Kinetic Stress and Particle Transport by Stochastic Fields and Turbulence
ORAL
Abstract
It is general wisdom that stochastic magnetic fields affect the electron heat transport in a tokamak. In the L-H transition, with resonant magnetic perturbation (RMP), the transport of ion heat, particles, toroidal momentum can also be influenced by stochastic fields due to RMP. A well-known model from Finn et al. discussed how toroidal flow is affected under the influence of stochastic fields. However, they merely have an Elsässer-like variable of parallel rotation and particle density—no explicit momentum and particle density transport presented. Moreover, they didn’t mention the kinetic stress which is critical in toroidal flow damping.
We propose a model to analytically derive the toroidal momentum transport and particle transport—we calculate the real diffusivity of particle and parallel momentum. Also, the physics of kinetic stress (K) and compressible heat, which play important roles in momentum and particle evolution, are further analyzed. We address this magnetic geometry effect to understand this “tail wagging the dog” feedback. Besides recovering the effective diffusivity Deff = CsDM in ‘stochastic field regime’, where Cs is sound speed and DM is the familiar stochastic field diffusivity of Rosenbluth et al., we obtain a hybrid turbulent viscosity Dν = Cs2Σk |bx,k |2 /k⊥DT in ‘strong turbulent regime’ such that Κ=-Dν ∂x〈uz〉, where DT is turbulent fluid diffusivity. This indicates that the actual diffusivity Dν describes how the mean flow is scattered perpendicularly by the synergy of stochastic fields and the strongly turbulent flow. Finally, there are several implications of those results for the physics of the kinetic stress and toroidal rotation. Discussions of these will be presented.
We propose a model to analytically derive the toroidal momentum transport and particle transport—we calculate the real diffusivity of particle and parallel momentum. Also, the physics of kinetic stress (K) and compressible heat, which play important roles in momentum and particle evolution, are further analyzed. We address this magnetic geometry effect to understand this “tail wagging the dog” feedback. Besides recovering the effective diffusivity Deff = CsDM in ‘stochastic field regime’, where Cs is sound speed and DM is the familiar stochastic field diffusivity of Rosenbluth et al., we obtain a hybrid turbulent viscosity Dν = Cs2Σk |bx,k |2 /k⊥DT in ‘strong turbulent regime’ such that Κ=-Dν ∂x〈uz〉, where DT is turbulent fluid diffusivity. This indicates that the actual diffusivity Dν describes how the mean flow is scattered perpendicularly by the synergy of stochastic fields and the strongly turbulent flow. Finally, there are several implications of those results for the physics of the kinetic stress and toroidal rotation. Discussions of these will be presented.
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Publication: C.-C. Chen, P. H. Diamond, R. Singh, and S. M. Tobias, "Potential vorticity transport in weakly and strongly magnetized plasmas", Physics of Plasmas 28, 042302 (2021). <br>W.X. Ding, et al. Phys. Rev. Lett. 110, 065008 (2013)<br>M.N. Rosenbluth, et al. Nuclear Fusion 6, 297 (1966)
Presenters
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Chang-Chun Chen
University of California, San Diego
Authors
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Chang-Chun Chen
University of California, San Diego
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Patrick H Diamond
University of California, San Diego, UCSD
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Rameswar Singh
University of California, San Diego
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Steven Tobias
Univ of Leeds