Image 04
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| original | colour coded
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and with an inserted data grid:
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(in the middle of tiles, median of raw G-pixels values is given,
the bottom value is the tile luminance divided
by one candela per square meter).
# Date/Time : 2005:08:04 14:42:51
# Resolution : 2048 x 1536 in jpeg (2064x1540 in pgm/04.pgm)
# Focal length : 8.2mm
# Exposure time: 0.004 s (1/250)
# Aperture : f/7.0
# ISO equiv. : 100
#c li count min Yav max ovf min Cav max ovf min Gav max ovf min Mav max ovf
# % Y C G M readings Y C G M L / cd/m2
1 -22 -22 -30 -26 -17.3 -18.3 -29.2 -26.7 -13.7
10 2 2 -2 0 1.57 1.66 -1.95 0.00 2.63
50 1112 980 870 776 873 816 847 798 881
90 2860 2764 2306 2232 2.25E3 2.30E3 2.25E3 2.30E3 2.25E3
99 3432 3380 2806 2674 2.69E3 2.81E3 2.73E3 2.75E3 2.68E3
100 12406 12882 10544 10038 9.74E3 1.07E4 1.03E4 1.03E4 9.58E3
# flux from 6.28 sr ( 1.62E-5 sr/4px) is 6.40E3 lx (SQM 2.05E3 nt, 4.30 mag);
# tilewise luminance 991 cd/m2 with rel. SD 97.2 % (summing pixels below 16380)
# dark frame dark/off.pgm subtracted from all values
# Yell average=1291.8 minimum= -66 maximum=12406 over 16380: 0
# Cyan average=1252.6 minimum= -68 maximum=12882 over 16380: 0
# Gree average=1042.3 minimum= -94 maximum=10544 over 16380: 0
# Mage average=1007.7 minimum= -78 maximum=10038 over 16380: 0
End of results of "raw2lum" (version 1.22) with parameters:
-c YCGM -fa -w 7.3 -fc0.214 -o 16380 -d dark/off.pgm -sm200 -nh -i 04.txt -e 04.eps -n 04.ppm -t156 -c 3412 -s64 pgm/04.pgm

Logarithmic luminance scale (the unit is candela per square meter)
– intensities of snow illuminance in lux would be obtained by
multiplying the numeric value of luminance by 3.6. For asphalt,
such a coefficient is between 20 and 40
(or much less, for specular reflection of distant lamps)