Full text: Proceedings of ISP Commission 1 symposium on data acquisition and improvement of image quality and image geometry

ESTATE 
AS A 
m, between calibrations 6 and 7 is undoubtedly the result of the 
use of a larger number of points with extrapolated lens distortion 
corrections in connection with calibration 73 the number of these 
points is given in Table 5. 
This conclusion is supported by the results obtained using 
calibration 5. Elimination of the 12 points farthest away from the 
center of the photograph reduced my from 3.93 to 2.00. Although my 
and m, are significantly larger (by approximately 50%) than those 
for the other calibrations, X and Y are practically the same. The 
effect of the obviously less effective lens distortion correction 
in the corner areas of the format is felt primarily as elevation 
errors. Table 5 also lists for each calibration the maximum radius 
for which the lens distortion was actually determined. These radii 
are indicated in Figure 5 from which it is obvious that calibration 5 
cannot indicate the steep increase in lens distortion occurring in 
the corner areas. The same is true for calibrations 7, 2 and 6 
to an increasingly lesser extent. This figure underlines the 
necessity to determine the lens distortion as far as possible into 
the format corners. 
  
  
  
The root mean square positional errors within the groups of points 
were computed 2gain for the same calibration as before. They are 
3222 T. x e 
similar (m, - - 3.0 um, mys X 2.7 um). 
4. CONCLUSION 
Image quality and lens distortion data obtained from the still 
on-going activities of the Working Group on Image Geometry have 
been presented in the form in which they were documented by the 
working group members. Because of variations in data presentation, 
conclusions from data comparisons are general in nature and tentative. 
  
A number of contributions to the program have not yet been 
completed and documented. It is hoped that this will be done in time 
in order that the report to the 1980 congress will be the final report. 
Outstanding are all system calibrations over test fields and the 
calibrations carried out with the Itek Artificial Stellar Calibrator. 
  
It is also hoped that all data will become available to permit 
processing using the same procedures. Such processing is obviously 
required if calibrated focal lengths, reference point locations and 
lens distortion values are to be compared with each other. 
  
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