The impressive progress in ground-based and spaceborne solar observations and numerical modelling has led to dramatic changes of our picture of the Sun over the last few decades. It became clear that the solar atmosphere, i.e., the layers above the visible surface, has to be understood as a compound of intermittent, highly dynamic domains, which are intricately coupled to one another. These domains are structured on a large range of spatial scales and exhibit a multitude of physical processes, making the Sun a highly exciting plasma physics laboratory.
Fra 15. nov kl 14:00 to 15. nov kl 15:00
Fra 15. nov kl 14:00 to 15. nov kl 15:00