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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] 39396
# [MANUFAC] SiTECO
# [LUMCAT] 5UK587E1JT0B
# [LUMINAIRE] SC 50, Street light
# [MORE] Aluminium pressure die-cast housing, painted with grey aluminium (RAL
# [MORE] 9007), parallel compensated, ignitors with automatic disconnection
# [MORE] radial facetted reflector, clear diffuser acryl
# [MORE] indiv. Position, LP 1, RP 2
# [LAMPCAT] Philips: SON-T PIA PLUS 50W
# [LAMP] HST 50W
# TILT=NONE
# Bulbs: 1, 4400 lm each
# Number of measured angles: 37 vertical, 37 horizontal ones
# Photometric type: 1, Units type: 2
# Luminous openig width, length and height: 0.253 0.253 0.000
# Ballast factor: 1, Input power: 62 W
# Source file: ies/39396.ies
# Luminaire flux = 3401 lm,
# 77.3 % of the bulb flux
# between 75 and 90: 3.8 % of the luminaire flux
# - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above: max 87.5 cd / 1000 lm , 1.4 % of the luminaire flux
# 90deg and above: max 4.4 cd / 1000 lm , 0.4 % 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: 13 %
# Increase of Sky Luminance in Distant Places by light below 15.0 degrees
# due to light going from the luminaire directly above horizon: 57 %
# (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 465 cd / 1000 lm,
# 67.5 deg to < 76 deg: max 490 cd / 1000 lm,
# maximum spec. lum. intensity 490 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:
0.0 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176 176
5.0 174 173 178 179 181 181 183 186 188 189 190 194 197 199 204 206 205 197 191 197 205 206 204 199 197 194 190 189 188 186 183 181 181 179 178 173
10.0 160 161 163 164 171 180 187 191 195 198 205 211 220 231 233 224 219 219 208 219 219 224 233 231 220 211 205 198 195 191 187 180 171 164 163 161
15.0 149 151 155 159 162 168 175 184 189 201 211 220 228 239 241 245 235 228 218 228 235 245 241 239 228 220 211 201 189 184 175 168 162 159 155 151
20.0 143 148 151 152 155 161 168 173 183 199 218 236 243 248 253 238 240 230 218 230 240 238 253 248 243 236 218 199 183 173 168 161 155 152 151 148
25.0 138 139 144 144 149 154 158 163 171 190 215 233 245 248 243 229 216 209 207 209 216 229 243 248 245 233 215 190 171 163 158 154 149 144 144 139
30.0 138 139 143 141 143 146 146 153 163 174 195 220 247 237 220 206 191 193 186 193 191 206 220 237 247 220 195 174 163 153 146 146 143 141 143 139
35.0 122 125 134 134 137 138 141 148 162 181 206 224 221 218 208 190 186 183 169 183 186 190 208 218 221 224 206 181 162 148 141 138 137 134 134 125
40.0 111 115 130 134 134 131 134 144 157 189 213 229 222 205 184 166 154 146 127 146 154 166 184 205 222 229 213 189 157 144 134 131 134 134 130 115
45.0 98.6 103 113 130 134 136 135 141 153 183 218 230 223 192 169 141 131 114 94.6 114 131 141 169 192 223 230 218 183 153 141 135 136 134 130 113 103
50.0 90.5 95.0 108 122 153 142 140 144 153 209 266 239 214 180 156 127 111 98.3 79.2 98.3 111 127 156 180 214 239 266 209 153 144 140 142 153 122 108 95.0
55.0 78.7 78.3 87.5 135 133 144 138 144 160 242 334 315 234 191 178 126 112 86.1 67.9 86.1 112 126 178 191 234 315 334 242 160 144 138 144 133 135 87.5 78.3
60.0 64.7 64.0 76.7 114 137 157 195 152 154 231 384 401 292 197 162 110 100 66.0 49.5 66.0 100 110 162 197 292 401 384 231 154 152 195 157 137 114 76.7 64.0
65.0 48.3 52.0 68.3 110 111 128 130 132 152 299 465 421 270 174 138 89.6 86.5 47.4 36.0 47.4 86.5 89.6 138 174 270 421 465 299 152 132 130 128 111 110 68.3 52.0
70.0 37.0 39.6 51.0 75.4 85.0 90.3 98.6 97.3 120 427 490 298 189 127 92.1 71.8 45.4 29.9 22.1 29.9 45.4 71.8 92.1 127 189 298 490 427 120 97.3 98.6 90.3 85.0 75.4 51.0 39.6
75.0 17.4 19.6 23.5 18.4 28.8 14.6 16.7 19.9 56.0 369 292 75.6 27.7 25.3 28.2 26.2 29.7 25.6 16.4 25.6 29.7 26.2 28.2 25.3 27.7 75.6 292 369 56.0 19.9 16.7 14.6 28.8 18.4 23.5 19.6
80.0 5.4 12.8 10.2 5.5 6.5 8.8 10.9 13.4 22.8 87.5 54.9 14.1 8.0 6.0 4.2 3.3 2.9 2.6 2.5 2.6 2.9 3.3 4.2 6.0 8.0 14.1 54.9 87.5 22.8 13.4 10.9 8.8 6.5 5.5 10.2 12.8
85.0 1.5 1.7 2.9 3.9 5.4 7.2 8.2 9.1 10.2 12.6 11.9 7.1 4.8 3.6 2.6 1.8 1.5 1.2 1.2 1.2 1.5 1.8 2.6 3.6 4.8 7.1 11.9 12.6 10.2 9.1 8.2 7.2 5.4 3.9 2.9 1.7
90.0 0.5 0.9 1.3 2.1 2.3 3.1 3.3 3.9 4.4 3.7 3.7 3.2 2.5 1.6 1.1 0.7 0.6 0.5 0.5 0.5 0.6 0.7 1.1 1.6 2.5 3.2 3.7 3.7 4.4 3.9 3.3 3.1 2.3 2.1 1.3 0.9
95.0 0.2 0.5 1.0 1.5 1.7 2.2 2.6 3.2 3.3 2.8 2.8 2.5 2.1 1.5 1.0 0.7 0.5 0.4 0.2 0.4 0.5 0.7 1.0 1.5 2.1 2.5 2.8 2.8 3.3 3.2 2.6 2.2 1.7 1.5 1.0 0.5
100.0 0.2 0.2 0.7 1.0 1.2 1.7 1.8 2.2 2.2 2.2 2.3 2.1 1.5 1.1 0.9 0.5 0.2 0.2 0.2 0.2 0.2 0.5 0.9 1.1 1.5 2.1 2.3 2.2 2.2 2.2 1.8 1.7 1.2 1.0 0.7 0.2
105.0 0.2 0.2 0.2 0.5 0.9 1.0 1.3 1.6 1.5 1.5 1.3 1.2 1.0 0.9 0.5 0.4 0.2 0.2 0.2 0.2 0.2 0.4 0.5 0.9 1.0 1.2 1.3 1.5 1.5 1.6 1.3 1.0 0.9 0.5 0.2 0.2
110.0 0.2 0.2 0.2 0.4 0.6 0.7 0.7 1.0 1.0 0.9 1.0 0.9 0.7 0.5 0.2 0.2 0.2 0.2 0.2 0.2 0.2 0.2 0.2 0.5 0.7 0.9 1.0 0.9 1.0 1.0 0.7 0.7 0.6 0.4 0.2 0.2
115.0 0.2 0.2 0.2 0.5 0.5 0.7 0.7 0.7 0.7 0.9 0.7 0.6 0.5 0.5 0.2 0.2 0.2 0.2 0.2 0.2 0.2 0.2 0.2 0.5 0.5 0.6 0.7 0.9 0.7 0.7 0.7 0.7 0.5 0.5 0.2 0.2
120.0 0.5 0.2 0.5 0.5 0.5 0.5 0.7 0.9 0.5 0.7 0.7 0.7 0.5 0.5 0.2 0.2 0.2 0.2 0.2 0.2 0.2 0.2 0.2 0.5 0.5 0.7 0.7 0.7 0.5 0.9 0.7 0.5 0.5 0.5 0.5 0.2
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