Hall magnetohydrodynamics of partially ionized plasmas
B. P. Pandey, Mark Wardle

TL;DR
This paper develops a unified single-fluid model for partially ionized plasmas, clarifying how the Hall effect influences plasma dynamics across different ionization regimes, with implications for space and astrophysical systems.
Contribution
It introduces an approximate single-fluid framework that accurately describes Hall effects in partially ionized plasmas, bridging fully-ionized and weakly-ionized limits.
Findings
Hall effect becomes significant when dynamical frequency exceeds a specific threshold.
Derived length scale depends on ion to bulk mass density ratio and Hall beta parameter.
Model includes ohmic, ambipolar, and Hall diffusion effects.
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…
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