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Tail plasma velocity

Tail plasma velocity

Date: 22 September 2005
Copyright: J. Raeder, Space Science Center & Department of Physics, University of New Hampshire

A cut at x=-7.5 RE shows how the plasma becomes increasingly stagnant. This animation is part (page 8) of the presentation "Cold Dense Plasma Sheet Formation During Northward IMF" given by J. Reader at the 2005 Cluster-Double Star symposium.
Last Update: 1 September 2019
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19-Apr-2024 02:01 UT

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