xmlui.dri2xhtml.METS-1.0.item-contributor-funder:
Ministerio de Economía y Competitividad (España)
Sponsor:
The authors would like to thank the support and use of the facilities at the Electric Propulsion Laboratory at ESTEC. This work was performed in the framework of the ‘Model and Experimental validation of spacecraft-thruster Interactions (erosion) for electric propulsion thrusters plumes’ (MODEX) project (ESA contract number 4000116180/15/NL/PS). MODEX is a collaboration between Airbus-DS, UC3M, ONERA, CNRS-ICARE and KTH aiming to provide a better understanding of the plasma properties in the far plume of a Hall thruster. Additional funding for M Merino and P Fajardo came from Project ESP2016-75887 (Spainʼs National Research and Development Plan—MINECO/FEDER).
Project:
Gobierno de España. ESP2016-75887-P
Keywords:
Electric propulsion
,
Hall effect thrusters
,
Kinetic models
,
Collisionless plasma
,
Plasma plumes
A central challenge in the modeling of the near-collisionless expansion of a plasma thruster plume into vacuum is the inadequacy of traditional fluid closure relations for the electron species, such as isothermal or adiabatic laws, because the electron responsA central challenge in the modeling of the near-collisionless expansion of a plasma thruster plume into vacuum is the inadequacy of traditional fluid closure relations for the electron species, such as isothermal or adiabatic laws, because the electron response in the plume is essentially kinetic and global. This work presents the validation of the kinetic plasma plume model presented in (Merino et al 2018 Plasma Sources Sci. Technol. 27 035013) against the experimental plume measurements of a SPT-100-ML Hall thruster running on xenon presented in (Giono et al 2018 Plasma Sources Sci. Technol. 27 015006). The model predictions are compared against the experimentally-determined axial profiles of electric potential, electron density, and electron temperature, and the radial electric potential profile, for 6 different test cases, in the far expansion region between 0.5 and 1.5 m away from the thruster exit. The model shows good agreement with the experimental data and the error is within the experimental uncertainty. The extrapolation of the model to the thruster exit plane and far downstream is consistent with the expected trends with varying discharge voltage and mass flow rate. The lumped-model value of the polytropic cooling exponent gamma is similar for all test cases and varies in the range 1.26-1.31.[+][-]