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.


    Access

    Check access

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    Electron spectra deduced from solar hard X-ray bursts


    Contributors:
    Trottet, G. (author) / Vilmer, N. (author)

    Published in:

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


    Publication date :

    1984-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



    Venus planetary lightning rate as deduced from VLF bursts

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


    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


    Microwave and Hard X-Ray Bursts from Solar Flares

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


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

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