Curriculum Vitaes

Yukio YAMAMOTO

  (山本 幸生)

Profile Information

Affiliation
Associate Professor, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency

J-GLOBAL ID
201901015283902873
researchmap Member ID
B000362527

Papers

 66
  • K. Yumoto, E. Tatsumi, T. Kouyama, D. R. Golish, Y. Cho, T. Morota, S. Kameda, H. Sato, B. Rizk, D. N. DellaGiustina, Y. Yokota, H. Suzuki, J. de León, H. Campins, J. Licandro, M. Popescu, J. L. Rizos, R. Honda, M. Yamada, N. Sakatani, C. Honda, M. Matsuoka, M. Hayakawa, H. Sawada, K. Ogawa, Y. Yamamoto, D. S. Lauretta, S. Sugita
    Icarus, 420, Sep 15, 2024  
  • K. Yumoto, E. Tatsumi, T. Kouyama, D.R. Golish, Y. Cho, T. Morota, S. Kameda, H. Sato, B. Rizk, D.N. DellaGiustina, Y. Yokota, H. Suzuki, J. de León, H. Campins, J. Licandro, M. Popescu, J.L. Rizos, R. Honda, M. Yamada, N. Sakatani, C. Honda, M. Matsuoka, M. Hayakawa, H. Sawada, K. Ogawa, Y. Yamamoto, D.S. Lauretta, S. Sugita
    Icarus, 417 116122-116122, Jul, 2024  
  • Ryuji Okazaki, Bernard Marty, Henner Busemann, Ko Hashizume, Jamie D. Gilmour, Alex Meshik, Toru Yada, Fumio Kitajima, Michael W. Broadley, David Byrne, Evelyn Füri, My E.I. Riebe, Daniela Krietsch, Colin Maden, Akizumi Ishida, Patricia Clay, Sarah A. Crowther, Lydia Fawcett, Thomas Lawton, Olga Pravdivtseva, Yayoi N. Miura, Jisun Park, Ken Ichi Bajo, Yoshinori Takano, Keita Yamada, Shinsuke Kawagucci, Yohei Matsui, Mizuki Yamamoto, Kevin Righter, Saburo Sakai, Naoyoshi Iwata, Naoki Shirai, Shun Sekimoto, Makoto Inagaki, Mitsuru Ebihara, Reika Yokochi, Kunihiko Nishiizumi, Keisuke Nagao, Jong Ik Lee, Akihiro Kano, Marc W. Caffee, Ryu Uemura, Tomoki Nakamura, Hiroshi Naraoka, Takaaki Noguchi, Hikaru Yabuta, Hisayoshi Yurimoto, Shogo Tachibana, Hirotaka Sawada, Kanako Sakamoto, Masanao Abe, Masahiko Arakawa, Atsushi Fujii, Masahiko Hayakawa, Naoyuki Hirata, Naru Hirata, Rie Honda, Chikatoshi Honda, Satoshi Hosoda, Yu Ichi Iijima, Hitoshi Ikeda, Masateru Ishiguro, Yoshiaki Ishihara, Takahiro Iwata, Kosuke Kawahara, Shota Kikuchi, Kohei Kitazato, Koji Matsumoto, Moe Matsuoka, Tatsuhiro Michikami, Yuya Mimasu, Akira Miura, Tomokatsu Morota, Satoru Nakazawa, Noriyuki Namiki, Hirotomo Noda, Rina Noguchi, Naoko Ogawa, Kazunori Ogawa, Tatsuaki Okada, Chisato Okamoto, Go Ono, Masanobu Ozaki, Takanao Saiki, Naoya Sakatani, Hiroki Senshu, Yuri Shimaki, Kei Shirai, Seiji Sugita, Yuto Takei, Hiroshi Takeuchi, Satoshi Tanaka, Eri Tatsumi, Fuyuto Terui, Ryudo Tsukizaki, Koji Wada, Manabu Yamada, Tetsuya Yamada, Yukio Yamamoto, Hajime Yano
    Science (New York, N.Y.), 379(6634) eabo0431, Feb 24, 2023  
  • Hiroshi Naraoka, Yoshinori Takano, Jason P. Dworkin, Yasuhiro Oba, Kenji Hamase, Aogu Furusho, Nanako O. Ogawa, Minako Hashiguchi, Kazuhiko Fukushima, Dan Aoki, Philippe Schmitt-Kopplin, José C. Aponte, Eric T. Parker, Daniel P. Glavin, Hannah L. McLain, Jamie E. Elsila, Heather V. Graham, John M. Eiler, Francois Regis Orthous-Daunay, Cédric Wolters, Junko Isa, Véronique Vuitton, Roland Thissen, Saburo Sakai, Toshihiro Yoshimura, Toshiki Koga, Naohiko Ohkouchi, Yoshito Chikaraishi, Haruna Sugahara, Hajime Mita, Yoshihiro Furukawa, Norbert Hertkorn, Alexander Ruf, Hisayoshi Yurimoto, Tomoki Nakamura, Takaaki Noguchi, Ryuji Okazaki, Hikaru Yabuta, Kanako Sakamoto, Shogo Tachibana, Harold C. Connolly, Dante S. Lauretta, Masanao Abe, Toru Yada, Masahiro Nishimura, Kasumi Yogata, Aiko Nakato, Miwa Yoshitake, Ayako Suzuki, Akiko Miyazaki, Shizuho Furuya, Kentaro Hatakeda, Hiromichi Soejima, Yuya Hitomi, Kazuya Kumagai, Tomohiro Usui, Tasuku Hayashi, Daiki Yamamoto, Ryota Fukai, Kohei Kitazato, Seiji Sugita, Noriyuki Namiki, Masahiko Arakawa, Hitoshi Ikeda, Masateru Ishiguro, Naru Hirata, Koji Wada, Yoshiaki Ishihara, Rina Noguchi, Tomokatsu Morota, Naoya Sakatani, Koji Matsumoto, Hiroki Senshu, Rie Honda, Eri Tatsumi, Yasuhiro Yokota, Chikatoshi Honda, Tatsuhiro Michikami, Moe Matsuoka, Akira Miura, Hirotomo Noda, Tetsuya Yamada, Keisuke Yoshihara, Kosuke Kawahara, Masanobu Ozaki, Yu Ichi Iijima, Hajime Yano, Masahiko Hayakawa, Takahiro Iwata, Ryudo Tsukizaki, Hirotaka Sawada, Satoshi Hosoda, Kazunori Ogawa, Chisato Okamoto, Naoyuki Hirata, Kei Shirai, Yuri Shimaki, Manabu Yamada, Tatsuaki Okada, Yukio Yamamoto
    Science (New York, N.Y.), 379(6634) eabn9033, Feb 24, 2023  
  • Ryuji Okazaki, Yayoi N. Miura, Yoshinori Takano, Hirotaka Sawada, Kanako Sakamoto, Toru Yada, Keita Yamada, Shinsuke Kawagucci, Yohei Matsui, Ko Hashizume, Akizumi Ishida, Michael W. Broadley, Bernard Marty, David Byrne, Evelyn Füri, Alex Meshik, Olga Pravdivtseva, Henner Busemann, My E.I. Riebe, Jamie Gilmour, Jisun Park, Ken Ichi Bajo, Kevin Righter, Saburo Sakai, Shun Sekimoto, Fumio Kitajima, Sarah A. Crowther, Naoyoshi Iwata, Naoki Shirai, Mitsuru Ebihara, Reika Yokochi, Kunihiko Nishiizumi, Keisuke Nagao, Jong Ik Lee, Patricia Clay, Akihiro Kano, Marc W. Caffee, Ryu Uemura, Makoto Inagaki, Daniela Krietsch, Colin Maden, Mizuki Yamamoto, Lydia Fawcett, Thomas Lawton, Tomoki Nakamura, Hiroshi Naraoka, Takaaki Noguchi, Hikaru Yabuta, Hisayoshi Yurimoto, Yuichi Tsuda, Sei Ichiro Watanabe, Masanao Abe, Masahiko Arakawa, Atsushi Fujii, Masahiko Hayakawa, Naoyuki Hirata, Naru Hirata, Rie Honda, Chikatoshi Honda, Satoshi Hosoda, Yu Ichi Iijima, Hitoshi Ikeda, Masateru Ishiguro, Yoshiaki Ishihara, Takahiro Iwata, Kosuke Kawahara, Shota Kikuchi, Kohei Kitazato, Koji Matsumoto, Moe Matsuoka, Tatsuhiro Michikami, Yuya Mimasu, Akira Miura, Tomokatsu Morota, Satoru Nakazawa, Noriyuki Namiki, Hirotomo Noda, Rina Noguchi, Naoko Ogawa, Kazunori Ogawa, Tatsuaki Okada, Chisato Okamoto, Go Ono, Masanobu Ozaki, Takanao Saiki, Naoya Sakatani, Hiroki Senshu, Yuri Shimaki, Kei Shirai, Seiji Sugita, Yuto Takei, Hiroshi Takeuchi, Satoshi Tanaka, Eri Tatsumi, Fuyuto Terui, Ryudo Tsukizaki, Koji Wada, Manabu Yamada, Tetsuya Yamada, Yukio Yamamoto
    Science Advances, 8(46), Nov, 2022  

Misc.

 77
  • Honda Rie, Yamamoto Yukio, Yamazaki Junichi, Tachino Junichi, Mitsuhashi Seiji
    JAXA research and development report, 11 141-149, Mar, 2012  
    A data distribution system for still and video images acquired by High Definition Television System (HDTV) on board JAXA's Lunar Explorer Kaguya (SELENE) is now being developed aiming at providing 1.06 million HDTV frame images for both objectives of outreach and scientific analysis. The design and data model of the system based on PDAP are described in the paper.
  • Yamada Ryuhei, Yamamoto Yukio, Kuwamura Jun, Nakamura Yosio
    JAXA research and development report, 11 121-131, Mar, 2012  
    The NASA Apollo missions from 1969 to 1977 provided the first-ever seismic data from a planetary body other than the Earth. Forty years after the acquisition of these lunar seismic data, lunar scientists continue to analyze them and derive new results related to lunar geophysics. However, the users often find the data difficult to obtain and analyze because at present not all data are publicly available and archived with a convenient interface, and also because the format of the archived data is unfamiliar to many seismologists. To alleviate this difficulty, we have developed a retrieval system for the Apollo seismic data that enables the user to obtain the data and metadata necessary to use them properly. To accomplish this, we first collected most of the Apollo lunar seismic data and information required to analyze them. Then, we built a relational database consisting of the decoded lunar seismic data and an application to access the database on the World Wide Web. Using the database and application, one can search and obtain the required lunar seismic data online. This new data retrieval system will allow more people to access the existing lunar seismic data; and we anticipate that future analysis of the archived data will generate significant progress towards better understanding of the Moon and the solar system.
  • 海老沢 研, 篠原 育, 三浦 昭, 山本 幸生
    宇宙航空研究開発機構研究開発報告, 11, Mar, 2012  
  • 岡田 達明, 中村 良介, 福原 哲哉, 田口 真, 今村 剛, 関口 朋彦, 長谷川 直, 小川 佳子, 松永 恒雄, 和田 武彦, 荒井 武彦, 北里 宏平, 山本 幸生, 太刀川 純孝, はやぶさ, リモートセンシングサブチーム
    日本惑星科学会秋期講演会予稿集, 2011 45-45, Oct 23, 2011  
  • M. Ebihara, S. Sekimoto, N. Shirai, Y. Hamajima, M. Yamamoto, K. Kumagai, Y. Oura, T. R. Ireland, F. Kitajima, K. Nagao, T. Nakamura, H. Naraoka, T. Noguchi, R. Okazaki, A. Tsuchiyama, M. Uesugi, H. Yurimoto, M. E. Zolensky, M. Abe, A. Fujimura, T. Mukai, Y. Yada
    SCIENCE, 333(6046) 1119-1121, Aug, 2011  
  • 山本 幸生, 篠原 育, 笠羽 康正
    日本惑星科学会秋期講演会予稿集, 2010 44-44, Oct 6, 2010  
  • YAMADA Manabu, OGOHARA Kazunori, KOUYAMA Toru, HASHIMOTO George L., TAKAGI Masahiro, YAMAZAKI Atsushi, YAMAMOTO Yukio, IMAMURA Takeshi
    Planetary people, 19(2) 157-160, Jun 25, 2010  
  • YAMAMOTO Yukio, Management group of promotion of the education for planetary exploration
    Planetary People, 18(4) 244-245, Dec 25, 2009  
  • 寺薗淳也, 山本幸生, 篠原育, 安部正真, 祖父江真一, 笠羽康正
    日本惑星科学会秋季講演会予稿集, 2008 144, 2008  
  • 山本幸生, 篠原育, 安部正真, 祖父江真一, 寺薗淳也, 笠羽康正
    日本惑星科学会秋季講演会予稿集, 2008 34, 2008  
  • YAMAMOTO Yukio
    Planetary people, 16(3) 233-236, Sep 25, 2007  
  • Abe Masanao, Ogawa Kazutoshi, Demura Hirohide, Hirata Naru, Terazono Jun-ya, Gaskell Robert, Kominato Takashi, Hayabusa science team, Kitazato Kohei, Yoshikawa Makoto, Saito Jun, Ishiguro Masateru, Mukai Tadashi, Abe Shinsuke, Okada Tatsuaki, Yamamoto Yukio
    Abstracts for fall meeting of the Japanese Society for Planetary Science, 2007 107-107, 2007  
    The Hayabusa spacecraft, which was launched in May 2003, arrived at Asteroid Ito-kawa in September 2005, and it made observations of Itokawa and tried touch down in about three months.Hayabusa has four scientific instruments, that is Multi-Spectral Telescopic Imager (AMICA), Laser Altimeter (LIDAR), Near-Infrared Spectrometer (NIRS), and X-ray Fluorescence Spectrometer (XRS). The data obtained by these instruments were firstly analyzed by Hayabusa Science Team and some of the results have been pub-lished as scientific papers. At the same time, the science team was preparing to open them to the public and this work has almost been done. Therefore the science team release the data archives to public from April 24, 2007. All the scientific data that Hayabusa obtained are open to the public.The Hayabusa data archives can be accessed from the following web site:(URL) http://hayabusa.sci.isas.jaxa.jp/
  • 岡田達明, 白井慶, 山本幸生, 荒井武彦, 小川和律, 白石浩章, 岩崎正統, 岩崎正統, 川村太一, 森戸久貴, 三谷烈史, 加藤学
    日本惑星科学会秋季講演会予稿集, 2007 133-133, 2007  
    Analytical procedure and method is under development for the X-Ray Spectrometer onboard SELENE(Kaguya). We present the system in detail. Furterhmore, we investigate the datainterpretation for XRF, including the surface microscopic and macroscopic roughness as well as mineral mixing effects. For a daily automatic analysis for huge amount of data, correction equations for ther effects are necessary to be defined. We also present the currect status of the correction method.
  • 井上朋香, 小川和律, 岡田達明, 白井慶, 山本幸生, 荒井武彦, 加藤學
    日本惑星科学会秋季講演会予稿集, 2006 96-76, 2006  
    XRS (x-ray spectrometer) onboard Hayabusa has observed x-ray fluorescence from near-Earth asteroid 25143 Itokawa to determine major elemental composition. Okada et al. (2006) reported average elemental mass ratios of Mg/Si = 0.78 + - 0.09 and Al/Si = 0.07 + - 0.03. In this study, we attempted to estimate upper limits of Ca and Fe. To discussion about abundance of Ca and Fe, we need to integrate data longer time, fallowing the result of numerical simulation. In this poster, we report a result and the method of the analyses.
  • INOUE Tatsutoshi, YAMAMOTO Yukio, OKADA Tatsuaki, SHIRAI Kei, ARAI Takehiko, OGAWA Kazunori, INOUE Tomoka, KATO Manabu
    Proc ISAS Lunar Planet Symp (CD-ROM), 39th ROMBUNNO.21, 2006  
  • 小川和律, 加藤学, 岡田達明, 白井慶, 山本幸生, 荒井武彦, 菊池宣陽
    太陽系科学シンポジウム, 25th, 2004  
  • 菊池宣陽, 山本幸生, 荒井武彦, 白井慶, 岡田達明, 加藤学
    太陽系科学シンポジウム, 24th, 2003  
  • 岡田達明, 加藤學, 白井慶, 山本幸生, 荒井武彦, 荒井武彦
    搭載機器基礎開発実験経費・宇宙科学推進戦略的開発研究経費実績報告書, 2003, 2003  
  • 白井慶, 青木美希, 山本幸生, 荒井武彦, 赤川健一, 岡田達明, 加藤学
    宇宙科学シンポジウム 平成14年度 第3回, 87-88, 2003  
  • Abstracts Fall Meeting of the Japanese Society for Planetary Sciences, 2001 28-28, Oct 6, 2001  
    We are developing an X-Ray fluorescence Spectrometer (XRS) onboard the asteroid probe MUSES-C. Variation of solar X-rays must be considered to analyze major elements quantitatively. XRS observes solar X-rays indirectly using a standard sample. Therefore X-rays from a planetary surface can be calibrated with those from a standard sample in addition to investigation of the spectra and intensities of solar X-rays. We make a model of solar X-ray flux and simulate X-rays observed from a standard sample under various solar conditions. We estimate inversely solar X-rays with calculated emissions and investigate suitable integration times.
  • ARAI T, YAMAMOTO Y, OKADA T, KATO M
    Abstracts Fall Meeting of the Japanese Society for Planetary Sciences, 2001 84-84, Oct 6, 2001  
    We are developing an X-Ray fluorescence Spectrometer (XRS) onboard the asteroid probe MUSES-C. XRS contains 5 CCD chips. XRS will not carry in-flight calibration sources. Therefore we will observe cosmic X-ray objects for the calibration with XRS during the cruise. We performed numerical simulation of observing some known X-ray objects. Those simulations were run with exposure time about 3 hours, based on the best-fit models to the ASCA SIS spectra.
  • 山本幸生, 岡田達明, 加藤学
    太陽系科学シンポジウム, 22nd, 2001  
  • 増田英二, 岡田達明, 山本幸生, 加藤学
    太陽系科学シンポジウム, 22nd, 2001  
  • Yamamoto Yukio, Shirai Kei, Okada Tatsuaki, Matsuda Tomoki, Kato Manabu
    Abstracts Fall Meeting of the Japanese Society for Planetary Sciences, 1999 61-61, Nov 13, 1999  
  • Okada T., Shirai K., Yamamoto Y., Matsuda T., Kato M., Tsukahara F., Murao H., Taguchi K.
    Abstracts Fall Meeting of the Japanese Society for Planetary Sciences, 1999 62-62, Nov 13, 1999  
  • 岡田達明, 加藤学, 白井慶, 山本幸生, 常深博, 北本俊二
    地球惑星科学関連学会合同大会予稿集, 1998, 1998  
  • 山本幸生, 桑田良隆, 白井慶, 岡田達明, 加藤学
    地球惑星科学関連学会合同大会予稿集, 1998, 1998  

Research Projects

 3