Method and variables
Ra = Gr × Pr = gβ|ΔT|L3/(να). It can be calculated from known Grashof and Prandtl values, or from gravitational acceleration, thermal expansion, temperature difference, length, kinematic viscosity and thermal diffusivity.
Worked example
With Gr = 3.2 × 109 and Pr = 0.71 for air, Ra is approximately 2.27 × 109.
Important limits
Rayleigh number does not itself determine a heat-transfer coefficient or a universal transition threshold. Enclosure versus external flow, surface orientation, aspect ratio, boundary conditions, radiation and property variation all affect the correlation and interpretation.
References
- NASA Technical Report: Ra = Gr × Pr and natural-convection definitions
- Lawrence Berkeley National Laboratory: Rayleigh-number formulation
Related tools
Grashof Number Calculator · Prandtl Number Calculator · Dimensionless Numbers Calculators
Frequently asked questions
How are Rayleigh, Grashof and Prandtl numbers related?
Rayleigh number is Ra = Gr × Pr. It combines buoyancy-versus-viscosity effects with the ratio of momentum to thermal diffusion.
Does one Rayleigh value always mean convection starts?
No. Critical values depend on the geometry, orientation, boundary conditions and problem definition. Use a source appropriate to the actual configuration.
Which fluid properties should I use?
Use a mutually consistent set of properties at an appropriate reference state, often a film temperature for external natural convection.