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High-resolution simulation of propagation of interplanetary shock wave caused by a coronal mass ejection observed on November 13, 2003
https://doi.org/10.15094/00006403
https://doi.org/10.15094/0000640364ad9a73-6edb-4505-9506-50be9b288139
名前 / ファイル | ライセンス | アクション |
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KJ00003387690 (1.7 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 2005-08-01 | |||||
タイトル | ||||||
タイトル | High-resolution simulation of propagation of interplanetary shock wave caused by a coronal mass ejection observed on November 13, 2003 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | coronal mass ejection | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | interplanetary shock wave | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | three-dimensional simulation | |||||
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 | 10.15094/00006403 | |||||
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) |
Ogawa, Yasunobu
× Ogawa, Yasunobu× Den, Mitsue× Tanaka, Takashi× Yamashita, Kazuyuki |
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著者所属(英) | ||||||
en | ||||||
Space Simulation Group, National Institute of Information and Communications Technology/Space Simulation Group, National Institute of Information and Communications Technology/Department of Earth and Planetary Sciences, Kyushu University/The Center for Educational Research, University of Yamanashi | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We simulated the three-dimensional (3D) propagation of a shock wave caused by a coronal mass ejection (CME) on November 13, 2003. The 3D simulations were performed using a high-resolution adaptive mesh refinement (AMR) technique. The AMR technique enabled us to resolve near the sun with (0.06R_◎)^3-sized cells and to resolve the entire shock front with (0.24R_◎)^3-sized cells in an interplanetary simulation within a (500R_◎)^3-sized computational box. The solar wind was measured by an imaginary spacecraft positioned at point L1 in the simulations. A model fitted for solar wind density fluctuations observed by the ACE spacecraft was employed, and models in which some CME parameters were changed were employed for comparison. The relationships between the CME parameters and the solar wind fluctuations were also investigated, and the results were compared with the solar wind data observed at point L1 by the ACE spacecraft. | |||||
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 19, p. 71-79, 発行日 2005-08 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |