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** Atomic data from version 7 of the CHIANTI database **
%Observed energy levels (n=2 levels): Edlen, B., 1983, Physica Scripta, 28, 51
%Observed energy levels (n=3,4 levels): Lepson, J.K., Beiersdorfer, P., Behar, E., & Kahn, S.M. 2003, ApJ, 590, 604
%Observed energy levels (4,6,23,64,65,79): Fawcett, B.C., Gabriel, A.H., & Paget, T.M. 1971, J.Phys.B, 4, 986
%Observed energy level (10): Average from measurements of Lepson et al. (2003) and Fawcett et al. (1971)
%Observed energy levels (96,97): Connerade, J.P., Peacock, N.J., Speer, R.J., 1971, Solar Physics, 18, 63
%Observed energy levels (11-17,19,21,22,25-28,31-34,37,38,42,4350,51,54): Bengtsson, P., Engstroem, L., Jupen, C., 1994, Physica Scripta, 49, 297
%Comment: The energies from Bengtsson et al 1994 have been calculated using their observed wavelengths and
the energies of levels 4 to 10 (2s2.2p4.3s configuration) from the sources listed above.
%Theoretical energy levels: Witthoeft, M.C., Whiteford, A.D., & Badnell, N.R. 2007, J.Phys.B, 40, 2969
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% E. Landi - Feb 2007
%filename: ar_10.wgfa
%Observed energy levels (n=2 levels): Edlen, B., 1983, Physica Scripta, 28, 51
%Observed energy levels (n=3,4 levels): Lepson, J.K., Beiersdorfer, P., Behar, E., & Kahn, S.M. 2003, ApJ, 590, 604
%Observed energy level (10): Average from measurements of Lepson et al. (2003) and Fawcett et al. (1971)
%Observed energy levels (4,6,23,64,65,79): Fawcett, B.C., Gabriel, A.H., & Paget, T.M. 1971, J.Phys.B, 4, 986
%Observed energy levels (96,97): Connerade, J.P., Peacock, N.J., Speer, R.J., 1971, Solar Physics, 18, 63
%Observed energy levels (11-17,19,21,22,25-28,31-34,37,38,42,4350,51,54): Bengtsson, P., Engstroem, L., Jupen, C., 1994, Physica Scripta, 49, 297
%Comment: The energies from Bengtsson et al 1994 have been calculated using their observed wavelengths and
the energies of levels 4 to 10 (2s2.2p4.3s configuration) from the sources listed above.
%Theoretical energy levels: Witthoeft, M.C., Whiteford, A.D., & Badnell, N.R. 2007, J.Phys.B, 40, 2969
%Radiative data: Witthoeft, M.C., Whiteford, A.D., & Badnell, N.R. 2007, J.Phys.B, 40, 2969
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% E. Landi - Feb 2007
%filename: ar_10.splups
%Oscillator strengths: Witthoeft, M.C., Whiteford, A.D., & Badnell, N.R. 2007, J.Phys.B, 40, 2969
%Effective collision strengths: Witthoeft, M.C., Whiteford, A.D., & Badnell, N.R. 2007, J.Phys.B, 40, 2969
%comment: effective collision strengths are published for temperatures in the range 4.3 < Log T < 8.3
%comment: effective collision strengths are USED for temperatures in the range 4.9 < Log T < 7.0
%comment: data at very high or very low temperatures were sometimes discarded to improve the fit. At these
temperatures the Ar X abundance is negligible under equilibrium.
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% E. Landi - Jan 2007
2 23
1 2s2.2p5 2P3/2
2 2s2.2p5 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 1.32e+00
0 0 1.32e+00
0 0 1.32e+00
0 0 1.32e+00
0 0 1.31e+00
0 0 1.31e+00
0 0 1.30e+00
0 0 1.29e+00
0 0 1.27e+00
0 0 1.24e+00
0 0 1.19e+00
0 0 1.12e+00
0 0 1.02e+00
0 0 8.70e-01
0 0 7.01e-01
0 0 5.63e-01
0 0 4.68e-01
0 0 3.86e-01
0 0 3.36e-01
0 0 3.04e-01
0 0 2.81e-01
0 0 2.67e-01
0 0 2.41e-01
0 0 0
1 2 1.230e+02
1 4 0.0
2 2 18065.1
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