Bulletin of the American Physical Society
63rd Annual Meeting of the APS Division of Plasma Physics
Volume 66, Number 13
Monday–Friday, November 8–12, 2021; Pittsburgh, PA
Session BP11: Poster Session I:
BEAMS - Coherent radiation and intense laser-driven x-ray sources; Laser-plasma ion accelerators; Relativistic high-energy-density physics and high field physics
MFE - Low Aspect Ratio Tokamaks
9:30 AM - 12:30 PM
Monday, November 8, 2021
Room: Hall A
Abstract: BP11.00032 : Low frequency MHD activity in NSTX and NSTX-U discharges*
Presenter:
Stefano Munaretto
(Princeton Plasma Physics Laboratory)
Authors:
Stefano Munaretto
(Princeton Plasma Physics Laboratory)
Devon J Battaglia
(Princeton Plasma Physics Laboratory)
Nathaniel M Ferraro
(Princeton Plasma Physics Laboratory)
Stefan P Gerhardt
(Princeton Plasma Physics Laboratory)
Walter Guttenfelder
(Princeton Plasma Physics Laboratory)
Jong-Kyu Park
(Princeton Plasma Physics Laboratory)
Zhirui Wang
(Princeton Plasma Physics Laboratory)
Important performance limiting instability mechanisms in the NSTX spherical tokamak are often linked to low frequency and low toroidal periodicity (n) MHD activity. n=1 modes are quite common in long pulse NSTX plasmas. They have both a core kink component and a tearing component and they have been observed to deleteriously impact performance over a wide range of q95. Such modes can be triggered by edge localized modes (ELMs), energetic particles modes (EPMs) or grow from small amplitudes. Most of their dynamics is typical of the neoclassical tearing modes (NTM), but they also have a clear 1/1 component, which can be ideally unstable, and may account for the observed mode onset in the absence of an observable trigger. The presence of similar n=1 core kink/tearing modes was also observed in NSTX-U. In addition, M3D-C1 simulations suggest that observed low frequency, low-n MHD activity may flatten core temperature profiles via a soft-beta limit. A comparison of the NSTX-U and NSTX low frequency and low n MHD characteristics will be presented as well as predictions made with the resistive DCON code to identify regions of global and tearing stability for NSTX-U.
*Work supported by US DOE under DE-AC02-09CH11466
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