Source of bursty radio emissions from Uranus

Details Source of bursty radio emissions from Uranus Source of bursty radio emissions from Uranus

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988georl..15.1149b&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 15, Sept. 1988, p. 1149-1152.

Physics

6

Planetary Radiation, Radio Bursts, Uranus (Planet), Auroral Zones, High Energy Electrons, Planetary Magnetospheres, Voyager 2 Spacecraft, Wave Interaction

Scientific paper

The distribution of energetic electrons on the auroral field lines in the magnetosphere of Uranus can develop large anisotropies and a large loss cone. These, in turn, can lead to large-amplitude whistler waves and upper-hybrid waves. Nonlinear currents caused by interaction between these waves can produce radio emissions that are in good agreement with the bursty Uranian kilometric radiation observed by Voyager 2.

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