Degree
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Ph. D. ( 1990.3 The University of Tokyo )
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Master of Science ( Tohoku University )
Licenses and Qualifications
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高等学校（理科）専修免許
Classification of license or qualification：license
Category of license or qualification：Faculty
Current State of Research and Teaching Activities
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大学院生の修士論文は必ず学会発表させ、またできる限り学術論文として出版する。
Research Interests
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GEOTAIL
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月
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太陽風加速
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ようこう
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磁気流体波
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太陽風
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惑星間空間
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さきがけ
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平面状磁場構造
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プラズマ
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Interplanetary plasma physics
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かぐや衛星
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Coronal Mass Ejection
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反射プロトン
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地磁気変動
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太陽物理
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磁気圏物理
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惑星間空間プラズマ
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惑星間空間磁場
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Solar wind
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Solar physics
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Magnetospheric plasma physics
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非スパイラル磁場
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フラックスロープ
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月ウェイク
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磁気ロープ
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多点衛星観測
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帯電
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接線型不連続
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宇宙天気予報
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ARASE
Research Areas
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Energy Engineering / Fundamental plasma
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Natural Science / Space and planetary sciences
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Natural Science / Astronomy
Subject of Research
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太陽風と非磁化天体との相互作用
2003.4
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衛星帯電と光電子
2000.4
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下部ELF帯地磁気変動の動態の観測
1997.4
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太陽風と惑星磁気圏の相互作用の研究
1990.4
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太陽風磁場の3次元構造の解析
1985.4
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惑星間空間磁場観測の検定と較正、ノイズ分離
1985.4
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太陽風とハレー彗星の相互作用
1985.4 - 1987.3
Education
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The University of Tokyo
1987.4 - 1990.3
Country/Region： Japan
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東京大学大学院 理学系研究科 地球物理学専攻
1987.4 - 1990.3
Country/Region： Japan
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東北大学大学院 理学研究科 地球物理学専攻
1985.4 - 1987.3
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Tohoku University
1985.4 - 1987.3
Country/Region： Japan
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Tohoku University Faculty of Science
1981.4 - 1985.3
Country/Region： Japan
Research History
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Tohoku Institute of Technology Faculty of Engineering Department of Information and Communication Engineering Professor
2009.4
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Tohoku Institute of Technology Faculty of Engineering, Department of Information and Communication Engineering Associate Professor
2007.4 - 2009.3
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Tohoku Institute of Technology Faculty of Engineering, Department of Information and Communication Engineering Associate Professor
2004.4 - 2007.3
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Tohoku Institute of Technology Faculty of Engineering Associate Professor (as old post name)
1995.4 - 2004.3
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Tohoku Institute of Technology Faculty of Engineering Lecturer
1993.4 - 1995.3
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Tohoku Institute of Technology Department of Communication Engineering Assistant Professor
1992.5 - 1993.3
Country/Region：Japan
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日本学術振興会 特別研究員
1990.4 - 1992.3
Professional Memberships
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2023.11
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The Japanese society for planetary sciences
2021.4
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Astronomical Society of Japan
1996.5
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American Geophysical Union
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Society of Geomagnetism and Earth, Planetary and Space Sciences
Committee Memberships
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地球電磁気・地球惑星圏学会 学生発表賞 審査委員
2023 - 2025
Committee type：Academic society
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URSI URSI GASS 2023 Session H04 convener
2022.11 - 2023.8
Committee type：Academic society
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URSI URSI AT-AP-RASC2022 Session H03 convenor
2021.11 - 2022.7
Committee type：Academic society
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日本学術振興会 特別研究員等審査会専門委員及び国際事業委員会書面審査員・書面評価員
2021.7 - 2022.6
Committee type：Academic society
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Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS) Councilor
2021
Committee type：Academic society
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日本学術振興会 特別研究員等審査会専門委員及び国際事業委員会書面審査員・書面評価員
2020.7 - 2021.6
Committee type：Academic society
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URSI URSI GASS 2020/2021 Session H08 convener
2019.10 - 2021.9
Committee type：Academic society
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日本学術振興会 2020年度科学研究費委員会 審査・評価第二部会B小委員会2 基盤研究（S）
2019.1 - 2019.12
Committee type：Academic society
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地球電磁気・地球惑星圏学会 学生発表賞 審査委員
2019
Committee type：Academic society
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日本学術振興会 平成31(2019)年度科学研究費委員会 審査・評価第二部会B小委員会
2018.12 - 2019.11
Committee type：Academic society
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地球電磁気・地球惑星圏学会 フロンティア賞 推薦委員会委員
2018.1 - 2021.10
Committee type：Academic society
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日本学術振興会 平成31(2019)年度科学研究費委員会 審査・評価第二部会B小委員会3 基盤研究（S）
2018.1 - 2018.12
Committee type：Academic society
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地球電磁気・地球惑星圏学会 学生発表賞 審査委員
2018 - 2019
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平成30(2018)年度科学研究費委員会 審査・評価第二部会B小委員会
2017.12 - 2018.11
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科学研究費委員会委員平成29年度 挑戦的研究部会第17小委員会
2016.12 - 2017.11
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名古屋大学宇宙地球環境研究所 共同利用・共同研究委員会委員(太陽圏宇宙線専門委員会)
2015.11
Committee type：Other
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日本高等教育評価機構(JIHEE) 評価員
2014.6 - 2015.4
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地球電磁気・地球惑星圏学会 大林奨励賞候補者推薦委員会委員長
2013.11 - 2015.11
Committee type：Academic society
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地球電磁気・地球惑星圏学会 大林奨励賞候補者推薦委員会委員
2011.11 - 2013.11
Committee type：Academic society
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名古屋大学太陽地球環境研究所 共同利用委員
2010.4 - 2012.3
Committee type：Other
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名古屋大学太陽地球環境研究所 太陽圏専門委員 委員長
2010.4 - 2012.3
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名古屋大学太陽地球環境研究所 「地上ネットワーク観測大型共同研究 (重点研究)」審査員
2010.4 - 2011.3
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科学研究費委員会専門委員 (平成21年度 第１段審査委員)
2008.12 - 2009.11
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地球電磁気・地球惑星圏学会 波動分科会ワーキンググループ
2008
Committee type：Academic society
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科学研究費委員会専門委員 (平成19年度 第１段審査委員)
2006.12 - 2007.11
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名古屋大学太陽地球環境研究所 共同利用委員
2006.4 - 2008.3
Committee type：Other
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日本学術会議 電気電子工学委員会/ＵＲＳＩ分科会プラズマ波動小委員会委員
2006 - 2014.9
Committee type：Academic society
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American Geophysics Union Associate editor of JGR-Space Physics
2006 - 2007
Committee type：Academic society
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科学研究費委員会専門委員 (平成18年度 第１段審査委員)
2005.12 - 2006.11
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宇宙航空開発研究機構宇宙科学研究所 プロジェクト研究員(GEOTAILプロジェクト、あけぼのプロジェクト、BepiColomboプロジェクト)
2005
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地球電磁気・地球惑星圏学会 学生発表賞 審査委員
2005
Committee type：Academic society
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日本学術会議 電波科学研究連絡委員会Ｈ分科会委員
2004 - 2007
Committee type：Academic society
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科学研究費委員会専門委員 (平成16年度 第１段審査委員
2004
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地球電磁気・地球惑星圏学会 学生発表賞 審査委員
2004
Committee type：Academic society
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科学研究費委員会専門委員 (平成15年度 第１段審査委員)
2003
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名古屋大学太陽地球環境研究所 太陽圏専門委員
2002 - 2015.11
Job Achievement
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女子進学機会均等WG
2023.4
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人事委員会
2020.4 - 2024.3
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大学院人事委員会
2018.4 - 2024.3
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大学院通信工学専攻長
2018.4 - 2020.3
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退学者低減タスクフォース
2016.4 - 2017.3
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大学施設設備構想検討委員会
2013.4 - 2015.3
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建物の建替え計画策定WG
2013.4 - 2015.3
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ウェルネスセンター長
2012.4 - 2014.3
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人事委員会
2010.4 - 2014.3
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情報通信工学科オープンキャンパス担当
2009.4 - 2025.3
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情報通信工学科入試広報委員会
2009.4 - 2025.3
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ウェルネスセンター運営委員会
2006.4 - 2020.3
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大学施設設備構想検討委員会
2006.4 - 2012.3
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ハラスメント防止委員会
2005.9 - 2020.3
Papers
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人工衛星「あらせ」により観測された電場方向のずれの特性 Reviewed
中川朋子,三好由純, 笠羽康正,笠原禎也,土屋史紀, 熊本篤志, 北原理弘, 中村紗都子, 松岡彩子
東北工業大学紀要 理工学編・人文社会科学編 43 1 - 7 2023.3
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An Effect of Photoelectrons from Spherical Double Probes on Electric Field Measurement from ARASE Satellite Reviewed
Tomoko Nakagawa, Tomoaki Hori, Yasumasa Kasaba, Shoya Matsuda, Yoshiya Kasahara, Yoshizumi Miyoshi, Fuminori Tsuchiya, Atsushi Kumamoto, Atsuki Shinbori, And Ayako Matsuoka
Memoirs of the Tohoku Institute of Technology 45 1 - 9 2025.3
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Anticorrelation Between Sunspot Number and Spectral Resonance Structures of ELF Magnetic Variations Detected at Kawatabi, Miyagi, Japan Reviewed
URSI Radio Science Letters 5 2024.4
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Sub-ion-gyro scale magnetic field compressions generated by the solar wind interaction with the moon Reviewed
Tomoko Nakagawa, Futoshi Takahashi, Yoshifumi Saito, Hisayoshi Shimizu
Earth, Planets and Space 75 ( 1 ) 2023.12
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Diffuse whistler mode waves detected by Kaguya in the lunar polar region Reviewed
Nakagawa, T, Takahashi, F, Shimizu, H, Saito, Y
Radio Science, 57, 57 ( 1 ) e2021RS007369 2022.1
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Polarization Reversal of Low‐Frequency Magnetic Variation in the Lunar Wake Reviewed
Tomoko Nakagawa, Futoshi Takahashi, Yoshifumi Saito, Hisayoshi Shimizu
Journal of Geophysical Research: Space Physics 126 ( 8 ) 2021.8
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The BepiColombo–Mio Magnetometer en Route to Mercury Reviewed
W. Baumjohann, A. Matsuoka, Y. Narita, W. Magnes, D. Heyner, K.-H. Glassmeier, R. Nakamura, D. Fischer, F. Plaschke, M. Volwerk, T. L. Zhang, H.-U. Auster, I. Richter, A. Balogh, C. M. Carr, M. Dougherty, T. S. Horbury, H. Tsunakawa, M. Matsushima, M. Shinohara, H. Shibuya, T. Nakagawa, M. Hoshino, Y. Tanaka, B. J. Anderson, C. T. Russell, U. Motschmann, F. Takahashi, A. Fujimoto
Space Science Reviews 216 ( 8 ) 2020.12
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Electromagnetic Ion Cyclotron Waves Detected by Kaguya and Geotail in the Earth's Magnetotail Reviewed
Tomoko Nakagawa, Masaki N. Nishino, Hideo Tsunakawa, Futoshi Takahashi, Hidetoshi Shibuya, Hisayoshi Shimizu, Masaki Matsushima, Yoshifumi Saito
Journal of Geophysical Research: Space Physics 123 ( 2 ) 1146 - 1164 2018.2
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Wire Probe Antenna (WPT) and Electric Field Detector (EFD) of Plasma Wave Experiment (PWE) aboard the Arase satellite: specifications and initial evaluation results Reviewed
Yasumasa Kasaba, Keigo Ishisaka, Yoshiya Kasahara, Tomohiko Imachi, Satoshi Yagitani, Hirotsugu Kojima, Shoya Matsuda, Masafumi Shoji, Satoshi Kurita, Tomoaki Hori, Atsuki Shinbori, Mariko Teramoto, Yoshizumi Miyoshi, Tomoko Nakagawa, Naoko Takahashi, Yukitoshi Nishimura, Ayako Matsuoka, Atsushi Kumamoto, Fuminori Tsuchiya, Reiko Nomura
EARTH PLANETS AND SPACE 69 2017.12
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ULF/ELF Waves in Near-Moon Space Reviewed
Tomoko Nakagawa
Low-Frequency Waves in Space Plasmas 293 - 306 2016.2
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ELF magnetic fluctuations detected by Kaguya in deepest lunar wake associated with type-II protons Reviewed
Tomoko Nakagawa, Tatsuya Nakashima, Takuya Wada, Hideo Tsunakawa, Futoshi Takahashi, Hidetoshi Shibuya, Hisayoshi Shimizu, Masaki Matsushima, Yoshifumi Saito
EARTH PLANETS AND SPACE 67 ( Apr ) 2015.4
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Tomoko Nakagawa
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 118 ( 5 ) 1849 - 1860 2013.5
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A Disturbance of the Ion Tail of Comet Halley and the Heliospheric Structure as Observed by Sakigake Reviewed
Takao Saito, Kiyohumi Yumoto, Kunio Hirao, Keiji Saito, Tomoko Nakagawa, Edward J. Smith
Comet Encounters 821 2013.3
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Kiyohumi Yumoto, Takao Saito, Tomoko Nakagawa
Comet Encounters 825 2013.3
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Ion entry into the wake behind a nonmagnetized obstacle in the solar wind: Two-dimensional particle-in-cell simulations Reviewed
Tomoko Nakagawa
Journal of Geophysical Research: Space Physics 118 ( 5 ) 1849 - 1860 2013
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Large-amplitude monochromatic ULF waves detected by Kaguya at the Moon Reviewed
Tomoko Nakagawa, Akihito Nakayama, Futoshi Takahashi, Hideo Tsunakawa, Hidetoshi Shibuya, Hisayoshi Shimizu, Masaki Matsushima
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 117 ( A04101 ) 2012.4
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Large-amplitude monochromatic ULF waves detected by Kaguya at the Moon Reviewed
Tomoko Nakagawa, Akihito Nakayama, Futoshi Takahashi, Hideo Tsunakawa, Hidetoshi Shibuya, Hisayoshi Shimizu, Masaki Matsushima
Journal of Geophysical Research: Space Physics 117 ( 4 ) 2012
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NAKAGAWA Tomoko, KIMURA Shinya
EPS 63 ( 6 ) 477 - 486 2011.6
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Generation mechanism of the 100-second magnetic field variations observed by Kaguya around the moon
Memoirs of the Tohoku Institute of Technology. Ser.1, Science and engineering ( 31 ) 21 - 27 2011.3
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Non-monochromatic whistler waves detected by Kaguya on the dayside surface of the moon Reviewed
NAKAGAWA Tomoko, TAKAHASHI Futoshi, TSUNAKAWA Hideo, SHIBUYA Hidetoshi, SHIMIZU Hisayoshi, MATSUSHIMA Masaki
EPS 63 ( 1 ) 37 - 46 2011.1
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Role of the surface charging in the solar wind interaction with a small, non-magnetized, electrically non-conducting body studied in a two-dimensional electromagnetic full particle simulation Reviewed
Tomoko Nakagawa
2011 30th URSI General Assembly and Scientific Symposium, URSIGASS 2011 2011
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Fitting a toroidal force-free field to multispacecraft observations of a magnetic cloud Reviewed
Tomoko Nakagawa, Ayako Matsuoka
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 115 ( A10 ) A10113 2010.10
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Yoshifumi Saito, Shoichiro Yokota, Kazushi Asamura, Takaaki Tanaka, Masaki N. Nishino, Tadateru Yamamoto, Yuta Terakawa, Masaki Fujimoto, Hiroshi Hasegawa, Hajime Hayakawa, Masafumi Hirahara, Masahiro Hoshino, Shinobu Machida, Toshifumi Mukai, Tsugunobu Nagai, Tsutomu Nagatsuma, Tomoko Nakagawa, Masato Nakamura, Koh-ichiro Oyama, Eiichi Sagawa, Susumu Sasaki, Kanako Seki, Iku Shinohara, Toshio Terasawa, Hideo Tsunakawa, Hidetoshi Shibuya, Masaki Matsushima, Hisayoshi Shimizu, Futoshi Takahashi
SPACE SCIENCE REVIEWS 154 ( 1-4 ) 265 - 303 2010.7
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Magnetic field investigation of Mercury's magnetosphere and the inner heliosphere by MMO/MGF Reviewed
Wolfgang Baumjohann, Ayako Matsuoka, Werner Magnes, Karl-Heinz Glassmeier, Rumi Nakamura, Helfried Biernat, Magda Delva, Konrad Schwingenschuh, Tielong Zhang, Hans-Ulrich Auster, Karl-Heinz Fornacon, Ingo Richter, Andre Balogh, Peter Cargill, Chris Carr, Michele Dougherty, Timothy S. Horbury, Elizabeth A. Lucek, Fumio Tohyama, Takao Takahashi, Makoto Tanaka, Tsugunobu Nagai, Hideo Tsunakawa, Masaki Matsushima, Hideaki Kawano, Akimasa Yoshikawa, Hidetoshi Shibuya, Tomoko Nakagawa, Masahiro Hoshino, Yoshimasa Tanaka, Ryuho Kataoka, Brian J. Anderson, Christopher T. Russell, Uwe Motschmann, Manabu Shinohara
PLANETARY AND SPACE SCIENCE 58 ( 1-2 ) 279 - 286 2010.1
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Fitting a toroidal force-free field to multispacecraft observations of a magnetic cloud Reviewed
Tomoko Nakagawa, Ayako Matsuoka
Journal of Geophysical Research: Space Physics 115 ( 10 ) 2010
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KIMURA Shinya, NAKAGAWA Tomoko
EPS 60 ( 6 ) 591 - 599 2008.6
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A reexamination of pitch angle diffusion of electrons at the boundary of the lunar wake Reviewed
NAKAGAWA Tomoko, IIZIMA Masahide
EPS 58 ( 12 ) e17 - e20 2006.12
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Solar wind speed within 20 RS of the Sun estimated from limb coronal mass ejections Reviewed
Tomoko Nakagawa, Nat Gopalswamy, Seiji Yashiro
Journal of Geophysical Research: Space Physics 111 ( 1 ) 2006.1
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Solar wind speed within 20 R-S of the Sun estimated from limb coronal mass ejections Reviewed
T Nakagawa, N Gopalswamy, S Yashiro
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 111 ( A1 ) 2006.1
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The magnetosphere of Mercury and its solar wind environment: Open issues and scientific questions Reviewed
W. Baumjohann, A. Matsuoka, K. H. Glassmeier, C. T. Russell, T. Nagai, M. Hoshino, T. Nakagawa, A. Balogh, J. A. Slavin, R. Nakamura, W. Magnes
MERCURY, MARS AND SATURN 38 ( 4 ) 604 - + 2006
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The magnetosphere of Mercury and its solar wind environment: Open issues and scientific questions
W. Baumjohann, A. Matsuoka, K. H. Glassmeier, C. T. Russell, T. Nagai, M. Hoshino, T. Nakagawa, A. Balogh, J. A. Slavin, R. Nakamura, W. Magnes
ADVANCES IN SPACE RESEARCH 38 ( 4 ) 604 - 609 2006
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Pitch angle diffusion of electrons at the boundary of the lunar wake Reviewed
NAKAGAWA Tomoko, IIZIMA Masahide
EPS 57 ( 9 ) 885 - 894 2005.9
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瀬戸 正弘, 田頭 功, 中川 朋子
情報処理技術研究所紀要 18 ( 1 ) 81 - 92 2005.5
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Pitch angle diffusion of electrons at the boundary of the lunar wake Reviewed
T Nakagawa, M Iizima
EARTH PLANETS AND SPACE 57 ( 9 ) 885 - 894 2005
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GEOTAIL observation of upstream ULF waves associated with lunar wake Reviewed
NAKAGAWA Tomoko, TAKAHASHI Yoshinori, IIZIMA Masahide
EPS 55 ( 9 ) 569 - 580 2003.9
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瀬戸 正弘, 中川 朋子, 田頭 功
情報処理技術研究所紀要 16 ( 1 ) 25 - 36 2003.5
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GEOTAIL observation of upstream ULF waves associated with lunar wake Reviewed
T Nakagawa, Y Takahashi, M Iizima
EARTH PLANETS AND SPACE 55 ( 9 ) 569 - 580 2003
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NOZOMI observation of transient, non-spiral magnetic field in interplanetary space associated with limb CMEs Reviewed
T Nakagawa, A Matsuoka
SOLAR WIND TEN, PROCEEDINGS 679 117 - 120 2003
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瀬戸 正弘, 中川 朋子, 田頭 功
情報処理技術研究所紀要 15 ( 1 ) 53 - 63 2002.5
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Nozomi observation of the interplanetary magnetic field in 1998 Reviewed
T. Nakagawa, A. Matsuoka
Advances in Space Research 29 ( 3 ) 427 - 432 2002.2
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Nozomi observation of interplanetary transients ejected as limb coronal mass ejections Reviewed
T Nakagawa, A Matsuoka
MULTI-WAVELENGTH OBSERVATIONS OF CORONAL STRUCTURE AND DYNAMICS 13 307 - 308 2002
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瀬戸 正弘, 渡辺 富也, 中川 朋子
情報処理技術研究所紀要 14 ( 1 ) 9 - 23 2001.5
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栗原 英介, 中川 朋子
東北工業大学紀要 1 理工学編 ( 21 ) 21 - 27 2001.3
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瀬戸 正弘, 渡辺 富也, 中川 朋子
東北工業大学紀要 1 理工学編 ( 21 ) 37 - 43 2001.3
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太陽方向に伝搬するアルフベン波を利用した惑星間空間磁場の構造解析
湯村 智子, 中川 朋子
東北工業大学紀要 1 理工学編 21 ( 21 ) 29 - 35 2001.3
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GEOTAIL衛星を用いた地球前面定在衝撃波の厚さについて
栗原英介, 中川朋子
東北工業大学紀要 21 ( I ) 21 2001
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瀬戸 正弘, 渡辺 富也, 中川 朋子
情報処理技術研究所紀要 13 ( 1 ) 19 - 35 2000.5
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中川 朋子, 瀬戸 正弘, 渡辺 富也
情報処理技術研究所紀要 13 ( 1 ) 37 - 48 2000.5
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衛星電位と周辺プラズマの観測から求めた低密度プラズマ中のGEOTAIL衛星の光電子電流密度
石井 琢, 中川 朋子, 鶴田 浩一郎
東北工業大学紀要 1 理工学編 ( 20 ) 173 - 179 2000.3
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衛星電位と周辺プラズマの観測から求めた低密度プラズマ中のGEOTALL衛星の光電子電流密度(共著)
石井琢, 中川朋子, 鶴田浩一郎, 早川基, 向井利典
東北工業大学紀要 20 ( 1 ) 173 - 180 2000
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Plasma velocity in interplanetary planar magnetic structures Reviewed
T Nakagawa, S Kokubun, T Mukai
COUPLING OF THE HIGH AND LOW LATITUDE HELIOSPHERE AND ITS RELATION TO THE CORONA 26 ( 5 ) 811 - 814 2000
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Net current density of photoelectrons emitted from the surface of the GEOTAIL spacecraft Reviewed
NAKAGAWA Tomoko, ISHII Takuma, TSURUDA Koichiro, HAYAKAWA Hajime, MUKAI Toshifumi
EPS 52 ( 4 ) 283 - 292 2000
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渡辺 富也, 瀬戸 正弘, 中川 朋子
東北工業大学紀要 1 理工学編 ( 19 ) 47 - 55 1999.3
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中川朋子, 国分征, 向井利典, 斎藤義文
地球惑星科学関連学会合同大会予稿集 1998 173 1998.5
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Plasma Waves and Sounder (PWS) experiment onboard the Planet-B Mars orbiter
ONO Takayuki, OYA Hiroshi, MORIOKA Akira, KUMAMOTO Atsushi, KOBAYASHI Kaori, OBARA Takahiro, NAKAGAWA Tomoko
Earth Planets Space 50 ( 3 ) 213 - 221 1998.3
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Evaluation of Offset Components in SAKIGAKE Magnetic Field Data
NAKAGAWA Tomoko, YUMOTO Kiyohumi, SAITO Takao, KIMURA Hideto, KOBAYASHI Hiroaki
宇宙科学研究所報告 93 ( 93 ) 1 - 35 1997.3
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「さきがけ」で観測された磁場データの一次処理法:惑星間空間磁場と磁気バイアス・磁気オフセットの分離(共著)
中川朋子, 湯元清文, 斎藤尚生, 木村秀人, 小林博明
宇宙科学研究所報告 ( 93 ) 1 - 34 1997
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Evaluation of offset components in SAKIGAKE magnetic field data
Nakagawa, T, K. Yumoto, T. Saito, H. Kimura, H. Kobayashi
Bulletin of Institute of Space and Astronautical Science 93 1 - 34 1997
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中川 朋子, 鶴田 浩一郎, 早川 基
情報処理技術研究所紀要 9 ( 1 ) 5 - 14 1996.3
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地磁気座標について:地心双極子モデル,偏心双極子モデル,高次の非双極子成分を含むモデルに基づく三つの地磁気座標系の比較・検討
渡辺 富也, 中川 朋子
東北工業大学紀要 1 理工学編 ( 16 ) 29 - 45 1996.3
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Detection of active region expansion in interplanetary space by Sakigake spacecraft at 1 AU Reviewed
T Nakagawa, Y Uchida
MAGNETODYNAMIC PHENOMENA IN THE SOLAR ATMOSPHERE 503 - 504 1996
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科学衛星「あけぼの」電場観測に基づく磁気圏の静穏状態の研究(共著)
中川朋子, 鶴田浩一郎, 早川基, 松岡彩子
東北工業大学情報処理技術研究所紀要EOS 9 ( 1 ) 5 - 14 1996
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Interplanetary planar magnetic structures associated with expanding active regions Reviewed
T Nakagawa, Y Uchida
SOLAR WIND EIGHT - PROCEEDINGS OF THE EIGHTH INTERNATIONAL SOLAR WIND CONFERENCE ( 382 ) 465 - 468 1996
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5.磁気圏と太陽風の境界(<特集>GEOTAILが見た地球の尻尾)
中村 正人, 河野 英昭, 藤本 正樹, 中川 朋子, 長野 勇, 八木谷 聡, 寺沢 敏夫
遊・星・人 : 日本惑星科学会誌 4 ( 2 ) 100 - 107 1995.6
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SOLAR SOURCE OF THE INTERPLANETARY PLANAR MAGNETIC-STRUCTURES Reviewed
T NAKAGAWA
SOLAR PHYSICS 147 ( 1 ) 169 - 197 1993.9
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距離2000万kmにおける「さきがけ」マグネトテイル磁場観測
中川朋子
第2回科学衛星.宇宙観測シンポジウム(宇宙科学研究所) 1 1993
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Extreme-UV imaging of the Martian ionosphere and magnetosphere
Masato Nakamura, Koujun Yamashita, Koichiro Tsuruda, Takao Nakagawa, Yoshifumi Saito, Tomoko Nakagawa, Toshihiro Ogawa, Tatsundo Yamamoto
Proceedings of SPIE - The International Society for Optical Engineering 1744 104 - 109 1992
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SOUTHWARD MAGNETIC-FIELD IN THE NEUTRAL SHEET PRODUCED BY WAVY MOTIONS PROPAGATING IN THE DAWN-DUSK DIRECTION - REPLY Reviewed
T NAKAGAWA, A NISHIDA
GEOPHYSICAL RESEARCH LETTERS 18 ( 3 ) 481 - 481 1991.3
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On the Feasibility of Imagning Planetary Magnetosphere
NAKAGAWA TOMOKO, TSURUDA KOICHIRO
宇宙科学研究所報告. 特集 28 ( 28 ) p111 - 121 1991.3
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On the feasibility of imaging planetary magnetosphere
Nakagawa, T, K. Tsuruda
Bulletin of Institute of Space and Astronautical Science 28 1991
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惑星および地球磁気圏の撮像の可能性について(共著)
中川朋子, 鶴田浩一郎
宇宙科学研究所報告(特集巻28号) 28 1991
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Reply to Uberoi
Nakagawa, T, A. Nishida
Geophysical Research Letters 18 ( 3 ) 481 - 482 1991
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SOUTHWARD MAGNETIC-FIELD IN THE NEUTRAL SHEET PRODUCED BY WAVY MOTIONS PROPAGATING IN THE DAWN-DUSK DIRECTION Reviewed
T NAKAGAWA, A NISHIDA
GEOPHYSICAL RESEARCH LETTERS 16 ( 11 ) 1265 - 1268 1989.11
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PLANAR MAGNETIC-STRUCTURES IN THE SOLAR-WIND Reviewed
T NAKAGAWA, A NISHIDA, T SAITO
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 94 ( A9 ) 11761 - 11775 1989.9
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HYDROMAGNETIC-WAVES ASSOCIATED WITH COMETARY WATER GROUP IONS - SAKIGAKE OBSERVATION Reviewed
K YUMOTO, T SAITO, T NAKAGAWA
ASTRONOMY & ASTROPHYSICS 187 ( 1-2 ) 117 - 120 1987.11
-
Halleyすい星のIon Tailの擾乱とさきがけで観測された太陽風構造 I さきがけ磁場観測と太陽風構造
斎藤尚生, 湯元清文, 平尾邦雄, 小山孝一郎, 伊藤富造, 中川朋子, 小島正宣
宇宙科学研究所報告 ( 46 ) 16P 1987.3
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Studies on the Interplanetary Magnetic Field (IMF) observed by Sakigake
SAITO T., YUMOTO K., HIRAO K., ITOH T., NAKAGAWA T.
宇宙科学研究所報告. 特集 19 ( 19 ) 85 - 102 1987.3
-
Characteristics of IMF Structures Observed by Sakigake at the Closest Approach to Comet Halley
Nakagawa Tomoko, Saito Takao, Yumoto Kiyohumi
49 ( 49 ) p1 - 8 1987.3
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Saito Takao, Yumoto Kiyohumi, Hirao Kunio, Oyama Ko-Ichiro, Itoh Tomizo, Nakagawa Tomoko, Kojima Masanobu
46 ( 46 ) p1 - 15 1987.3
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Halleyすい星最接近時のSakigake/IMFによる惑星間空間磁場変動特性について
中川朋子, 斎藤尚生, 湯元清文
宇宙科学研究所報告 ( 49 ) 9P 1987.3
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Characteristics of IMF structures observed by Sakigake at the closest approach to comet Halley
Nakagawa,T, T. Saito, K. Yumoto
Bulletin of Institute of Space and Astronautical Science 49 1 1987
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Halley彗星最接近時のSakigake/IMFによる惑星間空間磁場変動特性について(共著)
中川朋子, 斎藤尚生, 湯元清文
宇宙科学研究所報告 49 1987
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Ring-Core Fluxgate Magnetometer Installed on Sakigake
YUMOTO Kiyohumi, SAITO Takao, NAKAGAWA Tomoko, HIRAO Kunio, AOYAMA Iwao, SETO Masahiro
15 45 - 57 1986.9
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A DISTURBANCE OF THE ION TAIL OF COMET HALLEY AND THE HELIOSPHERIC STRUCTURE AS OBSERVED BY SAKIGAKE Reviewed
T SAITO, K YUMOTO, K HIRAO, K SAITO, T NAKAGAWA, EJ SMITH
GEOPHYSICAL RESEARCH LETTERS 13 ( 8 ) 821 - 824 1986.8
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K YUMOTO, T SAITO, T NAKAGAWA
GEOPHYSICAL RESEARCH LETTERS 13 ( 8 ) 825 - 828 1986.8
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INTERACTION BETWEEN COMET HALLEY AND THE INTERPLANETARY MAGNETIC-FIELD OBSERVED BY SAKIGAKE Reviewed
T SAITO, K YUMOTO, K HIRAO, T NAKAGAWA, K SAITO
NATURE 321 ( 6067 ) 303 - 307 1986.5
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Geomagnetic Storm-Associated Interplanetrary Disturbances Observed by SAKIGAKE (Planet-A Mission)
YUMOTO Kiyohumi, OYAMA Kohichiro, SAITO Takao, HIRAO Kunio, HIRANO Takafumi, NAKAGAWA Tomoko
14 ( 14 ) p33 - 45 1986.3
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Characteristics of Interplanetary Magnetic Discontinuities Observed by SAKIGAKE (Planet-A Mission)
NAKAGAWA Tomoko, SAITO Takao, YUMOTO Kiyohumi
14 ( 14 ) p47 - 57 1986.3
-
Characteristics of interplanetary magnetic discontinuities observed by SAKIGAKE (Planet-A mission)
Nakagawa,T, T. Saito, K. Yumoto
Bulletin of Institute of Space and Astronautical Science 14 47 1986
-
「さきがけ」によって観測された太陽風磁気不連続の特性(共著)
湯元清文, 小山孝一郎, 斎藤尚生, 平尾邦雄, 平野孝文, 中川朋子
宇宙科学研究所報告(特集巻14号) 14 33 1986
Books
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ULF/ELF waves in the near-Moon space
NAKAGAWA Tomoko（Low-Frequency Waves in Space Plasmas）
American Geophysical Union 2016.2 （ ISBN:9781119055006 ）
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NOZOMI observation of transient, non-spiral magnetic field in interplanetary space associated with limb CMEs
Solar Wind Ten, edited by M. Velli, R.Bruno, and F.Malara, American Institute of Physics, Melville, New York 2003
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NOZOMI Observation of interplanetary transients ejected as limb coronal mass ejections.
COSPAR colloquia series Vol.13, Multi-wavaelength observations of coronal structures and dynamics, edited by Martens,C.H. and D.P.Cauffman, Pergaman, New York, 2002
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Detection of active region expansion in interplanetary space by SAKIGAKE spacecraft at 1 AU
Proceedings of I. A. U. Colloquim 153, "Magneto-dynamic Phenomena in the Solar Atmosphere -Proto types of stellar Magnetic activity-" (Kluwer Academic Publishers) 1996
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Interplanetary planar magnetic structures associated with expanding active regions
Solar Wind Eight (AIP Press) 1996
MISC
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Tomoko NAKAGAWA, Yasumasa KASABA, Yoshiya KASAHARA, Yoshizumi MIYOSHI
33 ( 1 ) 87 - 96 2021.2
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Polarization of ultra-low frequency waves observed by Kaguya at low altitude above the Moon in the earth’s magnetosphere
中川朋子, 遠藤聖也, 久保勇登, 高橋太, 清水久芳, 齋藤義文
地球電磁気・地球惑星圏学会総会及び講演会(Web) 150th 2021
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Electromagnetic full particle simulation of the electric field structure around the moon
木村進矢, 中川朋子
Memoirs of the Tohoku Institute of Technology. Ser.1, Science and engineering ( 27 ) 17 - 25 2007.3
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Reconstructed global feature of an interplanetary disturbance for the full-halo coronal mass ejection event on 1999 September 20 Reviewed
M. Tokumaru, M. Yamashita, M. Kojima, K. Fujiki, T. Nakagawa
CORONAL MASS EJECTIONS AND SOLAR PARTICLE EVENTS IN SOLAR CYCLE 23 38 ( 3 ) 547 - 551 2006
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中川朋子, 飯島雅英
宇宙航空研究開発機構特別資料 JAXA-SP- ( 05-024 ) 49 - 52 2005.12
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木村進矢, 中川朋子
宇宙航空研究開発機構特別資料 JAXA-SP- ( 05-024 ) 53 - 56 2005.12
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The Thickness of Earth's Bow Shock Obtained by GEOTAIL High Time Resolution Magnetic Field Data.
栗原英介, 中川朋子
東北工業大学紀要 1 理工学編 ( 21 ) 21 - 27 2001.3
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Anomalous ELF electromagnetic waves associated with earthquakes.
瀬戸正弘, 渡辺富也, 中川朋子, 田頭功, 山本光あき
東北工業大学情報処理技術研究所紀要 13 ( 1 ) 19 - 35 2000.5
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A Problem of Intrinsic Noises of the Preamplifier in Induction Magnetometer Systems.
田頭功, 瀬戸正弘, 渡辺富也, 中川朋子, 山本光あき
東北工業大学情報処理技術研究所紀要 12 ( 1 ) 29 - 38 1999.5
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渡辺富也, 瀬戸正弘, 中川朋子, 田頭功, 山本光あき
東北工業大学紀要 1 理工学編 ( 19 ) 47 - 55 1999.3
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渡辺富也, 中川朋子
東北工業大学紀要 1 理工学編 ( 16 ) 29 - 45 1996.3
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Observation Plan of Martian Ionosphere by using Plasma Waves and Sounder Experiments onboard Planet-B Spacecraft.
小野高幸, 大家寛, 熊本篤志, 中川朋子, 小原隆博, 岡田達明, 丸橋克英, 宮岡宏, 小林香
地球惑星科学関連学会合同大会予稿集 1996 1996
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The observation plan by PWS installed on Planet-B.
小野高幸, 森岡昭, 大家寛, 中川朋子, 小原隆博, 岡田達明, 丸橋克英, 宮岡宏, 小林香
科学衛星・宇宙観測シンポジウム 4th 144 - 147 1995.12
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GEOTAIL Observation of the Earth's Tail. Boundary between Magnetosphere and the Solar Wind.
中村正人, 河野英昭, 藤本正樹, 中川朋子, 長野勇, 八木谷聡, 寺沢敏夫
日本惑星科学会誌 遊・星・人 4 ( 2 ) 100 - 107 1995.6
-
Polar Cap Convection in Intervals of IMF Bz=0.
中川朋子, 鶴田浩一郎, 西田篤弘, 松岡彩子, 早川基, LEPPING R, 納谷朋広, 手嶋啓一
地球惑星科学関連学会合同大会予稿集 1994 570 1994.3
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Development of a large diameter electron beam source.
早川基, 河野祐一, 鶴田浩一郎, 松岡彩子, 中川朋子, 吉田潤
搭載機器基礎開発成果報告書 4 116 - 121 1991.3
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The construction of the space colony.
中川朋子
IATSS Rev (Int Assoc Traffic Saf Sci) 15 ( 1 ) 42 - 50 1989.3
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小島正宜, 寺沢敏夫, 袴田和幸, 桜井隆, 中川朋子, 松田卓也, 桜井邦朋, 斎藤尚生, 牧島一夫
磁気圏・電離圏シンポジウム 昭和63年度 106P 1989
Presentations
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Correlation of spacecraft potential to the latest electron density data observed by Arase
Keiya Kawagata, Yasumasa Kasaba, Atsuki Shinbori, Koki Tachi, Fuminori Tsuchiya, Yoichi Kazama, Tomoko Nakagawa, Yuto Katoh
SGEPSS 2025 2025.11
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The inner edge location of SAPS electric field and the ring current in the equatorial magnetosphere as observed by Arase and SuperDARN International coauthorship
Hori, T., Y. Miyoshi, S. Nakamura, Y. Kasaba, T. Nakagawa, M. Kitahara, S. Matsuda, N. Nishitani, S. G. Shepherd, J. M. Ruohoniemi, A. Kumamoto, F. Tsuchiya, Y. Kasahara, K. Asamura, Chae-Woo Jun, Y. Kazama, S.-Y. Wang, Sunny W. Y. Tam, K. Keika10, S. Kasahara, S. Yokota, A. Matsuoka, I. Shinohara
JpGU2023 2023.5 JpGU2023
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Estimation of a spurious electric field arising from spacecraft charging and photoelectron cloud using PWE/EFD onboard ARASE
Tsubasa Konno, Tomoko Nakagawa, Tomoaki Hori, Yasumasa Kasaba, Shoya Matsuda, Yoshiya Kasahara, Yoshizumi Miyoshi, Fuminori Tsuchiya, Atsushi Kumamoto, Atsuki Shinbori, Ayako Matsuoka
SGEPSS 2025 2025.11
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Estimation of spurious sunward electric field observed by double probes onboard Arase and Geotail
Tsubasa Konno, Tomoko Nakagawa, Tomoaki Hori, Yasumasa Kasaba, Shoya Matsuda, Yoshiya Kasahara, Yoshizumi Miyoshi, Fuminori Tsuchiya, Atsushi Kumamoto, Atsuki Shinbori, Ayako Matsuoka
SGEPSS 2025 2025.11
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Behavior of Spurious Electric Field Components and Spacecraft Charging Measured by Double Probes of PWE/EFD Onboard Arase Invited International conference
Tomoko Nakagawa, Tomoaki Hori, Yasumasa Kasaba, Shoya Matsuda, Yoshiya Kasahara, Yoshizumi Miyoshi, Fuminori Tsuchiya, Atsushi Kumamoto, Atsuki Shinbori, Ayako Matsuoka, Tsubasa Konno
Asia Oceania Geoscience Society 2025 2025.7 Asia Oceania Geoscience Society
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Estimation of spurious electric field components produced by spacecraft charging based on the double probe measurements International conference
Tomoko Nakagawa, Tomoaki Hori, Yasumasa Kasaba, Shoya Matsuda, Yoshiya Kasahara, Yoshizumi Miyoshi, Fuminori Tsuchiya, Atsushi Kumamoto, Atsuki Shinbori, Ayako Matsuoka
Japan Geoscience Union 2025 2025.5 Japan Geoscience Union
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Occurrence property of spectral resonance structures with frequency separation of 0.2 Hz detected at Kawatabi, Miyagi, Japan International conference
Ryuya Sonta, Yutaro Endo, Shunsuke Suto, and Tomoko Nakagawa
Japan Geoscience Union 2025 2025.5 Japan Geoscience Union
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Spatial extent of photoelectrons estimated from the spacecraft potential at electricfield waveform distortion
Nakagawa, T., T. Konno, H. Ito, K. Mano, T. Hori, Y. Kasaba, Y. Miyoshi, S. Matsuda, Y. Kasahara, I. Shinohara
156th SGEPSS Fall Meeting, 2024.11 SGEPSS
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Subtraction of spurious sunward electric field component generated by photoelectrons and spacecraft charging
Society of Geomagnetism and Earth, Planetary and Space Sciences 2023.9 Society of Geomagnetism and Earth, Planetary and Space Sciences
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Modeling Electric Potential Produced by Photoelectrons and Spacecraft charging: A case of the Arase satellite International conference
Nakagawa, T. T. Hori, S. Nakamura, Y. Kasaba, M. Shoji, Y. Miyoshi, M. Kitahara, S. Matsuda, Y. Kasahara, I. Shinohara
URSI GASS 2023 2023.8 URSI
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Waveform of DC to low-frequency electric field data obtained by PWE/EFD onboard the Arase satellite
Nakagawa, T, Y. Kasaba, M. Shoji, S. Nakamura, T. Hori, Y. Miyoshi, Kitahara, S. Matsuda, H. Kojima, Y. Kasahara, I. Shinohara
SGEPSS 2020.11
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MHD waves responsible for solar wind heating detected in the type III solar radio bursts
The Sixth International Workshop on Nonlinear Waves and Turbulence in Space Plasmas 2006
-
木村進矢, 中川朋子
宇宙航空研究開発機構特別資料 JAXA-SP- 2005.12
-
中川朋子, 飯島雅英
宇宙航空研究開発機構特別資料 JAXA-SP- 2005.12
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リムCMEの加速度を用いた20太陽半径以内の背景太陽風速の推定
中川朋子, YASHIRO Seiji, GOPALSWAMY Nat
日本天文学会年会講演予稿集 2004
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地球磁気圏ローブ中の月周辺のイオンサイクロトロン波の発生特性
中川朋子, 綱川秀夫, 斎藤義文
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2015
-
月ウェイク中でタイプIIプロトン侵入に伴って観測されたELF波動の発生機構について
中川朋子, 綱川秀夫, 斎藤義文
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2014
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月ウェイク中央で観測された0.1‐10Hzの磁場変動と太陽風プロトン
中川朋子, 綱川秀夫
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2013
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太陽風と無磁場天体との相互作用:ウェイクへのイオンの侵入過程
中川朋子
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2012
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かぐや衛星によって月周辺で観測される100秒周期磁場変動の発生機構
中山研仁, 中川朋子, 綱川秀夫, 松島政貴, 高橋太, 渋谷秀敏, 清水久芳
東北工業大学紀要 1 理工学編 2011.3
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中川朋子, 綱川秀夫
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2011
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かぐや衛星によって月周辺で観測される100秒周期磁場変動の発生機構
中山研仁, 中川朋子, 高橋太, 綱川秀夫
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2010
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磁場をもたない小天体と太陽風の相互作用の2次元PICシミュレーション
中川朋子
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2010
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Kaguyaで観測されたmonochromatic whistler waveの統計解析
津川靖基, 寺田直樹, 加藤雄人, 小野高幸, 綱川秀夫, 中川朋子
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2010
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かぐや(SELENE)衛星によって月の昼側で観測されたホイッスラー波
中川朋子, 高橋太, 綱川秀夫
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2009
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かぐや衛星による地球磁気圏ローブ中の月周辺のイオンサイクロトロン波の観測
中川朋子, 綱川秀夫
日本地球惑星科学連合大会予稿集(Web) 2015
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North-south asymmetry of sense of polarization of magnetic fluctuations at the wake boundary in the By-dominated solar wind magnetic field
Nakagawa, T, H. Tsunakawa, Y. Saito
JpGU2017 2017.5
-
Diffuse magnetic fluctuations in the frequency range 1-12Hz detected by Kaguya above the polar regions of the moon
Sugata, Y, S. Ito, T. Nakagawa, H. Tsunakawa
JpGU2017 2017.5
-
Software for virtual 3-dimensional display of Kaguya in-situ observation of magnetic field and the magnetic anomalies on the moon
Takatera, H, Nakagawa, T, H. Tsunakawa
JpGU2017 2017.5
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Polarization characteristics of Pc1 pearl structure observed at Kawatabi, Osaki, Miyagi prefecture
Shinya Miyake, Seiya Yamakawa, Yuma Doi, Tomoko Nakagawa
JpGU2017 2017.5
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Difference between North-South and East-West components of ELF magnetic disturbances associated with lightning detected at Kawatabi, Osaki, Miyagi, Japan
Takahashi, S, K. Nishiyama, T. Nakagawa
JpGU2017 2017.5
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かぐや衛星によって太陽風中で観測された10秒程度の磁場強度増大について
刈部陽子, 宮澤豪, 村上健太郎, 中川朋子, 綱川秀夫
日本地球惑星科学連合大会予稿集(Web) 2016
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かぐや衛星とGEOTAIL衛星によって観測された地球磁気圏尾部プラズマシート境界中のイオンサイクロトロン波
中川朋子, 綱川秀夫
日本地球惑星科学連合大会予稿集(Web) 2016
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月ウェイクへの太陽風電子の流入とELF帯磁場変動に関する考察
中川朋子, 綱川秀夫, 斎藤義文, 西野真木
日本地球惑星科学連合大会予稿集(Web) 2016
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衛星かぐやが月周辺で観測した周波数帯3‐10Hzの磁場変動の強さについて
渡邊祐輔, 照井孝輔, 香川翔吾, 中川朋子, 綱川秀夫
日本地球惑星科学連合大会予稿集(Web) 2015
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菅井智寛, 鵜池竜名, 中川朋子
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2015
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2衛星によって観測された磁気ロープのトーラス型モデルへのフィッティング
中川朋子
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2007
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Southward magnetic field in the neutral sheet produced by wavy motions propagating in the dawn-dusk direction
IAGA 1989
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Planar magnetic structures in the solar wind
IAGA 1989
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The polar cap in intervals of By=Bz=0 in the solar wind
AGU Western Pacific Geophysical Meeting 1992
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Magnetosphere under the IMF condition By=Bz=0
IUGG 1991
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Recurrence of planar magnetic structures
IUGG 1991
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Solar and solar wind conditions for planar magnetic structures
AGU Western Pacific Geophysical Meeting 1990
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磁気圏・電離圏シンポジウム 昭和63年度 文部省宇宙科学研究所S
小島正宜, 寺沢敏夫, 袴田和幸, 桜井隆, 中川朋子, 松田卓也, 桜井邦朋, 斎藤尚生, 牧島一夫
磁気圏・電離圏シンポジウム 昭和63年度 1989
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Finding the solar source of interplanetary planar magnetic structures: Expanding active regions
8th STEPsymposium of SCOSTEP 1994
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距離2000万kmにおける「さきがけ」マグネトテイル磁場観測
中川朋子, 湯元清文, 斎藤尚生, 大家寛, 森岡昭, 飯島雅英, 小山孝一郎, 阿部琢美
科学衛星・宇宙観測シンポジウム 1993.10
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Interplanetary planar magnetic structures and magnetic loops on the Sun
7th Scientific Assembly of IAGA 1993
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探査機「さきがけ」の磁気バイアスと磁気センサーオフセットの長期変化
中川朋子, 湯元清文, 斎藤尚生
地球惑星科学関連学会合同大会予稿集 1997.3
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Planet‐B搭載サウンダーならびにプラズマ波動観測装置による火星電離圏観測計画
小野高幸, 大家寛, 熊本篤志, 中川朋子, 小原隆博, 岡田達明, 丸橋克英, 宮岡宏, 小林香
地球惑星科学関連学会合同大会予稿集 1996.3
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中川朋子
地球惑星科学関連学会合同大会予稿集 1996.3
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Modeling geometrical configuration of interplanetary planar magnetic structures
Western Pacific Geophysics Meeting 1996
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小野高幸, 森岡昭, 大家寛, 中川朋子, 小原隆博, 岡田達明, 丸橋克英, 宮岡宏, 小林香
科学衛星・宇宙観測シンポジウム 1995.12
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Effect of IMF By on Polar Convection in the IMF Condition of Bz=0.
中川朋子, 鶴田浩一郎, 西田篤弘, 松岡彩子, 早川基
地球惑星科学関連学会合同大会予稿集 1995.3
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Interplanetary planar magnetic structures associated with expansion active region
Solar Wind 8 1995
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Detection of active region expansion in interplanetary space by Sakigake spacecraft at 1AU
International Astrophysics Union (IAU) Colloquium No.153 1995
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中川朋子, 内田豊
地球惑星科学関連学会合同大会予稿集 1994.3
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中川朋子, 鶴田浩一郎, 西田篤弘, 松岡彩子, 早川基, LEPPING R, 納谷朋広, 手嶋啓一
地球惑星科学関連学会合同大会予稿集 1994.3
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Interplanetary expansion of expanding active regions
2nd SOLTIP symposium 1994
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Net current density of photoelectrons emitted from the surface of the GEOTAIL spacecraft
The 8th GEOTAIL Workshop 2001
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Investigation of the thickness of the Earth's bow shock: GEOTAIL high time resolution data, The First S-RAMP Conference
First S-RAMP Conference 2000
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The global configuration of magnetic field lines with sunward-propagating Alfven waves
The First S-RAMP Conference 2000
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NOZOMI observation of the interplanetary magnetic field in 1998
COSPAR Scientific assembly 2000
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Multipoint observation of Interplanetary magnetic field structures by using NOZOMI spacecraft
Western Pacific Geophysics Meeting 2000
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Detection of sunward-propagating Alfven waves along IMF
Western Pacific Geophysics Meeting 2000
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The thickness of Earth's bow shock obtained by GEOTAIL high time resolution MGF data
Western Pacific Geophysics Meeting 2000
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On the thickness of Earth's Bow shock: GEOTAIL high time resolution magnetic field data
7th GEOTAIL Workshop 2000
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Detection of Alfven waves propagating toward the sun along IMF
7th GEOTAIL Workshop 2000
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鎌田友果, 森田諭, 野瀬友美, 小竹茂太, 岩井重陽, 小野貴士, 中川朋子, 内田豊
日本天文学会年会講演予稿集 1998
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Interplanetary planar magnetic structures and its relation to solar structure
Scientific Assembly of COSPAR 1998
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Magnetic structure of interplanetary counterpart of a halo CME: simultaneous observation by NOZOMI and ACE
COSPAR, Scientific assembly 2004
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Estimation of solar wind speed within 20Rs of the Sun by using limb CMEs
COSPAR, Scientific assembly 2004
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Electric potential at the boundary of the lunar wake investigated from upstream waves of whistler mode
AOGS 1st Annual Meeting 2004
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Solar wind speed within 20Rs of the Sun estimated from limb CMEs
AOGS 1st Annual Meeting 2004
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中川朋子
日本天文学会年会講演予稿集 2003
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Initial speed of CME and their propagation speed in interplanetary space
IUGG 2003
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Comparison of interplanetary magnetic field observed by Nozomi and Geotail spacecraft
The seventh GEOTAIL Workshop 2003
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NOZOMI observation of transient, non-spiral magnetic field in interplanetary space associated with limb CMEs
Solar Wind 10 2002
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NOZOMI Observation of interplanetary transients ejected as limb coronal mass ejections
Multi-wavelength observations of coronal structures and dynamics - Yohkoh 10 Anniversary Meeting 2002
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Interplanetary Alfven waves propagating toward the sun
The 8th GEOTAIL Workshop 2001
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Investigation of the thickness of the Earth's bow shock
The 8th GEOTAIL Workshop 2001
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かぐや(SELENE)衛星搭載磁力計によって観測された100秒周期の磁場変動の発生特性
中川朋子, 中山研仁, 高橋太, 綱川秀夫
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2009
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中川朋子
地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM) 2008
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A protrusion from the terminator of the Mars observed on November 4, 2003
37th COSPAR Scientific Assembly 2008, Montreal 2008
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Fitting a torus-type flux rope model to the multi-spacecraft observation of the magnetic cloud on April 16-18, 1999
37th COSPAR Scientific Assembly 2008, Montreal 2008
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Full particle simulation of the electric field structure around the moon and the lunar wake
37th COSPAR Scientific Assembly 2008, Montreal 2008
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木村進矢, 中川朋子
東北工業大学紀要 1 理工学編 2007.3
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Polarization of ultra-low frequency waves observed by Kaguya at low altitude above the Moon in the earth’s magnetosphere
SGEPSS 2021.11
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Evaluation of the Wire Probe Antenna (WPT) and Electric Field Detector (EFD) of Plasma Wave Experiment (PWE) aboard ARASE: The data qualifications and cautions from the first-year observations
JpGU2018 2018.5
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On the Kelvin-Helmholtz-like waves at the lunar wake boundary in the solar wind
Nakagawa, T, H. Tsunakawa, Y. Saito
SGEPSS 2017 2017.10
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Search of energy source of 1-16Hz Whistler Mode Waves Detected by Kaguya in the Lunar Polar Orbit
Nakagawa, T, F. Takahashi, H. Shimizu, Y. Saito
JpGU-AGU Joint Meeting 2020 2020.7
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Direction of oscillation of the ELF waves associated with the type-II entry protons in the deepest lunar wake
Nakagawa, T, F. Takahashi, H. Shimizu, Y. Saito
SGEPSS 2019.10
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Extremely Low Frequency Whistler Mode Wave above the Polar Region of the Moon Detected by Kaguya
Nakagawa, T, F. Takahashi, H. Shimizu, Y. Saito
URSI-JRSM2019 2019.9
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Energy conversion process at the lunar wake boundary
Nakagawa, T, H. Tsunakawa, Y. Saito
JpGU2019 2019.5
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Magnetic field disturbances associated with the magnetic dipolarization observed by Arase (ERG) in the inner magnetosphere
JpGU2019 2019.5
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Falling-tone ELF magnetic fluctuations detected by Kaguya above the lunar polar region
Nakagawa, T, H. Tsunakawa
SGEPSS 2018.11
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Field aligned electron flow generated by vortex at the lunar wake boundary
JpGU2018 2018.5
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Magnetic field disturbances observed by Arase (ERG) associated with the magnetic dipolarization
JpGU2018 2018.5
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Small scale limb compressions detected by Kaguya
Nakagawa, T, H. Tsunakawa
SELENE symposium 2017 2017.9
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Diffuse Whistler Mode Waves Detected by Kaguya in the Lunar Polar Orbit
Nakagawa, T, F. Takahashi, H. Shimizu, Y. Saito
URSI GASS 2021 2021.9
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Elliptically polarized 0.01-0.3 Hz magnetic field variation in the lunar wake
Nakagawa, T, F. Takahashi, H. Shimizu, Y. Saito
JpGU2021 2021.6
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Interference with electric field observation caused by spacecraft charging and photoelectrons
2022.11
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Short Period Magnetic Field Enhancements Detected by Kaguya Around the Moon in the Solar Wind
T. Nakagawa, F. Takahashi, H. Shimizu, Y. Saito
3rd URSI AT-AP-RASC 2022.5
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Hot flow anomalies and smallest scale limb compression detected by Kaguya around the moon in the solar wind
JpGU2022 2022.5
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Spin-modulated components in the spacecraft potential distorting the electric field measurement of the Arase satellite
2021.11
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Velocity of ions refilling the lunar wake observed by Kaguya
CHiba, K., K. Mochiishi, T. Nakagawa, Y. Saito, F. Takahashi
JpGU2022 2022.5
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- Invited
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- 2021.2 Nagoya University ISEE
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Spectral Resonance Structure in 0.5-8Hz Magnetic Field Variations Detected at Kawatabi, Miyagi, Japan International conference
Taiki Sato, Chihiro Kumagai, Tomoko Nakagawa
URSI GASS 2023 2023.8
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Anti-correlation between sunspot number and spectral resonance structures of ELF magnetic variations at Kawatabi, Japan
Taiki Sato, Chihiro Kumagai, Tomoko Nakagawa
JpGU2023 2023.5 JpGU
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Non-sinusoidal waveforms of electric potential produced by photoelectrons and spacecraft charging detected by Arase PWE
Nakagawa, T. T. Hori, S. Nakamura, Y. Kasaba, M. Shoji, Y. Miyoshi, M. Kitahara, S. Matsuda, Y. Kasahara, I. Shinohara
JpGU2003 2023.5 JpGU
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Removal of spurious sunward electric field components generated by photoelectrons and spacecraft charging
T. Nakagawa, T. Hori, Y. Kasaba, M. Shoji, Y. Miyoshi, S. Matsuda, Y. Kasahara, I. Shinohara
Japan Geophysical Union 2024 Assembly 2024.5 Japan Geophysical Union
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Spectral resonance structures with frequency separation of 0.2 Hz detected at Kawatabi, Miyagi, Japan
Hayato Konno, Makishi Kikuchi, Tomoko Nakagawa
Japan Geophysical Union 2004 assembly 2024.5 Japan Geophysical Union
Works
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太陽風中の月および月ウェイクの電磁環境
2009 - 2011
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太陽風速度の発展過程の研究
2005 - 2007
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Estimation of solar wind speed within 20Rs of the Sun by using limb CMEs
2002 - 2005
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非スパイラル太陽風磁場とCME
2002 - 2003
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Observation of Solar Wind Magnetic Field by using NOZOMI Spacecraft
1998
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惑星間空間非スパイラル磁場による太陽風の放出源の同定
1997 - 1998
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Electromagnetic Environment in Extreme Low Frequency Range
1997
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惑星間空間の平面状磁場構造
1995 - 1996
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Solar source of non-spiral magnetic field
1994 - 1995
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太陽風磁場構造の発展過程
1993
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太陽風磁場の三次元構造
1990 - 1991
Awards
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2020.5 SGEPSS
Nakagawa Tomoko
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Tanakadate Award
2020.5 Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS) Studies on solar wind magnetic structure and the interaction of small bodies with ambient plasma
Tomoko Nakagawa
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トーキン科学技術振興財団研究奨励賞
1994
Research Projects
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2024.4 - 2025.3
Planetary Plasma and Atmospheric Research Center (PPARC), Graduate School of Science, Tohoku University -
T. Nakagawa, Y. Kasaba, F. Tsuchiya
Authorship：Principal investigator
-
2023.4 - 2024.3
Planetary Plasma and Atmospheric Research Center (PPARC), Graduate School of Science, Tohoku University -
Authorship：Principal investigator
-
2022.4 - 2023.3
Planetary Plasma and Atmospheric Research Center (PPARC), Graduate School of Science, Tohoku University -
Authorship：Principal investigator
-
2019.4 - 2020.3
Planetary Plasma and Atmospheric Research Center (PPARC), Graduate School of Science, Tohoku University -
Authorship：Principal investigator
-
2018.4 - 2019.3
Planetary Plasma and Atmospheric Research Center (PPARC), Graduate School of Science, Tohoku University -
Authorship：Principal investigator
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First Mercury magnetospheric exploration by electromagnetic waves: Laying the groundwork and initial observational activities
Grant number：24K00687 2024.4 - 2028.3
Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B)
Authorship：Coinvestigator(s)
Grant amount：\18720000 （ Direct Cost: \14400000 、 Indirect Cost：\4320000 ）
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Solar wind interaction with the moon in the scale between magnetohydrodyamic and cyclotron radius scales
Grant number：18K03727 2018.4 - 2022.3
Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C) Grant-in-Aid for Scientific Research (C)
Nakagawa Tomoko
Authorship：Principal investigator
Grant amount：\3380000 （ Direct Cost: \2600000 、 Indirect Cost：\780000 ）
Knowledge of solar wind interaction with the moon has been renewed by recent high time resolution observations. In addition to previously known hydrodynamic scale phenomena such as wake formation and upstream wave generation by reflected ions, we have studied magnetic field variations such as limb compression and diamagnetic cavities with magnetic enhancements with duration shorter than ion gyro period, shear Alfven waves generated at thin wake boundary, or diffuse whistler mode waves above the polar region separated from their generator ions. Their generation mechanisms were related with smallness of the magnetic anomaly, lunar radius smaller than the Larmour radius of the ions reflected by the moon, or thin boundary of the lunar wake.
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Study on the electromagnetic environment formed by non-magnetized body in the solar wind
Grant number：24540480 2012.4 - 2016.3
Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C) Grant-in-Aid for Scientific Research (C)
Nakagawa Tomoko, TSUNAKAWA Hideo, SAITO Yoshifumi
Authorship：Principal investigator Grant type：Competitive
The ion entry into the wake behind an obstacle in the solar wind was studied using two-dimensional, electromagnetic full-particle simulations. The Electric field produced by the negative electric charge on the nightside surface of the obstacle accelerates ions toward the void, over longer Debye length than in the solar wind due to the reduced electron density. The ions can access the deepest wake behind a large-scale obstacle being accelerated over a long distance.
Kaguya detected low-frequency magnetic field fluctuations generated by the modified velocity distribution of the solar wind particles reflected or absorbed by the moon. The reflected protons are responsible for the generation of ULF and monochromatic ELF waves through interaction with magnetohydrodynamic and whistler waves in the solar wind. Beams of electrons reflected above the dayside lunar magnetic anomaly, or sucked into the proton rich region in the central wake are the source of broadband ELF waves. -
太陽風プラズマ流の中の月の電磁的役割の解明
2011.11 - 2013.5
住友財団 基礎科学助成
中川 朋子
Authorship：Principal investigator Grant type：Competitive
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Electromagnetic environment of the moon in the solar wind and the lunar wake
Grant number：21540461 2009.4 - 2012.3
Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C) Grant-in-Aid for Scientific Research (C)
NAKAGAWA Tomoko, TSUNAKAWA Hideo, SAITO Yoshifumi
Authorship：Principal investigator Grant type：Competitive
The solar wind interaction with the moon was studied using a two-dimensional electromagnetic full particle simulation and Kaguya observation. The solar wind magnetic field controls the direction of the thermal flow of the electrons and causes an asymmetry of the negative charging of the downstream-side surface. The solar wind ions are accelerated by the negative surface charging, while the solar wind electrons are expelled by the negative charging and flow away along the field line producing streaks of enhancements of the electron density. On the dayside surface, 0. 01 Hz and 0. 03-5 Hz magnetohydrodynamic waves are excited by the solar wind protons reflected by the moon through cyclotron resonance.
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Evolution process of solar wind speed
Grant number：17540424 2005.4 - 2007.3
Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C) Grant-in-Aid for Scientific Research (C)
NAKAGAWA Tomoko
Authorship：Principal investigator Grant type：Competitive
(1) By using the linear relationship between the initial speed and the initial acceleration of the limb CMEs, the solar wind speed in the vicinity of the Sun is estimated on the assumption that a dragging force is acting depending on the speed difference between the CMEs and the ambient plasma. The solar wind speed within 20 solar radii estimated from the low-latitude CMEs ranged from 100 to 700 km s^<-1>, while the solar wind speed measured at 1 AU ranged from 300 to 700 km s^<-1>. It suggests that the low-latitude solar wind almost completes accelerating within 20 solar radii, but occasionally additional acceleration is present beyond 20 solar radii.
(2) Magnetohydrodynamic (MHD) waves are thought to play an important role in heating and acceleration of the solar wind. An attempt was made to detect MHD waves in the decametric type-3 solar radio bursts in the frequency range from 15 to 40 MHz. There found 1-3 peaks at around 18, 23, or 31 MHz in the spectra, corresponding to the distance of about 1.3 to 1.7 solar radii from the Sun. It suggests that the effective energy conversion from electron-beam driven Langmuir waves to electromagnetic waves occurs under the enhanced plasma density fluctuations of the compressive MHD waves which are responsible to solar wind acceleration.
(3) A torus-type flux rope model applied to an interplanetary magnetic cloud was tested by the simultaneous magnetic field observations by ACE and NOZOMI spacecraft. On the basis of a single observation by ACE, the magnetic cloud was once fitted to a torus-shaped flux rope model through which the spacecraft passed at the southern tip, however, this study revealed that the spacecraft passed through the southern tip, suggesting that the magnetic rope originating from the northern hemisphere of the Sun crosses the equatorial plane. -
Non-Spiral Interplanetary Magnetic Field and Coronal Mass Ejections
Grant number：14540416 2002.4 - 2004.3
Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C) Grant-in-Aid for Scientific Research (C)
NAKAGAWA Tomoko
Authorship：Principal investigator Grant type：Competitive
The speeds of propagation of CMEs in interplanetary space are less distributed than their initial speeds measured on their departure from the limb of the Sun. Gopalswamy et al.(2000, 2001) presented a linear relationship between initial speeds of limb CMEs and their average acceleration during their travel time in interplanetary space. The linear relationship suggests that some dragging force is acting on CMEs. If similar relationship holds within 20 solar radii from the Sun, it would give information on the initial speed of 'ambient' solar wind in the vicinity of the Sun. The relationship between the initial acceleration and the initial speeds of limb CMEs was examined by using SOHO/LASCO CME Catalogue. For the cases for which correlation coefficient was fairly good (from -0.6 to -I), the 'ambient' solar wind speed within 20 solar radii was estimated to be 150 -570 km/s. It is somewhat slower than but close to the speeds of real solar wind measured in interplanetary space.
Interplanetary counterparts of a halo CME which occurred on April 13, 1999, were observed by NOZOMI and ACE on April 16-18, when the two spacecraft were within 3 degrees in heliocentric longitude and 0.2 AU in heliocentric distance. The interplanetary magnetic fields had filamentary structures with large Bz components, and the Bz component was positive at NOZOMI while negative at ACE. Both magnetic fields were different from a magnetic cloud. It implies that the CME had a number of filamentary structures of magetic field lines with various directions. An interplanetary magnetic field of this kind can be used for detection of candidates of interplanetary counterparts of CMEs. -
Solar source of non-spiral interplanetary magnetic field
Grant number：09640533 1997.4 - 1999.3
Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C) Grant-in-Aid for Scientific Research (C)
NAKAGAWA Tomoko
Authorship：Principal investigator Grant type：Competitive
Non-Parker type interplanetary magnetic field comes from non-static source on the Sun, and is expected as a key that relates solar wind and its solar source. As has been recognized in the Yohkoh soft X-ray images, there are various activities on the photosphere which release ejecta into interplanetary space. It is difficult to identify all the interplanetary counterparts of the ejecta because they can be easily missed by point observation from interplanetary spacecraft. It is more convenient to examine non-spiral magnetic field in interplanetary space and then to investigate their relationship to the solar phenomena.
In this study, non-Parker type interplanetary objects, planar magnetic structures, have been examined by using magnetic field and low-energy particle data obtained by GEOTAIL spacecraft. In a planar magnetic structure, magnetic field vectors are all parallel to a plane that is inclined to the ecliptic plane. Previous study showed that the sources often coincided with expanding ioops from active regions. In order to examine their magnetic connection to the photosphere, angular distribution of low-energy electrons in planar magnetic structures were examined by using Low Energy Particle(LEP) experiment onboard GEOTAIL.Bidirectional electrons characteristic of closed field lines were not found in planar magnetic structures.
Previous studies suggested that the jumps in magnetic field were tangential discontinuities, however, velocity jumps had not been investigated because of lack of high-time resolution observation of the solar wind velocity. In this study, GEOTAIL/LEP data were used to calculate velocity component Vn normal to the plane of the structure and the propagation speed U of the discontinuity surface. It resulted in that the jumps were tangential discontinuities in which the speed U was equal to Vn. -
Interplanetary Planar Magnetic Structures
Grant number：07640591 1995.4 - 1996.3
Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C) Grant-in-Aid for Scientific Research (C)
NAKAGAWA Tomoko
Authorship：Principal investigator Grant type：Competitive
Planar magnetic structures in which interplanetary magnetic field vector takes almost all directions that are parallel to a plane are correlated with EXPANDING ACTIVE REGIONS on the Sun by using Sakigake solar wind data and Yohkoh soft X-ray images of the Sun. During the period from January to July, 1993, we could identify three typical planar magnetic structures with the active region expansions found by Uchida et al. [1992] in the Yohkoh soft X-ray images, from which loop-like structures of active-region corona expand outward repeatedly at speeds of a few to a few tens of km/s even in the absence of any sizable flares. The active region expansions are expected to play an important role in mass loss from the Sun. On the other hand, not all the active regions were observed as planar structures in interplanetary space. In 16 Sakigake observations of solar wind plasma whose solar sources coincided with active regions, 9 had non-spiral magnetic field including planar structures, high ion density or both of them, but the other 7 (44%) exhibited no significant difference from average solar wind with spiral field.
Pressure gradient in the solar wind is examined as a candidate cause of planar magnetic structures. In five of Sakigake planar magnetic structures with no bulk-speed gradient, two were in the regions of pressure gradient but the others were not. Flattened, intertwined flux tubes of high-beta plasma (Crooker et al., 1996) are re-examined to model planar magnetic structures. In order to reproduce a planar magnetic structure, a large number of flux ropes with small helicity are required. Variation of field direction is mainly due to variation of orientation of rope axs, rather than to field rotations in each of ropes. -
太陽風磁場構造の発展過程
Grant number：05740311 1993.4 - 1994.3
文部省 科学研究費補助金 奨励（A) 奨励研究(A)
中川 朋子
Authorship：Principal investigator Grant type：Competitive
本研究の目的は、太陽面磁場構造と太陽風磁場構造をつなぐ重要な手がかりである非平均的な太陽風磁場、とりわけ、太陽磁場の時間発展を反映すると考えられる「太陽風中の平面状磁場構造」について、
1.太陽面上のどの磁場構造に対応付けられるかを、惑星間空間と太陽面の双方の観測から明らかにし、
2.太陽面上に両端を持つ磁力線が惑星間空間に引き出され「平面状磁場構造」として観測される、というモデルを確かめること
であったが、惑星間空間探査機「さきがけ」の磁場観測と太陽観測衛星「ようこう」軟X線望遠鏡観測を用いることによって、平面状磁場構造と光球面近傍の磁力線形状との対応付けに成功した。
対応付けを容易にするため、太陽面の静穏であった1993年1-7月を解析期間とし、この期間中,「さきがけ」によって観測された3つの典型的な平面状磁場構造について、太陽風速データを用いて構造が太陽から放出された日時を求め、その発生源と思われる領域を「ようこう」X線画像を用いて調べた。その結果、平面状磁場構造の発生源は3つとも最近「ようこう」で発見された「活動域膨張」を示している領域に対応することがわかった。「活動域膨張」は、下部コロナで観測される、太陽面上の活動域からループ状の構造が惑星間空間に向かって放出される現象である。活動域の磁場は非常に強いため、惑星間空間まで引き出されることはないという考えがこれまでの主流であったが、本研究によって「活動域膨張」が惑星間空間まで引き出されることが示された。発生源とみられる活動域のうち少なくともひとつはフレアを伴っておらず、近傍にフレアがある場合でも小規模のものしか無いことから、平面状磁場構造の発生は、フレアによらず「活動域膨張」によることがわかる。 -
Investigation of the Geomagnetic Tail by the GEOTAIL Satellite
Grant number：04044168 1992 - 1994
Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research Grant-in-Aid for international Scientific Research Grant-in-Aid for international Scientific Research
NISHIDA Atsuhiro, HOSHINO Masahiro, MACHIDA Shinobu, SAITO Yoshifumi, OBARA Takahiro, NAGAI Tsugunobu, MUKAI Toshifumi, TAKAHASHI Kazue, ARAKI Tooru, HIRAHARA Masafumi, MATSUMOTO Hiroshi, HASEBE Nobuyuki, MAEZAWA Kiyosi, FUJIMOTO Masaki, NAGATA Katsuaki, OKADA Toshimi, KIMURA Iwane, HASHIMOTO Kouzou, DOKE Tadayosi, ACUNA M., NAGANO Isamu, ANDERSON R.r., WILKEN B., WILLIAMS D.j., MOZER F., TROSHICHEV O., ZELENYI L., FELDSTEIN Y., SHIOKAWA Kazuo, NAKAMURA Tadasu, YAMAMOTO Tatsundo, TERASAWA Toshio, KOKUBUN Susumu, NAKAGAWA Tomoko, MATSUOKA Ayako, NAKAMURA Masato, FRANK L.a., HAYAKAWA Hajime, FAIRFIELD D.a., TSURUDA Koichiro
Grant amount：\25000000 （ Direct Cost: \25000000 ）
1. Global structure of the distant tail GEOTAIL observations have confirmed that the magnetotail extends to 200 Re and beyond. It flaps violently north-south as well as east-west with amplitudes comparable to its average radius of about 20 Re, but there is no indication that it is filamentary. Plasma sheet is clearly distinguishable from the lobe or the magnetosheath by high temperature (around 1 keV) and low density (around 0.1/cc). Its magnetic structure and internal convection profile are governed by the north-south polarity of the interplanetary magnetic field.
2. Distant tail under the southward IMF Under the southward IMF,magnetic field lines convect toward the neutral sheet where they are reconnected. The probability that open field lines are reconnected earthward of 150 Re is about 75%. The reconnection rate is the highest at the tail axis and decreases toward the flanks by a factor of 2 to 3.
3. Plasma heating and relaxation at the plasma-sheet lobe boundary At the plasma sheet boundary, the slow-mode shock is formed in the convective flow where the cold ions of the lobe become heated. Very energetic ions flow upstream from the shock. The mixed population of cold and hot particles in this boundary region is a rich source of plasma waves whose non-linear development is seen.
4. Distant tail under northward IMF Under the northward IMF,the open field lines which are presumably produced in the cusp region of the dayside magnetopause sweep across the tail. The convection is parallel to the neutral sheet which is highly twisted in the direction of IMF and has opposite directions (dawn to dusk vs dusk to dawn) on opposite sides of the neutral sheet. The source of the hot plasma in the plasma sheet which is located in the open field lines poses a new problem. -
太陽風磁場の三次元構造
Grant number：02952108 1990.4 - 1992.3
文部省 科学研究費補助金 奨励（学振) 奨励研究(特別研究員)
中川 朋子
Authorship：Principal investigator Grant type：Competitive
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Magnetotail observation at 3000 Earth Radii
Grant type：Competitive
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3-D structure of the solar wind magnetic field
Grant type：Competitive
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Interplanetary planer magnetic structures
Grant type：Competitive
Other
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学都「仙台・宮城」サイエンスマップ～光編～』「シューマン共振」
2019.7
Allotted Class
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解析Ⅱ及び同演習 full-time faculty
2023autumn semester
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環境電磁工学特論 full-time faculty
2023spring semester
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解析Ⅲ
2023spring semester
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解析I full-time faculty
2023spring semester
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解析II及び同演習
2022autumn semester
-
解析III full-time faculty
2022spring semester
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解析I full-time faculty
2022spring semester
Teaching Achievements
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学科数学系教員との連携
Type：Innovation in educational contents or methods (includes course evaluation etc.) 2023.4 - 2024.1
大学で学ぶ科目相互の関連性と有用性を認識させるため、線形代数、数学基礎などの科目の進度に合わせ、他科目の学習内容を活用した授業を行う とともに、数学関係教員および学習支援センター教員とで学生のパフォーマンスを共有
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授業全回における宿題提出と添削
Type：Innovation in educational contents or methods (includes course evaluation etc.) 2023.4 - 2023.7
授業内容理解の確認と、論述の仕方を身に着けさせるための答案の添削 （教員1名では無理なので、上級生を起用しチームで添削作業を行う） 2023年度1年必修解析1では、授業14回に対し14回宿題を出題、13回添削し返却
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manabi相談室との連携
Type：Other achievement about your educational practices (except for the above-mentioned) 2012.4 - 2016.9
解析演習の授業において数学の学力不足の学生の状況を共有、学生に対しmanabi相談室の利用を指示
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宿題の添削と返却
Type：Other achievement about your educational practices (except for the above-mentioned) 2005.4 - 2024.3
復習の習慣を付けるとともに正確な答案の記述方法の指導及び各学生に到達度を伝達するため
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授業前後の豆テストの実施と添削
Type：Other achievement about your educational practices (except for the above-mentioned) 2005.4 - 2024.3
物心両面での授業準備態勢の誘導と理解度チェックのため
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ウェブサイトによる問題解説
Type：Other achievement about your educational practices (except for the above-mentioned) 2005.4 - 2024.3
テイラー展開、ラプラス変換等、パターン化された解法を自学自習出るようなページを作成公開
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自動車学校方式による特別再履修
Type：Other achievement about your educational practices (except for the above-mentioned) 2005.4 - 2011.12
修得すべき内容を項目立てし、再履修者が勉強してきた項目ごとに見極めを行い、全項目見極めで検定を行う
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学生本人が自分の学習態度を考えるような授業アンケートの開発と実施
Type：Other achievement about your educational practices (except for the above-mentioned) 2002.4 - 2023.7
アンケートに答えることを通じて、自分の学習態度を顧みると同時に時自分の成長を感じることができる様な設問を考え、結果をウェブサイト上で公表
Textbooks and Teaching Materials
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初心者用 テイラー展開 解説
2021
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初心者用 たたみこみの解説
2021
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初心者用 オイラーの公式 解説
2021
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初心者用 ラプラス変換の解説
2004
https://www.ice.tohtech.ac.jp/nakagawa/taylorexp/taylor1.htm
Teaching Experience
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Analysis III
2021.4 Institution：Tohoku Institute of Technology
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Analysis I
2020.4 Institution：Tohoku Institute of Technology
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Analysis II and Excercises
2017.9 Institution：Tohoku Institute of Technology
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ANalysisi I and excercises,
2017.4 - 2019.8 Institution：Tohoku Institute of Technology
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解析演習I,II
2012.4 - 2017.3 Institution：東北工業大学
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電磁気学Ⅱ
2010.9 - 2011.3 Institution：東北工業大学
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解析I及び同演習、解析II及び同演習
2008.4 - 2012.3 Institution：東北工業大学
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環境電磁工学特論
2006 Institution：東北工業大学大学院
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Numerical Analysis
2002.9 - 2022.3 Institution：Tohoku Institute of Technology
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解析A,B
2002.4 - 2008.3 Institution：東北工業大学
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コンピュータとプログラミングＩ
2001 Institution：東北工業大学
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環境電磁工学特論
1996.4 - 1999.9 Institution：東北工業大学大学院
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数値解析特論
1995.4 - 2005.9 Institution：東北工業大学大学院
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プログラミングIA,IB
1994.4 - 2001.3 Institution：東北工業大学
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地球惑星科学
1994.4 - 2000.8 Institution：東北工業大学
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コンピューター演習
1994.4 - 1994.9 Institution：東北工業大学
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電気数学I,II
1993.9 - 2001.3 Institution：東北工業大学
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コンピューター基礎
1993.9 - 1995.3 Institution：東北工業大学
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情報通信工学実験III
Institution：東北工業大学
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現代科学総論
Institution：東北工業大学
Academic Activities
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Reviewer of Geophysical Research Letteres,Journal of Geohisical Research International contribution
Role(s)： Peer review
American Geophysical Union 2023.7 - 2024.2
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Session chair of H04 Radio diagnostics of space weather plasma processes International contribution
Role(s)： Panel moderator, session chair, etc.
URSI GASS 2023 （ Sapporo ） 2022.11 - 2023.8
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Session chair of H08 plasma waves around the moon and small bodies
Role(s)： Panel moderator, session chair, etc.
URSI GASS 2021 （ Rome ） 2019.6 - 2021.9