A poloidal magnetic field lies in meridional planes through the symmetry axis, in contrast to a toroidal magnetic field. For an axisymmetric vector field, it is represented by a poloidal magnetic flux function as Bp=R−1∇Ψ×eϕ.
Ancestors (6)
Incoming links (34)
- Axisymmetric magnetic flux surface
- Babcock-Leighton mechanism
- Ferraro's law of isorotation
- Field-line angular velocity of an axisymmetric wind
- Local alpha-Omega dynamo wave dispersion
- Magnetic axial angular momentum flux
- Material advection of an axisymmetric magnetic flux function
- Omega effect
- Past exam of the mathematics course of the University of Cambridge / 2001 / iii / Paper 35 / 4 / Solution
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- Solar dynamo
- Sub-Alfvénic isorotation in a steady axisymmetric wind
- Torsional Alfvén wave
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