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Poloidal–toroidal decomposition
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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

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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

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A toroidal vector field is tangential to spheres around the origin,[4]

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

[5]

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.[3]

Cartesian decomposition

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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]

See also

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Notes

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References

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