Source location of the smooth high-frequency radio emissions from Uranus

Details Source location of the smooth high-frequency radio emissions from Uranus Source location of the smooth high-frequency radio emissions from Uranus

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989georl..16..341f&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 16, May 1989, p. 341-344.

Astronomy and Astrophysics

Astronomy

7

Planetary Radiation, Radio Sources (Astronomy), Uranus (Planet), High Frequencies, Planetary Magnetic Fields, Radio Emission, Voyager Project, Uranus, Radio Waves, Emissions, Frequencies, Source, Position (Location), Techniques, Spacecraft Observations, Voyager 2 Mission, Pra Instrument, Diagrams, Statistical Analysis, Magnetic Fields, Procedure

Scientific paper

The source location of the smooth high-frequency radio emissions from Uranus has been determined. Specifically, by fitting the signal dropouts which occurred as Voyager traversed the hollow center of the emission pattern to a symmetrical cone centered on the source magnetic field direction at the cyclotron frequency, a southern-hemisphere (nightside) source was found at approximately 56 deg S, 219 deg W. The half-angle for the hollow portion of the emission pattern was found to be 13 deg.

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