Modeling of the planetary structure of the ionosphere and the protonosphere coupling

A planetary model of the ionosphere and the protonosphere coupling is described. The system of three-dimensional nonstationary modeling equations of continuity and motion for the ions O⁺ and H⁺ is presented. Some numerical results of model calculations are compared with the experimental data. The important role of electromagnetic drifts in the formation of large-scale morphological peculiarities of the ionosphere and the protonosphere coupling is shown.