|
class | fvDOM |
| Finite Volume Discrete Ordinates Method. Solves the RTE equation for n directions in a participating media, not including scatter and reflective walls. More...
|
|
class | noRadiation |
| No radiation - does nothing to energy equation source terms (returns zeros) More...
|
|
class | opaqueSolid |
| Radiation for solid opaque solids - does nothing to energy equation source terms (returns zeros) but creates absorptionEmissionModel and scatterModel. More...
|
|
class | P1 |
| Works well for combustion applications where optical thickness, tau is large, i.e. tau = a*L > 3 (L = distance between objects) More...
|
|
class | solarLoad |
| The solarLoad radiation model includes Sun primary hits, their reflective fluxes and diffusive sky radiative fluxes. More...
|
|
class | solarLoadBase |
| Base class for solarLoad models. More...
|
|
class | viewFactor |
| View factor radiation model. The system solved is: C q = b where: Cij = deltaij/Ej - (1/Ej - 1)Fij q = heat flux b = A eb - Ho and: eb = sigma*T^4 Ej = emissivity Aij = deltaij - Fij Fij = view factor matrix. More...
|
|
class | laserDTRM |
| Discrete Tray Radiation Method for collimated radiation flux. At the moment the particles are injected on a 2D disk in polar coordinates providing starting and finish locations. More...
|
|
This group contains radiation models