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i Detection of Smoke and Dust Aerosols Using Multi-sensor Satellite ...

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Sun <strong>Satellite</strong><br />

Figure 3.2: Basic radiative transfer model<br />

Based on the fundamental radiative transfer model (Liou, 2002; Li et al., 2001), the<br />

reflectance at TOA viewed from a satellite can be expressed as in Eq. 3.1.<br />

r( ; , ; , ) t( ; ) r ( ; , ; , ) t(<br />

; )<br />

0 0 0 s 0 0<br />

rs<br />

rg<br />

<br />

r ( ; , ) <br />

<br />

t t t<br />

<br />

g 0 0 *<br />

( ; 0 )exp exp ( ; , ) ( ; )<br />

* s <br />

0 1 rs ( ) rg<br />

( ) <br />

r ( ) <br />

<br />

t t t t<br />

<br />

g<br />

*<br />

( ; 0 ) s ( ; 0, 0 ) exp ( ; , ) ( ; )<br />

* s <br />

1 rs ( ) rg<br />

( ) <br />

22<br />

<strong>Smoke</strong> (dust)<br />

Ground<br />

(3.1)<br />

where λ is the wavelength <strong>and</strong> τ is optical depth <strong>of</strong> smoke layer. Two parameters, μo <strong>and</strong><br />

μ are the cosine <strong>of</strong> the solar zenith angle <strong>and</strong> view angle. t (λ, μo) is the transmittance<br />

from the top <strong>of</strong> atmosphere to smoke <strong>and</strong> t (λ, μ) is the transmittance in inverse direction<br />

in the view direction <strong>of</strong> satellite. Two azimuth angles, фo <strong>and</strong> ф, are viewed from sun <strong>and</strong><br />

satellite, respectively. In Eq. 3.1, the notation asterisks indicate that these quantities are

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