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

fe_15.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 (31,32): Eissner, W., Galavis, M.E., Mendoza, C., Zeippen, C.J., 1999, A&AS, 137, 165
%Experimental energy levels (50,51,52): Reader, J., Sugar, J., 1975, J.Phys.Chem.Ref.Data, 4, 424
%Theoretical energy levels (1-35): Eissner, W., Galavis, M.E., Mendoza, C., Zeippen, C.J., 1999, A&AS, 137, 165
%Theoretical energy levels (36-45): Griffin, D.C., Badnell, N.R., Pindzola, M.S., Shaw, J.A., 1999,
                                    J. Phys. B 32 2139-52 and 4129-31
%Theoretical energy levels (46-53): Bhatia, A.K., Mason, H.E., Blancard, C., 1997, ADNDT, 66, 83
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% E. Landi Jun 2001
 

fe_15.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 (31,32): Eissner, W., Galavis, M.E., Mendoza, C., Zeippen, C.J., 1999, A&AS, 137, 165
%Experimental energy levels (50,51,52): Reader, J., Sugar, J., 1975, J.Phys.Chem.Ref.Data, 4, 424
%Theoretical energy levels (36-45): Griffin, D.C., Badnell, N.R., Pindzola, M.S., Shaw, J.A., 1999,
                                    J. Phys. B 32 2139-52 and 4129-31
%Theoretical energy levels (46-53): Bhatia, A.K., Mason, H.E., Blancard, C., 1997, ADNDT, 66, 83
% Radiative data (levels 36-45): Griffin, D.C., Badnell, N.R., Pindzola, M.S., Shaw, J.A., 1999,
                                    J. Phys. B 32 2139-52 and 4129-31
% Radiative data (levels 46-53): Bhatia, A.K., Mason, H.E., Blancard, C., 1997, ADNDT, 66, 83
% Radiative data (n=3 levels): SUPERSTRUCTURE calculations by E. Landi
%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

                  Results are in agreement with Eissner et al (1999, table 3) within a few percent.

% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% E. Landi Jun 2001

fe_15.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_15.splups
%Oscillator strengths (n=3 levels): SUPERSTRUCTURE calculations by E. Landi (see fe_15.wgfa for details)
%Effective collision strengths (n=3 levels): Eissner, W., Galavis, M.E., Mendoza, C., Zeippen, C.J., 1999, A&AS, 137, 165
%Oscillator strengths (levels 36-45): Griffin, D.C., Badnell, N.R., Pindzola, M.S., Shaw, J.A., 
                     1999 J.Phys.B, 32, 2139-52 and 4129-31
%Effective collision strengths (levels 36-45): Griffin, D.C., Badnell, N.R., Pindzola, M.S., 
           Shaw, J.A., 1999 J.Phys.B, 32, 2139-52 and 4129-31
%Collision strengths (levels 46-53): Bhatia, A.K., Mason, H.E., Blancard, C., 1997, ADNDT, 66, 83
%Oscillator strengths (levels 46-53): Bhatia, A.K., Mason, H.E., Blancard, C., 1997, ADNDT, 66, 83
%Comment: original n=3 upsilons are provided for temperatures in the range 5.0 <= log T <= 7.0
%Comment: original upsilons for levels 36-45 are provided for temperatures in the range 5.05 <= log T <= 7.05
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Enrico Landi Jun 2001

fe_15.psplups (proton collision data)

contains the spline fits to the scaled proton collision strengths.

 

%filename: fe_15.psplups
%rates: Landman, D.A., Brown, T., 1979, ApJ 232, 636
%energies: Observed energies from CHIANTI .elvlc file.
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Peter Young   18-May-2001

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

fe_15_table.html (html table)


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