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Behaviour of Whistlers in Coronal Magnetic Traps and Its Relevance to a New Fine Structure in Solar Type IV Radio Bursts
Published online by Cambridge University Press: 19 July 2016
Extract
A possible contribution of whistlers to fine structure production due to the coalescence process with plasma waves 1 + w → t at frequencies ω1 ± ωw = ωt is estimated. A whistler ray tracing in the solar corona with the twice Newkirk density model and with a dipole magnetic field using a standard numerical integration of the Haselgrove two-dimensional equations is performed.
- Type
- IX. Solar Radio Emission
- Information
- Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 515 - 516
- Copyright
- Copyright © Kluwer 1990