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宇宙ダスト生成過程の解明に向けた気相からの均質核形成のその場観察実験
https://jaxa.repo.nii.ac.jp/records/13079
https://jaxa.repo.nii.ac.jp/records/13079c6a40d09-5c1c-4636-adc4-4a8fb4976e94
名前 / ファイル | ライセンス | アクション |
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65129019.pdf (332.4 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
タイトル | 宇宙ダスト生成過程の解明に向けた気相からの均質核形成のその場観察実験 | |||||
言語 | ||||||
言語 | jpn | |||||
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 | |||||
その他のタイトル(英) | ||||||
その他のタイトル | In-situ observation of dust formation via homogeneous nucleation in vapor phase | |||||
著者 |
木村, 勇気
× 木村, 勇気× 田中, 今日子× 三浦, 均× 塚本, 勝男× 稲富, 裕光× Kimura, Yuki× Tanaka, Kyoko× Miura, Hitoshi× Tsukamoto, Katsuo× Inatomi, Yuko |
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著者所属 | ||||||
東北大学 | ||||||
著者所属 | ||||||
北海道大学 | ||||||
著者所属 | ||||||
東北大学 | ||||||
著者所属 | ||||||
東北大学 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構 (JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University | ||||||
著者所属(英) | ||||||
en | ||||||
Hokkaido University | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency (JAXA) | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | |||||
書誌情報 |
宇宙利用シンポジウム: 第27回: 平成22年度 en : Space Utilization Research, Vol. 27 2011: Proceedings of The Twenty-seventh Space Utilization Symposium 巻 27, p. 47-50, 発行日 2011-03 |
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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27回宇宙利用シンポジウム (2011年1月24日-25日, 宇宙航空研究開発機構宇宙科学研究所相模原キャンパス), 相模原市, 神奈川県 | |||||
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 Twenty-seventh Space Utilization Symposium (January 24-25, 2011. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | To know the formation process of cosmic dust particles, we attempted for the first time interferometric observation to a condensation experiment in vapor phase, the gas evaporation method. Homogeneous nucleation is a fundamental process of dust formation in universe. For the first step, temperature distribution around evaporation source was measured with respect to the source temperature in the gas evaporation method for the first time in a quarter century. We visualized a condensation of smoke particles in gas phase and temperature history including a cooling rate of produced particles after nucleation was recognized. Homogeneously condensed WO3 nuclei initially maintain their temperature for ca.5 ms and then cool down with a rate of ca.5×10(exp 4) K/s. The degree of supersaturation during the nucleation was at least as high as 10(exp 7). | |||||
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 | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AN10324210 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0065129019 |