Distribution of high-energy backflow ions near cathode plume in microwave discharge ion thruster

Y Yasuaki Aiba (Space and Astronautical Science, Graduate Institute for Advanced Studies, SOKENDAI 1 , Sagamihara, Kanagawa 252-5210,) M Marco Riccardo Inchingolo (Aerospace Engineering Department, Universidad Carlos III de Madrid 2 , Leganés, Madrid 28911,) R Rémi Pigret (Department of Space Systems Engineering (ELS – Space, Launchers and Satellites), IPSA—Institut Polytechnique des Sciences Avancées 3 , Ivry-sur-Seine, Val-de-Marne 94200,) T Takato Morishita (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA) 4 , Sagamihara, Kanagawa 252-5210,) Y Yusuke Yamashita (National Museum of Japanese History) R Ryudo Tsukizaki (Space and Astronautical Science, Graduate Institute for Advanced Studies, SOKENDAI 1 , Sagamihara, Kanagawa 252-5210,) K Kazutaka Nishiyama (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA) 4 , Sagamihara, Kanagawa 252-5210,)

Abstract

Backflowing ions generated by electric thrusters are known to cause sputtering and surface degradation on spacecraft, which may ultimately shorten mission lifetimes. In this study, velocity measurements for metastable xenon ions were conducted near the cathode plume of the microwave discharge ion thruster μ10 using the laser-induced fluorescence technique. In addition, a spatial distribution of plasma potential was measured by an emissive probe. The ion velocity distribution functions showed different features depending on the measurement position. The mean velocity of the drifting population at each measurement position was visualized as a velocity field. A comparison of the velocity field with the plasma potential distribution or ion number density distribution revealed a diverging center that coincided with the cathode plume, suggesting that a certain number of backflow ions originated from the cathode plume region. In particular, high-energy ions were observed between the cathode plume and the spacecraft surface. Asymmetric features were found in both the plasma potential distribution and the ion number density distribution, which implies that the effect of the magnetic field is not negligible in this region.

Article Details

Volume / Issue Vol. 139, Issue 15
Published April 21, 2026
ISSN 0021-8979
Publisher American Institute of Physics

Journal Info

Journal of Applied Physics

American Institute of Physics

ISSN: 0021-8979 Physical Sciences

Authors (7)

Y

Yasuaki Aiba

Space and Astronautical Science, Graduate Institute for Advanced Studies, SOKENDAI 1 , Sagamihara, Kanagawa 252-5210,

M

Marco Riccardo Inchingolo

Aerospace Engineering Department, Universidad Carlos III de Madrid 2 , Leganés, Madrid 28911,

R

Rémi Pigret

Department of Space Systems Engineering (ELS – Space, Launchers and Satellites), IPSA—Institut Polytechnique des Sciences Avancées 3 , Ivry-sur-Seine, Val-de-Marne 94200,

T

Takato Morishita

Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA) 4 , Sagamihara, Kanagawa 252-5210,

Y

Yusuke Yamashita

National Museum of Japanese History

R

Ryudo Tsukizaki

Space and Astronautical Science, Graduate Institute for Advanced Studies, SOKENDAI 1 , Sagamihara, Kanagawa 252-5210,

K

Kazutaka Nishiyama

Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA) 4 , Sagamihara, Kanagawa 252-5210,