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Solar-like stars' models at increasing rotation rates: magnetic field, velocity field and helicities

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Viviani,  Mariangela
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Max Planck Research Group in Solar and Stellar Magnetic Activity (Mag Activity) – SOLSTAR, Max Planck Institute for Solar System Research, Max Planck Society;
IMPRS for Solar System Science at the University of Göttingen, Max Planck Institute for Solar System Research, Max Planck Society;

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Käpylä,  Maarit J.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Warnecke,  Jörn
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Viviani, M., Käpylä, M. J., Warnecke, J., Käpylä, P. J., Rheinhardt, M., & Brandenburg, A. (2019). Solar-like stars' models at increasing rotation rates: magnetic field, velocity field and helicities. Talk presented at Solar Helicities in Theory and Observations: Implications for Space Weather and Dynamo Theory. Stockholm, Schweden. 2019-03-04 - 2019-03-29.


Cite as: https://hdl.handle.net/21.11116/0000-0003-B632-7
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