Image 41
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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 : 2005:08:05 01:22:12
# Resolution : 2048 x 1536 in jpeg (2064x1540 in pgm/41.pgm)
# Focal length : 8.2mm
# Exposure time: 0.250 s (1/4)
# Aperture : f/2.5
# 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 -38 -38 -46 -42 -0.0565 -0.0599 -0.0849 -0.0819 -0.0480
10 -20 -20 -24 -22 -0.0298 -0.0315 -0.0443 -0.0429 -0.0254
50 0 0 0 0 0.00 0.00 0.00 0.00 0.00
90 22 22 26 24 0.0327 0.0347 0.0480 0.0468 0.0282
99 40 40 48 44 0.0595 0.0631 0.0886 0.0858 0.0508
100 16318 16304 16314 16318 24.3 25.7 30.1 31.8 22.5
# flux from 0.528 sr ( 7.01E-7 sr/4px) is 6.32E-4 lx;
# tilewise luminance 7.40E-4 cd/m2 with rel. SD 587 % (summing pixels below 16380)
# dark frame dark/off.pgm subtracted from all values
# Yell average= 0.9 minimum= -100 maximum=16318 over 16380: 14
# Cyan average= 0.4 minimum= -84 maximum=16304 over 16380: 11
# Gree average= 0.8 minimum= -98 maximum=16314 over 16380: 15
# Mage average= 0.8 minimum= -88 maximum=16318 over 16380: 7
End of results of "raw2lum" (version 1.22) with parameters:
-c YCGM -fa -w 7.3 -fc1.03 -o 16380 -d dark/off.pgm -sm200 -nh -i 41.txt -e 41.eps -n 41.ppm -t168 -c 3412 -s64 pgm/41.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)