
The influence of magnetic geometry on ion temperature gradient modes in the CFQS
Moshan Li, Jie Huang, Yuhong Xu, Akihiro Shimizu, Mitsutaka Isobe, Shoichi Okamura, Haifeng Liu, Xian-Qu Wang, Y Q Wu, X Zhang, et al.
A key feature of the stellarator is its inherent three-dimensional magnetic configuration, which leads to numerous differences in plasma physics between stellarators and tokamaks. The influence of this three-dimensional geometry on ion temperature gradient (ITG) modes in the Chinese First Quasi-axisymmetric Stellarator (CFQS) is investigated through linear gyrokinetic simulations using the gyrokinetic Vlasov (GKV) code. Across different radial and toroidal positions, the ITG mode exhibits a strong toroidal dependence and a weak radial dependence. The eigenmode localization is primarily determined by the perpendicular wavenumber k_{\perp }^{2} and the normal curvature {\kappa }_{y}: the ITG mode peaks where {\kappa }_{y} is negative and k_{\perp }^{2} is minimized. For ITG modes with k_{x}=0, the growth rate mainly exhibits a toroidal dependence. As the toroidal angle ϕ increases, the peak growth rate decreases and shifts to the low k_{y}{\rho }_{i} region. For modes with k_{x}\neq 0, the most unstable modes acquire a finite k_{x} at all three radial positions for \phi ={90}^{\circ }, and at ρ=0.8 for \phi ={45}^{\circ }. This finite k_{x} alters the value of k_{\perp }^{2} and modifies its distribution along the field line, thereby changing the eigenmode structure. By combining the eigenmode structure with the overall distributions of magnetic geometry parameters, the variation of the growth rate across different spatial positions can be qualitatively estimated.




