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

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.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0002-1862-5 Version Permalink: https://hdl.handle.net/21.11116/0000-0002-1863-4
Genre: Journal Article

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 Creators:
Viviani, M.1, 2, Author
Warnecke, Jörn1, 2, Author           
Käpylä, Maarit J.1, 2, Author           
Käpylä, P. J., Author
Olspert, N., Author
Cole-Kodikara, E. M., Author
Lehtinen, Jyri1, 2, 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, Max Planck Institute for Solar System Research, Max Planck Society, Justus-von-Liebig-Weg 3, 37077 Göttingen, DE, ou_2265638              

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Language(s): eng - English
 Dates: 2018-09-1720172018-04-232018
 Publication Status: Published online
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1051/0004-6361/201732191
 Degree: -

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Title: Astronomy and Astrophysics
  Other : Astron. Astrophys.
Source Genre: Journal
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Publ. Info: Berlin : Springer-Verlag
Pages: - Volume / Issue: 616 Sequence Number: A 160 Start / End Page: - Identifier: ISSN: 0004-6361
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219_1