The CHIANTI atomic database was first released in 1996 and has since become the standard resource for the interpretation of UV spectra from the transition regions and coronae of the Sun and other cool stars. We describe the contents of the most recent release (v.3) and some of the uses that have been found for the database.
The Future of Cool-Star Astrophysics: 12th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
- Pub Date:
- October 2003