Turbulence modeling is a crucial aspect of simulating complex fluid flows in engineering applications. It tackles the challenges of predicting chaotic, unsteady behavior across multiple scales, from large eddies to small-scale structures.
Various approaches exist, including Reynolds-averaged Navier-Stokes (RANS) models, large eddy simulation (LES), and direct numerical simulation (DNS). Each method balances accuracy and computational cost, aiming to capture turbulent flow dynamics efficiently for practical applications.
Turbulence modeling overview
Turbulence modeling plays a crucial role in simulating and understanding complex fluid flows encountered in various engineering applications (aerospace, automotive, energy systems)
Turbulent flows exhibit chaotic, unsteady, and multiscale behavior, making them challenging to predict and control
Characteristics of turbulent flows
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Top images from around the web for Characteristics of turbulent flows
HESS - Turbulent mixing and heat fluxes under lake ice: the role of seiche oscillations View original
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Fluid Dynamics – University Physics Volume 1 View original
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HESS - Turbulent mixing and heat fluxes under lake ice: the role of seiche oscillations View original
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Turbulent flows are characterized by irregular velocity fluctuations, enhanced mixing, and increased dissipation of energy
Exhibit a wide range of spatial and temporal scales, from large eddies to small-scale turbulent structures (Kolmogorov scales)
Display high sensitivity to initial and boundary conditions, leading to chaotic behavior and limited predictability
Challenges in turbulence modeling
Capturing the complex, multiscale nature of turbulent flows requires sophisticated mathematical and computational models
Direct numerical simulation (DNS) of turbulent flows is computationally expensive, often prohibitive for high Reynolds number flows
Turbulence models aim to provide accurate and efficient approximations of turbulent flow behavior while reducing computational costs
Reynolds-averaged Navier-Stokes (RANS) models
RANS models are based on the concept of decomposing flow variables into mean and fluctuating components
Introduce additional terms in the governing equations, representing the effects of turbulent fluctuations on the mean flow
Concept of Reynolds averaging
Reynolds averaging involves decomposing flow variables (velocity, pressure) into mean and fluctuating components
Resulting in the Reynolds-averaged Navier-Stokes (RANS) equations, which govern the mean flow behavior
Introduces the Reynolds stress tensor, representing the effects of turbulent fluctuations on the mean flow
Boussinesq eddy-viscosity hypothesis
The Boussinesq hypothesis relates the Reynolds stress tensor to the mean strain rate tensor through an eddy viscosity
Assumes that the effect of turbulence can be modeled as an increased viscosity, known as the turbulent or eddy viscosity
Simplifies the closure problem by reducing the number of unknown terms in the RANS equations
Zero-equation models
Zero-equation models, such as the mixing length model, estimate the eddy viscosity based on algebraic expressions
Rely on empirical relations and do not involve additional transport equations for turbulence quantities
Suitable for simple flows but have limited accuracy and generality
One-equation models
One-equation models, such as the Spalart-Allmaras model, solve a transport equation for a turbulence quantity (turbulent kinetic energy or eddy viscosity)
Provide improved accuracy compared to zero-equation models by accounting for the transport and history effects of turbulence
Widely used in aerospace applications due to their robustness and computational efficiency
Two-equation models
Two-equation models, such as the k-epsilon and k-omega models, solve transport equations for two turbulence quantities (turbulent kinetic energy and dissipation or specific dissipation rate)
Offer a balance between accuracy and computational cost, making them popular in industrial applications
k-epsilon model
The k-epsilon model solves transport equations for the turbulent kinetic energy (k) and its dissipation rate (epsilon)
Robust and widely used in various engineering applications due to its simplicity and numerical stability
Performs well for free-shear flows but has limitations in predicting near-wall behavior and adverse pressure gradients
k-omega model
The k-omega model solves transport equations for the turbulent kinetic energy (k) and the specific dissipation rate (omega)
Provides improved near-wall treatment compared to the k-epsilon model, making it suitable for wall-bounded flows
Sensitive to freestream turbulence levels and requires careful treatment of boundary conditions
SST model
The Shear Stress Transport (SST) model combines the advantages of the k-epsilon and k-omega models
Employs a blending function to switch between the k-omega model near the wall and the k-epsilon model in the freestream
Offers improved predictions of flow separation and adverse pressure gradients compared to the standard k-epsilon and k-omega models
Reynolds stress models
Reynolds stress models (RSM) solve transport equations for each component of the Reynolds stress tensor
Capture the anisotropic nature of turbulence and provide more accurate predictions for complex flows (swirling, rotating, or strongly separated flows)
Computationally expensive compared to eddy-viscosity models due to the increased number of equations solved
Large eddy simulation (LES)
LES is a turbulence modeling approach that directly resolves large-scale turbulent structures while modeling the effects of small-scale structures
Applies a spatial filtering operation to the Navier-Stokes equations, separating resolved and subgrid-scale (SGS) motions
Concept of spatial filtering
Spatial filtering in LES decomposes the flow field into resolved (large-scale) and subgrid-scale (small-scale) components
The resolved scales are directly computed, while the effects of the subgrid scales are modeled using SGS models
Filtering operation is typically based on the grid resolution, with the filter width related to the grid size
Subgrid-scale (SGS) modeling
SGS models aim to represent the effects of the unresolved, small-scale turbulent structures on the resolved flow
Account for the energy transfer between the resolved and subgrid scales and the dissipation of energy at small scales
Commonly used SGS models include the Smagorinsky model, dynamic models, and scale-similarity models
Smagorinsky model
The Smagorinsky model is a simple and widely used SGS model in LES
Relates the SGS stresses to the resolved strain rate tensor through an eddy-viscosity assumption
Employs a constant model coefficient, which requires calibration and can lead to excessive dissipation in certain flow regions
Dynamic SGS models
Dynamic SGS models, such as the dynamic Smagorinsky model, dynamically compute the model coefficients based on the resolved flow information
Adapt the model coefficients to the local flow conditions, reducing the need for a priori calibration
Provide improved predictions compared to the standard Smagorinsky model, especially in transitional and wall-bounded flows
Direct numerical simulation (DNS)
DNS involves directly solving the Navier-Stokes equations without any turbulence modeling assumptions
Resolves all spatial and temporal scales of turbulence, from the largest eddies to the Kolmogorov scales
Concept of DNS
DNS captures the full spectrum of turbulent motions by resolving all relevant scales
Requires extremely fine spatial and temporal resolution to accurately represent the smallest turbulent structures
Provides detailed information about turbulence dynamics, energy transfer, and dissipation mechanisms
Computational requirements for DNS
DNS is computationally expensive due to the high resolution required to capture all turbulent scales
Computational cost scales with the Reynolds number, making DNS feasible only for low to moderate Reynolds number flows
Requires massive computational resources and parallel computing techniques for large-scale simulations
Applications of DNS
DNS is primarily used for fundamental research and understanding of turbulence physics
Provides benchmark data for validating and improving turbulence models and numerical methods
Offers insights into complex flow phenomena, such as transition to turbulence, turbulent mixing, and heat transfer
Hybrid RANS-LES methods
Hybrid RANS-LES methods combine the advantages of RANS models and LES to efficiently simulate complex turbulent flows
Employ RANS modeling in near-wall regions and LES in detached or separated flow regions
Detached eddy simulation (DES)
DES is a hybrid RANS-LES approach that switches between RANS and LES based on a model-specific criterion
Uses RANS modeling in attached boundary layers and LES in detached or separated flow regions
Provides a computationally efficient alternative to full LES while capturing important unsteady flow features
Delayed detached eddy simulation (DDES)
DDES is an improved version of DES that addresses the issue of grid-induced separation in the original DES formulation
Employs a shielding function to delay the switch from RANS to LES, preventing premature activation of LES in attached boundary layers
Offers better control over the RANS-LES transition and improved predictions of flow separation
Improved delayed detached eddy simulation (IDDES)
IDDES further enhances the DDES formulation by combining the advantages of DDES and wall-modeled LES (WMLES)
Includes a modified subgrid length scale definition and a blending function for smooth transition between RANS and LES
Provides improved predictions of complex flows with both attached and separated regions, such as high-lift configurations and aeroacoustics
Wall modeling for LES
Wall modeling in LES aims to reduce the computational cost associated with resolving the near-wall turbulent structures
Allows for coarser grid resolution near the walls while still capturing the essential flow physics
Importance of near-wall resolution
Near-wall turbulent structures play a crucial role in determining wall shear stress, heat transfer, and flow separation
Resolving the near-wall region in LES requires extremely fine grid resolution, leading to high computational costs
Wall modeling approaches aim to relax the near-wall resolution requirements while maintaining accuracy
Wall functions
Wall functions are algebraic models that relate the near-wall velocity to the wall shear stress using empirical laws (logarithmic law of the wall)
Provide a computationally efficient way to represent the near-wall flow behavior without resolving the viscous sublayer
Suitable for high Reynolds number flows with attached boundary layers but have limitations in predicting flow separation and heat transfer
Two-layer models
Two-layer models divide the near-wall region into a viscous sublayer and a logarithmic layer
Employ simplified RANS-like equations in the viscous sublayer and LES in the outer layer
Provide improved predictions compared to wall functions by capturing the essential near-wall physics
Require additional grid resolution compared to wall functions but still offer significant computational savings compared to fully-resolved LES
Turbulence model validation
Validation of turbulence models is essential to assess their accuracy, reliability, and range of applicability
Involves comparing model predictions with experimental data or high-fidelity simulations (DNS or resolved LES)
Benchmark test cases
Benchmark test cases are well-documented experimental or numerical datasets that serve as reference for turbulence model validation
Cover a range of flow configurations, such as channel flows, boundary layers, jets, wakes, and separated flows
Provide detailed measurements of velocity fields, Reynolds stresses, and other turbulence statistics
Comparison with experimental data
Comparing turbulence model predictions with experimental data is a critical step in model validation
Experimental data can include mean velocity profiles, turbulence intensities, Reynolds stresses, and flow visualizations
Assesses the ability of turbulence models to capture key flow features and turbulence characteristics
Uncertainty quantification in turbulence modeling
Uncertainty quantification (UQ) aims to quantify the impact of model assumptions, input uncertainties, and numerical errors on the simulation results
Employs techniques such as sensitivity analysis, Bayesian inference, and stochastic collocation methods
Provides a framework for assessing the reliability and robustness of turbulence model predictions and guiding model improvement efforts
Turbulence modeling in complex geometries
Turbulence modeling in complex geometries poses additional challenges related to mesh generation and near-wall treatment
Requires careful consideration of grid resolution, quality, and adaptivity to accurately capture the flow physics
Challenges in mesh generation
Complex geometries often involve irregular shapes, sharp edges, and small-scale features that require special attention during mesh generation
Ensuring adequate grid resolution in critical flow regions while maintaining computational efficiency is a key challenge
Unstructured or hybrid grids are commonly used to handle complex geometries, but they can introduce numerical errors and increase computational costs
Near-wall treatment
Near-wall treatment in complex geometries is crucial for accurate prediction of wall shear stress, heat transfer, and flow separation
Requires careful grid design to capture the steep gradients and anisotropic turbulence in the near-wall region
Wall functions and two-layer models need to be adapted to handle non-planar or curved walls and to account for the local flow conditions
Adaptive mesh refinement
Adaptive mesh refinement (AMR) is a technique that dynamically adapts the grid resolution based on the local flow features and turbulence characteristics
Allows for efficient use of computational resources by refining the mesh in regions of interest while coarsening it in less critical areas
Helps capture the multiscale nature of turbulence and improves the accuracy of turbulence model predictions in complex geometries
Future trends in turbulence modeling
Turbulence modeling continues to evolve, driven by advances in computational resources, numerical methods, and data-driven approaches
Emerging trends aim to improve the accuracy, efficiency, and generality of turbulence models
Machine learning-based models
Machine learning (ML) techniques, such as neural networks and Gaussian processes, are being explored for turbulence modeling
ML-based models can learn complex relationships between flow variables and turbulence quantities from high-fidelity simulation data or experimental measurements
Offer the potential for improved accuracy and reduced computational cost compared to traditional physics-based models
Data-driven modeling approaches
Data-driven modeling approaches leverage large datasets from high-fidelity simulations or experiments to inform turbulence model development
Employ techniques such as dimensionality reduction, sparse regression, and Bayesian inference to extract relevant turbulence features and model coefficients
Aim to develop turbulence models that are tailored to specific flow configurations or operating conditions, improving their predictive capabilities
Multiscale modeling strategies
Multiscale modeling strategies aim to bridge the gap between different levels of turbulence modeling (DNS, LES, RANS) and capture the multiscale nature of turbulence
Employ techniques such as hybrid RANS-LES methods, scale-resolving simulations, and concurrent multiscale approaches
Allow for efficient simulation of complex turbulent flows by combining the strengths of different modeling approaches and resolving the relevant scales of turbulence