A method for estimating the number of regolith particles in a dust cloud in a discharge initiated by gyrotron radiation

The article proposes a new method for estimating the number of particles in experiments on modeling the interaction of cosmic and lunar dust with the surface of spacecraft. The experiments are based on the creation of a dusty plasma cloud, when exposed to radiation from a powerful pulsed gyrotron on a substance simulating cosmic or lunar dust. This approach was tested using a lunar regolith simulator. The dynamics of particles in dust clouds obtained as a result of microwave discharge is analyzed using the ImageJ program.

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Publication Details

Journal
Астрономический журнал
Published
2024-10-08
DOI
https://doi.org/10.31857/s0004629924040053
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00
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article

A method for estimating the number of regolith particles in a dust cloud in a discharge initiated by gyrotron radiation

Д. В. Малахов, В. Д. Степахин, A. S. Sokolov, Т. E. Gayanova et al.
Астрономический журнал
Ionosphere and magnetosphere dynamics
article

A method for estimating the number of regolith particles in a dust cloud in a discharge initiated by gyrotron radiation

Д. В. Малахов, В. Д. Степахин, A. S. Sokolov, Т. E. Gayanova, А. К. Kozak, I. R. Nugaev, D. Е. Kharlachev
article en

Abstract

The article proposes a new method for estimating the number of particles in experiments on modeling the interaction of cosmic and lunar dust with the surface of spacecraft. The experiments are based on the creation of a dusty plasma cloud, when exposed to radiation from a powerful pulsed gyrotron on a substance simulating cosmic or lunar dust. This approach was tested using a lunar regolith simulator. The dynamics of particles in dust clouds obtained as a result of microwave discharge is analyzed using the ImageJ program.

Астрономический журналVol. 101(4)
Prokhorov General Physics Institute (RU)
Openalex Percentile: Top 87%
Ionosphere and magnetosphere dynamics
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