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Beaming of Jupiter's decametric emission
Authors:Riihimaa  Jorma J.
Affiliation:(1) Aarne Karjalainen Observatory, University of Oulu, Finland
Abstract:Dynamic spectra of a Jovian non-Io-A storm recorded simultaneously by the Voyager 1 spacecraft and by the Kiiminki radio spectrograph are compared. It seems that the emission beam of the storm co-rotates with the planet and has a sloped leading edge, in accordance with the result of Maeda and Carr (1984).
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