Alfvenic fronts and the turning-off of the energy release in solar flares

Details Alfvenic fronts and the turning-off of the energy release in solar flares Alfvenic fronts and the turning-off of the energy release in solar flares

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasau..11...25w&link_type=abstract

Astronomical Society of Australia, Proceedings, vol. 11, no. 1, p. 25-27

Astronomy and Astrophysics

Astrophysics

2

Energy Transfer, Magnetohydrodynamic Waves, Solar Corona, Solar Flares, Astrophysics, Impedance Matching, Solar Wind, Time Measurement, Wave Propagation

Scientific paper

The effect of impulsively turning off the dissipation in an existing model for energy propagation through Alfvenic fronts into the coronal site of enerrgy 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.

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