9 |
|
][ |
10 |
|
.B \-V |
11 |
|
][ |
12 |
< |
.B \-c |
12 |
> |
.B "\-c count" |
13 |
|
][ |
14 |
|
.B \-fo |
15 |
|
| |
58 |
|
(No search takes place if a file name begins with a '.', '/' or '~' |
59 |
|
character.)\0 |
60 |
|
.PP |
61 |
+ |
If the |
62 |
+ |
.I \-n |
63 |
+ |
option is specified with a value greater than 1, multiple |
64 |
+ |
.I rtrace |
65 |
+ |
processes will be used to accelerate computation on a shared |
66 |
+ |
memory machine. |
67 |
+ |
Note that there is no benefit to using more processes |
68 |
+ |
than there are local CPUs available to do the work, and the |
69 |
+ |
.I rtcontrib |
70 |
+ |
process itself may use a considerable amount of CPU time. |
71 |
+ |
.PP |
72 |
|
By setting the boolean |
73 |
|
.I \-V |
74 |
|
option, you may instruct |
97 |
|
.I \-V- |
98 |
|
coefficients contain an additonal factor of PI. |
99 |
|
.PP |
100 |
+ |
The |
101 |
+ |
.I \-c |
102 |
+ |
option tells |
103 |
+ |
.I rtcontrib |
104 |
+ |
how many rays to accumulate for each record. |
105 |
+ |
The default value is 1, meaning a full record will be produced for |
106 |
+ |
each input ray. |
107 |
+ |
For values greater than 1, contributions will be averaged together |
108 |
+ |
over the given number of input rays. |
109 |
+ |
If set to zero, only a single record will be produced at the very |
110 |
+ |
end, corresponding to the sum of all rays given on the input |
111 |
+ |
(rather than the average). |
112 |
+ |
This is equivalent to passing all the output records through a program like |
113 |
+ |
.I total(1) |
114 |
+ |
to sum RGB values together, but is much more efficient. |
115 |
+ |
Using this option, it is possible to reverse sampling, sending rays from |
116 |
+ |
a parallel source such as the sun to a diffuse surface, for example. |
117 |
+ |
Note that output flushing via zero-direction rays is disabled |
118 |
+ |
for accumulated evaluations. |
119 |
+ |
.PP |
120 |
|
The output of |
121 |
|
.I rtcontrib |
122 |
|
has many potential uses. |
128 |
|
can be used to compute arbitrary input-output relationships in optical |
129 |
|
systems, such as luminaires, light pipes, and shading devices. |
130 |
|
.PP |
100 |
– |
Setting the |
101 |
– |
.I \-c |
102 |
– |
option instructs |
103 |
– |
.I rtcontrib |
104 |
– |
to accumulate values rather than reporting one record per ray. |
105 |
– |
With this option, only a single record will be produced at the very |
106 |
– |
end, corresponding to the sum of all rays given on the input. |
107 |
– |
This is equivalent to passing all the output records through a program like |
108 |
– |
.I total(1) |
109 |
– |
to sum RGB values together, but is much more efficient. |
110 |
– |
Using this option, it is possible to reverse sampling, sending rays from |
111 |
– |
a parallel source such as the sun to a diffuse surface, for example. |
112 |
– |
Care must be taken to perform normalization based on the |
113 |
– |
radiation density and the number of rays sampled. |
114 |
– |
.PP |
131 |
|
.I Rtcontrib |
132 |
|
calls |
133 |
|
.I rtrace(1) |
146 |
|
.I \-r |
147 |
|
option is specified, data recovery is attempted on existing files. |
148 |
|
(If |
149 |
< |
.I \-c |
149 |
> |
.I "\-c 0" |
150 |
|
is used together with the |
151 |
|
.I \-r |
152 |
|
option, existing files are read in and new ray evaluations are added |
258 |
|
suitable for manipulation with |
259 |
|
.I pcomb(1) |
260 |
|
and related tools. |
245 |
– |
.PP |
246 |
– |
If the |
247 |
– |
.I \-n |
248 |
– |
option is specified with a value greater than 1, multiple |
249 |
– |
.I rtrace |
250 |
– |
processes will be used to accelerate computation on a shared |
251 |
– |
memory machine. |
252 |
– |
Note that there is no benefit to using more processes |
253 |
– |
than there are local CPUs available to do the work, and the |
254 |
– |
.I rtcontrib |
255 |
– |
process itself may use a considerable amount of CPU time. |
261 |
|
.PP |
262 |
|
Options may be given on the command line and/or read from the |
263 |
|
environment and/or read from a file. |