@inproceedings{oai:jaxa.repo.nii.ac.jp:00013150,
 author = {西野, 耕一 and 河村, 洋 and 大西, 充 and 上野, 一郎 and 松本, 聡 and 鈴木, 諒 and 川添, 彰 and 佐々木, 公祐 and 依田, 眞一 and 田中, 哲夫 and Nishino, Koichi and Kawamura, Hiroshi and Onishi, Mitsuru and Ueno, Ichiro and Matsumoto, Satoshi and Suzuki, Ryo and Kawazoe, Akira and Sasaki, Kimihiro and Yoda, Shinichi and Tanaka, Tetsuo},
 book = {宇宙利用シンポジウム, Space Utilization Research: Proceedings of Space Utilization Symposium},
 month = {Feb},
 note = {第26回宇宙利用シンポジウム(2010年1月25日-26日, 宇宙航空研究開発機構宇宙科学研究本部相模原キャンパス), The Twenty-sixth Space Utilization Symposium (January 25-26, 2010: ISAS/JAXA Sagamihara, Japan), Marangoni convection experiments have been carried out in the period from July 30 to August 25, 2009. This is the second series of Marangoni Experiment in Space (MEIS2), the first one (MEIS1) being carried out in the period from August 22 to December 16, 2008. MEIS2 aims at (1) determining critical temperature difference, deltaTcr, for the onset of oscillatory flow for Ar up to 2.0, where Ar is the aspect ratio of the liquid bridge, (2) revealing three-dimensional flow fields in oscillatory state and (3) clarifying the characteristics of surface velocity. In this presentation, some preliminary, but important results from MEIS2 are given together with the results from MEIS1., 形態: カラー図版あり, 共催: 日本学術会議, Physical characteristics: Original contains color illustrations, joint hosting: The Science Council of Japan, 資料番号: AA0064730003},
 publisher = {宇宙航空研究開発機構宇宙科学研究本部, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)},
 title = {「きぼう」における表面張力流の宇宙実験},
 volume = {26},
 year = {2010}
}