arf40_ls#w70.dat
Resolved Specific Ion Data Collections
- Ion
- W70+
- Temperature Range
- 87.03 eV → 1.301 x 105 eV
ADF04
- Filename
- arf40_ls#w70.dat
- Full Path
- adf04/coparf#74/arf40_ls#w70.dat
Download data
- Spontaneous Emission: W+70(i) → W+70(j) + hv
- Electron Impact Excitation: W+70(i) + e → W+70(j) + e
| 22 1S0.0 | 0.0 cm-1 |
| 12513 3P4.0 | 8206360.0 cm-1 |
| 12513 1P1.0 | 14096100.0 cm-1 |
| 12514 3S1.0 | 88552100.0 cm-1 |
| 12514 1S0.0 | 88772100.0 cm-1 |
| 12515 3P4.0 | 91147100.0 cm-1 |
| 12515 1P1.0 | 92783100.0 cm-1 |
| 12516 3D7.0 | 93417100.0 cm-1 |
| 12516 1D2.0 | 94017100.0 cm-1 |
| 12517 3S1.0 | 118810000.0 cm-1 |
| 12517 1S0.0 | 118880000.0 cm-1 |
| 12518 3P4.0 | 119880000.0 cm-1 |
| 12518 1P1.0 | 120560000.0 cm-1 |
| 12519 3D7.0 | 120830000.0 cm-1 |
| 12519 1D2.0 | 121070000.0 cm-1 |
| 1251b 3S1.0 | 132520000.0 cm-1 |
| 1251b 1S0.0 | 132550000.0 cm-1 |
| 1251c 3P4.0 | 133060000.0 cm-1 |
| 1251c 1P1.0 | 133410000.0 cm-1 |
| 1251d 3D7.0 | 133540000.0 cm-1 |
| 1251d 1D2.0 | 133670000.0 cm-1 |
| 1251g 3S1.0 | 139860000.0 cm-1 |
| 1251g 1S0.0 | 139870000.0 cm-1 |
| 1251h 3P4.0 | 140160000.0 cm-1 |
| 1251h 1P1.0 | 140360000.0 cm-1 |
| 1251i 3D7.0 | 140440000.0 cm-1 |
| 1251i 1D2.0 | 140510000.0 cm-1 |
| 1251m 3S1.0 | 144230000.0 cm-1 |
| 1251m 1S0.0 | 144240000.0 cm-1 |
| 1251n 3P4.0 | 144420000.0 cm-1 |
| 1251n 1P1.0 | 144550000.0 cm-1 |
| 1251o 3D7.0 | 144600000.0 cm-1 |
| 1251o 1D2.0 | 144640000.0 cm-1 |
Contributors
- Adam Foster
- Martin O'Mullane
-------------------------------------------------------------------------------- Configuration Eissner == Standard R Parentage 1 22 == 2S2 1 1S 1S/ 2 12513 == 2S1 2P1 1 2S 2S/ 1 2P 3P/ 3 12513 == 2S1 2P1 1 2S 2S/ 1 2P 1P/ 4 12514 == 2S1 3S1 1 2S 2S/ 1 2S 3S/ 5 12514 == 2S1 3S1 1 2S 2S/ 1 2S 1S/ 6 12515 == 2S1 3P1 1 2S 2S/ 1 2P 3P/ 7 12515 == 2S1 3P1 1 2S 2S/ 1 2P 1P/ 8 12516 == 2S1 3D1 1 2S 2S/ 1 2D 3D/ 9 12516 == 2S1 3D1 1 2S 2S/ 1 2D 1D/ 10 12517 == 2S1 4S1 1 2S 2S/ 1 2S 3S/ 11 12517 == 2S1 4S1 1 2S 2S/ 1 2S 1S/ 12 12518 == 2S1 4P1 1 2S 2S/ 1 2P 3P/ 13 12518 == 2S1 4P1 1 2S 2S/ 1 2P 1P/ 14 12519 == 2S1 4D1 1 2S 2S/ 1 2D 3D/ 15 12519 == 2S1 4D1 1 2S 2S/ 1 2D 1D/ 16 1251B == 2S1 5S1 1 2S 2S/ 1 2S 3S/ 17 1251B == 2S1 5S1 1 2S 2S/ 1 2S 1S/ 18 1251C == 2S1 5P1 1 2S 2S/ 1 2P 3P/ 19 1251C == 2S1 5P1 1 2S 2S/ 1 2P 1P/ 20 1251D == 2S1 5D1 1 2S 2S/ 1 2D 3D/ 21 1251D == 2S1 5D1 1 2S 2S/ 1 2D 1D/ 22 1251G == 2S1 6S1 1 2S 2S/ 1 2S 3S/ 23 1251G == 2S1 6S1 1 2S 2S/ 1 2S 1S/ 24 1251H == 2S1 6P1 1 2S 2S/ 1 2P 3P/ 25 1251H == 2S1 6P1 1 2S 2S/ 1 2P 1P/ 26 1251I == 2S1 6D1 1 2S 2S/ 1 2D 3D/ 27 1251I == 2S1 6D1 1 2S 2S/ 1 2D 1D/ 28 1251M == 2S1 7S1 1 2S 2S/ 1 2S 3S/ 29 1251M == 2S1 7S1 1 2S 2S/ 1 2S 1S/ 30 1251N == 2S1 7P1 1 2S 2S/ 1 2P 3P/ 31 1251N == 2S1 7P1 1 2S 2S/ 1 2P 1P/ 32 1251O == 2S1 7D1 1 2S 2S/ 1 2D 3D/ 33 1251O == 2S1 7D1 1 2S 2S/ 1 2D 1D/ (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 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 Map to LS levels : 1 2 2 2 3 4 5 6 6 6 7 8 8 8 9 10 11 12 12 12 13 14 14 14 15 16 17 18 18 18 19 20 20 20 21 22 23 24 24 24 25 26 26 26 27 28 29 30 30 30 31 32 32 32 33 -------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program From IFG file : ./ifg#adf34_tungsten_w70.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 375 204 522 initially 180 66 252 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 : 15/05/09 -------------------------------------------------------------------------------- Correct the orbital energy line to insert 0.0 for orbitals not present in the set of configurations. Martin O'Mullane 29-11-2011 -------------------------------------------------------------------------------