Theory of zonal flow growth and propagation in toroidal geometry

Fuente: arXiv
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Main Authors: Nies, Richard, Parra, Felix
Format: Preprint
Published: 2025
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author Nies, Richard
Parra, Felix
author_facet Nies, Richard
Parra, Felix
contents The toroidal geometry of tokamaks and stellarators is known to play a crucial role in the linear physics of zonal flows, leading to e.g. the Rosenbluth-Hinton residual and geodesic acoustic modes. However, descriptions of the nonlinear zonal flow growth from a turbulent background typically resort to simplified models of the geometry. We present a generalised theory of the secondary instability to model the zonal flow growth from turbulent fluctuations in toroidal geometry, demonstrating that the radial magnetic drift substantially affects the nonlinear zonal flow dynamics. In particular, the toroidicity gives rise to a new branch of propagating zonal flows, the toroidal secondary mode, which is nonlinearly supported by the turbulence. We present a theory of this mode and compare the theory against gyrokinetic simulations of the secondary mode. The connection with other secondary modes -- the ion-temperature-gradient and Rogers-Dorland-Kotschenreuther secondary modes -- is also examined.
format Preprint
id arxiv_https___arxiv_org_abs_2504_09785
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Theory of zonal flow growth and propagation in toroidal geometry
Nies, Richard
Parra, Felix
Plasma Physics
The toroidal geometry of tokamaks and stellarators is known to play a crucial role in the linear physics of zonal flows, leading to e.g. the Rosenbluth-Hinton residual and geodesic acoustic modes. However, descriptions of the nonlinear zonal flow growth from a turbulent background typically resort to simplified models of the geometry. We present a generalised theory of the secondary instability to model the zonal flow growth from turbulent fluctuations in toroidal geometry, demonstrating that the radial magnetic drift substantially affects the nonlinear zonal flow dynamics. In particular, the toroidicity gives rise to a new branch of propagating zonal flows, the toroidal secondary mode, which is nonlinearly supported by the turbulence. We present a theory of this mode and compare the theory against gyrokinetic simulations of the secondary mode. The connection with other secondary modes -- the ion-temperature-gradient and Rogers-Dorland-Kotschenreuther secondary modes -- is also examined.
title Theory of zonal flow growth and propagation in toroidal geometry
topic Plasma Physics
url https://arxiv.org/abs/2504.09785