Fe XIII - VERSION 11.0


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

  1. fe_13.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    
    Observed energies:
    
    Del Zanna, G. 2011, A&A, 533, A12  (EUV lines)  doi = {10.1051/0004-6361/201117121},
    
    Del Zanna, G. 2012, A&A, 546, A97 (soft X-ray lines)  doi = {10.1051/0004-6361/201219923}
    
    with the following exceptions:
    
    We adopt the tentative new identifications given by Zhang et al. (2021, ApJ, 257,2,56)
    for the 3D-3F transitions: 7-60, 9-65 , 8-61 
    observed by Del Zanna (2012) at 201.49, 197.02, 199.24 Angstroms.
    We also adopt the new identification given by Zhang et al. (2021)
    for the  7-331 line at 76.867 Angstroms.
    
    We note that several other tentative identifications are  given  by Zhang et al.
    
    
    Theoretical energies (second column): whenever available,
    (i.e. all except the last few states where we have  AUTOSTRUCTURE energies)
    MCDHF calculation by
    Zhang X.H., Del Zanna G., Wang K., Rynkun P., Jonsson P., 
             Godefroid M., Gaigalas G., Radziute L., Ma L.H., Si R., 
             Xiao J., Chen Z.B., Yan J., Wu Y., Chen C.Y., 2021, ApJ, 257,2,56
     doi = {10.3847/1538-4365/ac2a3f}	 
    assuming the level identifications given by Zhang et al.
    
    
    Theoretical energies (third column): AUTOSTRUCTURE calculation by 
    Del Zanna, G. & Storey, P. J. 2012, A&A, 543, A14
     doi		= {10.1051/0004-6361/201219193}
     
    Note: the theoretical energies are the 'best energies', i.e. 
    are the empirically-adjusted theoretical energies.
    
    
    Produced for the CHIANTI database by Giulio Del Zanna  Apr 2023
    
    
    -1
     
    

  3. fe_13.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.

     
    
    
    Observed energies:
    
    Del Zanna, G. 2011, A&A, 533, A12  (EUV lines)  doi = {10.1051/0004-6361/201117121},
    
    Del Zanna, G. 2012, A&A, 546, A97 (soft X-ray lines)  doi = {10.1051/0004-6361/201219923}
    
    with the following exceptions:
    
    We adopt the tentative new identifications given by Zhang et al. (2021, ApJ, 257,2,56)
    for the 3D-3F transitions: 7-60, 9-65 , 8-61 
    observed by Del Zanna (2012) at 201.49, 197.02, 199.24 Angstroms.
    We also adopt the new identification given by Zhang et al. (2021)
    for the  7-331 line at 76.867 Angstroms.
    
    We note that several other tentative identifications are  given  by Zhang et al.
    
    
    Theoretical energies: whenever available,
    MCDHF calculation by
    Zhang X.H., Del Zanna G., Wang K., Rynkun P., Jonsson P., 
             Godefroid M., Gaigalas G., Radziute L., Ma L.H., Si R., 
             Xiao J., Chen Z.B., Yan J., Wu Y., Chen C.Y., 2021, ApJ, 257,2,56
     doi = {10.3847/1538-4365/ac2a3f}	 
    assuming the level identifications given by Zhang et al.
    
    otherwise
    
    AUTOSTRUCTURE calculation by 
    Del Zanna, G. & Storey, P. J. 2012, A&A, 543, A14
     doi		= {10.1051/0004-6361/201219193}
    
    gf and A-values:
    Del Zanna, G. & Storey, P. J. 2012, A&A, 543, A14
    
    Only transitions with a branching ratio of 10^-5 have been retained.
    
    
    Produced for the CHIANTI database by Giulio Del Zanna  Apr 2023
     
    %File processed with wgfa_tidy by pryoung on 31-May-2023
    %File processed with wgfa_tidy by pryoung on 31-May-2023
    

  5. fe_13.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    
    Produced for the CHIANTI database  by Giulio Del Zanna Apr 2023
    
     doi		= {10.1051/0004-6361/201219193}                          
    Del Zanna, G. & Storey, P. J. 2012, A&A, 543, A14              
    
    Data from:                                                     
    
    

  7. fe_13.psplups (proton collision data)
  8. contains the spline fits to the scaled proton collision strengths.

     
    
    %filename: fe_13.psplups
    %rates: Landman D.A., A&A 43, 285, 1975
    %energies: Landman D.A., A&A 43, 285, 1975
    %comment: Landman tabulates rates between the individual magnetic sublevels of 
        the ground configuration levels. For CHIANTI we sum over these 
        sublevels using Eq. 8 of Landman.
    %comment: These fits reproduce the original data to within 2%. The original 
        data cover the temperature range 1e-6 to 3e-6.
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % Peter Young   12-Jun-2001
    


    The html tables below contain the radiative data of the brightest lines sorted in wavelength

    Page created by Giulio Del Zanna on Tue Dec 3 13:23:56 2024