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| In the left half of the left plot, specific illuminance by a continuous row of luminaires spaced 5 heights is shown (right half is for a single luminaire). | The right plot is for a single luminaire, unrotated. |
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.
# [MANUFAC] .hess
# [TEST] 358/NO45-02R
# [LUMINAIRE] NOVARA Q
# [LUMCAT] 12.02633.0
# [DATE] 23.12.03/24.11.1995/KLAISS |23.12.03 LUMCat
# down given: 100%
# out given: 72.3%
# tilt: 0.0
# [LAMP] HIT-DE 250W
# Source file: ldt/N4502rai.ldt
# Luminaire flux = 721 raw, for the given bulb(s) it would be 14414 lm,
# 72.1 % of the bulb flux
# between 75 and 90: 0.0 % of the luminaire flux
# - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above: max 4.0 cd / 1000 lm , 0.2 % of the luminaire flux
# 90deg and above: max 1.0?cd / 1000 lm , 0.0?% of the luminaire flux
# CutOff Type: CIE_CutOff
# Increase of Sky Luminance due to light going
# from the luminaire difectly above horizon, as compared with the
# luminance produced by the light dispersed from the ground: 0?%
# Increase of Sky Luminance in Distant Places by light below 15.0 degrees
# due to light going from the luminaire directly above horizon: 0?%
# (for the zenith luminance such an angle suits places up to 19 km distance)
# The increases concern the following situation:
# Albedo = 0.10
# Zenith Extinction = 0.30 mag (i.e., direct light remaining 76 %)
# Indicatrix type =0 (0: acc. to P.Cinzano, 4..6: CIE sky types)
# (the downward-scattered part of lambertian uplight is 0.1108 then)
# 62.5 deg to <67.5 deg: max -99 cd / 1000 lm,
# 67.5 deg to < 76 deg: max 9 cd / 1000 lm,
# maximum spec. lum. intensity 541 cd / 1000 lm
# The following table gives luminous intensities which would be produced
# using a hypothetic bulb giving a luminous flux of 1000 lm (i.e., cd/klm):
# H: 0.0 10.0 20.0 30.0 40.0 50.0 60.0 70.0 80.0 90.0
#V:
0.0 541 541 541 541 541 541 541 541 541 541
10.0 415 421 424 436 450 466 487 506 525 534
20.0 369 373 388 390 404 404 423 455 493 520
30.0 274 294 310 332 383 379 398 415 477 540
40.0 49.0 56.0 75.0 129 176 273 313 332 381 464
50.0 19.0 19.0 19.0 23.0 40.0 62.0 133 175 202 225
60.0 8.0 9.0 9.0 9.0 12.0 15.0 21.0 31.0 38.0 35.0
70.0 5.0 5.0 5.0 5.0 6.0 6.0 7.0 8.0 9.0 8.0
80.0 3.0 3.0 3.0 3.0 3.0 3.0 3.0 3.0 4.0 3.0
90.0 1.0 1.0 1.0 1.0 1.0 1.0 1.0 1.0 1.0 1.0