Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993georl..20..321r&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 20, no. 4, p. 321-324.
Astronomy and Astrophysics
Astronomy
25
Jupiter (Planet), Planetary Magnetospheres, Planetary Radiation, Radio Emission, Radio Sources (Astronomy), Northern Hemisphere, Planetary Magnetic Fields, Ulysses Mission, Jupiter, Source, Origin, Position (Location), Emissions, Polarization, Radiowaves, Hectometer Waves, Intensity, Frequencies, Magnetosphere, Spacecraft Observations, Ulysses Mission, Latitude, Polar Regions, Parameters
Scientific paper
Northern Jovian hectometric (HOM) radio emissions, detected from high Jovian latitudes by the Unified Radio and Plasma Wave experiment on the Ulysses spacecraft, were observed at all Jovian longitudes. This emission was observed to be predominantly right-hand circularly polarized, but some left-hand circular polarization was observed implying the presence of O mode emissions from the northern Jovian hemisphere. Intense HOM emissions, with well-defined directions and polarizations, were often confined to similar longitudinal regions where intense HOM emissions were previously observed at low latitudes. The present analysis confirms that these northern HOM sources lie in the Jovian polar regions on magnetic field lines that pass through the Io plasma torus. The observations may be consistent with emission from either a filled cone beam or a longitudinal distribution of thin hollow cones.
Fainberg Joe
Reiner M. J.
Stone Robert G.
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