English

Well-posedness of some initial-boundary-value problems for dynamo-generated poloidal magnetic fields

Solar and Stellar Astrophysics 2012-12-14 v1 Earth and Planetary Astrophysics Analysis of PDEs

Abstract

Given a bounded domain GRdG \subset \R^d, d3d\geq 3, we study smooth solutions of a linear parabolic equation with non-constant coefficients in GG, which at the boundary have to C1C^1-match with some harmonic function in Rd\ovG\R^d \setminus \ov{G} vanishing at spatial infinity. This problem arises in the framework of magnetohydrodynamics if certain dynamo-generated magnetic fields are considered: For example, in the case of axisymmetry or for non-radial flow fields, the poloidal scalar of the magnetic field solves the above problem. We first investigate the Poisson problem in GG with the above described boundary condition as well as the associated eigenvalue problem and prove the existence of smooth solutions. As a by-product we obtain the completeness of the well-known poloidal "free decay modes" in R3\R^3 if GG is a ball. Smooth solutions of the evolution problem are then obtained by Galerkin approximation based on these eigenfunctions.

Keywords

Cite

@article{arxiv.1212.3180,
  title  = {Well-posedness of some initial-boundary-value problems for dynamo-generated poloidal magnetic fields},
  author = {Ralf Kaiser and Hannes Uecker},
  journal= {arXiv preprint arXiv:1212.3180},
  year   = {2012}
}

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Corrected version

R2 v1 2026-06-21T22:53:58.712Z