2005
DOI: 10.1016/j.fluiddyn.2005.03.003
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Numerical study of a thin liquid film on a disk under non-uniform rotation—thermocapillary effects

Abstract: The axisymmetric flow of a viscous heat conducting uniform liquid film on a rotating disk is considered and the governing equations are solved numerically. The model described highlights the effects of thermocapillary force and the effects of different spin-up protocols on the rate of thinning of the film on a rotating disk.

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Cited by 6 publications
(1 citation statement)
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“…3 At higher Reynolds numbers, thin film stability influences the heat and mass transfer characteristics, thereby controlling the performance of falling film and spinning disc reactors, condensers, and reboilers. [4][5][6][7] Studies of thin film stability have examined the dynamics of single-and two-layer flows accounting for a wide variety of effects; these range from capillarity and thermocapillarity, [8][9][10][11][12] surface activity, [13][14][15][16][17] non-Newtonian rheology, [18][19][20][21] and those associated with intermolecular forces [22][23][24][25][26][27] to gravitational, 7,28-34 centrifugal, [35][36][37][38] electrostatic, and electrokinetic [39][40][41] forcing. These studies have successfully elucidated the mechanisms underlying phenomena such as rupture, dewetting, fingering, and wave formation (and even transition to chaos 42,43 ) and their dependence on the relevant system parameters.…”
Section: Introductionmentioning
confidence: 99%
“…3 At higher Reynolds numbers, thin film stability influences the heat and mass transfer characteristics, thereby controlling the performance of falling film and spinning disc reactors, condensers, and reboilers. [4][5][6][7] Studies of thin film stability have examined the dynamics of single-and two-layer flows accounting for a wide variety of effects; these range from capillarity and thermocapillarity, [8][9][10][11][12] surface activity, [13][14][15][16][17] non-Newtonian rheology, [18][19][20][21] and those associated with intermolecular forces [22][23][24][25][26][27] to gravitational, 7,28-34 centrifugal, [35][36][37][38] electrostatic, and electrokinetic [39][40][41] forcing. These studies have successfully elucidated the mechanisms underlying phenomena such as rupture, dewetting, fingering, and wave formation (and even transition to chaos 42,43 ) and their dependence on the relevant system parameters.…”
Section: Introductionmentioning
confidence: 99%