WEKO3
アイテム
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Source of high energy electrons in Saturn's outer magnetosphere
https://jaxa.repo.nii.ac.jp/records/20474
https://jaxa.repo.nii.ac.jp/records/20474898965cb-efa3-439c-870c-21472773b4c6
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 | Source of high energy electrons in Saturn's outer magnetosphere | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 土星 | |||||
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 | タイタン | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | オーロラ | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 高エネルギー電子 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 電子加速 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 惑星磁場 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 速度分布 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Cassiniミッション | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Saturn | |||||
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 | Titan | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | aurora | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | high energy electron | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | electron acceleration | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | planetary magnetic field | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | velocity distribution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Cassini mission | |||||
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 |
河原木, 皓
× 河原木, 皓× 森岡, 昭× 三澤, 浩昭× 土屋, 史紀× Kawaragi, Ko× Morioka, Akira× Misawa, Hiroaki× Tsuchiya, Fuminori |
|||||
著者所属 | ||||||
東京大学 大学院新領域創成科学研究科 | ||||||
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 | ||||||
University of Tokyo Graduate School of Frontier Sciences | ||||||
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39回月・惑星シンポジウム en : Proceedings of the 39th ISAS Lunar and Planetary Symposium p. 45-48, 発行日 2006-08-07 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Saturn's outer magnetosphere is considered to be one of sources of auroral particles, inducing the complex interaction between magnetospheric particles and Titan. In 1980s, Voyager 1 and 2 had revealed the existence of high energy (approximately keV) electrons with non-Maxwellian distribution in this region, although the source of these electrons has not been clear. We investigated the possibility that the source of high energy electrons is resulted by the electron acceleration accompanied by aurora in the polar region. Then we analyzed the electron flux and radio wave data observed by Cassini spacecraft. Analyzed results showed correspondence between emission power of SKR (Saturn Kilometric Radiation), index of auroral activity, and magnetospheric electron flux. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0063505012 |