MHD simulations of flux rope formation and eruption KU Leuven
In this thesis, we study magnetic flux rope (MFR) formation and eruption driven by photospheric converging motion. Two-and-a-half-dimensional magnetohydrodynamics (MHD) simulation and forward modelling analysis are conducted.
Chapter 1 introduces general research background. In Section 1.1, the structure and evolution of the Sun, the solar radiation feature, and the properties of solar magnetic fields are summarised. Section 1.2 reviews ...