Physics
Scientific paper
Apr 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....94.3505k&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 94, April 1, 1989, p. 3505-3512. Research supported by NASA.
Physics
4
Planetary Magnetic Fields, Planetary Magnetospheres, Plasma Waves, Uranus Atmosphere, Flyby Missions, Magnetic Field Configurations, Plasma Probes, Voyager 2 Spacecraft, Uranus, Plasma Waves, Magnetotail, Voyager 2 Mission, Frequencies, Spacecraft Observations, Intensity, Emissions, Lecp Instrument, Diagrams, Spectra, Position (Location), Charged Particles, Pws Instrument, Nightside, Comparisons
Scientific paper
Plasma wave phenomena observed during the Voyager 2 passing through the magnetotail of Uranus after its encounter with the planet on January 24, 1986 are described. The location of the wave events, their probable mode of propagation, and their association with various plasma and charged particle observations are presented. It was found that the most remarkable magnetotail plasma waves were inside the distance of about 23 Uranus radii, with an additional event occurring between about 48 and 56 Uranus radii. The frequency of these magnetotail plasma waves was found to be below about 100 Hz, extending down to the 10-Hz lower frequency limit of the receiver. The shape of the spectrum and the location of the wave activity near the boundary layer suggest that these waves may be similar to broadband electrostatic waves observed in similar regions of the earth's magnetotail.
Gurnett Donald A.
Kurth Willaim S.
Mauk Barry H.
Scarf Frederick L.
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