Detection of slowly rotating n = 1 mode with signal compensation for an externally perturbed field in the KSTAR tokamak

Abstract A mode identification method for slowly rotating (or non-rotating) n (toroidal mode number) = 1 plasma instabilities has been newly established with the signal compensation method used for an external time-varying magnetic field. The mode identification method is based on the Fourier decomposition scheme and processes the signal of the magnetic probes (MPs) on the passive stabilizer in the Korea Superconducting Tokamak Advanced Research (KSTAR) tokamak. To exclude the non-plasma magnetic perturbation by the external current coils and their secondary eddy currents on the passive stabilizer that may not be easily characterized, the ARX-SISO (autoregressive with exogenous terms-single input single output) method has been introduced in the signal compensation process. Preliminary off-line analysis presented herein confirms that this method can adequately detect the time evolution of the mode-locking, along with a slowly rotating state, even in the presence of external magnetic perturbations.

[1]  A. Loarte,et al.  Enhanced understanding of non-axisymmetric intrinsic and controlled field impacts in tokamaks , 2017 .

[2]  S. Fietz,et al.  Influence of externally applied magnetic perturbations on neoclassical tearing modes at ASDEX Upgrade , 2014 .

[3]  H. L. Yang,et al.  Design features of the KSTAR in-vessel control coils , 2009 .

[4]  N C Logan,et al.  An upgrade of the magnetic diagnostic system of the DIII-D tokamak for non-axisymmetric measurements. , 2014, The Review of scientific instruments.

[5]  E. J. Strait,et al.  MHD limits to tokamak operation and their control , 2003 .

[6]  N. W. Eidietis,et al.  Progress and plan of KSTAR plasma control system upgrade , 2016 .

[7]  F. Volpe,et al.  Error field detection in DIII-D by magnetic steering of locked modes , 2014 .

[8]  D. A. Humphreys,et al.  An overview of KSTAR results , 2013 .

[9]  Faa Federico Felici,et al.  Development and validation of a tokamak skin effect transformer model , 2012 .

[10]  S. G. Lee,et al.  Diamagnetic loop measurement in Korea Superconducting Tokamak Advanced Research machine. , 2011, The Review of scientific instruments.

[11]  G. A. Navratil,et al.  Resistive wall stabilization of high-beta plasmas in DIII-D , 2002 .

[12]  Yuejin Tang,et al.  Development of the saddle loop sensors on the J-TEXT tokamak , 2017 .

[13]  S. G. Lee,et al.  Suppression of edge localized modes in high-confinement KSTAR plasmas by nonaxisymmetric magnetic perturbations. , 2012, Physical review letters.

[14]  N. W. Eidietis,et al.  Achievements and lessons learned from the operation of KSTAR plasma control system upgrade , 2018 .

[15]  Michio Okabayashi,et al.  Extremely low intrinsic non-axisymmetric field in KSTAR and its implications , 2015 .

[16]  R. Sweeney,et al.  Statistical analysis of m/n  =  2/1 locked and quasi-stationary modes with rotating precursors at DIII-D , 2016, 1606.04183.

[17]  M. Gryaznevich,et al.  Cross-machine comparison of resonant field amplification and resistive wall mode stabilization by plasma rotation , 2005 .

[18]  J. Ferreira,et al.  Effect of resonant magnetic perturbations on COMPASS-C tokamak discharges , 1992 .

[19]  Lennart Ljung,et al.  System Identification: Theory for the User , 1987 .

[20]  E. D. Fredrickson,et al.  β-Limiting MHD instabilities in improved-performance NSTX spherical torus plasmas , 2003 .

[21]  E. J. Strait,et al.  Magnetic diagnostic system of the DIII-D tokamak , 2006 .

[22]  N. J. Lopes Cardozo,et al.  Large amplitude quasi-stationary MHD modes in JET , 1988 .

[23]  E. J. Strait,et al.  MHD mode identification of tokamak plasmas from Mirnov signals , 1999 .

[24]  A. Boozer Error field amplification and rotation damping in tokamak plasmas. , 2001, Physical review letters.

[25]  Satoshi Konishi,et al.  DEMO plant design beyond ITER , 2002 .

[26]  J. G. Bak,et al.  Versatile controllability of non-axisymmetric magnetic perturbations in KSTAR experiments , 2015 .