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Pisma v Zhurnal Tekhnicheskoi Fiziki, 2020 Volume 46, Issue 16, Pages 32–34 (Mi pjtf5020)

This article is cited in 3 papers

Fluxes of dust particles in the Martian system

S. I. Popel, A. P. Golub', G. G. Dol'nikov, A. V. Zakharov, A. A. Kartasheva

Space Research Institute, Russian Academy of Sciences, Moscow

Abstract: Fluxes of mass and dust particles are calculated, which appear in orbit around Mars due to collisions of meteoroids with Phobos and Deimos. Size distributions of dust particles captured in orbit around Mars are determined. Knowledge of parameters of these particles is important when planning the experimental studies on dust in the system of Mars within the framework of the future space missions.

Keywords: future space missions, Mars, Phobos, Deimos, dust particles, dusty plasmas, piezoelectric impact sensor, charge-sensitive grid.

Received: 25.02.2020
Revised: 25.02.2020
Accepted: 18.05.2020

DOI: 10.21883/PJTF.2020.16.49851.18264


 English version:
Technical Physics Letters, 2020, 46:8, 812–814

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© Steklov Math. Inst. of RAS, 2024