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: http://www.arcetri.astro.it/science/chianti/chianti_4.2/database/fe/fe_23.html
Дата изменения: Thu Dec 4 19:12:59 2003 Дата индексирования: Sat Dec 22 14:02:10 2007 Кодировка: Поисковые слова: п п п п р п р п р п |
The CHIANTI database consists of 4 primary ASCII files for each ion in the database.
contains the energy levels in cm^(-1) It includes both experimental data and theoretical values of the levels energies.
References:
%observed energy levels: Shirai,T., Sugar,J., Musgrove,A., Wiese,W.L., 2000, J.Phys.Chem.Ref.Data, Monograph 8
%observed energy levels (12,21,22,25,29,34,37,39-42): Martin,W.C., Sugar,J., Musgrove,A., Dalton,G.R.,
1995, NIST Database, Version 2.0, NIST Standard Reference Database 61.
%comment: the following NIST observed energy levels have been changed.
old value new value
2p3d 3F2 9646000 9638000
3D2 9728000 9646000
1D2 9638000 9728000
3P2 9753000 9753000
%theoretical energy levels (n=2): Chidichimo,M.C., Zeman,V., Tully,J.A., Berrington,K.A., 1999,A&AS, 137, 175
%theoretical energy levels (n=3): Sampson,D.H., Goett, S.J., Clark, R.E.H., 1984, ADNDT, 30, 125
%theoretical energy levels (n=4): Bhatia, 1996, unpublished calculations
%Observed energy level innershell: Martin,W.C., Sugar,J., Musgrove,A., Dalton,G.R., 1995, NIST Database,
Version 2.0, NIST Standard Reference Database 61.
%theoretical energy levels innershell: from the Flexible Atomic Code (developed by Dr. Ming-Feng Gu)
%comment: innershell levels have been added to account for important spectral features at around 1.870 A
(Oct 2003). All the rest is unchanged.
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% E.Landi - Oct 2003
contains wavelengths, gf and A values for each transition. Wavelengths are based on experimental level energies where available; wavelengths calculated from theoretical energies are less accurate and are given as negative values.
References:
%observed energy levels: Shirai,T., Sugar,J., Musgrove,A., Wiese,W.L., 2000, J.Phys.Chem.Ref.Data, Monograph 8
%observed energy levels (12,21,22,25,29,34,37,39-42): Martin,W.C., Sugar,J., Musgrove,A., Dalton,G.R.,
1995, NIST Database, Version 2.0, NIST Standard Reference Database 61.
%theoretical energy levels (n=2): Chidichimo,M.C., Zeman,V., Tully,J.A., Berrington,K.A., 1999, A&AS, 137, 175
%theoretical energy levels (n=3): Sampson,D.H., Goett, S.J., Clark, R.E.H., 1984, ADNDT, 30, 125
%theoretical energy levels (n=4): Bhatia, 1996, unpublished calculations
%comment: the following NIST observed energy levels have been changed.
old value new value
2p3d 3F2 9646000 9638000
3D2 9728000 9646000
1D2 9638000 9728000
3P2 9753000 9753000
%oscillator strengths (n=2 levels): Zhang, H.L., Sampson. D.H., 1992, ADNDT, 1992, 52, 143
%oscillator strengths (n=3 levels): Sampson,D.H., Goett,S.J., Clark,R.E.H., 1984, ADNDT, 30, 125
%oscillator strengths (n=4 levels): Bhatia, 1996, unpublished calculations
%comment: gf values for transitions 19-26 and 23-26 were simply taken to be
equal to the O V gf values reported by Hibbert, 1980, J. Phys. B, 13, 1721.
The A values were obtained from the gf values by using the wavelengths listed.
%Observed energy level innershell: Martin,W.C., Sugar,J., Musgrove,A., Dalton,G.R., 1995, NIST Database,
Version 2.0, NIST Standard Reference Database 61.
%theoretical energy levels innershell: from the Flexible Atomic Code (developed by Dr. Ming-Feng Gu)
%Radiative data innershell: from the Flexible Atomic Code (developed by Dr. Ming-Feng Gu)
%comment: The wavelength of the 1 - 57 transition has been considered observed even though it comes from
theoretical energies.
%comment: innershell levels have been added to account for important spectral features at around 1.870 A
(Oct 2003). All the rest is unchanged.
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% E. Landi - Oct 2003
contains the spline fits to the electron collision strengths scaled according to 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.
References:
%filename: fe_23.splups
%oscillator strengths (n=2 levels): Zhang, H.L., Sampson. D.H., 1992, ADNDT, 1992, 52, 143
%oscillator strengths (n=3 levels): Sampson,D.H., Goett,S.J., Clark,R.E.H., 1984, ADNDT, 30, 125.
%oscillator strengths (n=4 levels): Bhatia, 1996, unpublished calculations
%effective collision strengths (n=2): Chidichimo,M.C., Zeman,V., Tully,J.A., Berrington,K.A., 1999, A&AS, 137, 175
%collision strengths (n=3): Sampson, D.H., Goett, S.J., Clark, R.E.H., 1984, ADNDT, 30, 125
%collision strengths all other transitions: Bhatia A.K. (private communications)
%gf values innershell: from the Flexible Atomic Code (developed by Dr. Ming-Feng Gu)
%Collision strengths innershell: from the Flexible Atomic Code (developed by Dr. Ming-Feng Gu)
%comment: Effective collision strengths from Chidichimo et al are provided for 6.3 < log T < 8.1
%comment: innershell levels have been added to account for important spectral features at around 1.870 A
(Oct 2003). All the rest is unchanged.
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Enrico Landi May 2001 (n=2, n=4); K.P. Dere Sept. 97 (n=3); Enrico Landi Oct 2003 (innershell)
contains the spline fits to the scaled proton collision strengths.
References:
%filename: fe_23.psplups %rates: Ryans R.S.I., Foster-Woods V.J, Copeland F., Keenan F.P., Matthews A., Reid R.H.G., 1998, ADNDT 70, 179-229 %energies: CHIANTI database, ver.1, Dere et al., A&AS 125, 149, 1997 %comment: Fits valid for temperatures 4e6 to 3e8 K. %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % Peter Young 24-Oct-00