The auroral kilometric radiation from Uranus and its magnetospheric implications

Details The auroral kilometric radiation from Uranus and its magnetospheric implications The auroral kilometric radiation from Uranus and its magnetospheric implications

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987repm.work.....c&link_type=abstract

Universitaet Graz and Oesterreichische Akademie der Wissenschaften, International Workshop on Radio Emissions from Planetary Mag

Computer Science

Auroral Zones, Kilometric Waves, Planetary Magnetospheres, Planetary Radiation, Radio Emission, Uranus Atmosphere, Electron Cyclotron Heating, Electron Density (Concentration), Frequency Ranges, Voyager 2 Spacecraft

Scientific paper

The Gulkis and Carr (1987) emission beam model for the kilometric radio emission from Uranus and types of information regarding the Uranian inner magnetosphere that may be derivable from its application are discussed. A modeled electron density profile is presented. The manner in which the hollow-cone beam from each element of the distributed auroral-zone source varies with frequency is determined. It is suggested that the observed effects might be due to refraction by a smooth component of the electron density variation with distance, together with multiple small refractions by electron density inhomogeneities along the ray path.

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