Radiative Transfer Code is a computer routine to solve the equations describing Radiative Transfer (RT), i.e., the propagation of energy from Electromagnetic Radiation (EMR) passing through an Atmosphere (gas or Plasma) including the effects of Absorption, Emission, and scattering. The equations are sufficiently complex that they need to be solved numerically. Referenced by: Code Computational Astrophysics Hyperion Stellar Model Atmosphere Turtlebeach |