CHIANTI -- An Atomic Database for UV and X-ray Cool star spectroscopy

Details CHIANTI -- An Atomic Database for UV and X-ray Cool star spectroscopy CHIANTI -- An Atomic Database for UV and X-ray Cool star spectroscopy

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003csss...12.1119y&link_type=abstract

The Future of Cool-Star Astrophysics: 12th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (2001 July 30 - August

Astronomy and Astrophysics

Astrophysics

1

Chianti, Soho

Scientific paper

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.

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