OLAS Axexo2 Teoria Flujos
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Transcript of OLAS Axexo2 Teoria Flujos
Computational
analysis of
viscous effects
on submerged
bodies
Julen García Ibáñez
1. INTRODUCTION
2. STATE OF ART
3. CONCEPTUAL OVERVIEW
1. INTRODUCTION
Aim of work
Objectives
AIM OF WORK
“The aim of this work is the
development of methodologies for
an efficient simulation of flow
around bodies with different
turbulence models, applying
comparative studies between
numerical and experimental
results.”
OBJECTIVES
Analyze the flow around a circular cylinder, and the effect
of variations of the Reynolds number on it
Obtain force coefficients and velocity vector fields of the
flow
Simulate vortex shedding phenomenon in turbulent
situations: von Kármán Vortex street
Study and compare the different turbulence models
Apply grid convergence theory to validate computational
results
Objectives
2. STATE OF ART
Overview Navier-Stokes equations
Computational Fluid Dynamics
Discretisation
Direct Numerical Simulation
Turbulence models Reynolds Averaged Navier-Stokes
Large Eddy Simulations (LES)
Dettached Eddy Simulations (DES)
OVERVIEW
Navier-Stokes equations
Computational Fluid Dynamics
Discretisation
Direct Numerical Simulation
Navier-Stokes equations
Set of partial differential equations (PDE)
Conservation of mass:
A) Continuity equation
Newton’s Second Law of Motion:
B) Momentum equation
First law of Thermodynamics:
C) Conservation of energy
Allow obtaining the pressure and velocity of the fluid
throughout the flow
Navier-Stokes equations
A) Continuity equation:
B) Momentum equation
Navier-Stokes equations
C) Conservation of energy
Computational Fluid Dynamics
Solves Navier-Stokes equations numerically
Three main elements:
A) Pre-processor
B) Solver
C) Post-processor
CFD allows the study of complex flow fluid and has
become a key part of nowadays engineering
researching projects
Computational Fluid Dynamics
A) Pre-processor
The real problem is defined in a suitable form for
the use of the software
The computational domain is created as a big
number of discrete elements that set up the mesh
Properties of the fluid and boundary conditions
need to be defined
Computational Fluid Dynamics
B) Solver
The governing equations are solved using the
information given in the pre-processing stage
By succesive iterations the solution is derived
Convergence is a key part to ensure the wellness
of the solutions
Residuals need to be as small as possible
Computational Fluid Dynamics
C) Post-processor
It is used to analyze the results given by the
solver
Actual CFD packages provide vector and contour
plots to display the properties of the flow as
velocity, pressure, vorticity, viscosity…
Furthermore, specific reports can be presented by
mixing data like force & lift coefficients in specific
places
Discretisation
The real surface cannot be analyzed by the CFD
Thus, a set of some regularly and irregularly spaced
nodes needs to be generated: the mesh
The mesh breaks up the domain, in order to allow
time dependant calculations to be made
The discretisation is divided into:
A) Equation discretisation
B) Spatial discretisation
C) Temporal discretisation
Discretisation
A) Equation discretisation
The translation of the governing equations into a
numerical modelisation that can be solved by the
computer
Can be achieved by Finite Difference Method
(FDM), Finite Element Method (FEM), Finite
Volume Method (FVM)
The analysis of this document uses FVM
Discretisation
A) Equation discretisation
In FVM, the domain is separated into a finite
number of elements: control volumes
The Navier-Stokes equations are solved
iteratively on each control volume
The integration of the results of the algebraic
equations for each control volume derive the flow
It’s efficiency makes FVM standard in CFD codes
Discretisation
B) Spatial discretisation
The division of the computational domain into
small sub-domains that put together the mesh
Structured, unstructured and multi-block
structured mesh can be created
Unstructuration and multi-blocking allow a more
efficient use of the elements and higher
adaptability to complex geometries
Discretisation
C) Temporal discretisation
The splitting of the time in the continuous flow into
discrete time steps
In time-dependent situations, the PDE need
either an implicit or explicit solving method
Explicit methods are straight forward, but small
time-steps are needed to obtain convergence.
Implicit ones, even if require more computational
time, have a bigger range of stability
Direct Numerical Simulation
DNS involves the direct solving of Navier-Stokes
equations, without any approximation
All scales of motion are solved, even down to
Kolmogorv scales, where energy dissipation
happens
It’s computational cost is unaffordable
Spalart estimates that nearly a century would be
needed for DNS to be interesting for enegineering
TURBULENCE MODELS
Reynolds Averaged Navier-Stokes
Large Eddy Simulations
Dettached Eddy Simulations
Reynolds Averaged Navier-Stokes
In RANS, the flow is separated into mean and
fluctuating components
Time-averaged Navier-Stokes equations are obtained
Reynolds Averaged Navier-Stokes
Reynolds stress: correlation between the fluctuating
velocity components
RANS models have been developed based on the
concept that a velocity scale and a length scale is
sufficient to describe the effects of turbulence in a flow
Reynolds Averaged Navier-Stokes
A) k-ε TURBULENCE MODEL
Solves the flow assuming that the rate of
production and dissipation of turbulence are in
near-balance in energy transfer
The dissipation rate, ε of the energy, is:
where k is the kinetic energy of the flow and
L is the length scale involved
Reynolds Averaged Navier-Stokes
A) k-ε TURBULENCE MODEL
Advantages:
• Robustness of the formulation
• A very used and proven model
• Low computational cost
Disadvantages:
• Turbulence over-prediction at the stagnation
point
• Too large length scales
• Fails in the solving of flows with large strains
Reynolds Averaged Navier-Stokes
B) k-ω TURBULENCE MODEL (Reynolds Stress Model)
Uses similar mathematics to the k-ε turbulence
model
Substitutes the energy dissipation rate, ε,
by the energy dissipation rate per unit of kinetic energy, ω
Reynolds Averaged Navier-Stokes
B) k-ω TURBULENCE MODEL (Reynolds Stress Model)
Advantages:
• Simple and robust sub layer analysis
• No need of additional damping functions to
solve ω equation
Disadvantages:
• Inaccurate prediction of eddy viscosity values
• Higher computational power than k-ε
Reynolds Averaged Navier-Stokes
C) Shear Stress Transport (SST) TURBULENCE MODEL
Tries to overcome the problems of k-ε and k-ω
turbulence models
Uses k-ω near the wall to reduce the over-
prediction of length scales
Uses near the boundary layer edge to overcome
the problem of free-stream dependancy
The application is restricted to periodical flows
Large Eddy Simulation (LES)
Computes directly the large-scale turbulent structures
responsible for the transfer of energy and momentum
in a flow (large scale eddies)
Models the smaller scale of dissipative and isotropic
structures (small scale eddies)
A filter function is used to dictate which eddies are of
large scale and which ones are of small scale
Large Eddy Simulation (LES)
The most used filter function in LES is the top hat
filter:
The filtered equations governing the flow in LES are:
Large Eddy Simulation (LES)
An unknown stress term needs to be obtained
For that purpose the following equation has been derived:
Subgrid Scale (SGS) Reynolds Stress: Represents the
large scale momentum flux due to turbulence motion
Large Eddy Simulation (LES)
To obtain the SGS Reynolds Stress , a subgrid scale
model has to be used
The most used model is the Smagorinsky model
Basically, the Smagorinsky SGS model simulates the
tranference of energy between the large and the
subgrid-scale eddies
It takes into account the SGS eddy viscosity νSGS, and
the backscattering (reverse of cascade process)
Large Eddy Simulation (LES)
Advantages:
• The influence of turbulence is very well
captured in LES
Disadvantages:
• Too disipative in laminar regions
• Special near wall treatment
• Backscatter of flow is uncertain
• High computational cost o Re1.8 near to the viscous sublayer
o Re0.4 away from the wall
Dettached Eddy Simulation (DES)
DES uses the RANS models (generally SST) close to
the wall and LES in the wake region of a flow where
flow unsteadiness appear
Basically, DES employs a turbulent length scale, Lt, to
determinate which approach to use during a simulation
The activation of LES or the switching to RANS models
is controlled by a blending factor F
where CDES constant
Dettached Eddy Simulation (DES)
The blending factor is defined as:
where CDES is a constant
SST-DES model offers great potential in the application
of simulations for a large class of flows at high Reynolds
numbers
DES is the more practical, computationally efficient and
widely used turbulence model nowadays
3. CONCEPTUAL OVERVIEW
Reynolds number
Vortex shedding
Drag and Lift coefficients
REYNOLDS NUMBER
Reynolds number (Re)
The flow varies with the Reynolds number around a
circular cylinder
In small Reynolds numbers, small vicous flows
where frictional forces are dominant take place
With the increase of Reynolds number, flows have
rapid regions with velocity changes, thus generating
vortices and turbulence
Reynolds number (Re)
Matematically:
where u is the inlet velocity, D the diameter of the cylinder and ν the kinematic viscosity of the flow
From Roshko’s experiment was obtained:
Stable range: 40 – 150
Transitional range: 150 – 300
Irregular range: 300 – 200,000
Reynolds number (Re)
VORTEX SHEDDING
Vortex shedding
The separation of the flow around a circular cylinder
creates pairs of eddies to form alternately on the bottom
and top part of the cylinder
This eddies travel into the wake region thus generating
vortex shedding
Vortex shedding
Strouhal number is a dimensionless number that
describes the shedding of the vortices in the wake
region
where fs is the shedding frecuency of the vortices (1/T),
u is the inlet velocity and D cylinders diameter
Vortex shedding is very usual in engineering
Vortex shedding
The frecuency at which vortices are shed remains
constant within Re=250 and Re=10,000 frecuencies
DRAG AND LIFT COEFFICIENTS
Drag and Lift coefficients
A dimensionless quantity that is used to quantify the
resistance of an object in a fluid environment such as
air or water
where A is the projected are in the flow and F is the sum
of the pressure force and the viscous force components
on the cylinder surface (in the along-flux direction)
Drag and Lift coefficients
Drag coefficient is made up of three components:
• Viscous force Ff
• Pressure force Fp
Wave force Fo
The figure shows the evolution of CD with Re
!!!
Drag and Lift coefficients
Roshko stated that Strouhal number and the Drag
Coefficient of the flow are related in the sub-critical
range (Re<10,000), where an increase in the Strouhal
number is accompained by a decrease in CD
Lift coefficient is defined similarly but vertical force is
considered
Drag and Lift coefficients
Theoretically, in a vortex shedding situation, the drag
force is changing at twice the frecuency of the lift force
in a flow involving separation
It is important that any turbulence model can simulate
this accordingly and should be measured
Julen García Ibáñez
Contact: [email protected]