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Low frequency oscillation in the discharge channel of Hall thruster is an important physical phenomenon that affects its performance and stability. In this paper, the characteristics of low-frequency oscillation of the discharge current of Hall thruster and its suppression method are numerically studied by using a one-dimensional fluid model. Assuming that the discharge channel satisfies the quasi-neutral condition, the effects of electron-neutral collision, electron anomalous transport and electron-wall collision on conductivity are considered. The changes of plasma parameters and the effects of magnetic field, preionization rate, and atomic velocity on the amplitude and frequency of discharge current oscillation are also studied. Research results show that the variation of electron temperature in the discharge channel is closely related to the ionization process, and the electron temperature increases as the ionization intensity increases. The fluctuations in neutral gas flow rate and atomic density in the discharge process cause the ionization region to move forward and backward and the ionization intensity to change, which are the main driving forces for the low-frequency oscillation of discharge current in the channel. The magnetic field intensity in the discharge channel affects the axial current by influencing the electron mobility. With the increase of field strength, the oscillation frequency of current decreases, and under different magnetic field strengths, the current amplitude drops as the discharge voltage decreases. When the preionization rate of the working gas increases to above 4%, the amplitude of the discharge current oscillation gradually decreases. When the preionization rate is greater than 3% and the atomic velocity is less than 160 m/s, the discharge current oscillation in the channel exhibits damping attenuation, achieving a stabilizing effect which conduces to stabilizing the discharge of the Hall thruster.
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Keywords:
- low-frequency oscillation /
- fluid simulation /
- discharge characteristics /
- preionization rate
[1] Morozov A I 2003 Plasma Phys. Rep. 29 235Google Scholar
[2] 杨三祥, 王倩楠, 高俊, 贾艳辉, 耿海, 郭宁, 陈新伟, 袁兴龙, 张鹏 2022 71 105201Google Scholar
Yang S X, Wang Q N, Gao J, Jia Y H, Geng H, Guo N, Chen X W, Yuan X L, Zhang P 2022 Acta Phys. Sin. 71 105201Google Scholar
[3] 魏立秋, 李文博, 蔡海阔, 孙建宁, 杨鑫勇, 于达仁 2020 宇航学报 41 666Google Scholar
Wei L Q, Li W B, Cai H K, Sun J N Yang X Y, Yu D R 2020 J. Astronaut. 41 666Google Scholar
[4] Duan P, Bian X Y, Cao A N, Liu G R, Chen L, Yin Y 2016 Plasma Sci. Technol. 18 525Google Scholar
[5] Duan P, Liu G R, Bian X Y, Chen L, Yin Y, Cao A N 2016 Plasma Sci. Technol. 18 382Google Scholar
[6] Wei L Q, Li W B, Ding Y J, Yu D R 2018 Plasma Sci. Technol. 20 075502Google Scholar
[7] 韩轲, 汪颖, 鲁海峰 2020 推进技术 41 1434Google Scholar
Han K, Wang Y, Lu H F 2020 Journal of Propulsion Technology 41 1434Google Scholar
[8] Wei L Q, Han L, Ding Y J, Yu D R, Zhang C H 2017 Rev. Sci. Instrum. 88 073502Google Scholar
[9] Wang C, Wei L, Yu D 2011 Contrib. Plasma Phys. 51 981Google Scholar
[10] Han L, Ding Y J, Wei L Q, Yu D R 2014 Rev. Sci. Instrum. 85 066113Google Scholar
[11] Chauhan S, Ranjan M, Bandyopadhyay M, Mukherjee S 2016 Phys. Plasmas 23 123524Google Scholar
[12] Yu D R, Wei L Q, Zhao Z Y, Han K, Yan G J 2008 Phys. Plasmas 15 043502Google Scholar
[13] Wang C S, Wei L Q, Ning Z X, Yu D R 2011 Phys. Plasmas 18 013507Google Scholar
[14] Fife J, Martinez-Sanchez M, Szabo J 1997 33rd Joint Propulsion Conference and Exhibit (Seattle: AIAA) p3052
[15] Morozov A I, Savel’ev V 2000 Plasma Phys. Rep. 26 219Google Scholar
[16] Morozov A I, Savel’ev V 2000 Plasma Phys. Rep. 26 875Google Scholar
[17] Boeuf J P, Garrigues L 1998 J. Appl. Phys. 84 3541Google Scholar
[18] 张雯, 史锐, 费王华 2015 导弹与航天运载技术 4 99
Zhang W, Shi R, Fei W H 2015 Missiles Space Veh. 4 99
[19] Hara K, Mikellides I G 2018 Joint Propulsion Conference (Cincinnati: AIAA) p4904
[20] Wei L Q, Li W B, Ding Y J, Han L, Yu D R, Cao Y 2017 Eur. Phys. J. Plus 132 452Google Scholar
[21] Lafleur T, Chabert P, Bourdon A 2021 J. Appl. Phys. 130 053305Google Scholar
[22] Dorf L, Raitses Y, Fisch N J 2006 Phys. Plasmas 13 057104Google Scholar
[23] Bareilles J, Hagelaar G J M, Garrigues L, Boniface C, Boeuf J P, Gascon N 2004 Phys. Plasmas 11 3035Google Scholar
[24] Hara K 2015 Ph. D. Dissertation (Ann Arbor: University of Michigan)
[25] Yu D R, Wang C S, Wei L Q, Gao C, Yu G 2008 Phys. Plasmas 15 113503Google Scholar
[26] Barral S, Ahedo E 2009 Phys. Rev. E 79 046401Google Scholar
[27] Garrigues L, Heron A, Adam J C 2000 Plasma Sources Sci. Technol. 9 219Google Scholar
[28] Chapurin O, Smolyakov A I, Hagelaar G, Raitses Y 2021 J. Appl. Phys. 129 233307Google Scholar
[29] 王雨龙 2013 硕士学位论文 (哈尔滨: 哈尔滨工业大学)
Wang Y L 2013 M. S. Dissertation (Harbin: Harbin Institute of Technology) (in Chinese)
[30] Hara K, Sekerak M J, Boyd I D, Gallimore A D 2014 Phys. Plasmas 21 122103Google Scholar
[31] Dale E T, Jorns B A 2019 Phys. Plasmas 26 013516Google Scholar
[32] Hara K 2019 Plasma Sources Sci. Technol. 28 044001Google Scholar
[33] Andreussi T, Giannetti V, Leporini A, Saravia M M, Andrenucci M 2017 Phys. Plasmas 60 014015Google Scholar
[34] Lafleur T, Baalrud S D, Chabert P 2016 Phys. Plasmas 23 053503Google Scholar
[35] 权路路, 邢伟, 鹿畅, 龚科瑜, 曹勇 2016 中国空间科学技术 36 51
Quan L L, Xing W, Lu C, Gong K Y, Cao Y 2016 Chin. Space Sci. Technol. 36 51
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图 10 通道原子速度对电流振荡和电离区位置的影响 (a)
${V_{\text{a}}} = 100 {\text{m}}/{\text{s}}$ 时电流振荡变化; (b)${V_{\text{a}}} = 150 {\text{m}}/{\text{s}}$ 时电流振荡随时演化; (c)${V_{\text{a}}} = 200 {\text{m}}/{\text{s}}$ 时电流振荡随时演化; (d) 3种原子速度下电离区中心位置随时演化Figure 10. The influence of channel atomic velocity on current oscillation and ionization region position: (a) The evolution of current oscillation over time when
${V_{\text{a}}} = 100 {\text{m}}/{\text{s}}$ ; (b) the evolution of current oscillation over time when${V_{\text{a}}} = 150 {\text{m}}/{\text{s}}$ ; (c) the evolution of current oscillation over time when${V_{\text{a}}} = 200 {\text{m}}/{\text{s}}$ ; (d) the evolution of the ionization zone position under different atomic velocities. -
[1] Morozov A I 2003 Plasma Phys. Rep. 29 235Google Scholar
[2] 杨三祥, 王倩楠, 高俊, 贾艳辉, 耿海, 郭宁, 陈新伟, 袁兴龙, 张鹏 2022 71 105201Google Scholar
Yang S X, Wang Q N, Gao J, Jia Y H, Geng H, Guo N, Chen X W, Yuan X L, Zhang P 2022 Acta Phys. Sin. 71 105201Google Scholar
[3] 魏立秋, 李文博, 蔡海阔, 孙建宁, 杨鑫勇, 于达仁 2020 宇航学报 41 666Google Scholar
Wei L Q, Li W B, Cai H K, Sun J N Yang X Y, Yu D R 2020 J. Astronaut. 41 666Google Scholar
[4] Duan P, Bian X Y, Cao A N, Liu G R, Chen L, Yin Y 2016 Plasma Sci. Technol. 18 525Google Scholar
[5] Duan P, Liu G R, Bian X Y, Chen L, Yin Y, Cao A N 2016 Plasma Sci. Technol. 18 382Google Scholar
[6] Wei L Q, Li W B, Ding Y J, Yu D R 2018 Plasma Sci. Technol. 20 075502Google Scholar
[7] 韩轲, 汪颖, 鲁海峰 2020 推进技术 41 1434Google Scholar
Han K, Wang Y, Lu H F 2020 Journal of Propulsion Technology 41 1434Google Scholar
[8] Wei L Q, Han L, Ding Y J, Yu D R, Zhang C H 2017 Rev. Sci. Instrum. 88 073502Google Scholar
[9] Wang C, Wei L, Yu D 2011 Contrib. Plasma Phys. 51 981Google Scholar
[10] Han L, Ding Y J, Wei L Q, Yu D R 2014 Rev. Sci. Instrum. 85 066113Google Scholar
[11] Chauhan S, Ranjan M, Bandyopadhyay M, Mukherjee S 2016 Phys. Plasmas 23 123524Google Scholar
[12] Yu D R, Wei L Q, Zhao Z Y, Han K, Yan G J 2008 Phys. Plasmas 15 043502Google Scholar
[13] Wang C S, Wei L Q, Ning Z X, Yu D R 2011 Phys. Plasmas 18 013507Google Scholar
[14] Fife J, Martinez-Sanchez M, Szabo J 1997 33rd Joint Propulsion Conference and Exhibit (Seattle: AIAA) p3052
[15] Morozov A I, Savel’ev V 2000 Plasma Phys. Rep. 26 219Google Scholar
[16] Morozov A I, Savel’ev V 2000 Plasma Phys. Rep. 26 875Google Scholar
[17] Boeuf J P, Garrigues L 1998 J. Appl. Phys. 84 3541Google Scholar
[18] 张雯, 史锐, 费王华 2015 导弹与航天运载技术 4 99
Zhang W, Shi R, Fei W H 2015 Missiles Space Veh. 4 99
[19] Hara K, Mikellides I G 2018 Joint Propulsion Conference (Cincinnati: AIAA) p4904
[20] Wei L Q, Li W B, Ding Y J, Han L, Yu D R, Cao Y 2017 Eur. Phys. J. Plus 132 452Google Scholar
[21] Lafleur T, Chabert P, Bourdon A 2021 J. Appl. Phys. 130 053305Google Scholar
[22] Dorf L, Raitses Y, Fisch N J 2006 Phys. Plasmas 13 057104Google Scholar
[23] Bareilles J, Hagelaar G J M, Garrigues L, Boniface C, Boeuf J P, Gascon N 2004 Phys. Plasmas 11 3035Google Scholar
[24] Hara K 2015 Ph. D. Dissertation (Ann Arbor: University of Michigan)
[25] Yu D R, Wang C S, Wei L Q, Gao C, Yu G 2008 Phys. Plasmas 15 113503Google Scholar
[26] Barral S, Ahedo E 2009 Phys. Rev. E 79 046401Google Scholar
[27] Garrigues L, Heron A, Adam J C 2000 Plasma Sources Sci. Technol. 9 219Google Scholar
[28] Chapurin O, Smolyakov A I, Hagelaar G, Raitses Y 2021 J. Appl. Phys. 129 233307Google Scholar
[29] 王雨龙 2013 硕士学位论文 (哈尔滨: 哈尔滨工业大学)
Wang Y L 2013 M. S. Dissertation (Harbin: Harbin Institute of Technology) (in Chinese)
[30] Hara K, Sekerak M J, Boyd I D, Gallimore A D 2014 Phys. Plasmas 21 122103Google Scholar
[31] Dale E T, Jorns B A 2019 Phys. Plasmas 26 013516Google Scholar
[32] Hara K 2019 Plasma Sources Sci. Technol. 28 044001Google Scholar
[33] Andreussi T, Giannetti V, Leporini A, Saravia M M, Andrenucci M 2017 Phys. Plasmas 60 014015Google Scholar
[34] Lafleur T, Baalrud S D, Chabert P 2016 Phys. Plasmas 23 053503Google Scholar
[35] 权路路, 邢伟, 鹿畅, 龚科瑜, 曹勇 2016 中国空间科学技术 36 51
Quan L L, Xing W, Lu C, Gong K Y, Cao Y 2016 Chin. Space Sci. Technol. 36 51
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