“…Equation () states the RTE equation and its dependences.where, I λ is the monochromatic radiation intensity, d t and d s are the time and space derivatives, respectively, c is the speed of light, j λ is the emission function, β ext is the extinction coefficient, β scat is the scattering coefficient, φ is the scattering phase function and Ω is the solid angle. Numerous approaches have been proposed to solve the RTE and Howell et al 42,43 ranked the most used methods, listing their advantages and drawbacks. Using the diffusive approach developed by Clark, 44 the RTE can be combined with the heat transfer partial differential equations (PDE) resulting in the calculation of k rad .…”