# IESNA: LM-63-1995
# [TEST] 76777  
# [DATE] 7/08/97
# [MANUFAC] COOPER LIGHTING
# [LUMCAT] MPW15SXX55
# [LUMINAIRE] 150W HPS TYPE V POST TOP 
# [LAMP] 150W HPS CL ED-23.5
# [_REFLECTOR] TOP OF CANOPY
# [_REFRACTOR] ACRYLIC PRISMATIC TYPE V
# [_SOCKET POSITION] VERTICAL BASE DOWN
# [_LAMP LUMENS] 16000
# TILT=NONE                                   
# Bulbs: 1,  16000 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:  150 W


# Source file: mpw1s55.ies
# Luminaire flux =  9276 lx,
#                   58.0 % of the bulb flux
# between 75 and 90: 33.7 % of the luminaire flux
#  - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above:  max 137.0 cd/1000lm , 25.8 % of the luminaire flux
# 90deg and above:  max  48.8 cd/1000lm , 10.1 % 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: 368 %
#  Increase of Sky Luminance in Distant Places by light below 30.0 degrees
#    due to light going from the luminaire directly above horizon: 769 %
#  (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:    8.6
#   for a unit case (glass at 1 m height, 1000 lm bulb) its illumination:
#  Maximum:    18.4 lx
#  Average:   10.0 lx
#  Minimum:    4.9 lx
#  Average/Minimum:    2.0

# 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   4.9
  2.5   6.9
  5.0   8.8
  7.5  12.3
 10.0  16.0
 12.5  18.9
 15.0  20.4
 17.5  20.2
 20.0  18.5
 22.5  16.8
 25.0  14.5
 27.5  13.5
 30.0  13.9
 32.5  13.6
 35.0  12.7
 37.5  12.6
 40.0  14.0
 42.5  16.8
 45.0  21.1
 47.5  27.8
 50.0  36.8
 52.5  47.0
 55.0  58.3
 57.5  70.2
 60.0  86.1
 62.5 111.9
 65.0 149.4
 67.5 178.3
 70.0 193.1
 72.5 195.9
 75.0 191.9
 77.5 175.7
 80.0 137.0
 82.5 102.6
 85.0  77.0
 87.5  60.8
 90.0  48.8
 95.0  33.0
105.0  12.4
115.0   4.2
125.0   1.0
135.0   0.1
145.0   0.0
155.0   0.0
165.0   0.0
175.0   0.0
180.0   0.0