Plasma Flow Reversals in the Magnetotail and Their Implications on Substorm Models
DOI: 10.1007/978-90-481-3499-1_30
Bibcode: 2010ASSP...11..429L
Lui, A. T. Y.
United States
Abstract
Intervals of plasma flow reversals in the magnetotail are considered as times when the observing satellite encounters the process responsible for substorm disturbances. We consider the expected signatures during plasma flow reversals to evaluate the validity of two prevalent substorm models.
2010
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The Cluster Active Archive
Cluster
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