Full text: XVIIIth Congress (Part B3)

    
   
   
    
   
      
  
   
    
     
   
   
   
    
   
    
  
     
    
     
    
    
    
     
   
   
    
    
     
    
    
   
   
   
    
    
    
   
   
    
   
    
  
    
  
   
Use Mapping 
> framework of 
ustrian Science 
rview of a pro- 
1. The physical 
understanding 
s are defined in 
| Rahmen des 
chischen Fonds 
ein vorgeschla- 
1) Modells der 
wird formuliert 
otischen Satel- 
h geometrische 
ration and the 
: expert knowl- 
remote sensing 
ledge in an au- 
image acquisi- 
(more exactly: 
. Image analy- 
his process: In 
erived from an 
therefore is to 
nodel of image 
ical model con- 
> radiometry of 
tric calibration 
lation parame- 
and reflectance 
thematic map 
gions, line ob- 
rted here, the 
t frequent ob- 
d considerably 
| segmentation 
quisition is ap- 
nalysis system 
trated in Fig.1 
  
reality model 
  
n t scene 
| objects 
(exposure 
model)" 
: : image 
image —{ segmentation | — objects 
  
  
  
  
  
     
  
  
  
  
  
  
  
  
  
  
  
  
  
  
  
  
Figure 1: Information flow in the proposed image understand- 
ing system: Subdivision of the problem into segmentation and 
physical model application 
[Schneider, Bartl, 1995]. 
Starting from the image, image objects are identified by seg- 
mentation according to homogeneity criteria. The advantage 
of this approach is twofold: 
1. The amount of information to be processed in the fol- 
lowing analysis is reduced so that it becomes man- 
agable, and 
2. the mixed-pixel-problem can be brought under con- 
trol: A high percentage of the pixels of a satellite 
image are mixed pixels containing radiometric infor- 
mation of more than one surface category at an un- 
known mixing ratio. If the segmentation is performed 
employing spatial subpixel analysis [Schneider, 1993, 
Steinwendner, 1996], objects with pure spectral signa- 
tures can be obtained even in the case of a very high 
percentage of mixed pixels in the original image. 
The physical model of image acquisition transforms the re- 
flectance characteristics px; of objects à (regions on the ter- 
rain surface) in spectral bands k, to pixel values di; in the 
image. This transformation is influenced by global parame- 
ters pA, describing the various absorption and scattering pro- 
cesses in the atmosphere, and by sensor parameters pr. The 
parameters pa usually are unknown. 
The image understanding problem is to assign every region 
object à to one surface category C;. The set of possible sur- 
face categories is defined a priori by the (mean) reflectance 
values pic of the categories C in the spectral bands k. For 
certain categories C, other properties (geometrical parame- 
ters such as shape or size descriptors of the regions belonging 
to these categories) may be characteristic. The mean values 
of these geometrical parameters for categoty C are denoted 
gio where j is an index defining the parameter. gj; is the 
geometrical parameter j for object i as determined from the 
image. The image understanding problem can now be for- 
mulated in the following way: Given are 
e the physical model 
dpi = du (Phi, PA,PI) (1) 
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B3. Vienna 1996 
the sensor parameters pr, 
e the (mean) pixel values dx; of the objects, 
e the (mean) reflectance values pc of the surface cate- 
gories to be identified, and 
e the (mean) geometrical parameter gc of the surface 
categories to be identified. 
The problem is to find the global parameters DA and the 
category C; of every object in such a way that 
3a : (pri — Pk). N° b; - (gji — 9;c;). — Min. (2) 
ki ji 
The quantities a; and b; here are the weights of the different 
spectral bands and geometrical parameters. These weights 
also determine the relative importance of the geometrical pa- 
rameters as compared to the spectral characteristics. 
Reference information ("ground truth data") can be used 
in this image understanding scheme: "Radiometric control 
points" (reference surfaces on the terrain with given re- 
flectance data) may provide input values for px;, and "the- 
matic control points” (regions with known land use) may 
provide input values for C;. 
3 PHYSICAL MODEL 
Object reflectance, radiance and irradiance quantities as well 
as atmospheric absorption and scattering are expressed as in- 
tegral quantities for the individual discrete spectral bands of 
the sensor. Assuming a sensor with linear radiometric re- 
sponse, the pixel value dg; is related to the radiance Lj; 
incident on the sensor instrument I by 
dri = myLik; 0; (3) 
mx and a, are the multiplicative factor and the additive term, 
respectively, characterizing the response of the sensor to in- 
cident radiation in the spectral band k. 
Lik; can be traced back to pk; with the use of a computer- 
coded numeric model such as LOWTRANT: 
Li Lm. pi) (4) 
This method is very general and fairly accurate, but compu- 
tationally expensive. One has to bear in mind that numerous 
evaluations of (4) are necessary to solve (2). 
In an attempt to formulate the problem analytically to facili- 
tate computation, Lj; can be regarded as a sum of 3 terms 
(Fig. 2): of the radiance reflected by the terrain surface, Lj; 
(i.e. the signal proper), attenuated by the transmission of 
the atmosphere for a vertical path 4 = 0, 70x, the radiance 
of solar radiation scattered by the atmosphere directly to the 
sensor, LA, (u stands for upwards), and the radiance re- 
flected by the terrain surface and scattered afterwards by the 
atmosphere to the sensor, Lpuki: 
Liki — LokiTok - LAuk + Lpuki (5) 
Assuming a terrain surface with Lambertian reflectance char- 
acteristics, the reflected radiance is 
1 
Loi ; PEG + Pri (6)
	        
Waiting...

Note to user

Dear user,

In response to current developments in the web technology used by the Goobi viewer, the software no longer supports your browser.

Please use one of the following browsers to display this page correctly.

Thank you.