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A method is given to rapidly compute quasisymmetric stellarator magnetic fields for plasma confinement, without the need to call a three-dimensional magnetohydrodynamic equilibrium code inside an optimization iteration. The method is based…

等离子体物理 · 物理学 2019-12-04 Matt Landreman , Wrick Sengupta

Quasisymmetric stellarators are appealing intellectually and as fusion reactor candidates since the guiding center particle trajectories and neoclassical transport are isomorphic to those in a tokamak, implying good confinement. Previously,…

等离子体物理 · 物理学 2019-01-23 Matt Landreman , Wrick Sengupta , Gabriel G Plunk

A method is demonstrated to rapidly calculate the shapes and properties of quasi-axisymmetric and quasi-helically symmetric stellarators. In this approach, optimization is applied to the equations of magnetohydrodynamic equilibrium and…

等离子体物理 · 物理学 2023-01-04 Matt Landreman

The confinement of guiding center trajectories in a stellarator is determined by the variation of the magnetic field strength $B$ in Boozer coordinates $(r, \theta, \varphi)$, but $B(r,\theta,\varphi)$ depends on the flux surface shape in a…

等离子体物理 · 物理学 2019-01-16 Matt Landreman , Wrick Sengupta

We apply the near-axis expansion method for quasisymmetric magnetic fields with anisotropic pressure (developed in the companion paper, Part I [E. Rodriguez, A. Bhattacharjee, arXiv:2008.04715 (2020)]) to construct numerical solutions to…

等离子体物理 · 物理学 2021-02-24 Eduardo Rodriguez , Amitava Bhattacharjee

Optimising stellarators for quasisymmetry leads to strongly reduced collisional transport and energetic particle losses compared to unoptimised configurations. Though stellarators with precise quasisymmetry have been obtained in the past,…

等离子体物理 · 物理学 2024-12-25 Richard Nies , Elizabeth J. Paul , Dario Panici , Stuart R. Hudson , Amitava Bhattacharjee

Optimized stellarator configurations and their analytical properties are obtained using a near-axis expansion approach. Such configurations are associated with good confinement as the guiding center particle trajectories and neoclassical…

等离子体物理 · 物理学 2020-08-26 R. Jorge , W. Sengupta , M. Landreman

Quasisymmetry can greatly improve the confinement of energetic particles and thermal plasma in a stellarator. The magnetic field of a quasisymmetric stellarator at high plasma pressure is significantly affected by the bootstrap current, but…

等离子体物理 · 物理学 2022-08-17 Matt Landreman , Stefan Buller , Michael Drevlak

The condition of omnigenity is investigated, and applied to the near-axis expansion of Garren and Boozer (1991a). Due in part to the particular analyticity requirements of the near-axis expansion, we find that, excluding quasi-symmetric…

等离子体物理 · 物理学 2020-01-08 G. G. Plunk , M. Landreman , P. Helander

The near-axis theory for quasi-isodynamic stellarator equilibria is reformulated in terms of geometric inputs, to allow greater control of the ``direct construction'' of quasi-isodynamic configurations, and to facilitate understanding of…

等离子体物理 · 物理学 2025-08-19 G. G. Plunk , E. Rodríguez

A direct construction of equilibrium magnetic fields with toroidal topology at arbitrary order in the distance from the magnetic axis is carried out, yielding an analytical framework able to explore the landscape of possible magnetic flux…

等离子体物理 · 物理学 2020-01-29 R. Jorge , W. Sengupta , M. Landreman

In this study, we explore the influence of the helicity of the magnetic axis-defined as the self-linking number of the curve-on the quality of quasi-isodynamic stellarator-symmetric configurations constructed using the near-axis expansion…

等离子体物理 · 物理学 2023-08-30 Katia Camacho Mata , Gabriel G. Plunk

We develop the formalism of the first order near-axis expansion of the MHD equilibrium equations described in Garren & Boozer (1991), Plunk et al. (2019) and Plunk et al. (2021), for the case of a quasi-isodynamic, N-field period,…

等离子体物理 · 物理学 2022-11-29 Katia Camacho Mata , Gabriel G. Plunk , Rogerio Jorge

A new paradigm for rapid stellarator configuration design has been recently demonstrated, in which the shapes of quasisymmetric or omnigenous flux surfaces are computed directly using an expansion in small distance from the magnetic axis.…

等离子体物理 · 物理学 2021-03-08 Matt Landreman

Filament-based coil optimizations are performed for several quasihelical stellarator configurations, notably the one from [M. Landreman, E. Paul, PRL 128, 035001, 2022], demonstrating that precise quasihelical symmetry can be achieved with…

等离子体物理 · 物理学 2023-11-29 Alexander Vyacheslav Wiedman , Stefan Buller , Matt Landreman

Stellarators confine fusion plasmas using three-dimensional magnetic fields composed of nested toroidal magnetic surfaces. In generic stellarators, trapped particles can drift across these surfaces and degrade plasma confinement. Certain…

There is currently no agreed-upon methodology for characterizing a stellarator magnetic field geometry, and yet modern stellarator designs routinely attain high levels of magnetic-field quasi-symmetry through careful flux-surface shaping.…

等离子体物理 · 物理学 2026-01-01 M. J. Gerard , M. J. Pueschel , S. Stewart , H. O. M. Hillebrecht , B. Geiger

A method is demonstrated to optimize a stellarator's geometry to eliminate magnetic islands and achieve other desired physics properties at the same time. For many physics quantities that have been used in stellarator optimization,…

等离子体物理 · 物理学 2021-09-22 Matt Landreman , Bharat Medasani , Caoxiang Zhu

In stellarator optimization studies, the boundary of the plasma is usually described by Fourier series that are not unique: several sets of Fourier coefficients describe approximately the same boundary shape. A simple method for eliminating…

等离子体物理 · 物理学 2021-10-04 Sophia A. Henneberg , Per Helander , Michael Drevlak

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…

等离子体物理 · 物理学 2022-02-03 Eduardo Rodriguez , Amitava Bhattacharjee
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