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Fluctuation driven transport and stationary profiles

2011/05/01 by J. Kesner, D. Garnier, D. T. Garnier +1 · 1 citation
Physics and Astronomy · #Ionosphere and magnetosphere dynamics #Magnetic confinement fusion research #Solar and Space Plasma Dynamics

paper · doi:10.1063/1.3590935

openalex publication_date 2011/05/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/22

Abstract

Transport equations for particles and energy can be derived when the fluctuations conserve adiabatic invariants. The transport equations determine both stationary density and pressure profiles and the direction of the turbulence-driven fluxes which can be inward or outward. An inward turbulent pinch is predicted which creates stationary profiles and reverses direction depending on the density and temperature gradients. The transport fluxes are independent of the underlying drive that leads to plasma turbulence. For low frequency turbulence, the formulation remains correct when the collisional time scale is faster than the confinement time scale.

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