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Comparing ray/doc/man/man1/dctimestep.1 (file contents):
Revision 1.3 by greg, Thu Jun 14 22:42:21 2012 UTC vs.
Revision 1.4 by greg, Fri Jan 11 05:07:47 2013 UTC

# Line 1 | Line 1
1   .\" RCSid $Id$"
2   .TH DCTIMESTEP 1 12/09/09 RADIANCE
3   .SH NAME
4 < dctimestep - compute annual simulation time-step via matrix multiplication
4 > dctimestep - compute annual simulation time-step(s) via matrix multiplication
5   .SH SYNOPSIS
6   .B dctimestep
7 + [
8 + .B "\-n nsteps"
9 + ][
10 + .B "\-o ospec"
11 + ]
12   .B DCspec
13   [
14 < .B skyvec
14 > .B skyf
15   ]
16   .br
17   .B dctimestep
18 + [
19 + .B "\-n nsteps"
20 + ][
21 + .B "\-o ospec"
22 + ]
23   .B Vspec
24   .B Tbsdf.xml
25   .B Dmat.dat
26   [
27 < .B skyvec
27 > .B skyf
28   ]
29   .SH DESCRIPTION
30   .I Dctimestep
# Line 22 | Line 32 | has two invocation forms.
32   In the first form,
33   .I dctimestep
34   is given a daylight coefficient specification and an optional sky
35 < vector, which may be read from the standard input if unspecified.
36 < The daylight coefficients are multiplied against this vector and the results
37 < are written to the standard output.
35 > vector or matrix, which may be read from the standard input if unspecified.
36 > The daylight coefficients are multiplied against these sky values
37 > and the results are written to the standard output.
38   This may be a list of color values or a combined Radiance image,
39   as explained below.
40   .PP
# Line 46 | Line 56 | This is usually computed using
56   with
57   .I rcontrib
58   in a separate run for each window or skylight orientation.
59 < The final input is the sky contribution vector,
59 > The final input is the sky contribution vector or matrix,
60   usually computed by
61   .I genskyvec(1),
62   which may be passed on the standard input.
# Line 68 | Line 78 | interpreted as a list of
78   .I Radiance
79   component pictures, which will be summed according to the computed
80   vector.
81 + .PP
82 + The
83 + .I \-n
84 + option may be used to compute multiple time steps in a
85 + single invocation.
86 + The sky input file must contain the number of
87 + columns specified in each sky patch row, whether it is read
88 + from the standard input or from an ASCII file.
89 + The columns do not need to be given on the same
90 + line, so long as the number of values totals 3*Nsteps*Npatches.
91 + Input starts from the first patch at the first time step, then the
92 + first patch at the second time step, and so on.
93 + .PP
94 + The
95 + .I \-o
96 + option may be used to specify a file or a set of output files
97 + to use rather than the standard output.
98 + If the given specification contains a '%d' format string, this
99 + will be replaced by the time step index, starting from 1.
100 + In this way, multiple output pictures may be produced,
101 + or separate results vector (one per time step).
102   .SH EXAMPLES
103   To compute workplane illuminances at 3:30pm on Feb 10th:
104   .IP "" .2i

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