Models for Jupiter's decametric arcs

Astronomy and Astrophysics – Astronomy

Scientific paper

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Arcs, Astronomical Models, Decametric Waves, Jupiter (Planet), Planetary Radiation, Radio Emission, Fine Structure, Io, Magnetohydrodynamic Waves, Plasma Interactions, Refracted Waves, Toroidal Plasmas, Voyager Project, Wave Interaction, Wave Propagation, Jupiter, Models, Decameter Waves, Arcs, Wavelengths, Emissions, Io, Voyager 1, Voyager 2, Magnetic Properties, Polarization, Longitude, Source Medium, Polar Regions, Structure, Surface, Diagrams, Geometry, Satellites, Plasma Torus, Alfven Waves, Asymmetry

Scientific paper

Arc-shaped structures that dominate Jupiter's decametric emission are discussed in terms of a magnetic fine structure. The sequence of arcs manifest the occurence of widespread fine structures similar to the white ovals on Jupiter's visible surface. An arc concave toward increasing time occurs at the east limb passage, and an arc convex occurs at the west limb passage, which is consistent with the early source producing vertex early arcs, and the late source producing vertex late arcs. Due to the geometry of the Io plasma torus (IPT) which is arranged so that Io skims the northern surface of the IPT, for any connection between Io and Jupiter's surface that involves Alfven waves, the propagation time, the refraction and the directional defocusing of these waves must be strongly influenced by the amount of Alfven wave path length between the instantaneous position of Io and the surface of the IPT.

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