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Shock-wave heating chondrule formation: Generation of shock waves at upper region of solar nebula by X-ray flares and expanding magnetic bubbles
https://jaxa.repo.nii.ac.jp/records/20591
https://jaxa.repo.nii.ac.jp/records/205917ab05560-a14f-4c5e-ab24-f06214b0bb96
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: Generation of shock waves at upper region of solar nebula by X-ray flares and expanding magnetic bubbles | |||||
言語 | ||||||
言語 | eng | |||||
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 | コンドリュール形成 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 模型 | |||||
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 | MHDシミュレーション | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 磁気気泡 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | X線フレア | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 気体密度 | |||||
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 | chondrule formation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | model | |||||
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 | MHD simulation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | magnetic bubble | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | X-ray flare | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | gas density | |||||
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 | 衝撃波加熱コンドリュール形成:X線フレアおよび膨張磁気バブルによる太陽星雲上層部での衝撃波の発成 | |||||
著者 |
中本, 泰史
× 中本, 泰史× 林, 満× 木多, 紀子× 橘, 省吾× Nakamoto, Taishi× Hayashi, Mitsuru R.× Kita, Noriko T.× Tachibana, Shogo |
|||||
著者所属 | ||||||
筑波大学 計算科学研究センター | ||||||
著者所属 | ||||||
国立天文台 | ||||||
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 | ||||||
University of Tsukuba Center for Computational Sciences | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory | ||||||
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37回月・惑星シンポジウム en : Proceedings of the 37th ISAS Lunar and Planetary Symposium p. 49-52, 発行日 2004-02 |
|||||
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, examined are whether the shock waves in the solar nebula are generated by X-ray flares and whether the shock conditions are suitable for chondrule formation. MHD simulations of X-ray flares and subsequent expansion of magnetic bubbles have been conducted, and it was found that shock waves of several tens km/s with velocity could be generated at the upper region of the solar nebula where the gas density is low. Such shock conditions at the upper region of the nebula 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: AA0047898013 |