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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...

Ausführliche Beschreibung

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Bibliografische Detailangaben
Hauptverfasser: Xuebang Gao, Li Xie, Xuqiang Dou, Jun Zhou
Format: Artigo
Sprache:Inglês
Veröffentlicht: MDPI AG 2022-04-01
Schriftenreihe:Remote Sensing
Schlagworte:
Online-Zugang:https://www.mdpi.com/2072-4292/14/9/2072
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