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Statistical study of ion flows in the dayside and nightside plasmasphereA statistical survey of ion flows has been performed with the DE-1 high-altitude plasma instrument during a period of solar maximum conditions. The results indicate that a significant dayside to nightside interhemispheric flow occurs in the outer plasmasphere during periods of increased magnetic activity along convecting magnetic field lines. The ion temperature is found to decrease steadily equatorward into the outer plasmasphere. Although ion abundance ratios obtained using the retarding ion mass spectrometer show that the predominant ion species was H(+), relatively large densities of O(+) were observed in the plasmasphere on several passes.
Document ID
19880059506
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Menietti, J. D.
(Southwest Research Inst. San Antonio, TX, United States)
Burch, J. L.
(Southwest Research Institute San Antonio, TX, United States)
Gallagher, D. L.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 13, 2013
Publication Date
July 1, 1988
Publication Information
Publication: Planetary and Space Science
Volume: 36
ISSN: 0032-0633
Subject Category
Geophysics
Report/Patent Number
ISSN: 0032-0633
Accession Number
88A46733
Funding Number(s)
CONTRACT_GRANT: NAS5-28711
Distribution Limits
Public
Copyright
Other

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