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The CHIANTI Database

Published online by Cambridge University Press:  30 March 2016

E. Landi,
K.P. Dere,
P.R. Young,
M. Landini,
H.E. Mason and
G. Del Zanna
E. Landi
Affiliation:
Naval Research Laboratory, Washington, DC 20375, USA
K.P. Dere
Affiliation:
Naval Research Laboratory, Washington, DC 20375, USA
P.R. Young
Affiliation:
Rutherford Appleton Laboratory, Chilton, Didcot, 0X11 OQX, UK
M. Landini
Affiliation:
University of Florence, Largo E. Fermi 2, 51025 Firenze, Italy
H.E. Mason
Affiliation:
Dept. of Appl. Math, and Theor. Phys., University of Cambridge, UK
G. Del Zanna
Affiliation:
Dept. of Appl. Math, and Theor. Phys., University of Cambridge, UK

Abstract

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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.

Information

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005, pp. 653 - 656
Copyright
Copyright © Astronomical Society of Pacific 2005

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