man/man1/dctimestep.1

.\" RCSid $Id: dctimestep.1,v 1.16 2019/10/23 17:00:14 greg Exp $"
.TH DCTIMESTEP 1 12/09/09 RADIANCE
.SH NAME
dctimestep - compute annual simulation time-step(s) via matrix multiplication
.SH SYNOPSIS
.B dctimestep
[
.B "\-n nsteps"
][
.B "\-h"
][
.B "\-o ospec"
][
.B "\-x xres"
][
.B "\-y yres"
][
.B "\-i{f|d}
][
.B "\-o{f|d|c}
]
.B DCspec
[
.B skyf
]
.br
.B dctimestep
[
.B "\-n nsteps"
][
.B "\-h"
][
.B "\-o ospec"
][
.B "\-i{f|d}
][
.B "\-o{f|d}
]
.B Vspec
.B Tbsdf
.B Dmat.dat
[
.B skyf
]
.SH DESCRIPTION
.I Dctimestep
has two invocation forms.
In the first form,
.I dctimestep
is given a daylight coefficient specification and an optional sky
vector or matrix, which may be read from the standard input if unspecified.
The daylight coefficients are multiplied against these sky values
and the results are written to the standard output.
This may be a list of color values or a combined Radiance image,
as explained below.
.PP
In the second form,
.I dctimestep
takes four input files, forming a matrix expression.
The first argument is the View matrix file that specifies how window output
directions are related to some set of measured values, such as an array of
illuminance points or images.
This matrix is usually computed by
.I rfluxmtx(1)
or
.I rcontrib(1)
for a particular set of windows or skylight openings.
The second argument is the window transmission matrix, or BSDF, given as
a matrix or a standard XML description.
The third argument is the Daylight matrix file that defines how sky patches
relate to input directions on the same opening.
This is usually computed using
.I rfluxmtx
with separate runs for each window or skylight orientation.
The last file is the sky contribution vector or matrix,
typically computed by
.I genskyvec(1)
or
.I gendaymtx(1),
and may be passed on the standard input.
.PP
If the input sky data lacks a header, the
.I \-n
option may be used to indicate the number of time steps, which
will be 1 for a sky vector.
The sky input file must otherwise contain the number of
columns (time steps) specified in each sky patch row,
whether it is read from the standard input or from a file.
Input starts from the first patch at the first time step, then the
first patch at the second time step, and so on.
Note that all matrix elements are RGB triplets, so the actual size
of the sky vector or matrix is three times the number of steps times
the number of sky patches.
The
.I \-if
or
.I \-id
option may be used to specify that sky data is in float or double
format, respectively, which is more efficient for large matrices.
These options are unnecessary when the sky input includes a header.
.PP
Any of the matrix or vector files may be read from a command
instead of a file by
using quotes and a beginning exclamation point ('!').
.PP
The standard output of
.I dctimestep
is either a color vector with as many RGB triplets
as there are rows in the View matrix, or a combined
.I Radiance
picture.
Which output is produced depends on the first argument.
A regular file name will be loaded and interpreted as a matrix to
generate a color results vector.
A file specification containing a '%d' format string will be
interpreted as a list of
.I Radiance
component pictures, which will be summed according to the computed
vector.
.PP
The
.I \-o
option may be used to specify a file or a set of output files
to use rather than the standard output.
If the given specification contains a '%d' format string, this
will be replaced by the time step index, starting from 0.
In this way, multiple output pictures may be produced,
or separate result vectors (one per time step).
If input is a matrix rather than a set of images, the
.I \-x
and/or
.I \-y
options may be necessary to set the output image size.
If only one dimension is specified, the other is computed based
on the number of rows in the result vectors.
.PP
A header will normally be produced on the output, unless the
.I \-h
option is specified.
The
.I \-of,
.I \-od,
or
.I \-oc
option may be used to specify IEEE float, double, or RGBE (picture) output
data, respectively.
.SH EXAMPLES
To compute workplane illuminances at 3:30pm on Feb 10th:
.IP "" .2i
gensky 2 10 15:30 | genskyvec | dctimestep workplaneDC.dmx > Ill_02-10-1530.dat
.PP
To compute an image at 10am on the equinox from a set of component images:
.IP "" .2i
gensky 3 21 10 | genskyvec | dctimestep dcomp%03d.hdr > view_03-21-10.hdr
.PP
To compute a set of illuminance contributions for Window 1 on
the Winter solstice at 2pm:
.IP "" .2i
gensky 12 21 14 | genskyvec | dctimestep IllPts.vmx Blinds20.xml Window1.dmx > Ill_12-21-14.dat
.PP
To compute Window2's contribution to an interior view at 12 noon on the Summer solstice:
.IP "" .2i
gensky 6 21 12 | genskyvec | dctimestep view%03d.hdr Blinds30.xml
Window2.dmx > view_6-21-12.hdr
.PP
To generate an hourly matrix of sensor value contributions from Skylight3
using a 3-phase calculation, where output columns are time steps:
.IP "" .2i
gendaymtx -of Tampa.wea | dctimestep WPpts.vmx
shade3.xml Skylight3.dmx > wp_win3.dat
.PP
Generate a series of pictures corresponding to timesteps
in an annual simulation:
.IP "" .2i
gendaymtx NYCity.wea | dctimestep -o tstep%04d.hdr dcomp%03d.hdr
.PP
To multiply an irradiance view matrix through a pair of XML window layers using
a given exterior daylight matrix and sky vector:
.IP "" .2i
dctimestep Illum.vmx "!rmtxop -ff Blinds1.xml Windo1.xml" Exter.dmx Jan20.sky
.PP
To multiply two matrices into a IEEE-float result with header:
.IP "" .2i
dctimestep -of Inp1.fmx Inp2.fmx > Inp1xInp2.fmx
.SH AUTHOR
Greg Ward
.SH "SEE ALSO"
gendaymtx(1), genskyvec(1), getinfo(1),
mkillum(1), rcollate(1), rcontrib(1),
rfluxmtx(1), rmtxop(1), rtrace(1), vwrays(1)
Revision:	1.17
Committed:	Fri Mar 11 02:27:02 2022 UTC (3 years, 9 months ago) by greg
Branch:	MAIN
Changes since 1.16:	+12 -1 lines
Log Message:	feat(dctimestep): Added -x and -y options to specify picture output dimensions
#	User	Rev	Content
1	greg	1.17	.\" RCSid $Id: dctimestep.1,v 1.16 2019/10/23 17:00:14 greg Exp $"
2	greg	1.1	.TH DCTIMESTEP 1 12/09/09 RADIANCE
3			.SH NAME
4	greg	1.4	dctimestep - compute annual simulation time-step(s) via matrix multiplication
5	greg	1.1	.SH SYNOPSIS
6			.B dctimestep
7	greg	1.4	[
8			.B "\-n nsteps"
9			][
10	greg	1.10	.B "\-h"
11			][
12	greg	1.4	.B "\-o ospec"
13	greg	1.5	][
14	greg	1.17	.B "\-x xres"
15			][
16			.B "\-y yres"
17			][
18	greg	1.10	.B "\-i{f\|d}
19	greg	1.8	][
20	greg	1.16	.B "\-o{f\|d\|c}
21	greg	1.4	]
22	greg	1.2	.B DCspec
23			[
24	greg	1.4	.B skyf
25	greg	1.2	]
26			.br
27			.B dctimestep
28	greg	1.4	[
29			.B "\-n nsteps"
30			][
31	greg	1.10	.B "\-h"
32			][
33	greg	1.4	.B "\-o ospec"
34	greg	1.5	][
35	greg	1.10	.B "\-i{f\|d}
36	greg	1.8	][
37			.B "\-o{f\|d}
38	greg	1.4	]
39	greg	1.1	.B Vspec
40	greg	1.12	.B Tbsdf
41	greg	1.1	.B Dmat.dat
42			[
43	greg	1.4	.B skyf
44	greg	1.1	]
45			.SH DESCRIPTION
46			.I Dctimestep
47	greg	1.2	has two invocation forms.
48			In the first form,
49			.I dctimestep
50			is given a daylight coefficient specification and an optional sky
51	greg	1.4	vector or matrix, which may be read from the standard input if unspecified.
52			The daylight coefficients are multiplied against these sky values
53			and the results are written to the standard output.
54	greg	1.2	This may be a list of color values or a combined Radiance image,
55			as explained below.
56			.PP
57			In the second form,
58			.I dctimestep
59	greg	1.1	takes four input files, forming a matrix expression.
60			The first argument is the View matrix file that specifies how window output
61			directions are related to some set of measured values, such as an array of
62			illuminance points or images.
63			This matrix is usually computed by
64	greg	1.12	.I rfluxmtx(1)
65			or
66	greg	1.3	.I rcontrib(1)
67	greg	1.1	for a particular set of windows or skylight openings.
68			The second argument is the window transmission matrix, or BSDF, given as
69	greg	1.12	a matrix or a standard XML description.
70	greg	1.1	The third argument is the Daylight matrix file that defines how sky patches
71			relate to input directions on the same opening.
72			This is usually computed using
73	greg	1.12	.I rfluxmtx
74			with separate runs for each window or skylight orientation.
75	greg	1.6	The last file is the sky contribution vector or matrix,
76			typically computed by
77			.I genskyvec(1)
78			or
79			.I gendaymtx(1),
80			and may be passed on the standard input.
81	greg	1.10	.PP
82			If the input sky data lacks a header, the
83			.I \-n
84			option may be used to indicate the number of time steps, which
85			will be 1 for a sky vector.
86	greg	1.13	The sky input file must otherwise contain the number of
87	greg	1.12	columns (time steps) specified in each sky patch row,
88			whether it is read from the standard input or from a file.
89	greg	1.10	Input starts from the first patch at the first time step, then the
90			first patch at the second time step, and so on.
91	greg	1.12	Note that all matrix elements are RGB triplets, so the actual size
92			of the sky vector or matrix is three times the number of steps times
93			the number of sky patches.
94	greg	1.5	The
95			.I \-if
96			or
97			.I \-id
98			option may be used to specify that sky data is in float or double
99	greg	1.6	format, respectively, which is more efficient for large matrices.
100	greg	1.14	These options are unnecessary when the sky input includes a header.
101	greg	1.1	.PP
102	greg	1.11	Any of the matrix or vector files may be read from a command
103			instead of a file by
104			using quotes and a beginning exclamation point ('!').
105			.PP
106	greg	1.9	The standard output of
107	greg	1.1	.I dctimestep
108	greg	1.8	is either a color vector with as many RGB triplets
109	greg	1.1	as there are rows in the View matrix, or a combined
110			.I Radiance
111			picture.
112	greg	1.2	Which output is produced depends on the first argument.
113	greg	1.1	A regular file name will be loaded and interpreted as a matrix to
114			generate a color results vector.
115			A file specification containing a '%d' format string will be
116			interpreted as a list of
117			.I Radiance
118			component pictures, which will be summed according to the computed
119			vector.
120	greg	1.4	.PP
121			The
122			.I \-o
123			option may be used to specify a file or a set of output files
124			to use rather than the standard output.
125			If the given specification contains a '%d' format string, this
126	greg	1.15	will be replaced by the time step index, starting from 0.
127	greg	1.4	In this way, multiple output pictures may be produced,
128	greg	1.6	or separate result vectors (one per time step).
129	greg	1.17	If input is a matrix rather than a set of images, the
130			.I \-x
131			and/or
132			.I \-y
133			options may be necessary to set the output image size.
134			If only one dimension is specified, the other is computed based
135			on the number of rows in the result vectors.
136	greg	1.8	.PP
137	greg	1.10	A header will normally be produced on the output, unless the
138			.I \-h
139			option is specified.
140	greg	1.8	The
141	greg	1.16	.I \-of,
142			.I \-od,
143	greg	1.8	or
144	greg	1.16	.I \-oc
145			option may be used to specify IEEE float, double, or RGBE (picture) output
146	greg	1.8	data, respectively.
147	greg	1.1	.SH EXAMPLES
148	greg	1.2	To compute workplane illuminances at 3:30pm on Feb 10th:
149			.IP "" .2i
150			gensky 2 10 15:30 \| genskyvec \| dctimestep workplaneDC.dmx > Ill_02-10-1530.dat
151			.PP
152			To compute an image at 10am on the equinox from a set of component images:
153			.IP "" .2i
154	greg	1.6	gensky 3 21 10 \| genskyvec \| dctimestep dcomp%03d.hdr > view_03-21-10.hdr
155	greg	1.2	.PP
156	greg	1.1	To compute a set of illuminance contributions for Window 1 on
157			the Winter solstice at 2pm:
158			.IP "" .2i
159			gensky 12 21 14 \| genskyvec \| dctimestep IllPts.vmx Blinds20.xml Window1.dmx > Ill_12-21-14.dat
160			.PP
161			To compute Window2's contribution to an interior view at 12 noon on the Summer solstice:
162			.IP "" .2i
163	greg	1.6	gensky 6 21 12 \| genskyvec \| dctimestep view%03d.hdr Blinds30.xml
164			Window2.dmx > view_6-21-12.hdr
165			.PP
166			To generate an hourly matrix of sensor value contributions from Skylight3
167			using a 3-phase calculation, where output columns are time steps:
168			.IP "" .2i
169	greg	1.10	gendaymtx -of Tampa.wea \| dctimestep WPpts.vmx
170	greg	1.6	shade3.xml Skylight3.dmx > wp_win3.dat
171			.PP
172			Generate a series of pictures corresponding to timesteps
173			in an annual simulation:
174			.IP "" .2i
175	greg	1.10	gendaymtx NYCity.wea \| dctimestep -o tstep%04d.hdr dcomp%03d.hdr
176	greg	1.8	.PP
177	greg	1.12	To multiply an irradiance view matrix through a pair of XML window layers using
178			a given exterior daylight matrix and sky vector:
179			.IP "" .2i
180			dctimestep Illum.vmx "!rmtxop -ff Blinds1.xml Windo1.xml" Exter.dmx Jan20.sky
181			.PP
182	greg	1.10	To multiply two matrices into a IEEE-float result with header:
183	greg	1.8	.IP "" .2i
184	greg	1.10	dctimestep -of Inp1.fmx Inp2.fmx > Inp1xInp2.fmx
185	greg	1.1	.SH AUTHOR
186			Greg Ward
187			.SH "SEE ALSO"
188	greg	1.12	gendaymtx(1), genskyvec(1), getinfo(1),
189			mkillum(1), rcollate(1), rcontrib(1),
190			rfluxmtx(1), rmtxop(1), rtrace(1), vwrays(1)