Effects of Charged Martian Dust on Martian Atmosphere Remote Sensing

In this paper, the extinction property and optical depth of charged Martian dust at infrared band 3 THz–300 THz are studied using the Mie scattering theory. It is found that the extinction coefficients of Martian atmospheric dust and the dust optical depth (DOD) of the Martian atmosphere can be ampl...

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Main Authors: Xuebang Gao, Li Xie, Xuqiang Dou, Jun Zhou
Formato: Artigo
Idioma:Inglês
Publicado em: MDPI AG 2022-04-01
Colecção:Remote Sensing
Assuntos:
charged martian dust
Mars atmosphere Remote Sensing
optical depth
extinction coefficient
amplification resonance
extinction reduction
Acesso em linha:https://www.mdpi.com/2072-4292/14/9/2072
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