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Interaction of MRI and other sources of turbulence and what does it mean for galactic dynamo

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

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Käpylä, M. J. (2016). Interaction of MRI and other sources of turbulence and what does it mean for galactic dynamo. Talk presented at Max Planck Princeton Center for Plasma Physics Meeting. Princeton, USA. 2016-12-05 - 2016-12-09.


Cite as: https://hdl.handle.net/21.11116/0000-0000-D859-9
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