Results 1 to 10 of about 415 (105)

Quasi-Isodynamic Stellarators with Low Turbulence as Fusion Reactor Candidates

open access: yesPRX Energy
The stellarator is a type of fusion energy device that—if properly designed—could provide clean, safe, and abundant energy to the grid. To generate this energy, a stellarator must keep a hot mixture of charged particles (known as a plasma) sufficiently ...
Alan G. Goodman   +9 more
doaj   +7 more sources

A quasi-isodynamic configuration with good confinement of fast ions at low plasma β

open access: yesNuclear Fusion, 2023
A new quasi-isodynamic (QI) stellarator configuration optimized for the confinement of energetic ions at low plasma β is obtained. The numerical optimization is carried out using the STELLOPT suite of codes.
E. Sánchez   +3 more
doaj   +3 more sources

Trapped electron mode in a quasi-isodynamic stellarator

open access: yesNuclear Fusion
Global gyrokinetic simulations find a strongly unstable trapped electron mode excited by a density gradient in a quasi-isodynamic stellarator. The eigenmode structure localizes on the inner side of the torus with an unfavorable magnetic curvature and ...
Javier H. Nicolau   +4 more
doaj   +3 more sources

Statistical Analysis of Plasma Dynamics in Gyrokinetic Simulations of Stellarator Turbulence [PDF]

open access: yesEntropy, 2023
A geometrical method for assessing stochastic processes in plasma turbulence is investigated in this study. The thermodynamic length methodology allows using a Riemannian metric on the phase space; thus, distances between thermodynamic states can be ...
Aristeides D. Papadopoulos   +4 more
doaj   +2 more sources

Resilience of Quasi-Isodynamic Stellarators against Trapped-Particle Instabilities [PDF]

open access: yesPhysical Review Letters, 2012
It is shown that in perfectly quasi-isodynamic stellarators, trapped particles with a bounce frequency much higher than the frequency of the instability are stabilizing in the electrostatic and collisionless limit. The collisionless trapped-particle instability is therefore stable as well as the ordinary electron-density-gradient-driven trapped ...
Per Helander
exaly   +7 more sources

Constructing precisely quasi-isodynamic magnetic fields

open access: yesJournal of Plasma Physics, 2022
We present a novel method for numerically finding quasi-isodynamic stellarator magnetic fields with excellent fast-particle confinement and extremely small neoclassical transport.
Goodman, Alan   +8 more
core   +4 more sources

A promising approach to steady-state fusion: High-temperature superconducting strong-field stellarator with precise omnigenity [PDF]

open access: yesThe Innovation
The stellarator has inherent advantages over the tokamak in achieving steady-state operation, especially due to its absence of disruptions and lack of need for current drive and the associated recirculating power.
Guosheng Xu   +3 more
doaj   +2 more sources

Suppression of non-axisymmetric field-induced α-particle loss channels in a quasi-axisymmetric stellarator

open access: yesAIP Advances, 2022
In future fusion reactors, the confinement of α-particles is a crucial issue. The perfect omnigenity may be difficult to achieve in the quasi-isodynamic and quasi-symmetric stellarators when a multi-objective optimization is considered.
Yichao Zhang   +12 more
doaj   +1 more source

Robust stellarator optimization via flat mirror magnetic fields

open access: yesNuclear Fusion, 2023
Stellarator magnetic configurations need to be optimized in order to meet all the required properties of a fusion reactor. In this work, it is shown that a flat-mirror quasi-isodynamic (QI) configuration (i.e.
J.L. Velasco   +3 more
doaj   +1 more source

Collisionless microinstabilities in stellarators II - numerical simulations [PDF]

open access: yes, 2013
Microinstabilities exhibit a rich variety of behavior in stellarators due to the many degrees of freedom in the magnetic geometry. It has recently been found that certain stellarators (quasi-isodynamic ones with maximum-$J$ geometry) are partly resilient
Helander, P.   +2 more
core   +1 more source

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