Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.arcetri.astro.it/science/chianti/chianti_3.03/elements/al/al_9.html
Дата изменения: Thu Jul 20 21:42:44 2000 Дата индексирования: Sat Dec 22 14:01:06 2007 Кодировка: Поисковые слова: star trail |
%energy levels (n=2): Edlen, B, 1983, Phys. Scripta, 28, 483 %energy levels (n=3): Martin,W.C., Sugar,J., Musgrove,A., Dalton,G.R., 1995, NIST Database Version 1.0. %comment: energy of level 55 estimated by comparison with Sampson's values %theoretical energy levels: Sampson and Zhang, 1995, unpublished calculations %produced as part of the Arcetri/Cambridge/NRL atomic data base collaboration % % K.P.Dere and E.Landi 1999
% produced as part of the Arcetri/Cambridge/NRL atomic data base collaboration %produced as part of the Arcetri/Cambridge/NRL atomic data base collaboration %energy levels: Martin, W. C., Sugar, J., Musgrove, A., and Dalton, G. R., 1995, NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61. %comment: energy of level 55 estimated by comparison with Sampson's values %collision strengths: Zhang, H. L., Graziani, M., and Pradhan, A. K., 1994, A&A, 283, 319.
%energy levels (n=2): Edlen, B, 1983, Phys. Scripta, 28, 483 %energy levels (n=3): Martin,W.C., Sugar,J., Musgrove,A., Dalton,G.R., 1995, NIST Database Version 1.0 %oscillator strengths (n=3): Sampson and Zhang, 1995, unpublished calculations %note: gf and A values for transitions O5-K1 and O6-K2 are estimates