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: mn_10.elvlc %Observed energy levels: Smitt et al. 1976, Phys. Scr., 13, 293 %Observed energy levels (3d): Shirai, T., Sugar, J., Musgrove, A., & Wiese, W.L. 2000, J.Phys.Chem.Ref.Data, Monograph 8 %Theoretical energy levels: Enrico Landi, unpublished calculation % %Produced for the CHIANTI atomic database (http://www.chiantidatabase.org) % % Original file: Enrico Landi - Dec 2008 % % Update: Peter Young, 21-Oct-2016, added NIST energies for levels 38 and 41-47. -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.
%filename: mn_10.wgfa %Observed energy levels: Smitt et al. 1976, Phys. Scr., 13, 293 %Observed energy levels (3d): Shirai, T., Sugar, J., Musgrove, A., & Wiese, W.L. 2000, J.Phys.Chem.Ref.Data, Monograph 8 %Theoretical energy levels: Enrico Landi, unpublished calculation %A and gf values: Enrico Landi, unpublished calculation % %Produced for the CHIANTI atomic database (http://www.chiantidatabase.org) % %Original file: Enrico Landi - Dec 2008 % %Update: Peter Young, 21-Oct-2016, updated wavelengths following change to .elvlc file; % no change to A-values. %File processed with wgfa_tidy by pryoung on 6-Mar-2019
contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).
% Enrico Landi - Dec 2008 % %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration %Collision strengths: Landi & Young 2009, ApJ, in press %gf values: Landi & Young 2009, ApJ, in press %filename: mn_10.splups
Page created by Giulio Del Zanna on Wed Jun 8 16:08:16 2022