The CHIANTI atomic database

CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.

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Naval Research Laboratory (USA) - Rutherford Appleton Laboratory (UK)
University of Cambridge (UK) - George Mason University (USA) - Universita' degli Studi di Firenze (Italy)

CHIANTI spectral line lists

Version 6.0 Theoretical line lists and intensities

1-50 Å (pdf)
50-150 Å (pdf)
150-900 Å (pdf)
900-2000 Å (pdf)
2000-10000 Å (pdf)
10 000 - 600 000 Å (pdf)

Version 5.1 Theoretical line lists and intensities

1-50 Å (html) (pdf)
50-150 Å (html) (pdf)
150-900 Å (html) (pdf)
900-2000 Å (html) (pdf)
2000-10000 Å (html) (pdf)
10 000 - 600 000 Å (html) (pdf)

Version 4.2 (3 Dec 2003) Theoretical line lists and intensities

1-50 Å (html)
50-150 Å (html)
150-900 Å (html)
900-2000 Å (html)
2000-10000 Å (html)
10 000 - 600 000 Å (html)

Previous versions Theoretical line lists and intensities including solar identifications

1-50 Å (html) (ps) (from Dere et al., 2001, Version 3)
50-1100 Å (html) (ps) (from Dere et al., 1997, Version 1)

Last revised by G. Del Zanna on 4-Sep-2009