TY - GEN
T1 - Numerical Investigation of Carbon Sputtering and Transport for the Ion Thruster Testing in the Ground Facility
AU - Nishii, Keita
AU - Levin, Deborah A.
N1 - This work was partially supported by NASA through the Joint Advanced Propulsion Institute, a NASA Space Technology Research Institute, grant number 80NSSC21K1118. Thiswork used Expanse at the San Diego Supercomputer Center and Delta at the National Center for Supercomputing Applications through allocation TG-PHY220010 from the Advanced Cyberinfrastructure Coordination Ecosystem: Services & Support (ACCESS) program, which is supported by National Science Foundation grants #2138259, #2138286, #2138307, #2137603, and #2138296.
PY - 2023
Y1 - 2023
N2 - Carbon contamination due to backsputtering in an electric propulsion (EP) facility is a well-known concern in EP testing. Numerical simulation is a strong tool to isolate the facility effects from on-orbit performance and increase in wear characteristics as EP systems evolve toward larger power levels. This study uses particle-in-cell (PIC) and direct simulation Monte Carlo (DSMC) simulation results to study carbon backsputtering in a simplified vacuum chamber using a thruster modeled in our previous studies with new PIC and ion-surface interaction models. We investigate how the ion plume changes in a fully kinetic PIC simulation in addition to the quasi-neutral case that is commonly used. Ions, including those that have experienced MEX and CEX collisions, are sampled when they hit the vacuum chamber wall to understand the dynamics of backsputtering. In addition, we evaluate the impact of the ion-surface interaction model on the backsputtering rate on the thruster face by comparing theoretical semi-empirical expressions that have been used to fit past measurements with the classical cosine distribution. As a result, while the backsputtering rate is largely independent of differences in the PIC model, differences in the sputtering model have a significant impact.
AB - Carbon contamination due to backsputtering in an electric propulsion (EP) facility is a well-known concern in EP testing. Numerical simulation is a strong tool to isolate the facility effects from on-orbit performance and increase in wear characteristics as EP systems evolve toward larger power levels. This study uses particle-in-cell (PIC) and direct simulation Monte Carlo (DSMC) simulation results to study carbon backsputtering in a simplified vacuum chamber using a thruster modeled in our previous studies with new PIC and ion-surface interaction models. We investigate how the ion plume changes in a fully kinetic PIC simulation in addition to the quasi-neutral case that is commonly used. Ions, including those that have experienced MEX and CEX collisions, are sampled when they hit the vacuum chamber wall to understand the dynamics of backsputtering. In addition, we evaluate the impact of the ion-surface interaction model on the backsputtering rate on the thruster face by comparing theoretical semi-empirical expressions that have been used to fit past measurements with the classical cosine distribution. As a result, while the backsputtering rate is largely independent of differences in the PIC model, differences in the sputtering model have a significant impact.
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U2 - 10.2514/6.2023-0065
DO - 10.2514/6.2023-0065
M3 - Conference contribution
AN - SCOPUS:85197674263
SN - 9781624106996
T3 - AIAA SciTech Forum and Exposition, 2023
BT - AIAA SciTech Forum and Exposition, 2023
PB - American Institute of Aeronautics and Astronautics Inc, AIAA
T2 - AIAA SciTech Forum and Exposition, 2023
Y2 - 23 January 2023 through 27 January 2023
ER -