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Neutral atom emission coming from the direction of the high-latitude magnetopause under northward IMF
https://doi.org/10.15094/00006417
https://doi.org/10.15094/000064171abcb7e6-bfbd-4a94-9179-1555813cd782
名前 / ファイル | ライセンス | アクション |
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KJ00004322067 (1.4 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 2006-08-01 | |||||
タイトル | ||||||
タイトル | Neutral atom emission coming from the direction of the high-latitude magnetopause under northward IMF | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | cusp | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | neutral atoms | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | reconnection | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | IMF | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ID登録 | ||||||
ID登録 | 10.15094/00006417 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Taguchi, Satoshi
× Taguchi, Satoshi× Hosokawa, Keisuke× Murata, Yozo× Nakao, Akira× Collier, Michael R.× Moore, Thomas E.× Sato, Natsuo× Yukimatu , Akira S. |
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著者所属(英) | ||||||
en | ||||||
Department of Information and Communication Engineering, University of Electro-Communications/Department of Information and Communication Engineering, University of Electro-Communications/Sugadaira Space Radio Observatory, University of Electro-Communications/Department of Information and Communication Engineering, University of Electro-Communications/NASA Goddard Space Flight Center/NASA Goddard Space Flight Center/National Institute of Polar Research/National Institute of Polar Research | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The Low Energy Neutral Atom (LENA) imager on the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft in the magnetosphere can detect neutral particles coming from the direction of the magnetopause. During a period of dynamic pressure of ~6 nPa and IMF B_Z of ~15nT on March 27, 2001, significant neutral atom emissions occurred in the direction of the very high-latitude magnetopause. Simultaneous observations from IMAGE/LENA and SuperDARN radar show that the LENA emission appears concurrently with the enhancement of the sunward flow of the reverse convection in the ionosphere. In a recent paper (S. Taguchi et al., Geophys. Res. Lett., 33, L03101, doi: 10.1029/2005GL025020, 2006) this type of emission has been interpreted as being produced by the fast ion flow caused by cusp reconnection through charge exchange with the Earth's hydrogen exosphere. In other words, remote sensing using LENA imager can be applied in order to determine the stability of the reconnection site. From results of analyses of LENA emission data we show that the reconnection "spot" mapped on a sphere having a radius of 8 R_E shifts tailward by approximately 1 R_E over 10min while fluctuating. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11397422 | |||||
書誌情報 |
Advances in polar upper atmosphere research 巻 20, p. 17-26, 発行日 2006-08 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |