Thermocapillary effects during the melting of phase-change materials in microgravity: steady and oscillatory flow regimes

被引:41
作者
Salgado Sanchez, P. [1 ]
Ezquerro, J. M. [1 ]
Fernandez, J. [2 ]
Rodriguez, J. [1 ]
机构
[1] Univ Politecn Madrid, E USOC, Ctr Computat Simulat, Dept Aeronaves & Vehiculos Espaciales,Escuela Tec, Plaza Cardenal Cisneros 3, Madrid 28040, Spain
[2] Univ Politecn Madrid, E USOC, Ctr Computat Simulat, Dept Matemat Aplicada Ingn Aerosp,Escuela Tecn Su, Plaza Cardenal Cisneros 3, Madrid 28040, Spain
关键词
Marangoni convection; pattern formation; solidification; melting; MARANGONI NUMBER CONVECTION; HEAT-TRANSFER ENHANCEMENT; ENERGY-STORAGE; RECTANGULAR CAVITY; DESIGN; NEPCM; METAL; PCM;
D O I
10.1017/jfm.2020.852
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
A detailed numerical investigation of thermocapillary effects during the melting of phase-change materials in microgravity is presented. The phase-change transition is analysed for the high-Prandtl-number material n-octadecane, which is enclosed in a two-dimensional rectangular container subjected to isothermal conditions along the lateral walls. The progression of the solid/liquid front during the melting leaves a free surface, where the thermocapillary effect acts driving convection in the liquid phase. The nature of the flow found during the melting depends on the container aspect ratio, Gamma, and on the Marangoni number, Ma. For large Gamma, this flow initially adopts a steady return flow structure characterised by a single large vortex, which splits into a series of smaller vortices to create a steady multicellular structure (SMC) with increasing Ma. At larger values of Ma, this SMC undergoes a transition to oscillatory flow through the appearance of a hydrothermal travelling wave (HTW), characterised by the creation of travelling vortices near the cold boundary. For small Gamma, the thermocapillary flow at small to moderate Ma is characterised by an SMC that develops initially within a thin layer near the free surface. At larger times, the SMC evolves into a large-scale steady vortical structure. With increasing applied Ma, a complex oscillatory mode is observed. This state, referred to as an oscillatory standing wave (OSW), is characterised by the pulsation of the vortical structure. Finally, for an intermediate Gamma both HTWand OSWmodes can be found depending on Ma.
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页数:33
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