Titlebook: Microgravity Fluid Mechanics; IUTAM Symposium Brem Hans Josef Rath Conference proceedings 1992 Springer-Verlag Berlin Heidelberg 1992 Mater

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书目名称Microgravity Fluid Mechanics影响因子(影响力)




书目名称Microgravity Fluid Mechanics影响因子(影响力)学科排名




书目名称Microgravity Fluid Mechanics网络公开度




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书目名称Microgravity Fluid Mechanics被引频次




书目名称Microgravity Fluid Mechanics被引频次学科排名




书目名称Microgravity Fluid Mechanics年度引用




书目名称Microgravity Fluid Mechanics年度引用学科排名




书目名称Microgravity Fluid Mechanics读者反馈




书目名称Microgravity Fluid Mechanics读者反馈学科排名

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Brochure

Liquid Bridge Ocsillations: Analytical and Numerical Resultsvitational and surface tension forces means that liquid bridges have limited stability on earth. This has lead to interest in the application of processes involving liquid bridge in a micro-gravity environment such as can be achieved in space, see Walter [1]. However, processes in spacecraft are pro

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Viscosity Effects on the Dynamics of Long Axisymmetric Liquid Bridgesoblem has been solved by using an one-dimensional model known in the literature as the Cosserat model, which includes viscosity effects, where the axial velocity is considered constant in each section of the liquid bridge. The dynamic response of the bridge to an excitation consisting of a small amp

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NEEDY

Marangoni Convection in a Non-Spherical Liquid Dropion of the liquid drop. Assuming small deformation this has been neglected in former investigations and the free surface conditions have been satisfied at the surface of the sphere which is also a coordinate surface in spherical coordinates. In the analysis, presented here, the deviation from spheri

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Some Problems Raised by Marangoni Instability in Spherical Geometryby two concentric spherical surfaces: the inner one is rigid and uniformly heated while the outer is free: it exchanges heat with the external environment and is submitted to a temperature-dependent surface tension. In a first stage, the spherical support is assumed at rest and the outer surface is

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Pander

Stationary Marangoni Instability in a Liquid Layer due to Non-Isothermal Gas Absorptionis studied. As the effects of fluid density are negligibly small at reduced gravity, the mass transfer process can be influenced by a thermal interfacial convection. The analysis shows that the stationary convection sets on not only when the wall temperature is higher than that of the gas (according

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Three-Dimensional Transient Simulation of Marangoni Flow in a Cylindrical Enclosure under Various Gr isothermal top and bottom walls is studied numerically for various gravity levels. The three-dimensional transient code employs a hybrid finite difference scheme on a staggered grid with explicit time steps and an iterative pressure-velocity coupling. In zero-gravity an axisymmetric toroidal flow p