Abstract The direct measurements of the meridional flow velocities on stars are impossible today. To evaluate the meridional flow velocities on solar-like stars with stable activity periods, we supposed that during the stellar Hale cycle the matter on surfaces of stars passes the meridional way equivalent to 2 π R . We present here the dependence of the mean meridional flow velocity on Rossby number, which is an effective parameter of the stellar magnetic dynamo.


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    Title :

    Meridional flow velocities on solar-like stars with known activity cycles


    Contributors:

    Published in:

    Advances in Space Research ; 55 , 3 ; 817-821


    Publication date :

    2014-05-22


    Size :

    5 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English





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