Meridional flow velocities on solar-like stars with known activity cycles
arXiv:1406.2085 · doi:10.1016/j.asr.2014.05.029
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 . We present here the dependence of the mean meridional flow velocity on Rossby number, which is an effective parameter of the stellar magnetic dynamo.
arXiv commentAccepted for publication in Advances in Space Research
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