M. Pourtousia,
Mohammadjavad Zeinali*b,
P. Ganesan*a and
J. N. Sahu*c
aDepartment of Mechanical Engineering, University of Malaya, 50603 Kuala Lumpur, Malaysia. E-mail: poo_ganesan@um.edu.my
bVehicle System Engineering Laboratory, Malaysia-Japan International Institute of Technology, Universiti Teknologi Malaysia, Jalan Semarak, 54100 Kuala Lumpur, Malaysia. E-mail: javad_zeynaly@yahoo.com
cPetroleum and Chemical Engineering Programme Area, Faculty of Engineering, Institut Teknologi Brunei, Tungku Gadong, P.O. Box 2909, Brunei Darussalam. E-mail: jn.sahu@itb.edu.bn; jay_sahu@yahoo.co.in
First published on 30th September 2015
This work presents a combination of Computational Fluid Dynamics (CFD) and Adaptive Network-based Fuzzy Inference System (ANFIS) developed for flow characterization inside a cylindrical bubble column reactor. An attempt has been made to predict the liquid flow pattern and gas dynamics for various ring sparger diameters (i.e., 0.07–0.16 m) and bubble column heights. Gas hold-up, Turbulent Kinetic Energy (TKE) and axial liquid velocity are the output parameters predicted by using the ANFIS method with respect to sparger diameter, axial coordination and radial coordination. Various architectures of the ANFIS method were constructed in order to achieve an accurate prediction model of the liquid flow behavior and gas dynamics inside the bubble column. ANFIS approaches were trained and tested by using CFD simulation results. The performance of the ANFIS approaches was examined by comparing the root mean square error and correlation coefficient values of the prediction models. The CFD simulation results are validated with existing experimental and numerical data and mathematical correlations. Both CFD simulation and ANFIS prediction results show that ring sparger diameter significantly changes the liquid flow pattern and gas dynamics, resulting in different amounts of the gas inside the column. Different ANFIS structures were selected for precise estimation of gas hold-up, TKE and axial liquid velocity. Eventually, the mathematical correlations of the proposed ANFIS approaches are presented with correlation coefficients of 0.9717, 0.9917 and 0.9877 for gas hold-up, turbulent kinetic energy and axial liquid velocity prediction models. Hence, the ANFIS approach is able to provide a prediction of the 3D bubble column hydrodynamics in a continuous domain.
Design, optimization and manufacturing of these reactors highly depend on the complex dynamics of gas bubble interaction, liquid flow pattern and prevailing gas and liquid regime (i.e., homogeneous or heterogeneous).3,11–13,16–20 One of the main challenges in enhancing the design and manufacturing of the bubble column is to properly predict and measure the hydrodynamics properties, while the complex behavior of the gas and liquid movement, including the interaction between bubbles are unavoidable.1,3,11,12,15,21,22 Several experimental methods such as Particle Image Velocimetry (PIV), Laser Doppler Anemometry (LDA) and radioactive particle tracking have been developed in recent years to develop an insight into this arguably complex and nonlinear behavior of gas and liquid dynamics, particularly liquid flow pattern and amount of gas inside bubble column reactors.23–26
Apart from experimental techniques, many CFD approaches and mathematical calculations are available to predict bubble column hydrodynamics.3,7,13–15,27–29 Nowadays, high performance computers have enabled the use of detailed mathematical and computational approaches to study the liquid flow pattern and gas dynamics on a feasible time span and space. There are two main CFD approaches i.e., the Eulerian–Eulerian and Eulerian–Lagrangian to model multiphase fluid flow.3,6,10,13–15,19,27–30 In the Eulerian–Lagrangian approach (discrete particle model), each bubble is separately tracked inside the bubble column by solving forces acting on the bubbles, while continuum description is considered for the liquid phase.6 In this approach, the interaction between bubbles i.e., coalescence, break-up and collisions can be observed. However, this framework is limited for large bubble columns with high number of bubbles due to solving more equations in large domains. On the other hand, Eulerian–Eulerian approach (the two fluid model), considers gas bubbles and liquid in the Eulerian framework as two interpenetrating fluids. Unlike the discrete particle model, the Eulerian framework is an appropriate method to solve the large bubble column with high superficial gas velocity, particularly in industrial bubble column reactors.13–15,22,29
Although several experimental, numerical and mathematical methods have been used to measure and estimate the flow pattern and bubbles dynamics,3,5–7,9,31–39 there are some difficulties to completely predict the liquid flow pattern and gas dynamics (bubble coalescence, break-up, velocity, shape, size and gas hold-up) at each point of 3D bubble column reactors when the operation conditions (i.e., superficial gas velocity, column dimensions, gas and liquid properties and sparger parameters), flow regime and operation time change. For instance, measuring the fluid flow parameters inside the 3D bubble column reactor during experiment is extremely expensive and required much measurement equipment. Computation time and computer capability are the major limitations of the computational approaches in numerically simulation of the large bubble column and various operation conditions. Because of these limitations, soft computing methods have been developed to estimate the bubble column hydrodynamics in various conditions that have not been simulated or experimented at every point of the bubble column.37
There are several soft computing techniques (e.g., neural networks, support vector machines, evolutionary algorithms, and adaptive neuro fuzzy inference system) proposed in many studies to estimate phenomena behaviour in the real life applications.37,40–47 Among these techniques, Adaptive Network-based Fuzzy Inference System (ANFIS) has attracted researchers because of its ability to learn complex relationships and its vast application has been illustrated in numerous studies.41,48–50 The accuracy of the ANFIS approach can be altered by changing prediction model structure and adapted on the basis of the relationship complexity.40,41,51–58 ANFIS method can use either simulation or experimental results as training data to learn the phenomena behavior. An appropriate set of training data is required to successfully train ANFIS model.
Azwadi et al.41 used CFD results for training ANFIS method to estimate the temperature and flow fields in a 2D lid-driven cavity. They found that the result of ANFIS method is in good agreement with temperature and flow field obtained by CFD simulation. Recently, Pourtousi et al.37 employed this methodology to predict multiphase flow inside a bubble column reactor. They utilized bubble column hydrodynamics data (i.e., liquid velocity components, turbulent kinetic energy and gas hold-up), obtained by CFD (Eulerian method) simulation, at the bubble column bulk region for ANFIS learning process. It was found that the combination of CFD and ANFIS is a robust methodology to predict the bubble column hydrodynamics properties in a continuous domain. They showed that ANFIS method can be a favourable replacement with CFD simulation to predict the complex behaviour of multiphase flow inside the bubble column reactor when the flow regime is homogeneous.
In this study we develop the recent methodology (Pourtousi et al.’s research37) to propose an intelligent approach which is able to model multiphase flow inside the bubble column reactor for various sparger diameters. In addition, an attempt has also been made to improve the overall predictive capabilities of liquid flow pattern and gas hold-up using the combination of CFD and ANFIS methods. A new mathematical correlation is proposed to predict the bubble column hydrodynamics as the ring sparger diameters varied from 0.07 to 0.16 m. The effect of ring sparger diameter on liquid flow velocity, turbulent kinetic energy and gas hold-up is investigated using ANFIS and CFD results. Various ANFIS structures were constructed to realize the most accurate structure for each output. The accuracy of all prediction models was compared by two common error evaluation formulas; root means square error and correlation coefficient. The results of selected ANFIS models were compared to the CFD simulation results to illustrate the capability of the ANFIS approach.
The mass conservation equation for both liquid and gas is shown as follows:
![]() | (1) |
In the present numerical investigation, the control volume method is used to discretize the conservation equations. There are several solution methods (such as finite difference,59 Lattice Boltzmann,60–63 finite volume method,13–15,27,28 etc.) in the CFD to solve the fluid flow problems. The most robust, reliable and the one, on which CFX is based, is called finite volume discretization method. Based on the finite volume discretization method, the momentum transfer formulation for multi-bubbles and liquid phases can be described as:
![]() | (2) |
The right side of the momentum transfer formulation consists of the stress, pressure gradient, gravity and the momentum interfacial exchange between gas bubbles and liquid. In this equation, the stress term of phase k is represented as follows:
![]() | (3) |
μeff,I = μL + μT,L + μBI,L | (4) |
The effective gas viscosity is formulated based on the effective viscosity of liquid and it can be described as follows:
![]() | (5) |
In the current CFD simulation study, the model of Sato and Sekoguchi is employed for the extra term due to bubble induced turbulence, containing a constant value of Cμ,BI = 0.6. The viscosity due to the turbulence induced by the gas bubble flow has been described by ref. 64 and 65. They demonstrated a model taking account the turbulence induced by bubble agitation inside the liquid phase. In general, to predict momentum of bubble flow it is crucial to describe the turbulent structure of the continuous liquid phase, which may result in how to describe the contribution of bubble existence to the flow characteristics. Sato and Sekoguchi,64 reported that the turbulent shear stress in bubble flow is affected by two terms. Firstly, the inherent liquid turbulence which is independent of relative motion of bubbles in the liquid phase. Secondly, the additional liquid turbulence term, producing by bubble agitation (bubble motion).
μBI,L = ρLCμ,BI∈G![]() | (6) |
The last term in the momentum transfer equation is the total interfacial force. This term can be described as follows:
MI,L = −MI,G = MD,L + MTD,L | (7) |
The total interfacial forces, illustrated above, indicate the drag and turbulent dispersion force when the lift and virtual mass are neglected. The interphase momentum transfer between gas bubble and liquid phase due to drag force is shown as follows:
![]() | (8) |
Turbulent dispersion force model is used for current CFD investigations based on literature studies3,15,22,37,66 to improve the flow field prediction towards the walls. This model, formulated by Lopez de Bertodano,67 is on the basis of the analogy with molecular movement and interaction. It approximates a turbulent diffusion of the bubbles by the liquid eddies and can be described as:
MTD,L = −MTD,G = −CTDρLk∇∈L | (9) |
In addition to interfacial forces, a proper selection of turbulence model is necessary to appropriately predict the bubble column hydrodynamics.3,12–16,22,29,37,38,66 For the disperse bubbly phase a zero equation turbulence model is used. However, the standard k–ε model is applied for the continuous phase which have been used and recommended in prior CFD studies due to obtaining average results, simplicity and low computation time.3,12–16,22,27–29,37,66,68 As k–ε is employed for turbulence modelling, the turbulent eddy viscosity is calculated using the standard k–ε turbulence model, where k represents the turbulent kinetic energy and ε its dissipation rate in the liquid phase. k and ε determine the energy in turbulence and the scale of the turbulence, respectively. The turbulent eddy viscosity can be defined as follows:
![]() | (10) |
The turbulent kinetic energy (k) and its energy dissipation rate (ε) are calculated based on the following governing equations:
![]() | (11) |
![]() | (12) |
Being k and ε calculated from their conservation equations. The k–ε model is applied, in this work, with its standard constants values (model parameters): Cμ = 0.09, σk = 1, σε = 1, Cε1 = 1.44, Cε2 = 1.92. These constants, although not universal, are commonly used in the case of single-phase flow.19,69 The selection of these values based on recommendation of prior numerical studies.13,15,22,37,70 The term G indicates the production of turbulent kinetic energy and can be represented as:
G = τL:∇uL | (13) |
wi = μAi(Ds) × μBi(x) × μCi(H) | (14) |
In layer three, the relative value of firing strength of each rule is calculated. This value equals to the weight of each layer over the total amount of all rules' firing strengths:
![]() | (15) |
![]() ![]() |
A hybrid learning algorithm is utilized to update the parameters in which MFs parameters are updated by gradient descent method and consequent parameters are updated by Least Square Estimate (LSE) method.
![]() | (16) |
The equation of CC that provides the relationship strength between prediction and CFD simulation results is as:
![]() | (17) |
In this aim, bell-shaped, Gaussian and Sigmoidal MFs, and 27 combinations of number of MFs are employed to compare the estimation output errors. Table 1 portrays the equation of utilized MFs in the ANFIS model and Tables 2 and 3 depict the RMSE and CC values of various employed ANFIS structures.
Number of MF | Output | RMSE for | Number of MF | Output | RMSE for | ||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Ds | H | x | Bell-shaped MF | Gaussian MF | Sigmoidal MF | Ds | H | x | Bell-shaped MF | Gaussian MF | Sigmoidal MF | ||
2 | 2 | 2 | εg | 0.0059 | 0.0060 | 0.0060 | 3 | 3 | 4 | εg | 0.0041 | 0.0042 | 0.0040 |
TKE | 0.0025 | 0.0026 | 0.0030 | TKE | 0.0016 | 0.0017 | 0.0017 | ||||||
Vy | 0.0261 | 0.0263 | 0.0278 | Vy | 0.0131 | 0.0146 | 0.0162 | ||||||
2 | 2 | 3 | εg | 0.0049 | 0.0049 | 0.0051 | 3 | 4 | 2 | εg | 0.0056 | 0.0057 | 0.0057 |
TKE | 0.0021 | 0.0019 | 0.0022 | TKE | 0.0017 | 0.0021 | 0.0020 | ||||||
Vy | 0.0201 | 0.0207 | 0.0226 | Vy | 0.0189 | 0.0210 | 0.0225 | ||||||
2 | 2 | 4 | εg | 0.0046 | 0.0048 | 0.0048 | 3 | 4 | 3 | εg | 0.0041 | 0.0043 | 0.0043 |
TKE | 0.0022 | 0.0018 | 0.0022 | TKE | 0.0015 | 0.0016 | 0.0016 | ||||||
Vy | 0.0187 | 0.0182 | 0.0213 | Vy | 0.0131 | 0.0143 | 0.0174 | ||||||
2 | 3 | 2 | εg | 0.0059 | 0.0060 | 0.0059 | 3 | 4 | 4 | εg | 0.0039 | 0.0038 | 0.0039 |
TKE | 0.0022 | 0.0023 | 0.0024 | TKE | 0.0015 | 0.0015 | 0.0016 | ||||||
Vy | 0.0223 | 0.0237 | 0.0239 | Vy | 0.0111 | 0.0122 | 0.0137 | ||||||
2 | 3 | 3 | εg | 0.0047 | 0.0048 | 0.0047 | 4 | 2 | 2 | εg | 0.0057 | 0.0058 | 0.0058 |
TKE | 0.0019 | 0.0019 | 0.0018 | TKE | 0.0024 | 0.0026 | 0.0027 | ||||||
Vy | 0.0166 | 0.0178 | 0.0194 | Vy | 0.0255 | 0.0254 | 0.0265 | ||||||
2 | 3 | 4 | εg | 0.0046 | 0.0046 | 0.0044 | 4 | 2 | 3 | εg | 0.0045 | 0.0047 | 0.0047 |
TKE | 0.0019 | 0.0018 | 0.0018 | TKE | 0.0023 | 0.0023 | 0.0023 | ||||||
Vy | 0.0149 | 0.0152 | 0.0172 | Vy | 0.0192 | 0.0196 | 0.0216 | ||||||
2 | 4 | 2 | εg | 0.0058 | 0.0059 | 0.0059 | 4 | 2 | 4 | εg | 0.0044 | 0.0045 | 0.0044 |
TKE | 0.0020 | 0.0020 | 0.0026 | TKE | 0.0022 | 0.0018 | 0.0020 | ||||||
Vy | 0.0205 | 0.0222 | 0.0217 | Vy | 0.0168 | 0.0176 | 0.0198 | ||||||
2 | 4 | 3 | εg | 0.0044 | 0.0045 | 0.0047 | 4 | 3 | 2 | εg | 0.0057 | 0.0057 | 0.0057 |
TKE | 0.0017 | 0.0018 | 0.0018 | TKE | 0.0017 | 0.0020 | 0.0023 | ||||||
Vy | 0.0139 | 0.0163 | 0.0177 | Vy | 0.0218 | 0.0226 | 0.0225 | ||||||
2 | 4 | 4 | εg | 0.0043 | 0.0044 | 0.0040 | 4 | 3 | 3 | εg | 0.0042 | 0.0045 | 0.0043 |
TKE | 0.0017 | 0.0017 | 0.0018 | TKE | 0.0016 | 0.0017 | 0.0016 | ||||||
Vy | 0.0127 | 0.0109 | 0.0152 | Vy | 0.0153 | 0.0163 | 0.0180 | ||||||
3 | 2 | 2 | εg | 0.0057 | 0.0058 | 0.0058 | 4 | 3 | 4 | εg | 0.0037 | 0.0040 | 0.0039 |
TKE | 0.0024 | 0.0026 | 0.0029 | TKE | 0.0015 | 0.0016 | 0.0014 | ||||||
Vy | 0.0255 | 0.0255 | 0.0280 | Vy | 0.0124 | 0.0144 | 0.0148 | ||||||
3 | 2 | 3 | εg | 0.0045 | 0.0047 | 0.0047 | 4 | 4 | 2 | εg | 0.0055 | 0.0057 | 0.0056 |
TKE | 0.0024 | 0.0024 | 0.0020 | TKE | 0.0016 | 0.0018 | 0.0022 | ||||||
Vy | 0.0193 | 0.0196 | 0.0223 | Vy | 0.0204 | 0.0209 | 0.0203 | ||||||
3 | 2 | 4 | εg | 0.0044 | 0.0044 | 0.0045 | 4 | 4 | 3 | εg | 0.0040 | 0.0043 | 0.0042 |
TKE | 0.0024 | 0.0024 | 0.0019 | TKE | 0.0013 | 0.0015 | 0.0015 | ||||||
Vy | 0.0173 | 0.0179 | 0.0203 | Vy | 0.0130 | 0.0144 | 0.0163 | ||||||
3 | 3 | 2 | εg | 0.0057 | 0.0058 | 0.0058 | 4 | 4 | 4 | εg | 0.0037 | 0.0034 | 0.0032 |
TKE | 0.0018 | 0.0022 | 0.0021 | TKE | 0.0013 | 0.0013 | 0.0013 | ||||||
Vy | 0.0223 | 0.0224 | 0.0232 | Vy | 0.0094 | 0.0104 | 0.0127 | ||||||
3 | 3 | 3 | εg | 0.0043 | 0.0044 | 0.0043 | |||||||
TKE | 0.0017 | 0.0019 | 0.0017 | ||||||||||
Vy | 0.0157 | 0.0164 | 0.0189 |
Number of MF | Output | CC for | Number of MF | Output | CC for | ||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Ds | H | x | Bell-shaped MF | Gaussian MF | Sigmoidal MF | Ds | H | x | Bell-shaped MF | Gaussian MF | Sigmoidal MF | ||
2 | 2 | 2 | εg | 0.8997 | 0.8973 | 0.8984 | 3 | 3 | 4 | εg | 0.9524 | 0.9499 | 0.9552 |
TKE | 0.9598 | 0.9414 | 0.9124 | TKE | 0.9845 | 0.9776 | 0.9838 | ||||||
Vy | 0.9272 | 0.9265 | 0.9171 | Vy | 0.9821 | 0.9778 | 0.9728 | ||||||
2 | 2 | 3 | εg | 0.9331 | 0.9311 | 0.9282 | 3 | 4 | 2 | εg | 0.9110 | 0.9063 | 0.9088 |
TKE | 0.9771 | 0.9499 | 0.9750 | TKE | 0.9767 | 0.9653 | 0.9639 | ||||||
Vy | 0.9576 | 0.9548 | 0.9459 | Vy | 0.9627 | 0.9536 | 0.9465 | ||||||
2 | 2 | 4 | εg | 0.9399 | 0.9357 | 0.9342 | 3 | 4 | 3 | εg | 0.9531 | 0.9487 | 0.9486 |
TKE | 0.9775 | 0.9505 | 0.9752 | TKE | 0.9840 | 0.9831 | 0.9830 | ||||||
Vy | 0.9635 | 0.9655 | 0.9522 | Vy | 0.9823 | 0.9786 | 0.9682 | ||||||
2 | 3 | 2 | εg | 0.9008 | 0.8982 | 0.8993 | 3 | 4 | 4 | εg | 0.9582 | 0.9601 | 0.9572 |
TKE | 0.9704 | 0.9673 | 0.9533 | TKE | 0.9850 | 0.9826 | 0.9852 | ||||||
Vy | 0.9473 | 0.9406 | 0.9398 | Vy | 0.9874 | 0.9847 | 0.9804 | ||||||
2 | 3 | 3 | εg | 0.9379 | 0.9347 | 0.9373 | 4 | 2 | 2 | εg | 0.9080 | 0.9047 | 0.9043 |
TKE | 0.9798 | 0.9800 | 0.9770 | TKE | 0.9596 | 0.9237 | 0.9309 | ||||||
Vy | 0.9711 | 0.9669 | 0.9605 | Vy | 0.9310 | 0.9315 | 0.9252 | ||||||
2 | 3 | 4 | εg | 0.9413 | 0.9404 | 0.9460 | 4 | 2 | 3 | εg | 0.9422 | 0.9378 | 0.9386 |
TKE | 0.9813 | 0.9798 | 0.9796 | TKE | 0.9422 | 0.9401 | 0.9339 | ||||||
Vy | 0.9770 | 0.9759 | 0.9691 | Vy | 0.9616 | 0.9599 | 0.9507 | ||||||
2 | 4 | 2 | εg | 0.9025 | 0.8997 | 0.9016 | 4 | 2 | 4 | εg | 0.9459 | 0.9437 | 0.9455 |
TKE | 0.9749 | 0.9680 | 0.9586 | TKE | 0.9780 | 0.9490 | 0.9441 | ||||||
Vy | 0.9558 | 0.9480 | 0.9504 | Vy | 0.9707 | 0.9677 | 0.9589 | ||||||
2 | 4 | 3 | εg | 0.9460 | 0.9432 | 0.9386 | 4 | 3 | 2 | εg | 0.9081 | 0.9092 | 0.9064 |
TKE | 0.9811 | 0.9803 | 0.9783 | TKE | 0.9772 | 0.9740 | 0.9424 | ||||||
Vy | 0.9798 | 0.9724 | 0.9672 | Vy | 0.9498 | 0.9462 | 0.9465 | ||||||
2 | 4 | 4 | εg | 0.9493 | 0.9465 | 0.9556 | 4 | 3 | 3 | εg | 0.9511 | 0.9430 | 0.9491 |
TKE | 0.9822 | 0.9814 | 0.9801 | TKE | 0.9843 | 0.9812 | 0.9818 | ||||||
Vy | 0.9832 | 0.9877 | 0.9760 | Vy | 0.9757 | 0.9723 | 0.9660 | ||||||
3 | 2 | 2 | εg | 0.9067 | 0.9026 | 0.9037 | 4 | 3 | 4 | εg | 0.9611 | 0.9547 | 0.9573 |
TKE | 0.9537 | 0.9217 | 0.9281 | TKE | 0.9915 | 0.9832 | 0.9900 | ||||||
Vy | 0.9306 | 0.9308 | 0.9157 | Vy | 0.9840 | 0.9785 | 0.9774 | ||||||
3 | 2 | 3 | εg | 0.9422 | 0.9374 | 0.9372 | 4 | 4 | 2 | εg | 0.9126 | 0.9080 | 0.9096 |
TKE | 0.9651 | 0.9499 | 0.9762 | TKE | 0.9802 | 0.9708 | 0.9475 | ||||||
Vy | 0.9611 | 0.9596 | 0.9477 | Vy | 0.9564 | 0.9542 | 0.9567 | ||||||
3 | 2 | 4 | εg | 0.9457 | 0.9447 | 0.9440 | 4 | 4 | 3 | εg | 0.9553 | 0.9489 | 0.9508 |
TKE | 0.9440 | 0.9463 | 0.9824 | TKE | 0.9917 | 0.9893 | 0.9870 | ||||||
Vy | 0.9687 | 0.9664 | 0.9568 | Vy | 0.9824 | 0.9786 | 0.9722 | ||||||
3 | 3 | 2 | εg | 0.9082 | 0.9035 | 0.9056 | 4 | 4 | 4 | εg | 0.9612 | 0.9687 | 0.9717 |
TKE | 0.9695 | 0.9574 | 0.9601 | TKE | 0.9936 | 0.9930 | 0.9915 | ||||||
Vy | 0.9476 | 0.9470 | 0.9433 | Vy | 0.9909 | 0.9888 | 0.9834 | ||||||
3 | 3 | 3 | εg | 0.9494 | 0.9470 | 0.9473 | |||||||
TKE | 0.9824 | 0.9791 | 0.9816 | ||||||||||
Vy | 0.9742 | 0.9720 | 0.9625 |
Gaussian MF has two parameters (c and σ), bell-shaped MF has three parameters (a, b, and c), and Sigmoidal MF has four parameters (a1, a2, c1, and c2). These parameters are called premise parameters. Numbers of MF are varied from 2 to 4 for each input and ANFIS structures are configured from 2-2-2 configuration, which means 2 MFs for sparger diameter (Ds), axial coordination (H) and radial coordination (x), to 4-4-4 configuration.
As seen in Tables 2 and 3, the most accurate ANFIS structures in terms of RMSE and CC values are 4-4-4 configuration with Sigmoidal MF for gas hold-up, 4-4-4 configuration with bell-shaped MF for TKE and axial liquid velocity. Complexity of the model is another considerable parameter in selecting best ANFIS structure. In this aim, the total number of parameters, comprising premise and consequent parameters, is obtained for each model. This value is varied from 44 to 304 parameters.
Fig. 4, 6 and 8 portray gas hold-up, TKE and axial liquid velocity RMSE values of ANFIS structures in terms of number of parameters (premise and consequent) while Fig. 5, 7 and 9 show gas hold-up, TKE and axial liquid velocity CC values of ANFIS structures in terms of number of parameters. As seen in Fig. 4, RMSE results of gas hold-up illustrate an error reduction when the number of parameters increases. The RMSE results are distributed in two regions; high and low RMSE values. Different ANFIS configurations may have similar number of parameters which represents the complexity of the model.
As instance, ANFIS models with configuration of 2-3-4, 2-4-3, 3-2-4, 3-4-2, 4-2-3, and 4-3-2 have 114, 123, and 132 parameters for Gaussian, bell-shaped, and Sigmoidal MFs, respectively. Type of MF has a slight influence on the gas hold-up prediction accuracy of gas hold-up while the number of parameters has a key role on the model precision. ANFIS models with configurations of 2-3-4, 2-4-3, 4-2-3, and 3-2-4 are much more accurate than models with configurations of 3-4-2 and 4-3-2. This comparison shows that radial coordination (x) needs to be split into more spaces by means of more MFs for x. Hence, ANFIS model with 4-4-4 configuration and Sigmoidal MF is selected as the best model to predict gas hold-up by comparing the RMSE and CC values and the influence of the ANFIS model configuration on the prediction accuracy.
Fig. 6 depicts the relationship between TKE RMSE values of diverse ANFIS models and numbers of parameters. In contrast with error result of gas hold-up prediction, TKE RMSE results are close together and reduction rate is lesser. Thus, a simpler ANFIS structure with less number of parameters can be chosen due to its simplicity and low RMSE value. ANFIS model with configuration of 4-4-4 has 280, 292, and 304 parameters for Gaussian, bell-shaped, and Sigmoidal MFs while ANFIS model with configuration of 4-4-3 for bell-shaped MF has 225 parameters. The RMSE values of these ANFIS models are close together. Therefore, the ANFIS model with lowest number of parameters can be selected as the best model to predict TKE. Fig. 7 illustrates that the ANFIS model with configuration of 4-4-3 and bell-shaped MF has an appropriate performance in terms of CC value and is selected as the best ANFIS model for estimation of TKE.
Axial liquid velocity is another parameter that has been predicted by ANFIS method. Fig. 8 shows the RMSE values of diverse ANFIS structures versus number of parameters. As can be seen, the error result of utilizing Sigmoidal MF is higher than that of utilizing bell-shaped and Gaussian MFs. The RMSE and CC results of ANFIS model with 2-4-4 configuration and Gaussian MF are close to those of models with higher complexity such as 3-4-4 configuration with bell-shaped MF, 4-4-4 configuration with Gaussian and bell-shaped MFs (see Fig. 8 and 9). Hence, the best model in terms of both simplicity and accuracy is ANFIS model with 2-4-4 configuration and Gaussian MF to predict axial liquid velocity.
Fig. 11 shows the planer averaged gas hold-up versus bubble column heights for Grids 1 and 3 and Pfleger and Becker's investigation.13 In comparison to Pfleger and Becker's numerical study, current numerical results are in excellent agreement with experimental data, especially near the sparger. The Pfleger and Becker13 showed an overprediction for gas hold-up at various column heights (particularly near the spargers). The figure shows that, towards the sparger, the numerical study of Pfleger and Becker13 could not accurately estimate gas hold-up (over prediction), while the current CFD results are in good agreement with experimental data. In addition, the figure also illustrates that Grid 1 presents better agreement in comparison with Grid 3 in all column heights, particularly near the sparger.
![]() | ||
Fig. 11 Overall averaged gas hold up for CFD results, Grids 1, 3 and those from experiment and simulation in Pfleger and Becker at various heights. |
![]() | ||
Fig. 12 Average axial liquid velocity for CFD, Grids 1–3 and those from experiment and simulation in Pfleger and Becker at height 1.6 m. |
In general, the grid dependency test shows a good agreement when the grid size increases (coarse mesh), while the numerical results with finer mesh differ more from experimental data of Pfleger and Becker13 (see Fig. 11 and 12). Buwa et al.69 and Pfleger and Becker13 also reported that, as the grid size decreases, the agreement between numerical results of time averaged flow pattern and experimental finding deteriorates. Furthermore, Bech77 showed that transient turbulence models produce new modes of instability in the plume oscillation when the grid size decreases. Based on results of grid dependency illustrated in Fig. 11 and 12, the coarse mesh, containing 40500 grids, is used for all simulation cases in this study.
![]() | (18) |
ANFIS model has been trained by using CFD simulation results. To verify the trained model, four axial coordinates, 0.867, 1.3, 1.733 and 2.167 m, are employed to examine the prediction result. Fig. 13–15 depict both CFD simulation and ANFIS prediction results for gas hold-up, TKE and axial liquid velocity in the bubble column. These figures illustrate the high capability of ANFIS method to model the characteristics of bubbly flow.
Inside bubble column reactors, the amount of gas depends upon the regime operation (i.e., homogeneous/heterogeneous) which turn depends upon column dimensions, pressure, temperature, superficial gas velocity and sparger design parameters. Fig. 13(a)–(d) shows gas hold-up results of CFD simulation and ANFIS prediction model at various bubble column heights (0.867, 1.3, 1.73 and 2.16 m) and sparger diameters (0.08 m (Fig. 13(a)), 0.10 m (Fig. 13(b)), 0.12 m (Fig. 13(c)) and 0.14 m (Fig. 13(d)). According to this figure, both CFD and ANFIS methods show that gas bubbles tend to move towards the bubble column center due to centralized gas movement in the homogeneous regime. An increase in sparger diameter from 0.08 to 0.14 m causes a significant decrease in the magnitude of gas hold-up at the column center. Among all sparger diameters, the sparger diameter 0.14 m produces almost flatter gas hold-up profile inside the bubble column reactor. Both CFD and ANFIS methods show that the gas hold-up profile is most likely uniform near the bubble column outlet. The figures show that ANFIS prediction method can estimate gas hold-up profile almost identical with CFD method towards the column center for various sparger diameters and bubble column heights.
Another important parameter in prediction of bubble column is TKE. When bubbles travel to the column surface, the pressure energy is converted to turbulent kinetic energy. This parameter shows the intensity of turbulence inside the bubble column reactor. Fig. 14(a)–(d) compares CFD simulation and ANFIS prediction of TKE versus radial position in the column. According to the figure, TKE towards the column center is higher than other region, while near the wall region it reaches to zero due to higher fluctuations of turbulent fluid velocities at the column center. As the sparger diameter increases, TKE reduces particularly towards the column center. According to the figures, for all ring sparger diameters, TKE near the sparger region is much higher than bubble column outlet.
Axial liquid velocity is the last parameter that has been estimated by ANFIS approach. The ANFIS prediction result is compared with CFD simulation results in Fig. 15(a)–(d). As the sparger diameter rises, the liquid centerline velocity reduces and results in flatter liquid velocity profile. Additionally, the centerline liquid velocity decreases, as the column height increases. This is attributed to the fact that, near the sparger region, swarm bubbles supply higher energy to the liquid than bulk region, and resulting in higher turbulent dissipation energy. This energy transferring shows the critical bubble column location where bubble plume breaks and bubbles split to smaller bubbles (break-up). In summary, the results show that ANFIS approach beside the CFD method is a capable prediction methodology to estimate the local hydrodynamics parameters at various column locations and operation conditions.
This section provides information about 3D bubble column hydrodynamics surface plots in order to understand the flow pattern and gas dynamics throughout the bubble column for all column heights and sparger diameters. The predicted gas hold-up contour has been presented for various column heights and sparger diameters in Fig. 16. This figure shows the predicted gas hold-up for sparger diameters of 0.085 m (Fig. 16(a)), 0.115 m (Fig. 16(b)) and 0.145 m (Fig. 16(c)). According to the figure, the gas hold-up profile has a non-uniform behavior towards the sparger, while at the middle and surface region (e.g., 1.3 and 2.5 m) gas phase disperses uniformly. In general, the gas hold-up has a maximum value at the central region while the amount of gas decreases as sparger diameter increases around this region (see Fig. 16). Fig. 17 portrays the predicted axial liquid velocity in different column heights and sparger diameters. As seen, maximum liquid velocity occurs near the sparger region at almost every column height, while the liquid direction changes and results in two recirculation area near walls. Fig. 18 depicts the predicted TKE for various column heights and sparger diameters (0.085 m (Fig. 18(a)), 0.115 m (Fig. 18(b)) and 0.145 m (Fig. 18(c))). According to this figure, TKE towards the sparger is significantly higher than other regions. The figure shows that, with an increase in sparger diameter, TKE decreases.
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Fig. 16 Surface rules of selected ANFIS method in gas hold-up at sparger diameters of (a) 0.085 (b) 0.115 and (c) 0.145. |
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Fig. 17 Surface rules of selected ANFIS method in axial velocity at sparger diameters of (a) 0.085 (b) 0.115 and (c) 0.145. |
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Fig. 18 Surface rules of selected ANFIS method in turbulent kinetic energy at sparger diameters of (a) 0.085 (b) 0.115 and (c) 0.145. |
The ANFIS method can predict the BCR hydrodynamics with different operational conditions in less computational time and provide continuous results. In order to examine the prediction ability, the BCR hydrodynamics are predicted for different column heights. All predicted results are compared with CFD results which are not used in training process.
The ANFIS method is used to predict the results of ϵg at column heights (Y mesh coordinate) of 0.43, 0.86, 1.3, 1.73, 2.16 and 2.56 m. The number of prediction data in X and Z mesh coordinate is increased from 705 (CFD data) to 4800 nodes. For ANFIS training and model development, 70% of the actual data, which is the CFD results from benchmark case, at column heights of 0.217, 0.47, 0.73, 0.997, 1.3, 1.56, 1.8, 2.08, 2.3 and 2.6 m is given as an input. In addition, the number of data in X and Z mesh coordinate for the input is reduced to three quarter or to only 490 nodes. Please take note, the prediction is for the column heights that is not given as an input data to ANFIS model and hence the ability of the model is tested. Fig. 19 shows the predicted contour plot of gas hold-up at various column heights (i.e., 0.432, 0.86, 1.3, 1.73, 2.17 and 2.56 m) for ANFIS and CFD method. According to the figure, the ANFIS results are in good agreement with CFD results almost for all column heights. The ANFIS method predicts the circular gas hold-up distribution almost for all column heights, which is similar with CFD results. Both CFD and ANFIS show the higher gas hold-up at the center region of column, ranging 0.02–0.03, while this parameter reaches to zero value near the walls. Towards the sparger region (h = 0.432 m), the sparger has influence on the gas distribution, resulting ring shape gas fraction (with 0.0012 m inner and 0.09 m outer diameter). As the column height increases, this influence diminishes and results in uniform distribution of gas. In comparison to CFD results, ANFIS method slightly over predicts the gas hold-up towards the walls at 2.56 m. This may attribute to the fact that, ANFIS method cannot accurately recognize gas behaviour near the BCR boundary (particularly outlet). In order to enhance this over prediction, different ANFIS setting parameters or data filtering are required.
In summary, the combination of ANFIS and CFD prediction framework shows that, in case of a proper ANFIS learning process with CFD results, ANFIS approach can adequately predict bubble column hydrodynamics. In comparison to the CFD simulation, ANFIS approach provides the approximated bubble column hydrodynamics in a continuous domain. When the specific range of ring sparger diameters and column heights are trained in the ANFIS method, it can smartly approximate the flow pattern and gas dynamics within these particular ranges. On the other hand, in CFD simulation, the CFD simulation needs to be implemented for any changes in operation conditions due to production of discrete results. Therefore, providing a complete set of result for various conditions such as different sparger diameter requires computational efforts, resulting in large computational time.
In the last portion of this section, we propose the mathematical models of the liquid flow pattern and gas dynamics that have been estimated by selected ANFIS models. These mathematical correlations show the axial liquid velocity, gas hold-up and TKE at different column heights, radiuses and sparger diameters. The method of gaining mathematical models from ANFIS approach was described in section 2.4. The formula of the relationship between gas hold-up and effective variables, which are sparger diameter, axial coordination and radial coordination, can be written as,
![]() | (19) |
First subscription of μ shows the input number and the second subscription depicts the MF number. The values of MFs' parameters (premise parameters) are shown in Table 4. Subscription of m represents the rule number ranged from 1 to 64. Table 5 shows the values of pm, qm, rm, and sm (consequent parameters). Each MF has four parameters and linear portion of every rule has four parameters. As seen in Table 4, the values of a1 and a2 for all MFs of individual input are approximately equal.
Input | MF | a1 | c1 | a2 | c2 |
---|---|---|---|---|---|
Sparger diameter | 1 | 4.444 × 102 | 5.495 × 10−2 | 4.444 × 102 | 7.955 × 10−2 |
2 | 4.444 × 102 | 9.655 × 10−2 | 4.444 × 102 | 1.161 × 10−1 | |
3 | 4.444 × 102 | 1.067 × 10−1 | 4.444 × 102 | 1.333 × 10−1 | |
4 | 4.444 × 102 | 1.571 × 10−1 | 4.444 × 102 | 1.750 × 10−1 | |
Axial coordination | 1 | 1.538 × 10 | −4.332 × 10−1 | 1.539 × 10 | −6.853 × 10−2 |
2 | 1.539 × 10 | 1.943 × 10−1 | 1.538 × 10 | 1.286 | |
3 | 1.538 × 10 | 1.197 | 1.538 × 10 | 2.172 | |
4 | 1.538 × 10 | 2.160 | 1.538 × 10 | 3.033 | |
Radial coordination | 1 | 1.390 × 102 | −1.919 × 10−1 | 1.390 × 102 | −4.025 × 10−2 |
2 | 1.390 × 102 | −5.078 × 10−2 | 1.390 × 102 | 3.719 × 10−2 | |
3 | 1.390 × 102 | 3.270 × 10−2 | 1.390 × 102 | 6.373 × 10−2 | |
4 | 1.390 × 102 | 5.365 × 10−2 | 1.390 × 102 | 1.918 × 10−1 |
Rule | p | q | r | s | Rule | p | q | r | s |
---|---|---|---|---|---|---|---|---|---|
1 | 2.06 × 10−1 | −9.83 × 10−2 | −3.13 × 10−1 | −4.81 × 10−2 | 33 | 3.82 × 10−1 | 2.60 × 10−1 | 8.93 × 10−1 | 4.96 × 10−2 |
2 | −5.34 × 10−1 | 1.29 | −1.77 | 4.37 × 10−2 | 34 | −6.72 × 10−1 | −1.27 × 10−2 | 6.73 × 10−1 | 8.78 × 10−2 |
3 | 1.55 | 8.96 × 10−1 | −1.35 × 10 | 6.23 × 10−1 | 35 | −1.65 | 8.76 × 10−1 | 6.47 | −5.24 × 10−2 |
4 | −5.06 × 10−1 | −1.17 × 10−1 | −4.00 × 10−1 | 9.51 × 10−2 | 36 | 2.24 × 10−1 | 2.53 × 10−2 | 1.13 × 10−1 | −4.47 × 10−2 |
5 | −5.94 × 10−1 | 3.96 × 10−3 | 1.23 × 10−1 | 5.75 × 10−2 | 37 | −2.40 × 10−2 | 1.98 × 10−3 | 3.64 × 10−1 | 4.88 × 10−2 |
6 | −3.63 × 10−1 | 7.86 × 10−3 | 3.59 × 10−1 | 7.16 × 10−2 | 38 | −4.16 × 10−1 | −1.05 × 10−2 | 8.52 × 10−2 | 9.34 × 10−2 |
7 | 2.50 | 2.43 × 10−2 | 6.92 × 10−1 | −1.90 × 10−1 | 39 | 8.82 × 10−1 | 6.61 × 10−3 | 1.75 × 10−1 | −9.68 × 10−2 |
8 | −6.96 × 10−2 | 8.56 × 10−3 | −1.13 × 10−1 | 1.52 × 10−2 | 40 | −1.48 × 10−1 | 5.68 × 10−3 | −2.07 × 10−1 | 4.29 × 10−2 |
9 | −3.33 × 10−1 | 3.06 × 10−3 | 2.04 × 10−1 | 4.73 × 10−2 | 41 | −9.09 × 10−2 | 1.57 × 10−3 | 2.63 × 10−1 | 4.72 × 10−2 |
10 | 5.32 × 10−1 | −5.28 × 10−3 | 1.87 × 10−1 | 1.17 × 10−2 | 42 | −2.72 × 10−1 | −4.60 × 10−3 | 3.95 × 10−2 | 7.16 × 10−2 |
11 | 1.43 | 3.94 × 10−3 | 3.02 × 10−1 | −9.52 × 10−2 | 43 | 2.12 × 10−1 | −7.98 × 10−4 | 7.83 × 10−2 | −5.00 × 10−3 |
12 | 2.25 × 10−1 | 4.51 × 10−3 | −2.32 × 10−1 | 8.20 × 10−3 | 44 | 2.08 × 10−2 | 3.11 × 10−3 | −2.27 × 10−1 | 2.46 × 10−2 |
13 | −2.26 × 10−1 | 9.50 × 10−3 | 2.00 × 10−1 | 2.31 × 10−2 | 45 | −3.84 × 10−2 | 5.75 × 10−3 | 2.29 × 10−1 | 2.65 × 10−2 |
14 | 2.48 × 10−1 | 3.12 × 10−3 | 1.37 × 10−1 | 1.05 × 10−2 | 46 | −2.20 × 10−1 | −5.82 × 10−3 | 5.25 × 10−2 | 6.97 × 10−2 |
15 | 9.01 × 10−1 | −3.44 × 10−3 | 2.06 × 10−1 | −3.86 × 10−2 | 47 | 9.88 × 10−2 | 3.85 × 10−3 | 5.65 × 10−2 | −1.62 × 10−3 |
16 | 1.43 × 10−1 | 5.88 × 10−3 | −2.23 × 10−1 | 8.75 × 10−3 | 48 | 4.17 × 10−2 | 6.62 × 10−3 | −2.09 × 10−1 | 1.09 × 10−2 |
17 | 5.02 × 10−1 | 1.48 × 10−2 | 4.36 × 10−2 | −4.27 × 10−2 | 49 | −6.29 × 10−2 | 2.26 × 10−1 | 9.12 × 10−1 | 1.15 × 10−1 |
18 | −1.14 | 6.72 × 10−1 | −1.65 | 9.57 × 10−2 | 50 | −3.45 × 10−1 | 8.55 × 10−2 | 6.66 × 10−1 | 3.97 × 10−2 |
19 | −2.40 | 4.16 × 10−1 | −1.50 | 4.44 × 10−1 | 51 | −4.37 × 10−1 | −5.38 × 10−2 | −5.82 × 10−1 | 5.43 × 10−2 |
20 | 2.88 × 10−1 | 1.11 × 10−2 | 3.96 × 10−1 | −7.65 × 10−2 | 52 | −3.72 × 10−2 | 1.73 × 10−1 | −9.34 × 10−1 | 1.23 × 10−1 |
21 | −1.99 × 10−1 | 5.30 × 10−3 | 2.05 × 10−1 | 4.28 × 10−2 | 53 | 1.17 × 10−2 | 5.71 × 10−3 | 3.95 × 10−1 | 4.61 × 10−2 |
22 | −6.42 × 10−1 | −4.30 × 10−3 | 1.13 × 10−1 | 1.10 × 10−1 | 54 | −5.77 × 10−1 | −1.10 × 10−2 | −1.41 × 10−1 | 1.14 × 10−1 |
23 | 9.91 × 10−1 | 6.76 × 10−3 | 7.56 × 10−1 | −1.05 × 10−1 | 55 | −1.13 | −3.36 × 10−3 | −2.71 × 10−2 | 2.05 × 10−1 |
24 | 6.10 × 10−3 | 7.05 × 10−4 | −1.77 × 10−1 | 2.19 × 10−2 | 56 | 3.13 × 10−1 | 6.17 × 10−4 | −3.96 × 10−1 | 3.84 × 10−3 |
25 | −2.00 × 10−1 | 2.86 × 10−3 | 2.33 × 10−1 | 4.68 × 10−2 | 57 | 6.16 × 10−2 | 2.01 × 10−3 | 2.95 × 10−1 | 3.02 × 10−2 |
26 | −1.51 × 10−1 | −6.19 × 10−3 | 6.05 × 10−2 | 6.00 × 10−2 | 58 | −3.37 × 10−1 | −2.57 × 10−3 | −4.69 × 10−2 | 7.39 × 10−2 |
27 | 4.69 × 10−1 | −2.02 × 10−4 | 1.72 × 10−1 | −2.64 × 10−2 | 59 | −2.38 × 10−1 | −3.14 × 10−3 | −1.39 × 10−1 | 7.15 × 10−2 |
28 | 8.65 × 10−2 | 1.51 × 10−3 | −2.22 × 10−1 | 2.04 × 10−2 | 60 | 1.64 × 10−1 | 1.06 × 10−3 | −2.82 × 10−1 | 1.50 × 10−2 |
29 | −1.21 × 10−1 | 6.74 × 10−3 | 2.17 × 10−1 | 2.77 × 10−2 | 61 | 6.03 × 10−2 | 5.18 × 10−3 | 2.35 × 10−1 | 1.60 × 10−2 |
30 | −1.56 × 10−1 | 1.43 × 10−3 | 5.58 × 10−2 | 4.38 × 10−2 | 62 | −2.50 × 10−1 | −6.52 × 10−3 | −2.41 × 10−2 | 7.24 × 10−2 |
31 | 2.01 × 10−1 | 5.99 × 10−3 | 1.40 × 10−1 | −1.50 × 10−2 | 63 | −1.22 × 10−1 | −5.83 × 10−3 | −1.27 × 10−1 | 5.98 × 10−2 |
32 | 4.97 × 10−2 | 4.99 × 10−3 | −2.05 × 10−1 | 1.43 × 10−2 | 64 | 1.08 × 10−1 | 4.57 × 10−3 | −2.37 × 10−1 | 1.05 × 10−2 |
ANFIS model with 4-4-3 configuration and bell-shaped MF is select among 81 ANFIS structures for prediction of turbulent kinetic energy. This model can be represented mathematically as,
![]() | (20) |
Table 6 depicts premise parameters and illustrates that the values of b for all MFs are pretty close to each other while a and c values are different. Forty-eight rules were constructed on the basis of the selected ANFIS structure and the values of pm, qm, rm, and sm parameters in these rules are portrayed in Table 7.
Input | MF | a | b | c |
---|---|---|---|---|
Sparger diameter | 1 | 3.393 × 10−3 | 2.000 | 8.292 × 10−2 |
2 | 6.082 × 10−3 | 2.001 | 1.227 × 10−1 | |
3 | 1.200 × 10−2 | 2.000 | 1.804 × 10−1 | |
4 | 3.643 × 10−3 | 2.000 | 1.551 × 10−1 | |
Axial coordination | 1 | 4.189 × 10−1 | 1.996 | −2.915 × 10−2 |
2 | 4.684 × 10−1 | 2.001 | 8.275 × 10−1 | |
3 | 4.452 × 10−1 | 2.000 | 1.731 | |
4 | 4.316 × 10−1 | 2.000 | 2.604 | |
Radial coordination | 1 | 1.028 × 10−1 | 2.000 | −1.210 × 10−1 |
2 | 1.036 × 10−1 | 1.999 | 9.861 × 10−3 | |
3 | 1.078 × 10−1 | 1.999 | 1.299 × 10−1 |
Rule | p | q | r | s | Rule | p | q | r | s |
---|---|---|---|---|---|---|---|---|---|
1 | 2.80 × 10−1 | −1.33 × 10−2 | 6.51 × 10−2 | −1.84 × 10−2 | 25 | −1.19 | −1.45 × 10−1 | −7.61 × 10−1 | 5.80 × 10−2 |
2 | −4.17 × 10−1 | 1.94 × 10−1 | −1.85 × 10−1 | 2.40 × 10−2 | 26 | 2.03 | 7.35 × 10−2 | −6.50 × 10−1 | −2.77 × 10−1 |
3 | 1.07 × 10−1 | −4.24 × 10−2 | −2.82 × 10−1 | 4.06 × 10−2 | 27 | −8.98 × 10−1 | 6.99 × 10−2 | −7.17 × 10−1 | 2.47 × 10−1 |
4 | 1.60 × 10−1 | 2.09 × 10−4 | 6.26 × 10−1 | 8.82 × 10−2 | 28 | −1.18 | −2.83 × 10−3 | −1.10 × 10−1 | 1.56 × 10−1 |
5 | −8.39 × 10−2 | 2.38 × 10−3 | 3.88 × 10−1 | 4.28 × 10−4 | 29 | −2.52 | 1.10 × 10−2 | −1.51 × 10−1 | 3.12 × 10−1 |
6 | −1.53 × 10−1 | −5.04 × 10−3 | −2.20 × 10−1 | 3.61 × 10−2 | 30 | 1.79 | −7.02 × 10−3 | −1.02 | −8.78 × 10−2 |
7 | 7.07 × 10−2 | −1.14 × 10−3 | 5.45 × 10−1 | 8.36 × 10−2 | 31 | −1.05 × 10−1 | 2.31 × 10−3 | 1.94 × 10−1 | 5.19 × 10−2 |
8 | 2.65 × 10−1 | 2.77 × 10−3 | 2.38 × 10−1 | −3.78 × 10−2 | 32 | −3.10 | 1.05 × 10−2 | 4.82 × 10−1 | 4.13 × 10−1 |
9 | −2.50 × 10−1 | −4.47 × 10−3 | −2.82 × 10−1 | 6.38 × 10−2 | 33 | 1.11 | −1.03 × 10−2 | −2.47 × 10−1 | −1.15 × 10−1 |
10 | −1.36 × 10−2 | −6.68 × 10−4 | 3.57 × 10−1 | 6.19 × 10−2 | 34 | 1.80 × 10−1 | 1.41 × 10−2 | 1.36 × 10−1 | −3.22 × 10−2 |
11 | −2.73 × 10−2 | −1.92 × 10−3 | 1.88 × 10−1 | 3.26 × 10−3 | 35 | −6.42 × 10−1 | 1.17 × 10−2 | 1.98 × 10−1 | 6.21 × 10−2 |
12 | −5.67 × 10−2 | 7.82 × 10−3 | −1.84 × 10−1 | 7.49 × 10−3 | 36 | 8.92 × 10−2 | −2.20 × 10−2 | −1.53 × 10−1 | 5.87 × 10−2 |
13 | 1.78 × 10−1 | 6.15 × 10−3 | 3.50 × 10−1 | 3.15 × 10−2 | 37 | 8.98 × 10−1 | 5.27 × 10−2 | 6.83 × 10−1 | −3.04 × 10−2 |
14 | −7.65 × 10−2 | 1.20 × 10−1 | 1.18 × 10−1 | −1.25 × 10−2 | 38 | −1.75 | 5.31 × 10−2 | 3.79 × 10−1 | 2.31 × 10−1 |
15 | 3.50 × 10−2 | −1.32 × 10−2 | −2.33 × 10−1 | 2.75 × 10−2 | 39 | 1.27 | −1.36 × 10−2 | −1.27 × 10−1 | −1.84 × 10−1 |
16 | 1.65 × 10−1 | −1.60 × 10−3 | 7.61 × 10−1 | 1.04 × 10−1 | 40 | 9.84 × 10−1 | −4.15 × 10−3 | 9.44 × 10−1 | 1.32 × 10−2 |
17 | −2.55 × 10−1 | 3.30 × 10−3 | 3.92 × 10−1 | −3.91 × 10−4 | 41 | 1.59 | 3.29 × 10−3 | 5.41 × 10−1 | −2.92 × 10−1 |
18 | 9.51 × 10−3 | −3.17 × 10−3 | −3.84 × 10−1 | 4.86 × 10−2 | 42 | −1.44 | −9.89 × 10−3 | −3.76 × 10−1 | 2.67 × 10−1 |
19 | 7.87 × 10−2 | −1.26 × 10−3 | 5.14 × 10−1 | 7.51 × 10−2 | 43 | 9.84 × 10−2 | −3.64 × 10−3 | 4.83 × 10−1 | 7.11 × 10−2 |
20 | −1.78 × 10−1 | −2.31 × 10−3 | 1.73 × 10−1 | 3.81 × 10−3 | 44 | 2.00 | 9.41 × 10−4 | 1.84 × 10−1 | −3.23 × 10−1 |
21 | −6.91 × 10−2 | −6.62 × 10−4 | −3.70 × 10−1 | 6.18 × 10−2 | 45 | −9.52 × 10−1 | −4.91 × 10−3 | −2.55 × 10−1 | 1.87 × 10−1 |
22 | 2.01 × 10−2 | −2.73 × 10−3 | 3.56 × 10−1 | 6.24 × 10−2 | 46 | −3.14 × 10−1 | −1.11 × 10−2 | 3.23 × 10−1 | 1.28 × 10−1 |
23 | −2.22 × 10−1 | −1.68 × 10−3 | 1.36 × 10−1 | 1.70 × 10−2 | 47 | 1.22 × 10−1 | 9.00 × 10−3 | 1.33 × 10−1 | −5.63 × 10−2 |
24 | 3.18 × 10−2 | −1.55 × 10−3 | −2.62 × 10−1 | 3.70 × 10−2 | 48 | 6.67 × 10−2 | −5.35 × 10−3 | −1.83 × 10−1 | 2.88 × 10−2 |
Axial liquid velocity is another element predicted by ANFIS approach. The selected ANFIS model to estimate the axial liquid velocity has the highest simplicity among chosen ANFIS models for prediction of gas hold-up and TKE. The equation of this model as follows:
![]() | (21) |
The values of premise and consequent parameters for TKE are shown in Tables 6 and 7. Overall, there are 20 premise parameters and 128 consequent parameters that have been refined by using CFD simulation axial liquid velocity results (Tables 8 and 9). Providing these types of mathematical models assists in improving the knowledge of flow pattern (flow field) and gas dynamics for various operation conditions. In addition, this model can predict much smarter when the number of trained data increases as input parameters (i.e., bubble column dimension in X, Y and Z direction, superficial gas velocity, gas and liquid properties).
Input | MF | σ | c |
---|---|---|---|
Sparger diameter | 1 | 3.107 × 10−2 | 8.611 × 10−2 |
2 | 1.996 × 10−2 | 1.526 × 10−1 | |
Axial coordination | 1 | 2.215 × 10−1 | −1.589 × 10−1 |
2 | 4.978 × 10−1 | 8.053 × 10−1 | |
3 | 4.685 × 10−1 | 1.798 | |
4 | 9.646 × 10−2 | 2.793 | |
Radial coordination | 1 | 5.538 × 10−3 | −1.434 × 10−1 |
2 | 8.356 × 10−2 | −7.177 × 10−2 | |
3 | 6.069 × 10−2 | 4.728 × 10−2 | |
4 | 9.647 × 10−2 | 3.347 × 10−1 |
Rule | p | q | r | s | Rule | p | q | r | s |
---|---|---|---|---|---|---|---|---|---|
1 | 7.86 × 10−1 | −2.80 × 10−2 | 5.72 | 7.48 × 10−1 | 17 | 4.05 | −2.13 × 10−1 | −7.61 | −1.70 |
2 | −1.31 | −2.58 × 10−2 | −9.81 × 10−1 | −1.61 × 10−2 | 18 | −6.29 | 2.47 × 10−1 | 1.38 × 10−1 | 9.77 × 10−1 |
3 | 5.63 × 10−1 | 3.97 × 10−1 | −1.06 | 2.45 × 10−2 | 19 | 6.33 | 1.36 × 10−3 | 8.17 × 10−1 | −1.04 |
4 | 1.44 | −1.61 | −1.14 × 10 | 1.80 | 20 | −3.41 | −2.88 × 10−1 | −2.54 | 8.45 × 10−1 |
5 | 5.01 × 10−2 | −1.27 × 10−2 | −5.08 | −6.45 × 10−1 | 21 | 1.01 | −8.13 × 10−3 | −4.67 | −6.91 × 10−1 |
6 | −3.00 × 10−2 | 1.28 × 10−2 | 1.71 | 1.16 × 10−1 | 22 | −1.41 | 1.74 × 10−2 | 4.10 | 6.10 × 10−1 |
7 | 1.17 × 10−1 | 7.43 × 10−3 | −2.49 | 2.31 × 10−1 | 23 | 1.46 | −2.23 × 10−3 | 2.36 | −3.01 × 10−1 |
8 | 1.71 | −7.45 × 10−2 | 2.01 × 10 | −2.85 | 24 | 2.63 | 1.01 × 10−1 | 7.99 × 10 | −1.27 × 10 |
9 | −6.69 × 10−2 | −7.13 × 10−3 | −1.14 × 10 | −1.54 | 25 | 5.03 × 10−1 | −1.76 × 10−3 | −1.08 × 10 | −1.53 |
10 | 1.34 × 10−1 | 6.32 × 10−3 | 1.89 | 1.33 × 10−1 | 26 | −6.83 × 10−1 | 5.31 × 10−3 | 2.87 | 3.74 × 10−1 |
11 | −1.31 × 10−1 | −3.75 × 10−3 | −1.18 | 1.71 × 10−1 | 27 | 5.11 × 10−1 | 3.22 × 10−3 | 1.15 | −9.72 × 10−2 |
12 | 1.13 | −2.02 × 10−2 | 2.77 × 10 | −4.11 | 28 | 2.05 | 4.98 × 10−2 | 5.42 × 10 | −8.72 |
13 | 3.08 × 10−1 | 1.54 | 6.78 | −3.15 | 29 | −1.40 | 5.06 × 10−1 | 7.71 | −1.30 × 10−1 |
14 | −1.05 × 10−1 | −1.78 | −2.62 | 4.44 | 30 | 1.50 | −4.56 × 10−1 | −3.53 | 6.58 × 10−1 |
15 | −1.95 × 10−1 | −2.42 | 2.93 | 6.00 | 31 | −2.47 | 1.35 × 10−1 | 2.20 | −1.69 × 10−1 |
16 | −4.68 × 10−1 | 1.01 × 10 | −2.75 × 10 | −2.23 × 10 | 32 | −1.12 | −6.44 × 10−1 | −3.55 × 10 | 6.94 |
• Both CFD and ANFIS prediction method show that the axial liquid velocity, turbulent kinetic energy and gas hold-up rise towards the column centre, while these parameters reach to zero value near the column walls for various gas sparger diameters and bubble column heights. The larger ring sparger diameter produces flatter gas hold-up profile in the bubble column cross-section. In addition, for all sparger diameters, the centreline velocity, gas hold-up and turbulent kinetic energy are higher near the sparger region.
• ANFIS approach can predict the bubble column hydrodynamics in a very short time and provide a non-discrete result, while the CFD simulation needs to be employed for any changes in operation condition.
• Evaluation of different ANFIS structures illustrates that the type and number of membership function significantly affect the precision of the prediction model.
• The ANFIS method contains a good ability to predict hydrodynamics parameters of bubble column reactor which are not used in the training process. This will show that, this method can be used as assistance tools together with CFD methodology to predict parameters and minimize computational efforts, and numerical repetition.
CD | Drag force coefficient (−) |
CTD | Turbulent dispersion coefficient (−) |
Cε1 | Model parameter in turbulent dissipation energy equation (−) |
Cε2 | Model parameter in turbulent dissipation energy equation (−) |
Cμ | Constant in k–ε model (−) |
Cμ,BI | Constant in bubble induced turbulence model (−) |
dB | Bubble diameter (m) |
d0 | Sparger hole diameter (m) |
D | Diameter of the column (m) |
Ds | Sparger diameter (m) |
g | Gravitational constant (m s−2) |
G | Generation term (kg m−1 s−2) |
H | Height (m) |
k | Turbulent kinetic energy per unit mass (m2 s−2) |
MI | Total interfacial force acting between two phases (N m−3) |
MD | Drag force (N m−3) |
P | Pressure (N m−2) |
r | Radial distance (m) |
R | Column radius (m) |
ReB | Reynolds number (= dBVS/v) (−) |
VG | Superficial gas velocity (m s−1) |
Vy | Axial liquid velocity (m s−1) |
TKE | Turbulent kinetic energy |
MF | Membership function |
RMSE | Root mean square error |
ε | Turbulent energy dissipation rate per unit mass (m2 s−3) |
∈ | Fractional phase hold-up (−) |
∈ | Average fractional phase hold-up (−) |
μ | Molecular viscosity (Pa s) |
μBI | Bubble induced viscosity (Pa s) |
μeff | Effective viscosity (Pa s) |
ρ | Density (kg m−3) |
μT | Turbulent viscosity (Pa s) |
σ | Surface tension (N m−1) |
σε | Prandtl number for turbulent energy dissipation rate (−) |
σk | Prandtl number for turbulent kinetic energy (−) |
τk | Shear stress of phase k (Pa) |
εg | Air fraction/Gas hold-up |
G | Gas phase |
L | Liquid phase |
This journal is © The Royal Society of Chemistry 2015 |