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.


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    Title :

    Plasma Flow Reversals in the Magnetotail and Their Implications on Substorm Models


    Contributors:


    Publication date :

    2009-10-30


    Size :

    6 pages





    Type of media :

    Article/Chapter (Book)


    Type of material :

    Electronic Resource


    Language :

    English




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