ArticleAssessment of k–ε models using tetrahedral grids to describe the turbulent flow field of a PBT impeller and validation through the PIV technique
Introduction
Mixing in stirred tank reactors (STR) is one of the most important topics of chemical process engineering. Good mixing assures higher reaction efficiency and shorter process time, reducing process costs [1], [2]. Mixing in a STR relies on several geometrical parameters, configurations and operational conditions, but undoubtedly, impeller performance is the most influential factor of them all [3], [4], [5]. Therefore, careful analysis of the fluid flow driven by the impeller along the whole vessel is necessary to evaluate reactor performance. A large variety of impeller geometries have been developed to solve all sorts of industrial problems [6], [7], [8]. For its enhancement capabilities blending/mixing and heat transfer, one of the most studied impellers is the pitched blade turbine (PBT). Since the micro-mixing and macro-mixing rely on the flow velocities and turbulent components, suitable analytical, experimental and numerical tools are required to depict the overall flow patterns. In this sense, the solutions obtained using computational fluid dynamics (CFD) require a turbulence model capable of reproducing fairly the fluid behavior with a minimum computational effort. Reynolds-Averaged Navier–Stokes (RANS) models of the k–ε family represent a practical balance of the aforementioned constraints, since most powerful techniques as LES and DNS need an important amount of grid elements and simulation time, and thus, they are not suitable for practical engineering applications [9]. Several works have been devoted to analyze the flow inside a STR using different grid resolutions, spatial discretization, coupling scheme and turbulence model, either for PBT or Rushton turbines, using the Multiple Reference Frame (MRF) approach [10], [11], [12] or Sliding Mesh (SM) [6], [13], [14]. In such works, it is stated that the numerical models deliver fair predictions for mean velocities, but under-predicted values for the turbulent quantities (turbulent kinetic energy “k”, and dissipation rate “ε”), compared with the LDV or 2D PIV measurements. For example, Jaworski and Zakrzewska [15], performed a comparison of the Standard, RNG, Realizable and other models in a STR for a non-structured grid composed of 112,000 hexahedral elements, and subpredicted values were found for k. Murthy and Joshi [16], evaluated different turbulence models and impeller designs in domains composed of about 575,000 elements. According to their results, the Standard model performed weakly in the prediction of the turbulent production and dissipation profiles, specially near the blade regions where the flow is anisotropic. However, it is not clear if the zero thickness wall assumption adopted by the authors affected their predictions, as it is known that blade thickness influences the flow parameters [17]. Further, the Standard model was taken as the representative case for the k–ε family. Joshi et al. [18], [19], analyzed velocities and turbulent profiles induced by Rushton and PBT impellers using different turbulence models. The authors reported important deviations between the RNG and Standard model predictions for velocities, turbulent kinetic energy production and dissipation rates, and suggested that the Standard model performs well in unidirectional flow regions with weak recirculation. From the numerical point of view, at that time, the computational resources were limited in comparison to actual capabilities, and the grids solved were commonly of about half million cells or less, and were composed of hexahedral elements [11], [14], [20], [21]. Since grid refinement and cell number are important to capture the main flow gradients, especially for the turbulent parameters [22], it is desirable to assess those quantities using larger grids. Also, because the actual STRs contain accessories or their geometry is complex enough to be mapped by hexahedral grids, tetrahedral cells become an alternative, and its assessment becomes an interesting issue to address. Although this kind of cells has been proven with success in the CFD modeling of a STR agitated by impellers in complex geometries [23], [24], [25], there is no information about the performance of the different models under the same comparative basis. It must be taken into account that the different closure models Standard, RNG or Realizable obey to deep physic assumptions and care must be taken regarding generalizing the results of the Standard model as unique and representative for all closure scenarios. The importance of achieving good quality results from RANS simulations relies not only on the necessity of fair average quality predictions of mean flow velocity and turbulent parameters, but also, in the necessity of good starting solutions for unsteady approaches, to decrease the time required to reach the desired statistic convergence. Furthermore, the engineering modeling of multiphase flows, combustion, and thermally affected boundary layers still needs an adequate choice of a k–ε model to account for turbulence, as more sophisticated models (DNS, LES) demand a significant amount of computational resources. Based on the above discussion, the objective of this work is to assess the prediction capabilities of the Standard [26], RNG [27] and Realizable [28] k–ε models of the flow features in a STR with four baffles, driven by a 4 blade PBT impeller at Re ≈ 52,000, using unstructured grids. The validation is accomplished via estimation of the dissipation rate from torque measurements, and by 2D-PIV measurements of the flow field velocities and turbulent quantities near the impeller, when the full blade coincides with the measurement plane at 0°. This region was selected as it is the zone where the mean and turbulent energy are produced and transported, defining the subsequent flow patterns. Also, the performance of the Sliding Mesh (SM) method was assessed for the three turbulence models. The importance of this work, relies on the understanding of the models behavior in non-structured tetrahedral grids especially useful to represent complex geometries, which are the natural evolution of second generation STR devices.
Section snippets
Tank geometry and operational conditions
In Fig. 1a, the STR geometrical description is illustrated. For the purposes of the measuring technique, the vessel was built using a 2 mm thick acrylic sheet, with T = H = 0.25 m. Four baffles were used in order to break flow symmetry. The width of each baffle is T/10 with a thickness of 3.5 mm. The PBT was composed of 4 rotated blades at 45°, with diameter D = 0.0795 m, blade vertical projection of 14.3 mm and thickness of 1.5 mm. The bottom clearance of the tank was fixed at T/3, in order to obtain a
Solution methods and turbulence closure models
A 3D full model of the STR was solved using ANSYS-FLUENT V.13.0 in a segregated manner for both, the MRF and SM approaches, defining a rotational zone near the impeller and a non-rotational zone for the rest of the domain. All evaluated grids were composed of tetrahedral elements, all below the maximum skewness of 0.8, which were below the 0.95 limit listed in the Fluent user's manual [42]. The SIMPLE pressure–velocity coupling algorithm was implemented in the solution. Second order for
Total production and dissipation rates
Fig. 9 shows the power number from torque, the power number from dissipated power and the pumping number predicted from the three turbulence models. Again, the Nq and Np were adequately predicted for the Standard, RNG and Realizable models. For the RNG case, the influence of the swirl account “αs” did not improved the predictions, as the Np was overestimated about 20% for αs = 0.07, and subpredicted almost equally for αs = 0.25. Also, all models subpredicted the Np − ε by more than 26% of the
Conclusions
The operation of a PBT impeller inside a STR under fully turbulent conditions was simulated with tetrahedral grids, using Standard, RNG and Realizable turbulence models under the MRF and SM approaches. For validation purposes, axial and radial velocities, turbulence production k and dissipation rate ε were obtained from 2D PIV measurements. For the MRF approach all models delivered good Nq values because of the adequately predicted mean axial velocity. Although the Np derived from torque was in
Acknowledgments
The authors wish to express their acknowledgement to the National Council of Science and Technology, Mexico CONACyT for the support provided for this research, through the Basic Science project CB-2011/169786. Thanks are also due to the Engineering Center and Industrial Development from Mexico for the facilities provided during the accomplishment of this work.
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