man/man1/pcomb.1

.\" RCSid "$Id: pcomb.1,v 1.9 2008/11/10 19:08:17 greg Exp $"
.TH PCOMB 1 8/31/96 RADIANCE
.SH NAME
pcomb - combine RADIANCE pictures
.SH SYNOPSIS
.B pcomb
[
.B -h
][
.B -w
][
.B "\-x xres"
][
.B "\-y yres"
][
.B "\-f file"
][
.B "\-e expr"
]
[
[
.B -o
][
.B "\-s factor"
][
.B "\-c r g b"
]
.B "input .."
]
.SH DESCRIPTION
.I Pcomb
combines equal-sized RADIANCE pictures and sends the result to the
standard output.
By default, the result is just a linear combination of
the input pictures multiplied by
.I \-s
and
.I \-c
coefficients,
but an arbitrary mapping can be assigned with the
.I \-e
and
.I \-f
options.
Negative coefficients and functions are allowed, and
.I pcomb
will produce color values of zero where they would be negative.
.PP
The variables
.I ro,
.I go
and
.I bo
specify the red, green and blue output values, respectively.
Alternatively, the single variable
.I lo
can be used to specify a brightness value for black and white output.
The predefined functions
.I ri(n),
.I gi(n)
and
.I bi(n)
give the red, green and blue input values for
picture
.I n.
To access a pixel that is nearby the current one, these functions
also accept optional x and y offsets.
For example,
.I ri(3,-2,1)
would return the red component of the pixel from picture 3
that is left 2 and up 1 from the current position.
Although x offsets may be as large as width of the picture,
y offsets are limited to a small window (+/- 32 pixels) due to efficiency
considerations.
However, it is not usually necessary to worry about this problem --
if the requested offset is not available, the next best pixel is
returned instead.
.PP
For additional convenience, the function
.I li(n)
is defined as the input brightness for picture
.I n.
This function also accepts x and y offsets.
.PP
The constant
.I nfiles
gives the number of input files present,
and
.I WE
gives the white efficacy (lumens/brightness) for pixel values,
which may be used with the
.I \-o
option or the le(n) values to convert to absolute
photometric units (see below).
The variables
.I x
and
.I y
give the current output pixel location for use in
spatially dependent functions, the constants
.I xmax
and
.I ymax
give the input resolution, and the constants
.I xres
and 
.I yres
give the output resolution (usually the same, but see below).
The constant functions
.I "re(n), ge(n), be(n),"
and
.I le(n)
give the exposure values for picture
.I n,
and
.I pa(n)
gives the corresponding pixel aspect ratio.
Finally, for pictures with stored view parameters,
the functions
.I "Ox(n), Oy(n)"
and
.I Oz(n)
return the ray origin in world coordinates for the current pixel
in picture
.I n,
and
.I "Dx(n), Dy(n)"
and
.I Dz(n)
return the normalized ray direction.
In addition, the function
.I T(n)
returns the distance from the origin to the aft clipping plane
(or zero if there is no aft plane), and the function
.I S(n)
returns the solid angle of the current pixel in steradians
(always zero for parallel views).
If the current pixel is outside the view region,
.I T(n)
will return a negative value, and
.I S(n)
will return zero.
The first input picture with a view is assumed to correspond to the
view of the output picture, which is written into the header.
.PP
The
.I \-h
option may be used to reduce the information header size, which
can grow disproportionately after multiple runs of
.I pcomb
and/or
.I pcompos(1).
The
.I \-w
option can be used to suppress warning messages about invalid
calculations.
The
.I \-o
option indicates that original pixel values are to be used for the next
picture, undoing any previous exposure changes or color correction.
.PP
The
.I \-x
and
.I \-y
options can be used to specify the desired output resolution,
.I xres
and
.I yres,
and can be expressions involving other constants such as
.I xmax
and
.I ymax.
The constants
.I xres
and
.I yres
may also be specified in a file or expression.
The default output resolution is the same as the input resolution.
.PP
The
.I \-x
and
.I \-y
options must be present if there are no input files, when
the definitions of
.I ro,
.I go
and
.I bo
will be used to compute each output pixel.
This is useful for producing simple test pictures for various
purposes.
(Theoretically, one could write a complete renderer using just the
functional language...)
.PP
The standard input can be specified with a hyphen ('-').
A command that produces a RADIANCE picture can be given in place of a file 
by preceeding it with an exclamation point ('!').
.SH EXAMPLES
To produce a picture showing the difference between pic1 and pic2:
.IP "" .2i
pcomb \-e 'ro=ri(1)\-ri(2);go=gi(1)\-gi(2);bo=bi(1)\-bi(2)' pic1 pic2 > diff
.PP
Or, more efficiently:
.IP "" .2i
pcomb pic1 \-s \-1 pic2 > diff
.PP
To precompute the gamma correction for a picture:
.IP "" .2i
pcomb \-e 'ro=ri(1)^.4;go=gi(1)^.4;bo=bi(1)^.4' inp.hdr > gam.hdr
.PP
To perform some special filtering:
.IP "" .2i
pcomb \-f myfilt.cal \-x xmax/2 \-y ymax/2 input.hdr > filtered.hdr
.PP
To make a picture of a dot:
.IP "" .2i
pcomb \-x 100 \-y 100 \-e 'ro=b;go=b;bo=b;b=if((x-50)^2+(y-50)^2\-25^2,0,1)' > dot
.SH AUTHOR
Greg Ward
.SH "SEE ALSO"
getinfo(1), icalc(1), pcompos(1), pfilt(1), rpict(1)
Revision:	1.10
Committed:	Mon Feb 5 20:07:17 2018 UTC (7 years, 4 months ago) by greg
Branch:	MAIN
Changes since 1.9:	+3 -1 lines
Log Message:	Decided to share first input view in the output of pcomb
#	Content
1	.\" RCSid "$Id: pcomb.1,v 1.9 2008/11/10 19:08:17 greg Exp $"
2	.TH PCOMB 1 8/31/96 RADIANCE
3	.SH NAME
4	pcomb - combine RADIANCE pictures
5	.SH SYNOPSIS
6	.B pcomb
7	[
8	.B -h
9	][
10	.B -w
11	][
12	.B "\-x xres"
13	][
14	.B "\-y yres"
15	][
16	.B "\-f file"
17	][
18	.B "\-e expr"
19	]
20	[
21	[
22	.B -o
23	][
24	.B "\-s factor"
25	][
26	.B "\-c r g b"
27	]
28	.B "input .."
29	]
30	.SH DESCRIPTION
31	.I Pcomb
32	combines equal-sized RADIANCE pictures and sends the result to the
33	standard output.
34	By default, the result is just a linear combination of
35	the input pictures multiplied by
36	.I \-s
37	and
38	.I \-c
39	coefficients,
40	but an arbitrary mapping can be assigned with the
41	.I \-e
42	and
43	.I \-f
44	options.
45	Negative coefficients and functions are allowed, and
46	.I pcomb
47	will produce color values of zero where they would be negative.
48	.PP
49	The variables
50	.I ro,
51	.I go
52	and
53	.I bo
54	specify the red, green and blue output values, respectively.
55	Alternatively, the single variable
56	.I lo
57	can be used to specify a brightness value for black and white output.
58	The predefined functions
59	.I ri(n),
60	.I gi(n)
61	and
62	.I bi(n)
63	give the red, green and blue input values for
64	picture
65	.I n.
66	To access a pixel that is nearby the current one, these functions
67	also accept optional x and y offsets.
68	For example,
69	.I ri(3,-2,1)
70	would return the red component of the pixel from picture 3
71	that is left 2 and up 1 from the current position.
72	Although x offsets may be as large as width of the picture,
73	y offsets are limited to a small window (+/- 32 pixels) due to efficiency
74	considerations.
75	However, it is not usually necessary to worry about this problem --
76	if the requested offset is not available, the next best pixel is
77	returned instead.
78	.PP
79	For additional convenience, the function
80	.I li(n)
81	is defined as the input brightness for picture
82	.I n.
83	This function also accepts x and y offsets.
84	.PP
85	The constant
86	.I nfiles
87	gives the number of input files present,
88	and
89	.I WE
90	gives the white efficacy (lumens/brightness) for pixel values,
91	which may be used with the
92	.I \-o
93	option or the le(n) values to convert to absolute
94	photometric units (see below).
95	The variables
96	.I x
97	and
98	.I y
99	give the current output pixel location for use in
100	spatially dependent functions, the constants
101	.I xmax
102	and
103	.I ymax
104	give the input resolution, and the constants
105	.I xres
106	and
107	.I yres
108	give the output resolution (usually the same, but see below).
109	The constant functions
110	.I "re(n), ge(n), be(n),"
111	and
112	.I le(n)
113	give the exposure values for picture
114	.I n,
115	and
116	.I pa(n)
117	gives the corresponding pixel aspect ratio.
118	Finally, for pictures with stored view parameters,
119	the functions
120	.I "Ox(n), Oy(n)"
121	and
122	.I Oz(n)
123	return the ray origin in world coordinates for the current pixel
124	in picture
125	.I n,
126	and
127	.I "Dx(n), Dy(n)"
128	and
129	.I Dz(n)
130	return the normalized ray direction.
131	In addition, the function
132	.I T(n)
133	returns the distance from the origin to the aft clipping plane
134	(or zero if there is no aft plane), and the function
135	.I S(n)
136	returns the solid angle of the current pixel in steradians
137	(always zero for parallel views).
138	If the current pixel is outside the view region,
139	.I T(n)
140	will return a negative value, and
141	.I S(n)
142	will return zero.
143	The first input picture with a view is assumed to correspond to the
144	view of the output picture, which is written into the header.
145	.PP
146	The
147	.I \-h
148	option may be used to reduce the information header size, which
149	can grow disproportionately after multiple runs of
150	.I pcomb
151	and/or
152	.I pcompos(1).
153	The
154	.I \-w
155	option can be used to suppress warning messages about invalid
156	calculations.
157	The
158	.I \-o
159	option indicates that original pixel values are to be used for the next
160	picture, undoing any previous exposure changes or color correction.
161	.PP
162	The
163	.I \-x
164	and
165	.I \-y
166	options can be used to specify the desired output resolution,
167	.I xres
168	and
169	.I yres,
170	and can be expressions involving other constants such as
171	.I xmax
172	and
173	.I ymax.
174	The constants
175	.I xres
176	and
177	.I yres
178	may also be specified in a file or expression.
179	The default output resolution is the same as the input resolution.
180	.PP
181	The
182	.I \-x
183	and
184	.I \-y
185	options must be present if there are no input files, when
186	the definitions of
187	.I ro,
188	.I go
189	and
190	.I bo
191	will be used to compute each output pixel.
192	This is useful for producing simple test pictures for various
193	purposes.
194	(Theoretically, one could write a complete renderer using just the
195	functional language...)
196	.PP
197	The standard input can be specified with a hyphen ('-').
198	A command that produces a RADIANCE picture can be given in place of a file
199	by preceeding it with an exclamation point ('!').
200	.SH EXAMPLES
201	To produce a picture showing the difference between pic1 and pic2:
202	.IP "" .2i
203	pcomb \-e 'ro=ri(1)\-ri(2);go=gi(1)\-gi(2);bo=bi(1)\-bi(2)' pic1 pic2 > diff
204	.PP
205	Or, more efficiently:
206	.IP "" .2i
207	pcomb pic1 \-s \-1 pic2 > diff
208	.PP
209	To precompute the gamma correction for a picture:
210	.IP "" .2i
211	pcomb \-e 'ro=ri(1)^.4;go=gi(1)^.4;bo=bi(1)^.4' inp.hdr > gam.hdr
212	.PP
213	To perform some special filtering:
214	.IP "" .2i
215	pcomb \-f myfilt.cal \-x xmax/2 \-y ymax/2 input.hdr > filtered.hdr
216	.PP
217	To make a picture of a dot:
218	.IP "" .2i
219	pcomb \-x 100 \-y 100 \-e 'ro=b;go=b;bo=b;b=if((x-50)^2+(y-50)^2\-25^2,0,1)' > dot
220	.SH AUTHOR
221	Greg Ward
222	.SH "SEE ALSO"
223	getinfo(1), icalc(1), pcompos(1), pfilt(1), rpict(1)