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Evidence of Directivity of Solar Type III Radio Burst Storm Emission

Published online by Cambridge University Press:  25 April 2016

C. S. Wright
C. S. Wright*
Affiliation:
Dept. of Science, Solar Observatory, Culgoora
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Extract

Solar type III radio bursts often occur for prolonged periods (≳ 1 hour) with small time intervals (≲ 1 minute) between bursts. Such phenomena usually are confined to decametre wavelengths (frequency ≲ 100 MHz) and are called ‘type III storms’ (e.g. Stewart and Labrum 1972).

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 62 - 64
Copyright
Copyright © Astronomical Society of Australia 1980

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References

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