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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] 36509
# [MANUFAC] SiTECO
# [LUMCAT] 5CX62321AE01
# [LUMINAIRE] CX 100 BASIC, streetlight
# [MORE] "", "", "", "", "", "", "", ""
# [LAMPCAT] Osram: HQL 80W
# [LAMP] HME 80W
# TILT=NONE
# Bulbs: 1, 3800 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: 89 W
# Source file: ies/36509.ies
# Luminaire flux = 2983 lm,
# 78.5 % of the bulb flux
# between 75 and 90: 3.4 % of the luminaire flux
# - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above: max 33.8 cd / 1000 lm , 1.5 % of the luminaire flux
# 90deg and above: max 11.9 cd / 1000 lm , 0.5 % 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: 19 %
# Increase of Sky Luminance in Distant Places by light below 15.0 degrees
# due to light going from the luminaire directly above horizon: 95 %
# (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 290 cd / 1000 lm,
# 67.5 deg to < 76 deg: max 214 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:
0.0 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184 184
5.0 172 172 173 173 174 176 179 181 184 186 187 189 192 194 196 196 197 197 197 197 197 196 196 194 192 189 187 186 184 181 179 176 174 173 173 172
10.0 164 164 165 167 168 171 174 177 181 186 193 197 202 206 212 213 216 216 217 216 216 213 212 206 202 197 193 186 181 177 174 171 168 167 165 164
15.0 158 158 159 160 162 165 168 174 180 189 197 207 216 223 228 231 231 233 231 233 231 231 228 223 216 207 197 189 180 174 168 165 162 160 159 158
20.0 150 151 154 155 156 158 163 168 176 188 201 217 231 239 245 247 245 243 243 243 245 247 245 239 231 217 201 188 176 168 163 158 156 155 154 151
25.0 144 145 146 148 150 151 156 161 170 185 204 225 242 257 259 258 254 249 247 249 254 258 259 257 242 225 204 185 170 161 156 151 150 148 146 145
30.0 136 137 137 139 142 144 149 154 163 179 206 232 254 267 269 263 254 244 242 244 254 263 269 267 254 232 206 179 163 154 149 144 142 139 137 137
35.0 134 134 134 133 134 139 141 148 157 174 207 239 262 268 268 260 248 240 236 240 248 260 268 268 262 239 207 174 157 148 141 139 134 133 134 134
40.0 123 124 127 129 129 134 138 142 153 178 215 253 268 264 258 252 237 227 222 227 237 252 258 264 268 253 215 178 153 142 138 134 129 129 127 124
45.0 118 118 116 122 128 132 141 145 153 188 239 276 281 261 242 231 218 206 201 206 218 231 242 261 281 276 239 188 153 145 141 132 128 122 116 118
50.0 118 118 109 112 122 130 145 150 158 209 286 315 296 259 226 207 193 183 175 183 193 207 226 259 296 315 286 209 158 150 145 130 122 112 109 118
55.0 101 101 97.3 101 115 129 137 143 160 232 321 342 301 246 208 182 166 157 152 157 166 182 208 246 301 342 321 232 160 143 137 129 115 101 97.3 101
60.0 89.6 88.3 86.4 89.6 98.9 114 117 119 147 245 322 329 268 214 181 154 142 136 133 136 142 154 181 214 268 329 322 245 147 119 117 114 98.9 89.6 86.4 88.3
65.0 72.8 71.7 73.2 72.5 78.6 88.4 90.4 89.9 125 224 290 282 211 164 138 120 107 104 102 104 107 120 138 164 211 282 290 224 125 89.9 90.4 88.4 78.6 72.5 73.2 71.7
70.0 71.4 80.2 66.9 51.2 57.4 53.7 55.8 52.0 81.6 163 214 199 143 102 83.5 76.9 70.6 68.8 65.8 68.8 70.6 76.9 83.5 102 143 199 214 163 81.6 52.0 55.8 53.7 57.4 51.2 66.9 80.2
75.0 57.2 66.5 45.3 28.5 28.9 24.1 24.9 20.8 32.0 83.3 114 108 69.2 42.1 34.6 36.3 35.5 33.2 30.7 33.2 35.5 36.3 34.6 42.1 69.2 108 114 83.3 32.0 20.8 24.9 24.1 28.9 28.5 45.3 66.5
80.0 26.4 32.1 16.1 7.7 6.6 6.6 6.5 6.3 8.5 20.6 33.8 30.5 16.7 9.6 7.8 8.0 10.0 9.1 9.3 9.1 10.0 8.0 7.8 9.6 16.7 30.5 33.8 20.6 8.5 6.3 6.5 6.6 6.6 7.7 16.1 32.1
85.0 2.8 4.6 3.3 4.5 2.5 2.7 2.4 3.0 5.7 7.9 9.6 7.7 4.7 3.2 2.3 1.8 3.2 4.6 5.5 4.6 3.2 1.8 2.3 3.2 4.7 7.7 9.6 7.9 5.7 3.0 2.4 2.7 2.5 4.5 3.3 4.6
90.0 3.1 3.2 2.4 3.6 1.8 1.4 2.1 4.6 9.7 11.9 11.1 9.0 5.8 1.4 1.5 0.7 2.0 4.5 6.3 4.5 2.0 0.7 1.5 1.4 5.8 9.0 11.1 11.9 9.7 4.6 2.1 1.4 1.8 3.6 2.4 3.2
95.0 0.8 0.9 1.4 1.9 1.1 1.0 2.2 4.6 8.8 9.4 8.6 7.7 4.5 1.5 0.7 0.3 1.3 1.2 1.0 1.2 1.3 0.3 0.7 1.5 4.5 7.7 8.6 9.4 8.8 4.6 2.2 1.0 1.1 1.9 1.4 0.9
100.0 0.4 0.6 1.0 1.8 1.0 0.8 1.4 2.4 5.4 5.6 5.6 4.5 3.3 0.9 0.5 0.1 0.9 0.6 0.4 0.6 0.9 0.1 0.5 0.9 3.3 4.5 5.6 5.6 5.4 2.4 1.4 0.8 1.0 1.8 1.0 0.6
105.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.1 0.0 0.0 0.0 0.0 0.1 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.1 0.0 0.0 0.0 0.0 0.1 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