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Magnetic storm of September 4, 1984 - A synthesis of ring current spectra and energy densities measured with AMPTE/CCECompositional studies of the equatorial distributions of ring current ions during the September 4, 1984 magnetic storm have been made possible by comprehensive energy, charge state, and mass coverage data from the Charge Composition Explorer satellite. An examination of ion spectra at an L value of about 4 on September 5, in the local evening sector, shows that energy density was dominated by protons, with O ions contributing about 27 percent at the peak of about 150 keV, while He ions contributed less than about 2 percent. September 6 ion spectra, taken during the recovery phase of the storm, indicate that ion densities at more than 20 keV had decreased markedly, and that the ring current energy density was primarily provided by protons.
Document ID
19850052843
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Krimigis, S. M.
(Johns Hopkins Univ. Laurel, MD, United States)
Mcentire, R. W.
(Johns Hopkins University Laurel, MD, United States)
Potemra, T. A.
(Executive Office of the President, Office of Science and Technology, Washington, DC; Johns Hopkins University Laurel, MD, United States)
Gloeckler, G.
(Maryland, University College Park, MD, United States)
Scarf, F. L.
(TRW Inc. Defense and Space Systems Group, Redondo Beach, CA, United States)
Shelley, E. G.
(Lockheed Research Laboratories Palo Alto, CA, United States)
Date Acquired
August 12, 2013
Publication Date
May 1, 1985
Publication Information
Publication: Geophysical Research Letters
Volume: 12
ISSN: 0094-8276
Subject Category
Geophysics
Accession Number
85A34994
Funding Number(s)
CONTRACT_GRANT: N00024-83-C-5301
Distribution Limits
Public
Copyright
Other

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