Numerical modeling of solar wind and coronal mass ejection in the inner heliosphere: A review

The predictions of plasma parameters in the interplanetary medium are core space weather forecasts, and magnetohydrodynamics (MHD) numerical simulation is an important tool prediction parameters. Operational forecasts commonly produced by a heliosphere model whose inner boundary set at 18 R s or beyond. Such typically use empirical/physics-based conditions to solve MHD equations for simulation. In recent years, significant progress has been made modeling heliosphere. this paper, solar wind coronal mass ejection reviewed. particular, different used investigated since solutions predetermined treatment large extent. Discussion on further development model.