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Global and small-scale structure of the zodiacal dust cloud observed with AKARI
https://jaxa.repo.nii.ac.jp/records/3085
https://jaxa.repo.nii.ac.jp/records/30857f1676e8-974c-465d-8684-60f3ce26d508
名前 / ファイル | ライセンス | アクション |
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AA1730026011.pdf (1.3 MB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-05-16 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Global and small-scale structure of the zodiacal dust cloud observed with AKARI | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | zodiacal emission | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | interplanetary dust | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | comets | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | asteroids | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
著者 |
大坪, 貴文
× 大坪, 貴文× Otsubo, Takafumi |
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著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構(JAXA) | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料 en : JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life 巻 JAXA-SP-17-009E, p. 81-87, 発行日 2018-03-09 |
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会議概要(会議名, 開催地, 会期, 主催者等) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京 | |||||
会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The Solar System is filled with interplanetary dust and its thermal emission dominates the diffuse radiation in the mid-to far-infrared wavelength region. After the advent of infrared astronomical satellites, it was found that there are numerous small-scale structures in the zodiacal emission distribution, including dust-band pairs, a circumsolar ring, and cometary trails, in addition to a smooth background distribution. The dust-band pairs are well studied thus far and are now considered to be associated with disruptive events of asteroid families in the main asteroid belt, which would have occurred within the last 10 Myrs. AKARI detects the circumsolar ring and zodiacal dust-band structures at 9, 18, 65 and 90 micrometers bands. Furthermore, in the AKARI far-infrared map, partial young dust-band candidates can be seen, which are corresponding to the possible bands suggested by the IRAS observation. These small-scale structures are important to investigate the recent (less than 1 Myr) evolution of the dust in the Solar System. Here I summarize the current understanding of the zodiacal emission distribution. I will present the results of the AKARI mid- and far-infrared all-sky maps and spectroscopic observations for the global and small-scale structures of the zodiacal dust cloud, and discuss the evolution of the zodiacal dust cloud. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: カラー図版あり | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
ISSNONLINE | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 2433-2232 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA1730026011 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-17-009E |