Study of the Alfven eigenmodes stability in CFQS plasma using a Landau closure model

J. Varela, A. Shimizu, D. A. Spong, L. Garcia, Y. Ghai

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Abstract

The aim of this study is to analyze the stability of the Alfven eigenmodes (AE) in the Chinese First Quasi-axisymmetric Stellarator (CFQS). The AE stability is calculated using the code FAR3d that solves the reduced MHD equations to describe the linear evolution of the poloidal flux and the toroidal component of the vorticity in a full 3D system, coupled with equations of density and parallel velocity moment for the energetic particles (EP) species including the effect of the helical couplings and acoustic modes. The Landau damping and resonant destabilization effects are added in the model by a given closure relation. The simulation results indicate the destabilization of n = 1 to 4 AEs by EP during the slowing down process, particularly n = 1 and n = 2 toroidal AEs (TAE), n = 3 elliptical AE (EAE) and n = 4 non circular AE (NAE). If the resonance is caused by EPs with an energy above 17 keV (weakly thermalized EP), n = 2 EAEs and n = 3 NAEs are unstable. On the other hand, EPs with an energy below 17 keV (late thermalization stage) lead to the destabilization of n = 3 and n = 4 TAEs. The simulations for an off-axis NBI injection indicate the further destabilization of n = 2 to 4 AEs although the growth rate of the n = 1 AEs slightly decreases, so no clear optimization trend with respect to the NBI deposition region is identified. In addition, n = 2, 4 helical AE (HAE) are unstable above an EP β threshold. Also, if the thermal β of the simulation increases (higher thermal plasma density) the AE stability of the plasma improves. The simulations including the effect of the finite Larmor radius and electron-ion Landau damping show the stabilization of the n = 1 to 4 EAE/NAEs as well as a decrease of the growth rate and frequency of the n = 1 to 4 BAE/TAEs.

Original languageEnglish
Article number026023
JournalNuclear Fusion
Volume61
Issue number2
DOIs
StatePublished - Feb 2021

Funding

The authors would like to thank CFQS and LHD technical staff for their contributions. This work was supported by NIFS07KLPH004 and the project 2019-T1/AMB-13648 founded by the Comunidad de Madrid. Data available on request from the authors. The authors also want to acknowledge K.Y. Watanabe for fruitful discussion.

FundersFunder number
NIFS07KLPH0042019-T1/AMB-13648
Comunidad de Madrid

    Keywords

    • Alfven modes
    • CFQS
    • Energetic particles
    • MHD
    • Stellarator

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