作者: Dilyara Baklanova , Sergei Plachinda
DOI: 10.1016/J.ASR.2014.05.029
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摘要: Abstract The direct measurements of the meridional flow velocities on stars are impossible today. To evaluate solar-like with stable activity periods, we supposed that during stellar Hale cycle matter surfaces passes way equivalent to 2 π R ★ . We present here dependence mean velocity Rossby number, which is an effective parameter magnetic dynamo.