Image 07
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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 00:34:01
# Resolution : 2048 x 1536 in jpeg (2064x1540 in pgm/07.pgm)
# Focal length : 11.2mm
# Exposure time: 2.000 s
# Aperture : f/7.8
# 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 -36 -40 -52 -44 -0.0702 -0.0827 -0.126 -0.112 -0.0535
10 -12 -20 -24 -20 -0.0234 -0.0413 -0.0580 -0.0511 -0.0130
50 16 8 8 12 0.0312 0.0165 0.0193 0.0307 0.0348
90 60 36 44 48 0.117 0.0744 0.106 0.123 0.120
99 280 112 128 188 0.546 0.232 0.310 0.480 0.617
100 16332 16332 16340 16352 31.8 33.8 39.5 41.8 29.5
# flux from 5.55 sr ( 8.71E-6 sr/4px) is 0.317 lx (SQM 0.131 nt, 14.79 mag);
# tilewise luminance 0.0673 cd/m2 with rel. SD 210 % (summing pixels below 16380)
# dark frame dark/2s.pgm subtracted from all values
# Yell average= 31.1 minimum= -132 maximum=16332 over 16380: 115
# Cyan average= 13.1 minimum= -352 maximum=16332 over 16380: 139
# Gree average= 12.8 minimum= -284 maximum=16340 over 16380: 174
# Mage average= 20.5 minimum= -512 maximum=16352 over 16380: 119
End of results of "raw2lum" (version 1.22) with parameters:
-c YCGM -fa -w 7.3 -fc0.214 -o 16380 -d dark/2s.pgm -sm200 -nh -i 07.txt -e 07.eps -n 07.ppm -t156 -c 3412 -s64 pgm/07.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)