Abstract A comparative analysis has been carried out of the parameters of energetic electrons in the tail of the Earth’s magnetosphere that belong to three sources, i.e., electrons of solar origin, electrons generated in the magnetosphere of Jupiter, and electrons in the Earth’s magnetosphere. The differences in the time profiles of fluxes and energy spectra of the three electron sources, their relation to fluxes outside the magnetosphere, and periods of the occurrence of electron fluxes of each type are considered.


    Access

    Access via TIB

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    Energetic electrons in the tail and transition region of the magnetosphere


    Contributors:

    Published in:

    Publication date :

    2016




    Type of media :

    Article (Journal)


    Type of material :

    Print


    Language :

    English



    Classification :

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



    Energetic electrons in the tail and transition region of the magnetosphere

    Daibog, E. I. / Lazutin, L. L. / Logachev, Yu. I. et al. | Springer Verlag | 2016


    Evolution and Energization of Energetic Electrons in the Inner Magnetosphere

    Fennell, J.F. / Roeder, J.L. | British Library Conference Proceedings | 2009


    Evolution and Energization of Energetic Electrons in the Inner Magnetosphere

    Fennell, J. F. / Roeder, J. L. | Springer Verlag | 2009



    A statistical survey of tail plasma sheet energetic electrons

    Aasnes, A. / Friedel, R. W. H. / Lavraud, B. et al. | British Library Conference Proceedings | 2006