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.
Theoretical energies: Fernandez-Menchero, Del Zanna and Badnell, A&A, 2014, 566, A104 doi = {10.1051/0004-6361/201423864} Note: only the bound levels up to n=5 have been retained and indexing has been changed for levels above 116 Observed energies for the lower levels: NIST Atomic Spectra Database, (ver. 5.7.1), [Online]. https://physics.nist.gov/PhysRefData/ASD/levels_form.html Other observed energy levels: 23,24,25,28,32,35,37,40 ,41 ,45 68,72 75,76,77,80,82,84,85,91,92,96,97, 137, 149, 153,160 are from Khardi, S., Buchet-Poulizac, M.C., Buchet, J.P., Carre', M., Denis, A., Desesquelles, J., Livingstone, A.E., Martin, S., & Ouerdane, Y. 1994, Phys. Scr., 49, 571 Note: for the level 158 2p 5f 1F3 Khardi gives 2950400 which deviates substantially from the theoretical value. Produced as part of the 'CHIANTI' atomic data base collaboration by Giulio Del Zanna, May 2020 -1
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.
gf-values, A-values and theoretical energies: Fernandez-Menchero, Del Zanna and Badnell, A&A, 2014, 566, A104 doi = {10.1051/0004-6361/201423864} Only transition probabilities with a branching ratio greater than 10^(-5) have been retained. Note: only the bound levels up to n=5 have been retained and indexing has been changed for levels above 116 gf-values, A-values for the n=2,3 (lowest 20 levels): MBPT calculations by Wang, K. et al., 2015, ApJS, 218, 16 doi = {10.1088/0067-0049/218/2/16} Observed energies for the lower levels: NIST Atomic Spectra Database, (ver. 5.7.1), [Online]. https://physics.nist.gov/PhysRefData/ASD/levels_form.html Other observed energy levels: 23,24,25,28,32,35,37,40 ,41 ,45 68,72 75,76,77,80,82,84,85,91,92,96,97, 137, 149, 153,160 are from Khardi, S., Buchet-Poulizac, M.C., Buchet, J.P., Carre', M., Denis, A., Desesquelles, J., Livingstone, A.E., Martin, S., & Ouerdane, Y. 1994, Phys. Scr., 49, 571 ' Note: for the level 158 2p 5f 1F3 Khardi gives 2950400 which deviates substantially from the theoretical value. Produced as part of the 'CHIANTI' atomic data base collaboration by Giulio Del Zanna, May 2020 %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).
Giulio Del Zanna, May 2020 Produced as part of the 'CHIANTI' atomic data base collaboration by Note: only the bound levels up to n=5 have been retained. doi = {10.1051/0004-6361/201423864} Fernandez-Menchero, Del Zanna and Badnell, A&A, 2014, 566, A104 oscillator strengths and effective collision strengths:
contains the spline fits to the scaled proton collision strengths.
%filename: al_10.psplups %rates: Ryans R.S.I., Foster-Woods V.J, Copeland F., Keenan F.P., Matthews A., Reid R.H.G., 1998, ADNDT 70, 179-229 %energies: Martin W.C., Sugar J., Musgrove A., Dalton G.R., 1995, NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61. %comment: Fits valid for temperatures 2e5 to 5e7 K. %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % Peter Young, 19-Oct-00
Page created by Giulio Del Zanna on Tue Dec 3 13:23:00 2024