English

The Parker Magnetostatic Theorem

Solar and Stellar Astrophysics 2015-05-18 v1

Abstract

We demonstrate the Parker Magnetostatic Theorem in terms of a small neighborhood in solution space containing continuous force-free magnetic fields in small deviations from the uniform field. These fields are embedded in a perfectly conducting fluid bounded by a pair of rigid plates where each field is anchored, taking the plates perpendicular to the uniform field. Those force-free fields obtainable from the uniform field by continuous magnetic footpoint displacements at the plates have field topologies that are shown to be a restricted subset of the field topologies similarly created without imposing the force-free equilibirum condition. The theorem then follows from the deduction that a continuous nonequilibrum field with a topology not in that subset must find a force-free state containing tangential discontinuities.

Keywords

Cite

@article{arxiv.1002.4399,
  title  = {The Parker Magnetostatic Theorem},
  author = {B. C. Low},
  journal= {arXiv preprint arXiv:1002.4399},
  year   = {2015}
}

Comments

13 pages, no figure

R2 v1 2026-06-21T14:50:23.028Z