Transport and containment of plasma, particles and energy within flares

Details Transport and containment of plasma, particles and energy within flares Transport and containment of plasma, particles and energy within flares

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86...79a&link_type=abstract

(Japan Society for the Promotion of Science and National Science Foundation, U.S.-Japan Seminar on the Recent Advances in the Un

Physics

10

Magnetoplasmadynamics, Solar Flares, Solar Wind, Particle Motion, Rocket-Borne Instruments, Solar Corona, Solar Magnetic Field, Solar Maximum Mission, Stellar Models, X Ray Spectroscopy

Scientific paper

Results from the analysis of flares observed by the Solar Maximum Mission and a recent rocket experiment are discussed. The authors find evidence for primary energy release in the corona through the interaction of magnetic structures, particle and plasma transport into more than a single magnetic structure at the time of a flare and a complex and changing magnetic topology during the course of a flare. The rocket data are examined for constraints on flare cooling, within the context of simple loop models. These results form a basis for comments on the limitations of simple loop models for flares.

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