ls#xe4.dat
Resolved Specific Ion Data Collections
- Ion
- Xe4+
- Temperature Range
- 2.154 eV → 2154 eV
ADF04
- Filename
- ls#xe4.dat
- Full Path
- adf04/copmm#54/ls#xe4.dat
Download data
- Spontaneous Emission: Xe+4(i) → Xe+4(j) + hv
- Electron Impact Excitation: Xe+4(i) + e → Xe+4(j) + e
| 6860952b52c 3P4.0 | 0.0 cm-1 |
| 6860952b52c 1D2.0 | 17411.4 cm-1 |
| 6860952b52c 1S0.0 | 34958.6 cm-1 |
| 6860951b53c 5S2.0 | 76530.6 cm-1 |
| 6860951b53c 3D7.0 | 107429.0 cm-1 |
| 6860951b53c 3P4.0 | 123708.0 cm-1 |
| 6860951b53c 1D2.0 | 138058.0 cm-1 |
| 6860951b53c 3S1.0 | 147188.0 cm-1 |
| 6860952b51c51d 3F10.0 | 153998.0 cm-1 |
| 6860951b53c 1P1.0 | 160508.0 cm-1 |
| 6860952b51c51d 3P4.0 | 166528.0 cm-1 |
| 6860952b51c51d 1D2.0 | 171378.0 cm-1 |
| 6860952b51c51d 3D7.0 | 171988.0 cm-1 |
| 6860952b51c51d 1F3.0 | 186448.0 cm-1 |
| 6860952b51c51d 1P1.0 | 190328.0 cm-1 |
| 6860951a52b51c 3G13.0 | 190358.0 cm-1 |
| 6860951a52b51c 3F10.0 | 191128.0 cm-1 |
| 6860951a52b51c 1F3.0 | 195618.0 cm-1 |
| 6860951a52b51c 3D7.0 | 201798.0 cm-1 |
| 6860951a52b51c 1G4.0 | 209588.0 cm-1 |
| 6860951a52b51c 1D2.0 | 210948.0 cm-1 |
| 6860952b51c51f 3G13.0 | 324038.0 cm-1 |
| 6860952b51c51f 3H16.0 | 324258.0 cm-1 |
| 6860952b51c51f 1G4.0 | 332228.0 cm-1 |
| 6860952b51c51f 3F10.0 | 333178.0 cm-1 |
| 6860952b51c51f 1H5.0 | 333838.0 cm-1 |
| 6860952b51c51f 1F3.0 | 334338.0 cm-1 |
--------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program From IFG file : JETXPQ.IFG#54B.ARCHIVE(XE4) M O'Mullane 10:45 26/01/1998 SCF method used : HR Scale factors for Slater Parameters : 85 99 75 75 60 Optically allowed transitions : yes Optically forbidden transitions M1 : both Optically forbidden transitions E2 : both Born Collision-Strength - print : 9 - forbidden : 0 -> 2 - allowed : 1 -> 1 - included : 2,all Parity 1 Parity 2 Allowed 0 0 303 initially 0 0 126 reduced --------------------------------------------------------------------------------- Correct the orbital energy line to insert 0.0 for orbitals not present in the set of configurations. Martin O'Mullane 29-11-2011 -------------------------------------------------------------------------------