ic#cu28.dat
Resolved Specific Ion Data Collections
- Ion
- Cu28+
- Temperature Range
- 14.48 eV → 1.594 x 105 eV
ADF04
- Filename
- ic#cu28.dat
- Full Path
- adf04/copmm#29/ic#cu28.dat
Download data
- Spontaneous Emission: Cu+28(i) → Cu+28(j) + hv
- Electron Impact Excitation: Cu+28(i) + e → Cu+28(j) + e
| 11 2S0.5 | 0.0 cm-1 |
| 12 2S0.5 | 69921200.0 cm-1 |
| 13 2P0.5 | 69925800.0 cm-1 |
| 13 2P1.5 | 70180800.0 cm-1 |
| 14 2S0.5 | 82949800.0 cm-1 |
| 15 2P0.5 | 82951100.0 cm-1 |
| 15 2P1.5 | 83026800.0 cm-1 |
| 16 2D1.5 | 83028200.0 cm-1 |
| 16 2D2.5 | 83052800.0 cm-1 |
| 17 2S0.5 | 87499300.0 cm-1 |
| 18 2P0.5 | 87499800.0 cm-1 |
| 18 2P1.5 | 87531700.0 cm-1 |
| 19 2D1.5 | 87532300.0 cm-1 |
| 19 2D2.5 | 87542700.0 cm-1 |
U+28 29 29 90097220.0 -------------------------------------------------------------------------------- Configuration Eissner == Standard R % Parentage 1 11 == 1S1 100 1 2S 2S/ 2 12 == 2S1 100 1 2S 2S/ 3 13 == 2P1 100 1 2P 2P/ 4 13 == 2P1 100 1 2P 2P/ 5 14 == 3S1 100 1 2S 2S/ 6 15 == 3P1 100 1 2P 2P/ 7 15 == 3P1 100 1 2P 2P/ 8 16 == 3D1 100 1 2D 2D/ 9 16 == 3D1 100 1 2D 2D/ 10 17 == 4S1 100 1 2S 2S/ 11 18 == 4P1 100 1 2P 2P/ 12 18 == 4P1 100 1 2P 2P/ 13 19 == 4D1 100 1 2D 2D/ 14 19 == 4D1 100 1 2D 2D/ (R) - Levels (or levels within a term) have been reassigned from their principal component. -------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program From IFG file : ./ifg#cu29-28_adf34.dat Options in effect Coupling Avalue numtemps Lweight Isonuclear Comment Level IC YES 14 NO YES 2 Cowan code options ------------------ Cowan plane wave Born method Scale factors 85 95 85 85 50 Parity 1 Parity 2 Allowed 28 15 42 initially 28 15 42 reduced Note: The Born method does NOT calculate spin changing transitions correctly. You should supplement for important transitions of this type. -------------------------------------------------------------------------------- Code : ADAS801 Producer : Martin O'Mullane Date : 16/12/04 --------------------------------------------------------------------------------