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

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The dust has a high reflectivity at b<strong>and</strong> 7 but a low reflectivity at b<strong>and</strong> 3 (blue b<strong>and</strong>).<br />

Contrarily, blue b<strong>and</strong> is sensitive to cloud but b<strong>and</strong> 7 is insensitive to cloud. This inverse<br />

spectral feature helps greatly for distinguishing dust <strong>and</strong> cloud. Qu et al. (2006) raised<br />

NDDI to detect dust, with the formula NDDI = (R3 − R7) / (R3 + R7).<br />

The BTD (3.7, 11) is selected to separate dust from surface scenes. Both dust <strong>and</strong><br />

surface scenes have a similar BT at the b<strong>and</strong> 20 (3.7μm) but dust has much lower BT at<br />

the LWIR than surface scenes. Among b<strong>and</strong>s in LWIR, the BTD <strong>of</strong> b<strong>and</strong> 31 (11μm)<br />

relative to b<strong>and</strong> 20 has the largest statistical difference between dust <strong>and</strong> surface scenes.<br />

Moreover, in reflective solar spectrum the relative large reflectance difference<br />

between dust <strong>and</strong> surface scenes (both bright <strong>and</strong> dark surfaces) is found at b<strong>and</strong> 1.<br />

Therefore, the single reflectance <strong>of</strong> b<strong>and</strong> 1 is picked up to differentiate dust from surface<br />

scenes.<br />

Overall, the BTD (12, 11) <strong>and</strong> NDDI are chosen for discriminating dust <strong>and</strong> cloud,<br />

while BTD (3.7, 11) <strong>and</strong> the single reflectance <strong>of</strong> b<strong>and</strong> 1 are chosen for identify dust over<br />

both dark <strong>and</strong> bright surfaces. In each branch, both RSBs <strong>and</strong> TEBs are used.<br />

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