Stellarators close to quasisymmetry
Rotation is favorable for confinement, but a stellarator can rotate at high speeds if and only if it is sufficiently close to quasisymmetry. This article investigates how close it needs to be. For a magnetic field $\mathbf{B} = \mathbf{B}_0 + \alpha \mathbf{B}_1$, where $\mathbf{B}_0$ is quasisymmet...
Main Authors: | Calvo, I, Parra, F, Velasco, J, Alonso, J |
---|---|
Formato: | Journal article |
Idioma: | English |
Publicado: |
2013
|
Títulos similares
-
Flow damping in stellarators close to quasisymmetry
por: Calvo, I, et al.
Publicado: (2014) -
Quasisymmetry equations for conventional stellarators /
por: 243354 Pustovitov, V. D.
Publicado: (1994) -
The effect of tangential drifts on neoclassical transport in stellarators close to omnigeneity
por: Calvo, I, et al.
Publicado: (2017) -
Optimizing stellarators for large flows
por: Calvo, I, et al.
Publicado: (2014) -
Omnigenity as Generalized Quasisymmetry
por: Landreman, Matt, et al.
Publicado: (2015)