Beaming of Jupiter's decametric emission

Computer Science

Scientific paper

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Decametric Waves, Jupiter Atmosphere, Planetary Radiation, Radio Spectra, Voyager 1 Spacecraft

Scientific paper

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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