WEKO3
アイテム
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The response of the Jovian synchrotron radiation at 325 MHz associated with the strong solar activity during October to November 2003
https://jaxa.repo.nii.ac.jp/records/20621
https://jaxa.repo.nii.ac.jp/records/20621bb0c1e96-17cd-4d0f-81cf-2d938dd955bf
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 | The response of the Jovian synchrotron radiation at 325 MHz associated with the strong solar activity during October to November 2003 | |||||
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 | 太陽活動 | |||||
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 | 相対論的電子 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 飯舘惑星電波望遠鏡 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 放射線帯 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | アンテナ温度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 変動 | |||||
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 | solar activity | |||||
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 | relativistic electron | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Iitate Planetary Radio Telescope | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | radiation belt | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | antenna temperature | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | variation | |||||
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 | 2003年10月から11月の期間の強い太陽活動に関連した325MHzの木星シンクロトロン放射の応答 | |||||
著者 |
土屋, 史紀
× 土屋, 史紀× 三澤, 浩昭× 渡邉, 拓男× 野村, 詩穂× 森岡, 昭× 三好, 由純× 近藤, 哲朗× Tsuchiya, Fuminori× Misawa, Hiroaki× Watanabe, Takuo× Nomura, Shiho× Morioka, Akira× Miyoshi, Yoshizumi× Kondo, Tetsuro |
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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 | ||||||
名古屋大学太陽地球環境研究所 | ||||||
著者所属 | ||||||
情報通信研究機構 | ||||||
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 | ||||||
Solar-Terrestrial Environment Laboratory, Nagoya University | ||||||
著者所属(英) | ||||||
en | ||||||
National Institution of Information and Communications Technology | ||||||
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. 167-170, 発行日 2004-02 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Jovian synchrotron radiations (JSR) which are emitted from relativistic electrons trapped in the Jupiter's radiation belt were observed during a rarely strong solar event occurred on October 28 and 29, 2003. The observation was made by the Iitate Planetary Radio Telescope (IPRT) at Iitate Observatory in Japan during the period from October 16 to November 20 in 2003. Variations of the JSR intensity were compared with the solar F10.7 flux and it was found that the intensity of the JSR showed unusual increase of its magnitude by about 50 percent and the subsequent rapid decrease after the solar event with the decay rate of about 0.3 Jy/day. Comparing with the previous observations of the short term variation of the JSR, an unusual response of Jupiter's radiation belt associated with the rarely strong solar activity is supposed. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0047898043 |