man/man1/pcond.1

.\" RCSid "$Id: pcond.1,v 1.5 2021/04/07 21:13:52 greg Exp $"
.TH PCOND 1 10/27/98 RADIANCE
.SH NAME
pcond - condition a RADIANCE picture for output
.SH SYNOPSIS
.B pcond
[
.B options
]
.B input
[
.B output
]
.SH DESCRIPTION
.I Pcond
conditions a Radiance picture for output to a display or hard copy
device.
If the dynamic range of the scene exceeds that of the display (as is
usually the case),
.I pcond
will compress the dynamic range of the picture such that both
dark and bright regions are visible.
In addition, certain limitations in human vision may be mimicked in
order to provide an appearance similar to the experience one might
have in the actual scene.
.PP
Command line switches turn flags off and on, changing program behavior.
A switch given by itself toggles the flag from off to on or on to
off depending on its previous state.
A switch followed by a '+' turns the option on explicitly.
A switch followed by a '-' turns the option off.
The default is all switches off.
Other options specify output device parameters in order to get more
accurate color and contrast.
.TP 10n
.BI -h [+-]
Mimic human visual response in the output.
The goal of this process is to produce output that correlates
strongly with a person's subjective impression of a scene.
This switch is a bundle of the
.I \-a,
.I \-v,
.I \-s
and
.I \-c
options.
.TP
.BI -a [+-]
Defocus darker regions of the image to simulate human visual acuity loss.
This option will not affect well-lit scenes.
.TP
.BI -v [+-]
Add veiling glare due to very bright regions in the image.
This simulates internal scattering in the human eye, which
results in a loss of visible contrast near bright sources.
.TP
.BI -s [+-]
Use the human contrast sensitivity function in determining the
exposure for the image.
A darker scene will have relatively lower exposure with lower
contrast than a well-lit scene.
.TP
.BI -c [+-]
If parts of the image are in the mesopic or scotopic range where
the cone photoreceptors lose their efficiency, this switch will
cause a corresponding loss of color visibility in the output and a
shift to a scotopic (blue-dominant) response function.
.TP
.BI -w [+-]
Use a center-weighted average for the exposure rather than the
default uniform average.
This may improve the exposure for scenes with high or low peripheral
brightness.
.TP
.BI -i \ fixfrac
Set the relative importance of fixation points to
.I fixfrac,
which is a value between 0 and 1.
If
.I fixfrac
is zero (the default), then no fixation points are used in
determining the local or global adaptation.
If
.I fixfrac
is greater than zero, then a list of fixation points is read from
the standard input.
These points are given as tab-separated (x,y) picture
coordinates, such as those produced by the
.I \-op
option of
.I ximage(1).
The foveal samples about these fixation points will then be weighted
together with the global averaging scheme such that the fixations receive
.I fixfrac
of the total weight.
If
.I fixfrac
is one, then only the fixation points are considered for
adaptation.
.TP
.BI -I [+-]
Rather than computing a histogram of foveal samples from the source picture,
use the precomputed histogram provided on the standard input.
This data should be given in pairs of the base-10 logarithm of
world luminance and a count for each bin in ascending order, as
computed by the
.I phisto(1)
script.
This option is useful for producing identical exposures of multiple
pictures (as in an animation), and provides greater control
over the histogram computation.
.TP
.BI -l [+-]
Use a linear response function rather than the standard dynamic
range compression algorithm.
This will prevent the loss of usable physical values in the output
picture, although some parts of the resulting image may be too
dark or too bright to see.
.TP
.BI -e \ expval
Set the exposure adjustment for the picture to
.I expval.
This may either be a real multiplier, or a (fractional) number of
f-stops preceeded by a '+' or '-'.
This option implies a linear response (see the
.I \-l
option above).
.TP
.BI -u \ Ldmax
Specifies the top of the luminance range for the target output device.
That is, the luminance (in candelas/m^2) for an output pixel value
of (R,G,B)=(1,1,1).
The default value is 100 cd/m^2.
.TP
.BI -d \ Lddyn
Specifies the dynamic range for the target output device, which is
the ratio of the maximum and minimum usable display luminances.
The default value is 100.
.TP
.BI -p " xr yr xg yg xb yb xw yw"
Specifies the RGB primaries for the target output device.
These are the 1931 CIE (x,y) chromaticity values for red, green,
blue and white, respectively.
.TP
.BI -f \ macbeth.cal
Use the given output file from
.I macbethcal(1)
to precorrect the color and contrast for the target output device.
This does a more thorough job than a simple primary correction
using the
.I \-p
option.
Only one of
.I \-f
or
.I \-p
may be given.
.TP
.BI -x \ mapfile
Put out the final mapping from world luminance to display luminance to
.I mapfile.
This file will contain values from the minimum usable world
luminance to the maximum (in candelas/m^2) in one column, and their
corresponding display luminance values (also in candelas/m^2) in the
second column.
This file may be used for debugging purposes, or to plot the mapping
function created by
.I pcond.
.SH EXAMPLES
To display an image as a person might perceive it
in the actual scene:
.IP "" .2i
pcond \-h final.hdr > display.hdr
.br
ximage display.hdr ; rm display.hdr &
.PP
To do the same on a 24\-bit display with known primary values:
.IP "" .2i
setenv DISPLAY_PRIMARIES ".580 .340 .281 .570 .153 .079 .333 .333"
.br
pcond \-h \-p $DISPLAY_PRIMARIES final.hdr | ximage &
.PP
To prepare a picture to be sent to a film recorder destined eventually
for a slide projector with a minimum and maximum screen luminance of
1.5 and 125 candelas/m^2, respectively:
.IP "" .2i
pcond \-d 83 \-u 125 final.hdr > film.hdr
.PP
To do the same if the output colors of the standard image
"ray/lib/lib/macbeth_spec.hdr" have been measured:
.IP "" .2i
macbethcal \-c mbfilm.xyY > film.cal
.br
pcond \-d 83 \-u 125 \-f film.cal final.hdr > film.hdr
.PP
To further tweak the exposure to bring out certain areas indicated by
dragging the right mouse button over them in
.I ximage:
.IP "" .2i
ximage \-op \-t 75 final.hdr | pcond \-i .5 \-d 83 \-u 125 \-f film.cal
final.hdr > film.hdr
.PP
To use a histogram computed on every 10th animation frame:
.IP "" .2i
phisto frame*0.hdr > global.hist
.br
pcond \-I \-s \-c frame0352.hdr < global.hist | ra_tiff \- frame0352.tif
.SH REFERENCE
Greg Ward Larson, Holly Rushmeier, Christine Piatko,
``A Visibility Matching Tone Reproduction Operator for High Dynamic Range
Scenes,''
.I "IEEE Transactions on Visualization and Computer Graphics",
December 1997.
.PP
http://www.sgi.com/Technology/pixformat/Larsonetal.html
.SH NOTES
Hyperspectral Radiance pictures (.hsr files) are
converted to approximate RGB pixels.
However, the colors may not be very accurate.
Pass the HSR picture through
.I rcomb(1)
first if greater color fidelity is required.
.SH AUTHOR
Greg Ward Larson
.SH "SEE ALSO"
getinfo(1), macbethcal(1), normtiff(1),
pcompos(1), pflip(1), phisto(1), pinterp(1),
pvalue(1), protate(1), ra_xyze(1), rad(1),
rcomb(1), rpict(1), ximage(1)
Revision:	1.6
Committed:	Wed Sep 11 18:56:11 2024 UTC (7 months, 3 weeks ago) by greg
Branch:	MAIN
CVS Tags:	HEAD
Changes since 1.5:	+10 -2 lines
Log Message:	feat(pcond,pvalue): Added hyperspectral input handling
#	Content
1	.\" RCSid "$Id: pcond.1,v 1.5 2021/04/07 21:13:52 greg Exp $"
2	.TH PCOND 1 10/27/98 RADIANCE
3	.SH NAME
4	pcond - condition a RADIANCE picture for output
5	.SH SYNOPSIS
6	.B pcond
7	[
8	.B options
9	]
10	.B input
11	[
12	.B output
13	]
14	.SH DESCRIPTION
15	.I Pcond
16	conditions a Radiance picture for output to a display or hard copy
17	device.
18	If the dynamic range of the scene exceeds that of the display (as is
19	usually the case),
20	.I pcond
21	will compress the dynamic range of the picture such that both
22	dark and bright regions are visible.
23	In addition, certain limitations in human vision may be mimicked in
24	order to provide an appearance similar to the experience one might
25	have in the actual scene.
26	.PP
27	Command line switches turn flags off and on, changing program behavior.
28	A switch given by itself toggles the flag from off to on or on to
29	off depending on its previous state.
30	A switch followed by a '+' turns the option on explicitly.
31	A switch followed by a '-' turns the option off.
32	The default is all switches off.
33	Other options specify output device parameters in order to get more
34	accurate color and contrast.
35	.TP 10n
36	.BI -h [+-]
37	Mimic human visual response in the output.
38	The goal of this process is to produce output that correlates
39	strongly with a person's subjective impression of a scene.
40	This switch is a bundle of the
41	.I \-a,
42	.I \-v,
43	.I \-s
44	and
45	.I \-c
46	options.
47	.TP
48	.BI -a [+-]
49	Defocus darker regions of the image to simulate human visual acuity loss.
50	This option will not affect well-lit scenes.
51	.TP
52	.BI -v [+-]
53	Add veiling glare due to very bright regions in the image.
54	This simulates internal scattering in the human eye, which
55	results in a loss of visible contrast near bright sources.
56	.TP
57	.BI -s [+-]
58	Use the human contrast sensitivity function in determining the
59	exposure for the image.
60	A darker scene will have relatively lower exposure with lower
61	contrast than a well-lit scene.
62	.TP
63	.BI -c [+-]
64	If parts of the image are in the mesopic or scotopic range where
65	the cone photoreceptors lose their efficiency, this switch will
66	cause a corresponding loss of color visibility in the output and a
67	shift to a scotopic (blue-dominant) response function.
68	.TP
69	.BI -w [+-]
70	Use a center-weighted average for the exposure rather than the
71	default uniform average.
72	This may improve the exposure for scenes with high or low peripheral
73	brightness.
74	.TP
75	.BI -i \ fixfrac
76	Set the relative importance of fixation points to
77	.I fixfrac,
78	which is a value between 0 and 1.
79	If
80	.I fixfrac
81	is zero (the default), then no fixation points are used in
82	determining the local or global adaptation.
83	If
84	.I fixfrac
85	is greater than zero, then a list of fixation points is read from
86	the standard input.
87	These points are given as tab-separated (x,y) picture
88	coordinates, such as those produced by the
89	.I \-op
90	option of
91	.I ximage(1).
92	The foveal samples about these fixation points will then be weighted
93	together with the global averaging scheme such that the fixations receive
94	.I fixfrac
95	of the total weight.
96	If
97	.I fixfrac
98	is one, then only the fixation points are considered for
99	adaptation.
100	.TP
101	.BI -I [+-]
102	Rather than computing a histogram of foveal samples from the source picture,
103	use the precomputed histogram provided on the standard input.
104	This data should be given in pairs of the base-10 logarithm of
105	world luminance and a count for each bin in ascending order, as
106	computed by the
107	.I phisto(1)
108	script.
109	This option is useful for producing identical exposures of multiple
110	pictures (as in an animation), and provides greater control
111	over the histogram computation.
112	.TP
113	.BI -l [+-]
114	Use a linear response function rather than the standard dynamic
115	range compression algorithm.
116	This will prevent the loss of usable physical values in the output
117	picture, although some parts of the resulting image may be too
118	dark or too bright to see.
119	.TP
120	.BI -e \ expval
121	Set the exposure adjustment for the picture to
122	.I expval.
123	This may either be a real multiplier, or a (fractional) number of
124	f-stops preceeded by a '+' or '-'.
125	This option implies a linear response (see the
126	.I \-l
127	option above).
128	.TP
129	.BI -u \ Ldmax
130	Specifies the top of the luminance range for the target output device.
131	That is, the luminance (in candelas/m^2) for an output pixel value
132	of (R,G,B)=(1,1,1).
133	The default value is 100 cd/m^2.
134	.TP
135	.BI -d \ Lddyn
136	Specifies the dynamic range for the target output device, which is
137	the ratio of the maximum and minimum usable display luminances.
138	The default value is 100.
139	.TP
140	.BI -p " xr yr xg yg xb yb xw yw"
141	Specifies the RGB primaries for the target output device.
142	These are the 1931 CIE (x,y) chromaticity values for red, green,
143	blue and white, respectively.
144	.TP
145	.BI -f \ macbeth.cal
146	Use the given output file from
147	.I macbethcal(1)
148	to precorrect the color and contrast for the target output device.
149	This does a more thorough job than a simple primary correction
150	using the
151	.I \-p
152	option.
153	Only one of
154	.I \-f
155	or
156	.I \-p
157	may be given.
158	.TP
159	.BI -x \ mapfile
160	Put out the final mapping from world luminance to display luminance to
161	.I mapfile.
162	This file will contain values from the minimum usable world
163	luminance to the maximum (in candelas/m^2) in one column, and their
164	corresponding display luminance values (also in candelas/m^2) in the
165	second column.
166	This file may be used for debugging purposes, or to plot the mapping
167	function created by
168	.I pcond.
169	.SH EXAMPLES
170	To display an image as a person might perceive it
171	in the actual scene:
172	.IP "" .2i
173	pcond \-h final.hdr > display.hdr
174	.br
175	ximage display.hdr ; rm display.hdr &
176	.PP
177	To do the same on a 24\-bit display with known primary values:
178	.IP "" .2i
179	setenv DISPLAY_PRIMARIES ".580 .340 .281 .570 .153 .079 .333 .333"
180	.br
181	pcond \-h \-p $DISPLAY_PRIMARIES final.hdr \| ximage &
182	.PP
183	To prepare a picture to be sent to a film recorder destined eventually
184	for a slide projector with a minimum and maximum screen luminance of
185	1.5 and 125 candelas/m^2, respectively:
186	.IP "" .2i
187	pcond \-d 83 \-u 125 final.hdr > film.hdr
188	.PP
189	To do the same if the output colors of the standard image
190	"ray/lib/lib/macbeth_spec.hdr" have been measured:
191	.IP "" .2i
192	macbethcal \-c mbfilm.xyY > film.cal
193	.br
194	pcond \-d 83 \-u 125 \-f film.cal final.hdr > film.hdr
195	.PP
196	To further tweak the exposure to bring out certain areas indicated by
197	dragging the right mouse button over them in
198	.I ximage:
199	.IP "" .2i
200	ximage \-op \-t 75 final.hdr \| pcond \-i .5 \-d 83 \-u 125 \-f film.cal
201	final.hdr > film.hdr
202	.PP
203	To use a histogram computed on every 10th animation frame:
204	.IP "" .2i
205	phisto frame*0.hdr > global.hist
206	.br
207	pcond \-I \-s \-c frame0352.hdr < global.hist \| ra_tiff \- frame0352.tif
208	.SH REFERENCE
209	Greg Ward Larson, Holly Rushmeier, Christine Piatko,
210	``A Visibility Matching Tone Reproduction Operator for High Dynamic Range
211	Scenes,''
212	.I "IEEE Transactions on Visualization and Computer Graphics",
213	December 1997.
214	.PP
215	http://www.sgi.com/Technology/pixformat/Larsonetal.html
216	.SH NOTES
217	Hyperspectral Radiance pictures (.hsr files) are
218	converted to approximate RGB pixels.
219	However, the colors may not be very accurate.
220	Pass the HSR picture through
221	.I rcomb(1)
222	first if greater color fidelity is required.
223	.SH AUTHOR
224	Greg Ward Larson
225	.SH "SEE ALSO"
226	getinfo(1), macbethcal(1), normtiff(1),
227	pcompos(1), pflip(1), phisto(1), pinterp(1),
228	pvalue(1), protate(1), ra_xyze(1), rad(1),
229	rcomb(1), rpict(1), ximage(1)