# IESNA:LM-63-1995
# [TEST] 767827
# [DATE] 8/26/97
# [MANUFAC] COOPER LIGHTING
# [LUMCAT] GMX91SXXAR
# [LUMINAIRE] 1000W HPS AREA ROUND
# [LAMP] 1000W HPS CL ED-37
# [_REFLECTOR] SPUN AND STAMPED ALUMINUM
# [_REFRACTOR] CONVEX GLASS
# [_SOCKET POSITION] VERTICAL BASE UP
# [_LAMP LUMENS] 135000
# TILT=NONE    
# Bulbs: 1, 135000 lm each
# Number of measured angles:  47 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: gmx9sar.ies
# Luminaire flux = 86951 lx,
#                   64.4 % of the bulb flux
# between 75 and 90: 15.4 % of the luminaire flux
#  - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above:  max  87.8 cd/1000lm ,  5.7 % of the luminaire flux
# 90deg and above:  max   3.0 cd/1000lm ,  0.4 % 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:  14 %
#  Increase of Sky Luminance in Distant Places by light below 30.0 degrees
#    due to light going from the luminaire directly above horizon:  29 %
#  (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:   20.1
#   for a unit case (glass at 1 m height, 1000 lm bulb) its illumination:
#  Maximum:    39.0 lx
#  Average:   25.9 lx
#  Minimum:   10.2 lx
#  Average/Minimum:    2.5

# 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  24.6
  2.5  24.8
  5.0  25.6
  7.5  28.8
 10.0  32.8
 12.5  37.2
 15.0  41.1
 17.5  43.2
 20.0  44.6
 22.5  46.1
 25.0  48.8
 27.5  52.6
 30.0  57.3
 32.5  62.4
 35.0  69.5
 37.5  77.7
 40.0  86.8
 42.5  96.3
 45.0 104.9
 47.5 112.4
 50.0 119.7
 52.5 126.1
 55.0 130.9
 57.5 142.2
 60.0 154.5
 62.5 165.2
 65.0 175.8
 67.5 182.7
 70.0 180.9
 72.5 170.0
 75.0 150.1
 77.5 121.8
 80.0  87.8
 82.5  52.4
 85.0  22.6
 87.5   5.6
 90.0   3.0
 95.0   1.7
105.0   0.1
115.0   0.0
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