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Spectral Unmixing Applied to Desert Soils for the - Naval ...

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<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 />

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