Non-Dimensional Quantities

The most common non-dimensional quantity used in turbulence modeling is the Reynolds number, which is the ratio of inertial over viscous forces. The following definitions are used throughout the theory of turbulence modeling:

Wall-distance Reynolds number:

图 1. EQUATION_DISPLAY
Re⁡d=kdν
(1134)

where:

  • k is the turbulent kinetic energy.
  • d is the distance to the wall.
  • ν is the kinematic viscosity.

Turbulent Reynolds number:

图 2. EQUATION_DISPLAY
Re⁡t=k2νε
(1135)

or:

图 3. EQUATION_DISPLAY
Re ⁡ t = k ν ω
(1136)

or:

Re ⁡ t = μ t μ
(1137)

where:

  • ε is the turbulent dissipation rate.
  • ω is the specific dissipation rate.
  • μ t is the turbulent eddy viscosity.
  • μ is the dynamic viscosity.

Kolmogorov Reynolds number:

图 4. EQUATION_DISPLAY
Re⁡ε=(νε)1/4dν
(1138)

Strain-rate Reynolds number:

图 5. EQUATION_DISPLAY
Reν= d2Sν
(1139)

where S is given by Eqn. (1129).

Another useful number is the Rayleigh number, defined as:

图 6. EQUATION_DISPLAY
Ra=‖gi‖βΔTLref3να
(1140)

where:

  • ‖gi‖ is the norm of the gravity vector.
  • β is the thermal expansion coefficient.
  • ΔT is the temperature difference (typically between fluid and containing walls).
  • Lref is the characteristic length.
  • α is the thermal diffusivity.

α is usually defined as α=νPr⁡, with Pr⁡ the Prandtl number defined as:

图 7. EQUATION_DISPLAY
Pr=Cpμκ
(1141)

where:

  • Cp is the specific heat.
  • κ is the thermal conductivity.