惑星分光観測衛星プロジェクトチーム

小財 正義

コザイ マサヨシ  (Masayoshi Kozai)

基本情報

所属
情報・システム研究機構 データサイエンス共同利用基盤施設 極域環境データサイエンスセンター 特任研究員
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 (大学共同利用システム研究員)
学位
博士(理学)(2016年3月 信州大学)

J-GLOBAL ID
201901017116726616
researchmap会員ID
B000376637

分野横断型 研究データ公開システム AMIDER

https://amider.rois.ac.jp/

極域環境データサイエンスセンター

http://pedsc.rois.ac.jp/


論文

 96
  • M. Kozai, Y. Hayashi, K. Fujii, K. Munakata, C. Kato, N. Miyashita, A. Kadokura, R. Kataoka, S. Miyake, M. L. Duldig, J. E. Humble, K. Iwai
    2024年9月5日  
    The north-south (NS) anisotropy of galactic cosmic rays (GCRs) is dominated by a diamagnetic drift flow of GCRs in the interplanetary magnetic field (IMF), allowing us to derive key parameters of cosmic-ray propagation, such as the density gradient and diffusion coefficient. We propose a new method to analyze the rigidity spectrum of GCR anisotropy and reveal a solar cycle variation of the NS anisotropy's spectrum using ground-based muon detectors in Nagoya, Japan, and Hobart, Australia. The physics-based correction method for the atmospheric temperature effect on muons is used to combine the different-site detectors free from local atmospheric effects. NS channel pairs in the multi-directional muon detectors are formed to enhance sensitivity to the NS anisotropy, and in this process, general graph matching in graph theory is introduced to survey optimized pairs. Moreover, Bayesian estimation with the Gaussian process allows us to unfold the rigidity spectrum without supposing any analytical function for the spectral shape. Thanks to these novel approaches, it has been discovered that the rigidity spectrum of the NS anisotropy is dynamically varying with solar activity every year. It is attributed to a rigidity-dependent variation of the radial density gradient of GCRs based on the nature of the diamagnetic drift in the IMF. The diffusion coefficient and mean-free-path length of GCRs as functions of the rigidity are also derived from the diffusion-convection flow balance. This analysis expands the estimation limit of the mean-free-path length into $\le200$ GV rigidity region from $<10$ GV region achieved by solar energetic particle observations.
  • Masayoshi Kozai, Yoshimasa Tanaka, Shuji Abe, Yasuyuki Minamiyama, Atsuki Shinbori, Akira Kadokura
    2024年8月5日  
    The AMIDER, Advanced Multidisciplinary Integrated-Database for Exploring new Research, is a newly developed research data catalog to demonstrate an advanced database application. AMIDER is characterized as a multidisciplinary database equipped with a user-friendly web application. Its catalog view displays diverse research data at once beyond any limitation of each individual discipline. Some useful functions, such as a selectable data download, data format conversion, and display of data visual information, are also implemented. Further advanced functions, such as visualization of dataset mutual relationship, are also implemented as a preliminary trial. These characteristics and functions are expected to enhance the accessibility to individual research data, even from non-expertized users, and be helpful for collaborations among diverse scientific fields beyond individual disciplines. Multidisciplinary data management is also one of AMIDER's uniqueness, where various metadata schemas can be mapped to a uniform metadata table, and standardized and self-describing data formats are adopted. AMIDER website (https://amider.rois.ac.jp/) had been launched in April 2024. As of July 2024, over 15,000 metadata in various research fields of polar science have been registered in the database, and approximately 500 visitors are viewing the website every day on average. Expansion of the database to further multidisciplinary scientific fields, not only polar science, is planned, and advanced attempts, such as applying Natural Language Processing (NLP) to metadata, have also been considered.
  • A.Stoessl, for the GAPS collaboration, T.Aramaki, M.Boezio, S.E.Boggs, V.Bonvicini, G.Bridges, D.Campana, W.W.Craig, P.v.Doetinchem, E.Everson, L.Fabris, S.N.Feldman, H.Fuke, F.Gahbauer, C.Gerrity, L.Ghislotti, C.J.Hailey, T.Hayashi, A.Kawachi, M.Kozai, M.Law, P.Lazzaroni, A.Lenni, A.Lowell, M.Manghisoni, N.Marcelli, K.Mizukoshi, E.Mocchiutti, B.Mochizuki, S.A.I.Mogne, K.Munakata, R.Munini, S.Okazaki, J.Olson, R.A.Ong, G.Osteria, K.Perez, F.Perfetto, S.Quinn, V.Re, E.Riceputi, B.Roach, F.Rogers, J.L.Ryan, N.Saffold, V.Scotti, Y.Shimizu, K.Shu, R.Sparvoli, A.Stoessl, A.Tiberio, E.Vannuccini, M.Xiao, M.Yamatani, K.Yee, T.Yoshida, G.Zampa, J.Zeng, J.Zweerink
    Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023) 2023年9月27日  
  • M. Amenomori, S. Asano, Y. W. Bao, X. J. Bi, D. Chen, T. L. Chen, W. Y. Chen, Xu Chen, Y. Chen, Cirennima, S. W. Cui, Danzengluobu, L. K. Ding, J. H. Fang, K. Fang, C. F. Feng, Zhaoyang Feng, Z. Y. Feng, Qi Gao, A. Gomi, Q. B. Gou, Y. Q. Guo, Y. Y. Guo, Y. Hayashi, H. H. He, Z. T. He, K. Hibino, N. Hotta, Haibing Hu, H. B. Hu, K. Y. Hu, J. Huang, H. Y. Jia, L. Jiang, P. Jiang, H. B. Jin, K. Kasahara, Y. Katayose, C. Kato, S. Kato, I. Kawahara, T. Kawashima, K. Kawata, M. Kozai, D. Kurashige, Labaciren, G. M. Le, A. F. Li, H. J. Li, W. J. Li, Y. Li, Y. H. Lin, B. Liu, C. Liu, J. S. Liu, L. Y. Liu, M. Y. Liu, W. Liu, H. Lu, X. R. Meng, Y. Meng, K. Munakata, K. Nagaya, Y. Nakamura, Y. Nakazawa, H. Nanjo, C. C. Ning, M. Nishizawa, R. Noguchi, M. Ohnishi, S. Okukawa, S. Ozawa, X. Qian, X. L. Qian, X. B. Qu, T. Saito, Y. Sakakibara, M. Sakata, T. Sako, T. K. Sako, T. Sasaki, J. Shao, M. Shibata, A. Shiomi, H. Sugimoto, W. Takano, M. Takita, Y. H. Tan, N. Tateyama, S. Torii, H. Tsuchiya, S. Udo, H. Wang, S. F. Wang, Y. P. Wang, Wangdui, H. R. Wu, Q. Wu, J. L. Xu, L. Xue, Z. Yang, Y. Q. Yao, J. Yin, Y. Yokoe, Y. L. Yu, A. F. Yuan, L. M. Zhai, H. M. Zhang, J. L. Zhang, X. Zhang, X. Y. Zhang, Y. Zhang, Yi Zhang, Ying Zhang, S. P. Zhao, Zhaxisangzhu, X. X. Zhou, Y. H. Zou
    954(2) 200-200 2023年9月1日  査読有り
  • Chihiro Kato, Kazuoki Munakata, Ryuho Kataoka, Shoko Miyake, Masayoshi Kozai, Yuki Hayashi, Yoshiki Masuda, Mizuki Matsumoto
    Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023) 2023年8月18日  

講演・口頭発表等

 89

所属学協会

 6

Works(作品等)

 1

共同研究・競争的資金等の研究課題

 9

学術貢献活動

 14

社会貢献活動

 1