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all.zip | 2011-01-10 00:30 | 838K | ||
rect_ilcSmetanova.sh | 2016-08-11 23:22 | 7.1K | ||
r-1.5625_1.5625_-0.1875_0.875c3.125_min.htm | 2016-08-11 23:23 | 2.4K | ||
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r-1.5625_1.5625_-0.1875_0.875c3.125_min.txt | 2016-08-11 23:23 | 2.2K | ||
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scripts/ | 2011-01-10 00:29 | - | scripts and batches | |
r-1.5625_1.5625_-0.1875_0.875c3.125/ | 2016-08-11 23:22 | - | ||
photom_files/ | 2011-01-10 00:30 | - | ||
large_single/ | 2011-01-10 00:12 | - | 361x361 images | |
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ies/ | 2011-01-10 00:30 | - | ||
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Specific illuminances are coded logarithmically by colours. Each colour comprises one decadic order, shades within the colour are 0.5 mag each (so five shade steps are 2.5 mag, what corresponds to ratio of 1:10).
Values below the scale are illuminance / 1 lx. This is for (unrealistic) “unit” case that luminaires would have lamps producing 1 klm only, would be point-like and just 1 m over the terrain. A more realistic case would be lamps producing 10 klm each and being 10 m over the terrain: then the illuminances would be just 10× less.
The overview has been created using a Jan 2007 version of ies2tab.