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アイテム
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Laboratory simulation of the heliosphere using an MPD device
https://jaxa.repo.nii.ac.jp/records/12760
https://jaxa.repo.nii.ac.jp/records/12760bae459b0-c738-4ed7-8100-61b67e3b1e33
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 | Laboratory simulation of the heliosphere using an MPD device | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | MPD | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | MHD方程式 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽圏 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 磁場配位 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | カレントシート | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 中性シート | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 数値シミュレーション | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 横方向磁場 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 研究開発 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 子午面 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽コロナ | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | MPD | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | MHD equation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | heliosphere | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | magnetic field configuration | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | sun | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | current sheet | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | neutral sheet | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | numerical simulation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | transverse magnetic field | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | research and development | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | meridional plane | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | solar corona | |||||
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 | MPD装置を用いた太陽圏の実験室シミュレーション | |||||
著者 |
南, 繁行
× 南, 繁行× Rizwan, Rana× 森本, 峰行× 武智, 誠次× Podgorny, Alexander× Podgorny, Igor× Minami, Shigeyuki× Rizwan, Rana× Morimoto, Mineyuki× Takechi, Seiji× Podgorny, Alexander× Podgorny, Igor |
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著者所属 | ||||||
大阪市立大学 大学院工学研究科 | ||||||
著者所属 | ||||||
大阪市立大学 大学院工学研究科 | ||||||
著者所属 | ||||||
大阪市立大学 大学院工学研究科 | ||||||
著者所属 | ||||||
大阪市立大学 大学院工学研究科 | ||||||
著者所属 | ||||||
Russian Academy of Sciences Lebedev Institute of Physics | ||||||
著者所属 | ||||||
Russian Academy of Sciences Institute of Astronomy | ||||||
著者所属(英) | ||||||
en | ||||||
Osaka City University Graduate School of Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Osaka City University Graduate School of Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Osaka City University Graduate School of Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Osaka City University Graduate School of Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Russian Academy of Sciences Lebedev Institute of Physics | ||||||
著者所属(英) | ||||||
en | ||||||
Russian Academy of Sciences Institute of Astronomy | ||||||
出版者 | ||||||
出版者 | 宇宙科学研究所 | |||||
出版者(英) | ||||||
出版者 | The Institute of Space and Astronautical Science (ISAS) | |||||
書誌情報 |
スペース・プラズマ研究会 平成14年度 en : Space Plasma Conference FY2002 p. 37-40, 発行日 2003-06 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | A laboratory simulation of the heliosphere has been made to investigate the magnetic field configuration near the sun using an MPD device. The high-speed plasma flow interacts with a transverse magnetic field. The result shows that there exists deformation of the magnetic field due to the current sheet creation in the meridional plane, while there is no neutral sheet as is predicted by Newmann and Kopp [1971]. The result is compared with the numerical simulation of the heliosphere and these are consistent with each other. It is found that the illumination of the streamer corresponds to the current sheet region of the heliosphere. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0045919010 |