WEKO3
アイテム
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Development of a dual frequency system for the observation of the Jovian Synchrotron Radiation using the Iitate Planetary Radio Telescope (IPRT)
https://jaxa.repo.nii.ac.jp/records/20472
https://jaxa.repo.nii.ac.jp/records/204728b618eb9-ea4d-4546-bb6f-5a2345d75507
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 | Development of a dual frequency system for the observation of the Jovian Synchrotron Radiation using the Iitate Planetary Radio Telescope (IPRT) | |||||
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 | 電波放射 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽風 | |||||
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 | 粒子加速 | |||||
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 | 電波望遠鏡 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 2重周波数観測 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 感度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | ダイポールアンテナ | |||||
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 | radio emission | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | solar wind | |||||
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 | particle acceleration | |||||
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 | radio telescope | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | dual frequency observation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | sensitivity | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | dipole antenna | |||||
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 | |||||
著者 |
今井, 浩太
× 今井, 浩太× 三澤, 浩昭× 土屋, 史紀× 森岡, 昭× 渡辺, 拓男× 工藤, 理一× Imai, Kota× Misawa, Hiroaki× Tsuchiya, Fuminori× Morioka, Akira× Watanabe, Takuo× Kudo, Riichi |
|||||
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 | ||||||
明星電気 | ||||||
著者所属 | ||||||
NTT先端技術総合研究所 未来ねっと研究所 | ||||||
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 | ||||||
Meisei Electric Co. Ltd. | ||||||
著者所属(英) | ||||||
en | ||||||
NTT Science and Core Technology Laboratory Group Network Innovation Laboratories | ||||||
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39回月・惑星シンポジウム en : Proceedings of the 39th ISAS Lunar and Planetary Symposium p. 37-40, 発行日 2006-08-07 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We have made regular observations of the Jovian Synchrotron Radiation (JSR) with the Iitate Planetary Radio Telescope (IPRT) at 325 MHz since 2003. As a further project of IPRT, we have developed a new dual frequency receiver system which enables simultaneous JSR observations at both 325 MHz and a new frequency of 785 MHz. JSR is generated by relativistic electrons trapped in the Jovian radiation belt. We can obtain more information of the Jovian radiation belt from the dual frequency observations; i.e., dynamical processes of particle acceleration/heating for approximately 12 MeV electrons in addition to approximately 7 MeV electrons from the 785 MHz and 325 MHz observations, respectively. The new receiver system has individual front-end systems for both frequencies consisting of dipole-type feed systems, low noise amplifiers, frequency conversion sections, and a common back-end system. Development of the new 785 MHz receiver system has been almost finished, regular observations at 785 and 325 MHz have been started since June 2006. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0063505010 |