B. Finite difference equations of the model   d. Radiation
B.d.iv. Infrared radiation of dust The infrared radiative transfer equations of dust (A.33), (A.34), which are described in Appendix A.d.iii, are discretized as follows. When , Equations (B.53), (B.54) can also be represented in matrix form as follows. Where,
A Numerical Simulation of Thermal Convection in the Martian Lower Atmosphere with a Two-Dimensional Anelastic Model