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: http://www.arcetri.astro.it/science/chianti/chianti_3.03/elements/fe/fe_13.html
Дата изменения: Thu Jul 20 21:44:20 2000 Дата индексирования: Sat Dec 22 14:07:07 2007 Кодировка: Поисковые слова: south pole |
% Filename: fe_13.elvl %produced as part of the Arcetri/Cambridge/NRL atomic data collaboration %energy levels(1-3): Penn & Kuhn, Ap.J.Lett, 1995, in press %energy levels(6,9- 11,13,15,16,22): Jupen et al., MNRAS, 264, 627, 1993 %energy levels(4-5,7-8,12,14,17-21,23-27): NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61, 1995. %Theoretical energy levels: Gupta, G.P., Tayal, S.S., 1998, ApJ, 506, 464 %Theoretical energy for level 6: Fawcett & Mason, 1989, ADNDT, 43, 245
% effective collision strengths: Gupta, G.P., Tayal, S.S., 1998, ApJ, 506, 464 %produced as part of the Arcetri/Cambridge/NRL atomic data base collaboration 'CHIANTI' % % E. Landi Apr. 1999
% A values: computed from 'superstructure' using a 24 configuration model of Fe XIII. % comment: the model of Fe XIII included the following configurations: 3s2 {3p2 3p3d 3d2} 3s23p {4s 4p 4d 4f} 3s3p2 {3d 4s 4p 4d 4f} 3p3 {3d 4s 4p 4d} 3s3d {4s 4p 4d 4f} 3p4 3s {3p3 3d3 3p3d2} % note: that level 18 is metastable, and can decay down to levels in the 3s3p^3 and 3s^23p3d configurations via electric quadrupole and magnetic dipole transitions. However, the strongest transitions are down to the ground configuration via two magnetic QUADRUPOLE transitions. These transitions are accurately known since the line strength hardly changes when extra configurations are added to the model.