研究者業績

船木 一幸

フナキ イッコウ  (Ikkoh Funaki)

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 宇宙飛翔工学研究系 教授
総合研究大学院大学 先端学術院 宇宙科学コース 教授
学位
博士(工学)(1995年3月 東京大学)

J-GLOBAL ID
200901056190267532
researchmap会員ID
1000253787

外部リンク

論文

 290
  • Rinpei Sakata, Masahiro Inada, Noboru Itouyama, Ken Matsuoka, Jiro Kasahara, Akira Kawasaki, Akiko Matsuo, Ikkoh Funaki
    Journal of Propulsion and Power 1-10 2024年6月20日  
    A coupled cylindrical rotating detonation engine (RDE) with two cylindrical RDEs (both combustors had a combustor inner diameter of 23 mm and an axial length of 30 mm) placed next to each other was tested for rocket clustering application. The objective of the experiment was to achieve two-engine synchronized initiation with a single igniter. Experiments were conducted on the inner wall of the combustors with different connecting-hole diameters and wall heights to evaluate the ignition delay time, combustion mode, and propulsion performance. The propellants were gaseous ethylene and oxygen, and experiments were conducted under constant conditions of mass flow rate ([Formula: see text]), equivalence ratio ([Formula: see text]), and backpressure (approximately 10 kPa). When the two combustion chambers were completely separated by a wall, ignition occurred with a time delay of 260 ms in the chamber without an igniter. However, when a large hole ([Formula: see text] diameter) was placed in the wall separating the two combustion chambers, synchronous initiation was successful. Synchronous initiation was also successful when the wall height was lowered (7-mm height). Under both conditions, the same level of specific impulse was achieved as for RDEs operating at the same mass flux.
  • Tomoki Sato, Kotaro Nakata, Kazuki Ishihara, Noboru Itouyama, Ken Matsuoka, Jiro Kasahara, Akira Kawasaki, Daisuke Nakata, Hikaru Eguchi, Masaharu Uchiumi, Akiko Matsuo, Ikkoh Funaki
    Combustion and Flame 264 113443-113443 2024年6月  
  • Kazuki Ishihara, Tomoki Sato, Tomoaki Kimura, Kosuke Nakajima, Kotaro Nakata, Noboru Itouyama, Akira Kawasaki, Ken Matsuoka, Koichi Matsuyama, Jiro Kasahara, Hikaru Eguchi, Daisuke Nakata, Masaharu Uchiumi, Akiko Matsuo, Ikkoh Funaki
    Journal of Spacecraft and Rockets 1-11 2024年5月28日  
    There are few experimental studies on rotating detonation engines (RDEs) with liquid propellants. This study reveals the static thrust performance of a cylindrical RDE with ethanol and liquid nitrous oxide as propellants under atmospheric pressure. This RDE had an inner diameter of 40 mm, a maximum combustor length of 230 mm, a nozzle contraction ratio of 1.7, and a nozzle expansion ratio of 9.1. Nineteen experiments were conducted at total mass flow rates of [Formula: see text], mixture ratios of 3.6–5.9, and combustion pressures of 0.35–0.46 MPa, resulting in a maximum detonation velocity of [Formula: see text] (approximately 80% of the theoretical detonation velocity, [Formula: see text]), maximum thrust at sea level of 294 N, and maximum specific impulse at sea level of 148 s. In addition, the maximum characteristic exhaust velocity, [Formula: see text], was [Formula: see text], which was 99% of the theoretical value. The characteristic length of the combustion chamber at this time was 0.15 m. Since conventional rocket combustion requires 1.57 m to achieve the same [Formula: see text] efficiency, this study shows that detonation combustion can reduce the combustor size by 88%.
  • Yuki Murayama, Ryota Hara, Yoshiki Yamagiwa, Yuya Oshio, Hiroyuki Nishida, Ikkoh Funaki
    Journal of Evolving Space Activities 71(2) 67-77 2024年3月  査読有り
  • Yusuke Oda, Satoru Sawada, Noboru Itouyama, Ken Matsuoka, Jiro Kasahara, Akira Kawasaki, Akiko Matsuo, Ikkoh Funaki
    Proceedings of the Combustion Institute 40(1-4) 105735-105735 2024年  

MISC

 206
  • H. Nishida, H. Ogawa, I. Funaki, K. Fujita, H. Yamakawa, Y. Inatani
    41st AIAA/ASME/SAE/ASEE Joint Propulsion Conference and Exhibit 2005年  査読有り
    A Magnetic Sail is a deep space propulsion system which captures the momentum of the solar wind by a large artificial magnetic field produced around a spacecraft. To verify the momentum transfer process from the solar wind to the spacecraft, we simulated the interaction between the solar wind and the artificial magnetic field of the Magnetic Sail using the magnetohydrodynamic model. The result showed the same plasma flow and magnetic field structure as those of the Earth. The change of the solar wind momentum results in a pressure distribution along the magnetopause, which is the boundary between the solar wind plasma and the magnetosphere. The pressure on the magnetopause is then transferred to the spacecraft through the Lorentz force between the induced current along the magnetopause and the current along the coil of the spacecraft. The simulation successfully demonstrated that the change of the momentum of the solar wind is transferred to the spacecraft via the Lorentz force. The drag coefficient (thrust coefficient) of the Magnetic Sail was estimated to be 5.0, and it became clear that the Magnetic Sail has weathercock stability. Copyright © 2005 by the American Institute of Aeronautics and Astronautics, Inc. All rights reserved.
  • 國中均, 船木一幸
    日本航空宇宙学会誌 Vol.52(No.600) 6-14 2004年  
  • 國中均, 船木一幸
    日本航空宇宙学会誌 Vol.52(No.601) 37-47 2004年  
  • 船木一幸, 山川宏, 藤田和央, 野中聡
    日本物理学会誌 58(4) 266-269 2003年  
  • I. Funaki, R. Asahi, H. Yamakawa, K. Fujita, H. Ogawa, S. Nonaka, S. Sawai, H. Kuninaka, H. Otsu
    34th AIAA Plasmadynamics and Lasers Conference 2003年  査読有り
    If a dense plasma were exhausted near the center of a magneetic sail, the magnetic field could be expanded far away from the spacecraft, thus the energy of the solar wind can be captured by this huge magnetic field in spite of very low-density solar wind. Then the magnetic sail can propel a spacecraft by the solar wind in the inerplanetary space. Such a magnetoplasma sail was analytically studied, and large thrust to power ratio as much as 250mN/kW was explained. When applied to short-term deep space missions, the magnetoplasma sail has great advantage against other electric propulsion systems because of its ability to achieve larger thrust to power ratio. © 2003 by the American Institute of Aeronautics and Astronautics, Inc. All rights reserved.
  • Funaki, I, H Kuninaka, K Toki, Y Shimizu, K Nishiyama, Y Horiuchi
    JOURNAL OF PROPULSION AND POWER 18(1) 169-175 2002年1月  
    An ion beam optics for a 10-cm-diam 400-W-class microwave discharge ion thruster was fabricated and its applicability to a long-term space mission was demonstrated. The optics consists of three 1-mm-thick flat carbon-carbon composite panels with approximately 800 holes that were mechanically drilled and positioned with +/-0.02-mm accuracy. When mounted on an aluminum ring, spacing for the three grids was kept at 0.5 mm by three sets of spacers. The thruster produced an ion beam current of 140 mA with a microwave power of 32 W for plasma generation and a total acceleration voltage of 1.8 kV. Although the grid is sputtered by the impingement of slow ions produced in charge-exchange collisions between fast beam ions and neutral atoms leaking from the engine, the grid showed only slight damage even after an 18,000-h endurance test. Also, other qualification tests including a mechanical test under launch conditions as well as a thermal vacuum test simulating the spacecraft thermal environment were successfully completed. Hence, the grid system was qualified for spacecraft propulsion.

主要な書籍等出版物

 6
  • 船木 一幸, 山川 宏
    In-Tech 2012年3月 (ISBN: 9789535103394)

講演・口頭発表等

 561

共同研究・競争的資金等の研究課題

 28

産業財産権

 4