Source location of the Jovian hectometric radiation via ray-tracing technique

Details Source location of the Jovian hectometric radiation via ray-tracing technique Source location of the Jovian hectometric radiation via ray-tracing technique

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....95.6423l&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 95, May 1, 1990, p. 6423-6435. Research supported by the European Thesis

Physics

26

Jupiter (Planet), Planetary Radiation, Radio Emission, Ray Tracing, Cyclotron Radiation, Kilometric Waves, Laser Stability, Lines Of Force, Masers, Planetary Magnetic Fields, Jupiter, Radiation, Emissions, Hectometer Waves, Source, Techniques, Origin, Ray Tracing, Spacecraft Observations, Voyager Missions, Beaming, Pra Instrument, Diagrams, Geometry, Simulations, Magnetic Fields, Position (Location), Parameters

Scientific paper

The source location of the Jovian hectometric radiation (HOM) was investigated by ray tracing using realistic magnetic field and plasma models. The results strongly indicate that the HOM sources lie within the tail-field aurora, whose field lines connect the polar regions to the Jovian magnetic tail, at distances from 2 to 7 Jupiter radii from Jupiter's center. Although the exact source location in magnetic latitude is related to the assumed cone half-angle theta, an HOM source at the tail-field auroral region accounts for a large variety of the phenomena observed so far.

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