Abstract Information regarding the acceleration of electrons in solar flares may be deduced from the hard X ray emission they produce through bremsstrahlung. From these observations, the electron energy spectra and temporal evolution as well as some characteristics of the ambient medium can be deduced through models. Here, a model of hard X ray emission is briefly presented and some of the results are discussed in the light of hard X ray observations and acceleration processes.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    Electron spectra deduced from solar hard X-ray bursts


    Beteiligte:
    Trottet, G. (Autor:in) / Vilmer, N. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 4 , 2-3 ; 153-156


    Erscheinungsdatum :

    1984-01-01


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



    Venus Planetary Lightning Rate as Deduced from VLF Bursts

    Ho, C.-M. / Strangeway, R. J. / Russell, C. T. et al. | British Library Conference Proceedings | 1995


    Venus planetary lightning rate as deduced from VLF bursts

    Ho, C.-M. / Strangeway, R. J. / Russell, C. T. | NTRS | 1995


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

    Cliver, E. W. / Dennis, B. R. / Kiplinger, A. et al. | NTRS | 1986



    Mesospheric ozone densities deduced from solar occultation measurements

    Ohle, K.H. / Sonnemann, G. / Fichtelmann, B. | Elsevier | 1984