研究者業績
基本情報
- 所属
- 国立研究開発法人宇宙航空研究開発機構 宇宙科学研究所 助教
- ORCID ID
https://orcid.org/0000-0001-9888-7137
- J-GLOBAL ID
- 202201021399605332
- researchmap会員ID
- R000038113
研究キーワード
4経歴
4-
2025年8月 - 現在
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2025年4月 - 現在
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2022年4月 - 2025年3月
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2020年4月 - 2022年3月
学歴
4-
2019年4月 - 2022年3月
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2017年4月 - 2019年3月
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2013年4月 - 2017年3月
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2010年4月 - 2013年3月
受賞
8論文
26-
Journal of Applied Physics 2025年8月7日 査読有り
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Physics of Plasmas 2025年4月1日 査読有り筆頭著者責任著者
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Journal of Spacecraft and Rockets 1-15 2025年2月13日 査読有りMultiparametric study of a thrust force exerted on a model electric (E) sail spacecraft by the solar wind is conducted with a particle-in-cell method. Several effects relevant to the thrust performance are examined with the focus on the accuracy of the obtained results, reflected in the improved initial conditions and physically realistic boundary conditions set at the external boundaries and the near field of a tether. These effects include thrust sensitivity to the solar wind density, temperature, and relative velocity between the solar wind and the spacecraft as well as the influence of the tether potential on the resulting thrust force. The dependence of thrust [Formula: see text] on the distance between the spacecraft and the sun [Formula: see text] is found to have an exponential form approximated by [Formula: see text]. Numerical estimates of the electric current to the E-sail tether mesh give values that are on average about 50% higher than those predicted by the orbital motion limited theory. In addition to single tethers, tether arrays are also studied and shown to have lower thrust per tether that that of a single tether.
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Plasma Sources Science and Technology 33(11) 115018-115018 2024年11月1日 査読有りAbstract A multi-fluid moment model, a drift-diffusion (DD) model, and a particle-in-cell/Monte Carlo collision (PIC-MCC) model are compared to investigate direct-current breakdown accounting only for singly charged ions and electrons. The key difference between the moment and DD models is that the electron inertial terms are taken into account in the moment model while the DD models neglect the inertia terms. The breakdown voltage results obtained from the multi-fluid moment and PIC-MCC models are in good agreement with each other over a wide range of pd values, where p is the gas pressure and d is the distance between the cathode and anode. The steady-state electron momentum balance reveals the importance of the electron inertial term at low values of pd, showing the invalidity of the DD approximation under such conditions. The results also show that the main electron energy loss mechanism transitions from volumetric (collisional) losses at high pd regime, which corresponds to low reduced electric field, to convective heat to the anode at low pd regime, where the reduced electric field is high.
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Journal of Computational Physics 508 113030-113030 2024年7月 査読有り
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Journal of Applied Physics 135(24) 2024年6月27日 査読有りIonic liquid electrospray thrusters represent an alternative propulsion method for spacecraft to conventional plasma propulsion because they do not require plasma generation, which significantly increases the thrust efficiency. The porous emitter thruster has the advantages of simple propellant feeding and multi-site emissions, which miniaturize the thruster size and increase thrust. However, the multi-scale nature, that is, nano- to micrometer-sized menisci on the millimeter-size porous needle tip, makes modeling multi-site emissions difficult, and direct observation is also challenging. This paper proposes a simple model for multi-site emissions, which assumes that the ionic conductivity or ion transport in the porous media determines the ion-emission current. The conductivity was evaluated by comparing the experimental and numerical data based on the model. The results suggest that the ionic conductivity of the porous emitter is suppressed by the ion–pore wall friction stress. Additionally, the model indicates that the emission area expansion on the porous emitter creates the unique curve shape of the current vs voltage characteristics for multi-site emissions.
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Vacuum 220 112760-112760 2024年2月 査読有り
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56(38) 384003-384003 2023年6月20日 査読有り筆頭著者責任著者
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Journal of Evolving Space Activities 1 21 2023年6月 査読有り筆頭著者責任著者
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Journal of Evolving Space Activities 1 2023年4月 査読有り筆頭著者責任著者
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Journal of Electric Propulsion 1(1) 2022年12月 査読有り招待有り筆頭著者責任著者Abstract In electron cyclotron resonance (ECR) thrusters, the plasma mode transition is a critical phenomenon because it determines the maximum thrust performance. In ECR ion thrusters, ionization generally occurs in the magnetic confinement region, where electrons are continuously heated by ECR and confined by magnetic mirrors. However, as the flow rate increases, ionization is also observed outside the magnetic confinement region, and this induces the plasma mode transition. In our previous work, two-photon absorption laser-induced fluorescence (TALIF) analysis revealed that the stepwise ionization from the metastable state plays an important role in the ionization process. However, the distribution of the stepwise ionization has not yet been revealed because of the long lifetime of the metastable state. In this study, this distribution was investigated using one experimental and two numerical approaches. First, TALIF was applied to two types of gas injection with clear differences in thrust performance and ground-state neutral density distribution. In the first simulation, the metastable state particle simulation was used to estimate the excitation rate distribution. In the second study, simulations of the electric field of microwaves were used to estimate the contribution of the stepwise ionization to the plasma density. The experimental and numerical results revealed that the stepwise ionization spreads outside the magnetic confinement region because of the diffusion of metastable particles, and this spread induces the plasma mode transition, explaining the difference between the two types of gas injection.
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Vacuum 200 110962-110962 2022年6月 査読有り筆頭著者責任著者
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CEAS Space Journal 2022年3月1日 査読有り
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Investigation of plasma mode transition and hysteresis in electron cyclotron resonance ion thrustersPlasma Sources Science and Technology 30(9) 095023-095023 2021年9月1日 査読有り筆頭著者責任著者
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Acta Astronautica 185 179-187 2021年8月 査読有り筆頭著者責任著者
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Acta Astronautica 176 77-88 2020年11月 査読有り
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Acta Astronautica 174 367-376 2020年9月 査読有り
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Transactions of the Japan Society for Aeronautical and Space Sciences 63(6) 281-283 2020年 査読有り
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TRANSACTIONS OF THE JAPAN SOCIETY FOR AERONAUTICAL AND SPACE SCIENCES, AEROSPACE TECHNOLOGY JAPAN 18(3) 57-63 2020年 査読有り筆頭著者責任著者<p>The authors investigate the discharge chamber of the microwave ion thruster μ10 by using kinetic particle simulation. First, to investigate the plasma phenomena qualitatively, we conduct a particle-in-cell (PIC) simulation model. The simulation results indicate that the distribution of ion density is ring-shaped. To verify the simulation result with the experimental result, the simulation result is compared with the optical emission distribution. In low propellant flow rates, the distribution of ion density agrees with the optical emission distribution. However, in high propellant flow rates, the optical emission distribution is different from simulation results in the waveguide due to the excited neutral particles. In the thruster, the performance strongly depends on the location of injecting the propellant. Hence, to develop the plasma simulation for quantitative comparison with the experiment, the distribution of the neutral density is evaluated by using direct Monte Carlo simulation (DSMC). The results show the neutral density in the waveguide increases corresponding to the ratio of waveguide injection, which indicates that the density is one of the most important parameters for quantitative evaluation with the experiment.</p>
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Physics of Plasmas 2019年7月 査読有り筆頭著者責任著者
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Plasma Sources Science and Technology 27(10) 105006-105006 2018年10月16日 査読有り筆頭著者責任著者
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Plasma Sources Science and Technology 27(1) 2018年1月 査読有り
MISC
51講演・口頭発表等
1-
Plasma seminar @ Stanford University 2025年1月17日 招待有り
所属学協会
1共同研究・競争的資金等の研究課題
3-
日本学術振興会 科学研究費助成事業 2025年7月 - 2027年3月
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日本学術振興会 科学研究費助成事業 2023年4月 - 2025年3月
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日本学術振興会 科学研究費助成事業 2020年4月 - 2022年3月