Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...315l.151b&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 315, April 15, 1987, p. L151-L154.
Astronomy and Astrophysics
Astronomy
4
Auroral Irradiation, Kilometric Waves, Magnetic Properties, Planetary Magnetic Fields, Radio Waves, Uranus (Planet), Magnetic Dipoles, Planetary Rotation, Radio Bursts, Voyager 2 Spacecraft, Uranus, Kilometer Waves, Radiation, Beaming, Magnetic Fields, Latitude, Radio Waves, Emissions, Voyager 2, Spacecraft Observations, Analysis, Models, Source, Magnetic Poles, Dipole, Magnetic Moments, Interiors, Magnetosphere, Planetary Radio Astronomy Instrument, Frequencies, Pra
Scientific paper
Radio waves from Uranus at 481.2 kHz detected by Voyager 2 show a strong beaming effect. When the data are analyzed according to the magnetic latitude of the observer in an offset tilted dipole field model, a sharply defined emission beam extending from 25 to 55 deg latitude is evident consistent with a source over the south magnetic pole. The lack of prominent emission from the north magnetic pole can be attributed to the large spatial offset of the magnetic dipole resulting in much lower source frequencies. For proper alignment of the beam, an advance of the dipole axis longitude by 23 deg from the standard model is required. This phase shift is interpreted as the result of higher order magnetic moments producing a skew of the field lines at low altitudes in the polar source region. This conclusion further substantiates models of the interior of Uranus which predict a complex intrinsic field with significant nondipolar contributions to the surface magnetic field.
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