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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

M. S. Wheatland
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, Sydney, NSW 2006
D. B. Melrose
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, Sydney, NSW 2006

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
Copyright
Copyright © Astronomical Society of Australia 1994

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