Al VI - VERSION 10.1


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

  1. al_6.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename: al_6.elvlc
    %experimental 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
    % 
    % E. Landi - May 2004
     
    

  3. al_6.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:  /data2/svn/chianti/dbase/trunk/al/al_6/al_6.wgfa
    %filename: al_6.wgfa
    %experimental energy levels: Edlen, B., 1983, Phys. Scr., 28, 51
    %Radiative data: Landi, E., 2005, A&A, 434, 365
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % E. 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
    

  5. al_6.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    % Enrico Landi 1997
    %
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %         their model was not able to adequately describe.
    %         were uncertain due to the presence of resonances close to threshold, which
    %         configuration since, as noted by the authors themselves, their Al VI upsilons
    %         Butler & Zeippen, 1994, AASS, 108, 1 for transitions within the ground 
    %comment: interpolated data were preferred over Close Coupling calculations from 
    %comment: data are most accurate in the 3.0 < Log T < 5.0 temperature range.
    %effective collision strengths: interpolated using Ne III, Mg V, Si VII, S IX, Ar XI, Ca XIII
    %filename: al_6.splups
    

  7. al_6.psplups (proton collision data)
  8. contains the spline fits to the scaled proton collision strengths.

     
    
    %filename: al_6.psplups
    %rates: Landman, D.A., ApJ 240, 709, 1980
    %energies: Observed energies from CHIANTI .elvlc file
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % Peter Young   8-Jun-2001
    


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

    al_6_table.html (html table)

    Page created by Giulio Del Zanna on Mon Jun 26 11:13:48 2023