The Rayleigh number is simply defined as the product of the Grashof number, which describes the relationship between buoyancy and viscosity within a fluid, and the Prandtl number, which describes the relationship between momentum diffusivity and thermal diffusivity.
Rax = Grx . Pr
The Grashof number is defined as the ratio of the buoyant to a viscous force acting on a fluid in the velocity boundary layer. Its role in natural convection is much like that of the Reynolds number in forced convection. Natural convection occurs if this motion and mixing are caused by density variations resulting from temperature differences within the fluid. Usually, the density decreases due to increased temperature and causes the fluid to rise. This motion is caused by the buoyant force. The major force that resists the motion is the viscous force. The Grashof number is a way to quantify the opposing forces.
The Rayleigh number is used to express heat transfer in natural convection. The magnitude of the Rayleigh number is a good indication of whether the natural convection boundary layer is laminar or turbulent. The simple empirical correlations for the average Nusselt number, Nu, in natural convection are of the form:
Nux = C. Raxn
The values of the constants C and n depend on the geometry of the surface and the flow regime, which is characterized by the range of the Rayleigh number. The value of n is usually n = 1/4 for laminar flow and n = 1/3 for turbulent flow.
The Rayleigh number is defined as:
g is the acceleration due to Earth’s gravity
β is the coefficient of thermal expansion
Twall is the wall temperature
T∞ is the bulk temperature
L is the vertical length
α is the thermal diffusivity
ν is the kinematic viscosity.
For gases β = 1/T where the temperature is in K. For liquids, β can be calculated if the variation of density with the temperature at constant pressure is known. For a vertical flat plate, the flow turns turbulent for the value of:
Rax = Grx . Pr > 109
Example: Rayleigh Number
The property values required for this example are:
ν = 1.48 x 10-5 m2/s
ρ = 1.17 kg/m3
Pr = 0.700
β = 1/ (273 + 20) = 1/293
We know the natural circulation becomes turbulent at approximately Ra = Gr.Pr > 109, which is fulfilled at the following height: