Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.8501d&link_type=abstract
American Astronomical Society, 188th AAS Meeting, #85.01; Bulletin of the American Astronomical Society, Vol. 28, p.961
Astronomy and Astrophysics
Astrophysics
4
Scientific paper
A comprehensive set of accurate atomic data is required for analyses of astrophysical and solar spectra. CHIANTI provides an atomic database of energy levels (wavelengths), radiative data and electron excitation data for ions which are abundant in astrophysical plasmas. The most recent electron excitation data have been assessed and stored following the method of Burgess and Tully (1992). CHIANTI includes IDL (Interactive Data Language) routines to produce optically thin synthetic spectra for lambda > 50 Angstroms, assuming equilibrium conditions. It also includes IDL routines to calculate theoretical line intensities required for electron density or temperature diagnostics and emission measure studies. The CHIANTI atomic database and supporting IDL routines are available by anonymous FTP.
Dere Ken P.
Landi Enrico
Mason Harris E.
Monsignori-Fossi Brunella C.
Young Paul R.
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