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: http://www.arcetri.astro.it/science/chianti/chianti_5.1/database/fe/fe_24d.html
Дата изменения: Thu Sep 15 16:54:57 2005 Дата индексирования: Sat Dec 22 14:09:11 2007 Кодировка: |
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 (below ionization): Sugar, J., Corliss, C., 1979, J.Phys.Chem.Ref.Data, 8, 865 %observed energy levels (below ionization): Kelly, R.L., 1987, J.Phys.Chem.Ref.Data 16, Suppl. 1 %comment: 5s from Kelly %Theoretical energy levels: Zhang, H.L., Sampson, D.H., Fontes, C.J., 1990, ADNDT, 44, 31 %observed energy levels (n=2 above ionization): Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., 2003, A&A, 403, 1175 %theoretical energy levels (n=2 above ionization): Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., 2003, A&A, 403, 1175 %theoretical energy levels (n>2 above ionization): calculations of Safronova reported in Kato et al., 1997, ADNDT, 67, 225 %Comment: the theoretical energies from Palmeri et al. have been used as experimental ones when the latter were unavailable % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E. Landi - Feb 2005
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 (below ionization): Sugar, J., Corliss, C., 1979, J.Phys.Chem.Ref.Data, 8, 865 %observed energy levels (below ionization): Kelly, R.L., 1987, J.Phys.Chem.Ref.Data 16, Suppl. 1 %observed energy levels (above ionization, n=2): Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., 2003, A&A, 403, 1175 %theoretical energy levels (n>2 above ionization): calculations of Safronova reported in Kato et al., 1997, ADNDT, 67, 225 %oscillator strengths (below ionization): H.L.Zhang, D.H.Sampson, C.J.Fontes, 1990, ADNDT, 44, 31 %oscillator strengths (below ionization): Martin,I., Karwowski,J., Diercksen,G.H.F., Barrientos, C., 1993, A&AS, 100, 595 %A and gf values (above ionization, n=2): Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., 2003, A&A, 403, 1175 %Autoionization rates (above ionization, n=2): Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., 2003, A&A, 403, 1175 %A and gf values (above IP, n>2): calculations of Safronova reported in Kato et al., 1997, ADNDT, 67, 225 %A and gf values (Transitions between n=2 to 1s2l3l): calculations of Cornille reported in Kato et al., 1997, ADNDT, 67, 225 %Autoionization rates (above ionization, n>2): calculations of Safronova reported in Kato et al., 1997, ADNDT, 67, 225 %comment: Cornille's data for levels 74, 88 have been exchanged with those for levels 88, 153 respectively, due to changes in LS coupling notation. The exchange has been based on comparison with autoionization and radiative decay rates between Cornille and Safronova's calculations for n=3 to 1s2l3l satellite lines (E. Landi, 24 Aug 2004). %comment: theoretical energies have been used as experimental values for the dielectronic transitions %comment: corrected the wavelengths of dielectronic lines from n=6 levels (Sep 2004) % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E. Landi - Sep 2005
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_24d.splups %Effective collision strengths and autoionization rates (n=2): Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., 2003, A&A, 403, 1175 %Effective collision strengths and autoionization rates (n>2): calculations of Safronova reported in Kato et al., 1997, ADNDT, 67, 225 %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E. Landi - Oct 2004