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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] 913
# [LUMINAIRE] CANTO
# [LUMCAT] 10.07301.4500
# [DATE] 28.03.2000/fg
# down given: 100%
# out given: 81.8%
# tilt: 0.0
# [LAMP] HIT-CE 150W / WDL
# Source file: ldt/Can0913c.ldt
# Luminaire flux = 818 raw, for the given bulb(s) it would be 11448 lm,
# 81.8 % of the bulb flux
# between 75 and 90: 1.9 % of the luminaire flux
# - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above: max 18.7 cd / 1000 lm , 0.3 % of the luminaire flux
# 90deg and above: max 0.5?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 217 cd / 1000 lm,
# 67.5 deg to < 76 deg: max 182 cd / 1000 lm,
# maximum spec. lum. intensity 388 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:
0.0 267 267 267 267 267 267 267 267 267 267 267 267 267 267 267 267 267 267 267
5.0 220 228 223 215 212 212 217 221 225 232 236 242 246 254 263 274 280 284 292
10.0 164 165 170 178 185 193 205 224 241 255 262 268 259 255 243 240 240 243 234
15.0 138 132 138 150 167 190 218 245 253 271 291 301 290 275 260 240 226 213 206
20.0 111 113 122 140 161 186 210 236 265 288 299 318 320 290 251 233 215 198 189
25.0 104 104 117 139 158 175 185 207 238 289 287 326 308 278 244 223 207 183 174
30.0 98.2 103 119 142 157 159 155 163 196 257 288 342 343 286 250 218 196 181 169
35.0 92.8 99.8 127 153 164 150 141 156 194 242 268 333 379 364 285 221 195 175 167
40.0 85.3 94.4 124 152 167 171 174 182 211 223 235 267 319 388 364 246 195 162 142
45.0 76.8 85.9 102 124 129 170 189 196 215 228 239 257 271 307 380 315 170 124 115
50.0 50.4 59.1 73.8 89.6 116 156 184 229 235 283 270 271 261 269 308 288 153 115 105
55.0 46.0 54.5 71.3 81.7 95.2 134 190 222 207 246 268 281 292 243 249 215 151 112 103
60.0 39.9 51.5 67.7 77.4 89.6 111 155 187 199 224 237 243 252 248 225 206 145 101 90.9
65.0 34.9 50.0 62.0 70.4 82.5 99.5 140 142 183 198 208 211 212 217 183 158 118 87.8 80.4
70.0 18.9 29.5 47.3 57.7 65.0 85.7 101 141 135 157 168 176 182 166 126 108 92.1 77.3 73.3
75.0 4.1 4.7 4.9 5.7 18.7 17.1 20.3 28.4 32.1 41.1 44.8 48.3 67.1 106 96.8 68.4 69.7 60.3 48.2
80.0 2.0 2.3 2.3 2.2 2.3 3.0 3.6 8.2 10.9 15.5 17.1 18.7 16.4 12.4 9.8 7.3 6.3 4.9 3.7
85.0 1.0 0.9 0.9 0.9 0.9 1.0 1.2 1.5 2.0 2.2 2.3 2.6 2.3 1.8 1.7 1.5 1.5 1.5 1.2
90.0 0.4 0.4 0.4 0.4 0.5 0.5 0.4 0.4 0.5 0.4 0.4 0.4 0.4 0.4 0.4 0.4 0.4 0.4 0.3