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Polarization of Herringbone Structure in Type II Bursts

Published online by Cambridge University Press:  14 August 2015

S. Suzuki ,
R. T. Stewart  and
A. Magun
S. Suzuki
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia
R. T. Stewart
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia
A. Magun
Affiliation:
Institute of Applied Physics, University of Berne, Switzerland

Extract

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Herringbone Type II bursts were first described by Roberts (1959). These bursts are distinguished by their unusual structure - rib-like features (herringbones) extending on either side of a Type II backbone.

Type
Session IV - Solar Bursts - Meter Wavelengths
Information
Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 241 - 245
Copyright
Copyright © Reidel 1980 

References

Roberts, J.A.: 1959, Aust. J. Phys. 12, p. 327.Google Scholar
Sheridan, K.V., Dulk, G.A., and Suzuki, S.: 1980, Proc. IAU Symposium 86 (this volume), pp. 315.Google Scholar
Stewart, R.T.: 1966, Aust. J. Phys. 19, p. 209.Google Scholar
Suzuki, S., and Sheridan, K.V.: 1977, Izv. Vyssh. Uchebn. Zaved. Radiofiz. 20, p. 1432 (English transl. 20, p. 989).Google Scholar
Wild, J.P., Smerd, S.F., and Weiss, A.A.: 1963, Annu. Rev. Astron. Astrophys. 1, p. 291.Google Scholar