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

fe_15d.elvlc (energy levels)

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

 
%Experimental energy levels: Shirai,T., Sugar,J., Musgrove,A., Wiese,W.L.,2000, J.Phys.Chem.Ref.Data, Monograph 8
%Experimental energy levels (above ionization): Mendoza, C., Kallman, T.R., Bautista, M.A., Palmeri, P., 2004, A&A, 414, 377
%Theoretical energy levels: Eissner, W., Galavis, M.E., Mendoza, C., Zeippen, C.J., 1999, A&AS, 137, 165
%Theoretical energy levels (above ionization): Mendoza, C., Kallman, T.R., Bautista, M.A., Palmeri, P., 2004, A&A, 414, 377
%comment: the theoretical energies from Mendoza et al have been used as experimental ones
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% E. Landi - Jan 2005
 

fe_15d.wgfa (radiative data)

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.

 
%Experimental energy levels: Shirai,T., Sugar,J., Musgrove,A., Wiese,W.L.,2000, J.Phys.Chem.Ref.Data, Monograph 8
%Experimental energy levels (above ionization): Mendoza, C., Kallman, T.R., Bautista, M.A., Palmeri, P., 2004, A&A, 414, 377
%Radiative data (n=3 levels): Landi & Gu 2005, ApJ, in press
%comment:         The configurations used for the SUPERSTRUCTURE calculations are

                     3s2, 3s3p, 3p2, 3s3d, 3p3d, 3d2
                     3s4s, 3s4p, 3s4d, 3s4f
                     3p4s, 3p4p, 3p4d, 3p4f
                     3d4p, 3d4d, 3d4f, 4p2, 4d2
                     3s5s, 3p5s

%A values (above ionization): Mendoza, C., Kallman, T.R., Bautista, M.A., Palmeri, P., 2004, A&A, 414, 377
%Autoionization rates: Mendoza, C., Kallman, T.R., Bautista, M.A., Palmeri, P., 2004, A&A, 414, 377
%comment: A values for levels 2 and 11 to 20 are a fix
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration CHIANTI
%
% E.Landi - Jan 2005

fe_15d.splups (electron collision data)

contains the spline fits to the electron collision strengths scaled according the rules formulated by Burgess and Tully (1992). Accurate replication of the temperature averaged collision strength over a wide range of temperatures can be accomplished with the data in this file.

 

%filename: fe_15d.splups
%Effective collision strengths and autoionization rates: Mendoza, C., Kallman, T.R., Bautista, M.A., Palmeri, P., 2004, A&A, 414, 377
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
%  E. Landi - Sep 2005

---

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

fe_15d_table.html (html table)


Last revised by G. Del Zanna on 4-Sep-2009