Abstract
Ion-gyroradius-scale microinstabilities typically have a frequency comparable to the ion transit frequency. Due to the small electron-to-ion mass ratio and the large electron transit frequency, it is conventionally assumed that passing electrons respond adiabatically in ion-gyroradius-scale modes. However, in gyrokinetic simulations of ion-gyroradius-scale modes in axisymmetric toroidal magnetic fields, the nonadiabatic response of passing electrons can drive the mode, and generate fluctuations in narrow radial layers, which may have consequences for turbulent transport in a variety of circumstances. In flux tube simulations, in the ballooning representation, these instabilities reveal themselves as modes with extended tails. The small electron-to-ion mass ratio limit of linear gyrokinetics for electrostatic instabilities is presented, in axisymmetric toroidal magnetic geometry, including the nonadiabatic response of passing electrons and associated narrow radial layers. This theory reveals the existence of ion-gyroradius-scale modes driven solely by the nonadiabatic passing electron response, and recovers the usual ion-gyroradius-scale modes driven by the response of ions and trapped electrons, where the nonadiabatic response of passing electrons is small. The collisionless and collisional limits of the theory are considered, demonstrating parallels in structure and physical processes to neoclassical transport theory. By examining initial-value simulations of the fastest-growing eigenmodes, the predictions for mass-ratio scaling are tested and verified numerically for a range of collision frequencies. Insight from the small electron-to-ion mass ratio theory may lead to a computationally efficient treatment of extended modes.
Original language | English |
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Article number | 055004 |
Journal | Plasma Physics and Controlled Fusion |
Volume | 64 |
Issue number | 5 |
DOIs | |
State | Published - May 2022 |
Externally published | Yes |
Funding
The authors are grateful for productive discussions with N Christen, O Beeke, B Patel, J Maurino-Alperovich, S Trinczek, C M Roach, B F McMillan, A A Scheckochihin, W Dorland, J Ball, S Brunner, I Calvo, J M García Regaña, H Thienpondt, M Abazorius, J Ruiz Ruiz, D St-Onge, G Acton and V Hall-Chen. The simulations were performed using the GS2 branch https://bitbucket.org/gyrokinetics/gs2/branch/ms_pgelres , with the latest revision at the time of writing being commit ade5780. The GS2 input files used to perform the gyrokinetic simulations in this study are publicly available [], alongside scripts used to calculate the neoclassical transport coefficients. This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom Research and Training Programme 2014–2018 and 2019–2020 under Grant Agreement No. 633053, and from EPSRC (Grant Nos. EP/T012250/1 and EP/R034737/1). The views and opinions expressed herein do not necessarily reflect those of the European Commission. The authors acknowledge the use of the EUROfusion High Performance Computer (Marconi-Fusion) under Projects MULTEI and OXGK, ARCHER through the Plasma HEC Consortium EPSRC Grant Nos. EP/L000237/1 and EP/R029148/1 under the Projects e281-gs2 and e607, the JFRS-1 supercomputer at IFERC-CSC in Rokkasho Fusion Institute of QST (Aomori, Japan), and software support through the Plasma-CCP Network under EPSRC Grant No. EP/M022463/1.
Keywords
- electron response
- gyrokinetics
- magnetic confinement fusion
- microinstabilities
- turbulence