise, the RGB values should be in spectral watts/steradian/meter^2.
58   Specifying
59   .I \+o
60 < uses final values, which is the default.
60 > uses final exposed values, which is the default.
61   .TP
62   .BR \-h
63   Do not print header.
# Line 73 | Line 80 | causes the resolution string to be printed, which is t
80   Skip the specified number of bytes on the input header.
81   This option is useful for skipping unintelligible headers in
82   foreign file formats.
76 (Does not work when reading from standard input.)
83   .TP
84   .BI \-e \ exposure
85   Adjust the exposure by the amount specified.
# Line 177 | Line 183 | Specifying
183   converts from a Radiance picture to other values, which is the
184   default.
185   .TP
186 + .BI \-p " xr yr xg yg xb yb xw yw"
187 + On reverse conversion, RGB input uses the given set of color primaries.
188 + These are written into the output header with the PRIMARIES variable.
189 + .TP
190 + .BR \-pXYZ
191 + On reverse conversion, input is in CIE XYZ coordinates, rather than RGB.
192 + The Y channel is assumed to be in candelas/meter^2.
193 + .TP
194   .BI -y \ res
195   Set the output y resolution to
196   .I res.
# Line 207 | Line 221 | options determines whether the scanlines are sorted al
221   x or along y.
222   Most Radiance pictures are sorted top to bottom, then left
223   to right.
224 < This corresponds to a specification of the form "-y yres +x xres".
224 > This corresponds to a specification of the form "\-y yres +x xres".
225   Either an upper or lower case 'X' may be used for this option.
226   Like the
227   .I \-y
# Line 217 | Line 231 | options have no effect for forward conversions.
231   .SH EXAMPLE
232   To look at the original, unique pixels in picture:
233   .IP "" .2i
234 < pvalue -o -u picture | more
234 > pvalue \-o \-u picture | more
235   .PP
236   To convert from a 512x400 8-bit greyscale image in bottom to top,
237   left to right scanline ordering:
238   .IP "" .2i
239 < pvalue -r -db -b -h +y 400 +x 512 input.im > flipped.pic
239 > pvalue \-r \-db \-b \-h +y 400 +x 512 input.im > flipped.hdr
240   .br
241 < pflip -v flipped.pic > final.pic
241 > pflip \-v flipped.hdr > final.hdr
242   .SH AUTHOR
243   Greg Ward
244   .SH BUGS
245 < 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
245 > Input pixel locations are ignored during a reverse
246   conversion, so this information is not used in determining
247   the scanline ordering or picture size.
248   .SH "SEE ALSO"
249   getinfo(1), pcompos(1), pfilt(1), pflip(1),
250 < protate(1), rpict(1), rtrace(1), rview(1)
250 > protate(1), ra_xyze(1), rpict(1), rtrace(1), rvu(1)

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