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Shock-wave heating chondrule formation: MHD simulation of shockwave propagation inside of the disk
https://jaxa.repo.nii.ac.jp/records/20524
https://jaxa.repo.nii.ac.jp/records/205243debc081-322f-43b3-b966-aad74df56946
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 | Shock-wave heating chondrule formation: MHD simulation of shockwave propagation inside of the disk | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 原始惑星系円盤 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 惑星間塵 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 衝撃波 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 電磁流体力学シミュレーション | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | コンドルール | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 衝撃波加熱 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 衝撃波伝搬 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽星雲 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽フレア | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | おうし座T型星 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 密度分布 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | protoplanetary disk | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | interplanetary dust | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | shock wave | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | magnetohydrodynamic simulation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | chondrule | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | shock-wave heating | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | shock wave propagation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | solar nebula | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | solar flare | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | T Tauri star | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | density distribution | |||||
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 |
林, 満
× 林, 満× 中本, 泰史× 木多, 紀子× 橘, 省吾× Hayashi, Mitsuru R.× Nakamoto, Taishi× Kita, Noriko T.× Tachibana, Shogo |
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著者所属 | ||||||
国立天文台 | ||||||
著者所属 | ||||||
筑波大学 計算科学研究センター | ||||||
著者所属 | ||||||
地質調査所 | ||||||
著者所属 | ||||||
東京大学 大学院理学系研究科 | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tsukuba Center for Computational Sciences | ||||||
著者所属(英) | ||||||
en | ||||||
Geological Survey of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo 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38回月・惑星シンポジウム en : Proceedings of the 38th ISAS Lunar and Planetary Symposium p. 33-36, 発行日 2006-03 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Shock-wave heating model is one of the plausible models for chondrule formation, though the generation of shock waves has not been understood clearly. In this study, we have carried out MHD (MagnetoHydroDynamic) simulations of X-ray flares and subsequent expansion of magnetic bubbles and we examine whether the conditions of the shock waves inside of the solar nebula are suitable for chondrule formation. We found that shock waves of about 15 km/s with velocity could be generated at the upper region of the solar nebula at 3 AU from the central star. Such shock conditions at the upper region of the nebula at 3 AU seem to be appropriate for chondrule formation. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0063350009 |