Omnigeneity: Difference between revisions
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Omnigeneity (or omnigenity) is a property of the vacuum magnetic field such that the mean radial collisionless guiding center magnetic drift is zero. | Omnigeneity (or omnigenity) is a property of the vacuum magnetic field such that the mean radial collisionless guiding center magnetic drift is zero. | ||
Thus, in a perfectly omnigenous field, all collisionless trajectories are confined. | Thus, in a perfectly omnigenous field, all collisionless trajectories are confined. | ||
<ref>[[doi:10.1063/1. | <ref>D.A. Garren and A.H. Boozer, ''Existence of quasihelically symmetric stellarators'', [[doi:10.1063/1.859916|Phys. Fluids B 3 (1991) 2822]]</ref> | ||
<ref>M. Landreman and P.J. Catto, ''Omnigenity as generalized quasisymmetry'', [[doi:10.1063/1.3693187|Phys. Plasmas '''19''' (2012) 056103]]</ref> | |||
== See also == | |||
* [[Stellarator]] | |||
* [[Quasisymmetry]] | |||
== References == | == References == | ||
<references /> | <references /> | ||
Latest revision as of 10:40, 30 October 2015
Omnigeneity (or omnigenity) is a property of the vacuum magnetic field such that the mean radial collisionless guiding center magnetic drift is zero. Thus, in a perfectly omnigenous field, all collisionless trajectories are confined. [1] [2]
See also
References
- ↑ D.A. Garren and A.H. Boozer, Existence of quasihelically symmetric stellarators, Phys. Fluids B 3 (1991) 2822
- ↑ M. Landreman and P.J. Catto, Omnigenity as generalized quasisymmetry, Phys. Plasmas 19 (2012) 056103