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高マッハ数で伝播する衝撃波背後のCARS法による気体分子振動・回転温度計測
https://jaxa.repo.nii.ac.jp/records/14625
https://jaxa.repo.nii.ac.jp/records/146253e8ead42-3afd-4e76-ac03-27ad8ef8441d
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
タイトル | 高マッハ数で伝播する衝撃波背後のCARS法による気体分子振動・回転温度計測 | |||||
言語 | ||||||
言語 | jpn | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | マッハ数 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 宇宙機再突入 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 空力加熱 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 放射熱伝達 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 衝撃波 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | CARS | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 分子励起 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 振動温度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 回転温度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 分子分光 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Mach number | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | spacecraft reentry | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | aerodynamic heating | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | radiative heat transfer | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | shock wave | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | CARS | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | molecular excitation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | vibrational temperature | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | rotational temperature | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | molecular spectroscopy | |||||
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(英) | ||||||
その他のタイトル | Measurement of vibrational/rotational temperatures of gas molecules behind high Mach number shock waves by CARS spectroscopic system | |||||
著者 |
前野, 一夫
× 前野, 一夫× 豊田, 和弘× 安藤, 広行× 宮崎, 勝巳× Maeno, Kazuo× Toyoda, Kazuhiro× Ando, Hiroyuki× Miyazaki, Katsumi |
|||||
著者所属 | ||||||
千葉大学 工学部 都市環境システム学科 | ||||||
著者所属 | ||||||
千葉大学 工学部 都市環境システム学科 | ||||||
著者所属 | ||||||
千葉大学 大学院自然科学研究科 | ||||||
著者所属 | ||||||
千葉大学 大学院自然科学研究科 | ||||||
著者所属(英) | ||||||
en | ||||||
Chiba University Department of Urban Environment Systems, Faculty of Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Chiba University Department of Urban Environment Systems, Faculty of Engineering | ||||||
著者所属(英) | ||||||
en | ||||||
Chiba University Graduate School of Science and Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Chiba University Graduate School of Science and Technology | ||||||
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 |
宇宙航行の力学シンポジウム 平成16年度 en : Symposium on Flight Mechanics and Astrodynamics 2004 p. 69-73, 発行日 2005-03 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | When a space vehicle reenters onto the atmosphere with high velocity, radiative heating from the shocked air ahead of the vehicle plays an important role on the heat flux to the wall surface as well as convective heating. In the laboratory, the spectroscopic system has been developed for temperature measurement of radiation behind strong shock waves. In this paper, CARS method (Coherent Anti-Stokes Raman Spectroscopy) for radiative flow behind strong shock waves of high Mach number has been developed. The CARS measurement system consists of a YAG laser, a dye laser, optical system, and high-sensitivity I.I.-CCD camera systems with spectroscopy. The preliminary tests have been performed for the purpose of detecting CARS signal from strong shock waves with velocity range over 5 km/s. Finally, both vibrational and rotational temperatures could be estimated by fitting of the CARS spectra obtained from experiment and analytical calculation over Mach 15. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0048089018 |