The CHIANTI database has the following primary ASCII files for this ion:
contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.
%filename: cl_4.elvlc %observed energy levels: Version 3.0.3 of the NIST online database. http://physics.nist.gov/PhysRefData/ASD/index.html %theoretical energies: No theoretical energies available. % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % Peter Young - 20-Jun-2006
contains wavelengths, gf and A values of the transitions. The wavelengths are based on the experimental energy levels and should be the best available. Wavelengths calculated from the theoretical energies are of an indeterminate accuracy and their values are presented as negative values of the calculated wavelength.
%filename: cl_4.wgfa %observed energy levels: Version 3.0.3 of the NIST online database. http://physics.nist.gov/PhysRefData/ASD/index.html %A-values: Mendoza, C. & Zeippen, C.J., 1982, MNRAS, 199, 1025 % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % Peter Young - 20-Jun-2006 %File processed with wgfa_tidy by pryoung on 6-Mar-2019 %File processed with wgfa_tidy by pryoung on 31-May-2023
contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).
% Peter Young - 20-Jun-2006 % % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration %comment: The fits reproduce the original data to within 0.20% over the temperature range 3.0 <= logT <= 5.0. %Upsilons: Galavis, M.E., Mendoza, C., Zeippen, C.J. 1995, A&ASS 111, 347 %Theoretical energies: No theoretical energies available - observed energies from .elvlc file used instead. %filename: cl_4.splups
Page created by Giulio Del Zanna on Tue Dec 3 13:23:29 2024