Английская Википедия:Boussinesq approximation (buoyancy)
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In fluid dynamics, the Boussinesq approximation (Шаблон:IPA-fr, named for Joseph Valentin Boussinesq) is used in the field of buoyancy-driven flow (also known as natural convection). It ignores density differences except where they appear in terms multiplied by Шаблон:Mvar, the acceleration due to gravity. The essence of the Boussinesq approximation is that the difference in inertia is negligible but gravity is sufficiently strong to make the specific weight appreciably different between the two fluids. Sound waves are impossible/neglected when the Boussinesq approximation is used since sound waves move via density variations.
Boussinesq flows are common in nature (such as atmospheric fronts, oceanic circulation, katabatic winds), industry (dense gas dispersion, fume cupboard ventilation), and the built environment (natural ventilation, central heating). The approximation is extremely accurate for many such flows, and makes the mathematics and physics simpler.
The approximation
The Boussinesq approximation is applied to problems where the fluid varies in temperature (or composition) from one place to another, driving a flow of fluid and heat transfer (or mass transfer[1]). The fluid satisfies conservation of mass, conservation of momentum and conservation of energy. In the Boussinesq approximation, variations in fluid properties other than density Шаблон:Mvar are ignored, and density only appears when it is multiplied by Шаблон:Mvar, the gravitational acceleration.[2]Шаблон:Rp If Шаблон:Math is the local velocity of a parcel of fluid, the continuity equation for conservation of mass is[2]Шаблон:Rp
- <math> \frac{\partial\rho}{\partial t} + \nabla\cdot\left(\rho\mathbf{u}\right) = 0.</math>
If density variations are ignored, this reduces to[2]Шаблон:Rp Шаблон:NumBlk
The general expression for conservation of momentum of an incompressible, Newtonian fluid (the Navier–Stokes equations) is
- <math>\frac{\partial \mathbf{u}}{\partial t} + \left( \mathbf{u}\cdot\nabla \right) \mathbf{u} = -\frac{1}{\rho}\nabla p + \nu\nabla^2 \mathbf{u} + \frac{1}{\rho}\mathbf{F},</math>
where Шаблон:Mvar (nu) is the kinematic viscosity and Шаблон:Math is the sum of any body forces such as gravity.[2]Шаблон:Rp In this equation, density variations are assumed to have a fixed part and another part that has a linear dependence on temperature:
- <math>\rho = \rho_0 - \alpha\rho_0(T-T_0),</math>
where Шаблон:Mvar is the coefficient of thermal expansion.[2]Шаблон:Rp The Boussinesq approximation states that the density variation is only important in the buoyancy term.
If <math>F = \rho \mathbf{g}</math> is the gravitational body force, the resulting conservation equation is[2]Шаблон:Rp
Шаблон:NumBlk{\partial t} + \left( \mathbf{u}\cdot\nabla \right) \mathbf{u} = -\frac{1}{\rho_0}\nabla (p-\rho_0\mathbf{g}\cdot\mathbf{z}) + \nu\nabla^2 \mathbf{u} - \mathbf{g}\alpha(T-T_0).</math>|Шаблон:EquationRef}}
In the equation for heat flow in a temperature gradient, the heat capacity per unit volume, <math>\rho C_p</math>, is assumed constant and the dissipation term is ignored. The resulting equation is
where Шаблон:Mvar is the rate per unit volume of internal heat production and <math>k</math> is the thermal conductivity.[2]Шаблон:Rp
The three numbered equations are the basic convection equations in the Boussinesq approximation.
Advantages
The advantage of the approximation arises because when considering a flow of, say, warm and cold water of density Шаблон:Math and Шаблон:Math one needs only to consider a single density Шаблон:Mvar: the difference Шаблон:Math is negligible. Dimensional analysis showsШаблон:Clarify that, under these circumstances, the only sensible way that acceleration due to gravity Шаблон:Mvar should enter into the equations of motion is in the reduced gravity Шаблон:Mvar where
- <math>g' = g\frac{\rho_1-\rho_2}{\rho}.</math>
(Note that the denominator may be either density without affecting the result because the change would be of order Шаблон:Tmath.) The most generally used dimensionless number would be the Richardson number and Rayleigh number.
The mathematics of the flow is therefore simpler because the density ratio Шаблон:Math, a dimensionless number, does not affect the flow; the Boussinesq approximation states that it may be assumed to be exactly one.
Inversions
One feature of Boussinesq flows is that they look the same when viewed upside-down, provided that the identities of the fluids are reversed. The Boussinesq approximation is inaccurate when the dimensionless density difference Шаблон:Math is approximately 1, i.e. Шаблон:Math.
For example, consider an open window in a warm room. The warm air inside is less dense than the cold air outside, which flows into the room and down towards the floor. Now imagine the opposite: a cold room exposed to warm outside air. Here the air flowing in moves up toward the ceiling. If the flow is Boussinesq (and the room is otherwise symmetrical), then viewing the cold room upside down is exactly the same as viewing the warm room right-way-round. This is because the only way density enters the problem is via the reduced gravity Шаблон:Mvar which undergoes only a sign change when changing from the warm room flow to the cold room flow.
An example of a non-Boussinesq flow is bubbles rising in water. The behaviour of air bubbles rising in water is very different from the behaviour of water falling in air: in the former case rising bubbles tend to form hemispherical shells, while water falling in air splits into raindrops (at small length scales surface tension enters the problem and confuses the issue).
References
Further reading