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On the Origin of Modulation Lanes in the Dynamic Spectra of Jupiter’s Decametric Radiation*

Published online by Cambridge University Press:  25 April 2016

V. V. Zheleznyakov  and
V. E. Shaposhnikov
V. V. Zheleznyakov
Affiliation:
institute of Applied Physics, Gorky, USSR
V. E. Shaposhnikov
Affiliation:
institute of Applied Physics, Gorky, USSR
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Extract

In this paper, two models for the origin of modulation lanes in Jovian radiation are discussed. The results of calculations of dynamic spectra due to the Cotton-Mouton effect in Jupiter’s plasma envelope and due to modulation of the frequency spectrum in the source are reproduced. The characteristics of the theoretical spectra are then described. This offers the possibility of solving the problem of modulation lanes by comparison of observed Jovian dynamic spectra with the theoretical ones.

Type
Jupiter, Cosmic Rays
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 4 , 1978 , pp. 259 - 262
Copyright
Copyright © Astronomical Society of Australia 1978

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References

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