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科学衛星CORSA-bによるX線バースト源のモニター
https://jaxa.repo.nii.ac.jp/records/31765
https://jaxa.repo.nii.ac.jp/records/317655b1ffefe-4062-40ac-a61e-9ba670f25449
名前 / ファイル | ライセンス | アクション |
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SA0124806.pdf (623.2 kB)
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
タイトル | 科学衛星CORSA-bによるX線バースト源のモニター | |||||
言語 | ||||||
言語 | jpn | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
その他のタイトル(英) | ||||||
その他のタイトル | A Wide Field X-ray Burst Monitor Using A Rotating Modulation Collimator System | |||||
著者 |
宮本, 重徳
× 宮本, 重徳× 村上, 敏夫× 西村, 純× 小田, 稔× 小川原, 嘉明× 田原, 譲× MIYAMOTO, S.× MURAKAMI, T.× NISHIMURA, J.× ODA, M.× OGAWARA, Y.× TAWARA, Y. |
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著者所属 | ||||||
大阪大学理学部 | ||||||
著者所属 | ||||||
東京大学宇宙航空研究所 | ||||||
著者所属 | ||||||
東京大学宇宙航空研究所 | ||||||
著者所属 | ||||||
東京大学宇宙航空研究所 | ||||||
著者所属 | ||||||
東京大学宇宙航空研究所 | ||||||
著者所属 | ||||||
東京大学宇宙航空研究所 | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Aeronautical Science University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Aeronautical Science University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Aeronautical Science University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Aeronautical Science University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Aeronautical Science University of Tokyo | ||||||
出版者 | ||||||
出版者 | 東京大学宇宙航空研究所 | |||||
書誌情報 |
東京大学宇宙航空研究所報告 巻 13, 号 3_C, p. 1055-1067, 発行日 1977-10 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | A design of a rotating modulation collimator system which is appropriate to monitoring the occurrence of X-ray bursts in a wide field of the sky is described. Whenever the burst occurs in the field of view, its celestial position is determined to an accuracy of ~0.5° with the coarse collimator system, and when a certain burst source is continually active, the fine colimator system may be pointed to its approximate direction and the source position is determined to an accuracy of ~2 arcminutes which may be adequate to lead to the optical and/or radio identification. This system, which combines the precise determination of the source position with a wide field of view, is suited to a small satellite. A specific design is proposed for a small Japanese satellite CORSA-b which is due early in 1979. | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0563-8100 | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AN00161914 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: SA0124806000 |