By S. Kalliadasis, C. Ruyer-Quil, B. Scheid, M. G. Velarde
Falling Liquid Films supplies a close assessment of state of the art theoretical, analytical and numerical methodologies, for the research of dissipative wave dynamics and development formation at the floor of a movie falling down a planar susceptible substrate. This prototype is an open-flow hydrodynamic instability, that represents a very good paradigm for the examine of complexity in energetic nonlinear media with power provide, dissipation and dispersion. it's going to even be of use for a extra basic figuring out of particular occasions characterizing the transition to spatio-temporal chaos and weak/dissipative turbulence. specific emphasis is given to low-dimensional approximations for such flows via a hierarchy of modeling ways, together with equations of the boundary-layer kind, averaged formulations in line with weighted residuals ways and long-wave expansions. every time attainable the hyperlink among concept and scan is illustrated, and, as yet another bridge among the 2, the improvement of order-of-magnitude estimates and scaling arguments is used to facilitate the knowledge of easy, underlying physics.
This monograph will entice complex graduate scholars in utilized arithmetic, technology or engineering project examine on interfacial fluid mechanics or learning fluid mechanics as a part of their software. it is going to even be of use to researchers engaged on either utilized, basic theoretical and experimental points of skinny movie flows, in addition to engineers and technologists facing techniques concerning isothermal or heated movies. This monograph is basically self-contained and no history on interfacial fluid mechanics is believed.
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Extra resources for Falling liquid films
27, 58]. We examine this assumption S. 1007/978-1-84882-367-9_2, © Springer-Verlag London Limited 2012 21 22 2 Flow and Heat Transfer: Formulation Fig. 1 Sketch of the geometry for a viscous thin film flowing down an inclined plate forming an angle β with the horizontal direction. The system is unbounded in the x and z directions. h(x, z, t) is the local film thickness, h¯ N is the mean film thickness, typically < 1 mm, and g is gravitational acceleration. The surrounding gas phase is air maintained at temperature and pressure T∞ and p∞ , respectively.
High values of We mean that the viscous forces due to the flow fail to generate pressure capable of deforming the surface. 40b) ST: or expresses the relative importance of the thermocapillary stress induced by the surface tension gradient, γ T /h¯ N for ST or γ TN /h¯ N for HF, to the viscous normal stress generated by gravity at the film surface, μu¯ N /h¯ N = ρg h¯ N sin β. – The free-surface and wall film Biot numbers B= α h¯ N = BihN λ and Bw = αw h¯ N = Biw hN . 41) depend on the Nusselt flat film solution, which is controlled by the flow rate, they vary when the flow rate is varied.
We consider transverse perturbations without any free-surface deformation and we clearly identify the S- and P-modes mentioned earlier. We then proceed to the study of evolution of streamwise perturbations. By performing a small wavenumber expansion for the H-mode also mentioned earlier, we obtain the neutral stability curve and identify the wavenumber corresponding to the maximum growth rate. Subsequently, the energy and vorticity balances associated with the onset and growth of wavy perturbations are studied, elucidating the role played by vorticity, a point not considered by Kapitza in his much simpler approach.