MHD stability and the effects of shaping: a near-axis view for tokamaks and quasisymmetric stellarators

Abstract

How much does the cross-section of a toroidal magnetic field configuration tell us about its MHD stability? It is generally believed that positive triangularity (typically leading to bean-shaped cross-sections with their indentation on the inboard side in stellarators) contributes positively to MHD stability. In this paper, we explore the basis of this statement within a near-axis description for axisymmetric and quasisymmetric magnetic configurations. In agreement with the existing literature, we show that positive triangularity stabilises vertically elongated tokamaks. In quasisymmetric stellarators, the toroidal asymmetry of flux surfaces modifies this relation. The behaviour of stellarator-symmetric, quasisymmetric stellarators can still be described in terms of the shape of one of their up-down symmetric cross-sections. However, we show that for a sample of quasisymmetric configurations, the positive-bean-shaped cross-sections do not contribute positively to stability. Unlike in the axisymmetric case, we also learn that finite $\beta$ can improve stability even without magnetic shear.

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Cited by in corpus (6)

• Constructing the space of quasisymmetric stellarators
• Collisionless zonal-flow dynamics in quasisymmetric stellarators
• Stellarator Optimization with Constraints
• The shear Alfvén continuum of quasisymmetric stellarators
• The zonal-flow residual does not tend to zero in the limit of small mirror ratio
• Near-axis quasi-isodynamic database