2004
DOI: 10.1016/j.physd.2003.09.048
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Thin liquid films on a slightly inclined heated plate

Abstract: The behavior of a thin liquid film on a uniformly heated substrate is considered. When the substrate is horizontal and the Marangoni number sufficiently large the film breaks up into a periodic array of drops. When the substrate is slightly inclined this drop-like state slides down the substrate. The relation between these states is discussed and their stability properties with respect to longitudinal perturbations are determined. The results shed light on the multiplicity of states accessible to systems of th… Show more

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Cited by 113 publications
(130 citation statements)
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“…Then equation (2.1) is clearly not longer applicable. However, the possible stationary two-dimensional solutions of equation (2.1) with Π = 0 can be determined directly [6] independently of the fact that they cannot be reached from the initial condition of a flat film by integration in time. The stationary solutions consist of a vast family of drop solutions separated by dry regions of different lengths.…”
Section: Thin Film Equationmentioning
confidence: 99%
See 1 more Smart Citation
“…Then equation (2.1) is clearly not longer applicable. However, the possible stationary two-dimensional solutions of equation (2.1) with Π = 0 can be determined directly [6] independently of the fact that they cannot be reached from the initial condition of a flat film by integration in time. The stationary solutions consist of a vast family of drop solutions separated by dry regions of different lengths.…”
Section: Thin Film Equationmentioning
confidence: 99%
“…Oron and Rosenau studied the effects of a quadratic dependence of surface tension on temperature [4] and extended the study towards an inclined substrate [5]. In the latter case the evolution equation looses its variational structure allowing for a richer bifurcation structure, as studied recently in some detail by Thiele and Knobloch [6]. All the mentioned work focused on the structure formation in two spatial dimensions, i.e.…”
Section: Introductionmentioning
confidence: 99%
“…(i) The evolution of thin viscous films in the presence of gravity and thermo-capillary effects is modeled by u t + {u n (u xxx + u m−n u x − Au M−n u x )} x = 0, (1.2) where m, n, M, A are constants such that A 0, n > 0, m < M, as well as the more accurate variant of (1.2) given by u t + {u n (u xxx + h (u)u x )} x = 0, (1.3) where h (u) = −νG + B 1 /(u(1 + B 2 u) 2 ), G, B 1 , B 2 are positive constants, ν = ±1, and where ν = +1 [−1] represents stabilizing [destabilizing] gravitational forces [41,49,42]. Equation (1.2) with A = 0, u t + {u n (u xxx + u m−n u x )} x = 0, models thin films with thermo-capillary effects but without gravitational effects when m − n = −1 [21], or with destabilizing gravitational effects but without capillary effects when m − n = 0.…”
Section: Introductionmentioning
confidence: 99%
“…1 There has been considerable theoretical work focused on thermocapillary instabilities and wave formation in thin liquid films flowing over uniformly heated surfaces. 14,15 While inertial effects are significant in these studies, instabilities also lead to interesting behavior in the lubrication 16,17 and Stokes flow 18 regimes.…”
Section: Introductionmentioning
confidence: 99%