A new solar flare scenario: high-beta plasma disruption

Details A new solar flare scenario: high-beta plasma disruption A new solar flare scenario: high-beta plasma disruption

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..749s&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

1

Flare, High-Beta Plasma, Ballooning Instability, Turbulence

Scientific paper

A new solar flare scenario is proposed based on a high-beta plasma instability. Plasma confined in a curved magnetic field (magnetic loop) has free energy. This free energy will be converted to other forms explosively under certain conditions through localized quasi-interchange instability called "ballooning instability". Relations between solar flare phenomena and ballooning instability phenomena are discussed.

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