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Some initial ISEE-1 results on the ring current composition and dynamics during the magnetics storm of December 11, 1977On December 11, 1977 the ISEE-1 spacecraft traversed the equatorial magnetosphere in the prenoon and dawn sectors during the early recovery phase of a magnetic storm with peak DST of -125 gamma. Along the dayside leg O(+) was comparable to or exceeded H(+) in number density in the energy range 0.1-17 keV. The velocity distribution of O(+) showed a characteristic dispersion, consistent with the ions being transported to the dayside from the dusk to midnight sector. The high-energy slope of the H(+) and O(+) distribution functions showed different radial dependence, with the slope of H(+) being consistent with a harder component carrying most of the energy density.
Document ID
19790057277
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lennartsson, W.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Shelley, E. G.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Sharp, R. D.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Johnson, R. G.
(Lockheed Research Laboratories Palo Alto, Calif., United States)
Balsiger, H.
(Bern, Universitaet Berne, Switzerland)
Date Acquired
August 9, 2013
Publication Date
June 1, 1979
Publication Information
Publication: Geophysical Research Letters
Volume: 6
Subject Category
Geophysics
Accession Number
79A41290
Funding Number(s)
CONTRACT_GRANT: NAS5-20538
CONTRACT_GRANT: SNSF-2,886,77
Distribution Limits
Public
Copyright
Other

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