Nonlinear modeling of the effect of n = 2 resonant magnetic field perturbation on peeling-ballooning modes in KSTAR

S. K. Kim, S. Pamela, O. Kwon, M. Becoulet, G.T.A. Huijsmans, Y. In, M. Hoelzl, J. H. Lee, M. Kim, G. Y. Park, H. S. Kim, Y. H. Lee, G. J. Choi, C. Y. Lee, A. Kirk, A. Thornton, Y. S. Na (Corresponding author)

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16 Citaten (Scopus)

Samenvatting

Using the nonlinear 3D MHD code JOREK with reduced MHD equations (visco-resistive MHD), we have successfully simulated a recent n = 2 resonant magnetic perturbation (RMP)- driven edge localized mode (ELM) suppression in KSTAR. We have found that such ELM suppression has been attributable not only to the degraded pedestal but also to the direct coupling between the peeling-ballooning mode (PBM) and RMP-driven plasma response. Notably, the pedestal pressure gradient is reduced as the radial transport is enhanced because of the formation of the stochastic layer and increased convection fluxes due to tearing and the kink-peeling mode driven by RMPs. The increased transport in the stochastic layer is due to the parallel transport across the stochastic fields, described by the Braginskii model in the simulation. While the linear stability of the PBM improves owing to the degraded pedestal, it is not a sole contributor to ELM suppression, in that the nonlinear mode coupling plays a more critical role. This outcome is consistent with previous studies where mode coupling affects the ELM mitigation or suppression. In addition, PBM locking has been numerically achieved during the ELM suppression phase, which may support the relationship between VE×B ≈ 0 at the pedestal and the onset of ELM suppression. We suggest that PBM locking can enhance the mode interactions between RMPs and PBMs, which is significant for ELM suppression.

Originele taal-2Engels
Artikelnummer026009
TijdschriftNuclear Fusion
Volume60
Nummer van het tijdschrift2
DOI's
StatusGepubliceerd - feb. 2020

Financiering

The first author would like to express the deepest gratitude to the Plasma Laboratory for Advanced REsearch (PLARE) Team at Seoul National University for their kind support and fruitful discussions for this paper. This work was supported by the National R&D Program through the National Research Foundation of Korea (NRF), funded by the Ministry of Science, ICT & Future Planning (No. 2019-M1A7A1A03089798) and the R&D Program (Code No. CN-1901) through the National Fusion Research Institute of Korea (NFRI) funded by Government funds. The authors are thankful to The Research Institute of Energy and Resources, Seoul National University. The opinions included herein do not reflect those of the National Research Foundation of Korea.

FinanciersFinanciernummer
National Fusion Research Institute of Korea
Plasma Laboratory for Advanced REsearch
Research Institute of Energy and Resources
Horizon 2020 Framework Programme633053
Seoul National University
Ministry of Science, ICT and Future PlanningCN-1901, 2019-M1A7A1A03089798
National Research Foundation of Korea

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