Plasmoids Formation During Simulations of Coaxial Helicity Injection in the National Spherical Torus Experiment

F. Ebrahimi and R. Raman
Phys. Rev. Lett. 114, 205003 – Published 20 May 2015
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Abstract

The formation of an elongated Sweet-Parker current sheet and a transition to plasmoid instability has for the first time been predicted by simulations in a large-scale toroidal fusion plasma in the absence of any preexisting instability. Plasmoid instability is demonstrated through resistive MHD simulations of transient coaxial helicity injection experiments in the National Spherical Torus Experiment (NSTX). Consistent with the theory, fundamental characteristics of the plasmoid instability, including fast reconnection rate, have been observed in these realistic simulations. Motivated by the simulations, experimental camera images have been revisited and suggest the existence of reconnecting plasmoids in NSTX. Global, system-size plasmoid formation observed here should also have strong implications for astrophysical reconnection, such as rapid eruptive solar events.

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  • Received 2 March 2015

DOI:https://doi.org/10.1103/PhysRevLett.114.205003

© 2015 American Physical Society

Authors & Affiliations

F. Ebrahimi1 and R. Raman2

  • 1Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08543, USA
  • 2University of Washington, Seattle, Washington 98195, USA

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Issue

Vol. 114, Iss. 20 — 22 May 2015

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