WEKO3
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Selective production of soot with 216.5-224.5 nm sharp absorption feature and correlation with graphitic structure
https://jaxa.repo.nii.ac.jp/records/20715
https://jaxa.repo.nii.ac.jp/records/207154b8235c3-df5f-47ad-b7ba-c3a2cb68f7bb
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Selective production of soot with 216.5-224.5 nm sharp absorption feature and correlation with graphitic structure | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | すす | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 惑星間吸収 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | グラファイト構造 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 生成温度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 赤外線吸収 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 天体物理学 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | メタン | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | TEM | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | soot | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | interstellar absorption | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | graphitic structure | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | production temperature | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | ultraviolet absorption | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | astrophysics | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | methane | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | TEM | |||||
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 | |||||
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 | |||||
その他のタイトル | ||||||
その他のタイトル | 216.5〜224.5nmのシャープな吸収特徴を持つすすの選択的生成およびグラファイト構造との相関 | |||||
著者 |
木村, 勇気
× 木村, 勇気× 佐藤, 岳志× 墻内, 千尋× Kimura, Yuki× Sato, Takeshi× Kaito, Chihiro |
|||||
著者所属 | ||||||
立命館大学 理工学部 物理科学科 | ||||||
著者所属 | ||||||
立命館大学 理工学部 物理科学科 | ||||||
著者所属 | ||||||
立命館大学 理工学部 物理科学科 | ||||||
著者所属(英) | ||||||
en | ||||||
Ritsumeikan University Department of Physical Sciences, Faculty of Science and Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Ritsumeikan University Department of Physical Sciences, Faculty of Science and Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Ritsumeikan University Department of Physical Sciences, Faculty of Science and Engineering | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究本部 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS) | |||||
書誌情報 |
第36回月・惑星シンポジウム en : Proceedings of the 36th ISAS Lunar and Planetary Symposium p. 258-261, 発行日 2003-11 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The origin of the strong interstellar 217.5 nm absorption feature appearing in the interstellar extinction curve is a long-standing problem in astrophysics. In the present study, by a simple method, soot with sharp absorption features around 220 nm was produced from methane gas. Interestingly, it was found that the absorption peak positions of the present soot can be controlled by the production temperature. Analyzed results of soot by high-resolution electron microscope clarified that the origin of the absorption peak at 217.5 nm was a graphitic structure with a diameter of 5 nm order. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0046650066 |