Two-dimensional, time-dependent model calculations indicate that an interplay between velocity and spatial diffusion may be responsible for the acceleration of implanted heavy ions in the cometary preshock region. Velocity diffusion (second order Fermi acceleration) accelerates the pickup ions to moderate energies thus creating a seed population for the more efficient diffusive-compressive shock acceleration. Solar wind convection limits the time available for diffusive-compressive acceleration, therefore the resulting energy spectrum above 100 keV is a power law with a spectral index of 5 - 6, a value which is in reasonably good agreement with observations.


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    Titel :

    Combined first and second order Fermi acceleration at comets


    Beteiligte:
    Gombosi, T. I. (Autor:in) / Lorencz, K. (Autor:in) / Jokipii, J. R. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1989-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Combined first and second order Fermi acceleration at comets

    Gombosi, T.I. / Lorencz, K. / Jokipii, J.R. | Elsevier | 1989


    First-order Fermi shock acceleration in solar flares

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


    First-order Fermi shock acceleration in solar flares

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


    Acceleration Modes in Fermi Accelerator

    Saif, F. / Rehman, I. U. | British Library Online Contents | 2013


    Comets

    Engineering Index Backfile | 1953