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Test particle acceleration in resistive torsional fan magnetic reconnection using laboratory plasma parameters

Published online by Cambridge University Press:  10 December 2021

D.L. Chesny*
Affiliation:
SpaceWave, LLC, Satellite Beach, FL32937 OrangeWave Innovative Science, LLC, Moncks Corner, SC29461
N.B. Orange
Affiliation:
SpaceWave, LLC, Satellite Beach, FL32937 OrangeWave Innovative Science, LLC, Moncks Corner, SC29461 Etelman Observatory Research Center, University of the Virgin Islands, St. Thomas, USVI00802
K.W. Hatfield
Affiliation:
Department of Aerospace, Physics And Space Sciences, Florida Institute of Technology, Melbourne, FL32901
*
Email address for correspondence: [email protected]

Abstract

Particle acceleration via magnetic reconnection is a fundamental process in astrophysical plasmas. Experimental architectures are able to confirm a wide variety of particle dynamics following the two-dimensional Sweet–Parker model, but are limited in their reproduction of the fan-spine magnetic field topology about three-dimensional (3-D) null points. Specifically, there is not yet an experiment featuring driven 3-D torsional magnetic reconnection. To move in this direction, this paper expands on recent work toward the design of an experimental infrastructure for inducing 3-D torsional fan reconnection by predicting feasible particle acceleration profiles. Solutions to the steady-state, kinematic, resistive magnetohydrodynamic equations are used to numerically calculate particle trajectories from a localized resistivity profile using well-understood laboratory plasma parameters. We confine a thin, 10 eV helium sheath following the snowplough model into the region of this localized resistivity and find that it is accelerated to energies of ${\approx }2$ keV. This sheath is rapidly accelerated and focused along the spine axis propagating a few centimetres from the reconnection region. These dynamics suggest a novel architecture that may hold promise for future experiments studying solar coronal particle acceleration and for technology applications such as spacecraft propulsion.

Type
Research Article
Copyright
Copyright © The Author(s), 2021. Published by Cambridge University Press

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References

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