The main source of radio emission from the magnetosphere of Uranus.
Observations of kilometric radiation from Uranus made with the planetary radio astronomy experiment on the Voyager 2 spacecraft are presented and discussed.  Similarities between the auroral kilometric radiation from Earth and the observed Uranus emission are pointed out.  A geometrical beaming model is developed in which a single distributed source is located above the darkside auroral region and emits in the extraordinary mode by the cyclotron maser process.  The model can account for nearly all the Uranian kilometric radiation from the high-frequency limit near 850 kHz down to about 150 kHz and for much of it down to the lower limit of 20 kHz.
Gulkis
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Jet Propulsion Laboratory, California Institute of Technology, Pasadena, USA.
Carr
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D055580:Astronomical Phenomena; D001256:Astronomy; D017357:Cyclotrons; D005118:Extraterrestrial Environment; D008280:Magnetics; D008962:Models, Theoretical; D011846:Radio Waves; D013026:Space Flight / Q000295:instrumentation*; D018540:Uranus