cop98#10_ls#ne7.dat
Resolved Specific Ion Data Collections
- Ion
- Ne7+
- Temperature Range
- 2.757 eV → 5515 eV
ADF04
- Filename
- cop98#10_ls#ne7.dat
- Full Path
- adf04/adas#10/cop98#10_ls#ne7.dat
Download data
- Spontaneous Emission: Ne+7(i) → Ne+7(j) + hv
- Electron Impact Excitation: Ne+7(i) + e → Ne+7(j) + e
- Free Electron Recombination: Ne+8(i) + e → Ne+7(j)
| 1s2 2s1 2S0.5 | 0.0 cm-1 |
| 1s2 2p1 2P2.5 | 129252.0 cm-1 |
| 1s2 3s1 2S0.5 | 1099870.0 cm-1 |
| 1s2 3p1 2P2.5 | 1135180.0 cm-1 |
| 1s2 3d1 2D4.5 | 1147450.0 cm-1 |
| 1s2 4s1 2S0.5 | 1469640.0 cm-1 |
| 1s2 4p1 2P2.5 | 1484050.0 cm-1 |
| 1s2 4d1 2D4.5 | 1489170.0 cm-1 |
| 1s2 4f1 2F6.5 | 1489400.0 cm-1 |
| 1s2 5s1 2S0.5 | 1637410.0 cm-1 |
| 1s2 5p1 2P2.5 | 1644850.0 cm-1 |
| 1s2 5d1 2D4.5 | 1647380.0 cm-1 |
| 1s2 5f1 2F6.5 | 1647440.0 cm-1 |
| 1s2 5g1 2G8.5 | 1647770.0 cm-1 |
Predecessors
Dependents
Contributors
- Hugh Summers
- Martin O'Mullane
- Jim Lang
- Nigel Badnell
------------------------------------------------------------------------------- Combined two specific ion files Target : /disk3/summers/adas/adf04/cop98#10/copmm#10_ic#ne7.dat Supplementary : /disk3/summers/adas/adf04/cop98#10/cop98#10_ic#ne7.dat Replace SUPPLEMENTARY level into TARGET level 1 1 2 2 3 3 4 4 5 5 6 6 7 7 8 8 9 9 10 10 11 11 12 12 13 13 14 14 15 15 16 16 17 17 18 18 19 19 20 20 21 21 22 22 23 23 24 24 Code : /home/omullane/merge_adf04/merge_adf04 Date : 19/01/99 Producer : Martin O'Mullane ------------------------------------------------------------------------------- A value differences were detected for the following transitions and the target values are used. Tran. Target Supp 4 1 0.00D+00 1.00D-30 7 1 2.10D+07 1.00D-30 8 1 2.11D+07 1.00D-30 9 1 0.00D+00 1.00D-30 12 1 3.72D+06 1.00D-30 13 1 3.72D+06 1.00D-30 16 1 0.00D+00 1.00D-30 19 1 1.16D+06 1.00D-30 20 1 1.16D+06 1.00D-30 3 2 3.93D-02 1.00D-30 5 2 0.00D+00 1.00D-30 6 2 3.41D+06 1.00D-30 10 2 0.00D+00 1.00D-30 11 2 1.45D+06 1.00D-30 14 2 5.74D+03 1.00D-30 17 2 0.00D+00 1.00D-30 18 2 7.39D+05 1.00D-30 21 2 5.73D+03 1.00D-30 5 3 6.76D+06 1.00D-30 6 3 3.39D+06 1.00D-30 10 3 2.89D+06 1.00D-30 11 3 1.44D+06 1.00D-30 14 3 3.65D+06 1.00D-30 15 3 2.41D+04 1.00D-30 17 3 1.47D+06 1.00D-30 18 3 7.35D+05 1.00D-30 21 3 2.46D+06 1.00D-30 22 3 1.11D+07 1.00D-30 Choice of A values for the following transitions has been made 4 1, 7 1, 8 1, 9 1, 12 1, 13 1, 16 1, 19 1 20 1, 3 2, 5 2, 6 2, 10 2, 11 2, 14 2, 17 2 18 2, 21 2, 5 3, 6 3, 10 3, 11 3, 14 3, 15 3 17 3, 18 3, 21 3, 22 3 ------------------------------------------------------------------------------- Comments from target file --------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program From IFG file : JETXPQ.IFG#LI.ARCHIVE(NE7#B) M O'Mullane 16:45 6/10/1998 SCF method used : HR Scale factors for Slater Parameters : 98 99 90 90 0 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 : 8,all Parity 1 Parity 2 Allowed 53 56 92 initially 53 56 92 reduced Update: 13/11/98 HP Summers Adjusted energies from Lang re-assessment. --------------------------------------------------------------------------------- Comments from supplementary file ---------------------------------------------------------------------------------- The values in this file were obtained by interpolation using the program ATOM2.FORT(SMODMAN2) and the files COPSM#LI.DATA(PM#O5), (PM#SI11), (PM#TI19) and (PM#ZN27). WJD/PMW 1994 March 2. Update: 22 Sept. 1998 J. Lang - Energy levels for 2s and 2p taken from Edlen, Phys Scr 19, 225-266, 1979 Other energy levels andionisation potential from Kelly, 'Atomic and Ionic Spectrum Lines of Hygdrogen through Krypton' J Phys Chem Ref Data, Vol 16, Suppl 1, 1987. For some levels, particularly where there is no energy difference the level energies were taken from the NIST Standard Ref Database 61, NIST Database for Atomic Spectrocopy Version 1.0 where they use unpublished Kelly data. For 5g levles the original source is used (coppm#li_pm#ne7j.dat). The A values were updated. In their assessment Wiese, Fuhr and Deters ('Atomic Transition Probabilities of Carbon, Nitrogen and Oxygen, A critical Data Compilation' J Phys Chem Ref Data Mono 7, 1996.) state that for Li-like ions the Opacity Project work is used (Peach et al J Phys B 21, 3669, 1988)). Here we have taken the Opacity Project Vol 1 (IOP 1995) p 544 LS gf values and derived the split A values using LS rules and the updated energy levels. Where Opacity Project have no data we use original A value (transitions involving F and G terms). Allowed transitions involving 5g levels have no fill in data. Note that the fill-in data effective collision strengths were obtained from Impact Parameter program using original energies and A Values. ---------------------------------------------------------------------------------- Filtered adf04 file to - sort energy levels - remove non physical A values from energy level reversals - remove energies above ionisation potential - remove duplicate transitions Code : /home/omullane/adf04_utils/filter_adf04.x 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 Original level order : 1 2 3 4 5 6 7 8 9 10 11 12 13 15 14 16 17 18 19 20 21 22 23 24 Producer : Martin O'Mullane Date : 19/01/99 -------------------------------------------------------------------------------- File generated by compression of a J-resolved file Program: ADAS209 Source file: /home/adas/adas/adf04/adas#10/cop98#10_ic#ne7.dat Original level indexing: 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 Selection Vector: 1 2 2 3 4 4 5 5 6 7 7 8 8 9 9 10 11 11 12 12 13 13 14 14 Original parent metastables: (1S) Parent bundling vector: 0 Producer : Martin O'Mullane Date : 19/01/99 ------------------------------------------------------------------------------- RADIATIVE RECOMBINATION DATA ADDED PROCESSED BY ADAS211 ON : /home/adas/adas/adf08/rrc98/rrc98#he_ne8ls.dat Producer : Martin O'Mullane Date : 19/01/99 ------------------------------------------------------------------------------- Dielectronic data is post-processed from Badnell files as follows: /u/adas/adas/adf09/mom93#he/mom93#he_ne8ls12.dat /u/adas/adas/adf09/mom93#he/mom93#he_ne8ls22.dat The cross-referencing file is as follows: /home/mog/adas/adf18/a09_a04/drm96#li/drm96#li_ls#ne7.dat The parent metastable indices are as follows: 1. 1S2 (1)0( 0.0) 2. 1S1 2S1 (3)0( 1.0) 3. 1S1 2P1 (3)1( 4.0) 4. 1S1 2S1 (1)0( 0.0) Dielectronic data added to 15 existing rad. recom. level sets Producer : Martin O'Mullane Date : 19/01/99 ------------------------------------------------------------------------------- Added ionisation rates (S-lines) from : /home/adas/adas/adf07/szd96#ne/szd96#ne_ne.dat S 1 +1 ISEL = 54 Energy = 1928460.00 S 1 +2 ISEL = 55 Energy = 9228400.00 Code : ADAS807 Producer : Martin O'Mullane Date : 18/12/00 ------------------------------------------------------------------------------- Add the orbital energies. Martin O'Mullane 12-12-2019 -------------------------------------------------------------------------------