Initial Values (Radiation in Participating Media and Radiation in Absorbing-Scattering Media Interfaces)
This node adds an initial value for the radiative intensity I (when Discrete ordinates method is selected as the Radiation discretization method) or the incident radiation G (when P1 approximation is selected as the Radiation discretization method) that can serve as an initial condition for a transient simulation or as an initial guess for a nonlinear solver.
Initial Values
Discrete Ordinates Method
When Discrete ordinates method is selected as the Radiation discretization method for the physics interface, you should define the initial radiative intensity using one of the following options, depending on the Wavelength dependence of radiative properties set in the Participating Media Settings section of the interface.
If the Wavelength dependence of radiative properties is Constant, choose between the following options:
Use the Blackbody/Graybody assumption and set a value for the Initial temperature T, to define I = Ib(T). This option is only available in the Radiation in Participating Media interface.
Set a User defined value for the Initial radiative intensity I. The default is 0 in the Radiation in Absorbing-Scattering Media interface, and rpm.Ibinit in the Radiation in Participating Media interface.
If Wavelength dependence of radiative properties is Solar and ambient or Multiple spectral bands, choose among the following options:
When Initial value is set to Blackbody/Graybody, enter a value for the Initial temperature T, to define I = Ib(T). This option is only available in the Radiation in Participating Media interface.
When Initial value is set to User defined for each band, enter a value for the Initial radiative intensity for each spectral band in the table displayed underneath. Within a spectral band, each value is assumed to be independent of wavelength.
When Initial value is set to User defined distribution, enter a value or expression for the Initial radiative intensity distribution Iλ. The wavelength may be accessed through the rpm.lambda or rasm.lambda variable. This distribution is integrated over each spectral band to obtain the radiative intensity Ii,k for each spectral band.
P1 Approximation
When P1 approximation is selected as the Radiation discretization method for the physics interface, you should define the initial incident radiation using one of the following options, depending on the Wavelength dependence of radiative properties set in the Participating Media Settings section of the interface.
If the Wavelength dependence of radiative properties is Constant, choose between the following options:
Use the Blackbody/Graybody assumption and set a value for the Initial temperature T, to define G = 4πIb(T). This option is only available in the Radiation in Participating Media interface.
Set a User defined value for the Initial incident radiation G. The default is 0 in the Radiation in Absorbing-Scattering Media interface, and (4*pi)*rpm.Ibinit in the Radiation in Participating Media interface.
If Wavelength dependence of radiative properties is Solar and ambient or Multiple spectral bands, choose among the following options:
When Initial value is set to Blackbody/Graybody, enter a value for the Initial temperature T, to define G = 4πIb(T). This option is only available in the Radiation in Participating Media interface.
When Initial value is set to User defined for each band, enter a value for the Initial incident radiation for each spectral band in the table displayed underneath. Within a spectral band, each value is assumed to be independent of wavelength.
When Initial value is set to User defined distribution, enter a value or expression for the Initial incident radiation distribution Gλ. The wavelength may be accessed through the rpm.lambda or rasm.lambda variable. This distribution is integrated over each spectral band to obtain the incident radiation Gk for each spectral band.
Location in User Interface
Context Menus
Ribbon
Physics tab with Radiation in Participating Media or Radiation in Absorbing-Scattering Media selected: