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    Isotopic overabundances and the energetic particle model of solar flares (1985)
    In:  CASI
    Details
    Publication Date: 2019-06-28
    Description: According to the energetic particle model of solar flares particles are efficiently accelerated in the magnetic field loop of an active region (AR) by hydromagnetic turbulence. It is demonstrated that the isotopic overabundances observed in some flares are not a consequence of the flare itself but are characteristic of the plasma in the AR. Only when a flare releases the plasma into the interplanetary space it is possible to observe this anomalous composition at spacecraft locations.
    Keywords: SOLAR PHYSICS
    Type: SH-2.2-1 , 19th Intern. Cosmic Ray Conf - Vol. 4; p 257-260; NASA-CP-2376-VOL-4
    Format: application/pdf
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