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The New Mexico alpha-omega Dynamo Experiment: Modeling Astrophysical Dynamos

S. A. Colgate·V. I. Pariev·H. F. Beckley·R. Ferrel·V. D. Romero·J. C. Weatherall
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Abstract

A magnetic dynamo experiment is under construction at the New Mexico Institute of Mining and Technology. The experiment is designed to demonstrate in the laboratory the alpha-omega magnetic dynamo, which is believed to operate in many rotating and conducting astrophysical objects. The experiment uses the Couette flow of liquid sodium between two cylinders rotating with different angular velocities to model the omega-effect. The alpha-effect is created by the rising and expanding jets of liquid sodium driven through a pair of orifices in the end plates of the cylindrical vessel, presumably simulating plumes driven by buoyancy in astrophysical objects. The water analog of the dynamo device has been constructed and the flow necessary for the dynamo has been demonstrated. Results of the numerical simulations of the kinematic dynamo are presented. The toroidal field produced by the omega-effect is predicted to be B_ϕ \simeq (R_m/2π) B_{poloidal}\simeq 20 \times B_{poloidal} for the expected magnetic Reynolds number of R_m \sim 120. The critical rate of jets necessary for the dynamo self-excitation is predicted from the calculations to be a pair of plumes every 4 revolutions of the outer cylinder. For reasonable technical limitations on the strength of materials and the power of the drive, the self-excitation of the dynamo appears to be feasible.

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S. A. Colgate, V. I. Pariev, H. F. Beckley, R. Ferrel, V. D. Romero, J. C. Weatherall. 2001-12-25. The New Mexico alpha-omega Dynamo Experiment: Modeling Astrophysical Dynamos. https://arxiv.org/abs/astro-ph/0112541

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