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Analysis of short term variation of Jovian synchrotron radiation at a frequency of 327 MHz
https://jaxa.repo.nii.ac.jp/records/20617
https://jaxa.repo.nii.ac.jp/records/2061786fbc020-b649-4a17-906e-6a576cf51b6b
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 | Analysis of short term variation of Jovian synchrotron radiation at a frequency of 327 MHz | |||||
言語 | ||||||
言語 | eng | |||||
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 | シンクロトロン放射 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 木星 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 短期変動 | |||||
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 | JSRフラックス密度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 放射線帯 | |||||
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 | synchrotron radiation | |||||
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 | short term variation | |||||
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 | JSR flux density | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | radiation belt | |||||
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 | 振動数327MHzでの木星シンクロトロン放射の短期変動の解析 | |||||
著者 |
野村, 詩穂
× 野村, 詩穂× 三澤, 浩昭× 土屋, 史紀× 森岡, 昭× Nomura, Shiho× Misawa, Hiroaki× Tsuchiya, Fuminori× Morioka, Akira |
|||||
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(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 | ||||||
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37回月・惑星シンポジウム en : Proceedings of the 37th ISAS Lunar and Planetary Symposium p. 151-154, 発行日 2004-02 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The Jovian synchrotron radiation (JSR) is a radio wave emitted from the relativistic electrons in the Jovian radiation belt, which has information of dynamics of high-energy particles and electromagnetic disturbances in the Jovian inner magnetosphere. The intensity variation of JSR, however, has been little understood in its timescales and origin. Have been observed JSR for several months a year since 1994 to reveal characteristics of the flux variations especially at the time scales of days to months (short-term) and years (long-term). The regular observations have been made at a frequency of 327 MHz by using parabolic cylinder antennas of the Solar Terrestrial Environment Laboratory (STEL), Nagoya University. The observed JSR flux includes apparent variation due to inevitable system gain variation of the radio receiving system. In order to compensate the system gain variation, has been evaluated system gain using a flux reference radio source that was observed quasi-simultaneously with JSR, and have been made observations of actual galactic back-ground radiation (BG) with the highly stable radio receiving system of Tohoku University. In this paper, reported are the results of the JSR observations for 1994 (around the period of the comet Shoemaker-Levy 9 impacts to Jupiter) when the BG flux levels have not been sufficiently quantified in the previous analysis. The JSR flux became nearly twice as large as the flux before the impacts during the observation period. The observation result suggests that rapid and large number flux variation and/or pitch angle scattering occurred even for relatively low energetic electrons in the inner radiation belt. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0047898039 |