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On the Relative Importance of Radiative, Mechanical and Magnetic Energy Release of Flares

Published online by Cambridge University Press:  25 April 2016

D. J. McLean  and
G. A. Dulk
D. J. McLean
Affiliation:
Division of Radiophysics, CSIRO, Sydney
G. A. Dulk
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

For many years we have had evidence from solar radio bursts of violent mass motions in the solar corona: type II bursts reveal the passage of shock waves through the solar corona, and moving type IV bursts show that plasma and magnetic field travel to great distances without any sign of slowing down.

Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 4 , 1978 , pp. 251 - 252
Copyright
Copyright © Astronomical Society of Australia 1978

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