Solar wind modeling: global MHD to kinetic treatments. KU Leuven
In the present work we use analytical and computational methods in order to examine different dynamical scales in the solar atmosphere and the solar wind.
The latter represents the expansion of the atmosphere to large radial distances, further than the Earth's orbit.
After the introduction presented in chapter 1, we start our analysis with investigating and presenting potential force-free field extrapolations based on observational ...