Abstract
In magnetic confinement fusion devices, the ratio of the plasma pressure to the magnetic field energy, β, can become sufficiently large that electromagnetic microinstabilities become unstable, driving turbulence that distorts or reconnects the equilibrium magnetic field. In this paper, a theory is proposed for electromagnetic, electron-driven linear instabilities that have current layers localised to mode-rational surfaces and binormal wavelengths comparable to the ion gyroradius. The model retains axisymmetric toroidal geometry with arbitrary shaping, and consists of orbit-averaged equations for the mode-rational surface layer, with a ballooning space kinetic matching condition for passing electrons. The matching condition connects the current layer to the large scale electromagnetic fluctuations, and is derived in the limit that β is comparable to the square root of the electron-to-ion-mass ratio. Electromagnetic fluctuations only enter through the matching condition, allowing for the identification of an effective β that includes the effects of equilibrium flux surface shaping. The scaling predictions made by the asymptotic theory are tested with comparisons to results from linear simulations of micro-tearing and electrostatic microinstabilities in MAST discharge #6252, showing excellent agreement. In particular, it is demonstrated that the effective β can explain the dependence of the local micro-tearing mode (MTM) growth rate on the ballooning parameter θ 0-possibly providing a route to optimise local flux surfaces for reduced MTM-driven transport.
Original language | English |
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Article number | 045011 |
Journal | Plasma Physics and Controlled Fusion |
Volume | 65 |
Issue number | 4 |
DOIs | |
State | Published - Apr 2023 |
Externally published | Yes |
Funding
The authors are grateful for productive discussions with T Adkins, A A Schekochihin, A Zocco, P Helander, J Larakers, D Kennedy, R Gaur, M Anastopoulos-Tzanis, J Maurino-Alperovich, S Trinczek and G Acton. This work has received funding from EPSRC (Grant No. EP/R034737/1). This work was supported by the U.S. Department of Energy under contract number DE-AC02-09CH11466. The United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. The author acknowledges the use of the EUROfusion High Performance Computer (Marconi-Fusion) under projects OXGK and MULTISCA. This work made use of computational support by CoSeC, the Computational Science Centre for Research Communities, through CCP Plasma (EP/M022463/1) and HEC Plasma (EP/R029148/1). The simulations were performed using the GS2 branch https://bitbucket.org/gyrokinetics/gs2/branch/ms_pgelres , with commit ade5780. The GS2 input files used to perform the gyrokinetic simulations in this study are publicly available []. The authors are grateful for productive discussions with T Adkins, A A Schekochihin, A Zocco, P Helander, J Larakers, D Kennedy, R Gaur, M Anastopoulos-Tzanis, J Maurino-Alperovich, S Trinczek and G Acton. This work has received funding from EPSRC (Grant No. EP/R034737/1). This work was supported by the U.S. Department of Energy under contract number DE-AC02-09CH11466. The United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. The author acknowledges the use of the EUROfusion High Performance Computer (Marconi-Fusion) under projects OXGK and MULTISCA. This work made use of computational support by CoSeC, the Computational Science Centre for Research Communities, through CCP Plasma (EP/M022463/1) and HEC Plasma (EP/R029148/1). The simulations were performed using the GS2 branch https://bitbucket.org/gyrokinetics/gs2/branch/ms_pgelres, with commit ade5780. The GS2 input files used to perform the gyrokinetic simulations in this study are publicly available [46].
Funders | Funder number |
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MULTISCA | |
U.S. Department of Energy | DE-AC02-09CH11466, EP/M022463/1 |
Engineering and Physical Sciences Research Council | EP/R034737/1 |
Higher Education Commission, Pakistan | EP/R029148/1 |
Keywords
- electromagnetic microinstabilities
- electron physics
- gyrokinetics
- microtearing