7 |
|
[ |
8 |
|
.B "\-n nsteps" |
9 |
|
][ |
10 |
+ |
.B "\-h" |
11 |
+ |
][ |
12 |
|
.B "\-o ospec" |
13 |
|
][ |
14 |
|
.B "\-i{f|d} |
15 |
+ |
][ |
16 |
+ |
.B "\-o{f|d} |
17 |
|
] |
18 |
|
.B DCspec |
19 |
|
[ |
24 |
|
[ |
25 |
|
.B "\-n nsteps" |
26 |
|
][ |
27 |
+ |
.B "\-h" |
28 |
+ |
][ |
29 |
|
.B "\-o ospec" |
30 |
|
][ |
31 |
|
.B "\-i{f|d} |
32 |
+ |
][ |
33 |
+ |
.B "\-o{f|d} |
34 |
|
] |
35 |
|
.B Vspec |
36 |
|
.B Tbsdf.xml |
77 |
|
This data is assumed by default to be in ASCII format, whereas the |
78 |
|
formats of the View and Daylight matrices |
79 |
|
are detected automatically if given as binary data. |
80 |
+ |
.PP |
81 |
+ |
If the input sky data lacks a header, the |
82 |
+ |
.I \-n |
83 |
+ |
option may be used to indicate the number of time steps, which |
84 |
+ |
will be 1 for a sky vector. |
85 |
+ |
The sky input file must contain the number of |
86 |
+ |
columns specified in each sky patch row, whether it is read |
87 |
+ |
from the standard input or from a file. |
88 |
+ |
Input starts from the first patch at the first time step, then the |
89 |
+ |
first patch at the second time step, and so on. |
90 |
|
The |
91 |
|
.I \-if |
92 |
|
or |
93 |
|
.I \-id |
94 |
|
option may be used to specify that sky data is in float or double |
95 |
|
format, respectively, which is more efficient for large matrices. |
96 |
< |
(Note that binary double data may not be read from stdin.)\0 |
96 |
> |
These options are unnecessary in the when the sky |
97 |
> |
input has a header. |
98 |
|
.PP |
99 |
< |
Sent to the standard output of |
99 |
> |
Any of the matrix or vector files may be read from a command |
100 |
> |
instead of a file by |
101 |
> |
using quotes and a beginning exclamation point ('!'). |
102 |
> |
.PP |
103 |
> |
The standard output of |
104 |
|
.I dctimestep |
105 |
< |
is either an ASCII color vector with as many RGB triplets |
105 |
> |
is either a color vector with as many RGB triplets |
106 |
|
as there are rows in the View matrix, or a combined |
107 |
|
.I Radiance |
108 |
|
picture. |
116 |
|
vector. |
117 |
|
.PP |
118 |
|
The |
96 |
– |
.I \-n |
97 |
– |
option may be used to compute multiple time steps in a |
98 |
– |
single invocation. |
99 |
– |
The sky input file must contain the number of |
100 |
– |
columns specified in each sky patch row, whether it is read |
101 |
– |
from the standard input or from a file. |
102 |
– |
The columns do not need to be given on the same |
103 |
– |
line, so long as the number of values totals 3*Nsteps*Npatches. |
104 |
– |
Input starts from the first patch at the first time step, then the |
105 |
– |
first patch at the second time step, and so on. |
106 |
– |
.PP |
107 |
– |
The |
119 |
|
.I \-o |
120 |
|
option may be used to specify a file or a set of output files |
121 |
|
to use rather than the standard output. |
123 |
|
will be replaced by the time step index, starting from 1. |
124 |
|
In this way, multiple output pictures may be produced, |
125 |
|
or separate result vectors (one per time step). |
126 |
+ |
.PP |
127 |
+ |
A header will normally be produced on the output, unless the |
128 |
+ |
.I \-h |
129 |
+ |
option is specified. |
130 |
+ |
The |
131 |
+ |
.I \-of |
132 |
+ |
or |
133 |
+ |
.I \-od |
134 |
+ |
option may be used to specify IEEE float or double binary output |
135 |
+ |
data, respectively. |
136 |
|
.SH EXAMPLES |
137 |
|
To compute workplane illuminances at 3:30pm on Feb 10th: |
138 |
|
.IP "" .2i |
155 |
|
To generate an hourly matrix of sensor value contributions from Skylight3 |
156 |
|
using a 3-phase calculation, where output columns are time steps: |
157 |
|
.IP "" .2i |
158 |
< |
gendaymtx -of Tampa.wea | dctimestep -if -n 8760 WPpts.vmx |
158 |
> |
gendaymtx -of Tampa.wea | dctimestep WPpts.vmx |
159 |
|
shade3.xml Skylight3.dmx > wp_win3.dat |
160 |
|
.IP "" .2i |
161 |
|
.PP |
162 |
|
Generate a series of pictures corresponding to timesteps |
163 |
|
in an annual simulation: |
164 |
|
.IP "" .2i |
165 |
< |
gendaymtx NYCity.wea | dctimestep -n 8760 -o tstep%04d.hdr dcomp%03d.hdr |
165 |
> |
gendaymtx NYCity.wea | dctimestep -o tstep%04d.hdr dcomp%03d.hdr |
166 |
> |
.PP |
167 |
> |
To multiply two matrices into a IEEE-float result with header: |
168 |
> |
.IP "" .2i |
169 |
> |
dctimestep -of Inp1.fmx Inp2.fmx > Inp1xInp2.fmx |
170 |
|
.SH AUTHOR |
171 |
|
Greg Ward |
172 |
|
.SH "SEE ALSO" |
173 |
< |
gendaymtx(1), genklemsamp(1), genskyvec(1), |
174 |
< |
mkillum(1), rcollate(1), rcontrib(1), rtrace(1), vwrays(1) |
173 |
> |
gendaymtx(1), genklemsamp(1), genskyvec(1), getinfo(1), |
174 |
> |
mkillum(1), rcollate(1), rcontrib(1), rmtxop(1), rtrace(1), vwrays(1) |