Fast MHD oscillations in cylindrical prominence fibrils
Some observations suggest that quiescent solar prominences can be considered as composed by small-scale loops, or fibrils, which are stacked one after another in both the vertical and horizontal directions. In a previous work we studied, in Cartesian geometry, the propagation of fast MHD waves in a two-dimensional magnetostatic model representing
Díaz, A. J. et al.
Fecha de publicación:
10
2002