Full text: XVIIIth Congress (Part B3)

     
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B eu cooper oc mec modems tcc i we 
  
Inputs and outputs: The inputs of a de-shading system are: 
some candidate photometric models, a brightness image and its 
associated approximate height image (range image or DTM 
image). The outputs are: the light source, the photometric 
model approximating the brightness image, the albedo image or 
a 
Re rare oies rem bof nee ia ae 
the surface reflectance properties image (the value of each pixel 
in each image represents the albedo value or reflectance 
property value at its coordinates), the improved height image 
which is more precise than the approximate input height image. 
  
  
  
  
  
light source brightness approximate 
direction image height image 
(y) I( x, y) Z(x, y) 
  
  
  
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candidate 
photometric 
model 1 
gradient images 
p(x,y)andq(x, y) 
  
  
  
  
algorithm DRP [ 
algorithm DPM 
  
for determining the approximate 
  
for determining the reflectance 
properties 0 (x, y), sets Ox (x, » 
  
  
   
photometric model 
  
   
obtained approximate 
  
  
shading algorithm to 
obtain shaded image 
     
  
photometric model 
    
  
l'(x,y) 
  
  
em WN Y, y) t I'(x, »)Ÿ 
e decreases 
9 
  
  
  
  
| 
algorithm DHI (SFS) 
  
  
for determining updated height image Z'( x, y) 
and gradient images p'(x, y), qx. y) 
  
A 
  
  
    
  
output the obtained 
photometric model, 
photometric parameters 
$1 (x, y), ty $i x, y» 
updated height image Z'( x, y), 
and gradient images p' (x, y), q'(x, y) 
  
  
end 
  
WORKING FRAME 
— [Bue 
  
  
Fig.2. A de-shading system. 
3. DE-SHADING SYSTEM 
A de-shading system is proposed in the paper to perform the 
de-shading task. As described in the above section, the task of 
de-shading is to obtain the surface reflectance properties, the 
light source, the improved higher precision height image and 
the approximate photometric model from a given brightness 
image and its associated approximate height image. Obviously, 
this is not easy. Fortunately, there exist some methods being 
more or less relevant to parts of the task. E.g., the least square 
fitting method is used to calculate the surface reflectance 
properties (Ikeuchi and Sato, 1991; Kay and Caelli, 1994), SFS 
is used to obtain the surface orientation and height image 
(Ikeuchi and Horn, 1981; Pentland, 1984; Brooks and Horn, 
1985; Lee and Rosenfeld, 1985; Zheng and Cellappa, 1991; 
Kimmel and Bruckstein, 1995). But all the methods need some 
strong preconditions. Algorithms for calculating surface 
reflectance properties assume that the photometric model is 
known and that the reflectance properties are homogeneous 
over the entire surface, also a precision range image is required. 
The SFS algorithms assume that the surface reflectance 
properties and the photometric model are known. 
Unfortunately, the assumptions might be wrong or the 
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B3. Vienna 1996 
preconditions might not be available in practice. The 
photometric model plays an important role in these problems. 
In order to get the approximate photometric model, a probing 
method may be appropriate. It means, one can approximate the 
correct photometric model by using different known models as 
probing models. The proper model will yield the least error 
between the brightness image and the shaded image obtained 
by using the probing photometric model. But the precondition 
of this method needs a precision height image and the correct 
photometric parameters (reflectance properties). As we see so 
far, the difficulty is that one solution depends on another in a 
circular problem. If we divide the de-shading task into three 
sub-tasks: Determining Photometric Model (DPM), 
Determining Reflectance Properties (DRP) and Determining 
improved Height Image (DHI), each of these sub-tasks needs 
the outputs of the other two as its inputs. This can be illustrated 
as in Fig. 1. 
Considering the above analysis, a de-shading system shown in 
Fig. 2 is developed to perform the de-shading problem. It 
contains two frames. One is the training frame, the other is the 
working frame. The inputs to this system are the illumination 
direction (7,7), a brightness image I(x,y), and an 
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