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Possible Causes of Line Splitting in Drift Pair Solar Bursts

Published online by Cambridge University Press:  25 April 2016

D. B. Melrose  and
W. Sy
D. B. Melrose
Affiliation:
Department of Theoretical Physics, Faculty of Science, Australian National University
W. Sy
Affiliation:
Department of Theoretical Physics, Faculty of Science, Australian National University
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Extract

In this paper possible causes of line splitting in emission near the local plasma frequency are considered in connection with drift pair solar radio bursts. The basic model envisaged for the bursts involves a bunch of electrons streaming through the solar corona at several times the thermal velocity of electrons. The emission process assumed is the transformation of coherently generated electron plasma waves (I-waves) into electromagnetic waves (t-waves) with little change in frequency.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 1 , July 1971 , pp. 56 - 57
Copyright
Copyright © Astronomical Society of Australia 1971

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References

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