9 |
|
][ |
10 |
|
.B "\-h" |
11 |
|
][ |
12 |
< |
.B "\-d|\-s" |
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. |
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 |