Fig. 5From: Photochemical and radiation transport model for extensive use (PROTEUS)Application of PROTEUS to the Martian atmosphere. Vertical profiles of neutral density simulated by PROTEUS (solid) and one-dimensional Martian photochemical model by Chaffin et al. (2017) (dashed). The same boundary conditions, chemical reactions and their rate coefficient, binary and eddy diffusion coefficients, and temperature profile, were used in both simulations for validationBack to article page