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Magnetic cloud induced magnetic storms: a lack of classical substorm expansion phasesThe purpose of this paper will be to examine a specific but important subset of magnetic storms, those that are caused by large southward, smoothly rotating magnetic fields: interplanetary magnetic clouds.
Document ID
20060031553
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/12830
Authors
Tsurutani, B. T.
Zhou, X. Y.
Gonzalez, W. D.
Date Acquired
August 23, 2013
Publication Date
May 15, 2001
Publication Information
Publication: Journal of Geophysical Research
Subject Category
Geophysics
Distribution Limits
Public
Copyright
Other
Keywords
magnetic storms substorm expansion phases

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