Please use this identifier to cite or link to this item: https://hdl.handle.net/10356/178510
Title: A validation study of a bounce-averaged kinetic electron model in a KSTAR L-mode plasma
Authors: Yi, Sumin
Sung, C.
Yoon, Eisung
Kwon, Jae-Min
Hahm, T. S.
Kim, Daewoong
Kang, Jisung
Seo, Janghoon
Cho, Y. W.
Qi, Lei
Keywords: Physics
Issue Date: 2024
Source: Yi, S., Sung, C., Yoon, E., Kwon, J., Hahm, T. S., Kim, D., Kang, J., Seo, J., Cho, Y. W. & Qi, L. (2024). A validation study of a bounce-averaged kinetic electron model in a KSTAR L-mode plasma. Physics of Plasmas, 31(2), 022307-. https://dx.doi.org/10.1063/5.0178350
Journal: Physics of Plasmas 
Abstract: We extend the bounce-averaged kinetic (BK) electron model to be applicable in general tokamak magnetic geometries and implement it on the global δf particle-in-cell gyrokinetic code gKPSP. We perform a benchmark study of the updated BK model against the gyrokinetic electron model in flux-tube codes, CGYRO and GENE. From the comparisons among the simulations based on the local parameters of a KSTAR L-mode plasma, we confirm a reasonable agreement among the linear results from the different codes. In the nonlinear gKPSP simulation with a narrow plasma gradient region whose width comparable to the mode correlation length, ion and electron heat fluxes are compatible with those calculated by CGYRO. However, with an unstable region sufficiently wider than the mode correlation length, gKPSP predicts 2-3 times larger turbulent heat fluxes. Taking into account the differences between the flux-tube and global simulations, the overall agreement is encouraging for further validation and development of the BK electron model. In global simulations using a wide range of the experimental plasma profiles, we find an intricate coupling of turbulence spreading and a zonal flow in determining the radial profiles of turbulent heat fluxes, which has not been reported to date.
URI: https://hdl.handle.net/10356/178510
ISSN: 1070-664X
DOI: 10.1063/5.0178350
Schools: School of Physical and Mathematical Sciences 
Rights: © 2024 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution-NonCommercial-NoDerivs 4.0 International (CC BY-NC-ND) license (http://creativecommons.org/licenses/by-nc-nd/4.0/).
Fulltext Permission: open
Fulltext Availability: With Fulltext
Appears in Collections:SPMS Journal Articles

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