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Alfvénic Fronts and the turning-off of the Energy Release in Solar Flares
Published online by Cambridge University Press: 25 April 2016
Abstract
The effect of impulsively turning off the dissipation in an existing model for energy propagation through Alfvénic fronts into the coronal site of energy release in a solar flare is examined. In the optimum case of impedance matching, the flux tube re-stresses on a much longer timescale than it relaxes, suggesting an explanation for the timescales observed in homologous flares.
- Type
- Solar and Solar System
- Information
- Publications of the Astronomical Society of Australia , Volume 11 , Issue 1 , April 1994 , pp. 25 - 27
- Copyright
- Copyright © Astronomical Society of Australia 1994
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