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 | Assuming the existence of toroidally nested magnetic [[Flux surface|flux surfaces]], the rotational transform (field line pitch) is 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> | |||
:<math>\frac{\iota}{2 \pi} = \frac{d \psi}{d \phi}</math> | :<math>\frac{\iota}{2 \pi} = \frac{d \psi}{d \phi}</math> |
Revision as of 11:56, 31 July 2010
Assuming the existence of toroidally nested magnetic flux surfaces, the rotational transform (field line pitch) is defined as [1]
where ψ is the poloidal magnetic flux, and φ the toroidal magnetic flux. Thus, ι/2π 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.
Safety factor
In tokamak research, the quantity q = 2π/ι is preferred (called the "safety factor"). In a circular tokamak, the equations of a field line on the flux surface are, approximately: [2]
where φ and θ are the toroidal and poloidal angles, respectively. Thus q = m/n = dφ/dθ can be approximated by
See also
References
- ↑ A.H. Boozer, Physics of magnetically confined plasmas, Rev. Mod. Phys. 76 (2004) 1071
- ↑ K. Miyamoto, Plasma Physics and Controlled Nuclear Fusion, Springer-Verlag (2005) ISBN 3540242171