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

被引：0

作者：

Baklanova, Dilyara ^{[1
]}

Plachinda, Sergei ^{[1
]}

机构：

[1] Taras Shevchenko Natl Univ Kyiv, Crimean Astrophys Observ, UA-98409 Nauchnyi, Crimea, Ukraine

来源：

MAGNETIC FIELDS THROUGHOUT STELLAR EVOLUTION | 2014年 / 302期

关键词：

stars: late -type; stars: activity;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The direct measurements of the meridional flow velocities on stars are impossible today. We suppose that the matter on a surface of solar -like stars with stable activity period passes the way equal to 271-n during the stellar Hale cycle. We present here the dependence of meridional flow velocity on llossby number, which is an effective parameter of the stellar magnetic dynamo.

引用

页码：196 / 197

页数：2