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]=6.90, 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) |
|||||||
| 1.9268 | 4.33e-01 | 3.89e+14 | 1.00e+00 | 1.00e+00 | 1.00e+00 | 1.00e+00 | 2s2.2p5 | 2P3/2 | 1s.2s2.2p6 | 2S1/2 | 1 | 4 | 0 | 51902117 |
| 1.9306 | 2.17e-01 | 1.94e+14 | 4.98e-01 | 4.98e-01 | 4.98e-01 | 4.98e-01 | 2s2.2p5 | 2P1/2 | 1s.2s2.2p6 | 2S1/2 | 2 | 4 | 102597.58 | 51902117 |
Created by Giulio Del Zanna on Fri Sep 4 09:45:04 2009