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\pi R_\star. We present here the dependence of the mean meridional flow velocity on Rossby number, which is an effective parameter of the stellar magnetic dynamo.
Meridional flow velocities on solar-like stars with known activity cycles
Advances in space research ; 55 , 3 ; 817-821
2015
Aufsatz (Zeitschrift)
Englisch
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