NONLINEAR PERIODIC DUST ACOUSTIC WAVES IN THE MAGNETOSPHERE OF SATURN

A characteristic feature of the magnetosphere of Saturn is the presence of two types of electrons, hot and cold ones, which obey kappa distributions. Electrons, magnetospheric ions, and dust particles, which have been discovered within the Cassini mission, form a dusty plasma system in the magnetosphere of Saturn. Nonlinear periodic dust acoustic waves of arbitrary amplitude, which can propagate in the dusty magnetosphere of Saturn, are considered. The obtained results are important for the interpretation of future space observations.

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Publication Details

Journal
Физика плазмы / Plasma Physics Reports
Published
2025-01-01
DOI
https://doi.org/10.7868/s3034637125010094
Primary Topic
Astro and Planetary Science
Type
article
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article

NONLINEAR PERIODIC DUST ACOUSTIC WAVES IN THE MAGNETOSPHERE OF SATURN

Yulia Izvekova
Физика плазмы / Plasma Physics Reports
Astro and Planetary Science
article

NONLINEAR PERIODIC DUST ACOUSTIC WAVES IN THE MAGNETOSPHERE OF SATURN

Yulia Izvekova
article en

Abstract

A characteristic feature of the magnetosphere of Saturn is the presence of two types of electrons, hot and cold ones, which obey kappa distributions. Electrons, magnetospheric ions, and dust particles, which have been discovered within the Cassini mission, form a dusty plasma system in the magnetosphere of Saturn. Nonlinear periodic dust acoustic waves of arbitrary amplitude, which can propagate in the dusty magnetosphere of Saturn, are considered. The obtained results are important for the interpretation of future space observations.

Физика плазмы / Plasma Physics ReportsVol. 51(1)
Openalex Percentile: Top 80%
Astro and Planetary Science
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NONLINEAR PERIODIC DUST ACOUSTIC WAVES IN THE MAGNETOSPHERE OF SATURN — Yulia Izvekova · Физика плазмы / Plasma Physics Reports (2025) | TGRS Research Map | TGRS