There are two study types available for this physics interface. Using the Time Dependent study type, rotation is achieved through moving mesh functionality, also known as sliding mesh. Using the
Frozen Rotor study type, the rotating parts are kept frozen in position, and rotation is accounted for by the inclusion of centrifugal and Coriolis forces. Turbulence effects are modeled using the one-equation Spalart-Allmaras turbulence model. The Spalart-Allmaras model is a so-called low-Reynolds number model, which means that it resolves the velocity, pressure, and temperature fields all the way down to the wall. The Spalart-Allmaras model depends on the distance to the closest wall. The physics interface therefore includes a wall distance equation. A
Wall Distance Initialization study type is automatically added. It also supports heat transfer in solids as well as surface-to-surface radiation. However, only fluid domains adjacent to pair boundaries are supported.
When this multiphysics interface is added, the following default nodes are also added in the Model Builder under
High Mach Number Flow, Spalart-Allmaras —
Fluid,
Initial Values,
Wall, and
Thermal Insulation. When a pair boundary is created, the
Continuity node is automatically added. Then, from the
Physics toolbar, add other nodes that implement, for example, boundary conditions, volume forces, and heat sources. You can also right-click the node to select physics features from the context menu. See
Moving Mesh for more details of the
Rotating Domain node added automatically in the
Model Builder under
Definitions >
Moving Mesh.
The Label is the default physics interface name.
The Name is used primarily as a scope prefix for variables defined by the physics interface. Refer to such physics interface variables in expressions using the pattern
<name>.<variable_name>. In order to distinguish between variables belonging to different physics interfaces, the
name string must be unique. Only letters, numbers, and underscores (_) are permitted in the
Name field. The first character must be a letter.
The default Name (for the first physics interface in the model) is
hmnf.
The Reference temperature Tref is used to define the reference enthalpy
Href which is set to 0 J/kg at
pref (1 atm) and
Tref. When the
Include kinetic energy checkbox is selected, the conservative total-energy equation is solved.
The default Turbulence model type is
RANS, the default
Turbulence model is
Spalart-Allmaras, and the default
Heat transport turbulence model is
Kays–Crawford. Alternatively, select
User-defined turbulent Prandtl number. The turbulent Prandtl number model describes the influence of the turbulent fluctuations on the temperature field. It is always possible to have a user-defined model for the turbulence Prandtl number. Enter the user-defined value or expression for the turbulence Prandtl number in the
Model Inputs section of the
Fluid node.
The dependent variables (field variables) are the Velocity field u (SI unit: m/s), the
Pressure p (SI unit: Pa), and the
Temperature T (SI unit: K). For turbulence modeling,
Reciprocal wall distance G (SI unit: 1/m) and
Undamped turbulent kinematic viscosity nutilde (SI unit: m
2/s) variables are also available.