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Ganymede: A New Radio SourceObservations by the Galileo plasma wave receiver during the first two flybys of Ganymede revealed that this Jovian moon is the source of narrowband electromagnetic radio waves, making it the only satellite in the solar system known to generate non-thermal radio emissions. The emissions are the result of mode-coupling from electrostatic electron cyclotron emissions mu the upper hybrid resonance frequency, similar to non-thermal continuum radiation found at the known magnetized planets.
Document ID
19990009291
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kurth, W. S.
(Iowa Univ. Iowa City, IA United States)
Gurnett, D. A.
(Iowa Univ. Iowa City, IA United States)
Roux, A.
(Centre des Etudes Terrestraire et Planetaire Velizy, France)
Bolton, S. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 19, 2013
Publication Date
September 1, 1997
Publication Information
Publication: Geophysical Research Letters
Publisher: American Geophysical Union
Volume: 24
Issue: 17
ISSN: 0094-8534
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
Paper 97GL02249
Funding Number(s)
CONTRACT_GRANT: JPL-958779
Distribution Limits
Public
Copyright
Other

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