# IESNA: LM-63-1995
# [TEST] 768742
# [DATE] 9/07/01
# [MANUFAC] COOPER LIGHTING  
# [LUMCAT] ACN17MXX55X4X
# [LUMINAIRE] 175WATT MH TYPE V REFRACTIVE GLOBE
# [MORE] W/SPUN TOP  
# [LAMP] 175 WATT MH CLEAR ED-28
# [_REFLECTOR] NONE
# [_REFRACTOR] TYPE V ACRYLIC
# [_SOCKETPOS] FIXED BASE DOWN
# [_LAMPLUMENS] 14000
# TILT=NONE
# Bulbs: 1,  14000 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:  175 W


# Source file: arc1m54.ies
# Luminaire flux =  9082 lx,
#                   64.9 % of the bulb flux
# between 75 and 90: 28.1 % of the luminaire flux
#  - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above:  max 134.9 cd/1000lm , 18.7 % of the luminaire flux
# 90deg and above:  max  23.5 cd/1000lm ,  9.0 % 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: 232 %
#  Increase of Sky Luminance in Distant Places by light below 30.0 degrees
#    due to light going from the luminaire directly above horizon: 450 %
#  (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:    8.5
#   for a unit case (glass at 1 m height, 1000 lm bulb) its illumination:
#  Maximum:    15.8 lx
#  Average:   11.0 lx
#  Minimum:    4.2 lx
#  Average/Minimum:    2.6

# 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   4.6
  5.0   4.3
  7.5   4.7
 10.0   5.2
 12.5   5.8
 15.0   6.6
 17.5   7.1
 20.0   7.9
 22.5   9.0
 25.0  10.5
 27.5  12.9
 30.0  16.2
 32.5  17.6
 35.0  20.6
 37.5  22.4
 40.0  30.0
 42.5  38.7
 45.0  44.8
 47.5  46.4
 50.0  49.9
 52.5  62.3
 55.0  73.5
 57.5  72.1
 60.0  72.4
 62.5  76.4
 65.0 108.4
 67.5 181.9
 70.0 284.4
 72.5 336.6
 75.0 293.2
 77.5 208.0
 80.0 134.9
 82.5  80.1
 85.0  43.3
 87.5  29.4
 90.0  23.5
 95.0  18.1
105.0  14.1
115.0   9.4
125.0   6.6
135.0   4.7
145.0   3.2
155.0   1.8
165.0   0.7
175.0   0.3
180.0   0.3