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

被引：1

作者：

Dubinsky, A. Yu. ^{[1
]}

Reznichenko, Yu. S. ^{[2
]}

Popel, S. I. ^{[1
]}

机构：

[1] Russian Acad Sci, Space Res Inst, Moscow, Russia

[2] Natl Res Univ, Moscow Inst Phys & Technol, Dolgoprudnyi, Russia

来源：

SOLAR SYSTEM RESEARCH | 2023年 / 57卷 / 03期

关键词：

future space missions; Earth; Mars; dust particles; dusty plasma; sedimentation of layered structures; NOCTILUCENT CLOUDS; PLASMA STRUCTURES; ICE CLOUDS; WATER; MARS; MESOSPHERE; EVOLUTION;

D O I：

10.1134/S0038094623020016

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

-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.

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页码：214 / 220

页数：7

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