|
Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.arcetri.astro.it/science/chianti/chianti_5.1/database/cl/cl_2_table.html
Дата изменения: Wed Sep 14 18:43:24 2005 Дата индексирования: Sat Dec 22 14:28:14 2007 Кодировка: Поисковые слова: п п п п п п п п п п п п п п п п п п п п п п п п п |
Here you find various information on the brightest lines, ordered in wavelength:
Wavelengths (Angstroms); weighted oscillator strengths (gf);
transition probabilities (A);
intensities (normalised) at
106 , 1010, 1015, 1020
cm-3;
together with:
Configuration; Term; Index of the level (1=ground); Energy (observed if available - otherwise theoretical);
of the lower (l) and upper levels (u)
Note that intensities have been calculated at log T[K]=4.30, where the ion fraction peaks in ionization equilibrium. Only lines brighter than 0.001 the strongest line (at all densities) are retained.
Wavelength |
gf |
Aul |
R |
R |
R |
R |
Cl |
Tl |
Cu | Tu |
Il | Iu |
El | Eu |
(A) | (s-1) |
(106) |
(1010) |
(1015) |
(1020) |
(cm-1) | (cm-1) |
|||||||
| 3587.0549 | 0.00e+00 | 1.98e-02 | 1.66e-03 | 1.41e-02 | 1.41e-02 | 1.41e-02 | 3s2.3p4 | 3P4/2 | 3s2.3p4 | 1S0/2 | 1 | 5 | 0 | 27878.02 |
| 3678.9031 | 0.00e+00 | 1.30e+00 | 1.06e-01 | 8.99e-01 | 8.99e-01 | 8.99e-01 | 3s2.3p4 | 3P2/2 | 3s2.3p4 | 1S0/2 | 2 | 5 | 696 | 27878.02 |
| 6163.5410 | 0.00e+00 | 2.42e+00 | 1.18e-01 | 1.00e+00 | 1.00e+00 | 1.00e+00 | 3s2.3p4 | 1D4/2 | 3s2.3p4 | 1S0/2 | 4 | 5 | 11653.58 | 27878.02 |
| 8581.0537 | 0.00e+00 | 1.04e-01 | 1.00e+00 | 4.98e-01 | 4.97e-01 | 4.97e-01 | 3s2.3p4 | 3P4/2 | 3s2.3p4 | 1D4/2 | 1 | 4 | 0 | 11653.58 |
| 9126.1025 | 0.00e+00 | 2.87e-02 | 2.60e-01 | 1.30e-01 | 1.29e-01 | 1.29e-01 | 3s2.3p4 | 3P2/2 | 3s2.3p4 | 1D4/2 | 2 | 4 | 696 | 11653.58 |
| 143678.1562 | 0.00e+00 | 7.57e-03 | 1.24e-02 | 2.87e-03 | 2.86e-03 | 2.86e-03 | 3s2.3p4 | 3P4/2 | 3s2.3p4 | 3P2/2 | 1 | 2 | 0 | 696 |
Created by Giulio Del Zanna on Wed Sep 14 15:43:24 2005