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Coupling of the solar wind to measures of magnetic activityLinear prediction filtering was used to generate empirical response functions relating the solar wind electric field to the magnetic indices, AL, AU, Dst and ASYM. The empirical response functions were convolved with solar wind observations obtained during the International Magnetospheric Study to predict the indices. The predictions are compared with the observed indices during two, 3-day intervals. Differences between the observed and predicted indices are discussed in terms of the linear assumption and in terms of physical processes other than direct solar wind-magnetosphere interaction.
Document ID
19850016254
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Mcpherron, R. L.
(California Univ. Los Angeles, CA, United States)
Fay, R. A.
(California Univ. Los Angeles, CA, United States)
Garrity, C. R.
(California Univ. Los Angeles, CA, United States)
Bargatze, L. F.
(California Univ. Los Angeles, CA, United States)
Clauer, C. R.
(Stanford Univ. Albuquerque, New Mex., United States)
Searls, C.
(Sandia National Lab.)
Baker, D. N.
(LASL)
Date Acquired
August 12, 2013
Publication Date
September 1, 1984
Publication Information
Publication: ESA Achievements of the Intern. Magnetospheric Study (IMS)
Subject Category
Solar Physics
Accession Number
85N24565
Funding Number(s)
CONTRACT_GRANT: N000-14-C-0158
CONTRACT_GRANT: NSF ATM-83-18200
CONTRACT_GRANT: NGL-05-007-004
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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