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A New Solar Flare Scenario: High-beta Plasma Disruption View all abstracts by submitter

Kiyoto Shibasaki   Submitted: 2003-01-14 23:02

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.

Authors: Kiyoto Shibasaki
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Publication Status: ESA SP-506, 749 (2002)
Last Modified: 2003-01-14 23:02
Go to main E-Print page  SOHO/CDS and Ground Based Observations of a Two-Ribbon
 Flare:Spatially Resolved Signatures of Chromospheric Evaporation  Signature of Energy Release and Particle Acceleration Observed by the Nobeyama Radioheliograph  Edit Entry  Download Preprint  Delete Entry 

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