7 |
|
[ |
8 |
|
.B "\-v" |
9 |
|
][ |
10 |
< |
.B "\-d|\-s" |
10 |
> |
.B "\-h" |
11 |
|
][ |
12 |
+ |
.B "\-A" |
13 |
+ |
][ |
14 |
+ |
.B "\-d|\-s|\-n" |
15 |
+ |
][ |
16 |
+ |
.B "\-D sunfile" |
17 |
+ |
][ |
18 |
|
.B "\-r deg" |
19 |
|
][ |
20 |
|
.B "\-m N" |
46 |
|
.PP |
47 |
|
Increasing the |
48 |
|
.I \-m |
49 |
< |
parameter, typically by factors of two, yields a higher resolution |
49 |
> |
parameter yields a higher resolution |
50 |
|
sky using the Reinhart patch subdivision. |
51 |
|
For example, setting |
52 |
|
.I "\-m 4" |
57 |
|
yield 8760x3 (26280) values per output line (row). |
58 |
|
.PP |
59 |
|
The |
60 |
+ |
.I \-A |
61 |
+ |
option tells |
62 |
+ |
.I gendaymtx |
63 |
+ |
to generate a single column corresponding to an average sky |
64 |
+ |
computed over all the input time steps, rather than one |
65 |
+ |
column per time step. |
66 |
+ |
.PP |
67 |
+ |
The |
68 |
|
.I \-c |
69 |
|
option may be used to specify a color for the sky. |
70 |
< |
The gray value should equal 1 for proper energy balance |
70 |
> |
The gray value should equal 1 for proper energy balance. |
71 |
|
The default sky color is |
72 |
|
.I "\-c 0.960 1.004 1.118". |
73 |
|
Similarly, the |
79 |
|
.PP |
80 |
|
The |
81 |
|
.I \-d |
82 |
< |
option may be used to produce a sun-only matrix, with no sky contributions. |
82 |
> |
option may be used to produce a sun-only matrix, with no sky contributions, |
83 |
> |
and the ground patch also set to zero. |
84 |
|
Alternatively, the |
85 |
|
.I \-s |
86 |
< |
option may be used to exclude any direct solar component from the output. |
86 |
> |
option may be used to exclude any direct solar component from the output, |
87 |
> |
with the rest of the sky and ground patch unaffected. |
88 |
> |
If there is a sun in the description, |
89 |
> |
.I gendaymtx |
90 |
> |
will include its contribution in the four nearest sky patches, |
91 |
> |
distributing energy according to centroid proximity. |
92 |
|
.PP |
93 |
+ |
The |
94 |
+ |
.I \-n |
95 |
+ |
option may be used if no matrix output is desired. |
96 |
+ |
This may be used to merely check the input, or in combination with the |
97 |
+ |
.I \-D |
98 |
+ |
option, below. |
99 |
+ |
.PP |
100 |
+ |
The |
101 |
+ |
.I \-D |
102 |
+ |
option may be used to specify an output file to contain a list of |
103 |
+ |
solar positions and intensities corresponding to time steps in the |
104 |
+ |
weather tape where the sun is visible above the horizion. |
105 |
+ |
.PP |
106 |
|
By default, |
107 |
|
.I gendaymtx |
108 |
|
assumes the positive Y-axis points north such that the first sky patch |
134 |
|
.I \-O1 |
135 |
|
option specifies that output should be total solar radiance rather |
136 |
|
than visible radiance. |
137 |
+ |
The |
138 |
+ |
.I \-h |
139 |
+ |
option prevents the output of the usual header information. |
140 |
|
Finally, the |
141 |
|
.I \-v |
142 |
|
option will enable verbose reporting, which is mostly useful for |