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Radio emission from the magnetic equator of UranusThe major observational characteristics of the smooth, narrow bandwidth component of Uranus' radio emissions are well described by sources radiating near the local electron gyrofrequency, confined to the magnetic equatorial plane and encircling the planet at radial distances of approximately 2 to 3 R(U). The most intense emission appears to be generated in association with the epsilon ring at 2.0 R(U) radial distance. A cold electron density of less than or equal to 4/cu cm are inferred in this region.
Document ID
19890047386
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kaiser, M. L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Desch, M. D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Connerney, J. E. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
March 1, 1989
Publication Information
Publication: Journal of Geophysical Research
Volume: 94
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
89A34757
Distribution Limits
Public
Copyright
Other

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