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Library / Dimensional analysis and similarity / DIM-10

Dimensional analysis and similarity

Rayleigh number

Buoyancy driving relative to the combined damping of momentum and heat diffusion.

Ref
DIM-10
Rev
v1
Field
Dimensional analysis and similarity
Result
Ra

Ra = gβΔT L³/(να) combines buoyancy with both diffusive effects that resist it, momentum diffusion (ν) and heat diffusion (α). It equals the Grashof number times the Prandtl number, Pr = ν/α. Convection starts only when Ra exceeds a threshold that depends on the geometry, orientation and boundary conditions; for a thin horizontal layer between rigid plates heated from below it is about 1708, based on the layer depth. On a vertical plate, the boundary layer typically turns turbulent near Ra ≈ 10⁹.

Buoyancy driving relative to the combined damping of momentum and heat diffusion. It is the Grashof number times the Prandtl number, and decides whether natural convection starts and what regime it is in.

Calculator

Solve for
m/s²
130
10⁻³/K
0.0120
K
0.1500
m
0.00110
mm²/s
0.11,000
mm²/s
0.011,000
  • Prandtl number, ν/α0.75
  • Grashof number, Ra/Pr1,308,000
  • Ra with the length doubled7,848,000
  • Ra divided by the layer-onset value 1708574.4

What drives the result

Each variable is moved across its typical range while the others stay at the values above. The longest bar is the key driver.

Rayleigh number () current value 981,000
LCharacteristic lengthKey driver
0.9819.81e11
αThermal diffusivity
19,6001.96e9
νKinematic viscosity
14,7001.47e8
ΔTTemperature difference (magnitude)
9,8104.91e7
βVolumetric thermal expansion coefficient
3,2706,540,000
gGravitational acceleration
100,0003,000,000
  • For these conditions Ra = 981,000, well below the 10⁹ at which a vertical-plate boundary layer typically turns turbulent, so the flow is laminar.
  • Nusselt-number correlations for natural convection are written in Ra (and sometimes Pr), so this is usually the step before finding the heat-transfer coefficient h = Nu k/L.
Chart data as tables

Ranked variables

VariableTypical rangeLowest resultHighest resultSwing ()Local stepChange in result
L Characteristic length0.001 to 10 m0.9819.81e119.81e11+10%+33.1 %
α Thermal diffusivity0.01 to 1,000 mm²/s19,6201.962e91.962e9+10%−9.09 %
ν Kinematic viscosity0.1 to 1,000 mm²/s14,7201.472e81.471e8+10%−9.09 %
ΔT Temperature difference (magnitude)0.1 to 500 K9,8104.905e74.904e7+10%+10 %
β Volumetric thermal expansion coefficient0.01 to 20 10⁻³/K3,2706,540,0006,537,000+10%+10 %
g Gravitational acceleration1 to 30 m/s²100,0003,000,0002,900,000+10%+10 %

Sweep of Temperature difference (magnitude)

Temperature difference (magnitude) (K)Rayleigh number
0.19,810
0.2928,450
0.840982,490
2.438239,200
7.071693,700
20.52,012,000
59.465,833,000
172.41.691e7
5004.905e7

Sweep one variable

Rayleigh number ()Hover, touch, or use the arrow keys on the chart
010M20M30M40M50M 0.1110100 Temperature difference (magnitude) (K), log scale now 981,000

Variables and how each one contributes

Ra

Rayleigh number

Result ·

What the equation gives you. Everything else feeds it.

g

Gravitational acceleration

m/s² · typical 1 to 30

The gravitational acceleration, in m/s² (9.81 on Earth). Raises the Rayleigh number in direct proportion. Raising it by 10 % (to 10.79) moves the result by +10 %, from 981,000 to 1,079,000.

β

Volumetric thermal expansion coefficient

10⁻³/K · typical 0.01 to 20

The volumetric thermal expansion coefficient, in units of 10⁻³ per K: about 3.4 for air at room temperature and about 0.2 for water. Raises the Rayleigh number in direct proportion. Raising it by 10 % (to 3.3) moves the result by +10 %, from 981,000 to 1,079,000.

ΔT

Temperature difference (magnitude)

K · typical 0.1 to 500

The magnitude of the temperature difference across the fluid, in K. Raises the Rayleigh number in direct proportion. Raising it by 10 % (to 11) moves the result by +10 %, from 981,000 to 1,079,000.

L

Characteristic length

m · typical 0.001 to 10

The characteristic length, in m: the layer depth for a heated layer, or the height of a vertical surface. Raises the Rayleigh number with the cube of the length, so size is the strongest lever. Raising it by 10 % (to 0.11) moves the result by +33.1 %, from 981,000 to 1,306,000.

ν

Kinematic viscosity

mm²/s · typical 0.1 to 1,000

The kinematic viscosity, in mm²/s (air about 15, water about 1). Lowers the Rayleigh number in inverse proportion. Raising it by 10 % (to 16.5) moves the result by −9.09 %, from 981,000 to 891,800.

α

Thermal diffusivity

mm²/s · typical 0.01 to 1,000

The thermal diffusivity, in mm²/s (air about 20, water about 0.14). Lowers the Rayleigh number in inverse proportion. Raising it by 10 % (to 22) moves the result by −9.09 %, from 981,000 to 891,800.

Worked example with the values above

  1. Numerator: gβΔT L³ = 9.81 × 0.003 × 10 × 0.1³ = 2.943×10−4.
  2. Denominator: να = 1.5×10−5 × 2×10−5 = 3×10−10 m⁴/s².
  3. Ra = 981,000, which is Gr × Pr = 1,308,000 × 0.75.

Assumptions and limits

  • Natural convection with a small fractional density variation (the Boussinesq approximation).
  • The threshold for convection depends on the geometry and boundary conditions, and L is defined as in the correlation used.

Common mistakes

  • Using the Rayleigh number without the Prandtl number correction where a correlation needs Pr as well.
  • Mixing α and ν in different units.
  • Applying the 1708 onset value to a vertical surface or to different boundary conditions.

Statistics and uncertainty

The result is a product of powers, so to first order its relative error is the root sum of squares of each input’s relative error multiplied by its exponent (g × 1, β × 1, ΔT × 1, L × 3, ν × −1, α × −1). Length (cubed) dominates, and the fluid properties change with temperature, so evaluate them at the film temperature.

Where it is used

  • Predicting whether a heated fluid layer will start to convect, and in which regime.
  • Finding the natural-convection heat-transfer coefficient from a Nusselt correlation in Ra.

Maths you need

  • Prandtl number: ratio of momentum to thermal diffusivity
  • Thermal diffusivity: thermal conductivity over density times specific heat

Related formulas

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