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Theory of zonal flow growth and propagation in toroidal geometry

Abstract:
The toroidal geometry of tokamaks and stellarators is known to play a crucial role in the linear physics of zonal flows (ZFs), leading to e.g. the Rosenbluth–Hinton residual and geodesic acoustic modes. However, descriptions of the nonlinear ZF 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 ZF growth from turbulent fluctuations in toroidal geometry, demonstrating that the radial magnetic drift substantially affects the nonlinear ZF dynamics. In particular, the toroidicity gives rise to a new branch of propagating ZFs, 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.
Publication status:
Published
Peer review status:
Peer reviewed

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Files:
Publisher copy:
10.1088/1361-6587/ae56b8

Authors

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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0002-9508-1223
More by this author
Institution:
University of Oxford
Role:
Author
ORCID:
0000-0001-9621-7404


Publisher:
IOP Publishing
Journal:
Plasma Physics and Controlled Fusion More from this journal
Volume:
68
Issue:
4
Pages:
045028-045028
Publication date:
2026-03-24
DOI:
EISSN:
1361-6587
ISSN:
0741-3335


Language:
English
Keywords:
Pubs id:
2410264
Local pid:
pubs:2410264
Source identifiers:
W7140223819
Deposit date:
2026-05-08
ARK identifier:
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