ls#cu0.dat
Resolved Specific Ion Data Collections
- Ion
- Cu0+
- Temperature Range
- 0.043 eV → 43.08 eV
- Spontaneous Emission: Cu+0(i) → Cu+0(j) + hv
- Electron Impact Excitation: Cu+0(i) + e → Cu+0(j) + e
| 606517 2S0.5 | 0.0 cm-1 |
| 606518 2P2.5 | 27829.0 cm-1 |
| 60651b 2S0.5 | 39595.0 cm-1 |
| 606519 2D4.5 | 45589.0 cm-1 |
| 60651c 2P2.5 | 45597.0 cm-1 |
| 60651d 2D4.5 | 51132.0 cm-1 |
| 60651a 2F6.5 | 51220.0 cm-1 |
Contributors
- Martin O'Mullane
U+ 0 29 1 53712.9 -------------------------------------------------------------------------------- Configuration Eissner == Standard R Parentage 1 606517 == 3DA 4S1 1 2S 2S/ 2 606518 == 3DA 4P1 1 2P 2P/ 3 60651B == 3DA 5S1 1 2S 2S/ 4 606519 == 3DA 4D1 1 2D 2D/ 5 60651C == 3DA 5P1 1 2P 2P/ 6 60651D == 3DA 5D1 1 2D 2D/ 7 60651A == 3DA 4F1 1 2F 2F/ (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 Map to LS levels : 1 2 2 3 5 4 4 5 6 6 7 7 -------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program From IFG file : /home/mog/adas/pass/ifg#cu29-00_adf34.dat Options in effect Coupling Avalue numtemps Lweight Isonuclear Comment Level LS YES 14 NO NO 2 Cowan code options ------------------ SCF method used : HR Scale factors for Slater Parameters : 93 99 93 93 93 Optically allowed transitions : Yes Optically forbidden transitions (M1) : Both Parities Optically forbidden transitions (E2) : Both Parities Born Collision-Strength - forbidden : 0 -> 2 Born Collision-Strength - allowed : 1 -> 1 Parity 1 Parity 2 Allowed 13 12 23 initially 6 3 9 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 : 17/12/04 --------------------------------------------------------------------------------