Understanding dynamo mechanisms from 3D convection simulations of the Sun

Warnecke, Jörn; Käpylä, Petri J.; Käpylä, Maarit J.; Rheinhard, Matthias; Brandenburg, Axel

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Understanding dynamo mechanisms from 3D convection simulations of the Sun

Warnecke, J., Käpylä, P. J., Käpylä, M. J., Rheinhard, M., & Brandenburg, A. (2017). Understanding dynamo mechanisms from 3D convection simulations of the Sun. Talk presented at SOLARNET IV Meeting: The Physics of the Sun from the Interior to the Outer Atmosphere. Lanzarote, Spain. 2017-01-16 - 2017-01-20.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0000-D92A-D Version Permalink: https://hdl.handle.net/21.11116/0000-0001-9205-4

Genre: Talk

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Creators:
Warnecke, Jörn¹, Author
Käpylä, Petri J., Author
Käpylä, Maarit J.^{1, 2}, Author
Rheinhard, Matthias, Author
Brandenburg, Axel, 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, ou_2265638

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MPIS_GROUPS: Sun and Heliosphere

MPIS_GROUPS: Research Group Solar Stellar Mag Activity

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Dates: Created: 2017

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Identifiers: BibTex Citekey: Warnecke:2017-022P

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Title: SOLARNET IV Meeting: The Physics of the Sun from the Interior to the Outer Atmosphere.

Place of Event: Lanzarote, Spain

Start-/End Date: 2017-01-16 - 2017-01-20

Invited: Yes

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