Magnetic helicity transport in the advective gauge family
arXiv:1010.6177 · doi:10.1063/1.3533656
Abstract
Magnetic helicity fluxes are investigated in a family of gauges in which the contribution from ideal magnetohydrodynamics takes the form of a purely advective flux. Numerical simulations of magnetohydrodynamic turbulence in this advective gauge family exhibit instabilities triggered by the build-up of unphysical irrotational contributions to the magnetic vector potential. As a remedy, the vector potential is evolved in a numerically well behaved gauge, from which the advective vector potential is obtained by a gauge transformation. In the kinematic regime, the magnetic helicity density evolves similarly to a passive scalar when resistivity is small and turbulent mixing is mild, i.e. when the fluid Reynolds number is not too large. In the dynamical regime, resistive contributions to the magnetic helicity flux in the advective gauge are found to be significant owing to the development of small length scales in the irrotational part of the magnetic vector potential.
11 pages, 10 figures, submitted to Physics of Plasmas
References in corpus (7)
- Simulations of nonhelical hydromagnetic turbulence
- Persistent Magnetic Wreaths in a Rapidly Rotating Sun
- Galactic dynamo and helicity losses through fountain flow
- Small-scale magnetic helicity losses from a mean-field dynamo
- Magnetic helicity fluxes in an alpha-squared dynamo embedded in a halo
- Magnetic helicity flux in the presence of shear
- Dissipation in dynamos at low and high magnetic Prandtl numbers
Cited by in corpus (22)
- Current status of turbulent dynamo theory: From large-scale to small-scale dynamos
- Advances in mean-field dynamo theory and applications to astrophysical turbulence
- Magnetic Prandtl number dependence of kinetic to magnetic dissipation ratio
- Galactic spiral patterns and dynamo action I: A new twist on magnetic arms
- Dynamo-driven plasmoid ejections above a spherical surface
- Nonlinear small-scale dynamos at low magnetic Prandtl numbers
- Catastrophic quenching in alpha-Omega dynamos revisited
- Turbulent dynamo with advective magnetic helicity flux
- Decay of helical and non-helical magnetic knots
- Magnetic Helicity and Large Scale Magnetic Fields: A Primer
- Scaling of the Hosking integral in decaying magnetically-dominated turbulence
- Galactic Spiral Patterns and Dynamo Action II: Asymptotic Solutions
- Oscillatory large-scale dynamos from Cartesian convection simulations
- A Vector Potential implementation for Smoothed Particle Magnetohydrodynamics
- Orbital advection with magnetohydrodynamics and vector potential
- Comparison Between Turbulent Helical Dynamo Simulations and a Nonlinear Three-Scale Theory
- Robustness of oscillatory dynamos in spherical wedges
- Analytic solution of an oscillatory migratory alpha^2 stellar dynamo
- A global galactic dynamo with a corona constrained by relative helicity
- Magnetic helicity and fluxes in an inhomogeneous alpha squared dynamo
- Magnetic helicity fluxes in dynamos from rotating inhomogeneous turbulence
- From convective to stellar dynamos