Ion energy storage for post-flare loops

Details Ion energy storage for post-flare loops Ion energy storage for post-flare loops

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4...58h&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 58-61 (SEE N85-34729 23-92)

Physics

Coronal Loops, Energy Storage, Ions, Solar Flares, Solar Protons, Gamma Rays, High Temperature, Trapped Particles

Scientific paper

Low-energy non-thermal protons may have long lifetimes in coronal loops with low density and high temperature. If energy were stored in such protons in the initial phases of a solar flare, it could be released slowly during the later phases. Within the present observational limits for post-flare loops, this mechanism should be considered in addition to a field-line reconnection theory of the Kopp and Pneuman type. The thin-target gamma ray emission from the trapped protons is below present limits, but more sensitive observations can test the hypothesis.

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