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Simu Simula lation tion of of F Free ee-Su Surf rfac ace e Flo lows ws Wit ith h ST STAR AR-CC CCM+ M+ Samir Muzaferija and Milovan Peri CD-adapco Contents Introduction to multiphase flows Theoretical background for


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SLIDE 1

Simu Simula lation tion of

  • f F

Free ee-Su Surf rfac ace e Flo lows ws Wit ith h ST STAR AR-CC CCM+ M+

Samir Muzaferija and Milovan Perić CD-adapco

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SLIDE 2

Contents

 Introduction to multiphase flows  Theoretical background for VOF-method  High-Resolution Interface-Capturing (HRIC) scheme  Accounting for surface tension effects  Extensions of VOF-method  Waves: generation and propagation  Free surface flows: application examples  Future development

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Introduction to Multiphase Flows

VOF-approach is suitable, when the grid is fine enough to resolve the interface between two immiscible fluids. Sometimes not all parts of the flow are suited for VOF-treatment… Examples: Atomization nozzle flow and jet break-up (right) and flow around a hydrofoil (below)

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Interface Conditions

  • Conditions at an interface between two immiscibe fluids:

Kinematic condition: No flow through interface.

Dynamic conditions: Balance of normal and tangential stresses (surface tension forces):

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SLIDE 5

VOF: Theory, I

  • VOF considers a single effective fluid whose properties vary

according to volume fraction of individual fluids:

  • The mass conservation equation for fluid i reads:
  • It can be rearranged into an equation in integral form:

This equation is used to compute the transport of volume fraction αi.

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SLIDE 6

VOF: Theory, II

  • The mass conservation equation for the effective fluid is
  • btained by summing up all component equations and

using the condition:

  • The integral form of mass conservation equation (used to

compute pressure correction) reads:

  • The properties of effective fluid are computed according to

volume fractions:

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SLIDE 7

Interface-Capturing Method, I

  • For sharp interfaces, special discretization for convective

terms in the equation for volume fraction αi is needed (to avoid excessive spreading).

  • The method must produce bounded solutions, i.e. each

volume fraction must lie between 0 and 1 and the sum of all volume fractions must be 1 at each control volume.

  • Bounded schemes must fall within a certain region of the

normalized variable diagram; the normalized variables are defined as:

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SLIDE 8

Interface-Capturing Method, II

  • The boundedness requirement:

The normalized variable diagram and the proposed high-resolution interface- capturing (HRIC) scheme (details available in STAR- CCM+ documentation)

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SLIDE 9

HRIC-Scheme, IV

Simulation of sloshing in a tank due to sinusoidal sway motion:

  • ne-cell sharp interface before wave overturns (left) and smeared

Interface after splashing (right), when the interface is in reality not sharp…

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SLIDE 10

Interface Sharpening

  • In order to prevent dilution, one can activate “interface sharpening”

by setting “Sharpening factor” to a value >0.

  • The sharpening model is based on “anti-diffusion” and acts only in

cells at the interface…

  • This is usually required only for violent sloshing and similar

phenomena…

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SLIDE 11

Local Grid Refinement, I

  • One should, when possible, align grid with free surface where it is

flat…

  • One should, when possible, avoid vertical grid coarsening in free-

surface zone where its deformation is small…

  • The reason: volume fraction is convected into finer cells and leads

to smeared interface…

Flow around a vertical cylinder – two grids for the same initial free surface position

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Local Grid Refinement, II

Initial value from this cell feeds into next two, from there into next four – the smeared interface does not get sharper by refining time step (only “Sharpening Factor” helps – but it is better to adapt the grid to free surface that to use artificial anti-diffusion…) Impulsively started flow around a vertical cylinder

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Surface Tension Effects, I

  • The kinematic interface condition is implicitly accounted

for by the transport equation for volume fraction.

  • The dynamic interface conditions require additional forces

in the momentum equations in cells containing free surface…

  • Surface tension forces are converted to volume forces:

Since the gradient of volume fraction is zero away from interface, these terms are equal to zero everywhere except along interface…

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SLIDE 14

Surface Tension Effects, II

  • The unit vector normal to interface is obtained from the

gradient of volume fraction:

  • The curvature of free surface is obtained from the

divergence of the unit vector normal to interface:

  • The volume fraction field needs to be smoothed before

the curvature is computed (sharp interface leads to a non- smooth curvature field).

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SLIDE 15

Surface Tension Effects, III

  • The so called „parasitic currents“ can develop, if the fluid

moves only slowly or not at all, and the surface tension effects dominate (high curvature or surface tension coefficient)...

  • The reason: pressure and surface tension forces must be

in equilibrium when fluid is at rest – but the numerical approximations do not guarantee that (one term is linear and the other is non-linear):

  • There are many partial solutions to this problem in

literature, but none works in all situations…

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SLIDE 16

Surface Tension Effects, IV

  • Recently, a new model called “Interface Momentum

Dissipation” was introduced in STAR-CCM+ to reduce the effects of parasitic currents…

  • The momentum dissipation term is added to the

momentum equations only in the vicinity of the interface…

  • It acts similarly as an increased fluid viscosity near

interface (more on the gas side): µint grad(v)

  • Interface Momentum Dissipation decreases rapidly with

distance from interface…

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SLIDE 17

Surface Tension Effects, V

  • Where free surface is in contact with wall, contact angle

needs to be prescribed.

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Surface Tension Effects, VI

  • One can distinguish between:

 Static contact angle  Dynamic advancing contact angle on dry surface  Dynamic advancing contact angle on wet surface  Dynamic receding contact angle

  • The contact angle is enforced as:

nfs = - nw cos θw + tw sin θw

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SLIDE 19

Interface Momentum Dissipation: Ink Jet Droplet, I

Without IMD With IMD

Without IMD, parasitic currents are strong (maximum velocity 35.88 m/s); With IMD, parasitic currents are hardly visible (maximum velocity 8.98 m/s)

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SLIDE 20

Without IMD, the interface is smeared behind secondary droplet and at nozzle exit; With IMD, the interface is sharp almost everywhere…

Without IMD With IMD

Interface Momentum Dissipation: Ink Jet Droplet, II

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SLIDE 21

Without IMD: Strong parasitic currents, maximum velocity 4.97 m/s (10x web speed) With IMD: Very weak parasitic currents, maximum velocity 0.506 m/s (1% above web speed)

Interface Momentum Dissipation: Flow in a Slot Coater, I

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Interface Momentum Dissipation: Flow in a Slot Coater, II

Without IMD: Front meniscus has irregular shape due to high parasitic velocities With IMD: Smooth front meniscus

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Interface Momentum Dissipation: Flow in a Slot Coater, II

Without IMD: Flow rate at outlet fluctuates due to high parasitic velocities With IMD: Flow rate at outlet fluctuates less

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SLIDE 24

Interface Momentum Dissipation: Flow in and Around a Rising Bubble

Left: Without IMD Strong parasitic currents, maximum velocity 11.68 m/s, interface smeared through high velocity normal to it, the flow inside bubble cannot be recognized… Right: With IMD Hardly visible parasitic currents, maximum velocity 0.39 m/s (30 times lower than before), interface is sharp (resolved by one cell) and one can clearly see the flow inside bubble…

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Extensions of VOF-Method

  • One can add additional models in the equation for volume

fraction (diffusion, sources) in order to model effects like non-sharp interfaces, phase change etc.

  • This is the main advantage of this approach compared to

level-set and similar schemes...

  • VOF-framework is already used in STAR-CCM+ for the

following models:

 Evaporation and condensation  Melting and solidification  Cavitation  Boiling

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SLIDE 26
  • STAR-CCM+ provides several wave models:

– For initialization of volume fraction, velocity and pressure fields; – For transient inlet boundary conditions.

  • Currently available models:

– 1st-order linear wave theory – Non-linear 5th-order Stokes wave theory (Fenton, 1985) – Pierson-Moskowitz and JONSWAP long-crested wave spectra – Superposition of linear waves with varying amplitude, period and direction of propagation (can be set-up via Excel-file)

Wave Models

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SLIDE 27
  • Accurate wave propagation requires 2nd-order time-integration

method.

  • Second-order method (quadratic interpolation in time) requires

that the wave propagates less than half a cell per time step.

  • First-order scheme is always stable but less accurate…

Time-Accurate Wave Propagation

Scaled 10 times in vertical direction…

Stokes 5th-order wave after 11 periods (8.977 s), resolved by 80 cells per wave- length (125 m) and 20 cells per wave height (5 m); damping over the last 300 m

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Internal Wave Generation

  • The source term in equation for volume fraction can be used to

simulate injection and suction…

  • … which can be used to create waves at free surface…
  • By a suitable choice of the position and shape of the “source zone”

and an appropriate source term function, one can generate waves

  • f desired shape…
  • The advantage of this approach: waves radiated by a solid

structure can pass over the source region without reflection (which happens when waves are created by inlet boundary conditions)

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SLIDE 29
  • Improvements to the treatment of contact angle (better

recognition of contact line, distinguishing direction of motion etc.)

  • Transition to other multiphase models:

– VOF to Lagrangian and vice-versa – Fluid film to VOF and vice versa

  • Eulerian or Lagrangian multiphase models within VOF

phases

Future Developments: VoF

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SLIDE 30

Simulation of Pouring