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]=4.95, 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) |
|||||||
| 208463.6250 | 0.00e+00 | 2.98e-03 | 6.47e-03 | 7.03e-06 | 6.22e-06 | 6.22e-06 | 3d4 | 5D3 | 3d4 | 5D4 | 4 | 5 | 803.1 | 1282.8 |
| 259201.6562 | 0.00e+00 | 2.65e-03 | 4.24e-03 | 3.94e-06 | 3.49e-06 | 3.49e-06 | 3d4 | 5D2 | 3d4 | 5D3 | 3 | 4 | 417.3 | 803.1 |
Created by Giulio Del Zanna on Wed Apr 16 17:43:03 2025