Full text: Proceedings, XXth congress (Part 7)

International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV, Part B7. Istanbul 2004 
A comparison between the classifications indicated that they 
were significantly different. A Z statistic of 3.7 (Hyperion 
and RDACS-3) and a Z statistic of 4.5 ((Hyperion and 
AVIRIS) were computed for the pairwise comparisons. 
Because the Z statistic values were greater than 1.96, there 
were significant differences in the results of the classifications 
of the sensors. 
  
   
   
  
  
Rufledanse 
X 
== 
  
  
  
  
  
  
  
Mange TEE 
Figure 9. Spectra of black willow; healthy and under stress 
(the scale is between 0 and 1 (100%) for the reflectance axis) 
6. CONCLUSIONS 
Airborne and spaceborne hyperspectral imagery is becoming 
increasingly accessible due to the increasing number of 
companies and agencies operating hyperspectral scanners. 
Airborne data acquisitions benefit greatly over satellite based 
missions because the user has influence on the mission in 
terms of time schedules, flight line arrangements, calibration 
measurements, spectral/spatial resolutions, and acceptable 
weather conditions. However, airborne hyperspectral 
  
Figure 7. Classification map of the Hyperion dataset 
sensors are often very expensive due to fact that limited 
spatial coverage and multiple flight lines may be required to 
cover a study area. Also, data processing is usually complex 
and can cause problems. 
Another objective of this research was to outline forested 
areas that were under stress due to a drought. Figure 9 shows 
the spectra of black willow leaves; healthy (cyan, green and 
red lines), moderately stressed (blue) and severely stressed 
(black). Another objective was to map the water quality in 
the lakes using the hyperspectral data (Figure 10). However, 
because of the page limitations, these studies were not 
Airborne hyperspectral sensors are usually used to test 
spaceborne hyperspectral sensors, which provide continuous 
MR coverage of most of our planet as well planetary surfaces. 
included in this paper. 
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