cop98#10_ls#ne6.dat
Resolved Specific Ion Data Collections
- Ion
- Ne6+
- Temperature Range
- 0.844 eV → 8444 eV
ADF04
- Filename
- cop98#10_ls#ne6.dat
- Full Path
- adf04/adas#10/cop98#10_ls#ne6.dat
Download data
- Spontaneous Emission: Ne+6(i) → Ne+6(j) + hv
- Electron Impact Excitation: Ne+6(i) + e → Ne+6(j) + e
- Free Electron Recombination: Ne+7(i) + e → Ne+6(j)
| 1s2 2s2 1S0.0 | 0.0 cm-1 |
| 1s2 2s1 2p1 3P4.0 | 112209.0 cm-1 |
| 1s2 2s1 2p1 1P1.0 | 214954.0 cm-1 |
| 1s2 2p2 3P4.0 | 290276.0 cm-1 |
| 1s2 2p2 1D2.0 | 317692.0 cm-1 |
| 1s2 2p2 1S0.0 | 393121.0 cm-1 |
| 1s2 2s1 3s1 3S1.0 | 978321.0 cm-1 |
| 1s2 2s1 3s1 1S0.0 | 998264.0 cm-1 |
| 1s2 2s1 3p1 1P1.0 | 1025620.0 cm-1 |
| 1s2 2s1 3p1 3P4.0 | 1028630.0 cm-1 |
| 1s2 2s1 3d1 3D7.0 | 1054360.0 cm-1 |
| 1s2 2s1 3d1 1D2.0 | 1071900.0 cm-1 |
| 1s2 2p1 3s1 3P4.0 | 1121270.0 cm-1 |
| 1s2 2p1 3s1 1P1.0 | 1146480.0 cm-1 |
| 1s2 2p1 3p1 1P1.0 | 1148670.0 cm-1 |
| 1s2 2p1 3p1 3D7.0 | 1155970.0 cm-1 |
| 1s2 2p1 3p1 3S1.0 | 1165500.0 cm-1 |
| 1s2 2p1 3p1 3P4.0 | 1172310.0 cm-1 |
| 1s2 2p1 3d1 3F10.0 | 1175400.0 cm-1 |
| 1s2 2p1 3d1 1D2.0 | 1182120.0 cm-1 |
| 1s2 2p1 3p1 1D2.0 | 1184980.0 cm-1 |
| 1s2 2p1 3p1 1S0.0 | 1193000.0 cm-1 |
| 1s2 2p1 3d1 3D7.0 | 1194410.0 cm-1 |
| 1s2 2p1 3d1 3P4.0 | 1200240.0 cm-1 |
| 1s2 2p1 3d1 1F3.0 | 1214120.0 cm-1 |
| 1s2 2p1 3d1 1P1.0 | 1219390.0 cm-1 |
| 1s2 2s1 4s1 3S1.0 | 1299100.0 cm-1 |
| 1s2 2s1 4s1 1S0.0 | 1307080.0 cm-1 |
| 1s2 2s1 4p1 3P4.0 | 1309520.0 cm-1 |
| 1s2 2s1 4p1 1P1.0 | 1319870.0 cm-1 |
| 1s2 2s1 4f1 3F10.0 | 1325020.0 cm-1 |
| 1s2 2s1 4f1 1F3.0 | 1326340.0 cm-1 |
| 1s2 2s1 4d1 3D7.0 | 1328300.0 cm-1 |
| 1s2 2s1 4d1 1D2.0 | 1333920.0 cm-1 |
| 1s2 2s1 5s1 1S0.0 | 1433690.0 cm-1 |
| 1s2 2s1 5s1 3S1.0 | 1436360.0 cm-1 |
| 1s2 2s1 5p1 3P4.0 | 1439450.0 cm-1 |
| 1s2 2s1 5p1 1P1.0 | 1444040.0 cm-1 |
| 1s2 2s1 5d1 3D7.0 | 1446710.0 cm-1 |
| 1s2 2s1 5f1 3F10.0 | 1447170.0 cm-1 |
| 1s2 2s1 5f1 1F3.0 | 1447810.0 cm-1 |
| 1s2 2s1 5g1 3G13.0 | 1447900.0 cm-1 |
| 1s2 2s1 5g1 1G4.0 | 1447920.0 cm-1 |
| 1s2 2s1 5d1 1D2.0 | 1456680.0 cm-1 |
Dependents
Contributors
- Hugh Summers
- Martin O'Mullane
- Jim Lang
- Keith Berrington
- Douglas Sampson
------------------------------------------------------------------------------- Combined two specific ion files Target : /disk3/summers/adas/adf04/cop98#10/copmm#10_ic#ne6.dat Supplementary : /disk3/summers/adas/adf04/cop98#10/copjl#be_ic#ne6.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 16 14 13 15 14 16 15 17 17 18 18 19 19 20 20 21 21 22 22 23 23 24 24 25 25 26 26 27 27 28 28 29 29 30 30 31 31 32 32 33 33 34 34 35 36 36 35 37 37 38 38 39 39 40 40 41 43 42 42 43 41 44 44 45 45 46 46 Code : /home/omullane/merge_adf04/merge_adf04 Date : 18-Nov-98 Producer : Hugh Summers ------------------------------------------------------------------------------- A value differences were detected for the following transitions Tran. Target Supp 6 1 0.00D+00 1.00D-30 8 1 4.54D-01 1.00D-30 9 1 1.60D+03 1.00D-30 10 1 0.00D+00 1.00D-30 12 1 0.00D+00 1.00D-30 18 1 1.83D+02 1.00D-30 20 1 3.09D+07 1.00D-30 27 1 1.32D+01 1.00D-30 30 1 0.00D+00 1.00D-30 32 1 4.05D+01 1.00D-30 37 1 2.18D+04 1.00D-30 44 1 0.00D+00 1.00D-30 8 6 1.42D-08 1.00D-30 9 6 3.11D-06 1.00D-30 10 6 0.00D+00 1.00D-30 12 6 0.00D+00 1.00D-30 18 6 6.09D+03 1.00D-30 20 6 8.40D+01 1.00D-30 27 6 1.25D+06 1.00D-30 30 6 0.00D+00 1.00D-30 32 6 4.34D+05 1.00D-30 37 6 4.79D+02 1.00D-30 44 6 0.00D+00 1.00D-30 8 7 1.17D-02 1.00D-30 9 7 2.26D-01 1.00D-30 11 7 1.06D-02 1.00D-30 17 7 1.38D+04 1.00D-30 18 7 1.53D+03 1.00D-30 19 7 5.94D+03 1.00D-30 20 7 4.07D-01 1.00D-30 25 7 3.87D+04 1.00D-30 26 7 2.74D+06 1.00D-30 27 7 3.25D+05 1.00D-30 28 7 1.23D+06 1.00D-30 29 7 5.40D+02 1.00D-30 31 7 5.38D+05 1.00D-30 32 7 1.01D+06 1.00D-30 37 7 2.22D+03 1.00D-30 9 8 6.22D-01 1.00D-30 10 8 7.29D-02 1.00D-30 11 8 3.60D-02 1.00D-30 12 8 1.33D+02 1.00D-30 17 8 4.54D+03 1.00D-30 18 8 1.05D+04 1.00D-30 19 8 1.18D+04 1.00D-30 20 8 1.95D+01 1.00D-30 25 8 3.36D+04 1.00D-30 26 8 8.49D+05 1.00D-30 27 8 2.09D+06 1.00D-30 28 8 2.45D+06 1.00D-30 29 8 2.83D+03 1.00D-30 31 8 1.74D+06 1.00D-30 32 8 8.50D+05 1.00D-30 37 8 2.43D+03 1.00D-30 44 8 6.19D+02 1.00D-30 10 9 4.85D+01 1.00D-30 11 9 1.80D-01 1.00D-30 12 9 2.29D+05 1.00D-30 17 9 4.29D-02 1.00D-30 18 9 3.55D+00 1.00D-30 19 9 4.06D+00 1.00D-30 20 9 3.00D+04 1.00D-30 25 9 5.22D+06 1.00D-30 26 9 9.57D+04 1.00D-30 27 9 1.20D+01 1.00D-30 28 9 8.73D+02 1.00D-30 29 9 9.67D+03 1.00D-30 30 9 1.96D+03 1.00D-30 31 9 2.74D+03 1.00D-30 32 9 5.92D+03 1.00D-30 37 9 2.95D+06 1.00D-30 44 9 9.26D+06 1.00D-30 12 10 0.00D+00 1.00D-30 18 10 3.25D-01 1.00D-30 20 10 1.80D+05 1.00D-30 27 10 3.08D+01 1.00D-30 30 10 0.00D+00 1.00D-30 32 10 1.20D+03 1.00D-30 37 10 1.42D+06 1.00D-30 44 10 0.00D+00 1.00D-30 4 2 7.69D-03 1.44D-08 13 2 0.00D+00 1.00D-30 15 2 6.61D-03 1.00D-30 21 2 0.00D+00 1.00D-30 23 2 8.43D+03 1.00D-30 33 2 5.13D+06 1.00D-30 35 2 1.12D+02 1.00D-30 39 2 1.38D-02 1.00D-30 41 2 1.73D-02 1.00D-30 43 2 0.00D+00 1.00D-30 5 3 6.89D-01 1.00D-30 14 3 1.47D+06 1.00D-30 15 3 2.66D+06 1.00D-30 16 3 9.42D+03 1.00D-30 22 3 1.00D+04 1.00D-30 23 3 1.86D+04 1.00D-30 24 3 1.50D+01 1.00D-30 33 3 5.30D+06 1.00D-30 34 3 8.71D-01 1.00D-30 35 3 2.48D+06 1.00D-30 38 3 1.29D+07 1.00D-30 39 3 2.51D+06 1.00D-30 40 3 4.65D+06 1.00D-30 41 3 6.18D+06 1.00D-30 42 3 2.78D+06 1.00D-30 45 3 6.41D+03 1.00D-30 46 3 1.30D+04 1.00D-30 5 4 1.10D+00 1.00D-30 13 4 5.86D+06 1.00D-30 14 4 4.38D+06 1.00D-30 15 4 2.06D+06 1.00D-30 16 4 2.06D+04 1.00D-30 21 4 3.79D+04 1.00D-30 22 4 2.87D+04 1.00D-30 23 4 1.38D+04 1.00D-30 24 4 8.15D+01 1.00D-30 33 4 5.91D+05 1.00D-30 34 4 5.14D+06 1.00D-30 35 4 3.67D+05 1.00D-30 36 4 4.28D+04 1.00D-30 38 4 2.73D+06 1.00D-30 39 4 7.32D+06 1.00D-30 40 4 1.10D+07 1.00D-30 41 4 7.59D+06 1.00D-30 42 4 1.32D+07 1.00D-30 43 4 2.00D+05 1.00D-30 45 4 7.30D+02 1.00D-30 46 4 3.43D+02 1.00D-30 14 5 1.34D+04 1.00D-30 15 5 5.79D+01 1.00D-30 16 5 2.65D+06 1.00D-30 22 5 8.13D+01 1.00D-30 23 5 2.32D+00 1.00D-30 24 5 1.20D+04 1.00D-30 33 5 4.53D+06 1.00D-30 34 5 1.45D+06 1.00D-30 35 5 8.19D+06 1.00D-30 38 5 6.34D+03 1.00D-30 39 5 7.09D+03 1.00D-30 40 5 8.30D+04 1.00D-30 41 5 1.43D+04 1.00D-30 42 5 2.80D+03 1.00D-30 45 5 1.06D+07 1.00D-30 46 5 1.24D+07 1.00D-30 22 1 8.28D+06 1.00D-30 38 1 5.70D+06 1.00D-30 42 1 2.15D+06 1.00D-30 16 6 5.07D+05 1.00D-30 24 6 1.53D+07 1.00D-30 46 6 9.93D+07 1.00D-30 16 7 2.15D+05 1.00D-30 24 7 2.27D+07 1.00D-30 33 7 1.41D+07 1.00D-30 35 7 4.04D+08 1.00D-30 46 7 3.39D+07 1.00D-30 16 8 1.12D+06 1.00D-30 24 8 3.52D+06 1.00D-30 33 8 1.90D+08 1.00D-30 34 8 4.26D+08 1.00D-30 35 8 2.92D+07 1.00D-30 45 8 5.19D+06 1.00D-30 46 8 3.95D+04 1.00D-30 22 9 3.79D+07 1.00D-30 23 9 9.48D+06 1.00D-30 33 9 3.20D+10 1.00D-30 34 9 9.30D+07 1.00D-30 38 9 2.55D+07 1.00D-30 39 9 3.42D+06 1.00D-30 40 9 1.30D+06 1.00D-30 41 9 2.68D+08 1.00D-30 42 9 7.80D+06 1.00D-30 22 10 1.03D+07 1.00D-30 38 10 5.79D+07 1.00D-30 42 10 3.27D+07 1.00D-30 11 5 4.74D+05 1.00D-30 12 3 1.24D+06 1.00D-30 17 5 2.79D+06 1.00D-30 18 5 1.69D+06 1.00D-30 20 3 4.54D+06 1.00D-30 20 4 3.65D+05 1.00D-30 25 2 1.71D+08 1.00D-30 25 3 5.72D+08 1.00D-30 25 4 1.98D+06 1.00D-30 26 5 1.09D+09 1.00D-30 27 5 1.02D+07 1.00D-30 29 5 1.32D+08 1.00D-30 30 5 1.10D+07 1.00D-30 31 5 1.30D+07 1.00D-30 32 5 8.17D+07 1.00D-30 37 3 2.55D+07 1.00D-30 37 4 3.64D+07 1.00D-30 44 3 2.77D+07 1.00D-30 Choice of A values for the following transitions has been made 6 1, 8 1, 9 1, 10 1, 12 1, 18 1, 20 1, 27 1 30 1, 32 1, 37 1, 44 1, 8 6, 9 6, 10 6, 12 6 18 6, 20 6, 27 6, 30 6, 32 6, 37 6, 44 6, 8 7 9 7, 11 7, 17 7, 18 7, 19 7, 20 7, 25 7, 26 7 27 7, 28 7, 29 7, 31 7, 32 7, 37 7, 9 8, 10 8 11 8, 12 8, 17 8, 18 8, 19 8, 20 8, 25 8, 26 8 27 8, 28 8, 29 8, 31 8, 32 8, 37 8, 44 8, 10 9 11 9, 12 9, 17 9, 18 9, 19 9, 20 9, 25 9, 26 9 27 9, 28 9, 29 9, 30 9, 31 9, 32 9, 37 9, 44 9 12 10, 18 10, 20 10, 27 10, 30 10, 32 10, 37 10, 44 10 4 2, 13 2, 15 2, 21 2, 23 2, 33 2, 35 2, 39 2 41 2, 43 2, 5 3, 14 3, 15 3, 16 3, 22 3, 23 3 24 3, 33 3, 34 3, 35 3, 38 3, 39 3, 40 3, 41 3 42 3, 45 3, 46 3, 5 4, 13 4, 14 4, 15 4, 16 4 21 4, 22 4, 23 4, 24 4, 33 4, 34 4, 35 4, 36 4 38 4, 39 4, 40 4, 41 4, 42 4, 43 4, 45 4, 46 4 14 5, 15 5, 16 5, 22 5, 23 5, 24 5, 33 5, 34 5 35 5, 38 5, 39 5, 40 5, 41 5, 42 5, 45 5, 46 5 22 1, 38 1, 42 1, 16 6, 24 6, 46 6, 16 7, 24 7 33 7, 35 7, 46 7, 16 8, 24 8, 33 8, 34 8, 35 8 45 8, 46 8, 22 9, 23 9, 33 9, 34 9, 38 9, 39 9 40 9, 41 9, 42 9, 22 10, 38 10, 42 10, 11 5, 12 3 17 5, 18 5, 20 3, 20 4, 25 2, 25 3, 25 4, 26 5 27 5, 29 5, 30 5, 31 5, 32 5, 37 3, 37 4, 44 3 ------------------------------------------------------------------------------- Comments from target file --------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program From IFG file : ne6#IFG M G O'Mullane 18-Nov-98 SCF method used : HR Scale factors for Slater Parameters : 98 99 90 90 65 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 : 10,all Parity 1 Parity 2 Allowed 494 597 903 initially 494 597 903 reduced --------------------------------------------------------------------------------- Update: 18/11/98 HP Summers Adjusted energy levels using Lang up to 46 and the remainder from NIST (DAS) data. Data to adjust the following was not available: 49, 50, 51, 56, 57, 58, 59, 62, 63, 4, 65, 70, 71, 72, 74, 75, 76, 77, 78. --------------------------------------------------------------------------------- Comments from supplementary file ------------------------------------------------------------------------------- Ionisation Potentials from R L Kelly, J Phys Chem Ref Data, 16, Suppl 1, 1987 Energy Levels n=2 from Edlen Phys Scripta 28,51,1983 except for 2p2 3P which are from Edlen Phys Scripta 32,86,1985 n=3 2s3l from Tondello and Paget, J Phys B 3,1757,1970 except for 2s3d 3D which are from the book by Bashkin and Stoner. These differ by only up to 70 cm-1 in 1,000,000 from those of the NIST Standard Reference Database 61, Database for Atomic Spectroscopy version 1. n=3 2p3l mainly from the NIST work just quoted. The NIST source is given as unpublished work by R L Kelly. The NIST values were checked against Kelly J Phys Chem Ref Data 16, Suppl1, 1987. Levels 30 and 44 were not in the published table. In fact 44, 2p3p 1S, is taken as the Kelly value while Ramsbottom et al (see collision strength section below) predict it at a higher energy than Kelly gives. The 2p3d 3F levels are taken at the same energy namely that calculated by Ramsbottom et al. Transition Probabilities Updated to use Opacity Project A values which were obtained from the LS values. This procedure was justified for N IV and O V by Wiese, Fuhr and Deters 'Atomic Transition Probabilities of Carbon, Nitrogen and Oxygen, A Critical Data Compilation' J Phys Chem Ref Data Mono 7, 1996. The Be sequence opacity data was produced by Tully, Seaton and Berrington J Phys B 23, 381 1991) and the present LS results from the Opicty Project book vol 1. Since the Opacity Project was done some further results have been published. Most recently Jonsson, Froese Fischer and Trabert (J Phys B 31, 3497, 1998) from a MCDF calculation have published a value within 2 parts in 400 of the opacity value and that of Fleming et al (Phys Scr 53, 446, 1996) who published a CIV3 result. For the 2s2 1S - 2s2p 3P1 intercombination line the Jonsson, Froese Fischer and Trabert value is adopted and is within 6 parts in 200 of the CIV3 value of Fleming et al (MNRAS 279, 1289, 1996). The 1/z expansion calulation of Ralchenko and Vainstein (Phys Rev A 52, 2449, 1995) is somewhat higher and appears to be accepted as too high. For the 2s2 1S - 2s2p 3P2 transiiton the same two calculations are within 2 parts in 600 and e use the same source. We adopt the Fleming et al 1996 results for the A values between levels of the 2s2p 3P term. For the 2s2 1S - 2s3p 1P transition the opacity value, the MCDF results of Fritsche and Grant (Phys Scr 50, 473, 1994) and the Froese Fischer, Godefeid and Olsen (J Phy B 30, 1163, 1997) MCHF values span 4 parts in 110. The Fischer, Godefeid and Olsen reuslts are only 1 part in 110 different from the Opacity values and the former are adopted. For the 2s2 1S - 2s3p 3P1 transition Fritsche and Grant obtain 3.85 and 3.87 10+8 s-1, Ralchenko and Vainstein get 3.70 10+8 and Froese Fischer, Gaigalas and Godefried (J Phys B 30, 3333, 1997) get 4.15 10+8. We adopt the latter value, noting that they authors point out that a more extensive MCDF including the effect of the polaristaion of the core can possibly resolve the uncertainties. Note that the full-core plus correlation results of Zhu and Chung (Phys Scr 52, 654, 1996) are within about 5% of the opacity values for 2p2 1S and 1D to 3P levels apart from the 2p2 1S to 2s3p 1P transition where there is a factor of 2 differnece and earlier values also have a wider spread. For 2-2 transitions 3-9, 4-9, 3-10, 5-6, 7 and 8 the original A values of Nussbaumer and Storey Astron. and Astroph. 74, 244, 1979 are used as no update seems to have appeared. For 2-3 transitions 9 -15 and 16 and 10-15 the original values of Sampson, Goett and Clark (ADNDT 30, 125, 1984) remain. In fact the line strengths were input to the ADAS code when processing the collision strengths (for another Ne VII adf04 file) with the above energy levels and the output A values used. Ramsbottom et al also provide oscillator strengths. A comparsion with Opacity values shows that for 2-2 transitions the differences are no more than 1.4%. For 2 to 2snl transitions the differnces are similarapart from 2s2p 1P - 2s3d 1D (3.4%), 2p2 3P - 2s3p 3P (9.6%) and 2p2 1D - 2s3p 1P (11.5%). For 2 -2p3l transitions the differnces are less than 6.5% aprt from 2s2 1S - 2p3d 1P (12.4%) and 2p2 1D - 2p3d 1P (17.3%). Collision Strengths The result of Ramsbottom, Berrington and Bell (Atomic Data and Nuclear Data Tables, 61, 105-126, 1995) were used. These are from a multichannel R-matrix calculation. This was a 26 LS eigenstate calculation with the triplet-triplet transitions being transformed to fine structure resolution using Saraph's program (Com Phys Comm, 15, 247, 1978). Jim Lang 17 Nov 98 ------------------------------------------------------------------------------- File generated by altering the temperature set of an ADF04 file Program: ADAS215 Source file: /disk3/summers/adas/adf04/cop98#10/belike_jl98#ne6j.dat Producer: Hugh Summers Date: 18/11/98 ------------------------------------------------------------------------------- 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 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 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 Original level order : 1 2 3 4 5 6 7 8 9 10 11 12 16 13 14 15 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 36 35 37 44 38 39 40 41 42 43 45 46 47 48 49 50 51 52 56 57 58 60 55 53 54 59 62 61 63 64 65 66 67 68 69 70 71 72 74 75 76 77 78 73 Unphysical A values. Set A=1.0E-30 for following transitions : 78 74 A = 1.82D-12 78 75 A = 1.14D-08 78 77 A = 6.94D-07 15 13 A = 1.08D-03 16 13 A = 1.29D-03 36 35 A = 4.12D-11 39 38 A = 2.20D+02 43 38 A = 2.38D+02 58 53 A = 6.55D+05 59 53 A = 1.20D+05 59 54 A = 6.91D+05 59 56 A = 2.32D+00 57 53 A = 3.39D+03 57 54 A = 8.52D+04 57 55 A = 7.72D+05 57 56 A = 3.94D+00 60 56 A = 3.12D+03 78 73 A = 2.24D+03 Date : 19/01/99 Producer : Martin O'Mullane -------------------------------------------------------------------------------C File generated by compression of a J-resolved file Program: ADAS209 Source file: /u/mog/adas/adf04/cop98#10/cop98#10_ic#ne6.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 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 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 Selection Vector: 1 2 2 2 3 4 4 4 5 6 7 8 9 10 10 10 11 11 11 12 13 13 13 14 15 16 16 16 17 18 18 18 19 19 19 20 21 22 23 23 23 24 24 24 25 26 27 28 29 29 29 30 31 31 31 32 33 33 33 34 35 36 37 37 37 38 39 39 39 40 40 40 41 42 42 42 43 44 Original parent metastables: (1S) Parent bundling vector: 0 Date : 19/01/99 Producer : Martin O'Mullane ------------------------------------------------------------------------------- RADIATIVE RECOMBINATION DATA ADDED PROCESSED BY ADAS211 ON : /home/mog/adas/adf08/cop98#10/rrc98#li_ne7.dat Date : 20/01/99 Producer : Martin O'Mullane ------------------------------------------------------------------------------- Dielectronic data is post-processed from Badnell files as follows: /u/adas/adas/adf09/mom93#li/mom93#li_ne7ls12.dat /u/adas/adas/adf09/mom93#li/mom93#li_ne7ls22.dat /u/adas/adas/adf09/mom93#li/mom93#li_ne7ls23.dat The cross-referencing file is as follows: /home/mog/adas/adf18/a09_a04/drm96#be/drm96#be_ls#ne6.dat The parent metastable indices are as follows: 1. 1S2 2S1 (2)0( 0.5) Dielectronic data added to 27 existing rad. recom. level sets Date : 20/01/99 Producer : Martin O'Mullane ------------------------------------------------------------------------------- Ionisation pathways added. The ionisation pathways for the 1s2 2p parent with n=3 terms (1s2 2p 3n) have a parent which is not a metastable but it is a resonance transition to ground so parent 1 was used for these terms. Code : ADAS807 Producer : Martin O'Mullane Date : 19/12/00 ----------------------------------------------------------------- Added ionisation rates (S-lines) from : /home/adas/adas/adf07/szd96#ne/szd96#ne_ne.dat S 1 +1 ISEL = 50 Energy = 1671790.00 S 2 +1 ISEL = 52 Energy = 1559581.30 Code : ADAS807 Producer : Martin O'Mullane Date : 19/12/00 ----------------------------------------------------------------- Add the orbital energies. Martin O'Mullane 12-12-2019 -------------------------------------------------------------------------------