Abstract We outline an analytical method for studying the motion of charged dust particles that orbit an oblate planet having a tilted, offset, dipolar magnetic field. Our computed trajectories closely mimic previous numerical results; equilibrium dust potentials must be less then 10 volts or the Jovian ring would be thicker than observed. We identify several Lorentz resonances , where the periods of components of the Lorentz force, as seen by a reference particle moving in the equatorial plane, match the particle's orbital period; several seem to be near observed features of the Jovian ring system.


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    Titel :

    Dust motion in Jupiter's tilted magnetic field


    Beteiligte:
    Schaffer, L. (Autor:in) / Burns, J.A. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.01.1984


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



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