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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.
# IESNA:LM-63-1995
# [TEST] 36273
# [MANUFAC] SiTECO
# [LUMCAT] 5CX63321TS01
# [LUMINAIRE] CX 200 BASIC, streetlight
# [MORE] "", "", "", "", "", "", "", ""
# [LAMPCAT] Osram: NAV-E 400W SUPER
# [LAMP] HSE 400W
# TILT=NONE
# Bulbs: 1, 54000 lm each
# Number of measured angles: 37 vertical, 37 horizontal ones
# Photometric type: 1, Units type: 2
# Luminous openig width, length and height: 0.390 0.825 0.000
# Ballast factor: 1, Input power: 440 W
# Source file: ies/36273.ies
# Luminaire flux = 41170 lm,
# 76.2 % of the bulb flux
# between 75 and 90: 4.0 % of the luminaire flux
# - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above: max 25.8 cd / 1000 lm , 2.2 % of the luminaire flux
# 90deg and above: max 14.9 cd / 1000 lm , 0.8 % of the luminaire flux
# CutOff Type: IES_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: 28 %
# Increase of Sky Luminance in Distant Places by light below 15.0 degrees
# due to light going from the luminaire directly above horizon: 139 %
# (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 138 cd / 1000 lm,
# 67.5 deg to < 76 deg: max 98 cd / 1000 lm,
# maximum spec. lum. intensity 268 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 90.0 100.0 110.0 120.0 130.0 140.0 150.0 160.0 170.0 180.0 190.0 200.0 210.0 220.0 230.0 240.0 250.0 260.0 270.0 280.0 290.0 300.0 310.0 320.0 330.0 340.0 350.0
#V:
0.0 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228 228
5.0 215 216 216 217 219 220 222 224 225 227 229 230 231 232 233 234 234 235 235 235 234 234 233 232 231 230 229 227 225 224 222 220 219 217 216 216
10.0 203 203 205 207 211 215 219 222 227 230 234 236 237 241 241 242 241 243 242 243 241 242 241 241 237 236 234 230 227 222 219 215 211 207 205 203
15.0 190 191 193 197 202 209 215 222 228 234 239 243 246 248 249 249 248 248 249 248 248 249 249 248 246 243 239 234 228 222 215 209 202 197 193 191
20.0 175 177 180 185 191 200 211 222 233 240 247 250 253 255 255 254 253 252 253 252 253 254 255 255 253 250 247 240 233 222 211 200 191 185 180 177
25.0 165 166 170 176 185 195 207 223 239 250 256 257 259 258 258 254 252 249 248 249 252 254 258 258 259 257 256 250 239 223 207 195 185 176 170 166
30.0 155 157 161 169 179 191 205 221 238 254 262 264 264 263 258 251 244 241 239 241 244 251 258 263 264 264 262 254 238 221 205 191 179 169 161 157
35.0 146 147 150 158 169 184 199 218 240 256 266 268 267 264 254 243 232 225 223 225 232 243 254 264 267 268 266 256 240 218 199 184 169 158 150 147
40.0 133 133 136 144 157 173 193 216 238 253 261 263 262 256 242 226 212 204 202 204 212 226 242 256 262 263 261 253 238 216 193 173 157 144 136 133
45.0 118 119 124 133 145 162 185 208 228 240 245 246 243 233 218 200 184 175 172 175 184 200 218 233 243 246 245 240 228 208 185 162 145 133 124 119
50.0 106 107 112 121 132 149 172 194 211 222 227 225 219 203 185 167 153 142 138 142 153 167 185 203 219 225 227 222 211 194 172 149 132 121 112 107
55.0 92.2 93.5 98.9 106 118 134 154 173 188 202 204 202 190 170 148 134 123 114 111 114 123 134 148 170 190 202 204 202 188 173 154 134 118 106 98.9 93.5
60.0 76.8 78.7 84.4 89.9 102 117 133 150 163 174 173 169 159 138 115 103 97.7 90.7 89.1 90.7 97.7 103 115 138 159 169 173 174 163 150 133 117 102 89.9 84.4 78.7
65.0 62.6 64.3 69.9 74.5 84.8 96.9 107 119 130 136 138 133 123 105 87.1 77.9 72.8 68.7 68.2 68.7 72.8 77.9 87.1 105 123 133 138 136 130 119 107 96.9 84.8 74.5 69.9 64.3
70.0 46.2 47.9 53.3 58.2 66.2 72.3 77.1 86.9 93.7 97.8 97.0 94.4 85.9 70.7 59.4 54.7 50.0 48.7 49.2 48.7 50.0 54.7 59.4 70.7 85.9 94.4 97.0 97.8 93.7 86.9 77.1 72.3 66.2 58.2 53.3 47.9
75.0 27.5 28.6 32.4 37.6 42.0 45.8 48.3 54.2 57.1 58.3 56.9 54.0 49.9 41.0 34.8 33.2 32.0 31.9 31.7 31.9 32.0 33.2 34.8 41.0 49.9 54.0 56.9 58.3 57.1 54.2 48.3 45.8 42.0 37.6 32.4 28.6
80.0 10.5 11.2 13.4 16.4 17.5 18.7 20.9 23.2 25.8 25.4 25.0 22.7 19.7 16.0 14.5 15.8 17.1 18.0 17.5 18.0 17.1 15.8 14.5 16.0 19.7 22.7 25.0 25.4 25.8 23.2 20.9 18.7 17.5 16.4 13.4 11.2
85.0 0.8 1.6 2.7 2.9 3.4 6.1 9.9 13.1 15.9 15.8 14.5 12.2 8.6 5.1 3.8 3.9 4.6 6.3 6.7 6.3 4.6 3.9 3.8 5.1 8.6 12.2 14.5 15.8 15.9 13.1 9.9 6.1 3.4 2.9 2.7 1.6
90.0 1.7 1.5 1.0 1.1 1.6 4.7 8.5 12.0 14.9 14.9 13.0 10.4 6.5 2.2 1.4 1.6 2.7 5.1 6.8 5.1 2.7 1.6 1.4 2.2 6.5 10.4 13.0 14.9 14.9 12.0 8.5 4.7 1.6 1.1 1.0 1.5
95.0 0.4 1.3 0.6 0.4 0.8 2.6 5.8 9.5 12.7 12.0 9.2 7.2 3.7 0.8 0.4 1.1 2.8 4.0 5.0 4.0 2.8 1.1 0.4 0.8 3.7 7.2 9.2 12.0 12.7 9.5 5.8 2.6 0.8 0.4 0.6 1.3
100.0 0.1 0.6 0.4 0.4 0.6 1.9 4.8 8.0 10.8 10.4 7.8 5.7 3.3 0.6 0.1 1.0 2.0 2.4 2.1 2.4 2.0 1.0 0.1 0.6 3.3 5.7 7.8 10.4 10.8 8.0 4.8 1.9 0.6 0.4 0.4 0.6
105.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.4 0.8 1.2 0.8 0.3 0.0 0.1 0.1 0.0 0.0 0.0 0.1 0.1 0.0 0.3 0.8 1.2 0.8 0.4 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
110.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
115.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
120.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
125.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
130.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
135.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
140.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
145.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
150.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
155.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
160.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
165.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
170.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
175.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0
180.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0