# IESNA: LM-63-1995
# [TEST] 768835
# [DATE] 12/04/01
# [MANUFAC] COOPER LIGHTING  
# [LUMCAT] GFX91SXXAR
# [LUMINAIRE] MEDIUM GALLERIA AREA ROUND
# [LAMP] 1000 WATT HPS CLEAR ED-37
# [_REFLECTOR] PREM SPUN AREA ROUND
# [_REFRACTOR] FLAT GLASS
# [_SOCKETPOS] FIXED VERTICAL
# [_LAMPLUMENS] 135000
# TILT=NONE
# Bulbs: 1, 135000 lm each
# Number of measured angles:  37 vertical,   1 horizontal ones
# Photometric type: 1,  Units type: 1
# Luminous openig width, length and height:   0.000   0.000   0.000
# Ballast factor: 1,  Input power: 1000 W


# Source file: gfx9sar.ies
# Luminaire flux = 95063 lx,
#                   70.4 % of the bulb flux
# between 75 and 90:  2.1 % of the luminaire flux
#  - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above:  max   7.6 cd/1000lm ,  0.3 % 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:   27.7
#   for a unit case (glass at 1 m height, 1000 lm bulb) its illumination:
#  Maximum:    68.8 lx
#  Average:   39.0 lx
#  Minimum:    8.7 lx
#  Average/Minimum:    4.5

# 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  48.7
  2.5  49.3
  5.0  51.1
  7.5  54.4
 10.0  59.4
 12.5  65.2
 15.0  70.7
 17.5  76.3
 20.0  81.7
 22.5  87.2
 25.0  92.4
 27.5  97.5
 30.0 101.5
 32.5 104.0
 35.0 105.6
 37.5 105.8
 40.0 109.1
 42.5 116.8
 45.0 134.5
 47.5 164.2
 50.0 191.0
 52.5 211.0
 55.0 244.3
 57.5 265.6
 60.0 255.5
 62.5 226.3
 65.0 191.9
 67.5 154.8
 70.0 120.1
 72.5  85.0
 75.0  48.5
 77.5  17.6
 80.0   7.6
 82.5   3.4
 85.0   1.2
 87.5   0.2
 90.0   0.0