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Weakly Magnetized, Hall Dominated Plasma Couette Flow

K. Flanagan, J. Milhone, J. Egedal, D. Endrizzi, J. Olson, E. E. Peterson, R. Sassella, and C. B. Forest
Phys. Rev. Lett. 125, 135001 – Published 25 September 2020
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Abstract

A novel plasma equilibrium in the high-β, Hall regime that produces centrally peaked, high Mach number Couette flow is described. Flow is driven using a weak, uniform magnetic field and large, cross field currents. Large magnetic field amplification (factor 20) due to the Hall effect is observed when electrons are flowing radially inward, and near perfect field expulsion is observed when the flow is reversed. A dynamic equilibrium is reached between the amplified (removed) field and extended density gradients.

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  • Received 16 June 2020
  • Revised 14 August 2020
  • Accepted 18 August 2020

DOI:https://doi.org/10.1103/PhysRevLett.125.135001

© 2020 American Physical Society

Physics Subject Headings (PhySH)

Plasma Physics

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Reproducing Space Plasma in the Lab

Published 25 September 2020

Electromagnetic fields rotate a plasma and produce conditions that resemble the region around a newly forming star.

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Authors & Affiliations

K. Flanagan1, J. Milhone1, J. Egedal1, D. Endrizzi1, J. Olson1, E. E. Peterson2, R. Sassella1, and C. B. Forest1

  • 1Department of Physics, University of Wisconsin–Madison, 1150 University Avenue, Madison, Wisconsin 53706, USA
  • 2Plasma Science and Fusion Center, Massachusetts Institute of Technology, NW17, 77 Massachusetts Avenue, Cambridge, Massachusetts 02139, USA

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Issue

Vol. 125, Iss. 13 — 25 September 2020

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