-
In magnetic field design principle of microwave discharge ion thruster, it is universally received that enlarging the magnetic mirror region can confine more electrons to acquire better energy utilization rate, while reducing the magnetic field diffusion region can prevent electrons from losing at wall to reduce the discharge loss. However, recently the integrated simulation proposes a hypothesis that electrons can also be heated in the magnetic field diffusion region when the Child-Langmuir sheath is considered as a constraint condition for electrons. Therefore, herein a magnetic field structure for the magnet array microwave discharge ion thruster is designed to verify the hypothesis, in which the magnetic field diffusion region is located near the screen grid. Then, an integrated simulation is conducted for studying the initial discharge and ion beam extraction stages of the thruster. The simulation results show that in the magnetic field diffusion region, the electron temperature is 4–8 eV when the grid system voltage is not applied, while the electron temperature is 4–12 eV when the the grid system voltage is applied. And the plasma density in the latter case has one order of magnitude higher than that in the former case. It means that electrons are obviously heated in the magnetic field diffusion region when they are confined among the Child-Langmuir sheath, the plasma sheath at antenna surface, and magnetic mirror. This electron heating mode produces more high-energy electrons outside the magnetic mirror region to generate plasma in front of the grid system, which can significantly increase the plasma density and ion beam current density. The result shows that under the conditions of 0.3 sccm (1 sccm = 1 mL/min) xenon gas flow, 1 W input microwave power, 300 V screen grid voltage and –50 V acceleration grid voltage, the ion beam current and its density are 0.47 mA and 0.60 mA/cm2 for the magnet array microwave discharge ion thruster, while the ion beam current and its density are 1.2 mA and 0.38 mA/cm2 for the 2-cm microwave discharge ion thruster. The ion beam current density increases by 57.9%. Through the integrated simulation, a new electron heating mode in the magnetic field diffusion region is proved theoretically, which provides a theoretical basis for the magnetic field structure optimization of microwave discharge ion thruster.
-
Keywords:
- electron cyclotron resonance /
- ion thruster /
- electron confining /
- electron heating
[1] 杨涓, 牟浩, 耿海, 吴先明 2023 推进技术 44 78Google Scholar
Yang J, Mou H, Geng H, Wu X M 2023 J. Propuls. Tech. 44 78Google Scholar
[2] Watanabe S, Tsuda Y, Yoshikawa M, Tanaka S, Saiki T, Nakazawa S 2017 Space Sci. Rev. 208 3Google Scholar
[3] Koizumi H, Kawahara H, Yaginuma K, et al. 2016 Trans. JSASS Aerospace Tech. Jpn. 14 30Google Scholar
[4] 韩罗峰, 朱康武, 黄文斌, 于学文, 张辰乙, 鲁超, 刘通, 李航, 黄静 2022 真空与低温 28 98Google Scholar
Han L F, Zhu K W, Huang W B, Yu X W, Zhang C Y, Lu C, Liu T, Li H, Huang J 2022 Vacuum Cry. 28 98Google Scholar
[5] 于达仁, 乔磊, 蒋文嘉, 刘辉 2020 推进技术 41 1Google Scholar
Yu D R, Qiao L, Jiang W J, Liu H 2020 J. Propuls. Tech. 41 1Google Scholar
[6] Tsukizaki R, Ise T, Koizumi H, Togo H, Nishiyama K, Kuninaka H 2014 J. Propul. Power 30 5Google Scholar
[7] 夏旭, 杨涓, 金逸舟, 杭观荣, 付瑜亮, 胡展 2019 物理学报 68 235202Google Scholar
Xia X, Yang J, Jin Y Z, Hang G R, Fu Y L, Hu Z 2019 Acta Phys. Sin. 68 235202Google Scholar
[8] Fu S H, Ding Z F, Ke Y J, Tian L C 2020 IEEE Trans. Plasma Sci. 48 3Google Scholar
[9] Ke Y J, Sun X F, Zhao Y, Chen X K 2018 Prog. Electromagn. Res. Lett. 75 91Google Scholar
[10] Dey I, Toyoda Y, Yamamoto N, Nakashima H 2015 Rev. Sci. Instrum. 86 1868Google Scholar
[11] Takao Y, Koizumi H, Komurasaki K, Eriguchi K, Ono K 2014 Plasma Sources Sci. Technol. 23 064004Google Scholar
[12] Tani Y, Yamashita Y, Tsukizaki R, Nishiyama K, Kuninaka H 2020 Acta Astronau. 176 77Google Scholar
[13] Ataka Y, Nakagawa Y, Koizumi H, Komurasaki K 2021 Acta Astronau. 187 133Google Scholar
[14] Xia X, Yang J, Jin Y Z, Hang G R, Fu Y L, Hu Z 2020 Vacuum 179 109517Google Scholar
[15] Mou H, Jin Y Z, Yang J, Xia X, Fu Y L 2022 Chin. Phys. B 31 075202Google Scholar
[16] Coral G, Tsukizaki, Nishiyama K, Kuninaka H 2018 Plasma Sources Sci. Technol. 27 095015Google Scholar
[17] Koizumi H, Komurasaki K, Aoyama J, Yamaguchi K 2018 J. Propul. Power 34 4Google Scholar
[18] Motoki T, Takasaki D, Koizumi H, Ataka Y, Komurasaki K, Takao Y 2022 Acta Astronau. 196 231Google Scholar
[19] 夏旭 2022 博士学位论文(西安: 西北工业大学)
Xia X 2022 Ph. D. Dissertation (Xi’an: Northwestern Polytechnical University
[20] 付瑜亮, 杨涓, 夏旭, 孙安邦 2023 物理学报 72 175204Google Scholar
Fu Y L, Yang J, Xia X, Sun A B 2023 Acta Phys. Sin. 72 175204Google Scholar
[21] 付瑜亮 2022 博士学位论文(西安: 西北工业大学)
Fu Y L 2022 Ph. D. Dissertation (Xi’an: Northwestern Polytechnical University
[22] Fu Y L, Yang J, Mou H, Tan R W, Xia X, Gao Z Y 2022 Comput. Phys. Commun. 278 8395Google Scholar
-
-
[1] 杨涓, 牟浩, 耿海, 吴先明 2023 推进技术 44 78Google Scholar
Yang J, Mou H, Geng H, Wu X M 2023 J. Propuls. Tech. 44 78Google Scholar
[2] Watanabe S, Tsuda Y, Yoshikawa M, Tanaka S, Saiki T, Nakazawa S 2017 Space Sci. Rev. 208 3Google Scholar
[3] Koizumi H, Kawahara H, Yaginuma K, et al. 2016 Trans. JSASS Aerospace Tech. Jpn. 14 30Google Scholar
[4] 韩罗峰, 朱康武, 黄文斌, 于学文, 张辰乙, 鲁超, 刘通, 李航, 黄静 2022 真空与低温 28 98Google Scholar
Han L F, Zhu K W, Huang W B, Yu X W, Zhang C Y, Lu C, Liu T, Li H, Huang J 2022 Vacuum Cry. 28 98Google Scholar
[5] 于达仁, 乔磊, 蒋文嘉, 刘辉 2020 推进技术 41 1Google Scholar
Yu D R, Qiao L, Jiang W J, Liu H 2020 J. Propuls. Tech. 41 1Google Scholar
[6] Tsukizaki R, Ise T, Koizumi H, Togo H, Nishiyama K, Kuninaka H 2014 J. Propul. Power 30 5Google Scholar
[7] 夏旭, 杨涓, 金逸舟, 杭观荣, 付瑜亮, 胡展 2019 物理学报 68 235202Google Scholar
Xia X, Yang J, Jin Y Z, Hang G R, Fu Y L, Hu Z 2019 Acta Phys. Sin. 68 235202Google Scholar
[8] Fu S H, Ding Z F, Ke Y J, Tian L C 2020 IEEE Trans. Plasma Sci. 48 3Google Scholar
[9] Ke Y J, Sun X F, Zhao Y, Chen X K 2018 Prog. Electromagn. Res. Lett. 75 91Google Scholar
[10] Dey I, Toyoda Y, Yamamoto N, Nakashima H 2015 Rev. Sci. Instrum. 86 1868Google Scholar
[11] Takao Y, Koizumi H, Komurasaki K, Eriguchi K, Ono K 2014 Plasma Sources Sci. Technol. 23 064004Google Scholar
[12] Tani Y, Yamashita Y, Tsukizaki R, Nishiyama K, Kuninaka H 2020 Acta Astronau. 176 77Google Scholar
[13] Ataka Y, Nakagawa Y, Koizumi H, Komurasaki K 2021 Acta Astronau. 187 133Google Scholar
[14] Xia X, Yang J, Jin Y Z, Hang G R, Fu Y L, Hu Z 2020 Vacuum 179 109517Google Scholar
[15] Mou H, Jin Y Z, Yang J, Xia X, Fu Y L 2022 Chin. Phys. B 31 075202Google Scholar
[16] Coral G, Tsukizaki, Nishiyama K, Kuninaka H 2018 Plasma Sources Sci. Technol. 27 095015Google Scholar
[17] Koizumi H, Komurasaki K, Aoyama J, Yamaguchi K 2018 J. Propul. Power 34 4Google Scholar
[18] Motoki T, Takasaki D, Koizumi H, Ataka Y, Komurasaki K, Takao Y 2022 Acta Astronau. 196 231Google Scholar
[19] 夏旭 2022 博士学位论文(西安: 西北工业大学)
Xia X 2022 Ph. D. Dissertation (Xi’an: Northwestern Polytechnical University
[20] 付瑜亮, 杨涓, 夏旭, 孙安邦 2023 物理学报 72 175204Google Scholar
Fu Y L, Yang J, Xia X, Sun A B 2023 Acta Phys. Sin. 72 175204Google Scholar
[21] 付瑜亮 2022 博士学位论文(西安: 西北工业大学)
Fu Y L 2022 Ph. D. Dissertation (Xi’an: Northwestern Polytechnical University
[22] Fu Y L, Yang J, Mou H, Tan R W, Xia X, Gao Z Y 2022 Comput. Phys. Commun. 278 8395Google Scholar
Catalog
Metrics
- Abstract views: 2210
- PDF Downloads: 68
- Cited By: 0