Abstract A radial profile of the plasma mass distribution in Jupiter’s magnetosphere in the region beyond Io’s orbit up to ∼15 Jupiter radii RJ constructed according to the results of measurements on the Voyager 1 and Galileo spacecraft is used to determine the radial dependence and radial diffusion coefficient DLL. The initial profile is approximated by a function decreasing as L−5 ± 1. For this radial mass distribution, radial ion diffusion outside of Io’s orbit caused by centrifugal forces is possible. An estimate of (1.2–6.7)$ 10^{−11} $L6 ± 1 for DLL was obtained.


    Access

    Access via TIB

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    An analytical estimate of the coefficient for radial charged particle diffusion in Jupiter’s magnetosphere using plasma radial distribution


    Contributors:

    Published in:

    Publication date :

    2015




    Type of media :

    Article (Journal)


    Type of material :

    Print


    Language :

    English



    Classification :

    BKL:    55.60 Raumfahrttechnik / 39.00 Astronomie: Allgemeines / 50.93 Weltraumforschung
    Local classification TIB:    770/3520/8000




    ULF wave observations in Jupiter's magnetosphere

    Petkaki, Panagiota | Online Contents | 2001


    Corotation of Jupiter's Three-Dimensional Magnetosphere

    Hawkins, S. E. / Cheng, A. F. / Lanzerotti, L. J. et al. | British Library Conference Proceedings | 1995


    ULF Wave Observations in Jupiter's Magnetosphere

    Petkaki, P. / Dougherty, M. K. / International Council of Scientific Unions | British Library Conference Proceedings | 2001


    Corotation of Jupiter's Three-Dimensional Magnetosphere

    Hawkins III, S.E. | Online Contents | 1995