On the Kinetic Features of Sedimentation of Dust Particles in the Martian Atmosphere

A. Yu. Dubinsky; Дубинский А. Ю.; Yu. S. Reznichenkob; Резниченко Ю. С.; S. I. Popel; Попель С. И.

doi:10.31857/S0320930X23020019

On the Kinetic Features of Sedimentation of Dust Particles in the Martian Atmosphere

Authors: Dubinsky A.Y.¹, Reznichenkob Y.S.², Popel S.I.¹
Affiliations:
1. Space Research Institute, Russian Academy of Sciences, Moscow, Russia
2. Moscow Institute of Physics and Technology (National Research University), Dolgoprudny, Russia
Issue: Vol 57, No 3 (2023)
Pages: 225-231
Section: Articles
URL: https://journals.rcsi.science/0320-930X/article/view/134963
DOI: https://doi.org/10.31857/S0320930X23020019
EDN: https://elibrary.ru/NVINSD
ID: 134963

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Abstract
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Abstract

The mode of subsidence of layered structures in the ionosphere of Mars has been studied taking into account the compositional features of the Martian atmosphere. The characteristic sedimentation rates of dust particles, their sizes and charges, as well as the sedimentation time of layered structures are calculated. The results obtained can be used in the study of atmospheric phenomena on Mars in the course of upcoming space missions.

Keywords

future space missions, Earth, Mars, dust particles, dusty plasma, sedimentation of layered structures

About the authors

A. Yu. Dubinsky

Space Research Institute, Russian Academy of Sciences, Moscow, Russia

Email: nfkpb@bk.ru
Россия, Москва

Yu. S. Reznichenkob

Moscow Institute of Physics and Technology (National Research University), Dolgoprudny, Russia

Email: popel@iki.rssi.ru
Россия, Долгопрудный

S. I. Popel

Space Research Institute, Russian Academy of Sciences, Moscow, Russia

Author for correspondence.
Email: popel@iki.rssi.ru
Россия, Москва

References

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