A Spherical Plasma Dynamo Experiment
E. J. Spence, K. Reuter, and C. B. Forest

TL;DR
This paper proposes a plasma experiment to study astrophysical dynamos, enabling exploration of higher magnetic Reynolds numbers than liquid-metal experiments through simulations demonstrating dynamo action.
Contribution
It introduces a novel plasma experiment setup with simulations showing dynamo action at high magnetic Reynolds numbers, advancing astrophysical dynamo research.
Findings
Dynamo action observed at high magnetic Reynolds numbers in simulations.
Both laminar and turbulent dynamo regimes demonstrated.
Experiment design allows exploration of astrophysical magnetic phenomena.
Abstract
We propose a plasma experiment to be used to investigate fundamental properties of astrophysical dynamos. The highly conducting, fast-flowing plasma will allow experimenters to explore systems with magnetic Reynolds numbers an order of magnitude larger than those accessible with liquid-metal experiments. The plasma is confined using a ring-cusp strategy and subject to a toroidal differentially rotating outer boundary condition. As proof of principle, we present magnetohydrodynamic simulations of the proposed experiment. When a von K\'arm\'an-type boundary condition is specified, and the magnetic Reynolds number is large enough, dynamo action is observed. At different values of the magnetic Prandtl and Reynolds numbers the simulations demonstrate either laminar or turbulent dynamo action.
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