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]=6.10, 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) |
|||||||
| 165.5280 | 2.67e-01 | 3.25e+10 | 1.00e+00 | 1.00e+00 | 1.00e+00 | 1.00e+00 | 2s2.2p5 | 2P3/2 | 2s.2p6 | 2S1/2 | 1 | 3 | 0 | 604130 |
| 170.6430 | 1.28e-01 | 1.47e+10 | 4.37e-01 | 4.37e-01 | 4.37e-01 | 4.37e-01 | 2s2.2p5 | 2P1/2 | 2s.2p6 | 2S1/2 | 2 | 3 | 18110 | 604130 |
| 5521.8208 | 0.00e+00 | 1.06e+02 | 4.48e-02 | 3.76e-02 | 2.33e-06 | 2.15e-10 | 2s2.2p5 | 2P3/2 | 2s2.2p5 | 2P1/2 | 1 | 2 | 0 | 18110 |
Created by Giulio Del Zanna on Fri Aug 5 13:54:16 2005