WEKO3
アイテム
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Formation Flight All Sky Telescope (FFAST)
https://jaxa.repo.nii.ac.jp/records/11223
https://jaxa.repo.nii.ac.jp/records/11223a986ab8d-c25e-4386-8e93-59f9df01aa70
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 | ||||||
言語 | en | |||||
タイトル | Formation Flight All Sky Telescope (FFAST) | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | X線天文学 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 宇宙機搭載望遠鏡 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 宇宙機搭載天文学 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 編隊飛行 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | ケプラー軌道 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | CCD | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 衛星軌道 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 衛星配置 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 視野 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 低高度地球周回軌道 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | X ray astronomy | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | spaceborne telescope | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | spaceborne astronomy | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | formation flight | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Keplerian orbit | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | CCD | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | satellite orbit | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | satellite constellation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | field of view | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | low Earth orbit | |||||
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 |
常深, 博
× 常深, 博× 鳥居, 研一× 宮田, 恵美× 能町, 正治× 國枝, 秀世× 小賀坂, 康志× 伊藤, 真之× Tsunemi, Hiroshi× Torii, Kenichi× Miyata, Emi× Nomachi, Masaharu× Kunieda, Hideyo× Ogasaka, Yasushi× Ito, Masayuki |
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著者所属 | ||||||
大阪大学 大学院理学研究科 | ||||||
著者所属 | ||||||
大阪大学 大学院理学研究科 | ||||||
著者所属 | ||||||
大阪大学 大学院理学研究科 | ||||||
著者所属 | ||||||
大阪大学 大学院理学研究科 | ||||||
著者所属 | ||||||
名古屋大学 大学院理学研究科 | ||||||
著者所属 | ||||||
名古屋大学 大学院理学研究科 | ||||||
著者所属 | ||||||
神戸大学 発達科学部 | ||||||
著者所属(英) | ||||||
en | ||||||
Osaka University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Osaka University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Osaka University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Osaka University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Nagoya University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Nagoya University Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Kobe University Faculty of Human Development | ||||||
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6回宇宙科学シンポジウム en : Proceedings of the 6th Space Science Symposium p. 344-347, 発行日 2006-01-05 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We propose an all-sky-survey at hard X-ray region (up to 80 keV) by using a formation flight of two satellites. They consist of a telescope satellite, carrying a super mirror focusing at hard X-ray region, and a detector satellite, carrying scintillator deposited CCDs (SDCCDs (Scintillator Deposited Charge Coupled Devices)) for hard X-ray region. These two satellites are in the same orbit (altitude is about 500 km) in formation flight. Since the super mirror will be a thin-foil mirror with poor imaging capability. Therefore, they control the separation of 20 m +/- 10 cm. Both satellites are in Keplerian orbit, then the viewing direction (from the detector satellite to the telescope satellite) scans along a large circle. Due to the precession of the orbit, the large circle gradually moves in the sky so that we can cover a large fraction of the sky. We can cover a large fraction of the sky without consuming a lot of fuel. However, the unseen regions are left near the ecliptic poles. This project, Formation Flight All Sky Telescope (FFAST), will be the first all sky survey at hard X-ray region. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0063353032 |