The onset of convection induced by transient heat conduction in deep fluid is examined for two boundary conditions, namely: fixed surface temperature (FST) and linear rate of change of surface temperature with respect to time (LTR). Transient Rayleigh numbers (Ra) for these boundary conditions are d
On convection driven by surface tension caused by transient heat conduction
โ Scribed by Ka Kheng Tan; Rex B. Thorpe
- Publisher
- Elsevier Science
- Year
- 1999
- Tongue
- English
- Weight
- 128 KB
- Volume
- 54
- Category
- Article
- ISSN
- 0009-2509
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โฆ Synopsis
The onset of convection caused by surface tension (ST) during transient cooling of a thin layer of liquid is investigated. This study shows that it can be predicted by a newly defined transient Marangoni number Ma, which incorporates the mode and rate of cooling, where a non-linear temperature profile develops continuously until instability sets in. The spatio-temporal development of local hydrodynamic equilibrium can thus be traced to the point of instability. The onset of convection for evaporative-cooling can be predicted from the maximum transient Ma whose values are the same as those previously obtained by linear stability analysis for Biot number"0. The critical times and critical depths for stable heat conduction in liquids (before convection) can thus be determined accurately. Agreement with observed values from the literature is very good. The critical transient Marangoni numbers and the sizes of convection cells have also been predicted with reasonable accuracy. A theoretical limiting depth that demarcates between surface tension and buoyancy controlled convection is proposed. There exists theoretical and laboratory evidence to support that surface tension dominates in fluid depth less than 5 mm and buoyancy predominates over 10 mm.
๐ SIMILAR VOLUMES
A theory of formation of transient thermals or plumes generated by unsteady-state heat conduction is proposed. Rising or falling mushroom-shaped plumes formed during transient heating or cooling, respectively, originate from the extending thermal boundary layers. The sizes of the hemispherical caps