Understanding dynamo mechanisms from 3D convection simulations of the Sun

Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhardt, M.; Brandenburg, A.

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Understanding dynamo mechanisms from 3D convection simulations of the Sun

Warnecke, J., Käpylä, P. J., Käpylä, M. J., Rheinhardt, M., & Brandenburg, A. (2016). Understanding dynamo mechanisms from 3D convection simulations of the Sun. Talk presented at MHD Days. Göttingen, Germany. 2016-11-30 - 2016-12-02.

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Datensatz-Permalink: https://hdl.handle.net/21.11116/0000-0000-D7B7-F Versions-Permalink: https://hdl.handle.net/21.11116/0000-0001-EF22-C

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Urheber:
Warnecke, J.¹, Autor
Käpylä, P. J., Autor
Käpylä, M. J.^{1, 2}, 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, Max Planck Institute for Solar System Research, Max Planck Society, ou_2265638