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A Model of the Evolution of the Flux Density and Polarization in Isolated Moving Type IV Bursts

Published online by Cambridge University Press:  25 April 2016

E. J. Schmahl
E. J. Schmahl*
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

In the first four years of operation with the 80 MHz heliograph at Culgoora, 24 events classified as moving type IV were observed. Their observed characteristics can be interpreted in terms of gyro-synchrotron radiation from mildly relativistic electrons. Many of these events have been presented at previous ASA meetings and 12 have been discussed in the literature in detail.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 2 , March 1972 , pp. 95 - 98
Copyright
Copyright © Astronomical Society of Australia 1972

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References

1 Smerd, S. F. and Dulk, G. A., In ‘Solar Magnetic Fields’: Proceedings of IAU Symposium No. 43, (ed., Howard, Robert), D. Reidel, Dordrecht 1971, p. 616.Google Scholar
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3 Lehnert, B., ‘Dynamics of Charged Particles’, North-Holland, Amsterdam 1964.Google Scholar
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5 Trulsen, J. and Fejer, J. A., J. Plasma Phys., 4, 825 (1970).Google Scholar
6 Wild, J. P. and Hill, E. R., Aust. J. Phys., 24, 43 (1971).Google Scholar