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Flux surface: Difference between revisions
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:<math>\vec B \cdot \vec n = 0</math> | :<math>\vec B \cdot \vec n = 0</math> | ||
everywhere on ''S''. It is then possible to define a scalar ''flux function'' (''f'') such that its value is constant on the surface ''S'', and | everywhere on ''S''. | ||
In other words, the magnetic field does not ''cross'' the surface ''S'' anywhere, i.e., the magnetic flux traversing ''S'' is zero. | |||
It is then possible to define a scalar ''flux function'' (''f'') such that its value is constant on the surface ''S'', and | |||
:<math>\vec B \cdot \vec \nabla f = 0</math> | :<math>\vec B \cdot \vec \nabla f = 0</math> | ||
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[[File:Flux_definition.png|250px|thumb|right|Diagram showing the surfaces defining the poloidal (red) and toroidal (blue) flux]] | [[File:Flux_definition.png|250px|thumb|right|Diagram showing the surfaces defining the poloidal (red) and toroidal (blue) flux]] | ||
When ''B'' is a magnetic field with toroidal nested flux surfaces, two magnetic fluxes can be defined from two corresponding surfaces. | When ''B'' is a magnetic field with toroidal nested flux surfaces, two magnetic fluxes can be defined from two corresponding surfaces. | ||
<ref>R.D. Hazeltine, J.D. Meiss, ''Plasma Confinement'', Courier Dover Publications (2003) ISBN 0486432424</ref> | <ref>R.D. Hazeltine, J.D. Meiss, ''Plasma Confinement'', Courier Dover Publications (2003) {{ISBN|0486432424}}</ref> | ||
The poloidal flux is defined by | The poloidal flux is defined by | ||
:<math>\psi = \int_{S_p}{\vec B \cdot \vec n dS}</math> | :<math>\psi = \int_{S_p}{\vec B \cdot \vec n dS}</math> | ||
where ''S<sub>p</sub>'' is a ring-shaped ribbon stretched between the magnetic axis and the flux surface ''f'', | where ''S<sub>p</sub>'' is a ring-shaped ribbon stretched between the magnetic axis and the flux surface ''f''. | ||
(Complementarily, ''S<sub>p</sub>'' can be taken to be a surface spanning the central hole of the torus.<ref>[http://link.aps.org/doi/10.1103/RevModPhys.76.1071 A.H. Boozer, ''Physics of magnetically confined plasmas'', Rev. Mod. Phys. '''76''' (2005) 1071 - 1141]</ref>) | |||
Likewise, the toroidal flux is defined by | |||
:<math>\phi = \int_{S_t}{\vec B \cdot \vec n dS}</math> | :<math>\phi = \int_{S_t}{\vec B \cdot \vec n dS}</math> | ||
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* [[MHD equilibrium]] | * [[MHD equilibrium]] | ||
* [[Toroidal coordinates]] | |||
* [[Flux coordinates]] | |||
* [[Rotational transform]] | |||
* [[Magnetic shear]] | * [[Magnetic shear]] | ||
* [[Effective plasma radius]] | * [[Effective plasma radius]] | ||
* [[Separatrix]] | |||
* [[Flux tube]] | |||
== References == | == References == | ||
<references /> | <references /> | ||