Drag Coefficient Reference
Standard drag coefficients are used for drag force models that are composed of a Standard Drag Coefficient for a single particle together with a Drag Correction factor to account for multi-particle effects. Linearized drag coefficients are used for integrated models for the interphase drag or friction force.
The Drag Coefficient node is a child node of the Drag Force model.
Continuous-Dispersed Topology Drag Coefficient Properties
For a Continuous-Dispersed Topology phase interaction use one of the following methods for specifying the drag coefficient:
Method | Corresponding Properties/Method Nodes |
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Arastoopour
The Arastoopour drag coefficient method is provided for solid dispersed-phase applications such as fluidized beds, where particle loadings are high. This method is available only when the dispersed phase is a solid. |
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Bozzano-Dente The Bozzano-Dente drag coefficient method defines the standard drag coefficient using the Bozzano and Dente correlation. See Eqn. (1958). The Bozzano-Dente correlation is suitable for a wide range of liquid-gas bubble systems including water at low and high pressure, and highly viscous liquids such as some oils, glycerol, or molten glass. For small bubble diameters in low viscosity systems (for example, water), the Bozzano-Dente method gives a different asymptote to other standard drag correlations. The Bozzano-Dente correlation requires that gravity is activated for the physics continuum. This method is available only when the dispersed phase is a gas. |
The surface tension value must be specified in the Surface Tension node appears automatically when the Bozzano-Dente correlation is selected. node for the parent phase interaction. The |
EMMS
The EMMS (energy minimization multi-scale) drag coefficient method is suitable for applications involving a dispersed solid phase, particularly for modeling fluidized bed systems where the influence of heterogeneity from particle clusters becomes significant. This method is available only when the dispersed phase is a solid. |
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Field Function |
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Field Function (Linearized Coefficient) |
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Gidaspaw
The Gidaspow drag
coefficient method is appropriate for solid dispersed-phase applications,
such as fluidized beds, that have high particle loading. This method is available only when the dispersed phase is a solid. |
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Hamard and
Rybczynski The Hamard and Rybczynski drag coefficient method is used for viscous Newtonian fluid droplets dispersed in a second immiscible viscous Newtonian fluid. See Eqn. (1964). The Hamard and Rybczynski drag model is not valid for high Reynolds numbers, where the Schiller-Naumann model is expected to be more accurate. This method is suitable for spherical liquid droplets. |
None. |
Rusche-Issa
The Rusche-Issa drag coefficient method is appropriate when the dispersed phase volume fraction becomes high. This model accounts for the modification of the drag force due to the presence of other particles when the particles are densely-packed. For example, you would use this model when predicting the separation of oil and water in an emulsion settling experiment. See Eqn. (1954). |
Simcenter STAR-CCM+ includes two implementations of this model. The particular implementation that Simcenter STAR-CCM+ uses depends on the two phases:
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Linearized Emulsion
Topology Inversion
The Linearized Emulsion Topology Inversion drag coefficient method allows the phases to invert when the volume fraction of the dispersed phase reaches the specified Inversion Volume Fraction. When the dispersed volume fraction becomes larger than the specified value, the drag, the relative viscosity, and the normal relative viscosities are swapped between the phases. After inversion, the relative viscosities are calculated using a new value for the maximum packing in the relative viscosity models. This method is available only when the Emulsion Rheology model is selected. |
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Schiller-Naumann
Suitable for spherical solid particles, liquid droplets, and small-diameter (spherical) bubbles. This method is available only when the continuous phase is viscous. However, the continuous phase can be either Newtonian or non-Newtonian. See Eqn. (1946). |
None. |
Symmetric
The Symmetric drag coefficient method is recommended for flows where phase topology inversion occurs, that is, the dispersed phase in one region of the domain becomes the continuous phase in another. |
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Syamlal-O’Brien
The Syamlal-O’Brien drag coefficient method is based on measurements of terminal velocity that is made in settling beds. The Syamlal-O’Brien drag coefficient properties should be adjusted according to the parameters of the simulation. For more information and an example case, see the technical report Study of Gas-Solid Fluidized Bed - Tuning Syamlal-O'Brien Drag Model in the Technical Library on the Support Center portal, https://support.sw.siemens.com/en-US/product/226870983/downloads. This method is available only when the dispersed phase is a solid. |
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Tomiyama
The Tomiyama drag coefficient method determines the drag force depending on how contaminated the bulk flow is by impurities, such as surfactants. Surfactants reduce the liquid surface tension and prevent internal circulation in bubbles, hence increasing drag. The Tomiyama drag coefficient method is suitable for liquid-gas bubble systems with a low Reynolds number and low Morton number flow, for example, small bubbles in an air-water system. In such cases, the Bozzano-Dente model over-predicts the drag coefficient. The Tomiyama correlation requires that gravity is activated for the physics continuum. This method is available only when the continuous phase is viscous, and when the dispersed phase is a gas. It is not available for solid particles. |
The surface tension value must be specified in the Surface Tension node appears automatically when the Tomiyama correlation is selected. node for the parent phase interaction. The |
Wang Curve
Fit
Suitable for water-air bubble systems or similar systems at near atmospheric pressure, and should be used with care in any other conditions. See Eqn. (1973). The Wang Curve Fit drag coefficient method is available only when the continuous phase is viscous, and when the dispersed phase is a fluid. This method is not available for solid particles. |
None. |
Suspension
The Suspension drag coefficient method is a linearized form of the Schiller-Neumann drag model which allows to become infinitely large when maximum packing is reached. The maximum-packed structure prevents slip from occurring between the phases. This method is available only when the Suspension Rheology model is selected. |
None. |
- Rusche-Issa Drag Coefficient Properties
- Depending on the selection of phases for the drag force phase interaction
model, the following properties are available:
Method Corresponding Properties/Method Nodes Inversion Rusche-Issa This model allows you to model immiscible liquid (such as oil-water) separation without turning on all the detailed physics of the Emulsion rheology model.
- Parameter Options
- Specifies the choice of parameters that are used in
the Rusche-Issa drag coefficient, Eqn. (1954).
Simcenter STAR-CCM+ detects the type of dispersed phase and sets the default option accordingly to one of the following:
- Gas Bubble
- Liquid Droplet
- Solid Particle
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- User Parameters
- Available only when the Parameters
Options property setting is
User Parameters.
- K1, K2
- The parameter values ( and in Eqn. (1954)) are set automatically for the default dispersed phase type. These values are based on the averages that were obtained by Rusche [538]. These parameters are editable
- Start Volume Fraction (mixture regime), End Volume Fraction (mixture regime)
- The start and end values specify the range across which the drag limits are blended.
- Inversion Length Scale
- Specifies the size of the dispersed liquid drops after inversion.
Rusche-Issa This drag model allows hindered settling in a similar way to the Richardson-Zaki drag correction. - Parameter Options
- same as above.
Multiple Flow Regime Topology Drag Coefficient Properties
For a Multiple Flow Regime Topology phase interaction, you set the appropriate Drag Coefficient method for each phase interaction regime.
Method | Corresponding Properties/Method Nodes |
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Field Function
This method is available only for the first dispersed and second dispersed regimes. |
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Field Function (Linearized Coefficient) |
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Schiller-Naumann
With this
methods the drag coefficient is computed using the Schiller-Naumann correlation. This method is available only for the first dispersed and second dispersed regimes. |
None. |
Tomiyama The drag coefficient is computed using the Tomiyama drag coefficient method. Available for the first dispersed regime when the secondary phase is a gas and available for the second dispersed regime when the primary phase is a gas. The Tomiyama drag coefficient determines the drag force depending on how contaminated the bulk flow is by impurities, such as surfactants. Surfactants reduce the liquid surface tension and prevent internal circulation in bubbles, hence increasing drag. The Tomiyama correlation requires that gravity is activated for the physics continuum. |
The surface tension value must be specified in the Surface Tension node appears automatically when the Tomiyama correlation is selected. node for the parent phase interaction. The |
Blended
The intermediate regime
drag is calculated by blending the drags of the first dispersed regime and
the second dispersed regime on either side of the interface (see Eqn. (1977)). This method is available only for the intermediate regime. |
None. |
Strubelj-Tiselj
The drag coefficient is computed using the Strubelj and Tiselj interface drag method [549]. This method is available only for the intermediate regime. |
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