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Fine Structure in Solar Type III Radio Bursts Spectra

Published online by Cambridge University Press:  14 August 2015

M. R. Perrenoud
Affiliation:
Radio Astronomy Group, Federal Institute of Technology ETH, Zürich, Switzerland
A. R. Treumann
Affiliation:
Radio Astronomy Group, Federal Institute of Technology ETH, Zürich, Switzerland

Abstract

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The new digitalized polarispectrometer IKARUS (Perrenoud, 1979) at ETH, Zürich gave the possibility for a more detailed investigation of the solar type III spectral evolution.

Type
Session IV - Solar Bursts - Meter Wavelengths
Copyright
Copyright © Reidel 1980 

References

Alvarez, H., Lin, R. P., and Bame, S. J., Solar Phys. 44 (1975) 485.CrossRefGoogle Scholar
Gurnett, D. A., and Anderson, R. R., J. Geophys. Res. 82 (1977) 632.CrossRefGoogle Scholar
Gurnett, D. A., Baumback, M. M. and Rosenbauer, H., J. Geophys. Res. 83 (1978) 616.CrossRefGoogle Scholar
Lin, R. P., Evans, L. G., and Fainberg, J., Ap. J. 14 (1973) L191.Google Scholar
Melrose, D. B. Preprint Univ. Sydney 1979.Google Scholar
Papadopoulos, K., Phys. Fluids 18 (1975) 1769.CrossRefGoogle Scholar
Papadopoulos, K., and Freund, H. P., Naval Res. Lab. NRL Memorandum Rep. 3922, Wash., DC, Feb. 7, 1979.Google Scholar
Perrenoud, M. R., , ETH-Zürich, 1979.Google Scholar
Treumann, R., Phys. Lett. 68A (1978) 445.CrossRefGoogle Scholar
Vedenov, A. A., and Ryutov, D. D. in Rev. of Plasma Phys. Vol. 6, Consult. Bureau, N.Y. 1976, p. 1.Google Scholar