Cl II - VERSION 10.0.2


The CHIANTI database has the following primary ASCII files for this ion:

  1. cl_2.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename: cl_2.elvlc
    %observed energy levels: Fuhr, J.R., et al., "NIST Atomic Spectra Database" Ver. 2.0, March 1999, NIST Physical Reference Data
    %theoretical energy levels: Wilson, N.J., Bell, K.L. 2002, MNRAS 331, 389
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %  P.R. Young - 20-May-02
     
    

  3. cl_2.wgfa (radiative data)
  4. 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_2.wgfa
    %observed energy levels: Fuhr, J.R., et al., "NIST Atomic Spectra Database" Ver. 2.0, March 1999, NIST Physical Reference Data
    %A-values: From SSTRUCT calculation. See comments below.
    %comments: The A-values were derived using the code SSTRUCT, with a model of the 
       Cl II ion that contained the following 14 configurations:
    
       3s2.3p4
       3s.3p5
       3s2.3p3.3d
       3s2.3p3.4l  (l=s,p,d,f)
       3s2.3p3.5l  (l=s,p,d,f,g)
       3s2.3p3.6l  (l=s,p)
    
       Note that SSTRUCT is not best suited to ions with low charges, and 
       the derived A-values may not be good. However, there are no other values 
       in the literature.
    
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %  P.R. Young - 11-Jun-2002
    %File processed with wgfa_tidy by pryoung on  6-Mar-2019
    

  5. cl_2.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    %  P.R. Young - 23-Jan-03
    %
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
        transition 4-5. This has been corrected.
    %comment: An erratum was published in MNRAS 338, 544, revising the upsilons for 
        For the 3P level splitting observed energies were used.
    %comment: Wilson & Bell gave theoretical energies only for LS-resolved levels.
    %effective collision strengths: Wilson, N.J., Bell, K.L. 2002, MNRAS 331, 389 and MNRAS 338, 544
    %theoretical energy levels: Wilson, N.J., Bell, K.L. 2002, MNRAS 331, 389
    %filename: cl_2.splups
    

  7. (proton collisional data) Not available in this VERSION.

  8. The html table below contains the radiative data of the brightest lines sorted in wavelength

    cl_2_table.html (html table)

    Page created by Giulio Del Zanna on Wed Jun 8 16:02:41 2022