Spectral Unmixing Applied to Desert Soils for the - Naval ...
Spectral Unmixing Applied to Desert Soils for the - Naval ...
Spectral Unmixing Applied to Desert Soils for the - Naval ...
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
<strong>the</strong> Mazourka Canyon OHV park between Owens Valley and Death Valley at <strong>the</strong> base of<br />
<strong>the</strong> Inyo Mountains, <strong>the</strong> approximate coordinates <strong>for</strong> this site are 36 0 49’ 18”N, 118 0 05’<br />
17”W. A collection of spectra were also taken from <strong>the</strong> Santa Cruz mountains at<br />
approximately 37 0 07' 26.55"N, 122 0 00' 42.22"W <strong>for</strong> analysis of how soil reflectance<br />
changes with <strong>the</strong> same material under different disturbance conditions.<br />
B. METHODS<br />
1. Atmospheric Correction<br />
Atmospheric correction must be per<strong>for</strong>med on <strong>the</strong> AVIRIS data <strong>to</strong> remove <strong>the</strong><br />
effects of atmospheric absorption and scattering in order <strong>to</strong> obtain <strong>the</strong> surface reflectance<br />
of a material <strong>for</strong> comparison <strong>to</strong> library spectra (Figure 16). Atmospheric corrections are<br />
applied on a pixel by pixel basis in order <strong>to</strong> analyze reflectance <strong>for</strong> materials in specific<br />
regions of <strong>the</strong> imagery. AVIRIS data were atmospherically corrected using <strong>the</strong> Fast<br />
Line-of-sight Atmospheric Analysis of <strong>Spectral</strong> Hypercubes (FLAASH) method.<br />
Figure 16. In this figure from Birvio et al. (2001) <strong>the</strong> solar radiation interactions are<br />
illustrated. E0 is solar irradiance at <strong>the</strong> <strong>to</strong>p of <strong>the</strong> atmosphere, Ed is diffuse<br />
solar irradiance. Ls represents radiance emitted from <strong>the</strong> target, Ld is <strong>the</strong><br />
atmospheric path radiance and L0 is radiance measured by <strong>the</strong> sensor. θz and<br />
θv are downward and upward transmittance from <strong>the</strong> atmosphere,<br />
respectively, and θz and θv represent <strong>the</strong> solar zenith and sensor viewing<br />
zenith angles, respectively.<br />
34