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The ionosphere of NeptuneLimited knowledge of ionospheric processes of the outer planets and practically no information on the upper atmosphere of Neptune result in a range of possible ionospheres for Neptune. Various cases are investigated in order to establish a theoretical framework of the ionospheric structure against which the radio occultation measurements can be evaluated. The peak electron densities could range from 1000/cu cm to 10 to the 6th/cu cm depending on ion loss processes and particle ionization processes. The scale height could also range from 300 km to 2000 km depending on the exospheric temperature. Although various assumptions must be made, it is predicted that an auroral ionosphere with large electron densities and a large scale height will be observed by the ingress radio occultation measurement, and that a compressed ionosphere with small electron densities will be seen during the egress measurement.
Document ID
19890062613
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Shinagawa, H.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Waite, J. H., Jr.
(Southwest Research Institute San Antonio, TX, United States)
Date Acquired
August 14, 2013
Publication Date
August 1, 1989
Publication Information
Publication: Geophysical Research Letters
Volume: 16
ISSN: 0094-8276
Subject Category
Lunar And Planetary Exploration
Accession Number
89A49984
Distribution Limits
Public
Copyright
Other

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