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  Axi- to nonaxisymmetric dynamo transition in stellar models with varying rotation rate

Viviani, M., Cole-Kodicara, E., Käpylä, P. J., Käpylä, M. J., Olspert, N., & Warnecke, J. (2017). Axi- to nonaxisymmetric dynamo transition in stellar models with varying rotation rate. Talk presented at AG2017 The many Scales of Universe: Galaxies, theirs Suns and their Planets. Göttingen, Germany. 2017-09-18 - 2017-09-22.

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 Creators:
Viviani, M., Author
Cole-Kodicara, E., Author
Käpylä, P. J., Author
Käpylä, M. J.1, 2, Author           
Olspert, N., Author
Warnecke, J.2, Author           
Affiliations:
1Max Planck Research Group in Solar and Stellar Magnetic Activity, Max Planck Institute for Solar System Research, Max Planck Society, ou_2265638              
2Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              

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 Dates: 2017
 Publication Status: Not specified
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: BibTex Citekey: Viviani:2017-146P
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Title: AG2017 The many Scales of Universe: Galaxies, theirs Suns and their Planets
Place of Event: Göttingen, Germany
Start-/End Date: 2017-09-18 - 2017-09-22

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