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(-2) 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(-2) Pa, in-plume power losses surpass 25% of the discharge energy flux. Given that the ionisation energy for Xe is 12 eV, the 8 eV threshold indicates that a consistent percentage of electrons has energy enough to trigger ionisation. 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 thruster are significant if the facility pressure is greater than 10(-3) 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(-3) Pa.

Andriulli R., Andrews S., Souhair N., Magarotto M., Ponti F. (2024). Fully kinetic study of facility pressure effects on RF-source magnetic nozzles. ACTA ASTRONAUTICA, 215, 362-372 [10.1016/j.actaastro.2023.12.014].

Fully kinetic study of facility pressure effects on RF-source magnetic nozzles

Andriulli R.
;
Andrews S.;Souhair N.;Magarotto M.;Ponti F.
2024

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(-2) 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(-2) Pa, in-plume power losses surpass 25% of the discharge energy flux. Given that the ionisation energy for Xe is 12 eV, the 8 eV threshold indicates that a consistent percentage of electrons has energy enough to trigger ionisation. 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 thruster are significant if the facility pressure is greater than 10(-3) 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(-3) Pa.
2024
Andriulli R., Andrews S., Souhair N., Magarotto M., Ponti F. (2024). Fully kinetic study of facility pressure effects on RF-source magnetic nozzles. ACTA ASTRONAUTICA, 215, 362-372 [10.1016/j.actaastro.2023.12.014].
Andriulli R.; Andrews S.; Souhair N.; Magarotto M.; Ponti F.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/969558
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