Acta Optica Sinica, Volume. 40, Issue 13, 1329002(2020)
Simulation of Polarized Light Transmission Characteristics in Martian Dust Environment
Fig. 1. Optical properties of Martian dust particles varying with radius at different wavelengths. (a) Asymmetry factor; (b) scattering coefficient; (c) absorption coefficient
Fig. 2. Degree of depolarization of polarized light varying with transmission distance in different-particle-size dust at different wind speeds. (a) reff=2。34 μm, veff=0。86 μm; (b) reff=1。85 μm, veff=0。51 μm
Fig. 3. Polarization parameter of polarized light varying with transmission distance at different particle number concentrations and at different heights. (a) Height is 18 km, and particle number concentration is 1。8×109 m-3; (b) height is 18 km, and particle number concentration is 1。1×109 m-3; (c) height is 22 km, and particle number concentration is 4。0×108 m-3; (d) height is 22 km, and particle number concentration is 2。2×108
Fig. 4. Results under different polarized light. (a) Horizontal component of polarized light varying with transmission distance under light incidence with horizontal polarization;(b) vertical component of polarized light varying with transmission distance under light incidence with horizontal polarization; (c) horizontal component of polarized light varying with transmission distance under light incidence with vertical polarization; (d) vertical component of polarized light varying with transmission dis
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Yufeng Yang, Anli Han, Sichen Lei. Simulation of Polarized Light Transmission Characteristics in Martian Dust Environment[J]. Acta Optica Sinica, 2020, 40(13): 1329002
Category: Scattering
Received: Mar. 6, 2020
Accepted: Apr. 29, 2020
Published Online: Jul. 9, 2020
The Author Email: Yang Yufeng (yangyufeng@xaut.edu.cn), Han Anli (2292325631@qq.com), Lei Sichen (lsc429@163.com)