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A Study of Multiple Type II Solar Radio Events

Published online by Cambridge University Press:  25 April 2016

R.D. Robinson  and
K.V. Sheridan
R.D. Robinson
Affiliation:
Division of Radiophysics, CSIRO, Sydney
K.V. Sheridan
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

A Type II solar radio burst is a relatively narrow-bandwidth metre-wavelength emission which drifts outward in the solar corona at a velocity between 500 and 1500 km s-1. It was first described by Wild and McCready (1950) and since then it has been the subject of numerous investigations (see e.g. McLean 1974; Nelson and Robinson 1975).

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Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 4 , 1982 , pp. 392 - 396
Copyright
Copyright © Astronomical Society of Australia 1982

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References

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