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  • American Geophysical Union (AGU)  (2)
  • 1980-1984  (2)
Medientyp
Verlag/Herausgeber
  • American Geophysical Union (AGU)  (2)
Person/Organisation
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Erscheinungszeitraum
  • 1980-1984  (2)
Jahr
  • 1
    Online-Ressource
    Online-Ressource
    American Geophysical Union (AGU) ; 1983
    In:  Journal of Geophysical Research: Space Physics Vol. 88, No. A7 ( 1983-07), p. 5573-5579
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 88, No. A7 ( 1983-07), p. 5573-5579
    Kurzfassung: Saturn's broad E ring, the narrow G ring, and the structured and apparently time‐variable F ring(s) contain many micron and submicron‐sized particles, which make up the ‘visible’ component. These rings (or ring systems) are in direct contact with magnetospheric plasma. Fluctuations in the plasma density and/or mean energy, due to magnetospheric and solar wind processes, may induce stochastic charge variations on the dust particles, which in turn lead to an orbit perturbation and spatial diffusion. In addition, Coulomb drag forces may be important, in particular for the E ring. The possibility that electromagnetic effects may play a role in determining the F ring structure, and its possible time variations, is critically examined. Sputtering of micron‐sized dust particles in the E ring by magnetospheric ions yields lifetimes of 10² to 10 4 years. This effect as well as the plasma induced transport processes require an active source for the E ring, probably Enceladus.
    Materialart: Online-Ressource
    ISSN: 0148-0227
    Sprache: Englisch
    Verlag: American Geophysical Union (AGU)
    Publikationsdatum: 1983
    ZDB Id: 2033040-6
    ZDB Id: 3094104-0
    ZDB Id: 2130824-X
    ZDB Id: 2016813-5
    ZDB Id: 2016810-X
    ZDB Id: 2403298-0
    ZDB Id: 2016800-7
    ZDB Id: 161666-3
    ZDB Id: 161667-5
    ZDB Id: 2969341-X
    ZDB Id: 161665-1
    ZDB Id: 3094268-8
    ZDB Id: 710256-2
    ZDB Id: 2016804-4
    ZDB Id: 3094181-7
    ZDB Id: 3094219-6
    ZDB Id: 3094167-2
    ZDB Id: 2220777-6
    ZDB Id: 3094197-0
    SSG: 16,13
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
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  • 2
    Online-Ressource
    Online-Ressource
    American Geophysical Union (AGU) ; 1980
    In:  Geophysical Research Letters Vol. 7, No. 5 ( 1980-05), p. 305-308
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 7, No. 5 ( 1980-05), p. 305-308
    Kurzfassung: We have investigated the possibility of removing particles from Io by interactions with the Jovian magnetosphere. We find that dust grains of about 0.1 µm radius will rapidly become charged if exposed to the ambient Jovian plasma. For particles this size in Io's volcanic plumes, the Lorentz force can overcome Io's gravity and these particles can escape. Escaping dust will be controlled by the topology of the magnetosphere and we suggest that Io derived dust may be an important source of erosive impacts on large Jovian ring particles and destructive collisions with small particles. The ring particles themselves will interact with the Jovian plasma and we suggest that coulomb scattering of plasma particles by charged dust grains may produce a plasma gap or void in the vicinity of the rings.
    Materialart: Online-Ressource
    ISSN: 0094-8276 , 1944-8007
    Sprache: Englisch
    Verlag: American Geophysical Union (AGU)
    Publikationsdatum: 1980
    ZDB Id: 2021599-X
    ZDB Id: 7403-2
    SSG: 16,13
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
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