Physics
Scientific paper
Sep 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999sffg.conf...74s&link_type=abstract
Structure Formation and Function of Gaseous, Biological and Strongly Coupled Plasmas, p. 74
Physics
Magnetic Field Reconnection, Solar Magnetic Field, Solar Flares, Plasmas (Physics), Coronas, Stellar Mass Ejection, Coronal Loops, X Ray Sources, Solar X-Rays, X Ray Telescopes
Scientific paper
The solar X-ray observing satellite Yohkoh has discovered various new dynamic features in solar flares and corona, e.g., cusp-shaped flare loops, above-the-loop-top hard X-ray sources, X-ray plasmoid ejections from impulsive flares, transient brightenings (spatially resolved microflares), X-ray jets, large scale arcade formation associated with filament eruption or coronal mass ejections, and so on. It has soon become clear that many of these features are closely related to magnetic reconnection. We can now say that Yohkoh established (at least phenomenologically) the magnetic reconnection model of flares. In this paper, we review various evidence of magnetic reconnection in solar flares and corona, and present unified model of flares on the basis of these new Yohkoh observations.
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