7 |
|
[ |
8 |
|
.B "\-n nprocs" |
9 |
|
][ |
10 |
+ |
.B \-fo |
11 |
+ |
| |
12 |
+ |
.B \-r |
13 |
+ |
][ |
14 |
|
.B "\-e expr" |
15 |
|
][ |
16 |
|
.B "\-f source" |
17 |
|
][ |
18 |
< |
.B "\-o fspec" |
18 |
> |
.B "\-o ospec" |
19 |
|
][ |
20 |
|
.B "\-b binv" |
21 |
+ |
][ |
22 |
+ |
.B "\-bn nbins" |
23 |
|
] |
24 |
< |
.B "\-m mod .." |
24 |
> |
{ |
25 |
> |
.B "\-m mod | \-M file" |
26 |
> |
} |
27 |
> |
.. |
28 |
|
[ |
29 |
|
.B $EVAR |
30 |
|
] |
46 |
|
These modifiers are usually materials associated with |
47 |
|
light sources or sky domes, and must directly modify some geometric |
48 |
|
primitives to be considered in the output. |
49 |
+ |
A modifier list may also be read from a file using the |
50 |
+ |
.I \-M |
51 |
+ |
option. |
52 |
+ |
The RAYPATH environment variable determines directories to search for |
53 |
+ |
this file. |
54 |
+ |
(No search takes place if a file name begins with a '.', '/' or '~' |
55 |
+ |
character.)\0 |
56 |
+ |
.PP |
57 |
|
The output of |
58 |
|
.I rtcontrib |
59 |
|
has many potential uses. |
70 |
|
.I rtrace(1) |
71 |
|
with the -oTW option to calculate the daughter ray |
72 |
|
contributions for each input ray, and the output tallies |
73 |
< |
are sent to one or more files according to the given |
73 |
> |
are sent to one or more destinations according to the given |
74 |
|
.I \-o |
75 |
|
specification. |
76 |
+ |
If a destination begins with an exclamation mark ('!'), then |
77 |
+ |
a pipe is opened to a command and data is sent to its standard input. |
78 |
+ |
Otherwise, the destination is treated as a file. |
79 |
+ |
An existing file of the same name will not be clobbered, unless the |
80 |
+ |
.I \-fo |
81 |
+ |
option is given. |
82 |
+ |
If instead the |
83 |
+ |
.I \-r |
84 |
+ |
option is specified, data recovery is attempted on existing files. |
85 |
|
If an output specification contains a "%s" format, this will be |
86 |
|
replaced by the modifier name. |
87 |
|
The |
92 |
|
specification if present. |
93 |
|
The actual bin number is computed at run time based on ray direction |
94 |
|
and surface intersection, as described below. |
95 |
+ |
If the number of bins is known in advance, it should be specified with the |
96 |
+ |
.I \-bn |
97 |
+ |
option, and this is critical for output files containing multiple values |
98 |
+ |
per record. |
99 |
+ |
Since bin numbers start from 0, the bin count is always equal to |
100 |
+ |
the last bin plus 1. |
101 |
+ |
Set the this value to 0 if the bin count is unknown (the default). |
102 |
|
The most recent |
103 |
< |
.I \-b |
103 |
> |
.I \-b, |
104 |
> |
.I \-bn |
105 |
|
and |
106 |
|
.I \-o |
107 |
|
options to the left of each |
133 |
|
described in the |
134 |
|
.I rcalc(1) |
135 |
|
man page. |
136 |
+ |
Unlike |
137 |
+ |
.I rcalc, |
138 |
+ |
.I rtcontrib |
139 |
+ |
will search the RADIANCE library directories for each file given in a |
140 |
+ |
.I \-f |
141 |
+ |
option. |
142 |
|
.PP |
143 |
|
If no |
144 |
|
.I \-o |
145 |
|
specification is given, results are written on the standard output in order |
146 |
|
of modifier (as given on the command line) then bin number. |
147 |
< |
Concatenated data is also sent to a lone output file (i.e., an initial |
147 |
> |
Concatenated data is also sent to a single destination (i.e., an initial |
148 |
|
.I \-o |
149 |
|
specification without formatting strings). |
150 |
|
If a "%s" format appears but no "%d" in the |
219 |
|
.PP |
220 |
|
To compute an array of illuminance contributions according to a Tregenza sky: |
221 |
|
.IP "" .2i |
222 |
< |
rtcontrib -b tbin -o sky.dat -m skyglow -b 0 -o ground.dat -m groundglow |
222 |
> |
rtcontrib -I+ -b tbin -o sky.dat -m skyglow -b 0 -o ground.dat -m groundglow |
223 |
|
@render.opt -f tregenza.cal scene.oct < test.dat |
224 |
+ |
.SH ENVIRONMENT |
225 |
+ |
RAYPATH path to search for -f and -M files |
226 |
|
.SH AUTHOR |
227 |
|
Greg Ward |
228 |
|
.SH "SEE ALSO" |