Author:
Stannarius Ralf,Trittel Torsten,Klopp Christoph,Eremin Alexey,Harth Kirsten,Clark Noel A,Park Cheol S,Maclennan Joseph E
Abstract
Abstract
Freely suspended smectic films with in-plane temperature inhomogeneities can exhibit remarkable thermocapillary (Marangoni) effects. The temperature dependence of the surface tension
σ
(
T
)
promotes flow in the film plane, convection roll patterns, and climbing of smectic layers against gravitational forces. We discuss several experimental geometries where macroscopic material transport is driven by temperature gradients, including experiments under normal gravity and observations in microgravitation during suborbital rocket flights and on the International Space Station. In all these experiments, the temperature dependence of the surface tension drives unidirectional material flow. The divergence of this flow near the hot and cold film edges, and at the boundaries of film islands in the film, is associated with the creation, motion and removal of dislocations. These dissipative processes limit the flow velocity.
Funder
NSF
Deutsches Zentrum für Luft- und Raumfahrt
Deutsche Forschungsgemeinschaft
NASA
Subject
General Physics and Astronomy
Cited by
7 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献