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Chandrasekhar–Kendall function

Chandrasekhar–Kendall functions are the eigenfunctions of the curl operator derived by Subrahmanyan Chandrasekhar and P. C. Kendall in 1957 while attempting to solve the force-free magnetic fields. The functions were independently derived by both, and the two decided to publish their findings in the same paper.

Derivation
Taking curl of the equation \nabla\times\mathbf{H}=\lambda\mathbf{H} and using this same equation, we get :\nabla\times(\nabla\times\mathbf{H}) = \lambda^2\mathbf{H}. In the vector identity \nabla \times \left( \nabla \times \mathbf{H} \right) = \nabla(\nabla \cdot \mathbf{H}) - \nabla^{2}\mathbf{H}, we can set \nabla\cdot\mathbf{H}=0 since it is solenoidal, which leads to a vector Helmholtz equation, :\nabla^2\mathbf{H}+\lambda^2\mathbf{H}=0. Every solution of above equation is not the solution of original equation, but the converse is true. If \psi is a scalar function which satisfies the equation \nabla^2\psi + \lambda^2\psi=0, then the three linearly independent solutions of the vector Helmholtz equation are given by :\mathbf{L} = \nabla\psi,\quad \mathbf{T} = \nabla\times\psi\mathbf{\hat n}, \quad \mathbf{S} = \frac{1}{\lambda}\nabla\times\mathbf{T} where \mathbf{\hat n} is a fixed unit vector. Since \nabla\times\mathbf{S} =\lambda\mathbf{T}, it can be found that \nabla\times(\mathbf{S}+\mathbf{T})=\lambda(\mathbf{S}+\mathbf{T}). But this is same as the original equation, therefore \mathbf{H}=\mathbf{S}+\mathbf{T}, where \mathbf{S} is the poloidal field and \mathbf{T} is the toroidal field. Thus, substituting \mathbf{T} in \mathbf{S}, we get the most general solution as :\mathbf{H} = \frac{1}{\lambda}\nabla\times(\nabla\times\psi\mathbf{\hat n}) + \nabla \times \psi \mathbf{\hat n}. ==Cylindrical polar coordinates==
Cylindrical polar coordinates
Taking the unit vector in the z direction, i.e., \mathbf{\hat n}=\mathbf{e}_z, with a periodicity L in the z direction with vanishing boundary conditions at r=a, the solution is given by :\psi = J_m(\mu_jr)e^{im\theta+ikz}, \quad \lambda =\pm(\mu_j^2+k^2)^{1/2} where J_m is the Bessel function, k=\pm 2\pi n/L, \ n = 0,1,2,\ldots, the integers m =0,\pm 1,\pm 2,\ldots and \mu_j is determined by the boundary condition a k\mu_j J_m'(\mu_j a)+m \lambda J_m(\mu_j a) =0. The eigenvalues for m=n=0 has to be dealt separately. Since here \mathbf{\hat n}=\mathbf{e}_z, we can think of z direction to be toroidal and \theta direction to be poloidal, consistent with the convention. ==See also==
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