Fast MHD oscillations in prominence fine structures
High-resolution observations suggest that quiescent solar prominences are made of small-scale fibrils stacked one after another in both the vertical and horizontal directions. These fibrils are interpreted as the cool, highermost part of much larger coronal loops which are rooted in the solar photosphere. On the other hand, there is some evidence
Díaz, A. J. et al.
Fecha de publicación:
12
2001