Poloidal–toroidal decomposition
From Wikipedia, the free encyclopedia
In vector calculus, a topic in pure and applied mathematics, a poloidal–toroidal decomposition is a restricted form of the Helmholtz decomposition. It is often used in the spherical coordinates analysis of solenoidal vector fields, for example, magnetic fields and incompressible fluids.[1]
Definition
For a three-dimensional vector field F with zero divergence
this can be expressed as the sum of a toroidal field and poloidal vector field
where is a radial vector in spherical coordinates . The toroidal field is obtained from a scalar field,,[2] as the following curl,
and the poloidal field is derived from another scalar field ,[3] as a twice-iterated curl,
This decomposition is symmetric in that the curl of a toroidal field is poloidal, and the curl of a poloidal field is toroidal, known as Chandrasekhar–Kendall function.[4]
Geometry
Cartesian decomposition
A poloidal–toroidal decomposition also exists in Cartesian coordinates, but a mean-field flow has to be included in this case. For example, every solenoidal vector field can be written as
where denote the unit vectors in the coordinate directions.[6]