@inproceedings{oai:jaxa.repo.nii.ac.jp:00004715,
 author = {松尾, 裕一 and 阿部, 浩幸 and 吉澤, 徴 and Matsuo, Yuichi and Abe, Hiroyuki and Yoshizawa, Akira},
 book = {宇宙航空研究開発機構特別資料: 第42回流体力学講演会/航空宇宙数値シミュレーション技術シンポジウム2010 論文集, JAXA Special Publication: Proceedings of 42nd Fluid Dynamics Conference / Aerospace Numerical Simulation Symposium 2010},
 month = {Feb},
 note = {第42回流体力学講演会/航空宇宙数値シミュレーション技術シンポジウム2010 (2010年6月24日-25日. 米子コンベンションセンター BiG SHiP), 42nd Fluid Dynamics Conference / Aerospace Numerical Simulation Symposium 2010 (June 24-25,  2010. Yonago Convention Center BiG SHiP), Yonago, Tottori Japan, In this paper, we try to introduce the characteristic time scales intrinsic to turbulent separated flows into the RANS turbulence modeling, and propose a k‐epsilon type model in which the turbulent eddy viscosity is modified by the correction factor based on the time scales. We also show pros and cons of the proposed model by applying it to the separated airfoil flows and the backward facing step flows., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA0064967008, レポート番号: JAXA-SP-10-012},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {航空宇宙の剥離流への時間スケールに着目した乱流モデルの適用},
 volume = {JAXA-SP-10-012},
 year = {2011}
}