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Overview of results from the MST reversed field pinch experiment

Academic Article
Publication Date:
2015
abstract:
An overview of recent results from the MST reversed field pinch programme is presented. With neutral beam injection, bursty energetic particle (EP) modes are observed. The profiles of the magnetic and density fluctuations associated with these EP modes are measured using a far infrared interferometer-polarimeter. Equilibrium reconstructions of the quasi-single-helicity 3D helical state are provided by the V3FIT code that now incorporates several of MST's advanced diagnostics. The orientation of the helical structure is controlled using a new resonant magnetic perturbation technique. Gyrokinetic simulations based on experimental equilibria predict unstable trapped-electron modes (TEMs), and small-scale density fluctuations are detected in improved-confinement plasmas with TEM-like features. Upgraded pellet injection permits study of density and beta limits over MST's full range of operation, and an MST-record line-average density of 0.9 ×1020 m3 (n/nG = 1.4) has been obtained. Impurity ion temperature measurements reveal a charge-to-mass-ratio dependence in the rapid heating that occurs during a sawtooth crash. Runaway of NBI-born fast ions during the impulsive sawtooth event agrees with test-particle theory. Magnetic self-organization studies include measurements of the dynamo emf with an applied ac inductive electric field using oscillating field current drive.
Iris type:
01.01 Articolo in rivista
Keywords:
beta limit; density limit; energetic particles; gyrokinetics; Reversed field pinch; stellarator
List of contributors:
Martines, Emilio; Innocente, Paolo; Spolaore, Monica; Terranova, David; Piovesan, Paolo; Puiatti, MARIA ESTER; Cappello, Susanna
Authors of the University:
CAPPELLO SUSANNA
INNOCENTE PAOLO
SPOLAORE MONICA
TERRANOVA DAVID
Handle:
https://iris.cnr.it/handle/20.500.14243/337139
Published in:
NUCLEAR FUSION (ONLINE)
Journal
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URL

https://iopscience.iop.org/article/10.1088/0029-5515/55/10/104006
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