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Long-wavelength limit of gyrokinetics in a turbulent tokamak and its intrinsic ambipolarity

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abstract

Recently, the electrostatic gyrokinetic Hamiltonian and change of coordinates have been computed to order $\epsilon^2$ in general magnetic geometry. Here $\epsilon$ is the gyrokinetic expansion parameter, the gyroradius over the macroscopic scale length. Starting from these results, the long-wavelength limit of the gyrokinetic Fokker-Planck and quasineutrality equations is taken for tokamak geometry. Employing the set of equations derived in the present article, it is possible to calculate the long-wavelength components of the distribution functions and of the poloidal electric field to order $\epsilon^2$. These higher-order pieces contain both neoclassical and turbulent contributions, and constitute one of the necessary ingredients (the other is given by the short-wavelength components up to second order) that will eventually enter a complete model for the radial transport of toroidal angular momentum in a tokamak in the low flow ordering. Finally, we provide an explicit and detailed proof that the system consisting of second-order gyrokinetic Fokker-Planck and quasineutrality equations leaves the long-wavelength radial electric field undetermined; that is, the turbulent tokamak is intrinsically ambipolar.

fields

astro-ph.SR 1

years

2026 1

verdicts

CONDITIONAL 1

representative citing papers

A Transport Theory of Turbulent Coronal Heating in General Geometry

astro-ph.SR · 2026-07-09 · conditional · novelty 8.0

A controlled multiscale RMHD expansion in arbitrary magnetic geometry yields new geometry-driven turbulent heating and cross-field transport channels that can dominate standard reflection in structured coronal regions.

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  • A Transport Theory of Turbulent Coronal Heating in General Geometry astro-ph.SR · 2026-07-09 · conditional · none · ref 209 · internal anchor

    A controlled multiscale RMHD expansion in arbitrary magnetic geometry yields new geometry-driven turbulent heating and cross-field transport channels that can dominate standard reflection in structured coronal regions.