Cl X - VERSION 11.0

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

cl_10.elvlc (energy levels)

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

 
%filename: cl_10.elvlc
%observed energy levels: Edlen, B., 1983, Phys. Scr., 28, 51
%Theoretical energy levels: Landi, E. 2005, A&A, 434, 365
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
% 
% Enrico Landi - May 2004

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:  /data2/svn/chianti/dbase/trunk/cl/cl_10/cl_10.wgfa
%filename: cl_10.wgfa
%observed energy levels: Edlen, B., 1983, Phys. Scr., 28, 51
%A values and oscillator strengths: Landi, E. 2005, A&A, 434, 365
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Enrico Landi - May 2004

 K. Dere  -  minimum branching ratio =   1.00e-05
    2017 December 06
%File processed with wgfa_tidy by pryoung on  6-Mar-2019
%File processed with wgfa_tidy by pryoung on 31-May-2023

cl_10.scups (electron collision data)

contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

 
% Enrico Landi - May 2004                                                              
%                                                                                      
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%Collision strengths: Zhang, H.L., Sampson, D.H., 2002, ADNDT, 82, 357                 
%Oscillator strengths: Zhang, H.L., Sampson, D.H., 2002, ADNDT, 82, 357                
%filename: cl_10.splups

(proton collisional data) Not available in this VERSION.

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

cl_10_table.html (html table)