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Turbulent heat transport                                          283























           Fig. 6.2.1.5 A priori testing of different models of the wall-normal turbulent heat flux in
           generic situations of turbulent natural convection in a side-heated vertical infinite channel,
                   6
           Ra¼5 10 and Pr¼0.71. Note: SGDH and GGDH models are described in the next sections;
           AFM can be obtained by omitting the last term in the Eq. (6.2.1.10) and by assuming
           C t1 ¼ 1; and finally, NEW model represents the AHFM-2005 formulation
           (Kenjeres et al., 2005).


              Within the framework of the THINS project, this model was implemented in the
           commercial code STAR-CCM+. This model was originally developed to provide
           improved solutions for the natural convection flow regime for fluids with a Prandtl
           number close to unity (as shown in Fig. 6.2.1.5).

           AHFM-NRG (Shams et al., 2014)
           As mentioned earlier, within the THINS project, the AHFM-2005 was implemented in
           the commercial code STAR-CCM+ (Shams et al., 2014). The prime goal was to assess
           and further calibrate the AHFM-2005 for the application to natural, mixed, and forced
           convection flow regimes for low Prandtl fluids. In this regard, a number of test cases
           were considered and are described in Shams et al. (2014). Accordingly, the model
           coefficients were calibrated separately for the different flow regimes. It was shown
           that the AHFM with calibrated coefficients shows a significant improvement over
           the AHFM-2005 for the selected test cases in natural, mixed, and forced convection
           flow regimes. However, in the case of forced convection flows, the mean temperature
           was underpredicted for low Prandtl fluids (for details, see Shams et al. (2014)). The
           extent of this underprediction in the temperature field varies for different Reynolds
           and Prandtl numbers. The coefficient C t1 was further calibrated to overcome this
           underprediction with the help of DNS databases. Consequently, a correlation for
           C t1 was proposed, and the resulting model is called AHFM-NRG (see
           Table 6.2.1.1). The proposed correlation within the AHFM-NRG shows dependency
           of Reynolds and Prandtl numbers in a logarithmic manner to accommodate the wall-
           normal temperature gradient for the heat flux term and is shown in Fig. 6.2.1.6.
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