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Quasisymmetry (QS) is a hidden symmetry of the magnetic field strength, B, that enables effective confinement of charged particles in a fully three-dimensional (3D) toroidal plasma equilibrium. Such equilibria are typically modeled by the…

等离子体物理 · 物理学 2025-07-10 W. Sengupta , R. Madan , S. Buller , N. Nikulsin , E. J. Paul , R. Nies , A. A. Kaptanoglu , S. R. Hudson , A. Bhattacharjee

Quasisymmetry (QS), a hidden symmetry of the magnetic field strength, is known to support nested flux surfaces and provide superior particle confinement in stellarators. In this work, we study the ideal MHD equilibrium and stability of…

等离子体物理 · 物理学 2024-02-06 W. Sengupta , N. Nikulsin , R. Gaur , A. Bhattacharjee

Quasisymmetry (QS) is a property of special magnetic configurations, where the magnetic field strength, but not necessarily the full vector field, has a direction of symmetry. QS leads to reduced neoclassical transport and thus can be a…

等离子体物理 · 物理学 2025-06-10 Lanke Fu , Eduardo Rodriguez , Rory Conlin , Amitava Bhattacharjee

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

Quasisymmetry and omnigeneity of an equilibrium magnetic field are two distinct properties proposed to ensure radial localization of collisionless trapped particles in any stellarator. These constraints are incompletely explored, but have…

等离子体物理 · 物理学 2018-03-14 Wrick Sengupta , Harold Weitzner

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 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

Quasisymmetric stellarators are an attractive class of optimised magnetic confinement configurations. The property of quasisymmetry (QS) is in practice limited to be approximate, and thus the construction requires measures that quantify the…

等离子体物理 · 物理学 2022-02-16 Eduardo Rodriguez , Elizabeth Paul , Amitava Bhattacharjee

Quasisymmetry is an unusual symmetry that can be present in toroidal magnetic fields, enabling confinement of charged particles and plasma. Here it is shown that both quasi-axisymmetry and quasi-helical symmetry can be achieved to a much…

等离子体物理 · 物理学 2022-02-02 Matt Landreman , Elizabeth Paul

Most quasisymmetric stellarators to date have been designed by numerically optimizing the plasma boundary shape to minimize symmetry-breaking Fourier modes of the magnetic field strength $B$. At high aspect ratio, a faster approach is to…

等离子体物理 · 物理学 2019-06-26 Matt Landreman

A quasisymmetry is a special symmetry that enhances the ability of a magnetic field to trap charged particles. Quasisymmetric magnetic fields may allow the realization of next generation fusion reactors (stellarators) with superior…

等离子体物理 · 物理学 2022-07-08 Naoki Sato

A new optimized quasihelically symmetric configuration is described that has the desir-able properties of improved energetic particle confinement, reduced turbulent transportby 3D shaping, and non-resonant divertor capabilities. The…

We explore the existence of quasisymmetric magnetic fields in asymmetric toroidal domains. These vector fields can be identified with a class of magnetohydrodynamic equilibria in the presence of pressure anisotropy. First, using Clebsch…

偏微分方程分析 · 数学 2021-11-12 Naoki Sato , Zhisong Qu , David Pfefferlé , Robert L. Dewar

Analytical calculations based on a Landau Level (LL) picture are reported for a many-electron system moving in an interface (with a finite-width Quantum Well (QW)) and in the presence of an external perpendicular magnetic field. They lead…

介观与纳米尺度物理 · 物理学 2011-06-01 Georgios Konstantinou , Konstantinos Moulopoulos

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

The condition of quasi-isodynamicity is derived to second order in the distance from the magnetic axis. We do so using a formulation of omnigenity that explicitly requires the balance between the radial particle drifts at opposite bounce…

等离子体物理 · 物理学 2023-07-12 Eduardo Rodriguez , Gabe G. Plunk

We examine a large class of inhomogeneous spherically symmetric spacetimes that generalize the Lemaitre-Tolman-Bondi dust solutions to nonzero pressure ("LTB spacetimes"). Local covariant LTB objects can be expressed as perturbations of…

广义相对论与量子宇宙学 · 物理学 2010-05-12 Roberto A. Sussman

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

Transport properties of highly mobile 2D electrons are studied in symmetric GaAs quantum wells placed in titled magnetic fields. Quantum positive magnetoresistance (QPMR) is observed in magnetic fields perpendicular to the 2D layer.…

介观与纳米尺度物理 · 物理学 2016-11-29 William Mayer , Areg Ghazaryan , Pouyan Ghaemi , Sergey Vitkalov , A. A. Bykov

A necessary and sufficient set of conditions for a quasisymmetric magnetic field in the form of constraint equations is derived from first principles. Without any assumption regarding the magnetohydrodynamic (MHD) equilibrium of the plasma,…

等离子体物理 · 物理学 2020-06-24 Eduardo Rodriguez , Per Helander , Amitava Bhattacharjee
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