Profile Information
- Affiliation
- Associate professor, Institute of Space and Astronautical Science, Department of Spacecraft Engineering, Japan Aerospace Exploration Agency
- Degree
- Dr. Eng.(Mar, 2007, Tokyo Denki University)
- J-GLOBAL ID
- 200901094498520904
- researchmap Member ID
- 6000005907
- External link
Research Interests
7Research Areas
3Research History
1Papers
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Springer Aerospace Technology, 695-720, Dec 14, 2024
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Proceedings of the International Astronautical Congress, IAC, 2023-October, 2023A 6U CubeSat “OMOTENASHI” was developed to be the world's smallest moon lander. It was launched by NASA's SLS Artemis-1 on November 16, 2022. However, because of the spacecraft anomaly, the battery was depleted and the communication with the spacecraft had been lost. After we gave up the moon landing experiment, we have been conducting a search and rescue operation till September 2023. But it was unsuccessful, unfortunately. In this article, the mission objective, the spacecraft design, the planed mission scenario, and the in-orbit operation results are presented. Additionally, lessons learned from the development and the in-orbit operation are presented.
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Proceedings of the International Astronautical Congress, IAC, 2023-October, 2023This paper presents a collaborative effort between NASA and JAXA to make 3-way Doppler data from JAXA tracking stations available to the Artemis 1 navigation team to improve orbit determination. The paper describes the system configuration and concept of operation of this capability. Testing effort at the three JAXA's ground stations - the Uchinoura's 20-m and 34-m antennas and Usuda's 64-m antenna - are discussed. Both aspects of system testing are highlighted, first on the use of Artemis 1 recorded signal to ensure compatibility between ground and flight systems, and second on the tracking with the Lunar Reconnaissance Orbiter, as a substitute for Artemis before launch, to validate other key operational functions such as ephemeris processing, spacecraft tracking capability, data delivery, and interactions among multiple operational teams in different organizations. Results from actual support to Artemis 1's Orion spacecraft in November-December 2022 are also presented.
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ADVANCES IN COMMUNICATIONS SATELLITE SYSTEMS 2, 95 235-242, 2020This chapter presents an ongoing effort in preparing JAXA Uchinoura station support to the Artemis 1 mission, scheduled for launch in late 2020. The system involves three key participants: JAXA ground station at Uchinoura, the Deep Space Network (DSN) components at the Jet Propulsion Laboratory, California, and the Artemis 1 mission navigation at the NASA Johnson Space Center, Texas.Demonstration of Uchinoura station support to the future Artemis signal relies on the use of a low-cost, highly-portable software-defined radio (SDR) test equipment as well as the tracking of the Lunar Reconnaissance Orbiter (LRO) spacecraft. Using the SDR equipment, we validated the compatibility of signal format between the Artemis flight radio and the Uchinoura ground station without having to send the flight equipment to the station. By tracking an ongoing operational spacecraft such as LRO, we were able to calibrate the performance of the system in real operational conditions. The measured Doppler noise of 0.03 Hz (1-sigma), or 0.002 m/s range rate at S-band, for Uchinoura station is deemed suitable to the Artemis 1 mission navigation needs.This chapter also discusses the test equipment capability and its performance. In addition to being low cost, the equipment offers many advantages compared to the traditional full-scaled test signal simulator. Chief among them is portability making system easy to set up and transport, and the fidelity of the test signal that it captures from spacecraft flight equipment. Some of the lessons learned, such as internal frequency stability of the test signal, are also reflected.
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Proceedings of the International Astronautical Congress, IAC, 2020-October, 2020Copyright © 2020 by the International Astronautical Federation (IAF). All rights reserved. A 6U CubeSat “OMOTENASHI” will be the world's smallest moon lander which is launched by NASA SLS Artemis-1. Because of its severe mass and size limitation, it will adopt semi-hard landing scheme. That is, OMOTENASHI is decelerated from orbital velocity to less than 50 m/s by a small solid rocket motor and shock absorption mechanism has been developed to withstand the high-speed impact. Ultra small communication system (X-band and P-band) is also developed. It observes radiation environment of Earth and moon region with portable dosimeters. This paper shows the mission outline, the design, and the development results of OMOTENASHI.
Misc.
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JAXA Research and Development Report, JAXA-RR-24-003 1-134, Feb, 2025 Peer-reviewed
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宇宙科学技術連合講演会講演集(CD-ROM), 67th, 2023
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宇宙科学技術連合講演会講演集(CD-ROM), 67th, 2023
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宇宙科学技術連合講演会講演集(CD-ROM), 65th, 2021
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宇宙科学技術連合講演会講演集(CD-ROM), 63rd, 2019
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計測自動制御学会制御部門マルチシンポジウム(CD-ROM), 5th, 2018
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電子情報通信学会技術研究報告, 118(105(SANE2018 13-21)(Web)), 2018
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宇宙科学技術連合講演会講演集(CD-ROM), 62nd, 2018
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宇宙科学技術連合講演会講演集(CD-ROM), 62nd, 2018
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宇宙科学技術連合講演会講演集(CD-ROM), 62nd, 2018
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Earth, Planets and Space, 69(1), Dec 1, 2017© 2017 The Author(s). After the arrival of Akatsuki spacecraft of Japan Aerospace Exploration Agency at Venus in December 2015, the radio occultation experiment, termed RS (Radio Science), obtained 19 vertical profiles of the Venusian atmosphere by April 2017. An onboard ultra-stable oscillator is used to generate stable X-band downlink signals needed for the experiment. The quantities to be retrieved are the atmospheric pressure, the temperature, the sulfuric acid vapor mixing ratio, and the electron density. Temperature profiles were successfully obtained down to ~ 38 km altitude and show distinct atmospheric structures depending on the altitude. The overall structure is close to the previous observations, suggesting a remarkable stability of the thermal structure. Local time-dependent features are seen within and above the clouds, which is located around 48-70 km altitude. The H2SO4 vapor density roughly follows the saturation curve at cloud heights, suggesting equilibrium with cloud particles. The ionospheric electron density profiles are also successfully retrieved, showing distinct local time dependence. Akatsuki RS mainly probes the low and middle latitude regions thanks to the near-equatorial orbit in contrast to the previous radio occultation experiments using polar orbiters. Studies based on combined analyses of RS and optical imaging data are ongoing.[Figure not available: see fulltext.]
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電子情報通信学会技術研究報告 = IEICE technical report : 信学技報, 117(321) 97-100, Nov 23, 2017
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宇宙科学技術連合講演会講演集(CD-ROM), 61st, 2017
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宇宙科学技術連合講演会講演集(CD-ROM), 61st, 2017
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Nov, 2016Balloon Symposium 2016 (November 1-2, 2016. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan
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60 6p, Sep 6, 2016 Peer-reviewed
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60 6p, Sep 6, 2016 Peer-reviewed
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116(115) 7-11, Jun 24, 2016
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115(447) 25-30, Feb 16, 2016
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Jan, 201616th Space Science Symposium (January 6-7, 2016. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS)Sagamihara Campus), Sagamihara, Kanagawa Japan
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TTC 2016 - 7th ESA International Workshop on Tracking, Telemetry and Command Systems for Space Applications, Jan 1, 2016
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Technical report of IEICE. SANE, 114(448) 25-30, Feb 18, 2015A high-speed downlink communication system is required to meet various applications for nano/small satellites. Therefore, it is essential to implement a transmitter with small weight and power in such satellites. We have developed high speed communication system over 300 Mbps for small satellite. In order to reduce DC power consumption of transmitter, we have developed GaN-HEMT power amplifier for X band downlink. The Hodoyoshi-4 satellite equipped with the developed communication system was launched in 2014 and we demonstrated 348 Mbps downlink from 50-kg class satellite. This paper describes the summary of the developed system, the experiment of high speed downlink, and future works.
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Technical report of IEICE. SAT, 114(449) 43-48, Feb 18, 2015A high-speed downlink communication system is required to meet various applications for nano/small satellites. Therefore, it is essential to implement a transmitter with small weight and power in such satellites. We have developed high speed communication system over 300 Mbps for small satellite. In order to reduce DC power consumption of transmitter, we have developed GaN-HEMT power amplifier for X band downlink. The Hodoyoshi-4 satellite equipped with the developed communication system was launched in 2014 and we demonstrated 348 Mbps downlink from 50-kg class satellite. This paper describes the summary of the developed system, the experiment of high speed downlink, and future works.
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IEICE technical report. RCC, Reliable communication and control, 114(317) 55-60, Nov 20, 2014This report described measurements and characterization of ultra-wideband (UWB) radio propagation within a small scientific satellite and simulation of transmission performance based on propagation measurements, with a view to (at least partly) replacing wired on-board data buses with wireless communications. Adoption of wireless technologies within spacecrafts could contribute to (i) reduction of cable weight and resulting launching cost, (ii) reduction in the cost of manufacture and test, (iii) ensuring reliable robust communication due to effect of route diversity, (iv) more flexibility in layout of subsystems, and (v) more reliable connection at rotary, moving, and sliding joints. However, narrowband wireless communication systems yield dead spot and intersymbol interference (ISI) due to multipath propagation, particularly in metal-enclosed spaces such as inside of satellites. To apply wireless communication within satellites, a combination of UWB and orthogonal frequency division multiplexing (OFDM) overcomes the dead spots and ISI. Bit error rate (BER) performance of the UWB-OFDM wireless transmission was evaluated through simulation using measured propagation data. Simulation results revealed that the system attained BER ≦ 10^<-5> at 400 Mb/s in all measurement points while ensuring a margin of approximately 15 dB to -41.25-dBm/MHz equivalent isotropic radiated power.
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Technical report of IEICE. SANE, 114(264) 11-16, Oct 22, 2014A high-speed downlink communications system is required to meet various applications for nano/small satellites. It is essential to implement a transmitter with small weight and power in such satellites. We have developed a compact 348Mbps transmitter incorporating a powerful error correction on ground station receiver. This system has been demonstrated a high-speed down link communication system at "Hodoyoshi-4" satellite with 50 kg mass.
Professional Memberships
1-
Jun, 2002 - Present
Research Projects
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Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B), Japan Society for the Promotion of Science, Apr, 2014 - Mar, 2017
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Grants-in-Aid for Scientific Research Grant-in-Aid for Young Scientists (B), Japan Society for the Promotion of Science, 2008 - 2009
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Research on Signal Combination of Uplink and Downlink for Array Antennas of X and Ka Band Deep SpaceGrants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B), Japan Society for the Promotion of Science, 2005 - 2007