Rotational transform: Difference between revisions

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Assuming the existence of toroidally nested magnetic [[Flux surface|flux surfaces]], the rotational transform (field line pitch) is defined as
The rotational transform (or field line pitch) ''ι/2π'' is defined as the number of poloidal transits per single toroidal transit of a field line on a toroidal flux surface.
The definition can be relaxed somewhat to include field lines moving in a spatial volume between two nested toroidal surfaces (e.g., a stochastic field region).


:<math>\frac{\iota}{2 \pi} = \frac{d \psi}{d \phi}</math>
Assuming the existence of toroidally nested magnetic [[Flux surface|flux surfaces]], the rotational transform on such a surface may also be  defined as
<ref>[http://link.aps.org/doi/10.1103/RevModPhys.76.1071 A.H. Boozer, ''Physics of magnetically confined plasmas'', Rev. Mod. Phys. '''76''' (2004) 1071]</ref>


where ''&psi;'' is the poloidal magnetic flux, and ''&phi;'' the toroidal magnetic flux.
:<math>\frac{\iota}{2 \pi} = \frac{d \psi}{d \Phi}</math>
Thus, ''&iota;/2&pi;'' is the mean number of toroidal transits (''n'') divided by the
 
mean number of poloidal transits (''m'') of a field line on a flux surface.
where ''&psi;'' is the poloidal magnetic flux, and &Phi; the toroidal magnetic flux.


== Safety factor ==
== Safety factor ==


In [[Tokamak|tokamak]] research, the quantity ''q = 2&pi;/&iota;'' is preferred (called the "safety factor").
In [[Tokamak|tokamak]] research, the quantity ''q = 2&pi;/&iota;'' is preferred (called the "safety factor").
In a circular [[Tokamak|tokamak]],  
In a circular tokamak,  
the equations of a field line on the flux surface are, approximately:
the equations of a field line on the flux surface are, approximately:
<ref>K. Miyamoto, ''Plasma Physics and Controlled Nuclear Fusion'', Springer-Verlag (2005) ISBN 3540242171</ref>
<ref>K. Miyamoto, ''Plasma Physics and Controlled Nuclear Fusion'', Springer-Verlag (2005) {{ISBN|3540242171}}</ref>
 
:<math>\frac{r d\theta}{B_\theta} = \frac{Rd\varphi}{B_\varphi}</math>
 
where <math>\phi</math> and ''&theta;'' are the [[Toroidal coordinates|toroidal and poloidal angles]], respectively.
Thus <math>q = m/n = \left \langle d\varphi /d\theta \right \rangle </math> can be approximated by
 
:<math>q \simeq \frac{r B_\varphi}{R B_\theta}</math>
 
Where the poloidal magnetic field <math>{B_\theta}</math> is mostly produced by a toroidal plasma current. The principal significance of the safety factor ''q'' is that if <math>q \leq 2</math> at the last closed flux surface (the edge), the plasma is [[:Wikipedia:Magnetohydrodynamics|magnetohydrodynamically]] unstable.<ref>Wesson J 1997 Tokamaks 2nd edn (Oxford: Oxford University Press) p280 {{ISBN|0198509227}}</ref>


:<math>\frac{r d\theta}{B_\theta} = \frac{Rd\phi}{B_\phi}</math>
In [[Tokamak|tokamaks]] with a [[divertor]], ''q'' approaches infinity at the [[separatrix]], so it is more useful to consider ''q'' just inside the separatrix. It is customary to use ''q'' at the 95% flux surface (the flux surface that encloses 95% of the poloidal flux), ''q<sub>95</sub>''.


where ''&phi;'' and ''&theta;'' are the [[Toroidal coordinates|toroidal and poloidal angles]], respectively.
== See also ==
Thus ''q = m/n = d&phi;/d&theta;'' can be approximated by


:<math>q = \frac{r B_\phi}{R B_\theta}</math>
* [[Magnetic island]]
* [[Magnetic shear]]


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