On Anomalous Dissipation in Plasma of Dusty Mercury’s Exosphere

The anomalous dissipation related to the effect of charging of dust particles that gives rise to new physical phenomena, effects, and mechanisms represents one of the main specific features of dusty plasma that makes it different from conventional plasma containing no charged dust particles. We analyze the process of anomalous dissipation in the context of description of the dynamics of dust particles in dusty plasma of the Mercury’s exosphere. An analytical description of oscillations of a dust particle above the surface of Mercury is presented. The frequency of charging of dust particles that characterizes the anomalous dissipation determines the damping of such oscillations. It is demonstrated that the anomalous dissipation is important for substantiation of the model of levitating dust particles that is used for description of dusty plasma above Mercury. The results of numerical simulations that justify the use of the discussed model are presented.

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Publication Details

Journal
Физика плазмы
Published
2024-10-08
DOI
https://doi.org/10.31857/s0367292124020065
Primary Topic
Dust and Plasma Wave Phenomena
Type
article
Field-Weighted Citation Impact
0.00
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article

On Anomalous Dissipation in Plasma of Dusty Mercury’s Exosphere

Yu. N. Izvekova, S. I. Popel, A. P. Golub’
Физика плазмы
Dust and Plasma Wave Phenomena
article

On Anomalous Dissipation in Plasma of Dusty Mercury’s Exosphere

Yu. N. Izvekova, S. I. Popel, A. P. Golub’
article en

Abstract

The anomalous dissipation related to the effect of charging of dust particles that gives rise to new physical phenomena, effects, and mechanisms represents one of the main specific features of dusty plasma that makes it different from conventional plasma containing no charged dust particles. We analyze the process of anomalous dissipation in the context of description of the dynamics of dust particles in dusty plasma of the Mercury’s exosphere. An analytical description of oscillations of a dust particle above the surface of Mercury is presented. The frequency of charging of dust particles that characterizes the anomalous dissipation determines the damping of such oscillations. It is demonstrated that the anomalous dissipation is important for substantiation of the model of levitating dust particles that is used for description of dusty plasma above Mercury. The results of numerical simulations that justify the use of the discussed model are presented.

Физика плазмыVol. 50(2)
Space Research Institute (RU)
Openalex Percentile: Top 84%
Dust and Plasma Wave Phenomena
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On Anomalous Dissipation in Plasma of Dusty Mercury’s Exosphere — Yu. N. Izvekova, S. I. Popel, et al. · Физика плазмы (2024) | TGRS Research Map | TGRS