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] NO45-20R # [LUMINAIRE] NOVARA SL # [LUMCAT] 12.02651.4500 # [DATE] 07.04.1997/fg # down given: 100% # out given: 55.7% # tilt: 0.0 # [LAMP] TC-L 24W # Source file: ldt/NO45-20R.ldt # Luminaire flux = 549 raw, for the given bulb(s) it would be 1975 lm, # 54.9 % 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 12.2 cd / 1000 lm , 0.1 % of the luminaire flux # 90deg and above: max 0.8?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 57 cd / 1000 lm, # maximum spec. lum. intensity 235 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 90.0 100.0 110.0 120.0 130.0 140.0 150.0 160.0 170.0 180.0 #V: 0.0 211 211 211 211 211 211 211 211 211 211 211 211 211 211 211 211 211 211 211 10.0 175 176 178 180 183 187 190 196 203 224 229 225 225 228 230 233 234 232 235 20.0 158 158 161 164 167 172 175 181 189 208 215 216 218 221 226 230 232 233 235 30.0 137 138 139 141 143 148 153 157 165 186 192 195 199 204 210 213 216 220 222 40.0 127 127 127 125 122 121 125 130 138 153 161 166 170 174 183 187 192 195 197 50.0 100 101 102 102 101 99.1 94.7 97.2 103 114 122 129 134 140 147 150 153 154 155 60.0 67.5 68.3 70.9 71.8 70.4 69.3 67.9 63.5 65.0 73.5 80.3 88.4 94.0 97.3 102 105 108 108 108 70.0 33.5 33.3 34.4 35.4 36.0 37.2 36.0 33.5 30.9 34.7 40.2 46.6 49.6 52.3 55.6 57.4 56.6 54.2 53.8 80.0 4.4 4.8 5.4 6.3 7.2 7.9 8.6 8.5 7.3 6.9 9.0 11.4 12.2 11.3 10.3 9.3 8.8 7.8 7.8 90.0 0.6 0.6 0.6 0.5 0.4 0.4 0.4 0.4 0.4 0.7 0.8 0.4 0.4 0.4 0.4 0.4 0.4 0.4 0.4