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On the Radio Frequency Spectrum of Jupiter

Published online by Cambridge University Press:  25 April 2016

L. J. Gleeson ,
M. P. C. Legg  and
K. C. Westfold
L. J. Gleeson
Affiliation:
Monash University, Melbourne
M. P. C. Legg
Affiliation:
Monash University, Melbourne
K. C. Westfold
Affiliation:
Monash University, Melbourne
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Extract

Recent observations of the radio-frequency flux spectrum of Jupiter in the frequency range 80-10 000 MHz suggest that the synchrotron component is not independent of frequency as has been generally accepted. Rather, the flux decreases at frequencies below 300 MHz and above 3000 MHz. In this paper we show that extensions and variations of the well-known dipolar model for this emission can account for the modified spectrum.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 7 , April 1970 , pp. 320 - 322
Copyright
Copyright © Astronomical Society of Australia 1970

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References

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