Unsere Sonne macht es vor: Leichte Atomkerne verschmelzen zu schwereren. Gewaltige Energiemengen werden bei dieser Kernfusion freigesetzt: Es herrschen Temperaturen von mehr als 100 Millionen Grad Celsius. Forscher vom Max Planck-Institut f
This book bridges the gap between general plasma physics lectures and the real world problems in MHD stability. In order to support the understanding of concepts and their implication, it refers to real world problems such as toroidal mode coupling or nonlinear evolution in a conceptual and phenomenological approach. Detailed mathematical treatment will involve classical linear stability analysis and an outline of more recent concepts such as the ballooning formalism. The book is based on...
