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Electron Cyclotron Masers during Solar Flares

Published online by Cambridge University Press:  25 April 2016

S. M. White ,
D. B. Melrose  and
G. A. Dulk
S. M. White
Affiliation:
Dept. of Theoretical Physics, Uni. of Sydney
D. B. Melrose
Affiliation:
Dept. of Theoretical Physics, Uni. of Sydney
G. A. Dulk
Affiliation:
CSIRO Division of Radiophysics
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Extract

It has been suggested (Holman et al 1980; Melrose and Dulk 1982a) that solar microwave spike bursts are due to electron cyclotron maser action. These bursts have been observed in the range 1-3 Ghz, and occur in conjunction with flare-associated impulsive microwave and hard X-ray bursts. The bursts have rise times of a millisecond or less (e.g. Slottje 1978).

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 2 , 1983 , pp. 188 - 191
Copyright
Copyright © Astronomical Society of Australia 1983

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References

Chen Chuan-Le, and R. Loughhead, E., Proc. Astron. Soc. Aust., 5, (1983).Google Scholar
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