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Updated: Oct 23, 2025

Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Connection between quasisymmetric magnetic fields and anisotropic pressure equilibria in fusion plasmas
E Rodríguez1, A Bhattacharjee1
1Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey, 08543, USA and Princeton Plasma Physics Laboratory, Princeton, New Jersey, 08540, USA.
Abstract:
The stellarator as a concept of magnetic confinement fusion requires careful design to confine particles effectively. A design possibility is to equip the magnetic field with a property known as quasisymmetry. Though it is generally believed that a steady-state quasisymmetric equilibrium can only be exact locally (unless the system has a direction of continuous symmetry such as the tokamak), we suggest in this work that a change in the equilibrium paradigm can ameliorate this limitation. We demonstrate that there exists a deep physical connection between quasisymmetry and magnetostatic equilibria with anisotropic pressure, extending beyond the isotropic pressure equilibria commonly considered.
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