Fully kinetic study of facility pressure effects on RF-source magnetic nozzles
Abstract
A fully kinetic 2D axisymmetric Particle-in-Cell (PIC) model is used to examine the effects of background facility pressure on the plasma transport and propulsive efficiency of magnetic nozzles. Simulations are performed for a low-power (150 W class) cathode-less radio-frequency (RF) plasma thruster, operating with xenon, between background pressures up to 10 Pa and average electron discharge temperatures of 4 - 16 eV. When the electron temperature within the near-plume region reaches 8 eV, a decisive reduction in performance occurs: at 10 Pa, in-plume power losses surpass 25% of the discharge energy flux. Given that the ionization energy for Xe is 12 eV, the 8 eV threshold indicates that a consistent percentage of electrons has energy enough to trigger ionization. On the other hand, when the temperature is below such threshold, the primary collisions are charge-exchange and inelastic ion scattering, and the power loss remains less than 10%. It is established that losses in the considered HPT are significant if the facility pressure is greater than 10 Pa, at absorbed powers larger than 130 W. At the nominal 150 W, this results in a 15% thrust reduction. When facility pressure is taken into consideration over ideal vacuum simulations, numerical error is reduced to <30% when compared to experimental thrust measurements at 10 Pa.
Keywords
Cite
@article{arxiv.2310.16264,
title = {Fully kinetic study of facility pressure effects on RF-source magnetic nozzles},
author = {Raoul Andriulli and Shaun Andrews and Nabil Souhair and Mirko Magarotto and Fabrizio Ponti},
journal= {arXiv preprint arXiv:2310.16264},
year = {2023}
}
Comments
45 pages, 10 figures, 5 tables. Submitted to Acta Astronautica