| 91 |
|
.TP |
| 92 |
|
.BI h =kf |
| 93 |
|
Divide the hemisphere using the LBNL/Klems "full" sampling basis. |
| 94 |
+ |
(Use "h=-kf" for left-handed coordinates.) |
| 95 |
|
.TP |
| 96 |
|
.BI h =kh |
| 97 |
|
Divide the hemisphere using the LBNL/Klems "half" sampling basis. |
| 98 |
+ |
(Use "h=-kh" for left-handed coordinates.) |
| 99 |
|
.TP |
| 100 |
|
.BI h =kq |
| 101 |
|
Divide the hemisphere using the LBNL/Klems "quarter" sampling basis. |
| 102 |
+ |
(Use "h=-kq" for left-handed coordinates.) |
| 103 |
|
.TP |
| 104 |
|
.BI h =rN |
| 105 |
|
Divide the hemisphere using Reinhart's substructuring of the Tregenza |
| 109 |
|
If it is not given, |
| 110 |
|
.I N |
| 111 |
|
defaults to 1, which is just the Tregenza sky. |
| 112 |
+ |
(Use "h=-rN" for left-handed coordinates.) |
| 113 |
|
.TP |
| 114 |
+ |
.BI h =cie |
| 115 |
+ |
Divide the hemisphere into CIE sky scanner directions, which is |
| 116 |
+ |
similar to Tregenza but with different starting azimuths and |
| 117 |
+ |
reversing row direction at each new altitude. |
| 118 |
+ |
(Use "h=-cie" for left-handed coordinates.) |
| 119 |
+ |
.TP |
| 120 |
|
.BI h =scN |
| 121 |
|
Subdivide the hemisphere using the Shirley-Chiu square-to-disk mapping with an |
| 122 |
|
.I NxN |
| 123 |
|
grid over the square. |
| 124 |
+ |
(Use "h=-scN" for left-handed coordinates.) |
| 125 |
|
.TP |
| 126 |
|
.BI u =[-]{X|Y|Z|ux,uy,uz} |
| 127 |
|
Orient the "up" direction for the hemisphere using the indicated axis or direction |
| 128 |
|
vector. |
| 129 |
|
.TP |
| 130 |
< |
.BI o =output.mtx |
| 131 |
< |
Send the matrix data for this receiver to the indicated output file. |
| 130 |
> |
.BI o =output_spec |
| 131 |
> |
Send the matrix data for this receiver to the indicated file or command. |
| 132 |
> |
Single or double quotes may be used to contain strings with spaces, and |
| 133 |
> |
commands must begin with an exclamation mark ('!'). |
| 134 |
|
The file format will be determined by the command-line |
| 135 |
|
.I \-fio |
| 136 |
|
option and will include an information header unless the |
| 152 |
|
In the receiver file, the |
| 153 |
|
.I source |
| 154 |
|
primitive is supported as well, and multiple receivers (and multiple output |
| 155 |
< |
matrices) are identified by different modifier names. |
| 155 |
> |
matrices) may be identified by different modifier names. |
| 156 |
> |
(Make sure that surfaces using the same modifier are grouped together, |
| 157 |
> |
and that the modifiers are unique and not used elsewhere in the |
| 158 |
> |
scene description.)\0 |
| 159 |
|
Though it may be counter-intuitive, receivers are often light sources, |
| 160 |
|
since samples end up there in a backwards ray-tracing system such as RADIANCE. |
| 161 |
|
When using local geometry, the overall aperture shape should be close to flat. |
| 173 |
|
To generate a flux transfer matrix connecting input and output apertures |
| 174 |
|
on a light pipe: |
| 175 |
|
.IP "" .3i |
| 176 |
< |
rcontrib int_aperture.rad ext_aperture.rad lpipe.rad > lpipe.mtx |
| 176 |
> |
rfluxmtx int_aperture.rad ext_aperture.rad lpipe.rad > lpipe.mtx |
| 177 |
|
.SH AUTHOR |
| 178 |
|
Greg Ward |
| 179 |
|
.SH "SEE ALSO" |
| 180 |
< |
genBSDF(1), getinfo(1), rcalc(1), rcollate(1), rcontrib(1), rmtxop(1), vwrays(1) |
| 180 |
> |
genBSDF(1), getinfo(1), pvsum(1), rcalc(1), rcollate(1), rcomb(1), rcontrib(1), |
| 181 |
> |
rcrop(1), rmtxop(1), vwrays(1), wrapBSDF(1) |
