Object: SMPR Conference 2013

   
  
   
  
   
   
   
   
    
   
   
  
  
   
  
  
  
Table 1 Specifications of IKONOS satellite and MS imaging 
system 
Specifications value 
Speed on Orbit 7.5 kilometers (4.7 
miles) per second 
Orbit 98.1 degree, sun 
synchronous 
Altitude 681 kilometers (423 
miles) 
Over 8.5 Years 
10:30 a.m., local solar 
time 
3 days at 60 elevation 
11 days at 72 elevation 
141 days at 89 
Operational Life 
Descending node time 
Revisit time at mid-latitude 
  
  
  
  
   
  
  
   
   
   
  
   
    
   
  
  
   
   
   
  
  
   
   
   
  
  
  
  
elevation 
Optical telescope assembly 
Assembly mass without the 109 kg 
focal plane unit 
Total instrument mass 171 kg 
Primary mirror aperture 0.70 m 
Diameter 
Focal length om 
Focal ratio 8 14 ; 
pixels 
Detector array 48x48um 
pixel size 4 m (3.2 mat nadir) 
Spatial resolution 
Spectral range (um) 0.45-0.53, (blue) 
0.52-0.61, (green) 
0.64-0.72, (red) 
0.76-0.86, (NIR) 
ADPCM, 2.5 bits/pixel 
Data compression technique j 
11 bits 
Data quantization 
  
  
  
   
  
  
   
   
    
   
   
     
2. DARK OBJECT 
Among the common atmospheric correction methods, Dark 
Object Subtraction (DOS) is a simple and yet useful one to 
eliminate the effect of the atmosphere from images, especially 
when limited ground information is available (Gebreslasie, 
2009). To obtain the dark object, IKONOS should seek zero 
reflectance surface covers. In order to achieve zero reflectance 
pixels in the green and blue bands, tree shades, and in the red 
and infrared bands, water body can provide the dark object. 
Also, to avoid the effects of MTFC, the MTFC-off images 
should be selected (Pagnutti, 2003). 
The smallest value in each band of the image with a cover of 
forests and water bodies represents the DN value of dark object 
(Soudani, 2006), (Mahiny, 2007). It is often preferred this 
approach to radiative transfer model for eliminating the effect of 
atmosphere. That is because in the radiative transfer model, 
measuring the water vapor in the air along with the aerosols as 
well as describing atmospheric conditions along with collecting 
earth data is difficult. Nonetheless, from a practical standpoint, 
the smallest amount of DN may also contain errors. That is 
because selection of the dark object value is based on a visual 
examination from the histogram values. Another error in dark 
object values as used for atmosphere correction —which is 
discussed in this article - is the sensor noise. Despite these 
errors, dark object subtraction technique has always been a good 
correction for the atmospheric effect on remote sensing data 
(Soudani, 2006). 
The IKONOS image used in this work is an MS one from Quds 
town near Tehran. One of the main reasons for having chosen 
this region is that the image has both forests and water bodies. 
In Figure l, these scenes are shown in two bands of near 
infrared and green. Taking a look at the images, one can realize 
that, for example, the body of water in the infrared band and 
shade of dense trees in the green band seem dark. The smallest 
amount of image pixels in each band is calculated with ENVI 
software and shown in Table 2. The small value of infrared 
compared to other bands represents a low path radiation and the 
high transmittance of atmosphere through the band (Richter, 
2006). 
3. CCD NOISE MEASUREMENT 
The imaging system CCD can usually be demonstrated by three 
sub-systems. First, the CCD arrays convert photons within each 
pixel into electrons and voltage. Second, the electronic part of 
the camera performs a non-linear compression of the voltage 
values. Finally, the third sub-system is the analog to digital 
converter that generates digital image. During the process of 
converting radiation to digital image, various electronic noises 
enter into the system. In this paper, we investigate three noises, 
i.e. dark current noise, non-uniform pixel noise and Read noise, 
the first two of which are from CCD array noises and the last 
one is from CCD read circuit noises. 
Image obtained from the dark object (Epos) includes electronic 
sensor noise in addition to atmosphere effect (E44). The three 
noises can be modeled as a theoretical relation as follows: 
  
Figure 1. Separating image into green and infrared bands: the right image represents a body of water in the 
near infrared band and the left one shows trees in the red band. 
     
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