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Numerical Simulation of Type III Bursts

Published online by Cambridge University Press:  14 August 2015

T. Takakura
T. Takakura*
Affiliation:
Department of Astronomy, University of Tokyo, Tokyo, Japan

Extract

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By the use of semi-analytical method, modeling of three kinds of type III solar radio bursts have been made. Many basic problems about the type III bursts and associated solar electrons have been solved showing some striking or unexpected results. If the fundamental radio emissions should be really observed as the normal type III bursts, the emission mechanism would not be the currently accepted one, i.e. the scattering of plasma waves by ions.

Type
Session V - Solar Bursts - Meter-Decameter Wavelengths
Information
Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 299 - 302
Copyright
Copyright © Reidel 1980 

References

Takakura, T., and Shibahashi, H.: 1976, Solar Phys. 46, pp. 323–346.Google Scholar
Takakura, T.: 1977, Solar Phys. 52, pp. 429–461.Google Scholar
Takakura, T.: 1979a, Solar Phys. 61, pp. 143–159.Google Scholar
Takakura, T.: 1979b, Solar Phys. 61, pp. 161–186.CrossRefGoogle Scholar
Takakura, T.: 1979c, Solar Phys. 62, 375.Google Scholar
Takakura, T.: 1979d, Solar Phys. 62, 383.CrossRefGoogle Scholar
Magelssen, G. R., and Smith, D. F.: 1977, Solar Phys. 55, pp. 211–240.Google Scholar
Smith, D. F.: 1977, Astrophys. J. 216, pp. L53–L57.Google Scholar
Nicholson, D. R., Goldman, M. V., Hoyng, P., and Weatherall, J. C.: 1978, Astrophys. J. 223, pp. 605–619.Google Scholar