7 |
|
[ |
8 |
|
.B "\-n nprocs" |
9 |
|
][ |
10 |
+ |
.B \-r |
11 |
+ |
][ |
12 |
|
.B "\-e expr" |
13 |
|
][ |
14 |
|
.B "\-f source" |
15 |
|
][ |
16 |
< |
.B "\-o fspec" |
16 |
> |
.B "\-o ospec" |
17 |
|
][ |
18 |
|
.B "\-b binv" |
19 |
+ |
][ |
20 |
+ |
.B "\-bn nbins" |
21 |
|
] |
22 |
< |
.B "\-m mod .." |
22 |
> |
{ |
23 |
> |
.B "\-m mod | \-M file" |
24 |
> |
} |
25 |
> |
.. |
26 |
|
[ |
27 |
|
.B $EVAR |
28 |
|
] |
44 |
|
These modifiers are usually materials associated with |
45 |
|
light sources or sky domes, and must directly modify some geometric |
46 |
|
primitives to be considered in the output. |
47 |
+ |
A modifier list may also be read from a file using the |
48 |
+ |
.I \-M |
49 |
+ |
option. |
50 |
+ |
The RAYPATH environment variable determines directories to search for |
51 |
+ |
this file. |
52 |
+ |
(No search takes place if a file name begins with a '.', '/' or '~' |
53 |
+ |
character.)\0 |
54 |
+ |
.PP |
55 |
|
The output of |
56 |
|
.I rtcontrib |
57 |
|
has many potential uses. |
68 |
|
.I rtrace(1) |
69 |
|
with the -oTW option to calculate the daughter ray |
70 |
|
contributions for each input ray, and the output tallies |
71 |
< |
are sent to one or more files according to the given |
71 |
> |
are sent to one or more destinations according to the given |
72 |
|
.I \-o |
73 |
|
specification. |
74 |
+ |
If a destination begins with an exclamation mark ('!'), then |
75 |
+ |
a pipe is opened to a command and data is sent to its standard input. |
76 |
+ |
Otherwise, the destination is treated as a file. |
77 |
+ |
An existing file of the same name is clobbered, unless the |
78 |
+ |
.I \-r |
79 |
+ |
option is specified, in which case data recovery is attempted. |
80 |
|
If an output specification contains a "%s" format, this will be |
81 |
|
replaced by the modifier name. |
82 |
|
The |
87 |
|
specification if present. |
88 |
|
The actual bin number is computed at run time based on ray direction |
89 |
|
and surface intersection, as described below. |
90 |
+ |
If the number of bins is known in advance, it should be specified with the |
91 |
+ |
.I \-bn |
92 |
+ |
option, and this is critical for output files containing multiple values |
93 |
+ |
per record. |
94 |
+ |
Since bin numbers start from 0, the bin count is always equal to |
95 |
+ |
the last bin plus 1. |
96 |
+ |
Set the this value to 0 if the bin count is unknown (the default). |
97 |
|
The most recent |
98 |
< |
.I \-b |
98 |
> |
.I \-b, |
99 |
> |
.I \-bn |
100 |
|
and |
101 |
|
.I \-o |
102 |
|
options to the left of each |
134 |
|
will search the RADIANCE library directories for each file given in a |
135 |
|
.I \-f |
136 |
|
option. |
108 |
– |
(No search takes place if a file name begins with a '.', '/' or '~' |
109 |
– |
character.)\0 |
137 |
|
.PP |
138 |
|
If no |
139 |
|
.I \-o |
140 |
|
specification is given, results are written on the standard output in order |
141 |
|
of modifier (as given on the command line) then bin number. |
142 |
< |
Concatenated data is also sent to a lone output file (i.e., an initial |
142 |
> |
Concatenated data is also sent to a single destination (i.e., an initial |
143 |
|
.I \-o |
144 |
|
specification without formatting strings). |
145 |
|
If a "%s" format appears but no "%d" in the |
214 |
|
.PP |
215 |
|
To compute an array of illuminance contributions according to a Tregenza sky: |
216 |
|
.IP "" .2i |
217 |
< |
rtcontrib -b tbin -o sky.dat -m skyglow -b 0 -o ground.dat -m groundglow |
217 |
> |
rtcontrib -I+ -b tbin -o sky.dat -m skyglow -b 0 -o ground.dat -m groundglow |
218 |
|
@render.opt -f tregenza.cal scene.oct < test.dat |
219 |
|
.SH ENVIRONMENT |
220 |
< |
RAYPATH path to search for -f files |
220 |
> |
RAYPATH path to search for -f and -M files |
221 |
|
.SH AUTHOR |
222 |
|
Greg Ward |
223 |
|
.SH "SEE ALSO" |