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The source and acceleration of cosmic rays as viewed from the nature of the interstellar dust grains
https://jaxa.repo.nii.ac.jp/records/20607
https://jaxa.repo.nii.ac.jp/records/20607e6bfaa93-e598-427a-a581-57a0409e57ff
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 | The source and acceleration of cosmic rays as viewed from the nature of the interstellar dust grains | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 銀河宇宙線 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 加速 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 恒星間塵粒子 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 凝縮温度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 化学組成 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 隕石 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 核合成 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 天体物理学 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galactic cosmic ray | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | acceleration | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | interstellar dust grain | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | condensation temperature | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | chemical composition | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | meteorite | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | nucleosynthesis | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | astrophysics | |||||
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 | 星間塵粒の特性から見た宇宙線の線源と加速 | |||||
著者 |
晴山, 慎
× 晴山, 慎× 長谷部, 信行× 小平, 聡× 櫻井, 邦朋× Hareyama, Makoto× Hasebe, Nobuyuki× Kodaira, Satoshi× Sakurai, Kunitomo |
|||||
著者所属 | ||||||
早稲田大学 理工学総合研究センター | ||||||
著者所属 | ||||||
早稲田大学 理工学総合研究センター | ||||||
著者所属 | ||||||
早稲田大学 理工学総合研究センター | ||||||
著者所属 | ||||||
早稲田大学 理工学総合研究センター | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University Advanced Research Institute for Science and Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University Advanced Research Institute for Science and Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University Advanced Research Institute for Science and Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University Advanced Research Institute for Science and Engineering | ||||||
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. 111-114, 発行日 2004-02 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | A possible mechanism for the formation of the source composition of cosmic rays is proposed by taking into account the condensation process occurring in the interstellar space. This process may have produced the overabundance of heavy and ultra heavy nuclei in the source composition as compared with the chemical composition of the sun. Since the chemical composition of galactic cosmic ray source is similar to that of meteorite as classified as C2, that of galactic cosmic rays was compared with that of silicon carbide of presolar grains. It is found that both the iron isotope ratios and chemical composition of ultra heavy cosmic rays are similar to those in presolar grains. The chemical composition of presolar grains and meteorites may give a clue to search for the birth place of cosmic rays in the interstellar space. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0047898029 |