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Distant Tail Behavior During High Speed Solar Wind Streams and Magnetic StormsWe have examined the ISEE 3 distant tail data during three intense magnetic storms and have identified the tail response to high-speed solar wind streams, interplanetary magnetic clouds, and near-Earth storms.
Document ID
20060041678
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Ho, C. M.
Tsurutani, B. T.
Date Acquired
August 23, 2013
Publication Date
January 1, 1997
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
magnetic storms

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