# IESNA: LM-63-1995 # [TEST] E366-39 # [DATE] # [MANUFAC] COOPER LIGHTING # [LUMCAT] UTR17MXX22 # [LUMINAIRE] 175W MH TYPE II TRADITIONAIRE POST TOP # [LAMP] 175W MH CL ED-28 # [_REFLECTOR] NONE # [_REFRACTOR] ACRYLIC PRISMATIC TYPE II PANELS # [_SOCKET POSITION] VERTICAL BASE DOWN # [_LAMP LUMENS] 14000 # TILT=NONE # Bulbs: 1, 14000 lm each # (luminous intensites divided by 1.27 in the original ies file) # Number of measured angles: 19 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: utr1m22.ies # Luminaire flux = 5934 raw, for the given bulb(s) it would be 7552 lx, # 53.9 % of the bulb flux # between 75 and 90: 18.7 % of the luminaire flux # - this part causes just GLARE in case of road lighting and similar purposes # 80deg and above: max 63.6 cd/1000lm , 16.8 % of the luminaire flux # 90deg and above: max 27.3 cd/1000lm , 9.9 % of the luminaire flux # CutOff Type: CIE_Semi-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: 252 % # Increase of Sky Luminance in Distant Places by light below 30.0 degrees # due to light going from the luminaire directly above horizon: 485 % # (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: 28.1 # for a unit case (glass at 1 m height, 1000 lm bulb) its illumination: # Maximum: 53.5 lx # Average: 30.3 lx # Minimum: 14.2 lx # Average/Minimum: 2.1 # 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 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 16.4 5.0 18.2 18.2 18.2 17.7 17.7 17.7 17.3 16.8 16.4 15.9 15.9 15.9 15.9 15.9 15.9 15.0 15.0 15.0 15.0 15.0 20.5 20.5 20.5 19.5 19.1 18.2 18.2 18.2 18.2 17.3 17.3 17.3 15.9 15.0 14.5 14.5 14.5 14.5 14.5 25.0 33.2 34.1 30.5 27.3 26.4 28.6 29.5 30.0 31.4 26.8 25.0 23.6 21.4 20.9 20.5 20.5 23.6 24.5 24.5 35.0 63.2 62.3 57.3 52.3 48.2 69.1 97.3 86.8 77.3 64.5 45.0 37.3 34.1 34.1 38.6 42.7 45.5 50.0 51.4 45.0 78.2 76.8 70.5 66.8 57.7 60.9 109.5 139.5 118.2 80.5 52.3 42.3 38.6 42.3 50.9 58.6 59.5 61.8 62.3 55.0 104.1 107.7 97.7 90.5 76.4 75.5 112.3 188.2 181.8 116.8 61.4 45.0 41.8 48.2 59.1 70.5 75.0 72.7 74.5 65.0 186.8 185.9 181.8 155.9 128.6 131.8 169.5 295.4 354.5 239.1 95.5 54.5 49.5 53.2 60.9 61.8 61.4 50.0 48.6 75.0 185.9 179.1 170.5 146.8 121.4 109.1 142.7 265.0 344.5 214.5 86.4 48.2 45.9 40.5 39.5 34.1 28.6 22.7 20.0 85.0 45.5 43.2 41.8 42.3 38.6 35.5 36.4 52.3 63.6 46.8 28.6 23.6 25.0 25.9 24.5 21.8 19.5 15.9 13.6 95.0 15.9 16.4 18.2 20.5 20.9 20.5 21.8 23.2 27.3 20.9 15.9 15.5 15.9 17.7 16.8 15.9 13.6 11.4 11.4 105.0 9.5 9.5 10.9 12.7 13.2 13.2 14.5 14.1 15.5 13.2 10.9 10.9 12.7 12.3 11.8 11.4 10.5 9.5 9.5 115.0 7.3 7.3 7.7 8.2 8.6 8.6 10.9 10.0 10.0 9.1 7.7 7.7 9.1 9.1 9.1 9.1 8.2 7.7 8.2 125.0 6.4 6.4 6.4 6.8 6.8 6.8 7.3 7.7 8.2 7.3 6.8 6.4 6.4 6.8 6.8 6.8 6.8 6.8 6.8 135.0 6.4 5.9 5.5 4.5 3.6 3.6 5.9 8.2 8.2 6.8 5.5 4.5 4.5 3.6 3.2 5.0 5.0 5.0 5.0 145.0 3.2 2.7 2.3 2.3 2.3 2.3 2.3 2.3 2.3 3.2 2.3 2.3 1.8 1.4 1.4 2.3 2.3 2.3 3.2 155.0 1.8 1.8 1.8 1.8 1.8 1.8 1.4 1.4 1.4 1.8 1.8 1.8 1.4 0.9 0.9 1.8 1.8 1.8 1.8 165.0 1.8 1.8 1.8 1.8 1.8 1.8 1.4 1.4 1.4 1.4 1.4 1.4 0.0 0.0 0.0 0.9 0.9 0.9 0.9 180.0 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