Transition from axi- to nonaxisymmetric dynamo modes in spherical convection 
models of solar-like stars

Viviani, M.; Warnecke, Jörn; Käpylä, Maarit J.; Käpylä, P. J.; Olspert, N.; Cole-Kodikara, E. M.; Lehtinen, Jyri; Brandenburg, A.

doi:10.1051/0004-6361/201732191

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Transition from axi- to nonaxisymmetric dynamo modes in spherical convection models of solar-like stars

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Viviani, M.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Max Planck Research Group in Solar and Stellar Magnetic Activity, 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;
Max Planck Research Group in Solar and Stellar Magnetic Activity, 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;
Max Planck Research Group in Solar and Stellar Magnetic Activity, Max Planck Institute for Solar System Research, Max Planck Society;

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Lehtinen, Jyri
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Max Planck Research Group in Solar and Stellar Magnetic Activity, Max Planck Institute for Solar System Research, Max Planck Society;

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Viviani, M., Warnecke, J., Käpylä, M. J., Käpylä, P. J., Olspert, N., Cole-Kodikara, E. M., et al. (2018). Transition from axi- to nonaxisymmetric dynamo modes in spherical convection models of solar-like stars. Astronomy and Astrophysics, 616: A 160. doi:10.1051/0004-6361/201732191.

Cite as: https://hdl.handle.net/21.11116/0000-0002-1862-5

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