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

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.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0000-D859-9 Version Permalink: http://hdl.handle.net/21.11116/0000-0001-F0A7-3
Genre: Talk

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Käpylä, M. J.1, 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: 2016
 Publication Status: Not specified
 Pages: -
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 Identifiers: BibTex Citekey: Kapyla:2016-248P
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Title: Max Planck Princeton Center for Plasma Physics Meeting
Place of Event: Princeton, USA
Start-/End Date: 2016-12-05 - 2016-12-09

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