Appendix 1: description of ω-RSM
Most important features of the ω-RSM are described here on the basis of Fletcher et al. (2009) and ANSYS CFX-Solver Theory Guide (2010). In this narrative, the differential equations are presented with index notationFootnote 1. The Reynolds-averaged Navier–Stokes (RANS) equations of continuity and momentum transport for an incompressible fluid can be presented with following equations.
Continuity:
$$\frac{{{\text{D}}\rho }}{{{\text{D}}t}} = 0$$
(3)
Momentum transport:
$$\rho \frac{{{\text{D}}U_{i} }}{{{\text{D}}t}} = - \frac{\partial }{{\partial x_{i} }}\left[ {p + \frac{2}{3}\mu \frac{{\partial U_{k} }}{{\partial x_{k} }}} \right] + \frac{\partial }{{\partial x_{j} }}\left[ {\mu \left( {\frac{{\partial U_{i} }}{{\partial x_{j} }} + \frac{{\partial U_{j} }}{{\partial x_{i} }}} \right)} \right] - \rho \frac{\partial }{{\partial x_{j} }}\left( {\tau_{ij} } \right) + S_{i}$$
(4)
In Eq. (4), p is the static (thermodynamic) pressure; S
i
is the sum of body forces, and τ
ij
is the fluctuating Reynolds stress contributions.
A number of models are available in ANSYS CFX 13.0 for the Reynolds stresses (τ
ij
) in the RANS equations. Among the available models, ω-RSM is selected as the most suitable for the current work. In this model, τ
ij
is made to satisfy a transport equation. A separate transport equation is solved for each of the six Reynolds stress components of τ
ij
. The differential transport equation for Reynolds stress is as follows:
$$\rho \frac{{{\text{D}}\tau_{ij} }}{{{\text{D}}t}} = - \rho P_{ij} - \rho \varPhi_{ij} + \frac{2}{3}\beta '\rho \omega k\delta_{ij} + \frac{\partial }{{\partial x_{k} }}\left[ {\left( {\mu + \frac{{\mu_{t} }}{{\sigma_{k} }}} \right)\frac{{\partial \tau_{ij} }}{{\partial x_{k} }}} \right]$$
(5)
The Reynolds stress production tensor P
ij
is given by:
$$P_{ij} = \tau_{ik} \frac{{\partial U_{j} }}{{\partial x_{k} }} + \tau_{jk} \frac{{\partial U_{i} }}{{\partial x_{k} }}, P = \frac{1}{2}P_{kk}$$
(6)
The constitutive relation for the pressure–strain term Φ
ij
in Eq. (5) is expressed as follows:
$$\varPhi_{ij} = \beta^{\prime}C_{1} \rho \omega \left( {\tau_{ij} + \frac{2}{3}k\delta_{ij} } \right) - \hat{\alpha }\left( {P_{ij} - \frac{2}{3}P\delta_{ij} } \right) - \hat{\beta }\left( {D_{ij} - \frac{2}{3}P\delta_{ij} } \right) - \hat{\gamma }\rho k\left( {S_{ij} - \frac{1}{3}S_{kk} \delta_{ij} } \right)$$
(7)
In Eq. (7), the tensor D
ij
and the model coefficients are
$$D_{ij} = \tau_{ik} \frac{{\partial U_{k} }}{{\partial x_{j} }} + \tau_{jk} \frac{{\partial U_{k} }}{{\partial x_{i} }}$$
(8)
Model coefficients:
$$\beta^{\prime} = 0.09$$
$$\hat{\alpha } = \left( {8 + C_{2} } \right)/11$$
$$\hat{\beta } = \left( {8C_{2} - 2} \right)/11$$
$$\hat{\gamma } = \left( {60C_{2} - 4} \right)/55$$
In addition to the stress equations, the ω-RSM uses the following equations with corresponding coefficients for the turbulent eddy frequency ω and turbulent kinetic energy k.
$$\rho \frac{{{\text{D}}\omega }}{{{\text{D}}t}} = \alpha \rho \frac{\omega }{k}P_{k} - \beta \rho \omega^{2} + \frac{\partial }{{\partial x_{k} }}\left[ {\left( {\mu + \frac{{\mu_{t} }}{\sigma }} \right)\frac{\partial \omega }{{\partial x_{k} }}} \right]$$
(9)
$$\rho \frac{{{\text{D}}k}}{{{\text{D}}t}} = P_{k} - \beta^{\prime}\rho k\omega + \frac{\partial }{{\partial x_{j} }}\left[ {\left( {\mu + \frac{{\mu_{t} }}{{\sigma_{k} }}} \right)\frac{\partial k}{{\partial x_{j} }}} \right]$$
(10)
$$P_{k} = \mu_{t} \left( {\frac{{\partial U_{i} }}{{\partial x_{j} }} + \frac{{\partial U_{j} }}{{\partial x_{i} }}} \right)\frac{{\partial U_{i} }}{{\partial x_{j} }} - \frac{2}{3}\frac{{\partial U_{k} }}{{\partial x_{k} }}\left( {3\mu_{t} \frac{{\partial U_{k} }}{{\partial x_{k} }} + \rho k} \right)$$
(11)
Coefficients:
$$\alpha = \frac{\beta }{{\beta^{\prime}}} - \frac{{\kappa^{2} }}{{\sigma \left( {\beta^{\prime}} \right)^{0.5} }} = \frac{5}{9}$$
In the previously mentioned transport equations, the turbulent viscosity µ
t is defined as
$$\mu_{\text{t}} = \rho \frac{k}{\omega } .$$
(12)
Along with the basic differential equations, the flow near a stationary wall is significant for the turbulent model, ω-RSM. Usually a wall is treated with “no-slip” boundary condition for CFD simulations. Mesh-insensitive automatic near-wall treatment is available for the ω-RSM implementation in ANSYS CFX 13.0. The treatment is meant to control the smooth transition from the viscous sub-layer to the turbulent layer through the logarithmic zone. Important features of the near-wall treatment for ω-RSM are outlined as follows.
(1) In case of a hydrodynamically smooth wall, the viscous sub-layer is connected to the turbulent layer with a log-law region. Velocity profiles for the near-wall regions are as follows:Viscous sub-layer:
$$u^{ + } = y^{ + }$$
(13)
Log-law region:
$$u \, = \, (1/ \, k) \, \ln (y \, ) \, + \, B - \Delta B$$
(14)
Here, \(u^{ + } = U_{t} /u_{\tau }\), \(y^{ + } = \rho \Delta yu_{\tau } /\mu = \Delta yu_{\tau } /v\), and \(u_{\tau } = (\tau_{\text{w}} /\rho )^{0.5}\). In the log-law, B and ΔB are constants. The value of B is considered as 5.2 and that of ΔB is dependent on the wall roughness. For a smooth wall, ΔB = 0. The term Δy, in the definition of y
+, is calculated as the distance between the first and the second grid points off the wall. Special treatment of y
+ in CFX allows one to arbitrarily refine the mesh.
(2) For a hydrodynamically rough wall, the roughness is scaled with Nikuradse sand grain equivalent (k
s). Dimensional roughness \(k_{\text{s}}^{ + }\) is defined as \(k_{s}^{ + } u_{\tau } /v\). A wall is treated hydrodynamically rough when \(k_{\text{s}}^{ + }\) is greater than 70. The value of ΔB is empirically correlated to \(k_{\text{s}}^{ + }\) as follows.
$$\Delta B = \frac{1}{\kappa }\ln \left( {1 + 0.3k_{s}^{ + } } \right)$$
(15)
ΔB represents a parallel shift of logarithmic velocity profile compared to the smooth wall condition.
(3) At the fully rough condition (\(k_{\text{s}}^{ + } > 70\)), the viscous sub-layer is assumed to be destroyed. Effect of viscosity in the near-wall region is neglected.
(4) The equivalent sand grains are considered to have a blockage effect on the flow. This effect is taken into account by virtually shifting the wall by a distance of 0.5 k
s.
Appendix 2: sample calculation illustrating application of the proposed correlation
An example illustrating the application of the proposed correlation, i.e., Equation (3) is presented here. The correlation is used to predict the frictional pressure loss for a specific pipe flow case, and then, the predicted value is compared with the measured value. The data for this example are reported by McKibben et al. (2016).
Measured/known parameters
-
Internal diameter of the pipeline (D): 103.3 mm
-
Average water velocity (V): 1.0 m/s
-
Density of water (ρ
w): 997 kg/m3
-
Viscosity of water (µ
w): 0.001 Pa s
-
Average thickness of wall coating/fouling (t
c) (measured): 2.0 mm
Calculations
-
Effective diameter (D
eff): \(D_{\text{eff}} = D - 2t_{\text{c}} = 99.3 \,\,{\text{mm}}\)
-
Effective velocity (V
eff): \(V_{{\text{eff}}} = V\left( {\frac{D}{{D_{{\text{eff}}} }}} \right)^{2} = 1.1 \,\,{\text{m/s}}\)
-
Reynolds number (Re
w): \({Re}_{\text{w}} = \frac{{D_{\text{eff}} V_{{\text{eff}}} \rho_{\text{w}} }}{{\mu_{\text{w}} }} = 1.1 \times 10^{5}\)
-
Equivalent hydrodynamic roughness (k
s): \(k_{\text{s}} = 2.76t_{\text{c}} = 5.52\,\, {\text{mm}}\)
-
Darcy friction factor (f), obtained using the Swamee–Jain correlation: \(f = 0.25\left[ {\log \left( {\frac{{k_{\text{s}} }}{{3.7D_{\text{eff}} }} + \frac{5.74}{{Re_{\text{w}}^{0.9} }}} \right)} \right]^{ - 2} = 0.0756\)
Predicted pressure gradient
$$\frac{\Delta P}{L} = f\frac{{\rho_{\text{w}} V_{{\text{eff}}}^{2} }}{{2D_{\text{eff}} }} = 0.44 \,\,{\text{kPa/m}}$$
Measured pressure gradient
(∆P/L): 0.45 kPa/m