# IESNA: LM-63-1995 # [TEST] 763568 # [DATE] 2/24/94 # [MANUFAC] COOPER LIGHTING # [LUMCAT] EGL91SXX55 # [LUMINAIRE] 1000W HPS 5H X 5V FLOOD # [LAMP] 1000W HPS CL E-25 # [_REFLECTOR] SPUN ALUMINUM # [_REFRACTOR] CLEAR FLAT GLASS # [_SOCKET POSITION] AXIAL # [_LAMP LUMENS] 140000 # TILT=NONE # Bulbs: 1, 140000 lm each # Number of measured angles: 37 vertical, 1 horizontal ones # Photometric type: 1, Units type: 1 # Luminous openig diameter (and height?): 1.830 ( 1.750 ) # Ballast factor: 1, Input power: 1000 W # Source file: egl91s55.ies # Luminaire flux =109381 lx, # 78.1 % of the bulb flux # between 75 and 90: 0.0 % of the luminaire flux # - this part causes just GLARE in case of road lighting and similar purposes # 80deg and above: max 0.0 cd/1000lm , 0.0 % of the luminaire flux # 90deg and above: max 0.0 cd/1000lm , 0.0 % of the luminaire flux # CutOff Type: Full_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: 0 % # Increase of Sky Luminance in Distant Places by light below 30.0 degrees # due to light going from the luminaire directly above horizon: 0 % # (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: 46.8 # for a unit case (glass at 1 m height, 1000 lm bulb) its illumination: # Maximum: 1943.3 lx # Average: 73.1 lx # Minimum: 0.5 lx # Average/Minimum: 143.7 # 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): 0.01815.3 2.51948.9 5.01710.5 7.51263.8 10.0 907.0 12.5 685.5 15.0 545.0 17.5 455.2 20.0 391.9 22.5 345.9 25.0 310.1 27.5 281.7 30.0 257.4 32.5 235.4 35.0 217.7 37.5 206.4 40.0 196.4 42.5 185.4 45.0 170.7 47.5 152.6 50.0 129.1 52.5 98.5 55.0 65.9 57.5 43.2 60.0 30.6 62.5 22.2 65.0 15.2 67.5 9.1 70.0 3.6 72.5 0.1 75.0 0.0 77.5 0.0 80.0 0.0 82.5 0.0 85.0 0.0 87.5 0.0 90.0 0.0