There are three components of a conductivity tensor in atmospheric electrodynamics: the parallel conductivity along the direction of the magnetic field, the Pedersen conductivity (in the direction of the polarization electric field but perpendicular to the magnetic field), and the Hall conductivity (perpendicular to both the polarization electric field and the magnetic field).
It makes sense that if there’s an electric field along the magnetic field, it will induce a current in that direction. But what about the Pedersen and Hall currents? What is going on? What causes them?
Answer
It makes sense that if there’s an electric field along a magnetic field line, it will induce a current in that direction. But what about the Pedersen and Hall currents? What is going on? What causes them?
The three ionospheric conductivities derive from electric fields at an oblique but not exactly perpendicular angle to the background magnetic field (i.e., Earth's magnetic field).
The Hall term derives from the Hall effect, namely the drift induced by a finite value for E×B, called the ExB-drift. That it is a finite and not infinite conductivity results from charge-neutral, charge-charge collisions (i.e., Coulomb collisions between charged and neutral and/or charged species).
The Pederson conductivity does correspond to the component parallel to E, but it results from a combination of Coulomb collisions (similar to the Hall term) and drifts induced by E. To understand this more clearly, we need to examine their mathematical form.
Suppose we define the total collision frequency of species s as: νs=νsn+νss′
From a dimensional analysis point of view (and one of the simplest form of Ohm's law), a conductivity can be expressed as: σs=ns q2sms νs
The Hall and Pederson conductivities (assuming ne=ni) can be expressed as (after a bunch of algebra): σP=n e2(νeme1ν2e+Ω2ce+νimi1ν2i+Ω2ci)σH=n e2(Ωceme1ν2e+Ω2ce+Ωceme1ν2e+Ω2ce)
We can now see some of the physical implications of these conductivities by looking for the conditions that maximize them. One can see that σP maximizes when νi∼Ωci, or the ions experience roughly one collision per gyration which randomize their trajectories and lead to a net bulk flow along E. Conversely, σP increases with increasing νi, i.e., for large νi the ions collide so frequently that they cannot undergo an ExB-drift causing them to stay nearly stationary while the electrons freely undergo an ExB-drift. Thus, the electrons carry the current in the opposite direction to that of E×B.
Finally, the parallel conductivity is largely a result of the higher mobility of particles along vs. across B. σ∥ goes to infinity in the limit that νi→0, though on average σ∥ is already much much larger than both σP and σH. Thus, it is generally approximated to infinite for simplicity.
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