研究者業績
基本情報
経歴
5-
2011年4月 - 現在
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2007年9月 - 2011年3月
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2003年10月 - 2007年8月
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2000年4月 - 2003年9月
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1999年4月 - 2000年3月
学歴
3-
1997年4月 - 2000年3月
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1995年4月 - 1997年3月
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1991年4月 - 1995年3月
受賞
4-
2020年3月
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2013年4月
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2012年8月
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2008年7月
論文
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Journal of Spacecraft and Rockets 62(6) 2019-2029 2025年11月JAXA has been planning to adopt a nose-entry flight method, in which a glide flight is followed by a turnover maneuver, as a return flight method for vertical-takeoff and vertical-landing rockets. To clarify the aerodynamic characteristics during the turnover maneuver, both (conventional) static calculations with fixed angles of attack and (computationally challenging) dynamic calculations by continuously changing the angles of attack by [Formula: see text], corresponding to 1.0% of the freestream velocity at the nose were performed. The numerical results were verified and validated by corresponding experimental results. Then, these aerodynamic coefficients and flowfields were compared directly to investigate the turnover effects. The results revealed that the leeward vortex structures and aerodynamic coefficients at [Formula: see text] differ by 48% (pitching moment coefficient). Conversely, at [Formula: see text], the aerodynamic coefficients only differ by 4.8% (pitching moment coefficient), although a difference was observed in the base vortices. In summary, through the dynamic simulation, an important aerodynamic feature of the maneuvering vehicle was discovered, in which the flowfield at an earlier attitude significantly influenced that at the subsequent time; this cannot be reproduced or revealed by static simulations in which different angle-of-attack cases are conducted separately.
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Journal of Spacecraft and Rockets 61(2) 355-368 2024年3月The presence of protuberances can create an asymmetric flowfield, which contributes to side forces in slender-bodied launch vehicles. In this study, we conduct numerical calculations using a supercomputer at Japan Aerospace Exploration Agency (JAXA) on a slender body with a different-sized protuberance at Mach 1.5 to systematically determine the aerodynamic effects of the protuberance size. The protuberance size is varied in its height and width. According to the results, it is demonstrated that the side force significantly increases when the height of the protuberance increases. This is because, the higher the protuberance, the farther the wake vortex produced by the protuberance moved away from the body. Consequently, the flow asymmetry between the protuberance side and clean side is augmented, and the side force increases. In contrast, the side force is almost constant when only the width of the protuberance is changed. The results of this study indicate that when attaching the protuberance to the vehicles the height of the protuberance should be lowered, and the width of the protuberance should be increased to secure the volume of the protuberance and reduce the increase in side force.
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Journal of Evolving Space Activities 2024 Volume 2 2024年
MISC
214-
Collection of Technical Papers - 43rd AIAA/ASME/SAE/ASEE Joint Propulsion Conference 5 5296-5312 2007年
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Collection of Technical Papers - 44th AIAA Aerospace Sciences Meeting 5 3106-3114 2006年
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Collection of Technical Papers - AIAA Applied Aerodynamics Conference 2 1340-1349 2006年
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International Astronautical Federation - 56th International Astronautical Congress 2005 8 5216-5225 2005年
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JASMA : Journal of the Japan Society of Microgravity Application = 日本マイクログラビティ応用学会誌 21 71-71 2004年11月4日
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34th AIAA Fluid Dynamics Conference and Exhibit 2004年
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International Astronautical Federation - 55th International Astronautical Congress 2004 13 8502-8508 2004年
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日本流体力学会年会講演論文集 2004 614-615 2004年Magnetic sail and Magnetic plasma sail are propulsion systems that make use of the solar wind. These propulsion systems create a large magnetic field around a spacecraft and the magnetic field captures the energy of the solar wind. These propulsion systems are suited for deep space missions because it is estimated to achieve high thrust and efficiency. But there are some problems about these propulsion systems. The process of force transfering from the solar wind to the spacecraft is not understood in detail, thus the metods of estimating thrust vector and controlling thrust vector are not established. We simulated the interaction between the solar wind and the magnetic field of the spacecraft numerically, and verified the method of estimating thrust vector. Additionally we researched the methods of controlling thrust vector. 収集根拠 : NII-ELS 資料形態 : テキストデータ コレクション : 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > 学術機関 > 学協会 著者所属: 東大工 著者所属: ISAS, JAXA 著者所属: 防衛大 著者所属: 静岡大工 Affiliation: School of Engineering, The University of Tokyo Affiliation: ISAS, JAXA Affiliation: National Defense Academy Affiliation: Faculty of Engineering, Shizuoka University レポート・講演番号: D342
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39th AIAA/ASME/SAE/ASEE Joint Propulsion Conference and Exhibit 2003年
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34th AIAA Plasmadynamics and Lasers Conference 2003年
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33rd Plasmadynamics and Lasers Conference 2002年
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10th AIAA/NAL-NASDA-ISAS International Space Planes and Hypersonic Systems and Technologies Conference 2001年
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38th Aerospace Sciences Meeting and Exhibit 2000年
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38th Aerospace Sciences Meeting and Exhibit 2000年
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37th Aerospace Sciences Meeting and Exhibit 1999年
共同研究・競争的資金等の研究課題
6-
日本学術振興会 科学研究費助成事業 2024年4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 2021年4月 - 2024年3月
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日本学術振興会 科学研究費助成事業 基盤研究(C) 2018年4月 - 2021年3月
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日本学術振興会 科学研究費助成事業 基盤研究(B) 2011年4月 - 2014年3月
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日本学術振興会 科学研究費助成事業 基盤研究(B) 2003年 - 2005年