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The Distant Tail Behavior During High Speed Solar Wind Streams and Magnetic StormsWe have examined the ISEE-3 distant tail data during three intense (Dst< -100(sub n)T) magnetic storms and have identified the tail response to high speed solar wind streams, interplanetary magnetic clouds, and near-Earth storms. The three storms have a peak Dst ranging from -150 to -220 nT, and occur on Jan. 9, Feb. 4, and Aug. 8, 1993.
Document ID
20060036834
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, 1996
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
ISEE-3 solar wind streams solar wind magnetic clouds near Earth storms