PreprintCC BY 4.0arXiv
Exact nonsymmetric vacuum magnetic field with nested toroidal flux surfaces and nonzero rotational transform
Abstract
We show that an exact vacuum magnetic field without continuous Euclidean symmetry can fill a bounded solid torus with nested toroidal flux surfaces and nonzero rotational transform. We construct such a field in closed form and show that it is nowhere vanishing. Every off-axis field line closes after one toroidal transit and one poloidal turn, with rotational transform ι=−1 on every flux surface. The solution provides an exact benchmark for three-dimensional equilibrium codes.
Related
- Exact Nonsymmetric Vacuum Magnetic Fields with Nested Toroidal Surfaces
- Analytic toroidal 3D MHD equilibria and steady Euler flows with invariant surfaces
- Noninvasive Anisotropic Identification of Magnetic Properties in Toroidal Shaped Magnetic Steel
- Helicon wave propagation, plasma generation and interaction with low-frequency waves in toroidal magnetic configurations
- Odd-Parity Crystalline Electric Field and Multipoles in Icosahedral Quasicrystal and Approximant: Magnetic Toroidal and Electric Dipoles in Ce-Based Systems
BibTeX
@misc{lopez2026exact,
title = {{Exact nonsymmetric vacuum magnetic field with nested toroidal flux surfaces and nonzero rotational transform}},
author = {Omar E. López},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.29921},
eprint = {2610.29921},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.29921},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Exact nonsymmetric vacuum magnetic field with nested toroidal flux surfaces and nonzero rotational transform
AU - Omar E. López
PY - 2026
DA - 2026/10/21
PB - arXiv
DO - 10.48550/arxiv.2610.29921
UR - https://arxiv.org/abs/2610.29921
AB - We show that an exact vacuum magnetic field without continuous Euclidean symmetry can fill a bounded solid torus with nested toroidal flux surfaces and nonzero rotational transform. We construct such a field in closed form and show that it is nowhere vanishing. Every off-axis field line closes after one toroidal transit and one poloidal turn, with rotational transform ι=−1 on every flux surface. The solution provides an exact benchmark for three-dimensional equilibrium codes.
ER -