Participating Media Radiation (Spherical Harmonics) Reference

The Spherical Harmonics model uses spherical harmonics to describe the directional component of radiation intensity in media that can absorb, emit, or scatter thermal radiation .

The Participating Media Radiation (Spherical Harmonics) model is faster than the Participating Media Radiation (DOM) model but applies to a more limited range of scattering and boundary conditions. This model does not simulate refraction or specular reflection. It is lower in accuracy than the DOM model at boundaries and for situations with large directional gradients of intensity. It is not compatible with other radiation models or with overset mesh.

Theory See Participating Media Spherical Harmonics.
Provided By [physics continuum] > Models > Radiation
Example Node Path Continua > Physics 1 > Models > Participating Media Radiation (Spherical Harmonics)
Requires
  • Space: Any
  • Optional Models: Radiation
Properties Key properties are: Secondary Gradients. See Participating Media (Spherical Harmonics) Properties.
Activates Boundary Inputs See Participating Media (Spherical Harmonics) Boundary Settings.
Solvers Spherical Harmonics Radiation. See Spherical Harmonics Radiation Solver Properties.
Monitors P1
Field Functions Boundary Irradiation, Boundary Radiation Heat Flux, Boundary Radiosity, Incident Radiation, Radiative Absorbtion, Radiative Energy Source, Total Absorption Coefficient, Total Emissivity. See Radiation Field Function Reference.

Participating Media Radiation (Spherical Harmonics) Properties

Secondary Gradients
Neglects or includes the boundary secondary gradients for radiation or the interior secondary gradients at mesh faces.
On
Includes both secondary gradients.
Off
Excludes both secondary gradients.
Interior Only
Includes the interior secondary gradients only.
Boundaries Only
Includes the boundary secondary gradients only.

Boundary Settings

Inflow Boundaries, Pressure Outlet, Free Stream , Wall
Radiation Flux Option
This option allows you to model diffuse radiation sources at boundaries according to your own specification. See Diffuse Radiation Flux.
Radiation Flux Option Corresponding Physics Value Nodes
No flux None
Diffuse radiation flux
Diffuse Radiation Flux
The diffuse radiation flux is specified as a scalar profile. Requires the Multiband Thermal Radiation or Gray Thermal Radiation model.
Inflow Boundaries, Pressure Outlet, Free Stream
Radiation Temperature
The temperature of an open boundary that has a total radiant emittance identical to that of a black body. See Radiation Temperature.

Spherical Harmonics Radiation Solver Properties

冻结求解器
开启时,求解器在迭代过程中不更新任何物理量。该选项默认情况下关闭。这是一个调试选项,由于缺少储存,它可能导致不可恢复的错误和错误的求解。有关详细信息,请参见有限体积求解器参考
Solver Order Option
Sets the order of Legendre polynomial used for the spherical harmonics calculation Eqn. (1752). At present, the only value available is P1.