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IMF control of geomagnetic activityRecent work on the IMF control of geomagnetic activity is reviewed. The goal is to quantitatively express the temporal relation between the solar wind input and the ionospheric output from the magnetospheric system. Linear prediction filtering was used which treats the magnetosphere as a black box characterized by an impulse response. It is shown that an average impulse response can account for only about 40 percent of the variance in the AL index.
Document ID
19890046137
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mcpherron, R. L.
(California Univ. Los Angeles, CA, United States)
Bargatze, L. F.
(California Univ. Los Angeles, CA, United States)
Holzer, R. E.
(California, University Los Angeles, United States)
Baker, D. N.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Clauer, C. R.
(Stanford University CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Publication Information
Publication: Advances in Space Research
Volume: 8
Issue: 9-10
ISSN: 0273-1177
Subject Category
Geophysics
Report/Patent Number
ISSN: 0273-1177
Accession Number
89A33508
Funding Number(s)
CONTRACT_GRANT: NGL-05-007-004
CONTRACT_GRANT: NSF ATM-87-21904
CONTRACT_GRANT: N00014-85-K-0556
CONTRACT_GRANT: NOAA-40RANR708458
Distribution Limits
Public
Copyright
Other

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