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タイトルNumerical Simulation of the Effect of Free Surface Shape on Marangoni Convection in a Liquid Film Sustained in a Circular Ring with Different Prandtl Numbers
DOIinfo:doi/10.15011/jasma.33. 330309
著者(日)Adkar, Nikhil; 山本, 卓也; 高木, 洋平; 岡野, 泰則; Dost, Sadik
著者(英)Adkar, Nikhil; Yamamoto, Takuya; Takagi, Youhei; Okano, Yasunori; Dost, Sadik
著者所属(日)大阪大学; 大阪大学; 大阪大学; 大阪大学 : Crystal Growth Laboratory, University of Victoria; Crystal Growth Laboratory, University of Victoria
著者所属(英)Osaka University; Osaka University; Osaka University; Osaka University : Crystal Growth Laboratory, University of Victoria; Crystal Growth Laboratory, University of Victoria
発行日2016-07-31
発行機関などJapan Society of Microgravity Application (JASMA)
日本マイクログラビティ応用学会(JASMA)
刊行物名International Journal of Microgravity Science and Application (IJMSA)
33
3
開始ページ330309-1
終了ページ330309-7
刊行年月日2016-07-31
言語eng
抄録In 2003 NASA astronaut Dr. D. Pettit conducted thermocapillary experiments in a thin water film (Prandtl number; Pr = 7) sustained in a circular ring onboard the International Space Station (ISS). When a section of the ring was heated, a thermocapillary flow developed from the cold region towards the hotter region. This unusual flow phenomenon (being from cold to hot) was explained by the dependency of free surface shape on the flow pattern observed in the film. However, the dependency of flow behavior on the Prandtl number was not investigated previously. Motivated by the wide range of applications of the low-Prandtl-number liquids, numerical simulations for the flow phenomena observed in the films of different shapes and Prandtl numbers were performed under zero gravity. Results have shown that in the case of low-Prandtl-number film although the flow direction remained the same, the flow velocity increased significantly. This interesting phenomenon is explained by means of the temperature gradient in the film in the y- (vertical) and-θ(circumferential) directions.
内容記述Physical characteristics: Original contains color illustrations
形態: カラー図版あり
キーワードThermocapillary flow; Computational fluid dynamics; Low Prandtl number; Marangoni convection
資料種別Journal Article
NASA分類Space Processing
ISSN0915-3616
NCIDAN10537663
SHI-NOAA1640184000
URIhttps://repository.exst.jaxa.jp/dspace/handle/a-is/574426


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