Dimensionless numbers

Calculate 27 dimensionless numbers and see what each value means for your CFD set-up.

Method: White (2016); Incropera et al. (2007) · Reviewed by Christoffer Johansson, M.Sc. · Updated October 2026

Common in CFD
SI units

Reynolds number

Reynolds number Re

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How to use the dimensionless numbers calculator

1. Pick a number. The numbers are grouped by what they describe: flow regime, forces and losses, heat transfer, multiphase flow and particles, mass transfer, and waves and combustion.

2. Enter your values. Each field shows its unit; use SI units throughout. The defaults are a worked example, for instance water flowing at 1 m/s through a pipe of 1 m diameter for the Reynolds number.

3. Read the result and what it means. The note under the value gives the regime, for example laminar or turbulent pipe flow, or whether a lumped thermal model is valid. Copy the value with four significant figures.

Tip: the names in the definitions table below open each number directly in the calculator.

Why dimensionless numbers matter

A dimensionless number is a ratio of two effects, such as inertia and viscosity, in which all units cancel. Two flows with the same dimensionless numbers behave the same way whatever their size. This is dynamic similarity, and it is why a scale model in a wind tunnel can predict the flow around a full-size car.

The Buckingham π theorem tells you how many independent groups a problem has: the number of variables minus the number of base units. Pipe flow described by ρ, U, D and μ has four variables and three units (mass, length, time), so it has one group: the Reynolds number.

In CFD the same numbers decide which physics you switch on and which mesh and time step you need. The next section lists the checks to make before you set up a case.

Which numbers matter in a CFD set-up

Check these numbers before you choose the models in Simcenter STAR-CCM+ or any other solver:

NumberCheck againstWhat it changes in the set-up
Reynolds ReAbout 2300 in a pipe, 5 × 105 on a flat plateLaminar or turbulent model; with a turbulence model, the near-wall mesh and its y+
Mach MaAbout 0.3Ideal-gas density instead of constant density; above about 0.8, a mesh that resolves shocks
Knudsen KnAbout 0.01Slip walls or a particle method instead of no-slip Navier–Stokes
Courant CAbout 1The time step of an unsteady run; explicit schemes need C ≤ 1
Prandtl PrFar from 1How thin the thermal boundary layer is compared with the velocity boundary layer, and so the near-wall mesh
Richardson RiAbove about 0.1 (0.1–10 mixed, above 10 natural convection)Switch on gravity and a buoyancy-driven density model
We, Ca, EoOrder 1 or belowWhether surface tension must be modelled in a VOF or other multiphase set-up
Stokes StkAbout 0.1–1Whether particles act as passive tracers or need their own momentum (Lagrangian tracking)

Once the regime is clear, the turbulence model selector, the y+ calculator and the turbulence boundary conditions calculator take it from there.

Definitions of all 27 numbers

Each number with its definition and the ratio it expresses. Select a name to open it in the calculator.

NumberDefinitionRatio of
Flow regime
Reynolds numberRe = ρUL/μInertial to viscous forces
Mach numberMa = U/aFlow speed to the speed of sound
Froude numberFr = U/√(gL)Inertia to gravity
Knudsen numberKn = λ/LMolecular mean free path to the length scale
Strouhal numberSt = fL/UFlow time L/U to the oscillation period
Courant numberC = UΔt/ΔxDistance travelled in one time step to the cell size
Forces and losses
Drag coefficientCD = 2FD/(ρU2A)Drag force to dynamic pressure times area
Lift coefficientCL = 2FL/(ρU2S)Lift force to dynamic pressure times area
Pressure coefficientCp = (p − p∞)/(ρ∞U∞2/2)Pressure difference to dynamic pressure
Euler numberEu = Δp/(ρU2)Pressure drop to the inertial pressure ρU2
Fanning friction factorf = τw/(ρU2/2)Wall shear stress to dynamic pressure
Heat transfer
Nusselt numberNu = hL/kConvection to conduction in the fluid
Prandtl numberPr = cpμ/k = ν/αMomentum diffusivity to thermal diffusivity
Biot numberBi = hLc/ksConduction resistance in the solid to convection resistance at its surface
Péclet numberPe = LUρcp/k = Re PrHeat carried by the flow to heat conducted
Eckert numberEc = U2/(cpΔT)Kinetic energy to enthalpy difference
Grashof numberGr = gβΔTL3/ν2Buoyancy to viscous forces
Rayleigh numberRa = gβΔTL3/(να) = Gr PrBuoyancy to viscous and thermal diffusion
Richardson numberRi = gβΔTL/U2 = Gr/Re2Buoyancy to inertia
Multiphase and particles
Weber numberWe = ρU2L/σInertia to surface tension
Capillary numberCa = μU/σViscous forces to surface tension
Eötvös (Bond) numberEo = ΔρgL2/σGravity to surface tension
Stokes numberStk = t0U0/L0Particle response time to the flow time scale
Mass transfer
Schmidt numberSc = ν/DMomentum diffusivity to mass diffusivity
Sherwood numberSh = hmL/DConvective to diffusive mass transfer
Waves and combustion
Ursell numberUr = Hλ2/h3Wave steepness to the cube of the relative depth (nonlinearity of long waves)
Weaver flame speed numberWea = 100 w/wHLaminar flame speed of a gas to that of hydrogen

Conventions vary between textbooks. Some define the Euler number with ρU2/2, which makes it the pressure loss coefficient K, and the Darcy friction factor of the Moody chart is four times the Fanning factor in the table. The calculator uses the forms in the table.

Characteristic scales are a choice. State which length and speed you use (diameter or radius, chord or span, bulk or centreline velocity), because the value of a number and its critical thresholds depend on it.

References and changelog

References

F. M. White, Fluid Mechanics, 8th ed., McGraw-Hill, 2016: chapter 5, dimensional analysis and similarity.

F. P. Incropera, D. P. DeWitt, T. L. Bergman and A. S. Lavine, Fundamentals of Heat and Mass Transfer, 6th ed., Wiley, 2007: the dimensionless groups of heat and mass transfer.

R. Courant, K. Friedrichs and H. Lewy, “Über die partiellen Differenzengleichungen der mathematischen Physik”, Mathematische Annalen 100, 32–74, 1928: the Courant condition.

G. Karniadakis, A. Beskok and N. Aluru, Microflows and Nanoflows, Springer, 2005: Knudsen number flow regimes.

H. Schlichting and K. Gersten, Boundary-Layer Theory, 9th ed., Springer, 2017: transition Reynolds numbers for pipes and flat plates.

Review

Reviewed by Christoffer Johansson, M.Sc., Senior Application Specialist at Volupe. Version 2.0.

Changelog

October 2026: rebuilt as a live calculator. Automated checks confirm the same results as the previous version, except for these fixes:
– The lift coefficient divides by ρU²S; the old formula left out one factor of the speed, so it was only right at 1 m/s.
– The Biot inputs were relabelled; the heat transfer coefficient and the length had swapped labels.
– The Prandtl number describes k as the thermal conductivity, and its example uses air (k = 0.026 W/(m·K)) instead of 19 W/(m·K).
– The pressure coefficient describes p∞ as the free-stream static pressure, with 101 325 Pa as the example.
– Schmidt units read m²/s, the Knudsen symbol is Kn, the Euler and Eckert descriptions were corrected, and results are rounded to three significant figures.
New: the Courant, Grashof, Rayleigh and Richardson numbers, what each value means, Simcenter STAR-CCM+ hints and realistic examples. The first version of this page was based on Wikipedia’s list of dimensionless numbers in fluid mechanics.

Questions about these numbers

Calculator reviewed by

Christoffer Johansson

Senior Application Specialist, M.Sc.

Not sure which regime your case is in? We reply within one working day.

Ask a technical question →

What is a dimensionless number?

A ratio of two quantities with the same units, so the units cancel. In fluid mechanics most are ratios of forces or of transport rates: the Reynolds number compares inertia with viscosity, the Prandtl number momentum diffusion with heat diffusion. Flows with equal dimensionless numbers behave alike at any scale.

Which Reynolds number means turbulent flow?

It depends on the geometry and on the length you use. Pipe flow is laminar below about 2300 and usually turbulent above about 4000. On a flat plate the boundary layer starts to turn turbulent near Rex ≈ 5 × 105. Disturbances, roughness and inlet turbulence can move these values.

What Courant number should I aim for?

Explicit time stepping is only stable for C ≤ 1. Implicit solvers, such as implicit unsteady in Simcenter STAR-CCM+, stay stable at higher values, but scale-resolving simulations such as LES and DES usually aim for C ≤ 1 where the flow detail matters. Whatever you choose, check that the result does not change when you halve the time step.

When does compressibility matter?

When the Mach number exceeds about 0.3, density changes exceed about 5 % and you should use an ideal-gas density model. Below that, constant density is usually accurate, unless large temperature differences change the density; then check the Richardson number.

What is the difference between the Fanning and Darcy friction factors?

The Darcy friction factor, used in the Moody chart and in Δp = fD(L/D)½ρU², is four times the Fanning friction factor f = τw/(½ρU²). Check which one a correlation or a solver report uses before you compare values.

Do I have to use SI units?

The numbers themselves have no units, so any consistent unit system gives the same value. The calculator expects SI units in every field; mixing, for example, millimetres with metres gives a wrong result.

Can Volupe help me set up my simulation in Simcenter STAR-CCM+?

Yes. Our application engineers help you choose models, meshes and time steps in Simcenter STAR-CCM+ for your flow regime. Ask a technical question and we reply within one working day.

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