Models of Uranium continuum radio emission

Details Models of Uranium continuum radio emission Models of Uranium continuum radio emission

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jgr....9215189r&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 92, Dec. 30, 1987, p. 15189-15198.

Astronomy and Astrophysics

Astronomy

20

Astronomical Models, Continuous Spectra, Emission Spectra, Radio Bursts, Uranus Atmosphere, Kilometric Waves, Miranda, Planetary Magnetic Fields, Radiant Flux Density, Spatial Distribution, Voyager 2 Spacecraft

Scientific paper

Uranium continuum radio emission detected by the Voyager 2 Planetary Radio Astronomy experiment during the January 1986 encounter is considered. The continuum emissions comprised four components (equatorial emissions, anomaly emissions, strong nightside emissions, and weak nightside emissions) associated with different sources. The equatorial emissions appeared most prominently during the days before closest approach and extended from 40 kHz or below to about 120 kHz. The anomaly emissions were seen about 12 hours before closest approach and extended to about 250 kHz. The agreement found between Miranda's phase and strong radio emission at 20.4 kHz, just after closest approach, suggests intense dynamic activity on the Miranda L shell.

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