WEKO3
アイテム
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Investigation of the Jovian inner magnetosphere by spectrum observation of synchrotron radiation
https://jaxa.repo.nii.ac.jp/records/20707
https://jaxa.repo.nii.ac.jp/records/20707524e727c-d903-43af-8ef7-d065b1a3b434
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Investigation of the Jovian inner magnetosphere by spectrum observation of synchrotron radiation | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 木星 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | シンクロトロン放射 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | スペクトル観測 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 相対論的電子 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | エネルギー依存性 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 惑星磁気圏 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 内部放射帯 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 予備調査 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Jupiter | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | synchrotron radiation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | spectrum observation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | relativistic electron | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | energy dependence | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | planetary magnetosphere | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | inner radiation belt | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | feasibility study | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
その他のタイトル | ||||||
その他のタイトル | シンクロトロン放射のスペクトル観測による木星内部磁気圏の研究 | |||||
著者 |
三澤, 浩昭
× 三澤, 浩昭× 土屋, 史紀× 三好, 由純× 野澤, 宏大× 森岡, 昭× 渡邊, 拓男× 野村, 詩穂× 近藤, 哲朗× Misawa, Hiroaki× Tsuchiya, Fuminori× Miyoshi, Yoshizumi× Nozawa, Hiromasa× Morioka, Akira× Watanabe, Takuo× Nomura, Shiho× Kondo, Tetsuro |
|||||
著者所属 | ||||||
東北大学 大学院理学研究科 | ||||||
著者所属 | ||||||
東北大学 大学院理学研究科 | ||||||
著者所属 | ||||||
東北大学 大学院理学研究科 | ||||||
著者所属 | ||||||
東北大学 大学院理学研究科 | ||||||
著者所属 | ||||||
東北大学 大学院理学研究科 | ||||||
著者所属 | ||||||
東北大学 大学院理学研究科 | ||||||
著者所属 | ||||||
東北大学 大学院理学研究科 | ||||||
著者所属 | ||||||
通信総合研究所 鹿島宇宙通信研究センター | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Communications Research Laboratory Kashima Space Research Center | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究本部 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS) | |||||
書誌情報 |
第36回月・惑星シンポジウム en : Proceedings of the 36th ISAS Lunar and Planetary Symposium p. 226-229, 発行日 2003-11 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | A program of a multi-frequency observation for Jupiter's synchrotron radiation (JSR) is under planning in order to investigate dynamics of Jupiter's inner radiation belt, such as variations of particle flux, pitch angle distribution and radial diffusion of the relativistic electrons. In this program three observation frequencies measured with different facilities are adopted; i.e., 325 MHz at Tohoku University, Japan, 929 MHz at the European Incoherent Scatter Facility (EISCAT), Scandinavia and 2,250 MHz at Communications Research Laboratory (CRL), Japan. As for the 325 MHz observation, the Tohoku University system has just started a regular JSR observation since 2003. Two week sequential observations for JSR were successfully made at 2,250 MHz in both 1996 and 1997. At 929 MHz, a 10 day sequential observation for JSR was made in the autumn of 2002, and the method of JSR observation which was suitable for the EISCAT system was confirmed. Now the observation and data reduction methods have been already established for all frequencies. A coordinated JSR observation is going to be arranged as a sequential and simultaneous observation at the three frequencies in October, 2003 with the period of more than two weeks. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0046650058 |