Plasma Model Reference Topic

You can use the Plasma model with the Coupled Plasma Electron model to model plasmas that are in non-local thermal equilibrium.

Table 1. Coupled Plasma Electron Model Reference
Theory See Cold, Non-Thermal Plasma and Reacting Flow Plasma.
Provided By [physics continuum] > Models > Plasma
Example Node Path Continua > Physics 1 > Models > Coupled Plasma Electron Model
Requires
  • Space: any
  • Material: Gas or Multi-Component Gas
  • Optional Models: Plasma
Properties See Coupled Plasma Electron Model properties.
Activates Model Controls (child nodes) e-
Material Properties Charge Number, Mobility, Molecular Diffusivity, Molecular Weight.

Also, for the [gas component], the Elastic Electron Collisional Cross Section Material Property is available to set.

Initial Conditions Electron Number Density, Electron Temperature. See Initial Conditions.
Boundary Inputs Electron Number Density Specification, Electron Thermal Specification. See Boundary Settings.
Region Inputs Electron Energy Density Source Option, Electron Source Option. See Region Settings.
Solvers Coupled Plasma Electron. See Solvers.
Monitors Electron Density, Electron Energy
Field Functions
  • Charged Species Mobility of Electron
  • Elastic Electron Collisional Cross Section
  • Electron Elastic Collision Energy Source
  • Electron Energy Density
  • Electron Number Density
  • Electron Ohmic Energy Source
  • Electron Temperature
  • Molecular Diffusivity of Electron
See Field Functions.

Coupled Plasma Electron Model Properties

Transport
Allows you to specify how the electric potential is coupled with the electrons.
  • Electrons < > Electric Potential This selection is appropriate for modeling most plasma setups.
  • Electric Potential > Electrons
  • Electrons > Electric Potential
  • No Electric Potential Coupling
Secondary Gradients

Neglect or include the boundary secondary gradients for diffusion and/or the interior secondary gradients at mesh faces. See Omitting Secondary Gradients.

  • On

    Include both secondary gradients.

  • Off

    Exclude both secondary gradients.

  • Interior Only

    Include the interior secondary gradients only.

  • Boundaries Only

    Include the boundary secondary gradients only.

Initial Conditions

Electron Number Density
Sets the electron number density n e as a scalar profile.
Electron Temperature

Sets the temperature T e as a scalar profile.

Boundary Settings

Wall Boundaries
Electron Number Density Specification
Allows you to choose how the number density, n e , of the electrons is specified at the boundary.
Method Corresponding Physics Value Nodes
Impermeable
Specifies that the boundary is impermeable to electrons – which is essentially a vanishing flux that is provided at the boundary.
None
Specified Flux
Allows you to specify the electron number density as an influx or outflux of electrons. Also provides the physics condition, Wall Electron Number Density Flux Derivitave Option.
Electron Flux
Specifies the electron flux, Γ e , as a scalar profile.
Specified Value
Sets the electron number density to the specified value.
Electron Number Density
Specifies the electron number density as a scalar profile.
Wall Electron Number Density Flux Derivitave Option
Allows you to specify an electron number density flux derivative.
Method Corresponding Physics Value Nodes
None
None
Specified
Electron Flux Derivative
Specifies the electron flux derivative, Γ e , as a scalar profile.
Electron Thermal Specification
Allows you to choose how the thermal energy of the electrons is specified.
Method Corresponding Physics Value Nodes
Specified Electron Temperature
Sets the electron temperature T e .
Electron Temperature
Specifies the electron temperature as a scalar profile.
Specified Electron Energy Flux
Allows you to specify the thermal energy of the electrons as an energy flux. Also provides the physics condition, Wall Electron Energy Density Flux Derivative Option.
Electron Energy Flux
Specifies the electron energy flux, Γ , as a scalar profile.
Wall Electron Energy Density Flux Derivitave Option
Allows you to specify an electron energy density flux derivative.
Method Corresponding Physics Value Nodes
None
None
Specified
Electron Energy Flux Derivative
Specifies the electron energy flux derivative, Γ e , as a scalar profile.
Inflow and Outflow Boundaries
Electron Number Density
Specifies the electron number density, n e , at inflow and outflow boundaries as a scalar profile.
Electron Temperature
Specifies the electron temperature, T e , at inflow and outflow boundaries as a scalar profile.

Region Settings

Applies to fluid regions.

Electron Energy Density Source Option
Method Corresponding Physics Value Nodes
Electron Energy Source
When activated, allows you to specify the electron energy density source term and its derivative.
Electron Energy Source
Specifies the electron energy density source term, S , u s r as a scalar profile.
Electron Energy Source Derivative
Specifies the derivative of the electron energy density source term.
Electron Source Option
Method Corresponding Physics Value Nodes
Electron Source
When activated, allows you to specify the electron number density source term and its derivative.
Electron Source
Specifies the electron number density source term, S e , u s r , as a scalar profile. The electrons are assumed to be cold unless an electron energy source is added.
Electron Source Derivative
Allows you to specify the derivative of the electron number density source term.

Coupled Plasma Electron Solver Properties

Begin
Specifies the iteration or time-step after which the reactions are activated. During previous iterations or time-steps, reactions are deactivated. This feature is useful when modeling significant flow as you can deactivate reactions until a flow solution is found.
Solver Frozen
When On, the solver does not update any quantity during an iteration. It is Off by default. This is a debugging option that can result in non-recoverable errors and wrong solutions due to missing storage. See Finite Volume Solvers Reference for details.
Reconstruction Frozen
When On, Simcenter STAR-CCM+ does not update reconstruction gradients with each iteration, but rather uses gradients from the last iteration in which they were updated. Activate Temporary Storage Retained in conjunction with this property. This property is Off by default.
Reconstruction Zeroed
When On, the solver sets reconstruction gradients to zero at the next iteration. This action means that face values used for upwinding (Eqn. (905)) and for computing cell gradients (Eqn. (917) and Eqn. (918)) become first-order estimates. This property is Off by default. If you turn this property Off after having it On, the solver recomputes the gradients on the next iteration.
Temporary Storage Retained
When On, Simcenter STAR-CCM+ retains additional field data that the solver generates during an iteration. The particular data retained depends on the solver, and becomes available as field functions during subsequent iterations. Off by default.

Field Functions

Charged Species Mobility of Electron
Mobility of electrons, μ e
Elastic Electron Collisional Cross Section
Elastic collision momentum transfer cross-section σ ζ e which is used to calculate the collision frequency.
Electron Elastic Collision Energy Source
Electron elastic collision energy source term, Sel in Eqn. (4193).
Electron Energy Density
Electron energy density, e
Electron Number Density
Electron number density, n e
Electron Ohmic Energy Source
Electron Ohmic heating energy source term, SΩ in Eqn. (4193).
Electron Temperature
Electron temperature, T e
Molecular Diffusivity of Electron
Molecular diffusivity of electrons, D e