Full text: Technical Commission VII (B7)

kaolinite--smectite (HyMAP channels 6, 81, 108 and 119). We 
also defined diagnostic bands following the same criteria for a 
group of Fe minerals such as goethite, hematite and jarosite 
(HyMAP channels 4, 32, 62 and 103) and montmorillonite 
(HyMAP channels 4, 25, 81 and 94). 
  
(a) 
Figure 2. Colour composite of abundance for minerals (Alu- 
cyan, Illi-yelow, Kaol-purpel, Kaol+Sme-purpel2, Mont- 
maroon) from HyMAP image (a), from MASTER image (b), 
and thermal index THI (red-violet) between 10.16 um and 
12.21 um from MASTER image (c). 
Differents PCAs for each mineral in the image MASTER case 
have been carried out using the following channels: MASTER 
channels 4, 8, 21 and 24 for alunite; MASTER channels 4, 8, 21 
and 22 for illite; MASTER channels 4, 13 22 and 24 for 
kaolinite. 
The results obtained for HyMap and MASTER have been 
classified by K-Means algorithm. We calculated confusion 
matrices using field sampling considered as true value. An 
overlap accuracy of 82.5696 and Kappa coefficient of 0.75 have 
been obtained for HyMAP image. An overlap of accuracy of 
75.11% and Kappa coefficient of 0.69 have been obtained in the 
MASTER case. 
The results are strongly influenced by vegetation cover, which 
acts as an input error of reflectance in the computing of new 
variables or Principal Components (PCs). Nevertheless, we 
observe the scarce presence of materials of clay-phyllic 
alteration, contrasting with the abundance of iron oxide 
components. 
4.2 Spectral anomaly detection 
A RX algorithm (Reed and Xaoli, 1996), widely accepted as a 
standard spectral anomaly detection, has been applied to all set 
of data. 
Anomalies obtained for RX have been verified by those 
computed using a method based on projection pursuit (Malpica 
et al., 2008). The computation in both methods has been carried 
out separately for spectral ranges of reflective channels and 
emissive. MASTER thermal channels fused with aerial 
International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Volume XXXIX-B7, 2012 
XXII ISPRS Congress, 25 August — 01 September 2012, Melbourne, Australia 
   
   
   
   
  
  
  
  
   
   
  
  
  
  
  
  
   
    
   
   
  
  
   
   
   
   
   
  
   
   
   
  
  
  
  
   
   
   
  
  
  
   
photography at 2.5 m have been used to calculate thermal 
anomalies with the intention on improve the classes separability 
maintaining the raw spectral information acquired (Rejas ef al, 
2007). Eight new variables were obtained from MASTER 
channels 42 to 49. Variable number six was spatially projected 
and we realized that is was related to high humidity values, and 
it fitted a wide and well delimited area Northwest from 
Turrialba. 
We carried out pattern recognition analysis. For MASTER and 
ASTER images we calculated a thermal index (Rejas ef al, 
2009), profiting from the separability between covers in the 
emissive spectrum of both sensors. We generated image 
convolutions using a median filter, that were used afterwards to 
make a ratio between 10.16 um y 12.21 um wavelengths, 
weighted corrected by ratio between each channel gain. We 
established thresholds on the resultant variable for highlighting 
detected pixels as possible anomalies. 
conv (5 els )- conv un )l 3) 
THI. = 
0.24 [conv C = conv (Fe J 
  
where conv — image convolution median filter. 
L m radiance at sensor for wavelength. 
4.3 Results and Discusion 
The relationship between spectral anomalies and hydrothermal 
alterations, obtained in previous paragraphs, has been studied. 
In order to do that, it has been linearly adjusted, a sample space 
of 35 pairs of points, placing spectral anomalies in the Y axis 
and altered minerals in the X axis. All regressions have been 
calculated at a confidence level of 9596, removing in each 
adjustment, the sample values that showed unusual residues and 
which correspond mainly with clouds and shadows. The results 
obtained are summarized in Tables 1 and 2. 
HyMAP RX all chs 7 1101,61 * 9,86744*HA Alunite 
  
  
600 - 
Bu . R^ 2072 
E = t 
o Eo = 
$40- ^. 
© [2 o" a 
© 300 - . 
a. k s m 
< L = ><a 
= 200 . E. 
Fa 
T E ey EM 
L un 5 o "ua 
100 H s 
0 " L 1 1 1 L 1 rd i i Lt; = 
-190 -90 10 110 
AH Alunite 
Figure 3. Example of relationship between spectral anomalies 
RX and Alunite, from HyMAP images. 
  
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Models HyMAP P-value |Correlation |R* 
RX = 1101,61 + 9,86744*Alunite |0.0001 0.850365 72.31% 
RX = -1528,05 - 1,92404*IIlite 0.0379 |-0.554625 |30.76% 
RX = -611,046 + 1,03826*Kaolinite 10.0515 |0.511091 26.12% 
RX = 739,318 - 7,59725*Kaol+Sme |0.0182 |-0.599314 35.92% 
RX = 834,65 + 3,50578*Fe minerals |0.0153 |0.611924 37.45% 
RX- -796,88 - 1,47957*Montmoroll | 0.0851 |-0.45922 21.09% 
  
Table 1. 
Comparison of relationships between spectral 
anomalies and hydrothermal alteration, from HyMAP images. 
   
  
  
  
   
  
  
   
       
 
	        
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