Image 47
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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 01:31:12
# Resolution : 2048 x 1536 in jpeg (2064x1540 in pgm/47.pgm)
# Focal length : 13.8mm
# Exposure time: 0.004 s (1/250)
# Aperture : f/3.0
# 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 -38 -38 -46 -42 -5.09 -5.39 -7.64 -7.37 -4.32
10 -20 -20 -26 -22 -2.68 -2.84 -4.32 -3.86 -2.19
50 0 0 0 0 0.00 0.00 0.00 0.00 0.00
90 22 20 24 22 2.95 2.84 3.99 3.86 2.63
99 38 38 46 42 5.09 5.39 7.64 7.37 4.32
100 16304 11568 13662 11070 2.18E3 1.64E3 2.27E3 1.94E3 2.16E3
# flux from 0.193 sr ( 2.48E-7 sr/4px) is 0.0240 lx;
# tilewise luminance 0.120 cd/m2 with rel. SD 377 % (summing pixels below 16380)
# dark frame dark/off.pgm subtracted from all values
# Yell average= 0.7 minimum= -92 maximum=16304 over 16380: 0
# Cyan average= 0.3 minimum= -96 maximum=11568 over 16380: 0
# Gree average= -0.0 minimum= -114 maximum=13662 over 16380: 2
# Mage average= 0.4 minimum= -512 maximum=11070 over 16380: 0
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 47.txt -e 47.eps -n 47.ppm -t168 -c 3412 -s64 pgm/47.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)