Ray tracing of broadband bursty radio emissions from Uranus

Details Ray tracing of broadband bursty radio emissions from Uranus Ray tracing of broadband bursty radio emissions from Uranus

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990georl..17..109c&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 17, Feb. 1990, p. 109-112. Research supported by the Southwest Research Inst

Physics

Optics

6

Broadband, Planetary Radiation, Radio Astronomy, Radio Bursts, Ray Tracing, Uranus (Planet), Geometrical Optics, Geometrical Theory Of Diffraction, Magnetic Field Configurations, Night Sky, Plasma Waves, Voyager 2 Spacecraft, Uranus, Radio Waves, Emissions, Bursts, Source, Position (Location), Plasma, Magnetic Fields, Distribution, Models, Procedure, Distance, Voyager 2 Mission, Spacecraft Observations, Pra Instrument, Longitude, Frequencies

Scientific paper

To determine the source position of the broadband bursty emission, rays of X-mode emissin were traced from source positions along magnetic field lines with footprints that form a large grid centered approximately on the south magnetic pole of Uranus. For large wave normal angles, source regions different from those producing b-smooth emission were found. The emission observed prior to closest approach has a source along field lines that are distinct from those which generate emissions observed after closest approach.

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