# IESNA: LM-63-1995
# [TEST] 48312     
# [DATE] 1/6/81  
# [MANUFAC] COOPER LIGHTING   
# [LUMCAT] HMX40MXXDW  
# [LUMINAIRE] 400W MH TYPE V HIGH MAST  
# [LAMP] 400W MH CL ET-37  
# [_REFLECTOR] ANODIZED SPUN ALUMINUM  
# [_REFRACTOR] CONVEX GLASS 
# [_SOCKET POSITION] VERTICAL BASE UP 
# [_LAMP LUMENS] 34000 
# TILT=NONE
# Bulbs: 1,  34000 lm each
# Number of measured angles:  19 vertical,  21 horizontal ones
# Photometric type: 1,  Units type: 1
# Luminous openig diameter (and height?):   2.330  (   2.000 )
# Ballast factor: 1,  Input power:  400 W


# Source file: hmx4mdw.ies
# Luminaire flux = 17919 lx,
#                   52.7 % of the bulb flux
# between 75 and 90:  6.4 % of the luminaire flux
#  - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above:  max  14.6 cd/1000lm ,  0.7 % 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:   20.6
#   for a unit case (glass at 1 m height, 1000 lm bulb) its illumination:
#  Maximum:    95.0 lx
#  Average:   21.7 lx
#  Minimum:   14.9 lx
#  Average/Minimum:    1.5

# 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):

#  H:   0.0   5.0  15.0  25.0  35.0  45.0  55.0  65.0  75.0  85.0  90.0  95.0 105.0 115.0 125.0 135.0 145.0 155.0 165.0 175.0 180.0
#V:  
  0.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0  95.0
  5.0  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2  71.2
 10.0  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2  52.2
 15.0  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2  37.2
 20.0  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6  31.6
 25.0  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4  40.4
 30.0  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5  49.5
 35.0  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4  55.4
 40.0  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1  62.1
 45.0  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1  68.1
 50.0  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8  76.8
 55.0  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6  88.6
 60.0 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2 124.2
 65.0 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8 197.8
 70.0 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6 251.6
 75.0  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3  97.3
 80.0  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6  14.6
 85.0   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1   4.1
 90.0   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   0.0   0.0