| Item type |
紀要論文 / Departmental Bulletin Paper(1) |
| 公開日 |
2015-03-26 |
| タイトル |
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タイトル |
Observation of a faint glow of scattered sunlight from the dust trail of the Leonid parent comet 55P / Tempel-Tuttle |
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言語 |
en |
| 言語 |
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言語 |
eng |
| 資源タイプ |
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資源タイプ識別子 |
http://purl.org/coar/resource_type/c_6501 |
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資源タイプ |
departmental bulletin paper |
| 著者 |
臼井, 文彦
石黒, 正晃
Fumihiko, USUI
Masateru, ISHIGURO
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| 著者所属 |
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東京大学 |
| 著者所属 |
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宇宙科学研究所 固体惑星科学研究系 |
| 著者所属（英） |
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en |
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Department of Earth Science and Astronomy, Graduate School of Arts and Scieces, University of Tokyo |
| 著者所属（英） |
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en |
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Planetary Science Division, The Institute of Space and Astronautical Science |
| 出版者 |
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出版者 |
宇宙科学研究所 |
| 出版者（英） |
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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. 23-27,
発行日 2003-03
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| 抄録（英） |
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内容記述タイプ |
Other |
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内容記述 |
The faint glow at the direction of the dust trail of comet 55P/Tempel-Tuttlewas discovered during the Leonid meteor shower in 1998 (ΔMA = 0.136) by the photometricobservations at Mauna Kea, Hawaii (Nakamura et al. (2000)). This is considered as the scatteredsunlight by the sub-millimeter size dust particles located along the orbit of 55P/Tempel-Tuttle.To examine the orbital distribution of the dust particles, we observed the direction of the dusttrail on 2001 November 19 (ΔMA = O.705), at Akeno Observatory (138d30m(E), 35d47m(N),900m, Institute for Cosmic Ray Research, University of Tokyo, Japan) . The instruments were thesame one as Nakarnura et al. (2000) used. From our data, there is no prominent evidence detectedat that direction. Based on these two data obtained in 1998 and 2001, we discuss the spatialdistribution of the dust material observed as the dust tube in visible wavelength. |
| ISSN |
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収録物識別子タイプ |
ISSN |
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収録物識別子 |
0288-433X |
| 書誌レコードID |
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収録物識別子タイプ |
NCID |
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収録物識別子 |
AA10455137 |
| 資料番号 |
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内容記述タイプ |
Other |
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内容記述 |
資料番号: SA4636314000 |
SA4636314.pdf (366.6 kB)
