Hall magnetohydrodynamics of partially ionized plasmas
arXiv:0707.2688 · doi:10.1111/j.1365-2966.2008.12998.x
Abstract
The Hall effect arises in a plasma when electrons are able to drift with the magnetic field but ions cannot. In a fully-ionized plasma this occurs for frequencies between the ion and electron cyclotron frequencies because of the larger ion inertia. Typically this frequency range lies well above the frequencies of interest (such as the dynamical frequency of the system under consideration) and can be ignored. In a weakly-ionized medium, however, the Hall effect arises through a different mechanism -- neutral collisions preferentially decouple ions from the magnetic field. This typically occurs at much lower frequencies and the Hall effect may play an important role in the dynamics of weakly-ionised systems such as the Earth's ionosphere and protoplanetary discs. To clarify the relationship between these mechanisms we develop an approximate single-fluid description of a partially ionized plasma that becomes exact in the fully-ionized and weakly-ionized limits. Our treatment includes the effects of ohmic, ambipolar, and Hall diffusion. We show that the Hall effect is relevant to the dynamics of a partially ionized medium when the dynamical frequency exceeds the ratio of ion to bulk mass density times the ion-cyclotron frequency, i.e. the Hall frequency. The corresponding length scale is inversely proportional to the ion to bulk mass density ratio as well as to the ion-Hall beta parameter.
11 page, 1 figure, typos removed, numbers in tables revised; accepted for publication in MNRAS
References in corpus (13)
- On the Generation, Propagation, and Reflection of Alfven Waves from the Solar Photosphere to the Distant Heliosphere
- Linear Analysis of the Hall Effect in Protostellar Disks
- The Balbus-Hawley instability in weakly ionised discs
- Magnetic fields in protoplanetary disks
- The conductivity of dense molecular gas
- The Effect of the Hall Term on the Nonlinear Evolution of the Magnetorotational Instability: II. Saturation Level and Critical Magnetic Reynolds Number
- The Effect of the Hall Term on the Nonlinear Evolution of the Magnetorotational Instability: I. Local Axisymmetric Simulations
- Quiet Sun magnetic fields at high spatial resolution
- Magnetorotational instability in protoplanetary discs
- Ionization, Magneto-rotational, and Gravitational Instabilities in Thin Accretion Disks Around Supermassive Black Holes
- Magnetorotational instability in stratified, weakly ionised accretion discs
- Ion dynamics and the magnetorotational instability in weakly-ionized discs
- Dynamo and Electrical Jet in Hall Plasmas, Application to Astrophysics
Cited by in corpus (89)
- Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics
- Heating of the magnetized solar chromosphere by partial ionization effects
- Partially Ionized Plasmas in Astrophysics
- Can non-ideal magnetohydrodynamics solve the magnetic braking catastrophe?
- 2D Radiative MHD Simulations of the Importance of Partial Ionization in the Chromosphere
- Hall diffusion and the magnetorotational instability in protoplanetary discs
- Fluid description of multi-component solar partially ionized plasma
- Collisions, magnetization, and transport coefficients in the lower solar atmosphere
- The initial conditions for planet formation: Turbulence driven by hydrodynamical instabilities in disks around young stars
- Connecting the Sun and the Solar Wind: The Self-consistent Transition of Heating Mechanisms
- Propagation of Alfvénic Waves From Corona to Chromosphere and Consequences for Solar Flares
- A fast and explicit algorithm for simulating the dynamics of small dust grains with smoothed particle hydrodynamics
- Magnetohydrodynamic Waves in a Partially Ionized Filament Thread
- Two-dimensional Radiative Magnetohydrodynamic Simulations of Partial Ionization in the Chromosphere. II. Dynamics and Energetics of the Low Solar Atmosphere
- Rayleigh-Taylor instability in prominences from numerical simulations including partial ionization effects
- Magnetohydrodynamics of the Weakly Ionized Solar Photosphere
- Energy transport and heating by torsional Alfvén waves propagating from the photosphere to the corona in the quiet Sun
- Overdamped Alfven waves due to ion-neutral collisions in the solar chromosphere
- Resonantly Damped Kink Magnetohydrodynamic Waves in a Partially Ionized Filament Thread
- Ambipolar diffusion in smoothed particle magnetohydrodynamics
- Low mass planet migration in magnetically torqued dead zones - I. Static migration torque
- Accretion in giant planet circumplanetary disks
- Magneto-thermal evolution of neutron stars with coupled Ohmic, Hall and ambipolar effects via accurate finite-volume simulations
- NICIL: A stand alone library to self-consistently calculate non-ideal magnetohydrodynamic coefficients in molecular cloud cores
- Numerical simulations of quiet Sun magnetic fields seeded by Biermann battery
- MHDSTS: a new explicit numerical scheme for simulations of partially ionised solar plasma
- The impact of non-ideal magnetohydrodynamics on binary star formation
- The Role of Partial Ionization Effects in the Chromosphere
- Asymmetric Magnetic Reconnection in Weakly Ionized Chromospheric Plasmas
- On the effects of ion-neutral interactions in solar plasmas
- Low mass planet migration in magnetically torqued dead zones - II. Flow-locked and runaway migration, and a torque prescription
- The universally growing mode in the solar atmosphere: coronal heating by drift waves
- Multi-fluid approach to high-frequency waves in plasmas. III. Nonlinear regime and plasma heating
- Fast-to-Alfvén Mode Conversion Mediated by Hall Current. I. Cold Plasma Model
- Radiation thermo-chemical models of protoplanetary disks. Grain and polycyclic aromatic hydrocarbon charging
- Damping mechanisms for oscillations in solar prominences
- The effect of extreme ionisation rates during the initial collapse of a molecular cloud core
- Cut-off wavenumber of Alfven waves in partially ionized plasmas of the solar atmosphere
- On the origin of magnetic fields in stars
- Dust segregation in Hall-dominated turbulent protoplanetary disks
- Multi-fluid Approach to High-frequency Waves in Plasmas. II. Small-amplitude Regime in Partially Ionized Media
- A Simflowny-based high-performance 3D code for the generalized induction equation
- Multi-fluid approach to high-frequency waves in plasmas: I. Small-amplitude regime in fully ionized medium
- The vertical shear instability in poorly ionised, magnetized protoplanetary discs
- Magnetized High Velocity Clouds in the Galactic Halo: A New Distance Constraint
- Primordial magnetic fields in Population III star formation: a magnetised resolution study
- Equilibrium configurations of charged fluid around Kerr black hole
- Joint action of Hall and ambipolar effects in 3D magneto-convection simulations of the quiet Sun. I. Dissipation and generation of waves
- Shaken and stirred: the effects of turbulence and rotation on disc and outflow formation during the collapse of magnetised molecular cloud cores
- Magnetorotational instability in magnetic diffusion dominated accretion discs
- On the origin of magnetic fields in stars II: The effect of numerical resolution
- Hall instability of solar flux tubes
- Coalescence Instability in Chromospheric Partially Ionised Plasmas
- Electric fields in solar magnetic structures due to gradient driven instabilities: heating and acceleration of particles
- Magneto-thermal condensation modes including the effects of charged dust particles
- On the interpretation of the apparent existence of a preferred magnetic polarity in extragalactic jet sources
- Magnetic diffusion driven shear instability of solar flux tubes
- Hall equilibrium of thin Keplerian disks embedded in mixed poloidal and toroidal magnetic fields
- Thermal instability in ionized plasma
- Can Hall effect trigger Kelvin-Helmholtz instability in sub-Alfvenic flows?
- Shear-driven instabilities in Hall-MHD plasmas
- Electrically charged matter in permanent rotation around magnetized black hole: A toy model for self-gravitating fluid tori
- Efficient kinetic Lattice Boltzmann simulation of three-dimensional Hall-MHD Turbulence
- Influence of ambipolar and Hall effects on vorticity in 3D simulations of magneto-convection
- Ambipolar Diffusion in the Lower Solar Atmosphere: MHD Simulations of a Sunspot
- Efficient numerical treatment of ambipolar and Hall drift as hyperbolic system
- Two-dimensional partially ionized magnetohydrodynamic turbulence
- Taming Hamiltonian systems with balanced loss and gain via Lorentz interaction : General results and a case study with Landau Hamiltonian
- The non-ideal finite Larmor radius effect in the solar atmosphere
- Charged grains and Kelvin Helmholtz instability in molecular clouds
- Surface Wave Propagation in non--ideal plasmas
- MHD waves and instabilities in flowing solar structures in the framework of Hall magnetohydrodynamics
- Wave Conversion, Decay and Heating in a Partially Ionized Two-Fluid Magneto-Atmosphere
- Surface Waves in the paritally ionized solar plasma slab
- OpenFOAM computational fluid dynamics (CFD) solver for magnetohydrodynamic open cycles, applied to the Sakhalin pulsed magnetohydrodynamic generator (PMHDG)
- Normal mode analysis of fluid discontinuities: numerical method and application to magnetohydrodynamics
- Viscous Heating and Instabilities in the Partially Ionized Solar Atmosphere
- Hall-magnetohydrodynamic waves in flowing ideal incompressible solar-wind plasmas: Reconsidered
- Spectral Analysis of Non-Ideal MRI Modes: The effect of Hall diffusion
- Resistive Hot Accretion Flows with Anisotropic Pressure
- Wave Topology in Hall MHD
- MHD waves in the partially ionized plasma: from single to multi-fluid approach
- Low mass planet migration in Hall-affected disks
- Coupling of Alfvén and magnetosonic waves in rotating Hall magnetoplasmas
- Kelvin--Helmholtz instability in a cool solar jet in the framework of Hall magnetohydrodynamics: A case study
- Smoothed Particle Magnetohydrodynamics: A State of the Union
- Global Non-Axisymmetric Hall Instabilities in a Rotating Plasma
- Non-ideal MHD and protostellar feedback effects on disc formation and evolution in numerical simulations of star cluster formation
- A Theory about Electric Current and Heating in Plasma