Cl XI - VERSION 10.0.2


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

  1. cl_11.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename: cl_11.elvlc
    %Observed energy levels: Edlen, 1984, Phys.Scripta, 30, 135
    %Theoretical energy levels ground configuration: Merkelis et al, 1999, Physica Scripta, 59, 122
    %Theoretical energy levels excited configurations: Merkelis et al, 1997, Physica Scripta, 56, 41
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % E. Landi - 2004
     
    

  3. cl_11.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_17.wgfa
    %Observed energy levels: Edlen, 1984, Phys.Scripta, 30, 135
    %A values for transitions within the ground configuration: Merkelis et al, 1999, Physica Scripta, 59, 122
    %A values for all other transitions: Merkelis et al, 1997, Physica Scripta, 56. 41
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % E.Landi - Oct 2004
    %File processed with wgfa_tidy by pryoung on  6-Mar-2019
    

  5. cl_11.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    % E. Landi - Oct 2004
    %
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %Collision strengths: Zhang & Sampson, 1999, ADNDT, 72, 153
    %Oscillator strengths: Zhang & Sampson, 1999, ADNDT, 72, 153
    %filename: cl_11.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_11_table.html (html table)

    Page created by Giulio Del Zanna on Wed Jun 8 16:02:54 2022