arf40_ls#ar17.dat
Resolved Specific Ion Data Collections
- Ion
- Ar17+
- Temperature Range
- 5.584 eV → 8375 eV
ADF04
- Filename
- arf40_ls#ar17.dat
- Full Path
- adf04/coparf#18/arf40_ls#ar17.dat
Download data
- Spontaneous Emission: Ar+17(i) → Ar+17(j) + hv
- Electron Impact Excitation: Ar+17(i) + e → Ar+17(j) + e
| 11 2S0.5 | 0.0 cm-1 |
| 12 2S0.5 | 26771000.0 cm-1 |
| 13 2P2.5 | 26797000.0 cm-1 |
| 14 2S0.5 | 31741000.0 cm-1 |
| 15 2P2.5 | 31748000.0 cm-1 |
| 16 2D4.5 | 31754000.0 cm-1 |
| 17 2S0.5 | 33478000.0 cm-1 |
| 18 2P2.5 | 33481000.0 cm-1 |
| 19 2D4.5 | 33484000.0 cm-1 |
| 1b 2S0.5 | 34282000.0 cm-1 |
| 1c 2P2.5 | 34284000.0 cm-1 |
| 1d 2D4.5 | 34285000.0 cm-1 |
| 1g 2S0.5 | 34718000.0 cm-1 |
| 1h 2P2.5 | 34719000.0 cm-1 |
| 1i 2D4.5 | 34720000.0 cm-1 |
Contributors
- Adam Foster
- Martin O'Mullane
-------------------------------------------------------------------------------- Configuration Eissner == Standard R Parentage 1 11 == 1S1 1 2S 2S/ 2 12 == 2S1 1 2S 2S/ 3 13 == 2P1 1 2P 2P/ 4 14 == 3S1 1 2S 2S/ 5 15 == 3P1 1 2P 2P/ 6 16 == 3D1 1 2D 2D/ 7 17 == 4S1 1 2S 2S/ 8 18 == 4P1 1 2P 2P/ 9 19 == 4D1 1 2D 2D/ 10 1B == 5S1 1 2S 2S/ 11 1C == 5P1 1 2P 2P/ 12 1D == 5D1 1 2D 2D/ 13 1G == 6S1 1 2S 2S/ 14 1H == 6P1 1 2P 2P/ 15 1I == 6D1 1 2D 2D/ (R) - Levels (or levels within a term) have been reassigned from their principal component. -------------------------------------------------------------------------------- IC Level list : 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 Map to LS levels : 1 2 3 3 4 5 5 6 6 7 8 8 9 9 10 11 11 12 12 13 14 14 15 15 -------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program From IFG file : ./ifg#adf34_argon_ar17.dat Options in effect Coupling Avalue numtemps Lweight Isonuclear Comment Level LS 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 91 45 118 initially 45 10 50 reduced Note: The Born method does NOT calculate spin changing transitions correctly. You should supplement for important transitions of this type. -------------------------------------------------------------------------------- Code : ADAS801 Producer : Adam Foster Date : 13/05/09 -------------------------------------------------------------------------------- Correct the orbital energy line to insert 0.0 for orbitals not present in the set of configurations. Martin O'Mullane 29-11-2011 -------------------------------------------------------------------------------