Learning

Modeling the Solar Wind from the Sun to Earth

Solar Wind Observations and Properties → High-Performance Computing (HPC) for MHD Simulations

This learning path guides graduate students in solar physics through the theoretical foundations and practical skills needed to model the solar wind from its origin in the corona to its interaction with Earth's magnetosphere. It covers MHD theory, numerical methods, empirical and data-driven models, and culminates in applying these to space weather prediction.