Abstract First order Fermi shock acceleration of electrons, protons and alpha particles is compared to observations of energetic particle events. For each event, a unique shock compression ratio produces spectra in good agreement with observation. The simple model predicts that the acceleration time to a given energy will be approximately equal for electrons and protons and, for reasonable solar parameters, can be less than 1 second to ∼ 100 MeV.


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    Titel :

    First-order Fermi shock acceleration in solar flares


    Beteiligte:
    Ellison, D.C. (Autor:in) / Ramaty, R. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1984-01-01


    Format / Umfang :

    5 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



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