Abstract Observational evidence that the plasma in hot X-ray sources in solar flares is highly turbulent is presented. The turbulent flare kernels are considered to be the main source of the flare energy release. Properties of kernels in big flares are discussed.


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    Title :

    Investigation of turbulent kernels in solar flares


    Contributors:
    Jakimiec, J. (author) / Fludra, A. (author)

    Published in:

    Publication date :

    1991-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English





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