Full text: XIXth congress (Part B3,2)

  
Ono Tetsu 
  
3 ADVANTAGES OF 2D AFFINE PROJECTION MODEL 
2D affine projection model has superior characteristics due to the simple forms. Firstly, the model is quite 
robust and stable for image orientation and triangulation even without prior orbit information because of the 
linearity. Secondly, the higher spatial resolution of satellite imagery become, the more efficient this model will 
be in point of precision. Okamoto et al (1999) showed with orientation results of SPOT imagery and MOMS-2p 
one that the precision of this model corresponds well to that of central projection-based method. A further 
important point is that 2D affine projection model is very suitable for mapping. Image coordinates can be 
rapidly calculated from giving ground coordinates and orientation parameters. 
3.1 Real-time Positioning 
Stereo-plotter usually accepts ground coordinates X,Y,Z as input and the corresponding image coordinates 
are calculated for image positioning controls. In conventional aerial photograph, the image coordinates can be 
‘directly calculated by the collinearity equations. On the contrary, as the exterior orientation parameters of 
satellite imagery are described as a function of the image line number i, which is initially unknown, an initial 
approximation of image coordinate must be gradually refined by iterations. Whereas the collinearity equations 
for a pair of aerial photographs require 24 computer multiplications to transform ground coordinates to image 
coordinates, rigorous 1D central perspective approaches for a pair of satellite images require between 300 and 
500 computer multiplications (Gugan, 1987). For the real-time image positioning on digital stereo-plotter, the 
number of computer multiplications must be reduced. 
Fitting to a polynomial equation with small number of terms is an efficient approach (Kratky, 1989). But, 
2D affine projection model is faster than Kratky's fitting model. The same process requires only 20 multipli 
cations. If the translations from original imagery to affine imagery are carried out in advance, the number of 
multiplications is reduced to only 12. 
3.2 Generation of Ortho-Image with Existing DTMs 
With existing D'TMs, ortho-image can be generated from single satellite image. The ground coordinates of object 
field are given by DTMs and the corresponding image coordinates are computed by collinearity equations. In 
1D central perspective model, however, image coordinates are acquired by iterative calculation as discussed in 
the previous sections. 2D affine projection model has an advantage here again, which the image coordinates 
can be directly calculated by the collinearity equations. Figure 1 indicates the essential features of the process. 
  
Ground Truth/GPS Surveying Satellite Image Acquisition/Transfer 
Satellite Images 
| Observation of Image Points Epipolar Resampling 
  
  
  
  
  
     
   
GCPs, Check Points 
   
  
  
  
  
  
  
  
  
  
  
  
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With DTMs 
  
Single Image Orientation 
Orientation Parameters 
Ortho Image Generation 
Stereo Image Orientation Stereo Matching 
Orientation Parameters 
DTM creation/Editing 
Resampling 
  
  
  
  
  
         
    
  
  
  
  
  
  
  
  
ithout DTMs 
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Ortho Image 
Figure 1: Scheme for ortho-image production from satellite imagery 
  
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3.3 Generation of Ortho-Image without DTMs 
In case of ortho-image generation without existing DTMs, the necessary DTMs must be acquired via stereo 
matching methods. The sequence of the operations is followed: epipolar resampling, stereo matching and, 
  
674 International Archives of Photogrammetry and Remote Sensing. Vol.. XXXIII, Part B3. Amsterdam 2000. 
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