Full text: Technical Commission VIII (B8)

2. DATA AND METHODS 
A WV-2 image from March 21* was used in this study (figure 
1). The image was pre-processed and atmospherically 
corrected. Field reflectance measurements in the study area 
coincident with the satellite image acquisition, contributed to 
the validation of the atmospheric correction. 
  
Figure 1. True color combination of WV2 image for the study 
area, and description of the three main vegetation covers 
present. 
2.1 Spectral libraries 
Two sets of spectra were collected for different species. 
2.1.1 From pure image pixels: The first field dataset was 
a compilation of GPS locations where species were identified. 
The WV2 spectral signatures from the purest pixels were used 
later as endmembers in MESMA: the species registered were 
M. faya (12), L. novocanariensis (6) and Pinus radiata (15), 
and spectral signatures for herbaceous species and fern (19) in 
degraded areas were also collected. 
2.1.2 From field measurements: The second set was 
obtained from ASD FieldSpec 3 JR reflectance measurements 
in stands of M. faya, L. novocanariensis and E. arborea. A 
total of 69 spectral signatures were collected during a 4-day 
field campaign, including the day of the WV2 pass (March 
14*, 15". 20^ and 21%). 
International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Volume XXXIX-B8, 2012 
XXII ISPRS Congress, 25 August — 01 September 2012, Melbourne, Australia 
  
  
ASD field WV2 pure Empirical 
Wavelength | signature for | pixels signature calibration 
(nm) M. faya for M. faya ASD > WV2 
427 0.0111 0.0037 -0.0074 
478 0.0137 0.0157 0.0019 
546 0.0302 0.0299 -0.0003 
608 0.0267 0.0296 0.0029 
659 0.0214 0.0243 0.0029 
724 0.1630 0.1368 -0.0262 
831 0.3153 0.2573 -0.0580 
908 0.3454 0.2669 -0.0786 
  
  
  
  
  
  
Table 1. Empirical calibration parameters resulting from the 
comparison between M. faya field and WV2 image samples. 
—ADiield TESAIMpled ese 
spectral signatures 
(E. arborea) 
Reflectance 
  
  
  
427 478 546 608 659 724 831 908 
Wavelength (nm) 
eee E. arborea flowered = = E. arborea flowered (average) 
-" E arborea green E. arborea green (average) 
0.4 o WM 2-callibrated té tr I ta ERE 
spectral signatures 
0.3 - 
Reflectance 
  
  
  
  
427 478 546 608 659 724 831 908 
Wavelength (nm) 
E. arborea flowered == == [ arborea flowered (average) 
E. arborea green 
  
E. arborea green (average) 
Figure 2. Empirical calibration of field spectra from Erica 
arborea measurements for endmember extraction in WV2 
image. Two patterns noticeable between different phenological 
stages. 
2.1.3 From re-calibrated field measurements: Given its 
less defined crowns compared to other species, it was difficult 
to identify pure image pixels for E. arborea, only with ASD 
measurements available. This was solved empirically by 
comparing ASD and WV2 spectra in other species where both 
data sets were available, and then obtaining a conversion 
coefficient to each band (table 1). These coefficients were 
added to E. arborea ASD spectra as a calibration method to 
obtain WV2-adjusted spectra (figure 2). 
2.2 Forest mapping 
First, a NDVI threshold (Rouse et al., 1973)) was used to mask 
out all non-vegetation areas in the study area. Only pixels with 
NDVI > 0.5 were included in MESMA. Two unmixing cycles 
were applied. In the first cycle (mesmal), three endmember 
libraries were used: M. faya + L. novocanariensis -because of 
their spectral and ecological similarity they were fused 
together-, E. arborea and herbaceous/fern. 
For the second MESMA (mesma2) cycle only the pixels with a 
sub-pixel cover fraction estimate above 80% of M. faya + L. 
novocanariensis were analyzed. This second cycle allowed us 
to differentiate between the main dominant tree species in the 
area: M. faya, L. novocanariensis and P. radiata. 
  
  
    
  
  
  
  
  
   
    
   
   
   
    
  
  
   
  
  
   
   
   
   
  
  
   
   
    
   
   
  
   
  
   
  
  
  
   
    
   
   
  
  
  
   
  
   
  
   
  
  
    
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