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Detection of Jovian whistler mode chorus - Implications for the Io torus auroraNear the Io torus outer boundary (L of about 8), the Voyager 1 plasma wave instrument detected high frequency (f) waves near one-half the electron cyclotron frequency fc. High resolution waveform measurements demonstrate that these signals (f approximately equal to fc/2) are banded whistler mode chorus at f not greater than fc/2 and half-cyclotron frequency emissions with f slightly above fc/2. The density (about 2.5 per cu cm), the energy (a few keV), and the omnidirectional energy flux (100 ergs/sq cm-sec), of the electrons resonant with the chorus were determined.
Document ID
19800040000
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Coroniti, F. V.
(TRW Defense and Space Systems Group Redondo Beach, CA, United States)
Kennel, C. F.
(TRW Defense and Space Systems Group, Redondo Beach; California, University Los Angeles, Calif., United States)
Scarf, F. L.
(TRW Defense and Space Systems Group Redondo Beach, Calif., United States)
Kurth, W. S.
(TRW Defense and Space Systems Group Redondo Beach, CA, United States)
Gurnett, D. A.
(Iowa, University Iowa City, Iowa, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1980
Publication Information
Publication: Geophysical Research Letters
Volume: 7
Subject Category
Lunar And Planetary Exploration
Accession Number
80A24170
Funding Number(s)
CONTRACT_GRANT: JPL-954012
CONTRACT_GRANT: NGL-16-001-043
CONTRACT_GRANT: JPL-954013
Distribution Limits
Public
Copyright
Other

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