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Flare Model with Force-Free Fields and Helical Symmetry

Published online by Cambridge University Press:  14 August 2015

Dirk K. Callebaut
Dirk K. Callebaut*
Affiliation:
Physics Department, U.I.A., Universiteit Antwerpen. Universiteitsplein 1. B-2610 Wilrijk-Antwerpen. Belgium

Abstract

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Physical arguments are given indicating that solar flare magnetic energy storage may happen through force-free fields with helical symmetry (∂z + λ (r) ∂ɸ = o). The mathematical results turn out simple for helical fields whether general, in equilibrium or force-free. A preliminary stability analysis points to appropriate properties.

Type
Part IV. Solar Transient Phenomena Affecting the Corona and Interplanetary Medium: - Theoretical Considerations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 279 - 282
Copyright
Copyright © Reidel 1980 

References

Callebaut, D.K.: 1976, CECAM Report of Workshop on Plasma Physics Applied to Active Phenomena on the Sun (I) Aug. 1-Sept. 30, pp. 8–11.Google Scholar
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Callebaut, D.K.: 1979, CECAM Report, ibid. (II), June 1-30, (to appear).Google Scholar
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