Global gyrokinetic study of shaping effects on electromagnetic modes at NSTX aspect ratio with ad hoc parallel magnetic perturbation effects

Author:

Sharma A. Y.1ORCID,Cole M. D. J.1ORCID,Görler T.2ORCID,Chen Y.3ORCID,Hatch D. R.4ORCID,Guttenfelder W.1ORCID,Hager R.1ORCID,Sturdevant B. J.1ORCID,Ku S.1ORCID,Mishchenko A.5ORCID,Chang C. S.1ORCID

Affiliation:

1. Princeton Plasma Physics Laboratory, P.O. Box 451, Princeton, New Jersey 08543-0451, USA

2. Max Planck Institute for Plasma Physics, Boltzmannstr. 2, 85748 Garching, Germany

3. Department of Physics, University of Colorado at Boulder, 390 UCB, Boulder, Colorado 80309, USA

4. Institute for Fusion Studies, University of Texas at Austin, 1 University Station, C1500, Austin, Texas 78712, USA

5. Max Planck Institute for Plasma Physics, D-17491 Greifswald, Germany

Abstract

Plasma shaping may have a stronger effect on global turbulence in tight-aspect-ratio tokamaks than in conventional-aspect-ratio tokamaks due to the higher toroidicity and more acute poloidal asymmetry in the magnetic field. In addition, previous local gyrokinetic studies have shown that it is necessary to include parallel magnetic field perturbations in order to accurately compute growth rates of electromagnetic modes in tight-aspect-ratio tokamaks. In this work, the effects of elongation and triangularity on global, ion-scale, linear electromagnetic modes are studied at National Spherical Torus Experiment (NSTX) aspect ratio and high plasma β using the global gyrokinetic particle-in-cell code XGC. The effects of compressional magnetic perturbations are approximated via a well-known modification to the particle drifts that was developed for flux-tube simulations [Joiner et al., Phys. Plasmas 17, 072104 (2010)], without proof of its validity in a global simulation, with the gyrokinetic codes GENE and GEM being used for local verification and global cross-verification. Magnetic equilibria are re-constructed for each distinct plasma profile that is used. Coulomb collision effects are not considered. Within the limitations imposed by the present study, it is found that linear growth rates of electromagnetic modes (collisionless microtearing modes and kinetic ballooning modes) are significantly reduced in a high-elongation and high-triangularity NSTX-like geometry compared to a circular NSTX-like geometry. For example, growth rates of kinetic ballooning modes at high- β are reduced to the level of that of collisionless trapped electron modes.

Funder

U.S. Department of Energy

Publisher

AIP Publishing

Subject

Condensed Matter Physics

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