# IESNA:LM-63-2002
# [TEST]769295
# [TESTLAB]COOPER LIGHTING
# [ISSUEDATE]05/19/03
# [MANUFAC]COOPER LIGHTING
# [LUMCAT]GMX40MXXAR
# [LUMINAIRE]MEDIUM ARCHITECTURAL AREA LUMINAIRE- VERTICAL LAMP, ROUND DISTRIBUTION
# [LAMP]400 WATT MH CLEAR BT-37 BASE UP
# [_REFRACTOR]CLEAR SAG GLASS
# [_SOCKETPOS]FIXED VERTICAL BASE UP
# [LAMPLUMENS]36000
# TILT=NONE
# Bulbs: 1,  36000 lm each
# Number of measured angles:  73 vertical,   1 horizontal ones
# Photometric type: 1,  Units type: 1
# Luminous openig diameter (and height?):   1.604  (   0.000 )
# Ballast factor: 1,  Input power:  400 W


# Source file: gmx4mar.ies
# Luminaire flux = 24309 lx,
#                   67.5 % of the bulb flux
# between 75 and 90: 16.7 % of the luminaire flux
#  - this part causes just GLARE in case of road lighting and similar purposes
# 80deg and above:  max 100.9 cd/1000lm ,  5.6 % of the luminaire flux
# 90deg and above:  max   2.4 cd/1000lm ,  0.2 % 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:   8 %
#  Increase of Sky Luminance in Distant Places by light below 30.0 degrees
#    due to light going from the luminaire directly above horizon:  17 %
#  (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:   19.0
#   for a unit case (glass at 1 m height, 1000 lm bulb) its illumination:
#  Maximum:    37.8 lx
#  Average:   25.7 lx
#  Minimum:   10.8 lx
#  Average/Minimum:    2.4

# 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  36.1
  2.5  32.5
  5.0  29.5
  7.5  30.6
 10.0  32.4
 12.5  35.9
 15.0  39.7
 17.5  37.8
 20.0  39.8
 22.5  43.4
 25.0  47.4
 27.5  51.2
 30.0  54.9
 32.5  59.1
 35.0  64.3
 37.5  71.1
 40.0  81.2
 42.5  94.2
 45.0 105.5
 47.5 114.2
 50.0 119.9
 52.5 127.2
 55.0 128.7
 57.5 146.9
 60.0 161.5
 62.5 171.6
 65.0 181.4
 67.5 192.1
 70.0 202.3
 72.5 195.6
 75.0 177.1
 77.5 145.4
 80.0 100.9
 82.5  51.9
 85.0  22.6
 87.5   6.7
 90.0   2.4
 92.5   1.5
 95.0   1.0
 97.5   0.8
100.0   0.6
102.5   0.3
105.0   0.1
107.5   0.0
110.0   0.0
112.5   0.0
115.0   0.0
117.5   0.0
120.0   0.0
122.5   0.0
125.0   0.0
127.5   0.0
130.0   0.0
132.5   0.0
135.0   0.0
137.5   0.0
140.0   0.0
142.5   0.0
145.0   0.0
147.5   0.0
150.0   0.0
152.5   0.0
155.0   0.0
157.5   0.0
160.0   0.0
162.5   0.0
165.0   0.0
167.5   0.0
170.0   0.0
172.5   0.0
175.0   0.0
177.5   0.0
180.0   0.0