# Poloidal–toroidal decomposition

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.

## Definition

For a three-dimensional vector field F with zero divergence

$\nabla \cdot \mathbf {F} =0,$

this F can be expressed as the sum of a toroidal field T and poloidal vector field P

$\mathbf {F} =\mathbf {T} +\mathbf {P}$

where r is a radial vector in spherical coordinates (r, θ, φ). The toroidal field is obtained from a scalar field, Ψ(r, θ, φ), as the following curl,

$\mathbf {T} =\nabla \times (\mathbf {r} \Psi (\mathbf {r} ))$

and the poloidal field is derived from another scalar field Φ(r, θ, φ), as a twice-iterated curl,

$\mathbf {P} =\nabla \times (\nabla \times (\mathbf {r} \Phi (\mathbf {r} )))\,.$

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.

## Geometry

A toroidal vector field is tangential to spheres around the origin,

$\mathbf {r} \cdot \mathbf {T} =0$

while the curl of a poloidal field is tangential to those spheres

$\mathbf {r} \cdot (\nabla \times \mathbf {P} )=0.$ 

The poloidal–toroidal decomposition is unique if it is required that the average of the scalar fields Ψ and Φ vanishes on every sphere of radius r.

## 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

$\mathbf {F} (x,y,z)=\nabla \times g(x,y,z){\hat {\mathbf {z} }}+\nabla \times (\nabla \times h(x,y,z){\hat {\mathbf {z} }})+b_{x}(z){\hat {\mathbf {x} }}+b_{y}(z){\hat {\mathbf {y} }},$

where ${\hat {\mathbf {x} }},{\hat {\mathbf {y} }},{\hat {\mathbf {z} }}$  denote the unit vectors in the coordinate directions.