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The CHIANTI Database
Published online by Cambridge University Press: 30 March 2016
Abstract
The 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.
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- Copyright © Astronomical Society of Pacific 2005
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