# IESNA: LM-63-1995 # [TEST] E366-60 # [DATE] # [MANUFAC] COOPER LIGHTING # [LUMCAT] UTR15SXX55 # [LUMINAIRE] 150W HPS TYPE V TRADITIONAIRE POST TOP # [LAMP] 150W HPS CL ED-23.5 # [_REFLECTOR] NONE # [_REFRACTOR] ACRYLIC PRISMATIC TYPE V PANELS # [_SOCKET POSITION] VERTICAL BASE DOWN # [_LAMP LUMENS] 16000 # TILT=NONE # Bulbs: 1, 16000 lm each # Number of measured angles: 18 vertical, 21 horizontal ones # Photometric type: 1, Units type: 1 # Luminous openig width, length and height: 0.920 0.920 1.000 # Ballast factor: 1, Input power: 188 W # Source file: utr1s55.ies # Luminaire flux = 10785 lx, # 67.4 % of the bulb flux # between 75 and 90: 20.2 % of the luminaire flux # - this part causes just GLARE in case of road lighting and similar purposes # 80deg and above: max 31.3 cd/1000lm , 12.7 % of the luminaire flux # 90deg and above: max 18.8 cd/1000lm , 7.8 % 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: 195 % # Increase of Sky Luminance in Distant Places by light below 30.0 degrees # due to light going from the luminaire directly above horizon: 373 % # (for the zenith luminance such an angle suits places up to 10 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) # Illumination of a rectangle of 0.0:1.0:-2.5:2.5 pole heights: # Per cent of luminaire output falling there: 16.4 # for a unit case (glass at 1 m height, 1000 lm bulb) its illumination: # Maximum: 34.4 lx # Average: 22.1 lx # Minimum: 12.4 lx # Average/Minimum: 1.8 # The following table gives luminous intensities which would be produced # using a hypotetic bulb giving a luminous flux of 1000 lm (i.e., cd/klm): # H: 0.0 5.0 15.0 25.0 35.0 45.0 55.0 65.0 75.0 85.0 90.0 95.0 105.0 115.0 125.0 135.0 145.0 155.0 165.0 175.0 180.0 #V: 0.0 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 14.1 5.0 14.1 13.3 12.5 13.0 13.8 14.1 13.8 13.0 12.5 13.3 14.1 13.3 12.5 13.0 13.8 14.1 13.8 13.0 12.5 13.3 14.1 15.0 15.6 14.8 14.1 14.1 14.6 15.0 14.6 14.1 14.1 14.8 15.6 14.8 14.1 14.1 14.6 15.0 14.6 14.1 14.1 14.8 15.6 25.0 26.6 25.8 23.4 21.1 20.3 20.3 20.3 21.1 23.4 25.8 26.6 25.8 23.4 21.1 20.3 20.3 20.3 21.1 23.4 25.8 26.6 35.0 62.5 60.9 55.4 50.0 46.9 45.3 46.9 50.0 55.4 60.9 62.5 60.9 55.4 50.0 46.9 45.3 46.9 50.0 55.4 60.9 62.5 45.0 75.0 75.8 71.9 67.2 63.3 59.4 63.3 67.2 71.9 75.8 75.0 75.8 71.9 67.2 63.3 59.4 63.3 67.2 71.9 75.8 75.0 55.0 90.6 91.4 91.4 87.5 82.8 81.3 82.8 87.5 91.4 91.4 90.6 91.4 91.4 87.5 82.8 81.3 82.8 87.5 91.4 91.4 90.6 65.0 215.6 223.4 228.1 209.4 182.8 171.9 182.8 209.4 228.1 223.4 215.6 223.4 228.1 209.4 182.8 171.9 182.8 209.4 228.1 223.4 215.6 75.0 218.8 220.3 223.4 179.7 162.5 159.4 162.5 179.7 223.4 220.3 218.8 220.3 223.4 179.7 162.5 159.4 162.5 179.7 223.4 220.3 218.8 85.0 31.3 31.3 31.3 30.4 29.7 29.7 29.7 30.4 31.3 31.3 31.3 31.3 31.3 30.4 29.7 29.7 29.7 30.4 31.3 31.3 31.3 95.0 17.2 17.5 17.8 18.3 18.8 18.8 18.8 18.3 17.8 17.5 17.2 17.5 17.8 18.3 18.8 18.8 18.8 18.3 17.8 17.5 17.2 105.0 10.9 10.9 10.6 11.3 12.7 13.1 12.7 11.3 10.6 10.9 10.9 10.9 10.6 11.3 12.7 13.1 12.7 11.3 10.6 10.9 10.9 115.0 6.9 7.4 7.5 7.5 8.6 9.4 8.6 7.5 7.5 7.4 6.9 7.4 7.5 7.5 8.6 9.4 8.6 7.5 7.5 7.4 6.9 125.0 5.9 6.3 6.3 6.3 6.6 6.9 6.6 6.3 6.3 6.3 5.9 6.3 6.3 6.3 6.6 6.9 6.6 6.3 6.3 6.3 5.9 135.0 5.9 6.1 6.3 6.1 5.3 4.7 5.3 6.1 6.3 6.1 5.9 6.1 6.3 6.1 5.3 4.7 5.3 6.1 6.3 6.1 5.9 145.0 4.7 4.7 4.7 3.8 3.1 2.2 3.1 3.8 4.7 4.7 4.7 4.7 4.7 3.8 3.1 2.2 3.1 3.8 4.7 4.7 4.7 155.0 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 3.1 180.0 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