Logarithmic Separable Solutions of Force-Free Magnetic Fields in Plane-Parallel and Axial Symmetry
arXiv:2501.15232 · doi:10.3390/sym17020175
Abstract
This work introduces a systematic method for identifying analytical and semi-analytical solutions of force-free magnetic fields with plane-parallel and axial symmetry. The method of separation of variables is used, allowing the transformation of the non-linear partial differential equation, corresponding to force-free magnetic fields, to a system of decoupled ordinary differential equations, which nevertheless, are in general non-linear. It is then shown that such solutions are feasible for configurations where the electric current has a logarithmic dependence to the magnetic field flux. The properties of the magnetic fields are studied for a variety of physical parameters, through solution of the systems of the ordinary differential equations for various values of the parameters. It is demonstrated that this new logarithmic family of solutions has properties that are highly distinct from the known linear and non-linear equations, as it allows for bounded solutions of magnetic fields, for periodic solutions and for solutions that extend to infinity. Possible applications to astrophysical fields and plasmas are discussed as well as their use in numerical studies, and the overall enrichment of our understanding of force-free configurations.
References in corpus (23)
- Magnetic fields of non-degenerate stars
- The Axisymmetric Pulsar Magnetosphere
- A strong magnetic field around the supermassive black hole at the centre of the Galaxy
- Effects of Strong Magnetic Fields on Neutron Star Structure
- On Why Disks Generate Magnetic Towers and Collimate Jets
- Nonlinear force-free modeling of the solar coronal magnetic field
- Helical Magnetic Fields Associated with the Relativistic Jets of Four BL Lac Objects
- High-accuracy estimation of magnetic field strength in the interstellar medium from dust polarization
- Global Non-Potential Magnetic Models of the Solar Corona During the March 2015 Eclipse
- The contrasting magnetic fields of superconducting pulsars and magnetars
- Magnetic Jets from Swirling Disks
- Fields from a relativistic magnetic explosion
- Three-dimensional magnetohydrodynamical simulations of the morphology of head-tail radio galaxies based on magnetic tower jet model
- Structure of magnetic fields in intracluster cavities
- Relativistic expansion of a magnetized fluid
- Magnetic field structure of relativistic jets without current sheets
- Strongly magnetized pulsars: explosive events and evolution
- 3D MHD Simulations of Laboratory Plasma Jets
- Self-Similar Magnetic Arcades
- Arnold diffusion of charged particles in ABC magnetic fields
- Three-dimensional kinetic simulations of relativistic magnetostatic equilibria
- Investigating magnetically-induced distortions of neutron stars through gamma-ray burst X-ray plateaus
- Relativistically expanding cylindrical electromagnetic fields