# IESNA: LM-63-1995
# [TEST] 767755   
# [DATE] 6/25/97 
# [MANUFAC] COOPER LIGHTING
# [LUMCAT] MPB15SXX55
# [LUMINAIRE] 150W HPS TYPE V POST TOP
# [LAMP] 150W HPS CL ED-23.5
# [_REFLECTOR] TOP OF CANOPY
# [_REFRACTOR] ACRLYIC 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: mpb1s55.ies
# Luminaire flux =  8634 lx,
#                   54.0 % of the bulb flux
# between 75 and 90: 41.9 % of the luminaire flux
#  - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above:  max 172.1 cd/1000lm , 33.7 % of the luminaire flux
# 90deg and above:  max  47.1 cd/1000lm , 12.4 % 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: 397 %
#  Increase of Sky Luminance in Distant Places by light below 30.0 degrees
#    due to light going from the luminaire directly above horizon: 800 %
#  (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:    5.7
#   for a unit case (glass at 1 m height, 1000 lm bulb) its illumination:
#  Maximum:     8.3 lx
#  Average:    6.1 lx
#  Minimum:    3.4 lx
#  Average/Minimum:    1.8

# 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   3.6
  2.5   3.4
  5.0   3.4
  7.5   3.7
 10.0   4.3
 12.5   5.3
 15.0   5.9
 17.5   5.9
 20.0   5.8
 22.5   6.9
 25.0   7.8
 27.5   7.9
 30.0   8.7
 32.5   8.9
 35.0   9.6
 37.5   8.9
 40.0   8.7
 42.5   9.0
 45.0  10.0
 47.5  11.0
 50.0  13.3
 52.5  20.4
 55.0  32.2
 57.5  47.6
 60.0  66.2
 62.5  84.7
 65.0 109.5
 67.5 143.4
 70.0 170.3
 72.5 182.8
 75.0 188.3
 77.5 185.9
 80.0 172.1
 82.5 142.5
 85.0 102.4
 87.5  67.9
 90.0  47.1
 95.0  27.1
105.0  13.1
115.0   9.6
125.0   6.3
135.0   3.3
145.0   0.4
155.0   0.0
165.0   0.0
175.0   0.0
180.0   0.6