The DRESDYN project: liquid metal experiments on dynamo action and magnetorotational instability

Magnetic fields of planets, stars and galaxies are generated by self-excitation in moving electrically conducting fluids. Once produced, magnetic fields can play an active role in cosmic structure formation by destabilising rotational flows that would be otherwise hydrodynamically stable. For a long...

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Published inGeophysical and astrophysical fluid dynamics Vol. 113; no. 1-2; pp. 51 - 70
Main Authors Stefani, F., Gailitis, A., Gerbeth, G., Giesecke, A., Gundrum, Th, Rüdiger, G., Seilmayer, M., Vogt, T.
Format Journal Article
LanguageEnglish
Published Abingdon Taylor & Francis 04.03.2019
Taylor & Francis Ltd
Subjects
Conducting fluids
Dynamo
Experiments
Fluid flow
Fluids
Galaxies
instabilities
Instability
Liquid sodium
Magnetic field
Magnetic fields
Metals
Planets
Sodium
Stellar magnetic fields
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Abstract Magnetic fields of planets, stars and galaxies are generated by self-excitation in moving electrically conducting fluids. Once produced, magnetic fields can play an active role in cosmic structure formation by destabilising rotational flows that would be otherwise hydrodynamically stable. For a long time, both hydromagnetic dynamo action as well as magnetically triggered flow instabilities had been the subject of purely theoretical research. Meanwhile, however, the dynamo effect has been observed in large-scale liquid sodium experiments in Riga, Karlsruhe and Cadarache. In this paper, we summarise the results of liquid metal experiments devoted to the dynamo effect and various magnetic instabilities such as the helical and the azimuthal magnetorotational instability and the Tayler instability. We discuss in detail our plans for a precession-driven dynamo experiment and a large-scale Tayler-Couette experiment using liquid sodium, and on the prospects to observe magnetically triggered instabilities of flows with positive shear.
AbstractList Magnetic fields of planets, stars and galaxies are generated by self-excitation in moving electrically conducting fluids. Once produced, magnetic fields can play an active role in cosmic structure formation by destabilising rotational flows that would be otherwise hydrodynamically stable. For a long time, both hydromagnetic dynamo action as well as magnetically triggered flow instabilities had been the subject of purely theoretical research. Meanwhile, however, the dynamo effect has been observed in large-scale liquid sodium experiments in Riga, Karlsruhe and Cadarache. In this paper, we summarise the results of liquid metal experiments devoted to the dynamo effect and various magnetic instabilities such as the helical and the azimuthal magnetorotational instability and the Tayler instability. We discuss in detail our plans for a precession-driven dynamo experiment and a large-scale Tayler-Couette experiment using liquid sodium, and on the prospects to observe magnetically triggered instabilities of flows with positive shear.
Author Gundrum, Th
Stefani, F.
Seilmayer, M.
Vogt, T.
Rüdiger, G.
Giesecke, A.
Gailitis, A.
Gerbeth, G.
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  organization: Helmholtz-Zentrum Dresden-Rossendorf
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  publication-title: Magnetohydrodynamics
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Snippet Magnetic fields of planets, stars and galaxies are generated by self-excitation in moving electrically conducting fluids. Once produced, magnetic fields can...
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SubjectTerms Conducting fluids
Dynamo
Experiments
Fluid flow
Fluids
Galaxies
instabilities
Instability
Liquid sodium
Magnetic field
Magnetic fields
Metals
Planets
Sodium
Stellar magnetic fields
Title The DRESDYN project: liquid metal experiments on dynamo action and magnetorotational instability
URI https://www.tandfonline.com/doi/abs/10.1080/03091929.2018.1501481
https://www.proquest.com/docview/2223826061
Volume 113
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