Fast-drift shadow events in Jupiter's decametric radio spectra

Computer Science

Scientific paper

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Atmospheric Radiation, Decametric Waves, Jupiter Atmosphere, Planetary Radiation, Radio Spectra, Emission Spectra, Radio Bursts, Radio Spectroscopy, Shadows, Jupiter, Decameter Waves, Radio Waves, Spectra, Shadows, Bursts, Source, Emissions, Earth-Based Observations, Radio Methods, Formation, Origin, Models, Electrons

Scientific paper

High-resolution dynamic spectra of Jovian S-bursts frequently reveal sloping gaps crossing bands of L-burst emission with drift rates comparable to those of S-bursts. These fast-drift shadow events are often sharply bounded on one edge by an S-burst, and sometimes on both edges by a pair of S-bursts emanating from a common vertex. It is suggested that the investigation of such S- and L-burst interactions may provide new insights of considerable importance in the search for the Jovian decametric emission mechanism.

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