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Solar wind triggering of substorm expansion onsetA substantial fraction of all substorms with sudden onsets, as identified by minima in the AL index, are found to be triggered by the IMF. Analysis of data from the first six months of 1978 shows auroral zone magnetic records to be disturbed most of the time, with distinct substorms identified in 23 percent of these disturbed hours. For the subset of substorms with sharp onsets and corresponding solar wind data, 44 percent are found to be correlated with northward turnings of the IMF, while 28 percent occur during steady southward IMF. The results suggest that sharp substorm expansion onset is caused by a process internal to the magnetosphere which can be influenced by changes in the solar wind stress applied to the magnetosphere.
Document ID
19870047361
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mcpherron, R. L.
(Tokyo Univ. Japan)
Terasawa, T.
(Tokyo Univ. Japan)
Nishida, A.
(Tokyo, University Japan)
Date Acquired
August 13, 2013
Publication Date
January 1, 1986
Publication Information
Publication: Journal of Geomagnetism and Geoelectricity
Volume: 38
Issue: 11 1
ISSN: 0022-1392
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0022-1392
Accession Number
87A34635
Funding Number(s)
CONTRACT_GRANT: N00014-84-C-0158
CONTRACT_GRANT: NSF ATM-83-18200
CONTRACT_GRANT: NGL-05-007-004
Distribution Limits
Public
Copyright
Other

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