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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] 36328
# [MANUFAC] SiTECO
# [LUMCAT] 5CX622E1MS0408
# [LUMINAIRE] CX 100 COMFORT, streetlight
# [MORE] "", "", "", "", "", "", "", ""
# [LAMPCAT] Osram: NAV-E 70W 4Y
# [LAMP] HSE 70W
# TILT=NONE
# Bulbs: 1, 5600 lm each
# Number of measured angles: 37 vertical, 37 horizontal ones
# Photometric type: 1, Units type: 2
# Luminous openig width, length and height: 0.300 0.575 0.000
# Ballast factor: 1, Input power: 83 W
# Source file: ies/36328.ies
# Luminaire flux = 4291 lm,
# 76.6 % of the bulb flux
# between 75 and 90: 2.8 % of the luminaire flux
# - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above: max 34.9 cd / 1000 lm , 0.9 % of the luminaire flux
# 90deg and above: max 2.8 cd / 1000 lm , 0.1 % 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: 5 %
# Increase of Sky Luminance in Distant Places by light below 15.0 degrees
# due to light going from the luminaire directly above horizon: 22 %
# (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 294 cd / 1000 lm,
# 67.5 deg to < 76 deg: max 207 cd / 1000 lm,
# maximum spec. lum. intensity 342 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:
0.0 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191 191
5.0 177 177 178 180 181 183 185 188 190 193 194 197 199 200 202 203 204 204 204 204 204 203 202 200 199 197 194 193 190 188 185 183 181 180 178 177
10.0 168 169 170 172 175 178 182 185 191 196 201 206 211 216 219 221 222 222 222 222 222 221 219 216 211 206 201 196 191 185 182 178 175 172 170 169
15.0 160 161 163 165 168 172 176 182 189 199 209 219 228 234 237 239 239 237 236 237 239 239 237 234 228 219 209 199 189 182 176 172 168 165 163 161
20.0 151 153 156 159 162 166 170 178 187 199 215 230 243 253 257 255 251 248 246 248 251 255 257 253 243 230 215 199 187 178 170 166 162 159 156 153
25.0 143 144 148 151 155 158 164 170 180 195 217 240 258 270 271 265 257 250 247 250 257 265 271 270 258 240 217 195 180 170 164 158 155 151 148 144
30.0 134 135 139 142 146 151 156 164 175 192 218 247 269 279 277 269 257 244 242 244 257 269 277 279 269 247 218 192 175 164 156 151 146 142 139 135
35.0 129 132 135 135 138 143 149 158 169 189 221 255 275 280 274 263 247 233 229 233 247 263 274 280 275 255 221 189 169 158 149 143 138 135 135 132
40.0 122 125 127 131 134 141 149 153 164 192 234 273 284 275 263 246 230 216 210 216 230 246 263 275 284 273 234 192 164 153 149 141 134 131 127 125
45.0 117 118 115 122 132 140 148 153 162 200 258 296 294 268 242 223 207 193 189 193 207 223 242 268 294 296 258 200 162 153 148 140 132 122 115 118
50.0 109 114 107 110 124 134 144 149 160 218 295 327 299 256 218 194 178 168 161 168 178 194 218 256 299 327 295 218 160 149 144 134 124 110 107 114
55.0 89.5 93.1 91.4 97.3 109 121 125 132 154 233 326 342 287 228 193 165 150 140 137 140 150 165 193 228 287 342 326 233 154 132 125 121 109 97.3 91.4 93.1
60.0 75.3 77.0 75.5 81.8 89.4 99.1 104 111 144 236 339 335 250 187 155 135 123 114 111 114 123 135 155 187 250 335 339 236 144 111 104 99.1 89.4 81.8 75.5 77.0
65.0 59.8 62.3 63.1 64.0 69.6 75.0 79.8 82.9 116 200 294 277 190 139 112 97.2 87.8 83.4 81.9 83.4 87.8 97.2 112 139 190 277 294 200 116 82.9 79.8 75.0 69.6 64.0 63.1 62.3
70.0 62.6 70.0 53.4 44.1 45.9 47.1 49.9 52.1 75.9 142 207 187 126 87.0 66.9 60.2 56.0 54.0 53.4 54.0 56.0 60.2 66.9 87.0 126 187 207 142 75.9 52.1 49.9 47.1 45.9 44.1 53.4 70.0
75.0 40.5 51.2 36.4 25.6 26.6 25.5 26.5 26.0 34.9 71.3 100 91.4 58.8 37.6 31.7 30.3 29.4 28.6 28.3 28.6 29.4 30.3 31.7 37.6 58.8 91.4 100 71.3 34.9 26.0 26.5 25.5 26.6 25.6 36.4 51.2
80.0 14.5 19.3 15.9 10.0 10.5 10.1 9.5 9.6 10.5 22.4 34.9 31.1 17.0 11.0 9.2 9.0 9.5 9.5 8.8 9.5 9.5 9.0 9.2 11.0 17.0 31.1 34.9 22.4 10.5 9.6 9.5 10.1 10.5 10.0 15.9 19.3
85.0 0.6 3.7 4.8 3.8 5.2 4.8 3.0 2.0 1.8 2.7 4.5 4.6 2.9 1.9 1.2 1.1 1.0 0.2 0.1 0.2 1.0 1.1 1.2 1.9 2.9 4.6 4.5 2.7 1.8 2.0 3.0 4.8 5.2 3.8 4.8 3.7
90.0 0.1 0.3 0.6 1.2 2.8 2.6 1.4 0.7 0.6 1.0 1.9 2.1 1.7 0.8 0.2 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.2 0.8 1.7 2.1 1.9 1.0 0.6 0.7 1.4 2.6 2.8 1.2 0.6 0.3
95.0 0.0 0.0 0.3 1.1 1.4 2.2 0.9 0.7 0.5 0.7 1.6 1.9 1.4 0.5 0.1 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.1 0.5 1.4 1.9 1.6 0.7 0.5 0.7 0.9 2.2 1.4 1.1 0.3 0.0
100.0 0.0 0.1 0.2 0.4 0.9 1.2 0.7 0.5 0.4 0.7 1.1 1.6 0.8 0.4 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.4 0.8 1.6 1.1 0.7 0.4 0.5 0.7 1.2 0.9 0.4 0.2 0.1
105.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 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