Full text: Proceedings, XXth congress (Part 8)

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International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV, Part B-YF. Istanbul 2004 
  
  
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0,6 
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Coefficient of determination 
  
  
  
12 13 17 20 21 22 23 24 25:26 27 28 29 31 
  
  
  
Figure 3: Coefficient of determination for the different 
aggregated land cover classes (left column- VIS, 
right column= NIR) 
In order to investigate the regression quality of either NOAA 15 
and NOAA 16 sampling data, corresponding data sets were 
separately introduced into the MIB. Mean values of the 
obtained statistical parameters for all classes and channels are 
displayed in table 2 and are compared between those obtained 
by running the MIB with the combined sampling data set. 
  
  
  
  
Observations from Channel Avg R° Avg se 
NOAA 15 VIS 0.804 0.015 
NIR 0.814 0.019 
NOAA 16 VIS 0.870 0.016 
NIR 0.838 0.020 
NOAA 15 & 16 VIS 0.792 0.018 
NIR 0.830 0.023 
  
  
  
  
Table 2: Statistical results for model inversion for different 
input data sets 
The input data sampling set that combines NOAA 15 and 
NOAA 16 observations was also introduced into the MIB in 
order to compare the performance with the Roujean and the 
Modified Walthall model. Table 3 displays the corresponding 
results. The NTAM yields best values for the coefficient of 
determination, especially in the VIS channel. However, this is 
not too surprising as neither the Roujean model nor the MWM 
were designed to cope with sample data encompassing the 
entire growing season. 
  
  
  
  
  
  
Model Channel Avg R* Avg se 
Roujean VIS 0.545 0.016 
NIR 0.720 0.025 
Modified Walthall VIS 0.535 0.016 
NIR 0.721 0.024 
NTAM VIS 0.792 0.018 
NIR 0.830 0.023 
  
  
Table 3: Statistical results for model inversion for the three 
different models 
Another very interesting extension from the determination of 
the correction parameters consists in a graphical visualization of 
modelled reflectances for different sun sensor target geometries 
(Sandmeier & Itten 1999, Dymond et al. 2001). Again, the land 
cover class 17 (olive grows) is chosen for such a visualization. 
As NTAM modelled reflectances depend on values for the 
proxies 05, a criterion had to be established that allows to 
display modelled reflectances for land cover typical ot values: 
First, the mean à; value of the input sampling data was 
calculated for the two channels. Then, the corresponding 
standard deviation values were added and subtracted from the 
mean o; values. The figures 4 to 7 show modelled reflectances 
for the VIS and the NIR. The raa is the relative azimuth angle, 
the vza the view zenith angle and the sza is the sun zenith angle. 
The sza is set to the fixed value of 45 degrees in all graphics. 
Note that no input data with a vza » 45? are introduced. 
Modelling to a vza of 52.5? is done to demonstrate model 
behaviour outside the range of calibration. The displayed 
graphics allow to estimate seasonal and angular dependency of 
the BRDF on different land covers. The hot spot is clearly 
distinguishable in all graphics. 
  
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0.30 
0.27 
0.24 
0.21 
0.18 
0.15 
0.12 
0.09 
0.06 
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0.00 
  
Figure 4: Modelled VIS reflectance for olive grows where 
NDVI = NDVI ein - NDVldev 
  
raa 
C pup Sw S 
i CUNAG quot 
ye 588° 
Figure 5: Modelled VIS reflectance for olive grows where 
NDVI = NDVIean zh NDVI dev 
43 
 
	        
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