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The Emission Mechanism of Solar Moving Type IV Metre-Wave Radio Sources

Published online by Cambridge University Press:  25 April 2016

R. A. Duncan
R. A. Duncan*
Affiliation:
Division of Radiophysics, CSIRO
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Extract

The term ‘moving Type IV’ denotes a spectacular class of solar event in which the radio source, beginning low in the corona, moves outward, typically at hundreds of kilometres per second (Wild et al. 1963).

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Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 67 - 70
Copyright
Copyright © Astronomical Society of Australia 1980

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