2020
DOI: 10.1063/5.0008778
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Multi-scale multi-mode nonlinear interaction in tokamak plasma turbulence with moderate small-scale shear flow

Abstract: Effects of moderate small-scale shear flow, e.g., which may be created by the trapped electron mode, on electromagnetic (EM) ion-scale turbulence in tokamak plasmas are numerically investigated via a self-consistent Landau-fluid model. A modeling analysis is carried out in slab geometry to reveal the underlying mechanism of the multi-scale multi-mode nonlinear interaction. Results show that while a Kelvin–Helmholtz (KH) instability with long wavelengths may be excited by the shear flows to dominate the multi-s… Show more

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Cited by 4 publications
(10 citation statements)
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“…[36,37] This can also consistently capture the excitation of secondary KH mode when the flow shear is larger than the stability threshold. [35] The highly complex nonlinear interaction dynamics of cross-scale turbulence with ITG as well as KH modes are governed by normalized evolution equations of perturbed density n, the vorticity ∇ 2 ⊥ φ , parallel ion velocity υ , magnetic flux ψ (corresponding to the parallel vector potential through A = −ψ), as well as ion temperature T i as follows:…”
Section: Physical Model and Simulation Settingmentioning
confidence: 99%
See 3 more Smart Citations
“…[36,37] This can also consistently capture the excitation of secondary KH mode when the flow shear is larger than the stability threshold. [35] The highly complex nonlinear interaction dynamics of cross-scale turbulence with ITG as well as KH modes are governed by normalized evolution equations of perturbed density n, the vorticity ∇ 2 ⊥ φ , parallel ion velocity υ , magnetic flux ψ (corresponding to the parallel vector potential through A = −ψ), as well as ion temperature T i as follows:…”
Section: Physical Model and Simulation Settingmentioning
confidence: 99%
“…The normalizations are expressed as usual. [35] The code has been well checked for the convergency with enough high resolutions in radial real space and mode number spectral space. Other main parameters used in simulations are λ = 1.5, ŝ = 0.1 and the classical cross-field dissipations are set as D U = D n = η ⊥ = χ ⊥ = 0.01 which are included to damp smaller-scale fluctuations.…”
Section: Physical Model and Simulation Settingmentioning
confidence: 99%
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“…In additional, several physical effects, including the collisions, magnetic shear, finite β and finite Larmor radius effects [26][27][28][29][30][31][32] and other plasma parameters are considered as well. Furthermore, the turbulent transport is determined by the type of micro-turbulence [33,34] and it has been illustrated in the experiments, theories and simulations. Additional, transitions of turbulence in plasma density limits were discussed.…”
Section: Introductionmentioning
confidence: 99%