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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

G.P. Chernov
G.P. Chernov*
Affiliation:
IZMIRAN, 142092 Moscow region, Troitsk, USSR

Extract

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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 

References

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