EUV line emission during the dynamic formation of prominence condensations
Abstract
This contribution is a short summary of a paper recently submitted to Astrophysical Journal. We calculated the emission expected in EUV transition region lines during the process of dynamic formation of prominence condensations in coronal loops, as predicted by the thermal non-equilibrium model proposed by Antiochos et al. We present and discuss the principal characteristics of the line intensities and profiles synthesized from the hydrodynamic model at different times during the loop evolution.
- Publication:
-
Memorie della Societa Astronomica Italiana
- Pub Date:
- 2001
- Bibcode:
- 2001MmSAI..72..591S
- Keywords:
-
- Solar Prominences;
- Extreme UV