The CAMILA (co-axial magneto-isolated longitudinal anode) concept was introduced to improve the efficiency and the lifetime of low-power Hall thrusters (≤ 350 W). CAMILA represents a significant departure from conventional Hall thrusters and has not been yet thoroughly studied. The high efficiency of the thruster, as validated by measurements, increases the need for better understanding of the physical processes in this type of thruster. For this aim, an analysis of the CAMILA discharge based on experimental measurements was conducted. The experimental setup includes electrical probes mounted on a fast moving positioner, enabling to obtain the spatial distribution of plasma parameters inside the thruster channel. The results confirmed the basic assumptions used in the physical model of the CAMILA concept and revealed new phenomena related to the radial non-uniformity of the discharge. In particular, focusing equipotentials were discovered not only in the anode cavity, but in the dielectric channel as well, where the area of intense ionization was located. The physical processes contributing to the formation of the focusing equipotentials are discussed.
Nomenclature
A chCross sectional area of the channel, m 2 BMagnetic field, T eUnit charge, C E curv Electric field due to curvature drift, V/mm E ∇B,tot Electric field due to grad-B drifts, V/mm E mirror,rθ Electric field due to the magnetic mirror effect in the r-θ plane, V/mm E r,mirror Electric field due to the magnetic mirror effect in the r-z plane, V/mm I M Mass flow rate current, A