Abstract A technique developed for analysing the SMM X-ray spectra has been adapted to the interpretation of high resolution cooled germanium flare spectra. It is shown that these can be fitted equally well by simple all thermal or non-thermal distributions, and that the data set is insufficient to determine the non-thermal nature of the flare.


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    Title :

    Interpretation of X-ray spectra from solar flares


    Contributors:

    Published in:

    Advances in Space Research ; 11 , 1 ; 323-326


    Publication date :

    1991-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



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