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