Stability of magnetic configurations containing the toroidal and axial fields
arXiv:0710.4588 · doi:10.1051/0004-6361:20077476
Abstract
Stability properties of magnetic-field configurations containing the toroidal and axial field are considered. The stability is treated by making use of linear analysis. It is shown that the conditions required for the onset of instability are essentially different from those given by the necessary condition , where is the cylindrical radius. The growth rate of instability is calculated for a wide range of the parameters. We argue that the instability can operate in two different regimes depending on the strength of the axial field and the profile of the toroidal field.
arXiv comment8 pages, 7 figures, A&A, to appear
References in corpus (5)
Cited by in corpus (25)
- Axisymmetric magnetic fields in stars: relative strengths of poloidal and toroidal components
- Maximum gravitational-wave energy emissible in magnetar flares
- On the Stability of Non Force-Free Magnetic Equilibria in Stars
- Axisymmetric and stationary structures of magnetized barotropic stars with extremely strong magnetic fields deep inside
- Non-axisymmetric instability of axisymmetric magnetic fields
- Breakdown of chiral symmetry during saturation of the Tayler instability
- Stably stratified magnetized stars in general relativity
- The magnetohydrodynamic instability of current-carrying jets
- Helicity and dynamo action in magnetized stellar radiation zones
- Stability of the toroidal magnetic field in stellar radiation zones
- Resonance instability of axially-symmetric magnetostatic equilibria
- Solar Dynamo and Toroidal Field Instabilities
- Magnetic fields in massive spirals: The role of feedback and initial conditions
- Rotational suppression of the Tayler instability in stellar radiation zones
- Stably stratified stars containing magnetic fields whose toroidal components are much larger than the poloidal ones in general relativity: A perturbation analysis
- Stability of the toroidal magnetic field in rotating stars
- Force-free pulsar magnetosphere: instability and generation of MHD waves
- Migrating Dynamo Waves and Consequences for Stellar Current Sheets
- Formation of filament-like structures in the pulsar magnetosphere and the short-term variability of pulsar emission
- Element spots in Ap- and HgMn-stars from current-driven diffusion
- Current-driven instabilities in weakly ionized disks
- Diffusion in plasma: the Hall effect, compositional waves, and chemical spots
- Gravity's role in taming the Tayler instability in red giant cores
- Compositional waves and variations in the atmospheric abundances of magnetic stars
- The magnetorotational and Tayler instabilities in the pulsar magnetosphere