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Offset, tilted dipole models of Uranian smooth high-frequency radio emissionThe smooth high-frequency (SHF) component of the radio emission detected during the Voyager 2 encounter with Uranus (January 1986) is studied. An offset tilted dipole (OTD) investigation of the SHF emission at L shells is carried out within the range of the bursty source locations. A viable high L shell model is presented. It is suggested that Miranda, which reaches a minimum L shell at L = 5, may be related to the timing of several types of radio emissions.
Document ID
19900063367
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Schweitzer, Andrea E.
(Radiophysics, Inc. Boulder, CO, United States)
Romig, Joseph H.
(Radiophysics, Inc. Boulder, CO, United States)
Evans, David R.
(Radiophysics, Inc. Boulder, CO, United States)
Sawyer, Constance B.
(Radiophysics, Inc. Boulder, CO, United States)
Warwick, James W.
(Radiophysics, Inc. Boulder, CO, United States)
Date Acquired
August 14, 2013
Publication Date
September 1, 1990
Publication Information
Publication: Journal of Geophysical Research
Volume: 95
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
90A50422
Funding Number(s)
CONTRACT_GRANT: NAS7-918
Distribution Limits
Public
Copyright
Other

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