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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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Item Permalink: http://hdl.handle.net/21.11116/0000-0003-B632-7 Version Permalink: http://hdl.handle.net/21.11116/0000-0003-B635-4
Genre: Talk

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 Creators:
Viviani, Mariangela1, 2, 3, Author              
Käpylä, Maarit J.1, Author              
Warnecke, Jörn1, Author              
Käpylä, P. J., Author
Rheinhardt, M., Author
Brandenburg, A., Author
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              

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Title: Solar Helicities in Theory and Observations: Implications for Space Weather and Dynamo Theory
Place of Event: Stockholm, Schweden
Start-/End Date: 2019-03-04 - 2019-03-29

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