Author:
Landi E.,Dere K.P.,Young P.R.,Landini M.,Mason H.E.,Zanna G. Del
Abstract
AbstractThe CHIANTI database contains assessed atomic energy levels, wavelengths, radiative transition probabilities and excitation rates necessary to calculate line emissivities and synthetic spectra of a large number of ions of astrophysical interest. CHIANTI also includes a suite of programs to carry out plasma diagnostics. In the present paper we describe the contents of the CHIANTI database, its main applications and its future developments.
Publisher
Cambridge University Press (CUP)
Cited by
1 articles.
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