POSTER PAPER 11.06
CHIANTI -- An Atomic Database for UV and X-ray Cool Star Spectroscopy
Young, P.R., Landi, E., Bromage, G.E., Del Zanna, G., Dere, K.P., Landini, M., Mason, H.E.
Institute: Smithsonian Astrophysical Observatory
Institute: Naval Research Laboratory
Institute: University of Central Lancashire
Institute: University of Cambridge
Institute: Arcetri Astrophysical Observatory
Contact Email: G.Del-Zanna@damtp.cam.ac.uk
Abstract:
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.
Index Keywords: CHIANTI; SOHO
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Manuscript submitted: 2001-Sep-06
"The Future of Cool-Star Astrophysics", 2003, Eds. A. Brown,
G. M. Harper, & T. R. Ayres.
Proceedings of 12th Cambridge Workshop on Cool Stars, Stellar Systems,
& The Sun,
© 2003 University of Colorado.