A systematic study of the internal horizontal (line-of-sight) motions of quiescent prominences which were observed at the limb has been made by using fourier techniques to analyse the shift of the Ca ii K line as a function of height above the limb. The results indicate that a characteristic size for the velocity elements is present in ∼70% of the 13 prominences studied. This size of ∼4700 km is attributed to Alfvén waves induced by horizontal convective motions in the photosphere as previously suggested by Malville. The qualitative aspects of the observations are described by a simple model which is based on this hypothesis.
|Original language||English (US)|
|Number of pages||7|
|State||Published - Mar 1 1977|
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science