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

Viviani, Mariangela; Käpylä, Maarit J.; Warnecke, Jörn; Käpylä, P. J.; Rheinhardt, M.; Brandenburg, A.

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

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.

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Datensatz-Permalink: https://hdl.handle.net/21.11116/0000-0003-B632-7 Versions-Permalink: https://hdl.handle.net/21.11116/0000-0003-B635-4

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Viviani, Mariangela^{1, 2, 3}, Autor
Käpylä, Maarit J.¹, Autor
Warnecke, Jörn¹, Autor
Käpylä, P. J., Autor
Rheinhardt, M., Autor
Brandenburg, A., Autor

Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289
2Max Planck Research Group in Solar and Stellar Magnetic Activity (Mag Activity) – SOLSTAR, Max Planck Institute for Solar System Research, Max Planck Society, Justus-von-Liebig-Weg 3, 37077 Göttingen, DE, ou_2265638
3IMPRS for Solar System Science at the University of Göttingen, Max Planck Institute for Solar System Research, Max Planck Society, Justus-von-Liebig-Weg 3, 37077 Göttingen, DE, ou_1832290