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** Atomic data from version 7 of the CHIANTI database **
%Observed and Theoretical energies (levels 1-54): Del Zanna, Berrington, Mason, 2004, A&A, 422, 731
%Observed energy levels (55-172): NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard
Reference Database 61, 1995
%theoretical energy levels (55-172): Malinovsky et al., 1980, ApJ, 235, 665
%comment: The second column has the theoretical energies of the scattering calculations,
while the third column has the theoretical energies from the SUPERSTRUCTURE calculation
(with term energy corrections).
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Giulio Del Zanna and Peter Young - July 20, 2005
%filename: fe_10.wgfa
%Observed and Theoretical energies (levels 1-54): Del Zanna, Berrington, Mason, 2004, A&A, 422, 731
%Observed energy levels (55-172): NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard
Reference Database 61, 1995
%theoretical energy levels (55-172): Malinovsky et al., 1980, ApJ, 235, 665
%A values and oscillator strengths (levels 1-54): Del Zanna, Berrington, Mason, 2004, A&A, 422, 731
%comment: Theoretical wavelengths for levels 1-54 are obtained from the SUPERSTRUCTURE calculation
(with term energy corrections) in the .elvlc file, from Del Zanna, Berrington, Mason, 2004, A&A, 422, 731
%A values (levels 55-172): A SSTRUCT run performed by P.R.Young.
%comment: the A values for transitions between levels 55-172 have been calculated using a
configuration model of Fe X in SSTRUCT. The configurations included were:
3s2 3p5, 3s 3p6, 3s2 3p4 3d, 3s 3p5 3d, 3p6 3d
3s2 3p3 3d2, 3s 3p4 3d2
3s2 3p4 4s, 3s2 3p4 4p, 3s2 3p4 4d
3s2 3p4 4f, 3s2 3p4 5s, 3s2 3p4 5p
3s 3p5 4s, 3s 3p5 4p, 3s 3p5 5s
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Giulio Del Zanna and Peter Young - July 20, 2005
%filename: fe_10.splups
%Oscillator strengths (levels 1-54): Del Zanna, Berrington, Mason, 2004, A&A, 422, 731 (scattering calculation)
%Collision data for transitions to the first three levels: Pelan, Berrington, A&A 2001, 365, 258
%Collision data for transitions to levels up to 54: Del Zanna, Berrington, Mason, 2004, A&A, 422, 731
%collision strengths for transitions to levels 55-172: Malinovsky et al., ApJ 235, 665, 1980
%comment: Maxwellian-averaged collision strengths have been calculated in the temperature range 2.5 10^5 - 10^7 K
%comment: Although for many of the transitions involving levels >62 there
were gf values available, they have been fitted as Type 2
transitions. This is because, as Type 1 transitions they were often
difficult to fit (the 1-89 transition is a typical example).
Some of the 4s transitions (levels 55-62) showed unusual shapes
in the omega structure (e.g., 2-56, 1-58). I'm not sure how
trustworthy this data is.
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Giulio Del Zanna and Peter Young - July 20, 2005
2 23
1 3s2 3p5 2P3/2
2 3s2 3p5 2P1/2
100.0
158.5
251.2
398.1
631.0
1000.0
1584.9
2511.9
3981.1
6309.6
10000.0
15848.9
25118.9
39810.7
63095.8
100000.0
158489.2
251188.7
398107.1
630957.6
1000000.0
1584892.5
2511887.0
0
1 2 3.65e+00
0 0 3.65e+00
0 0 3.65e+00
0 0 3.65e+00
0 0 3.65e+00
0 0 3.65e+00
0 0 3.64e+00
0 0 3.64e+00
0 0 3.64e+00
0 0 3.63e+00
0 0 3.61e+00
0 0 3.59e+00
0 0 3.56e+00
0 0 3.51e+00
0 0 3.44e+00
0 0 3.33e+00
0 0 3.17e+00
0 0 2.97e+00
0 0 2.69e+00
0 0 2.27e+00
0 0 1.79e+00
0 0 1.35e+00
0 0 9.90e-01
0 0 0
1 2 6.938e+01
1 4 0.0
2 2 15683.1
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