# IESNA: LM-63-1995 # [TEST] 766070 # [DATE] 6/18/91 # [MANUFAC] COOPER LIGHTING # [LUMCAT] HMX91SXXNW # [LUMINAIRE] 1000W HPS TYPE V HIGH MAST # [LAMP] 1000W HPS E-25 # [_REFLECTOR] ANODIZED SPUN ALUMINUM # [_REFRACTOR] NONE # [_SOCKET POSITION] VERTICAL BASE UP # [_LAMP LUMENS] 140000 # TILT=NONE # Bulbs: 1, 140000 lm each # Number of measured angles: 31 vertical, 1 horizontal ones # Photometric type: 1, Units type: 1 # Luminous openig diameter (and height?): 2.330 ( 2.000 ) # Ballast factor: 1, Input power: 1000 W # Source file: hmx9snw.ies # Luminaire flux =114894 lx, # 82.1 % 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 124.1 cd/1000lm , 11.1 % of the luminaire flux # 90deg and above: max 24.2 cd/1000lm , 1.3 % of the luminaire flux # CutOff Type: IES_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: 54 % # Increase of Sky Luminance in Distant Places by light below 30.0 degrees # due to light going from the luminaire directly above horizon: 113 % # (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: 18.2 # for a unit case (glass at 1 m height, 1000 lm bulb) its illumination: # Maximum: 38.7 lx # Average: 29.8 lx # Minimum: 12.6 lx # Average/Minimum: 2.4 # 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): 0.0 33.8 5.0 36.2 15.0 31.4 25.0 42.5 35.0 66.4 45.0 109.5 50.0 142.7 55.0 180.6 60.0 220.8 62.5 235.6 65.0 235.9 67.5 224.4 70.0 208.4 72.5 188.2 75.0 164.8 77.5 143.6 80.0 124.1 82.5 100.3 85.0 74.1 87.5 46.6 90.0 24.2 95.0 5.0 105.0 0.0 115.0 0.1 125.0 0.0 135.0 0.0 145.0 0.0 155.0 0.0 165.0 0.0 175.0 0.0 180.0 0.0