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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2018, Volume 108, Issue 6, Pages 379–387
DOI: https://doi.org/10.1134/S0370274X18180030 (Mi jetpl5696) 		 
This article is cited in 15 scientific papers (total in 15 papers)

ASTROPHYSICS AND COSMOLOGY

Formation of dusty plasma clouds at meteoroid impact on the surface of the Moon

S. I. Popelab, A. P. Golub'a, A. V. Zakharova, L. M. Zelenyica, A. A. Berezhnoyd, E. S. Zubkoe, M. Itenf, R. Lenag, S. Sposettih, Yu. I. Velikodskyi, A. A. Tereshchenkoi, B. Atamaniukj

a Space Research Institute, Russian Academy of Sciences, Moscow, Russia
b National Research University Higher School of Economics, Moscow, Russia
c Moscow Institute of Physics and Technology (State University), Dolgoprudnyi, Moscow region, Russia
d Sternberg Astronomical Institute, Moscow State University, Moscow, Russia
e Far Eastern Federal University, Vladivostok, Russia
f Garden Observatory, Gordola, Switzerland
g Geologic Lunar Research (GLR) Group, Rome, Italy
h Gnosca Observatory, Gnosca, Switzerland
i National Aviation University, Kyiv, Ukraine
j Space Research Centre, Polish Academy of Sciences, Warsaw, Poland
Full-text PDF (729 kB) Citations (15)
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DOI: https://doi.org/10.1134/S0370274X18180030
Abstract: The nature of two dusty plasma clouds appearing because of the impact of a meteoroid on the surface of the Moon has been discussed. It has been shown that one of the clouds is formed by particles (or fragments) of regolith ejected into free space by a shock wave induced by the meteoroid impact on the surface of the Moon and the second cloud is formed by solidified melt droplets. The main characteristics of these clouds, including the cloud expansion rates, the characteristic sizes of particles in both clouds, and the concentrations and charges of particles, have been calculated. The calculated cloud expansion rates are in qualitative agreement with the observational data.
Funding agency Grant number
Russian Science Foundation 17-12-01458
Received: 06.08.2018
Revised: 17.08.2018
English version:
Journal of Experimental and Theoretical Physics Letters, 2018, Volume 108, Issue 6, Pages 356–363
DOI: https://doi.org/10.1134/S0021364018180091
Bibliographic databases:
Document Type: Article
Language: Russian
Citation: S. I. Popel, A. P. Golub', A. V. Zakharov, L. M. Zelenyi, A. A. Berezhnoy, E. S. Zubko, M. Iten, R. Lena, S. Sposetti, Yu. I. Velikodsky, A. A. Tereshchenko, B. Atamaniuk, “Formation of dusty plasma clouds at meteoroid impact on the surface of the Moon”, Pis'ma v Zh. Èksper. Teoret. Fiz., 108:6 (2018), 379–387; JETP Letters, 108:6 (2018), 356–363
Citation in format AMSBIB
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    • This publication is cited in the following 15 articles:
    Citing articles in Google Scholar: Russian citations, English citations
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