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Separation of 1699yr and 1866yr radiant points by use of the line detection method
https://jaxa.repo.nii.ac.jp/records/36701
https://jaxa.repo.nii.ac.jp/records/36701674c31e9-ff90-4fcb-92a6-af5e7c2afa4a
名前 / ファイル | ライセンス | アクション |
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SA4638960.pdf (850.1 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 | ||||||
言語 | en | |||||
タイトル | Separation of 1699yr and 1866yr radiant points by use of the line detection method | |||||
言語 | ||||||
言語 | eng | |||||
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 | |||||
著者 |
柳沢, 俊史
× 柳沢, 俊史× 大西, 浩次× 鳥居, 研一× 小浜, 光洋× 中島, 厚× David, ASHER× YANAGISAWA, Toshifumi× OHNISHI, Kouji× TORII, Ken'ichi× KOHAMA, Mitsuhiro× NAKAJIMA, Atsushi× ASHER, David |
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著者所属 | ||||||
航空宇宙技術研究所 | ||||||
著者所属 | ||||||
長野工業高等専門学校 | ||||||
著者所属 | ||||||
理化学研究所 | ||||||
著者所属 | ||||||
理化学研究所 | ||||||
著者所属 | ||||||
航空宇宙技術研究所 | ||||||
著者所属 | ||||||
Arnagh Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
National Aerospace Laboratory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
Nagano National College of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Riken | ||||||
著者所属(英) | ||||||
en | ||||||
Riken | ||||||
著者所属(英) | ||||||
en | ||||||
National Aerospace Laboratory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
Arnagh Observatory | ||||||
出版者 | ||||||
出版者 | 宇宙科学研究所 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science | |||||
書誌情報 |
en : The Institute of Space and Astronautical Science report. S.P. : Proceedings of the 2002 International Science Symposium on the Leonid Meteor Storms 巻 15, p. 39-45, 発行日 2003-03 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We have employed the new line detection method and successfully separated the tworadiant points that correspond to the dust trails of Comet 55P/Tempel-Tuttle's perihelion passagesin 1699 and 1866. This method integrates pixel values of a CCD image along a line direction, whichenables us to detect 30 times fainter meteors than usual detection methods. It can also determinethe angle of the line direction precisely. Radiant points of 2001 Leonids derived by this methodwere found to be consistent with those predicted by McNaught and Asher. | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0288-433X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA10455137 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: SA4638960000 |