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• W3194975089 abstract "Given the large anisotropy of transport processes in magnetized plasmas, the magnetic field structure can strongly impact the heat diffusion: magnetic surfaces and cantori form barriers to transport while chaotic layers and island structures can degrade confinement. When a small but finite amount of perpendicular diffusion is included, the structure of the magnetic field becomes less important, allowing finite pressure gradients to be supported across chaotic regions and island chains. We introduce a metric for the effective volume of non-integrability based on the solution to the anisotropic heat diffusion equation. To validate this metric, we consider model fields with a single island chain and a strongly chaotic layer for which analytic predictions of the relative parallel and perpendicular transport can be made. We also analyze critically chaotic fields produced from different sets of perturbations, highlighting the impact of the mode number spectrum on the heat transport. We propose that this metric be used to assess the impact of non-integrability on the heat transport in stellarator equilibria." @default.
• W3194975089 created "2021-08-30" @default.
• W3194975089 creator A5028430629 @default.
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• W3194975089 date "2021-08-13" @default.
• W3194975089 modified "2023-09-27" @default.
• W3194975089 title "Heat conduction in an irregular magnetic field: Part II. Heat transport as a measure of the effective non-integrable volume" @default.
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