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Shock Drift Acceleration and Type II Solar Radio Bursts
Published online by Cambridge University Press: 25 April 2016
Abstract
Shock drift acceleration of the electrons which produce herringbone structure in type II bursts is considered. A non-coplanar component of the magnetic field within the shock front and an electric field across the shock are taken into account. A quantitative difficulty with shock drift acceleration is identified, and possible ways of overcoming the difficulty are outlined.
- Type
- Solar and Solar System
- Information
- Publications of the Astronomical Society of Australia , Volume 11 , Issue 1 , April 1994 , pp. 21 - 24
- Copyright
- Copyright © Astronomical Society of Australia 1994
References
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