Curriculum Vitaes

Ikkoh Funaki

  (船木 一幸)

Profile Information

Affiliation
Professor, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
Professor, School of Physical Sciences Department of Space and Astronautical Science, The Graduate University for Advanced Studies
Degree
Doctor of Philosophy in Engineering(Mar, 1995, The University of Tokyo)

J-GLOBAL ID
200901056190267532
researchmap Member ID
1000253787

External link

Papers

 272
  • Yuki Murayama, Ryota Hara, Yoshiki Yamagiwa, Yuya Oshio, Hiroyuki Nishida, Ikkoh Funaki
    Journal of Evolving Space Activities, 71(2) 67-77, Mar, 2024  Peer-reviewed
    Magsail is a space propulsion system using the interactions between the solar wind and the magnetic field generated by the onboard coils. Magnetoplasma sail is a propulsion system that increases thrust by expanding the magnetosphere through plasma injection from the spacecraft. There are two mechanisms on the magnetospheric inflation: method using frozen-in of magnetic field to carry magnetic field lines by high dynamic pressure plasma and method using the diamagnetic current by thermal plasma, which is called the ring current. We investigated the effect of the dynamic pressure and thermal pressure on the MPS thrust performance used electromagnetic hydrodynamic simulation. It was shown that the ring current is enhanced by adding dynamic pressure to the thermal plasma and increases thrust gain. The high thrust gain over 2.25 was obtained at βth = 0.5 - 2 and βk = 4 - 8. However, the thrust is reduced because the super magneto acoustic wave region is generated in the magnetosphere, which prevents the propagation of thrust in large β conditions. The wide parameter survey reveals injection plasma parameter regions where thrust reduction is restrained and high thrust gain is obtained.
  • Yoshiki Matsunaga, Toru Takahashi, Hiroki Watanabe, Shinatora Cho, Hiroaki Kusawake, Kazuhiro Kajiwara, Fujio Kurokawa, Ikkoh Funaki
    Acta Astronautica, 213 645-656, Oct, 2023  Peer-reviewed
  • Frank Jansen, Tommaso Andreussi, Giovanni Cesarretti, Manfred Ehresmann, Julia Grill, Georg Herdrich, Ikkoh Funaki, Nathalie Girard, Jan Thimo Grundmann, David Krejci, Hans Leiter, Frederic Masson, Volker Maiwald, Tommaso Misuri, Stephane Oriol, Antonio Piragino, Alexander Reissner, Lars Schanz
    EPJ Techniques and Instrumentation, 10(1), Apr 17, 2023  Peer-reviewed
    Abstract This review deals with the selection of the electric propulsion system (EPS) for the internationally developed and designed, primary nuclear-electric space tug International Nuclear Power and Propulsion System (INPPS). INPPS is scheduled for interplanetary missions to Mars and Jupiter moon Europa missions by the end of decade 2020. Regarding specific technical and mission parameters preselected electric thruster (ET) types, developed by international companies and institutions, are analysed, evaluated and investigated for a possible application as propulsion system (PS), the so-called CET (Cluster of Electric Thrusters). It is analysed whether solely electric thrusters, combined in an adequate CET, enable the envisaged interplanetary missions—robotic and astronautic/crewed with the INPPS flagship. Thruster clusters with strategic consortium considerations are analysed as a feasible PS of the INPPS. The studied CET consists of the following: (a) only European ETs, (b) combination of German and European ETs, (c) Japanese and European ETs or at least (d) Japanese, European and US thrusters. The main results are (1) Robotic and crewed INPPS mission to Mars/Europa are realizable with EPS only (no chemical propulsion is needed), (2) that every CET, except (c) of only Japanese and part of European thrusters, is capable to perform the main part of envisaged INPPS flagship mission orbit to Mars, back to Earth and to Jupiter/Europa moon.
  • 村山裕輝, 原亮太, 山極芳樹, 大塩裕哉, 西田浩之, 船木一幸
    日本航空宇宙学会論文集, Apr, 2023  Peer-reviewed
  • Kazuki Ishihara, Kentaro Yoneyama, Hiroaki Watanabe, Noboru Itouyama, Akira Kawasaki, Ken Matsuoka, Jiro Kasahara, Akiko Matsuo, Ikkoh Funaki, Kazuyuki Higashino
    Journal of Propulsion and Power, 1-11, Feb 21, 2023  Peer-reviewed
    Rotating detonation engines (RDEs) have been actively researched around the world for application to next-generation aerospace propulsion systems because detonation combustion has theoretically higher thermal efficiency than conventional combustion. Moreover, because cylindrical RDEs have simpler combustors, further miniaturization of conventional combustors is expected. Therefore, in this study, with the aim of applying RDEs to space propulsion systems, a cylindrical RDE with a converging–diverging nozzle was manufactured; the combustor length [Formula: see text] was changed to 0, 10, 30, 50, and 200 mm; and the thrust performance and combustion mode with the different combustor lengths were compared. As a result, four combustion modes were confirmed. Detonation combustion occurred with a combustor length of [Formula: see text]: that is, a converging rotating detonation engine. The thrust performance of this engine was 94 to 100% of the theoretical rocket thrust performance, which is equivalent to the thrust performance of conventional rocket combustion generated at [Formula: see text]. This study shows that detonation combustion can significantly reduce engine weight while maintaining thrust performance.

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  Peer-reviewed
    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  
  • 國中均, 船木一幸
    日本航空宇宙学会誌, Vol.52(No.601) 37-47, 2004  
  • 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  
  • 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  Peer-reviewed
    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, Jan, 2002  
    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.

Major Books and Other Publications

 6
  • Ikkoh Funaki, Hiroshi Yamakawa
    In-Tech, Mar, 2012 (ISBN: 9789535103394)

Presentations

 561

Research Projects

 28

Industrial Property Rights

 4