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Flare Model with Force-Free Fields and Helical Symmetry
Published online by Cambridge University Press: 14 August 2015
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.
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van der Laan, P.C.T.: 1968, Proc. II ème Coll. Intern. Interactions Champs Oscillants et les Plasmas, Vol. 4, p. 1095, Saclay, France.Google Scholar