NASA NTRS · 20060036834
The Distant Tail Behavior During High Speed Solar Wind Streams and Magnetic Storms
Abstract
We 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.
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Ho, C. M., Tsurutani, B. T.. 1996-01-01. The Distant Tail Behavior During High Speed Solar Wind Streams and Magnetic Storms. https://ntrs.nasa.gov/citations/20060036834
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