man/man1/rcomb.1

.\" RCSid "$Id: rcomb.1,v 1.1 2023/12/12 16:31:45 greg Exp $"
.TH RCOMB 12/5/2023 RADIANCE
.SH NAME
rcomb - combine and convert matrices a row at a time
.SH SYNOPSIS
.B rcomb
[
.B \-h
][
.B \-w
][
.B \-f[afdc]
][
.B "\-f file"
][
.B "\-e expr"
][
.B "\-C {symbols|file}"
][
.B "\-c ce .."
][
.B "\-s sf .."
]
.B "m1 .."
[
.B "\-m mcat"
]
.SH DESCRIPTION
.I Rcomb
combines inputs given on the command line,
one matrix row or picture scanline at a time.
By default, the result is a linear combination of
the matrix elements or pixels transformed by
.I \-c
specifications and scaled by
.I \-s
coefficients, but an arbitrary mapping can be assigned with the
.I \-e
and
.I \-f
options, similar to the
.I pcomb(1)
and
.I rcalc(1)
commands.
(The definitions in each
.I \-f source
file are read and compiled from the RADIANCE library where it is found.)\0
.PP
If any
.I \-c
or
.I \-s
options follow the last input matrix, output results will be transformed
and/or scaled accordingly.
These operations are discussed in greater detail further on.
A single concatenation matrix may be applied after element operations
using the
.I \-m
option.
Matrix concatenation will happen before or after any trailing
operations, depending on relative command line placement.
.PP
Each input file must have a header containing the following metadata:
.sp
.nf
NROWS={number of rows}
NCOLS={number of columns}
NCOMP={number of components}
FORMAT={ascii|float|double|32-bit_rle_rgbe|32-bit_rle_xyze|Radiance_spectra}
.fi
.sp
The number of components indicates that each matrix element is actually
composed of multiple elements, most commonly an RGB triple.
This is essentially dividing the matrix into planes, where each component
participates in a separate calculation.
If an appropriate header is not present, it may be added with a call to
.I rcollate(1).
A matrix may be read from the standard input using a hyphen by itself ('-')
in the appropriate place on the command line.
Similarly, any of the inputs may be read from a command
instead of a file by
using quotes and a beginning exclamation point ('!').
.PP
In the case of Radiance picture files,
the number of columns is the X-dimension of the picture, and
the number of rows is the Y-dimension.
The picture must be in standard pixel ordering, and the zeroeth row
is at the top with the zeroeth column on the left.
Any exposure changes that were applied to the pictures before
.I rcomb
will be undone, similar to the
.I "pcomb \-o"
option.
Radiance spectral pictures with more than 3 components are also supported.
These are typically produced by
.I rtrace(1)
or
.I rfluxmtx(1).
.PP
Before each input, the
.I \-c
and/or
.I \-s
options may be used to modify the matrix elements.
The
.I \-c
option can "transform" the element values, possibly changing
the number of components in the matrix.
For example, a 3-component matrix can be transformed into a single-component
matrix by using
.I \-c
with three coefficients.
A four-component matrix can be turned into a two-component matrix using 8
coefficients, where the first four coefficients will be used to compute
the first new component, and the second four coefficients
yield the second new component.
Note that the number of coefficients must be an even multiple of the number
of original components.
.PP
Alternatively, a set of symbolic output components may be given to the
.I \-c
option, with the following definitions:
.sp
.nf
R       - red channel
G       - green channel
B       - blue channel
X       - CIE X channel
Y       - CIE Y channel (aka., luminance or illuminance)
Z       - CIE Z channel
S       - scotopic luminance or illuminance
M       - melanopic luminance or illuminance
A       - average component value
.fi
.sp
These letters may be given in any order as a single string, and if
.I "-c RGB"
or
.I "-c XYZ"
is specified for an input picture or the
.I "-fc"
option is given, the output will be written as a RGBE or XYZE picture.
Note that conversion from a float or RGBE color space applies a conversion
of 179 lumens/watt (for CIE or melanopic output) or 412 (for scotopic output),
and the reverse happens for conversion from XYZE input to RGB or RGBE output.
.PP
If a matrix or picture file path is given to the
.I \-c
option, then the color space of that file will be used, instead.
.PP
The
.I \-C
option takes either a symbolic color space or an input file, and will be
applied to all subsequent matrices that do not have their own associated
.I \-c
option.
.PP
Additionally, the
.I \-s
option applies the given scalar factor(s) to the elements of the matrix.
If only one factor is provided,
it will be used for all components.
If multiple factors are given, their number must match the number of matrix
components
.I after
application of any
.I \-c
option for this input matrix or picture, even if the
.I \-s
option appears first.
.PP
The number of components in all input
matrices after applying any
.I -c
transform must agree.
Similarly, the number of rows and columns of all results must match
exactly.
(The
.I rcrop(1)
utility may be used to trim inputs if necessary.)\0
.PP
If the
.I \-e
or
.I \-f
options are used to define a "co" variable or "co(p)" function,
this will be evaluated at each output
component for the current element.
The "co" variable defines identical operations for all components,
whereas "co(p)" may specify different operations for each component.
The element position is defined
by the "r" and "c" variables, where
.I r
goes from 0 to "nrows" minus one, and
.I c
goes from 0 to "ncols" minus one.
(Note that "nrows" may be zero if unspecified in inputs, and this
is a unique capability of
.I rcomb
to handle these.)\0
Component p from input i is accessed with the "ci(i,p)" function,
and the number of components is defined by the "ncomp" constant.
If given as "ci(i)", the function returns the current component
being evaluated by
.I rcomb.
A different component may be referenced using th second argument.
For example, "ci(1,2)" accesses
the second component from the first input.
If the input is a picture, the the constants "R", "G", and "B"
are conveniently defined as the channel numbers 1, 2, and 3,
respectively.
For color or spectral inputs, the function "wl(p)" gives the
central wavelength for channel
.I p
in nanometers.
For convenience and compatibility with
.I pcomb,
the functions "ri(i)", "gi(i)", and "bi(i)" are predefined as
"ci(i,R)", "ci(i,G)", and "ci(i,B)", respectively.
Accordingly, the "ro", "go", and "bo" 
variables may be used in place of "co(R)", "co(G)", and "co(B)".
Finally, the total number of input files is set in the constant "nfiles".
.PP
Results are sent to the standard output.
By default, the values will be written in the lowest precision format
among the inputs, but the
.I \-f[adfc]
option may be used to explicitly output components
as ASCII (-fa), binary doubles (-fd), floats (-ff), or common-exponent
colors/spectra (-fc).
In the latter case, the actual matrix dimensions are written in the resolution string rather than the header.
Also, matrix results will be written as standard
Radiance pictures if they have either one
or three components.
In the one-component case, the output is written as grayscale.
If more than 3 components are in the final matrix and
.I -fc
is specified, the output will be a Radiance spectral picture.
.PP
The
.I \-h
option may be used to reduce the information header size, which
can grow disproportionately, otherwise.
The
.I \-w
option turns off warnings about divide-by-zero and other non-fatal
calculation errors.
.SH EXAMPLES
To convert two hyperspectral inputs to RGB color space,
average them together, and write them out as a RADIANCE picture:
.IP "" .2i
rcomb -C RGB -s .5 img1.spc -s .5 img2.spc > avg.hdr
.PP
Divide one set of matrix elements by the Euclidean sum of two others:
.IP "" .2i
rcomb -e "co=ci(1)/sqrt(ci(2)^2+ci(3)^2)" inp1.mtx 
inp2.mtx inp3.mtx > out.mtx
.PP
Compute the absolute and relative differences between melanopic and photopic values
in a spectral image:
.IP "" .2i
rcomb -fa -C MY -e "abs(x):if(x,x,-x)"
-e "co(p)=select(p,abs(ci(1,1)-ci(1,2)),(ci(1,1)-ci(1,2))/ci(1,2))"
input_spec.hsr > compare.mtx
.PP
Concatenate a spectral flux coefficient matrix with a spectral sky
matrix to compute a set of melanopic lux values:
.IP "" .2i
rcomb view_spec.mtx -m sky_spec.mtx -c M > melux.mtx
.SH NOTES
The
.I rcomb
tool was created to overcome some limitations of
.I rmtxop
and
.I pcomb,
whose capabilities somewhat overlap.
The former loads each matrix into memory before operations,
and element components take 8 bytes apiece, adding up quickly.
Very large matrices therefore present a problem with that tool.
Furthermore, 
.I rmtxop
does not allow arbitrary expressions, limiting
what can be accomplished easily on the command-line.
In contrast,
.I pcomb
is fully programmable and operates on its input using a
scanline window, so it can handle much larger input dimensions.
It also handles single- and three-component float matrices on
input and output, but unlike
.I rmtxop,
.I pcomb
has not been extended to handle RADIANCE hyperspectral images
or more general matrix data.
.PP
The
.I rcomb
tool is a compromise that exceeds the capabilities of either of
its predecessors in certain circumstances.
In particular, very large matrices may be combined using
arbitrary, user-defined operations, and the convenient
color conversions of
.I rmtxop
are supported for both input and output.
Finally, a single matrix may be concatenated after operations,
permitting a flux transfer matrix with millions of rows to
pass through.
Generally speaking,
.I rcomb
should be preferred over
.I rmtxop
for any operations in can handle, which is everything except
multiple matrix concatenations and transpose
operations, which are handled more efficiently by
.I rcollate(1)
in any case.
That said, there is no significant difference for
simple operations on smallish matrices, and note that only
.I rmtxop
and
.I dctimestep(1)
currently accept XML files as inputs.
Also, the resizing function of
.I pcomb
is not supported in
.I rcomb,
and should instead be handled by
.I pfilt(1).
.SH AUTHOR
Greg Ward
.SH "SEE ALSO"
dctimestep(1), icalc(1), getinfo(1), pcomb(1), pfilt(1),
ra_xyze(1), rcalc(1),
rcollate(1), rcontrib(1), rcrop(1), rfluxmtx(1), 
rmtxop(1), rtpict(1), rtrace(1), vwrays(1)
Revision:	1.2
Committed:	Mon Dec 18 23:04:05 2023 UTC (22 months, 2 weeks ago) by greg
Branch:	MAIN
Changes since 1.1:	+5 -1 lines
Log Message:	fix(rcomb): Fixed handling of matrix inputs where NROWS is unspecified
#	User	Rev	Content
1	greg	1.2	.\" RCSid "$Id: rcomb.1,v 1.1 2023/12/12 16:31:45 greg Exp $"
2	greg	1.1	.TH RCOMB 12/5/2023 RADIANCE
3			.SH NAME
4			rcomb - combine and convert matrices a row at a time
5			.SH SYNOPSIS
6			.B rcomb
7			[
8			.B \-h
9			][
10			.B \-w
11			][
12			.B \-f[afdc]
13			][
14			.B "\-f file"
15			][
16			.B "\-e expr"
17			][
18			.B "\-C {symbols\|file}"
19			][
20			.B "\-c ce .."
21			][
22			.B "\-s sf .."
23			]
24			.B "m1 .."
25			[
26			.B "\-m mcat"
27			]
28			.SH DESCRIPTION
29			.I Rcomb
30			combines inputs given on the command line,
31			one matrix row or picture scanline at a time.
32			By default, the result is a linear combination of
33			the matrix elements or pixels transformed by
34			.I \-c
35			specifications and scaled by
36			.I \-s
37			coefficients, but an arbitrary mapping can be assigned with the
38			.I \-e
39			and
40			.I \-f
41			options, similar to the
42			.I pcomb(1)
43			and
44			.I rcalc(1)
45			commands.
46			(The definitions in each
47			.I \-f source
48			file are read and compiled from the RADIANCE library where it is found.)\0
49			.PP
50			If any
51			.I \-c
52			or
53			.I \-s
54			options follow the last input matrix, output results will be transformed
55			and/or scaled accordingly.
56			These operations are discussed in greater detail further on.
57			A single concatenation matrix may be applied after element operations
58			using the
59			.I \-m
60			option.
61			Matrix concatenation will happen before or after any trailing
62			operations, depending on relative command line placement.
63			.PP
64			Each input file must have a header containing the following metadata:
65			.sp
66			.nf
67			NROWS={number of rows}
68			NCOLS={number of columns}
69			NCOMP={number of components}
70			FORMAT={ascii\|float\|double\|32-bit_rle_rgbe\|32-bit_rle_xyze\|Radiance_spectra}
71			.fi
72			.sp
73			The number of components indicates that each matrix element is actually
74			composed of multiple elements, most commonly an RGB triple.
75			This is essentially dividing the matrix into planes, where each component
76			participates in a separate calculation.
77			If an appropriate header is not present, it may be added with a call to
78			.I rcollate(1).
79			A matrix may be read from the standard input using a hyphen by itself ('-')
80			in the appropriate place on the command line.
81			Similarly, any of the inputs may be read from a command
82			instead of a file by
83			using quotes and a beginning exclamation point ('!').
84			.PP
85			In the case of Radiance picture files,
86			the number of columns is the X-dimension of the picture, and
87			the number of rows is the Y-dimension.
88			The picture must be in standard pixel ordering, and the zeroeth row
89			is at the top with the zeroeth column on the left.
90			Any exposure changes that were applied to the pictures before
91			.I rcomb
92			will be undone, similar to the
93			.I "pcomb \-o"
94			option.
95			Radiance spectral pictures with more than 3 components are also supported.
96			These are typically produced by
97			.I rtrace(1)
98			or
99			.I rfluxmtx(1).
100			.PP
101			Before each input, the
102			.I \-c
103			and/or
104			.I \-s
105			options may be used to modify the matrix elements.
106			The
107			.I \-c
108			option can "transform" the element values, possibly changing
109			the number of components in the matrix.
110			For example, a 3-component matrix can be transformed into a single-component
111			matrix by using
112			.I \-c
113			with three coefficients.
114			A four-component matrix can be turned into a two-component matrix using 8
115			coefficients, where the first four coefficients will be used to compute
116			the first new component, and the second four coefficients
117			yield the second new component.
118			Note that the number of coefficients must be an even multiple of the number
119			of original components.
120			.PP
121			Alternatively, a set of symbolic output components may be given to the
122			.I \-c
123			option, with the following definitions:
124			.sp
125			.nf
126			R - red channel
127			G - green channel
128			B - blue channel
129			X - CIE X channel
130			Y - CIE Y channel (aka., luminance or illuminance)
131			Z - CIE Z channel
132			S - scotopic luminance or illuminance
133			M - melanopic luminance or illuminance
134			A - average component value
135			.fi
136			.sp
137			These letters may be given in any order as a single string, and if
138			.I "-c RGB"
139			or
140			.I "-c XYZ"
141			is specified for an input picture or the
142			.I "-fc"
143			option is given, the output will be written as a RGBE or XYZE picture.
144			Note that conversion from a float or RGBE color space applies a conversion
145			of 179 lumens/watt (for CIE or melanopic output) or 412 (for scotopic output),
146			and the reverse happens for conversion from XYZE input to RGB or RGBE output.
147			.PP
148			If a matrix or picture file path is given to the
149			.I \-c
150			option, then the color space of that file will be used, instead.
151			.PP
152			The
153			.I \-C
154			option takes either a symbolic color space or an input file, and will be
155			applied to all subsequent matrices that do not have their own associated
156			.I \-c
157			option.
158			.PP
159			Additionally, the
160			.I \-s
161			option applies the given scalar factor(s) to the elements of the matrix.
162			If only one factor is provided,
163			it will be used for all components.
164			If multiple factors are given, their number must match the number of matrix
165			components
166			.I after
167			application of any
168			.I \-c
169			option for this input matrix or picture, even if the
170			.I \-s
171			option appears first.
172			.PP
173			The number of components in all input
174			matrices after applying any
175			.I -c
176			transform must agree.
177			Similarly, the number of rows and columns of all results must match
178			exactly.
179			(The
180			.I rcrop(1)
181			utility may be used to trim inputs if necessary.)\0
182			.PP
183			If the
184			.I \-e
185			or
186			.I \-f
187			options are used to define a "co" variable or "co(p)" function,
188			this will be evaluated at each output
189			component for the current element.
190			The "co" variable defines identical operations for all components,
191			whereas "co(p)" may specify different operations for each component.
192			The element position is defined
193			by the "r" and "c" variables, where
194			.I r
195			goes from 0 to "nrows" minus one, and
196			.I c
197			goes from 0 to "ncols" minus one.
198	greg	1.2	(Note that "nrows" may be zero if unspecified in inputs, and this
199			is a unique capability of
200			.I rcomb
201			to handle these.)\0
202	greg	1.1	Component p from input i is accessed with the "ci(i,p)" function,
203			and the number of components is defined by the "ncomp" constant.
204			If given as "ci(i)", the function returns the current component
205			being evaluated by
206			.I rcomb.
207			A different component may be referenced using th second argument.
208			For example, "ci(1,2)" accesses
209			the second component from the first input.
210			If the input is a picture, the the constants "R", "G", and "B"
211			are conveniently defined as the channel numbers 1, 2, and 3,
212			respectively.
213			For color or spectral inputs, the function "wl(p)" gives the
214			central wavelength for channel
215			.I p
216			in nanometers.
217			For convenience and compatibility with
218			.I pcomb,
219			the functions "ri(i)", "gi(i)", and "bi(i)" are predefined as
220			"ci(i,R)", "ci(i,G)", and "ci(i,B)", respectively.
221			Accordingly, the "ro", "go", and "bo"
222			variables may be used in place of "co(R)", "co(G)", and "co(B)".
223			Finally, the total number of input files is set in the constant "nfiles".
224			.PP
225			Results are sent to the standard output.
226			By default, the values will be written in the lowest precision format
227			among the inputs, but the
228			.I \-f[adfc]
229			option may be used to explicitly output components
230			as ASCII (-fa), binary doubles (-fd), floats (-ff), or common-exponent
231			colors/spectra (-fc).
232			In the latter case, the actual matrix dimensions are written in the resolution string rather than the header.
233			Also, matrix results will be written as standard
234			Radiance pictures if they have either one
235			or three components.
236			In the one-component case, the output is written as grayscale.
237			If more than 3 components are in the final matrix and
238			.I -fc
239			is specified, the output will be a Radiance spectral picture.
240			.PP
241			The
242			.I \-h
243			option may be used to reduce the information header size, which
244			can grow disproportionately, otherwise.
245			The
246			.I \-w
247			option turns off warnings about divide-by-zero and other non-fatal
248			calculation errors.
249			.SH EXAMPLES
250			To convert two hyperspectral inputs to RGB color space,
251			average them together, and write them out as a RADIANCE picture:
252			.IP "" .2i
253			rcomb -C RGB -s .5 img1.spc -s .5 img2.spc > avg.hdr
254			.PP
255			Divide one set of matrix elements by the Euclidean sum of two others:
256			.IP "" .2i
257			rcomb -e "co=ci(1)/sqrt(ci(2)^2+ci(3)^2)" inp1.mtx
258			inp2.mtx inp3.mtx > out.mtx
259			.PP
260			Compute the absolute and relative differences between melanopic and photopic values
261			in a spectral image:
262			.IP "" .2i
263			rcomb -fa -C MY -e "abs(x):if(x,x,-x)"
264			-e "co(p)=select(p,abs(ci(1,1)-ci(1,2)),(ci(1,1)-ci(1,2))/ci(1,2))"
265			input_spec.hsr > compare.mtx
266			.PP
267			Concatenate a spectral flux coefficient matrix with a spectral sky
268			matrix to compute a set of melanopic lux values:
269			.IP "" .2i
270			rcomb view_spec.mtx -m sky_spec.mtx -c M > melux.mtx
271			.SH NOTES
272			The
273			.I rcomb
274			tool was created to overcome some limitations of
275			.I rmtxop
276			and
277			.I pcomb,
278			whose capabilities somewhat overlap.
279			The former loads each matrix into memory before operations,
280			and element components take 8 bytes apiece, adding up quickly.
281			Very large matrices therefore present a problem with that tool.
282			Furthermore,
283			.I rmtxop
284			does not allow arbitrary expressions, limiting
285			what can be accomplished easily on the command-line.
286			In contrast,
287			.I pcomb
288			is fully programmable and operates on its input using a
289			scanline window, so it can handle much larger input dimensions.
290			It also handles single- and three-component float matrices on
291			input and output, but unlike
292			.I rmtxop,
293			.I pcomb
294			has not been extended to handle RADIANCE hyperspectral images
295			or more general matrix data.
296			.PP
297			The
298			.I rcomb
299			tool is a compromise that exceeds the capabilities of either of
300			its predecessors in certain circumstances.
301			In particular, very large matrices may be combined using
302			arbitrary, user-defined operations, and the convenient
303			color conversions of
304			.I rmtxop
305			are supported for both input and output.
306			Finally, a single matrix may be concatenated after operations,
307			permitting a flux transfer matrix with millions of rows to
308			pass through.
309			Generally speaking,
310			.I rcomb
311			should be preferred over
312			.I rmtxop
313			for any operations in can handle, which is everything except
314			multiple matrix concatenations and transpose
315			operations, which are handled more efficiently by
316			.I rcollate(1)
317			in any case.
318			That said, there is no significant difference for
319			simple operations on smallish matrices, and note that only
320			.I rmtxop
321			and
322			.I dctimestep(1)
323			currently accept XML files as inputs.
324			Also, the resizing function of
325			.I pcomb
326			is not supported in
327			.I rcomb,
328			and should instead be handled by
329			.I pfilt(1).
330			.SH AUTHOR
331			Greg Ward
332			.SH "SEE ALSO"
333			dctimestep(1), icalc(1), getinfo(1), pcomb(1), pfilt(1),
334			ra_xyze(1), rcalc(1),
335			rcollate(1), rcontrib(1), rcrop(1), rfluxmtx(1),
336			rmtxop(1), rtpict(1), rtrace(1), vwrays(1)