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宇宙線超重核観測計画
https://jaxa.repo.nii.ac.jp/records/13390
https://jaxa.repo.nii.ac.jp/records/133903fc40e69-490e-461c-b264-2902dc7ac243
名前 / ファイル | ライセンス | アクション |
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63706014.pdf (927.9 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
タイトル | 宇宙線超重核観測計画 | |||||
言語 | ||||||
言語 | jpn | |||||
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 | 超重核 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 国際宇宙ステーション | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 天体物理学 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 固体飛跡検出器 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | SSTD | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | エッチピット | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 原子衝突 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 電荷 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 質量 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 衛星装置 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 検出 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 画像解析 | |||||
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 | ultra heavy nucleus | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | International Space Station | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | astrophysics | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | solid-state track detector | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | SSTD | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | etch pit | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | atomic collision | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | electric charge | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | mass | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | satellite instrument | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | detection | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | image analysis | |||||
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 | |||||
その他のタイトル(英) | ||||||
その他のタイトル | Observation program of ultra heavy nuclei in galactic cosmic rays | |||||
著者 |
小平, 聡
× 小平, 聡× 道家, 忠義× 長谷部, 信行× 晴山, 慎× 宮地, 孝× 宮島, 光弘× 桜井, 邦朋× 太田, 周也× 佐藤, 匡× 清水, 雄輝× Kodaira, Satoshi× Doke, Tadayoshi× Hasebe, Nobuyuki× Hareyama, Makoto× Miyachi, Takashi× Miyajima, Mitsuhiro× Sakurai, Kunitomo× Ota, Shuya× Sato, Masashi× Shimizu, Yuki |
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著者所属 | ||||||
早稲田大学 | ||||||
著者所属 | ||||||
早稲田大学 | ||||||
著者所属 | ||||||
早稲田大学 | ||||||
著者所属 | ||||||
早稲田大学 | ||||||
著者所属 | ||||||
早稲田大学 | ||||||
著者所属 | ||||||
早稲田大学 | ||||||
著者所属 | ||||||
早稲田大学 | ||||||
著者所属 | ||||||
早稲田大学 | ||||||
著者所属 | ||||||
早稲田大学 | ||||||
著者所属 | ||||||
早稲田大学 | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University | ||||||
著者所属(英) | ||||||
en | ||||||
Waseda University | ||||||
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 |
宇宙利用シンポジウム 第24回 平成19年度 en : Space Utilization Research: Proceedings of the Twenty-fourth Space Utilization Symposium p. 64-67, 発行日 2008-03 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The origin of Galactic Cosmic Rays (GCRs) nuclei is still unknown. The precise observation of ultra heavy nuclei (Z is greater than or equal to 30) in GCRs is important to resolve the problems remained in cosmic ray astrophysics. Observation program of these nuclei in GCRs is proposed with the use of high performance Solid-State Track Detector (SSTD) on board long-duration balloon or International Space Station (ISS). The program focuses to measure the isotopic abundance above iron-peak elements and the composition of the rare ultra heavy nuclei up to actinide elements with relativistic energy. The observation of their nuclear composition covers a wide range of scientific themes including studies of nucleosynthesis of cosmic ray sources, chemical evolution of galactic material, the characteristic time associated with cosmic rays, such as heating and acceleration mechanism of cosmic ray particles. In order to achieve the objectives, long-duration balloon and/or ISS capable of carrying very large scientific payloads for long extended period is thought as best suited. The possible approach is based on a large telescope array consisting of modularized SSTD stacks. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0063706014 |