11 |
|
][ |
12 |
|
.B "\-A" |
13 |
|
][ |
14 |
< |
.B "\-d|\-s" |
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" |
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 |