Fe III d - VERSION 8.0


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

  1. fe_3d.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename: fe_3d.elvlc
    %observed energy levels: Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., Melendez M., 2003, A&A, 410, 359
    %theoretical energy levels: Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., Melendez M., 2003, A&A, 410, 359
    %Comment: the theoretical energies from Palmeri et al. have been used as experimental ones
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %  E. Landi - Feb 2005
     
    

  3. fe_3d.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: fe_3d.wgfa
    %energy levels: Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., Melendez M., 2003, A&A, 410, 359
    %A values: Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., Melendez M., 2003, A&A, 410, 359
    %autoionization rates: Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., Melendez M., 2003, A&A, 410, 359
    %comment: A values for levels 2 to 45 are a fix
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %  E. Landi - Feb 2005
    

  5. fe_3d.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    %filename: fe_3d.splups
    %Effective collision strengths and autoionization rates: Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., Melendez M., 2003, A&A, 410, 359
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %  E. Landi - Oct 2004
    
    


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

    fe_3d_table.html (html table)

    Page created by Giulio Del Zanna on Fri Sep 18 13:27:23 2015