## What is Rayleigh Number

The **Rayleigh number** is a dimensionless number, named after Lord Rayleigh. The **Rayleigh number** is closely related to Grashof number and both numbers are used to decribe natural convection (Gr) and heat transfer by natural convection (Ra). 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.

**Ra _{x} = Gr_{x} . Pr**

The **Grashof number** is defined as the ratio of the buoyant to viscous force acting on a fluid in the velocity boundary layer. Its role in natural convection is much the same as that of the Reynolds number in forced convection. Natural convection occurs if this motion and mixing is caused by density variations resulting from temperature differences within the fluid. Usually the density decreases due to an increase in 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 as to 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:

**Nu _{x} = C. Ra_{x}^{n}**

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:

where:

g is acceleration due to Earth’s gravity

β is the coefficient of thermal expansion

T_{wall} is the wall temperature

T_{∞} is the bulk temperature

L is the vertical length

α is 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 variation of density with temperature at constant pressure is known. For a vertical flat plate, the flow turns turbulent for value of:

**Ra _{x} = Gr_{x} . Pr > 10^{9} **

As in forced convection the microspic nature of flow and convection correlations are distinctly different in the laminar and turbulent regions.

**Example: Rayleigh Number **

A vertical plate is maintained at 50°C in 20°C air. Determine the height at which the boundary layer will turn turbulent if turbulence sets in at Ra = Gr.Pr = 10^{9}.

Solution:

The property values required for this example are:

ν = 1.48 x 10^{-5} m^{2}/s

ρ = 1.17 kg/m^{3}

Pr = 0.700

β = 1/ (273 + 20) = 1/293

We know the natural circulation becomes turbulent at approximately Ra = Gr.Pr > 10^{9}, which is fulfilled at the following height:

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