Image 32

original colour coded

and with an inserted data grid:

(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 01:11:01
# Resolution   : 2048 x 1536 in jpeg (2064x1540 in pgm/32.pgm)
# Focal length : 23.4mm
# Exposure time: 0.250 s  (1/4)
# Aperture     : f/4.0
# 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      -0.145   -0.153   -0.217   -0.210   -0.123 
 10   -20   -20   -26   -22      -0.0762  -0.0808  -0.123   -0.110   -0.0622
 50     0     0     0     0       0.00     0.00     0.00     0.00     0.00  
 90    22    22    26    24       0.0838   0.0888   0.123    0.120    0.0721
 99    44    42    50    46       0.168    0.170    0.236    0.230    0.147 
100 16322 16320 16320 16320       62.2     65.9     77.1     81.4     57.7  
# flux from 0.0680 sr ( 8.61E-8 sr/4px) is  7.11E-4 lx;
# tilewise luminance  0.00981 cd/m2 with rel. SD  415 % (summing pixels below 16380)
# dark frame dark/off.pgm subtracted from all values
# Yell average=   2.7  minimum=  -80  maximum=16322   over 16380:  90
# Cyan average=   2.4  minimum=  -88  maximum=16320   over 16380: 108
# Gree average=   1.8  minimum= -102  maximum=16320   over 16380: 125
# Mage average=   3.2  minimum=  -88  maximum=16320   over 16380: 102

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 32.txt -e 32.eps -n 32.ppm -t168 -c 3412 -s64 pgm/32.pgm

Just points with luminances over 1.5 and below 50 cd/m2. In grid tiles, flux densities from these points and tiles are given.
# Date/Time    : 2005:08:05 01:11:01
# Resolution   : 2048 x 1536 in jpeg (2064x1540 in pgm/32.pgm)
# Focal length : 23.4mm
# Exposure time: 0.250 s  (1/4)
# Aperture     : f/4.0
# 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      -0.145   -0.153   -0.217   -0.210   -0.123 
 10   -20   -20   -26   -22      -0.0762  -0.0808  -0.123   -0.110   -0.0622
 50     0     0     0     0       0.00     0.00     0.00     0.00     0.00  
 90    22    22    26    24       0.0838   0.0888   0.123    0.120    0.0721
 99    44    42    50    46       0.168    0.170    0.236    0.230    0.147 
100 16322 16320 16320 16320       62.2     65.9     77.1     81.4     57.7  
# flux from 3.52E-5 sr ( 8.61E-8 sr/4px) is  2.90E-4 lx;
# tilewise luminance  0.500 cd/m2 with rel. SD  444 % (points with luminances over  1.5    and below   50   )
# dark frame dark/off.pgm subtracted from all values
# Yell average=2367.4  minimum=  -80  maximum=16322   out of range: 794172
# Cyan average=2949.4  minimum=  -88  maximum=16320   out of range: 794190
# Gree average=2346.1  minimum= -102  maximum=16320   out of range: 794207
# Mage average=3210.9  minimum=  -88  maximum=16320   out of range: 794184

End of results of "raw2lum" (version 1.22) with parameters:
  -c YCGM -ft -w 7.3 -fc1.03 -o 16380 -L1.5 -U50 -d dark/off.pgm -sm200 -nh -i 32.txt -e 32.eps -n 32.ppm -t168 -c 3412 -s64 pgm/32.pgm

Luminance scale / 1 
cd/m<sup>2</sup>
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)