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Time damping of non-adiabatic magnetohydrodynamic waves in a partially ionised prominence medium: Effect of a background flow
- Source :
- Astronomy and Astrophysics; January 2011, Vol. 525 Issue: 1
- Publication Year :
- 2011
-
Abstract
- Context.The simultaneous occurrence of flows and time damped small-amplitude oscillations in solar prominences is a common phenomenon. These oscillations are mostly interpreted in terms of magnetohydrodynamic (MHD) waves.
Details
- Language :
- English
- ISSN :
- 00046361 and 14320746
- Volume :
- 525
- Issue :
- 1
- Database :
- Supplemental Index
- Journal :
- Astronomy and Astrophysics
- Publication Type :
- Periodical
- Accession number :
- ejs22609853
- Full Text :
- https://doi.org/10.1051/0004-6361/201015499