Dusty Plasma Parameters in Saturn's Magnetosphere.

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Title: Dusty Plasma Parameters in Saturn's Magnetosphere.
Authors: Shokhrin, D. V.1 (AUTHOR), Kopnin, S. I.2 (AUTHOR) kopnin@cosmos.ru, Popel, S. I.2 (AUTHOR)
Source: Plasma Physics Reports. Jun2025, Vol. 51 Issue 6, p732-739. 8p.
Subjects: Dust, Photoelectric effect, Enceladus (Satellite), Electron distribution, Solar radiation, Dusty plasmas
Abstract: The dusty plasma parameters of Saturn's magnetosphere at different distances from the planet have been considered. Particular attention is paid to the parameters in the vicinity of the satellite Enceladus. The influence of the photoelectric effect caused by the interaction of the dust component of the plasma of Saturn's magnetosphere with solar radiation on its parameters is considered. Because of the photoelectric effect, situations are possible when dust particles can acquire a positive charge despite the significant distance from the Sun. Both cases are considered: positive and negative charge of dust particles. The conditions under which dust particles can have a positive charge are determined. The dusty plasma parameters of Saturn's magnetosphere are determined depending on the character of charging of dust particles. A qualitative method for determining situations when dust particles have a positive or negative charge is proposed. [ABSTRACT FROM AUTHOR]
Copyright of Plasma Physics Reports is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: Dusty Plasma Parameters in Saturn's Magnetosphere.
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  Data: <searchLink fieldCode="JN" term="%22Plasma+Physics+Reports%22">Plasma Physics Reports</searchLink>. Jun2025, Vol. 51 Issue 6, p732-739. 8p.
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  Data: <searchLink fieldCode="DE" term="%22Dust%22">Dust</searchLink><br /><searchLink fieldCode="DE" term="%22Photoelectric+effect%22">Photoelectric effect</searchLink><br /><searchLink fieldCode="DE" term="%22Enceladus+%28Satellite%29%22">Enceladus (Satellite)</searchLink><br /><searchLink fieldCode="DE" term="%22Electron+distribution%22">Electron distribution</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+radiation%22">Solar radiation</searchLink><br /><searchLink fieldCode="DE" term="%22Dusty+plasmas%22">Dusty plasmas</searchLink>
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  Data: The dusty plasma parameters of Saturn's magnetosphere at different distances from the planet have been considered. Particular attention is paid to the parameters in the vicinity of the satellite Enceladus. The influence of the photoelectric effect caused by the interaction of the dust component of the plasma of Saturn's magnetosphere with solar radiation on its parameters is considered. Because of the photoelectric effect, situations are possible when dust particles can acquire a positive charge despite the significant distance from the Sun. Both cases are considered: positive and negative charge of dust particles. The conditions under which dust particles can have a positive charge are determined. The dusty plasma parameters of Saturn's magnetosphere are determined depending on the character of charging of dust particles. A qualitative method for determining situations when dust particles have a positive or negative charge is proposed. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of Plasma Physics Reports is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1134/S1063780X25603001
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      – Code: eng
        Text: English
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        StartPage: 732
    Subjects:
      – SubjectFull: Dust
        Type: general
      – SubjectFull: Photoelectric effect
        Type: general
      – SubjectFull: Enceladus (Satellite)
        Type: general
      – SubjectFull: Electron distribution
        Type: general
      – SubjectFull: Solar radiation
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      – SubjectFull: Dusty plasmas
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      – TitleFull: Dusty Plasma Parameters in Saturn's Magnetosphere.
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              M: 06
              Text: Jun2025
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              Y: 2025
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