A recent study of solar gradual hard X-ray bursts is summarized. The data are interpreted in terms of a model involving the acceleration and trapping of electrons in post flare loop systems following coronal mass ejections. A controversy about the classification of the metric continuum that typically accompanies gradual hard X-ray events is addressed.


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    Title :

    Solar gradual hard X-ray bursts - Observations and an interpretation


    Contributors:
    Cliver, E. W. (author) / Dennis, B. R. (author) / Kiplinger, A. (author) / Kane, S. (author) / Neidig, D. F. (author)

    Published in:

    Publication date :

    1986-01-01



    Type of media :

    Miscellaneous


    Type of material :

    No indication


    Language :

    English


    Keywords :


    Satellite Observations of Solar Radio Bursts

    J. K. Alexander / H. H. Malitson / C. R. Somerlock et al. | NTIS | 1967


    Microwave and Hard X-Ray Bursts from Solar Flares

    S. S. Holt / R. Ramathy | NTIS | 1968


    Electron spectra deduced from solar hard X-ray bursts

    Trottet, G. / Vilmer, N. | Elsevier | 1984


    Observations of Solar Radio Bursts at 26.3 mc/S

    W. C. Erickson / H. H. Malitson | NTIS | 1965