# IESNA: LM-63-1995 # [TEST] E366-40 # [DATE] # [MANUFAC] COOPER LIGHTING # [LUMCAT] UTR17MXX55 # [LUMINAIRE] 175W MH TYPE V TRADITIONAIRE POST TOP # [LAMP] 175W MH CL ED-28 # [_REFLECTOR] NONE # [_REFRACTOR] ACRYLIC PRISMATIC TYPE V PANELS # [_SOCKET POSITION] VERTICAL BASE DOWN # [_LAMP LUMENS] 14000 # TILT=NONE # Bulbs: 1, 14000 lm each # Number of measured angles: 18 vertical, 19 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: 210 W # Source file: utr1m55.ies # Luminaire flux = 8419 lx, # 60.1 % of the bulb flux # between 75 and 90: 20.0 % of the luminaire flux # - this part causes just GLARE in case of road lighting and similar purposes # 80deg and above: max 38.2 cd/1000lm , 13.7 % of the luminaire flux # 90deg and above: max 17.3 cd/1000lm , 7.4 % 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: 187 % # Increase of Sky Luminance in Distant Places by light below 30.0 degrees # due to light going from the luminaire directly above horizon: 361 % # (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: 18.3 # for a unit case (glass at 1 m height, 1000 lm bulb) its illumination: # Maximum: 35.7 lx # Average: 22.0 lx # Minimum: 11.9 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 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 #V: 0.0 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 13.6 5.0 14.1 14.1 14.1 14.1 13.6 13.6 14.1 14.1 14.1 14.1 14.1 14.1 14.1 13.6 13.6 14.1 14.1 14.1 14.1 15.0 15.9 15.9 15.9 13.2 15.0 15.0 13.2 15.9 15.9 15.9 15.9 15.9 13.2 15.0 15.0 13.2 15.9 15.9 15.9 25.0 27.3 28.2 26.8 23.6 20.9 20.9 23.6 26.8 28.2 27.3 28.2 26.8 23.6 20.9 20.9 23.6 26.8 28.2 27.3 35.0 65.0 64.1 55.4 52.3 50.4 50.4 52.3 55.4 64.1 65.0 64.1 55.4 52.3 50.4 50.4 52.3 55.4 64.1 65.0 45.0 81.4 77.3 70.4 72.7 65.9 65.9 72.7 70.4 77.3 81.4 77.3 70.4 72.7 65.9 65.9 72.7 70.4 77.3 81.4 55.0 97.7 97.7 94.1 89.6 84.1 84.1 89.6 94.1 97.7 97.7 97.7 94.1 89.6 84.1 84.1 89.6 94.1 97.7 97.7 65.0 179.1 168.1 177.7 157.3 151.8 151.8 157.3 177.7 168.1 179.1 168.1 177.7 157.3 151.8 151.8 157.3 177.7 168.1 179.1 75.0 173.6 162.3 160.0 145.0 140.0 140.0 145.0 160.0 162.3 173.6 162.3 160.0 145.0 140.0 140.0 145.0 160.0 162.3 173.6 85.0 38.2 36.4 36.4 33.6 30.9 30.9 33.6 36.4 36.4 38.2 36.4 36.4 33.6 30.9 30.9 33.6 36.4 36.4 38.2 95.0 14.6 14.6 15.9 17.3 17.3 17.3 17.3 15.9 14.6 14.6 14.6 15.9 17.3 17.3 17.3 17.3 15.9 14.6 14.6 105.0 9.1 9.1 9.6 10.0 10.0 10.0 10.0 9.6 9.1 9.1 9.1 9.6 10.0 10.0 10.0 10.0 9.6 9.1 9.1 115.0 6.8 6.4 6.4 6.8 6.8 6.8 6.8 6.4 6.4 6.8 6.4 6.4 6.8 6.8 6.8 6.8 6.4 6.4 6.8 125.0 5.9 5.4 5.0 5.4 5.4 5.4 5.4 5.0 5.4 5.9 5.4 5.0 5.4 5.4 5.4 5.4 5.0 5.4 5.9 135.0 5.9 5.4 5.0 4.6 3.6 3.6 4.6 5.0 5.4 5.9 5.4 5.0 4.6 3.6 3.6 4.6 5.0 5.4 5.9 145.0 4.1 2.3 2.3 2.3 2.3 2.3 2.3 2.3 2.3 4.1 2.3 2.3 2.3 2.3 2.3 2.3 2.3 2.3 4.1 155.0 2.3 2.3 2.3 1.4 2.3 2.3 1.4 2.3 2.3 2.3 2.3 2.3 1.4 2.3 2.3 1.4 2.3 2.3 2.3 180.0 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