The goal of this oral presentation is to attempt to explain why the 3HE-rich events at 1AU appear to be 'scatter-free'. The largest 3HE- rich flux events of Kahler et al. (1985) are used to examine potential wave-particle interactions as the particles travel from the Sun to 1AU.


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    Title :

    3HE-rich Solar Particle Mean Free Paths


    Contributors:

    Publication date :

    1995-12-01


    Type of media :

    Preprint


    Type of material :

    No indication


    Language :

    English




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