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S.P. : Proceedings of the 2002 International Science Symposium on the Leonid Meteor Storms", "bibliographic_titleLang": "en"}]}]}, "item_9_description_17": {"attribute_name": "抄録(英)", "attribute_value_mlt": [{"subitem_description": "McNaught and Asher (2001) predicted the precise positions ofradiant points due to the4-rev (1866 yr.) and 9-rev (1699 yr) dust trails of the Leonids. To establish the dust trail theoryand to measure the flux and magnitude distribution of faint meteors, we performed telescopicobservations with the CCD camera, obtaining the high-resolution dust trail structure from thedeep imaging of the radiant point. 7 sites in Japan performed such coordinated observations; (i)Akeno observatory, (ii) RIBOTS at Bisei observatory; (iii) RIMOTS at Miyazaki Univ., (iv) Kisoobservatory, (v) KSC Schmidt, (vi) Miyazaki Univ., (vii) NAOJ Mitaka. We observed the Leonidsmeteor storm Nov.18 2001, and succeeded to separate the radiant points due to the 4-rev and9-rev dust trails. We also succeeded to detect the faint meteors under 10 magnitude. This paperdescribes the detailed observation circumstances and presents a highlight of preliminary results.Mainly, we report the distribution of faint meteors from 7th to 12th magnitude combining the dataof each sites. The cumulative flux of faint meteors is exponential growth with the index numberof 2.0, and the flux (4.2 ± 2.1) x l0-4km-2s-2(mag≦ +12). 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Leonid Radiant Project 2001
https://jaxa.repo.nii.ac.jp/records/36700
https://jaxa.repo.nii.ac.jp/records/36700d3cefad9-a823-4f7a-801e-498ba2eb8791
名前 / ファイル | ライセンス | アクション |
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SA4636317.pdf (1.4 MB)
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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 | Leonid Radiant Project 2001 | |||||
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 |
大西, 浩次
× 大西, 浩次× 柳沢, 俊史× 鳥居, 研一× 小浜, 光洋× 河合, 誠之× 佐藤, 理江× 廿日出, 勇× 茶屋, 道夫× 柴田, 博介× 西浦, 慎悟× 宮田, 隆志× 中田, 好一× 土橋, 一仁× 渡部, 潤一× 縣, 秀彦× 小池, 邦昭× 臼井, 文彦× 石黒, 正晃× 栄楽, 正光× 道上, 達広× 菅原, 章× 高野, 忠× 吉川, 真× 阿部, 新助× David, ASHER× OHNISHI, Kouji× YANAGISAWA, Toshifumi× TORII, Ken-ichi× KOHAMA, Mituhiro× KAWAI, Nobuyuki× SATO, Rie× HATUKADE, Isamu× CHAYA, Mitio× SHIBATA, Hirosuke× NISHIURA, Shingo× MIYATA, Takashi× NAKATA, Yoshikazu× DOBASHI, Kazuhito× WATANABE, Jun-ichi× AGATA, Hidehiko× KOIKE, Kuniaki× USUI, Fumihiko× ISHIGURO, Masateru× EIRAKU, Masamitu× MITUKAMI, Tatuhiro× SUGAWARA, Akira× TAKANO, Tadasi× YOSHIKAWA, Makoto× ABE, Shinsuke× ASHER, David |
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長野工業高等専門学校 | ||||||
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航空宇宙技術研究所 | ||||||
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理化学研究所 | ||||||
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理化学研究所 | ||||||
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東京工業大学 | ||||||
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東京工業大学 | ||||||
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宮崎大学 | ||||||
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宮崎大学 | ||||||
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宮崎大学 | ||||||
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東京大学 | ||||||
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東京大学 | ||||||
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東京大学 | ||||||
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東京学芸大学 | ||||||
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国立天文台 | ||||||
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国立天文台 | ||||||
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東京理科大学 | ||||||
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長野工業高等専門学校 | ||||||
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長野工業高等専門学校 | ||||||
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長野工業高等専門学校 | ||||||
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長野工業高等専門学校 | ||||||
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長野工業高等専門学校 | ||||||
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長野工業高等専門学校 | ||||||
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長野工業高等専門学校 | ||||||
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長野工業高等専門学校 | ||||||
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国立天文台 | ||||||
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Nagano National College of Technology | ||||||
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National Aerospace Laboratory of Japan | ||||||
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RIKEN | ||||||
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RIKEN | ||||||
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Tokyo Institute of Technology | ||||||
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Tokyo Institute of Technology | ||||||
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Miyazaki University | ||||||
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Miyazaki University | ||||||
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Miyazaki University | ||||||
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Kiso observatory, Institute of Astronomy, University of Tokyo | ||||||
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Kiso observatory, Institute of Astronomy, University of Tokyo | ||||||
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Kiso observatory, Institute of Astronomy, University of Tokyo | ||||||
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Tokyo Gakugei University | ||||||
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National Astronomical Observatory | ||||||
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National Astronomical Observatory | ||||||
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Tokyo Science University | ||||||
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Nagano National College of Technology | ||||||
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Nagano National College of Technology | ||||||
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Nagano National College of Technology | ||||||
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Nagano National College of Technology | ||||||
著者所属(英) | ||||||
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Nagano National College of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Nagano National College of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Nagano National College of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Nagano National College of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical 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. 29-38, 発行日 2003-03 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | McNaught and Asher (2001) predicted the precise positions ofradiant points due to the4-rev (1866 yr.) and 9-rev (1699 yr) dust trails of the Leonids. To establish the dust trail theoryand to measure the flux and magnitude distribution of faint meteors, we performed telescopicobservations with the CCD camera, obtaining the high-resolution dust trail structure from thedeep imaging of the radiant point. 7 sites in Japan performed such coordinated observations; (i)Akeno observatory, (ii) RIBOTS at Bisei observatory; (iii) RIMOTS at Miyazaki Univ., (iv) Kisoobservatory, (v) KSC Schmidt, (vi) Miyazaki Univ., (vii) NAOJ Mitaka. We observed the Leonidsmeteor storm Nov.18 2001, and succeeded to separate the radiant points due to the 4-rev and9-rev dust trails. We also succeeded to detect the faint meteors under 10 magnitude. This paperdescribes the detailed observation circumstances and presents a highlight of preliminary results.Mainly, we report the distribution of faint meteors from 7th to 12th magnitude combining the dataof each sites. The cumulative flux of faint meteors is exponential growth with the index numberof 2.0, and the flux (4.2 ± 2.1) x l0-4km-2s-2(mag≦ +12). We have found no apparent cutoff inthe magnitude range brighter than ~12 mag. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 著者人数: 25名 | |||||
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: SA4636317000 |