The first-order Fermi shock acceleration model is compared with specific observations where electron, proton, and alpha particle spectra are available. In all events, it is found that a single shock with a compression ratio as inferred from the low-energy proton spectra can reasonably produce the full proton, electron, and alpha particle spectra. The 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 sec 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



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    First-order Fermi shock acceleration in solar flares

    Ellison, D.C. / Ramaty, R. | Elsevier | 1984


    Electron Acceleration in Solar Flares

    Litvinenko, Y. E. / International Council of Scientific Unions | British Library Conference Proceedings | 2003


    Electron acceleration in solar flares

    Litvinenko, Yuri E. | Elsevier | 2003


    Electron acceleration in solar flares

    Litvinenko, Yuri E. | Online Contents | 2003