Theory of the collisional presheath in an oblique magnetic field

K.‐U. Riemann

Physics of Plasmas · 1994 · 178 citations · 11 references

Concepts

TL;DR

In the limit of a small Debye length, the plasma boundary layer near a negative wall splits into a collision‑free sheath and a quasineutral presheath where ions accelerate to the sound speed, and presheath dynamics depend on collisional friction, ionization, geometry, or a magnetic field nearly parallel to the wall, leading to contradictory conclusions for field‑aligned versus collisional transport. To obtain a coherent picture, a hydrodynamic model of the presheath that incorporates an oblique magnetic field and collisions is investigated. The model treats ion dynamics hydrodynamically, incorporating an oblique magnetic field and collisional effects to describe presheath transport. The limiting cases are discussed, showing that presheath ion acceleration always depends on elementary processes, and that a strong magnetic field compresses the collisional presheath into a thin layer of order the ion gyroradius.

Abstract

In the limit of a small Debye length (λD→0), the plasma boundary layer in front of a negative absorbing wall is split up into a collision-free planar space charge sheath and a quasineutral presheath, where the ions are accelerated to ion sound speed (Bohm criterion). Usually the presheath mechanism depends decisively on collisional friction of the ions, on ionization, or on geometric ion current concentration. If the ion dynamics in the presheath is dominated by a magnetic field (nearly) parallel to the wall, an additional effect must be considered to provide an ion transport to the wall. The special cases (a) of an ion transport by field lines intersecting the wall at a finite angle and (b) of an ion transport by collisions result in somewhat contradictory conclusions. To get a coherent picture, a hydrodynamic model of the presheath is investigated accounting for an oblique magnetic field and for collisions. The limiting cases (a) and (b) are discussed, and it is shown that (in plane geometry) the presheath ion acceleration depends always on elementary processes. The main effect of a strong magnetic field is to ‘‘compress’’ the collisional presheath into a thin layer with a characteristic extension of the ion gyroradius ρi.

References

11