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

Käpylä, M. J.

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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: https://hdl.handle.net/21.11116/0000-0000-D859-9 Version Permalink: https://hdl.handle.net/21.11116/0000-0001-F0A7-3

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Käpylä, M. J.^{1, 2}, Author

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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: Created: 2016

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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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