Isotopic overabundances and the energetic particle model of solar flares

Details Isotopic overabundances and the energetic particle model of solar flares Isotopic overabundances and the energetic particle model of solar flares

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..257p&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 257-260 (SEE N85-34729 23-92)

Computer Science

Energetic Particles, Interplanetary Space, M Region, Magnetic Fields, Magnetohydrodynamic Turbulence, Solar Flares, Flux (Rate), Magnetic Anomalies, Particle Acceleration, Plasma Turbulence, Solar Atmosphere, Solar Wind

Scientific paper

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.

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