In an isotropically conducting medium the electric field and current density are associated by Ohm's law. This, together with Maxwell's equations, leads to |∇²H=4π σ∂ H/∂ t\,-curl\,(υ × H)+c⁻²∂²H∂t²,| where H , υ and σ are the magnetic field, velocity of the medium and conductivity. This equation describes any electromagnetic field in a moving (or fixed) conductor. It includes the “telegraph equation” of radio waves and also describes any hydromagnetic wave. Ionized gas in a sufficiently strong magnetic field is anisotropically conducting and σ is replaced by a tensor. An equation analogous to the above is derived for these conditions, allowing the study of electromagnetic disturbances in a medium with Hall conductivity. The equation is used on some simple problems of astrophysical interest, including hydromagnetic waves.
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J. H. Piddington (1954) studied this question.