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The Distant Tail Behavior During High Speed Solar Wind Streams and Magnetic Storms

The Distant Tail Behavior During High Speed Solar Wind Streams and Magnetic Storms

Ho, C. M.; Tsurutani, B. T.
URI: http://hdl.handle.net/2014/27744
Date: 1996

Abstract:

We have examined the ISEE-3 distant tail data during three intense (Dst< -100<sub>n</sub>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.

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