There are two main approaches to developing practical algorithms that can extract useful and reliable data about trace gas concentrations from the complex combination of factors that are involved in remote sensing measurements from space.
These simulate physical processes on individual photons using probability functions. The analysis of a large group of photons yields a probability distribution of photon paths.
These simplify the Radiative Transfer Equation by using approximations such as a plane parallel atmosphere or only single scattering. The solution uses standard methods for integral-differential equations.