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Layered Marangoni convection with the Navier slip condition

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Abstract

A new exact solution to the problem of Marangoni layered convection is obtained. This solution describes a layered steady-state flow of a viscous incompressible fluid at varying gradients of temperature and pressure. The velocity components depend only on the transverse coordinate; the temperature and pressure fields are three-dimensional. The Marangoni effect is observed on the upper free surface of the fluid layer. On the lower solid surface of the fluid layer, three different cases of defining boundary conditions are considered: the no-slip condition, the perfect slip condition and the Navier slip condition. The obtained exact solution is determined by the interaction of three flows: a flow caused by pressure drop (the Poiseuille flow), a flow caused by heating/cooling and the effect of the gravity force (the thermogravitational flow), and a flow caused by heating/cooling and the fluid surface tension effect (the thermocapillary flow). The obtained exact solutions in the case of each of the three types of boundary conditions specified on the lower surface are analyzed in detail. It has been proved that, when certain ratios of the boundary value problem parameters are fulfilled, the velocity components may acquire stagnation points, this being indicative of the presence of counterflow areas in the fluid layer under consideration. In particular, the presence of up to two stagnation points in each of the two longitudinal velocity components may cause a stratification of the velocity field in more than two regions. The obtained exact solution of the Marangoni layered convection problem can describe flows in thin films through the variation of the geometric anisotropy factor.

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Correspondence to Natalya V Burmasheva.

List of symbols

List of symbols

AB:

values of temperature gradients on upper boundary of fluid layer

g :

acceleration of gravity

\(Ga, \, Gr\) :

Galileo and Grashof dimensionless numbers

h :

thickness of fluid layer

Ma :

Marangoni dimensionless number

P :

pressure, divided by average fluid density

\(P_0, P_1, P_2\) :

components of pressure field

Pr :

Prandtl dimensionless number

Q :

fluid flow rate through the layer thickness

\(S_1, \,S_2\) :

values of pressure gradients on upper boundary of fluid layer

T :

temperature

\(T_0, T_1, T_2\) :

components of temperature field

\(\mathbf {V}\) :

velocity vector

\(V_x, V_y, V_z\) :

projections of velocity vector on coordinate axis

UuV:

components of velocity field

xyz:

Cartesian coordinates

Z :

dimensionless vertical coordinate

\(\alpha \) :

dimensional slip factor (slip length)

\(\beta \) :

temperature coefficient of volume expansion

\(\delta \) :

ratio of the vertical to horizontal characteristic dimension

\(\zeta \) :

ratio of the longitudinal components of the temperature gradients

\(\eta \) :

coefficient of dynamic viscosity

\(\nu \) :

coefficient of kinematic viscosity of the fluid

\(\xi \) :

ratio of the longitudinal components of the pressure gradients

\(\sigma \) :

coefficient of temperature surface tension

\(\tau _{xz}, \tau _{yz}\) :

tangential stresses

\(\chi \) :

coefficient of thermal diffusivity of the fluid

\(\Omega _x, \Omega _y\) :

vorticity components

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Burmasheva, N.V., Privalova, V.V. & Prosviryakov, E.Y. Layered Marangoni convection with the Navier slip condition. Sādhanā 46, 55 (2021). https://doi.org/10.1007/s12046-021-01585-5

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  • DOI: https://doi.org/10.1007/s12046-021-01585-5

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