The Temporal Evolution of Linear Fast and Alfvén MHD Waves in Solar Coronal Arcades
The excitation and temporal evolution of fast and Alfvén magnetohydrodynamic oscillations in a two-dimensional coronal arcade are investigated. The approach is to consider an equilibrium magnetic and plasma structure and then to introduce a perturbation trying to mimic a nearby disturbance, such as a flare or filament eruption. By numerically
Rial, S. et al.
Fecha de publicación:
0
2010