Particle acceleration in solar flares

Details Particle acceleration in solar flares Particle acceleration in solar flares

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..121..431v&link_type=abstract

(IAU, Colloquium on Solar and Stellar Flares, 104th, Stanford, CA, Aug. 15-19, 1988) Solar Physics (ISSN 0038-0938), vol. 121, n

Physics

Nuclear Physics

22

Particle Acceleration, Solar Corpuscular Radiation, Solar Flares, Electric Fields, Ion Motion, Nuclei (Nuclear Physics), Plasma Turbulence, Shock Wave Propagation

Scientific paper

After discussing a few key observational results which seem to indicate a need for new thinking in research on particle acceleration during solar flares, a number of new theoretical ideas are reviewed which indicate that the solar corona is probably full of small magnetic tubes (fibers). The acceleration mechanisms proposes so far are briefly reviewed, and a new acceleration mechanism proposed especially for a fibrous corona is discussed.

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