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Dynamic Spectra of Jupiter Radio Bursts

Published online by Cambridge University Press:  25 April 2016

G. R. A. Ellis*
Affiliation:
Department of Physics, University of Tasmania

Extract

Extensive observations of the spectra of the decametric radio bursts for Jupiter have been made by Riihimaa, principally at frequencies between 18 and 23 MHz and with frequency resolution of 50 kHz. These showed much fine frequency-time structure in the bursts but pointed to the need for higher frequency resolution and greater antenna sensitivity. This paper reports the results of observations made of the Jupiter bursts between February and April, 1972, using the Llanherne low frequency telescope (Ellis,).

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1972

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References

1 Riihimaa, J. J., Nature, 202, 476 (1964).Google Scholar
3 Riihimaa, J. J., The radio spectrum of Jupiter. Report S22, University of Oulo, Finland (1971).Google Scholar
3 Ellis, G. R. A., Proc. ASA, p. 135 (1972).CrossRefGoogle Scholar
4 Ellis, G. R. A., J. Radio Sci., 69D, 1513 (1965).Google Scholar