| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1764193 | Advances in Space Research | 2015 | 5 Pages |
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 2πR★2πR★. We present here the dependence of the mean meridional flow velocity on Rossby number, which is an effective parameter of the stellar magnetic dynamo.
Keywords
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Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Dilyara Baklanova, Sergei Plachinda,