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Plasma observations at the earth's magnetic equatorNew observations of particle and wave data from the magnetic equator from the DE 1 spacecraft are reported. The results demonstrate that the equatorial plasma population is predominantly hydrogen and that the enhanced ion fluxes observed at the equator occur without an increase in the total plasma density. Helium is occasionally found heated along with the protons, and forms about 10 percent of the equatorially trapped population at such times. The heated H(+) ions can be characterized by a bi-Maxwellian with kT(parallel) = 0.5-1.0 eV and kT = 5-50 eV, with a density of 10-100/cu cm. The total plasma density is relatively constant with latitude. First measurements of the equatorially trapped plasma and coincident UHR measurements show that the trapped plasma is found in conjunction with equatorial noise.
Document ID
19870049542
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Olsen, R. C.
(Alabama, University Huntsville, United States)
Shawhan, S. D.
(NASA Headquarters Washington, DC United States)
Gallagher, D. L.
(Alabama Univ. Huntsville, AL, United States)
Chappell, C. R.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Green, J. L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 13, 2013
Publication Date
March 1, 1987
Publication Information
Publication: Journal of Geophysical Research
Volume: 92
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
87A36816
Funding Number(s)
CONTRACT_GRANT: NSF ATM-83-00426
CONTRACT_GRANT: NAS5-28701
CONTRACT_GRANT: NAS8-33982
Distribution Limits
Public
Copyright
Other

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