Principle
of Rayleigh-Benard instability
Mathematical
theory : determination of the critical Rayleigh number
Manifestations
of Rayleigh-Benard instability
Principle of Rayleigh-Benard instability
This problem of Rayleigh-Benard instability is a problem of convection inside a fluid.
This instability occurs inside a fluid confined between
two infinite horizontal planes at different temperatures
and
.
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If
then the system is stable and stays stratified in
temperature. But, if
and if a perturbation is introduced in the system, then
for a critical value of the difference of temperature (
) it can
appear movements inside the fluid : the system is unstable and movements are
organized in periodic contrarotative rolls. These rolls, or also called cells of
Rayleigh-Benard, appear when there is a coupling between the dynamic field and
the thermal field.
Rolls of Rayleigh-Benard
The principle of the instability is simple. Consider a drop of fluid near the lower plane. The drop is heated so its density decreases and it goes up inside the fluid due to the Archimede force. When the drop reaches the upper plane, more cold, it is cooled so its density increases and it can goes down inside the fluid. Rolls of Rayleigh-Benard instability are caused by this mechanism.
The Archimede force must surpass the viscous drag force and the heat diffusion to allow convection inside the fluid. So there is a notion of threshold.
Effectively, this instability occurs following the value
of the Rayleigh number which is:

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| Enthalpie field for Ra=1468 | Enthalpie field for Ra=4405 |
The critical value of the Rayleigh number for apparition
of Rayleigh-Benard instability is 1707. For this critical value we can observe 2
rolls inside the fluid. This state of the fluid with two rolls is the most
stable. But if initial conditions are well chosen, if Rayleigh number increases,
number of rolls inside the fluid increases too.
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To study this problem, we have to solve classic equations of continuity, motion and heat conduction.
For this problem, Boussinesq approximation is used and we have following equations for incompressible fluid:






The velocity limit conditions are
for z=0 and z=d. For temperature we can take constant temperatures or
constant gradients of temperature for z=0 and z=d.
The equations become, in thermal adimensionnal form (
,
and
), and for the 2D case:




Velocity limit conditions become :
for z=0 and z=1.
Determination of the critical Rayleigh number :
The fonction
is
introduced :
and
. The
problem become after linearisation :


If we look for solutions with the following form
, the
system of equations gives :
Limit conditions for z=0 and z=1 are :
By solving this sytem we can find the value of critical Rayleigh number et critical value of k :
Graphic of stability
Note:
We have studied the case where there are two planes under
and above the fluid. Then, velocity limit conditions are two rigid conditions
:
for
z=0 and z=d.
Two others cases exist following the type of boundary. Fluid can be placed on a heated plane but its upper face can be a free surface.
Case where there is one free surface
In this case we have a rigid condition for the lower
boundary
(
for z=0 ) and a free condition for the upper boundary (
and w=0 for
z=d) . So critical values to see instability change :
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The last case is the case where the fluid is confined
between two free surfaces :
and w=0 for z=0
and z=d .
Case where there is two free surfaces
The critical values are now :
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| Rayleigh-Benard instability visualization | 3D Rayleigh-Benard instability |
This phenomenon of Rayleigh-Benard instability is very
important in the industrial domain. Examples are numerous : cooling of nuclear
plants, heating of building, exchanges between atmosphere and oceans..... But
manifestations of Rayleigh-Benard instability are not always visible to our eyes
that's why we have not a lot of pictures of it.