Image 30

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 01:10:25
# Resolution   : 2048 x 1536 in jpeg (2064x1540 in pgm/30.pgm)
# Focal length : 23.4mm
# Exposure time: 0.017 s  (1/60)
# 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   -40   -46   -42      -2.17    -2.42    -3.26    -3.14    -1.85  
 10   -22   -22   -24   -22      -1.26    -1.33    -1.70    -1.65    -1.12  
 50     0     0     0     0       0.00     0.00     0.00     0.00     0.00  
 90    22    22    24    22       1.26     1.33     1.70     1.65     1.12  
 99    40    40    46    40       2.29     2.42     3.26     2.99     1.99  
100 16314 16300 16302 16300        932      987     1.16E3   1.22E3    865  
# flux from 0.0680 sr ( 8.61E-8 sr/4px) is  0.00340 lx;
# tilewise luminance  0.0515 cd/m2 with rel. SD  607 % (summing pixels below 16380)
# dark frame dark/off.pgm subtracted from all values
# Yell average=   0.8  minimum=  -90  maximum=16314   over 16380:   5
# Cyan average=   0.5  minimum=  -80  maximum=16300   over 16380:   2
# Gree average=   0.6  minimum= -102  maximum=16302   over 16380:  11
# Mage average=   0.2  minimum= -242  maximum=16300   over 16380:   4

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 30.txt -e 30.eps -n 30.ppm -t168 -c 3412 -s64 pgm/30.pgm

Just points with luminances over 50 and below 6.0E2 cd/m2. In grid tiles, flux densities from these points and tiles are given.
# Date/Time    : 2005:08:05 01:10:25
# Resolution   : 2048 x 1536 in jpeg (2064x1540 in pgm/30.pgm)
# Focal length : 23.4mm
# Exposure time: 0.017 s  (1/60)
# 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   -40   -46   -42      -2.17    -2.42    -3.26    -3.14    -1.85  
 10   -22   -22   -24   -22      -1.26    -1.33    -1.70    -1.65    -1.12  
 50     0     0     0     0       0.00     0.00     0.00     0.00     0.00  
 90    22    22    24    22       1.26     1.33     1.70     1.65     1.12  
 99    40    40    46    40       2.29     2.42     3.26     2.99     1.99  
100 16314 16300 16302 16300        932      987     1.16E3   1.22E3    865  
# flux from 1.20E-5 sr ( 8.61E-8 sr/4px) is  0.00231 lx;
# tilewise luminance  6.00 cd/m2 with rel. SD  553 % (points with luminances over   50    and below  6.0E2 )
# dark frame dark/off.pgm subtracted from all values
# Yell average=3239.9  minimum=  -90  maximum=16314   out of range: 794494
# Cyan average=2895.5  minimum=  -80  maximum=16300   out of range: 794491
# Gree average=2619.2  minimum= -102  maximum=16302   out of range: 794500
# Mage average=2688.9  minimum= -242  maximum=16300   out of range: 794493

End of results of "raw2lum" (version 1.22) with parameters:
  -c YCGM -ft -w 7.3 -fc1.03 -o 16380 -L50 -U600 -d dark/off.pgm -sm200 -nh -i 30.txt -e 30.eps -n 30.ppm -t168 -c 3412 -s64 pgm/30.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)