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MHD パラシュート効果による超軌道再突入環境下の空力加熱低減の可能性
https://jaxa.repo.nii.ac.jp/records/3840
https://jaxa.repo.nii.ac.jp/records/3840fd0bd9a7-3669-4fb5-a4e5-057efccba87d
名前 / ファイル | ライセンス | アクション |
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AA1530023005.pdf (9.0 MB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-04-28 | |||||
タイトル | ||||||
タイトル | MHD パラシュート効果による超軌道再突入環境下の空力加熱低減の可能性 | |||||
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 | Possibility of Reduction in Aerodynamic Heating by MHD Parachute Effect in Super Orbital Reenty Flights | |||||
著者 |
下澤, 雄太
× 下澤, 雄太× 益田, 克己× 藤野, 貴康× Shimosawa, Yuta× Masuda, Katsumi× Fujino, Takayasu |
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著者所属 | ||||||
筑波大学 | ||||||
著者所属 | ||||||
筑波大学 | ||||||
著者所属 | ||||||
筑波大学 | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tsukuba | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tsukuba | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tsukuba | ||||||
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: 第46回流体力学講演会/第32回航空宇宙数値シミュレーション技術シンポジウム論文集 en : JAXA Special Publication: Proceedings of the 46th Fluid Dynamics Conference / 32nd Aerospace Numerical Simulation Symposium 巻 JAXA-SP-14-010, p. 23-28, 発行日 2015-03-25 |
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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46回流体力学講演会/第32回航空宇宙数値シミュレーション技術シンポジウム (2014年7月3日-4日. 弘前文化センター), 弘前市, 青森県 | |||||
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 | 46th Fluid Dynamics Conference / 32nd Aerospace Numerical Simulation Symposium (July 3-4, 2014. Hirosaki Bunka Center), Hirosaki, Aomori, Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The MHD flow control in super orbital reentry flight is numerically analyzed with taking MHD parachute effect and radiative heating into account. We conducted a coupled numerical simulation of MHD flow and flight trajectories of a reentry body, where the initial altitude and velocity are set to 75 km and 12.4 km/s, respectively. The initial flight path angle is also set to 5 degree. In the simulation, the strength of magnetic field is varied parametrically in a range of 0 to 1.0 T. The numerical results show that the MHD flow control in super orbital reentry flight can mitigate the total heat flux, which is defined as the sum of the convective and radiative heat flux, owing to a decrease in flight velocity by MHD parachute effect. In order to reduce a peak amount of the total heat flux at stagnation point, the use of weak magnetic fields such as 0.25 T is desirable because increase in radiative heat flux by MHD flow control at high altitudes can be suppressed. In order to reduce a time integration of wall heat from 75 km to 45 km, however, strong magnetic fields such as 1.0 T should be use because convective and radiative wall heat load can be mitigated due to a decrease in flight velocity by strong MHD parachute effect. | |||||
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 | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1349-113X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11984031 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA1530023005 | |||||
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-14-010 |