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Leonids Radiant Project 2001 in Japan
https://shinshu.repo.nii.ac.jp/records/3384
https://shinshu.repo.nii.ac.jp/records/3384e978d5a6-7628-49a8-a829-b66800688fd7
名前 / ファイル | ライセンス | アクション |
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https://nagano-nct.repo.nii.ac.jp/?action=repository_action_common_download&item_id=110&item_no=1&attribute_id=22&file_no=1
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Item type | Departmental Bulletin Paper(1) | |||||
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公開日 | 2018-04-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Leonids Radiant Project 2001 in Japan | |||||
その他(別言語等)のタイトル | ||||||
その他のタイトル | Leonids Radiant Project 2001 in Japan | |||||
作成者(その他言語) |
OHNISHI, Kouji
× OHNISHI, Kouji |
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公開者(その他言語) | ||||||
姓名 | 長野工業高等専門学校 | |||||
書誌情報 |
長野工業高等専門学校紀要 en : Memoirs of Nagano National College of Technology 巻 38, p. 79-86, 発行日 2004-06-30 |
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言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Leonids 2001 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | mass index | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | flux | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Ham-band Radio Observation (HRO) | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | beam antenna | |||||
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 | |||||
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 | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | McNaught and Asher (2001) predicted the precise positions of radiant points due to the 4-rev (1866 yr.) and 9-rev (1699 yr) dust trails of the Leonids. To establish the dust trail theory and to measure the flux and magnitude distribution of very faint meteors, we performed deep imaging telescopic observations with the cooled CCD camera toward the radiant points of the Leonids. 7 sites in Japan performed such coordinated observations; (i) Akeno Observatory, Institute for Cosmic Ray Research University of Tokyo, (ii) RIBOTS at Bisei Observatory, (iii) RIMOTS at Miyazaki Univ., (iv) Kiso Observatory, Institute of Astronomy, The University of Tokyo, (v) KSC Schmidt, Uchinoura Space Center, Institute of Space and Astronautical Science, (vi) Miyazaki Univ., (vii) NAOJ Mitaka. We observed the Leonids meteor storm Nov.18 UT 2001, and succeeded to separate the radiant points due to the 4-rev and 9-rev dust trails (Yanagisawa et al. 2003, Torii et al. 2003). We also succeeded to detect the faint meteors under 10 magnitudes (Ohnishi et al. 2003). This paper describes the detailed observation circumstances and a highlight of preliminary results. | |||||
日付 | ||||||
日付 | 2012-05-31 | |||||
日付タイプ | Created | |||||
フォーマット | ||||||
内容記述タイプ | Other | |||||
内容記述 | application/pdf | |||||
資源識別子URI | ||||||
識別子 | http://id.nii.ac.jp/1051/00000107/ | |||||
識別子タイプ | URI | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0286-1909 | |||||
処理レコードID(総合目録DB) | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AN00179170 | |||||
権利 | ||||||
権利情報 | CC BY-NC-ND | |||||
著者版フラグ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 |