Full text: XVIIIth Congress (Part B1)

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Three different methods of weighting the pixels were 
used, being binary (Bl), grey value (GV) and grey value 
squared (GV^2). The binary method applied a weight of 
one to each pixel, the grey value method weighted each 
pixel by its grey value and therefore, the brighter the grey 
value the more importance was put on the pixel. The 
grey value squared method used the square of the grey 
value at the weight to be applied, thus exaggerating the 
effect as described in the grey value method. Each 
method produced a separate set of observations and 
each was processed through the bundle adjustment. The 
results from each method have been tabulated in 
Section 5. However, only the binary results have been 
graphed in Figures 5, 6, 7 and 8 as the results from each 
method were very similar. 
The program described above was customised to output 
files in the format compatible with the bundle adjustment 
being used. Three bundle adjustment programs were 
used initially for comparisons, with SPGA (Fraser, 1982) 
eventually being the sole bundle adjustment used as it 
was flexible, fast and efficient. 
Prior to processing the observations in the bundle 
adjustment, the decentering distortion parameters P1 and 
P2 were determined using a plumbline lens calibration. 
These values were used as initial values in the bundle 
adjustment, to overcome the correlation problems with 
the offsets to the principal point, as previously 
mentioned. 
5. RESULTS 
The results from the calibration procedure have been 
tabulated and graphed in this section and include the 
calibration parameters for each camera, an analysis of 
the benefits of averaging images from video cameras, 
and an analysis of the benefits of radiometric corrections 
for ‘bad’ pixels and a comparison of the suitability of each 
camera for close-range photogrammetric measurement. 
The calibration parameters for each camera are shown in 
Table 4. This table includes: the root mean square of the 
image coordinate errors in x and y; the focal length; the 
offsets to the principal point in x and y; lens distortion 
parameters K; , Ke , P; and P» ; and the degrees of 
freedom from each bundle adjustment. From this table, 
it can be seen that the Single Frame of the Right Philips 
camera is only marginally worse in image coordinate 
RMS than the averaged binary, GV or GV squared, 
however, the averaging does improve the visual quality of 
the images, removing phase patterns and line jitter. The 
focal length was determined consistently for each 
camera. The Right Philips camera was shown to have a 
relatively large x component in the principal point offsets. 
The final values for P; as shown in Table 4 vary by only 
5-1096 from the initial values determined by the 
plumbline lens calibration. 
The radiometric investigation, as described in 
Section 3.2, determined that there were no 'bad' pixels in 
these digital still cameras, and 'bad' pixels found in the 
analog video cameras were more due to sampling and 
signal transmission than problems in array. This was 
141 
concluded after many images were acquired to find the 
'bad' pixels in the video cameras, and the results were 
not consistent, but changed with each image. 
The lens distortion parameters are graphed in Figures 5, 
6, 7 and 8 in Section 5.3. The resultant values for the 
binary, grey value and grey value squared methods were 
all very similar, as can be seen in Table 4 and only the 
results of the binary method are graphed. The large 
radial distortion of the Apple Quicktake and the Logitech 
Fotoman should be noted. At a radial distance of 2mm, 
it is equivalent to a shift of 2 pixels, and at the edges of 
the array amounted to approximately 6 to 7 pixels. This 
would have to be considered when using the cameras for 
photogrammetric applications. Any targets or objects to 
be measured would best be situated close to the centre 
of the image to ensure the best results. 
5.1 Statistical Results of Target Centroiding. 
  
  
Camera Average Average Average Pixels 
Maximum Minimum Threshold above 
GV GV (0-255) Threshold 
Left Philips 253.54 6.92 167.19 117.10 
Right Philips 253.79 2.92 165.72 131.48 
Apple Quicktake 254.55 1.18 159.76 24.19 
Logitech Fotoman 255.00 12.76 170.98 29.38 
  
  
Table 2. Statistical Results of Target Centroiding 
As referred to in Section 4, Table 2 shows that the 
contrast between the targets (average maximum grey 
value) and the background (average minimum grey 
value) on the images was very high, which is beneficial 
for the centroiding of the targets. 
5.2 Additional Parameters. See Section 3.1 for a 
mathematical description. 
  
  
  
  
Camera Di b2 Ds ai 
Left Philips 
Binary 0.246E-3 0.0298 ** 0.452E-3 0.202E-2 * 
GV 0.274E-3 0.0298 ** 0.351E-3 0.221E-2 * 
GV^2 0.259E-3 0.0298 ** 0.427E-3 0.221E-2* 
Right Philips 
Binary 0.270E-3 0.0298 ** -0.302E-4 0.173E-2 * 
GV 0.269E-3 0.0298 ** -0.859E-4 0.174E-2 * 
GV^2 0.256E-3 0.0299 ** -0.721E-4 0.171E-2 * 
Single Frame 0.112E-3 0.0298 ** 0.137E-3 0.191E-2 * 
Apple Quicktake 
Binary 0.273E-4 0.518E-4 -0.331E-4 -0.380E-4 
GV 0.233E-4 0.448E-4 -0.210E-4 -0.484E-4 
GV^2 0.267E-4 0.315E-4 0.249E-5 -0.418E-4 
Logitech Fotoman 
Binary 0.698E-4 0.729E-4 -0.716E-4 -0.933E-4 
GV 0.689E-4 0.752E-4 -0.815E-4 -0.894E-4 
GV^2 0.716E-4 0.720E-4 -0.770E-4 -0.830E-4 
* Significant ** Very Significant 
( Significance determined by Fisher statistical analysis, 
see Fraser, 1982) 
Table 3. Additional Parameters. 
The most notable additional parameter in Table 3 is that 
of b» for the Philips cameras, showing that the actual 
size of the pixel in the y direction is 396 different from the 
initial value used. 
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B1. Vienna 1996 
 
	        
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