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: http://www.arcetri.astro.it/science/chianti/chianti_4.01/database/s/s_14d.html
Дата изменения: Mon Dec 2 20:41:44 2002 Дата индексирования: Sat Dec 22 14:04:04 2007 Кодировка: Поисковые слова: m 31 |
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: Martin, W.C., Zalubas, R., Musgrove, A., 1990, J.Phys.Chem.Ref.Data, 19, 821 %Theoretical energy levels: Zhang, H.L., Sampson, D.H., Fontes, C.J., 1990, ADNDT, 44, 31 %comment: 6l energy levels are a rough estimate %comment: S XV (1S<0>) Limit: 5702400 %energy levels (above IP): 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 % % Ken Dere Jan 1999
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: Martin, W.C., Zalubas, R., Musgrove, A., 1990, J.Phys.Chem.Ref.Data, 19, 821 %Theoretical energy levels: Zhang, H.L., Sampson, D.H., Fontes, C.J., 1990, ADNDT, 44, 31 %energy levels (above IP): calculations of Safronova reported in Kato et al., 1997, ADNDT, 67, 225 %comment: 6l energy levels are a rough estimate %oscillator strengths: H.L. Zhang, D.H. Sampson, C.J. Fontes, 1990, ADNDT, 44, 31 %oscillator strengths: Martin, I., Karwowski, J., Diercksen, G.H.F., Barrientos, C., 1993, A&AS, 100, 595 %oscillator strengths: Wiese, W.L., Smith, M.W., Glennon, B.M., 1966, Atomic Transition Probabilities, NSRDS-NBS-4 %note: hydrogenic f values %A values (above IP): calculations of Safronova reported in Kato et al., 1997, ADNDT, 67, 225 %comment: theoretical energies have been used as experimental values for the dielectronic transitions %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % Ken Dere Jan 1999
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: s_14d.splups %collision strength values from 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 % % Ken Dere - Jan 1999