Omnigeneity - Revision history

Jlvelasco at 10:55, 9 February 2026

2026-02-09T10:55:17Z

← Older revision		Revision as of 12:55, 9 February 2026
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	* [[Stellarator]]		* [[Stellarator]]
	* [[Quasisymmetry]]		* [[Quasisymmetry]]
			* [[Piecewise_omnigeinity]]

	== References ==		== References ==
	<references />		<references />

Admin at 09:40, 30 October 2015

2015-10-30T09:40:50Z

← Older revision		Revision as of 11:40, 30 October 2015
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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:10.1063/1.859916\|~~D.A. Garren and A.H. Boozer, ''Existence of quasihelically symmetric stellarators'', Phys. Fluids B 3 (1991) 2822]]</ref>		<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>~~[[doi:10.1063/1.3693187\|~~M. Landreman and P.J. Catto, ''Omnigenity as generalized quasisymmetry'', Phys. Plasmas '''19''' (2012) 056103]]</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 ==		== See also ==

Admin at 12:19, 6 September 2013

2013-09-06T12:19:26Z

← Older revision		Revision as of 14:19, 6 September 2013
Line 1:		Line 1:
	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:10.1063/1.859916\|D.A. Garren and A.H. Boozer, ''Existence of quasihelically symmetric stellarators'', Phys. Fluids B 3 (1991) 2822]]</ref>
	<ref>[[doi:10.1063/1.3693187\|M. Landreman and P.J. Catto, ''Omnigenity as generalized quasisymmetry'', Phys. Plasmas '''19''' (2012) 056103]]</ref>		<ref>[[doi:10.1063/1.3693187\|M. Landreman and P.J. Catto, ''Omnigenity as generalized quasisymmetry'', Phys. Plasmas '''19''' (2012) 056103]]</ref>

Admin at 12:12, 6 September 2013

2013-09-06T12:12:20Z

← Older revision		Revision as of 14:12, 6 September 2013
Line 2:		Line 2:
	Thus, in a perfectly omnigenous field, all collisionless trajectories are confined.		Thus, in a perfectly omnigenous field, all collisionless trajectories are confined.
	<ref>[[doi:10.1063/1.3693187\|M. Landreman and P.J. Catto, ''Omnigenity as generalized quasisymmetry'', Phys. Plasmas '''19''' (2012) 056103]]</ref>		<ref>[[doi:10.1063/1.3693187\|M. Landreman and P.J. Catto, ''Omnigenity as generalized quasisymmetry'', Phys. Plasmas '''19''' (2012) 056103]]</ref>

			== See also ==
			* [[Stellarator]]
			* [[Quasisymmetry]]

	== References ==		== References ==
	<references />		<references />

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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.
Thus, in a perfectly omnigenous field, all collisionless trajectories are confined.
<ref>[[doi:10.1063/1.3693187|M. Landreman and P.J. Catto, ''Omnigenity as generalized quasisymmetry'', Phys. Plasmas '''19''' (2012) 056103]]</ref>

== References ==
<references />