The following topics are discussed:
The Intermittency transition model [224] is a further development
based on the -
transition model. The Intermittency transition model solves
only one transport equation for the turbulence intermittency,
, and avoids the need
for the second
equation of the
-
transition model. The Intermittency transition model has
the following advantages over the
-
transition model:
It reduces the computational effort by solving one transport equation instead of two.
It avoids the dependency of the
equation on the speed
. This makes the Intermittency transition model Galilean invariant. It can therefore be applied to surfaces that move relative to the coordinate system for which the velocity field is computed.
The model has provisions for crossflow instability that are not available for the
-
or
-
transition model.
The model formulation is simple and can be fine-tuned based on a small number of user parameters.
Like the -
transition model, the Intermittency transition model is based
strictly on local variables. The Intermittency transition model is also
available only in combination with the following turbulence models:
BSL
-
model
SST
-
model
Scale-Adaptive Simulation with BSL or SST
Detached Eddy Simulation with BSL or SST
Note the following limitations:
The Intermittency transition model is only applicable to wall-bounded flows. Like all other engineering transition models, the model is not applicable to transition in free shear flows. The model will predict free shear flows as being fully turbulent.
The Intermittency transition model has only been calibrated for classical boundary layer flows. Application to other types of wall-bounded flows is possible, but might require a modification of the underlying correlations.
The Intermittency transition model has not be calibrated in combination with other physical effects that affect the source terms of the turbulence model, such as:
Buoyancy
Multiphase turbulence
Guidelines on the use of the Intermittency transition model
are similar to those developed for the -
model as outlined in Ansys CFX Laminar-Turbulent Transition Models in the CFX-Solver Modeling Guide.
The transport equation for intermittency is the following:
The formulation of the source terms is similar in nature to
the corresponding terms in the -
transition model. The transition source term is
defined as:
where is the strain rate magnitude and
.
The destruction/relaminarization source is defined as follows:
where is the magnitude of the absolute vorticity rate,
and
. The transition onset is controlled by the following functions:
(2–156) |
where is the wall distance and
is a correlation
used to trigger the transition model:
In this correlation, is the critical
momentum thickness Reynolds number, and
and
are locally defined variables that approximate the freestream turbulence
intensity and the pressure gradient parameter, respectively. A local
formulation that provides
levels in the middle of the boundary layer similar
to the freestream turbulence intensity,
, is
expressed as:
The formula for reads as:
(2–157) |
For numerical robustness, was bounded as follows:
(2–158) |
The function accounts for the influence of the pressure
gradient on transition, and is defined as:
The Intermittency transition model has been calibrated against
a wide range of generic as well as turbomachinery and external aeronautical
test cases. While you should not have to adjust the model coefficients
in most situations, the model provides access to the coefficients
so that you can fine-tune the model. This should only be done based
on detailed experimental data. You can adjust the following constants
in the correlations: ,
,
,
,
,
,
,
,
,
.
The constant defines the
minimal value of critical
number, whereas
the sum of
and
defines
the maximal value of
. The
controls
how fast the
decreases as
the turbulence intensity (
) increases. The
and
constants
adjust the value of critical
number in areas
with favorable and adverse pressure gradient, respectively. The
constant
becomes active in regions with separation, correcting the
value if necessary. Additionally, the size of the separation bubble
can be tuned by another constant,
, which enters
the model through the source terms directly rather than the correlations
(see Coupling to SST Model). The constants
and
define the limits
of the
function; while they typically do not need
to be adjusted, it is possible to do so (for details, contact your
support engineer).
For crossflow transition, a widely used experimental correlation is the C1 correlation proposed by Arnal (1984) [223]. According to that correlation, transition occurs when the following condition is met:
where
The crossflow Reynolds number is defined as:
In the previous equations, is
the crossflow Reynolds number, the index
refers to a coordinate system
that is aligned with the freestream velocity
(where
refers to the boundary
layer edge),
is the crossflow velocity normal to the direction of the freestream
velocity. The value of 150 is the calibration constant of the Arnal
C1 criterion corresponding to a critical Reynolds number.
The Intermittency transition model accounts for the crossflow transition through a separate correlation, which approximates the C1 correlation through a local formulation. The formulation uses only local information and has the following functional form:
The function accounts for the influence of pressure gradient
(shape factor); the function
accounts for the ratio of the crossflow
strength relative to the streamwise strength; the Reynolds number
effect is included through
. The correlation can be adjusted by the constant
. The
transition location due to the crossflow instability will move upstream
as
increases.
The function is computed as follows:
where is a local
variable used to approximate the pressure gradient parameter and is
defined similarly to
(see Equation 2–157 and Equation 2–158):
The crossflow indicator function is a non-dimensional measure
of the local crossflow strength relative to the streamwise strength.
It is computed based on the wall normal change of the normalized vorticity
vector
, which serves as a measure
of the three-dimensionality of the velocity profile and which becomes
zero for 2D flow.
Here, is the vorticity vector and
is the wall normal vector.
The indicator function is proportional to the local change of
the flow angle and therefore a measure of the overall crossflow strength.
The triggering function that accounts for the crossflow effects is defined as follows:
The source term in the Intermittency equation is then triggered, either by the
primary triggering function (see Equation 2–156) of the
Intermittency transition model, or by
: whichever
has a maximal value.
The factor of 100 is used in in order
to speed up the transition process.
The default values for the model constants are the following:
= 100.0,
= 1000.0,
= 1.0,
= 14.68,
= -7.34,
= 0.0,
= 1.5,
= 3.0,
= 1.0,
= 1.0
The coupling between the Intermittency transition model and
the SST -
, SAS with SST and DES with SST models is
the same as for the
-
model and is accomplished by modifying the equations
of the original SST model as follows:
where and
are the production and destruction terms from the turbulent kinetic
energy equation in the original SST turbulence model. The
term is computed using Kato-Launder formulation:
An additional production term, , has been introduced
into the
-equation to ensure proper generation of
at transition points for
arbitrarily low (down to zero)
levels. The additional
term is designed to turn itself off when the transition process is
completed and the boundary layer has reached the fully turbulent state.
The expression for the
reads as:
The constants and
are adjustable. When
the laminar boundary layer separates, the size of the separation bubble
can be controlled by changing the constant
. The default
value of the constant is set to 1.0; a higher value results in a shorter
bubble. This mechanism is different from the one used for the
-
model, where the effective intermittency,
, is allowed
to exceed 1.0 whenever the laminar boundary layer separates. It should
be noted however, that the
constant has an effect
only for the bubbles developing under low
conditions
(<0.5%). It might also slightly affect the length of transition
in attached boundary layers under very low freestream turbulence intensity.