High coronal flares and impulsive acceleration of solar energetic particles

Details High coronal flares and impulsive acceleration of solar energetic particles High coronal flares and impulsive acceleration of solar energetic particles

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...366l..91c&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 366, Jan. 10, 1991, p. L91-L94.

Astronomy and Astrophysics

Astrophysics

25

Energetic Particles, Particle Acceleration, Particle Emission, Solar Corona, Solar Flares, Coronal Loops, Current Sheets, Helium Ions, Solar Electrons

Scientific paper

Evidence is reviewed which suggests that the source regions of high coronal flares (HCFs) are hot. A scenario is considered in which the source region of He-3 enhancement in solar energetic particle events from impulse flares is distinct from the source region of the enhanced abundances of high-Z ions. It is proposed that HCFs occur due to reconnection in the neutral current sheets of coronal streamers.

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