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contributor authorHiroshi Kawamura
contributor authorKoichi Nishino
contributor authorSatoshi Matsumoto
contributor authorIchiro Ueno
date accessioned2017-05-09T00:52:24Z
date available2017-05-09T00:52:24Z
date copyrightMarch, 2012
date issued2012
identifier issn0022-1481
identifier otherJHTRAO-27935#031005_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/149511
description abstractThis paper reports some important results obtained from a series of microgravity experiments on the Marangoni convection that takes place in liquid bridges. This project, called Marangoni Experiment in Space (MEIS), started from August 22, 2008 as the first science experiment on the Japanese Experimental Module “KIBO” at the ISS. Two series of experiments, MEIS-1 and 2, were conducted in 2008 and 2009, respectively. The experimental methods used are explained in some detail. The maximum size of the liquid bridge that could be realized during these experiments was 30 mm in diameter and 60 mm in length, giving an aspect ratio of 2.0. The results are obtained for a wide range of aspect ratios of the liquid bridges, including the values that cannot be reached in 1 g experiments, and therefore, they provide indispensable amount of data for the study of instability mechanisms of the Marangoni convection.
publisherThe American Society of Mechanical Engineers (ASME)
titleReport on Microgravity Experiments of Marangoni Convection Aboard International Space Station
typeJournal Paper
journal volume134
journal issue3
journal titleJournal of Heat Transfer
identifier doi10.1115/1.4005145
journal fristpage31005
identifier eissn1528-8943
keywordsOscillations
keywordsFlow (Dynamics)
keywordsTemperature
keywordsFluids
keywordsConvection
keywordsParticulate matter AND Disks
treeJournal of Heat Transfer:;2012:;volume( 134 ):;issue: 003
contenttypeFulltext


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