cop98#7_ic#n3.dat
Resolved Specific Ion Data Collections
- Ion
- N3+
- Temperature Range
- 1.379 eV → 276 eV
ADF04
- Filename
- cop98#7_ic#n3.dat
- Full Path
- adf04/adas#7/cop98#7_ic#n3.dat
Download data
- Spontaneous Emission: N+3(i) → N+3(j) + hv
- Electron Impact Excitation: N+3(i) + e → N+3(j) + e
| 1s2 2s2 1S0.0 | 0.0 cm-1 |
| 1s2 2s1 2p1 3P0.0 | 67209.2 cm-1 |
| 1s2 2s1 2p1 3P1.0 | 67272.3 cm-1 |
| 1s2 2s1 2p1 3P2.0 | 67416.3 cm-1 |
| 1s2 2s1 2p1 1P1.0 | 130694.0 cm-1 |
| 1s2 2p2 3P0.0 | 175535.0 cm-1 |
| 1s2 2p2 3P1.0 | 175608.0 cm-1 |
| 1s2 2p2 3P2.0 | 175733.0 cm-1 |
| 1s2 2p2 1D2.0 | 188882.0 cm-1 |
| 1s2 2p2 1S0.0 | 235369.0 cm-1 |
| 1s2 2s1 3s1 3S1.0 | 377285.0 cm-1 |
| 1s2 2s1 3s1 1S0.0 | 388855.0 cm-1 |
| 1s2 2s1 3p1 3P0.0 | 405972.0 cm-1 |
| 1s2 2s1 3p1 3P1.0 | 405988.0 cm-1 |
| 1s2 2s1 3p1 3P2.0 | 406023.0 cm-1 |
| 1s2 2s1 3p1 1P1.0 | 404522.0 cm-1 |
| 1s2 2s1 3d1 3D1.0 | 420046.0 cm-1 |
| 1s2 2s1 3d1 3D2.0 | 420050.0 cm-1 |
| 1s2 2s1 3d1 3D3.0 | 420058.0 cm-1 |
| 1s2 2s1 3d1 1D2.0 | 429160.0 cm-1 |
| 1s2 2p1 3s1 3P0.0 | 465292.0 cm-1 |
| 1s2 2p1 3s1 3P1.0 | 465371.0 cm-1 |
| 1s2 2p1 3s1 3P2.0 | 465537.0 cm-1 |
| 1s2 2p1 3s1 1P1.0 | 473029.0 cm-1 |
| 1s2 2p1 3p1 1P1.0 | 480884.0 cm-1 |
| 1s2 2p1 3p1 3D1.0 | 484498.0 cm-1 |
| 1s2 2p1 3p1 3D2.0 | 484595.0 cm-1 |
| 1s2 2p1 3p1 3D3.0 | 484746.0 cm-1 |
| 1s2 2p1 3p1 3S1.0 | 487607.0 cm-1 |
| 1s2 2p1 3p1 3P0.0 | 494253.0 cm-1 |
| 1s2 2p1 3p1 3P1.0 | 494309.0 cm-1 |
| 1s2 2p1 3p1 3P2.0 | 494402.0 cm-1 |
| 1s2 2s1 4s1 1S0.0 | 495058.0 cm-1 |
| 1s2 2p1 3d1 3F2.0 | 495406.0 cm-1 |
| 1s2 2p1 3d1 3F3.0 | 495483.0 cm-1 |
| 1s2 2p1 3d1 3F4.0 | 495586.0 cm-1 |
| 1s2 2s1 4s1 3S1.0 | 498046.0 cm-1 |
| 1s2 2p1 3d1 1D2.0 | 498310.0 cm-1 |
| 1s2 2p1 3p1 1D2.0 | 499706.0 cm-1 |
| 1s2 2p1 3d1 3D1.0 | 505554.0 cm-1 |
| 1s2 2p1 3d1 3D2.0 | 505588.0 cm-1 |
| 1s2 2p1 3d1 3D3.0 | 505631.0 cm-1 |
| 1s2 2p1 3d1 3P2.0 | 511509.0 cm-1 |
| 1s2 2p1 3d1 3P1.0 | 511560.0 cm-1 |
| 1s2 2p1 3d1 3P0.0 | 511591.0 cm-1 |
| 1s2 2p1 3d1 1F3.0 | 506285.0 cm-1 |
| 1s2 2s1 4p1 1P1.0 | 507028.0 cm-1 |
| 1s2 2s1 4p1 3P2.0 | 503680.0 cm-1 |
| 1s2 2s1 4p1 3P1.0 | 503692.0 cm-1 |
| 1s2 2s1 4p1 3P0.0 | 503700.0 cm-1 |
| 1s2 2s1 4d1 3D1.0 | 511440.0 cm-1 |
| 1s2 2s1 4d1 3D2.0 | 511446.0 cm-1 |
| 1s2 2s1 4d1 3D3.0 | 511448.0 cm-1 |
| 1s2 2s1 4d1 1D2.0 | 514648.0 cm-1 |
| 1s2 2p1 3p1 1S0.0 | 515570.0 cm-1 |
| 1s2 2p1 3d1 1P1.0 | 518610.0 cm-1 |
| 1s2 2s1 4f1 3F2.0 | 516553.0 cm-1 |
| 1s2 2s1 4f1 3F3.0 | 516561.0 cm-1 |
| 1s2 2s1 4f1 3F4.0 | 516572.0 cm-1 |
| 1s2 2s1 4f1 1F3.0 | 521863.0 cm-1 |
| 1s2 2s1 5s1 3S1.0 | 544813.0 cm-1 |
| 1s2 2s1 5s1 1S0.0 | 546731.0 cm-1 |
| 1s2 2s1 5p1 3P0.0 | 548871.0 cm-1 |
| 1s2 2s1 5p1 3P1.0 | 548867.0 cm-1 |
| 1s2 2s1 5p1 3P2.0 | 548862.0 cm-1 |
| 1s2 2s1 5p1 1P1.0 | 550233.0 cm-1 |
| 1s2 2s1 5d1 3D1.0 | 552790.0 cm-1 |
| 1s2 2s1 5d1 3D2.0 | 552790.0 cm-1 |
| 1s2 2s1 5d1 3D3.0 | 552791.0 cm-1 |
| 1s2 2s1 5f1 3F2.0 | 554572.0 cm-1 |
| 1s2 2s1 5f1 3F3.0 | 554572.0 cm-1 |
| 1s2 2s1 5f1 3F4.0 | 554572.0 cm-1 |
| 1s2 2s1 5d1 1D2.0 | 554301.0 cm-1 |
| 1s2 2s1 5g1 3G3.0 | 554340.0 cm-1 |
| 1s2 2s1 5g1 3G4.0 | 554340.0 cm-1 |
| 1s2 2s1 5g1 3G5.0 | 554340.0 cm-1 |
| 1s2 2s1 5g1 1G4.0 | 554339.0 cm-1 |
| 1s2 2s1 5f1 1F3.0 | 554996.0 cm-1 |
Contributors
- Martin O'Mullane
- Hugh Summers
------------------------------------------------------------------------------- Combined two specific ion files Target : /u/hps/adas/adf04/cop98#7/copmm#7_ic#n3.dat Supplementary : /u/hps/adas/adf04/cop98#7/copjl#be_ic#n3.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 35 36 36 37 37 38 38 39 39 40 40 41 41 42 42 43 43 44 44 45 45 46 46 47 47 48 48 49 49 50 50 51 51 52 52 53 53 54 54 55 55 56 56 57 57 58 58 59 59 60 60 61 61 62 62 63 63 64 64 65 65 66 66 67 67 68 68 69 69 70 70 71 71 72 72 73 73 74 74 75 75 76 76 77 77 78 78 Code : /u/hps/merge_adf04/merge_adf04 ------------------------------------------------------------------------------- A value differences were detected for the following transitions Tran. Target Supp 6 1 0.00D+00 1.00D-30 10 1 0.00D+00 1.00D-30 12 1 0.00D+00 1.00D-30 18 1 5.47D-01 1.00D-30 20 1 1.73D+06 1.00D-30 8 6 6.28D-12 4.69D-12 9 6 1.81D-08 4.00D-08 10 6 0.00D+00 1.00D-30 12 6 0.00D+00 1.00D-30 18 6 1.52D+02 1.00D-30 20 6 2.22D-01 1.00D-30 11 7 1.24D-05 1.00D-30 17 7 3.43D+02 1.00D-30 18 7 3.81D+01 1.00D-30 19 7 1.51D+02 1.00D-30 20 7 7.17D-04 1.00D-30 12 8 4.80D-01 1.00D-30 17 8 1.14D+02 1.00D-30 18 8 2.65D+02 1.00D-30 19 8 3.01D+02 1.00D-30 20 8 6.04D-02 1.00D-30 11 9 1.48D-04 1.00D-30 12 9 9.61D+03 1.00D-30 17 9 2.78D-04 1.00D-30 18 9 7.10D-03 1.00D-30 19 9 7.33D-03 1.00D-30 20 9 1.32D+03 1.00D-30 12 10 0.00D+00 1.00D-30 18 10 6.21D-04 1.00D-30 20 10 5.16D+03 1.00D-30 4 2 4.63D-01 6.53D-12 13 2 0.00D+00 1.00D-30 15 2 1.66D-05 1.00D-30 14 3 6.94D+04 1.00D-30 15 3 1.25D+05 1.00D-30 16 3 3.92D+01 1.00D-30 13 4 2.77D+05 1.00D-30 14 4 2.08D+05 1.00D-30 15 4 9.70D+04 1.00D-30 16 4 8.74D+01 1.00D-30 14 5 4.83D+01 1.00D-30 15 5 1.17D-01 1.00D-30 16 5 1.11D+05 1.00D-30 16 6 3.18D+03 1.00D-30 16 7 1.22D+03 1.00D-30 16 8 2.45D+04 1.00D-30 14 9 3.62D+05 1.00D-30 15 9 2.49D+02 1.00D-30 14 10 1.02D+04 1.00D-30 11 5 3.95D+03 1.00D-30 12 3 1.89D+04 1.00D-30 17 5 1.84D+04 1.00D-30 18 5 1.08D+04 1.00D-30 20 3 5.15D+04 1.00D-30 20 4 2.19D+03 1.00D-30 Choice of A values for the following transitions has been made 6 1, 10 1, 12 1, 18 1, 20 1, 8 6, 9 6, 10 6 12 6, 18 6, 20 6, 11 7, 17 7, 18 7, 19 7, 20 7 12 8, 17 8, 18 8, 19 8, 20 8, 11 9, 12 9, 17 9 18 9, 19 9, 20 9, 12 10, 18 10, 20 10, 4 2, 13 2 15 2, 14 3, 15 3, 16 3, 13 4, 14 4, 15 4, 16 4 14 5, 15 5, 16 5, 16 6, 16 7, 16 8, 14 9, 15 9 14 10, 11 5, 12 3, 17 5, 18 5, 20 3, 20 4 ------------------------------------------------------------------------------- For the following transitions target A values have been preferred Tran. Target Supp 18 1 5.47D-01 1.00D-30 20 1 1.73D+06 1.00D-30 18 6 1.52D+02 1.00D-30 20 6 2.22D-01 1.00D-30 11 7 1.24D-05 1.00D-30 17 7 3.43D+02 1.00D-30 18 7 3.81D+01 1.00D-30 19 7 1.51D+02 1.00D-30 20 7 7.17D-04 1.00D-30 11 8 3.84D-05 1.00D-03 12 8 4.80D-01 1.00D-30 17 8 1.14D+02 1.00D-30 18 8 2.65D+02 1.00D-30 19 8 3.01D+02 1.00D-30 20 8 6.04D-02 1.00D-30 11 9 1.48D-04 1.00D-30 12 9 9.61D+03 1.00D-30 17 9 2.78D-04 1.00D-30 18 9 7.10D-03 1.00D-30 19 9 7.33D-03 1.00D-30 20 9 1.32D+03 1.00D-30 18 10 6.21D-04 1.00D-30 20 10 5.16D+03 1.00D-30 4 2 4.63D-01 6.53D-12 15 2 1.66D-05 1.00D-30 14 3 6.94D+04 1.00D-30 15 3 1.25D+05 1.00D-30 16 3 3.92D+01 1.00D-30 13 4 2.77D+05 1.00D-30 14 4 2.08D+05 1.00D-30 15 4 9.70D+04 1.00D-30 16 4 8.74D+01 1.00D-30 14 5 4.83D+01 1.00D-30 15 5 1.17D-01 1.00D-30 16 5 1.11D+05 1.00D-30 16 6 3.18D+03 1.00D-30 16 7 1.22D+03 1.00D-30 16 8 2.45D+04 1.00D-30 14 9 3.62D+05 1.00D-30 15 9 2.49D+02 1.00D-30 14 10 1.02D+04 1.00D-30 11 5 3.95D+03 1.00D-30 12 3 1.89D+04 1.00D-30 17 5 1.84D+04 1.00D-30 18 5 1.08D+04 1.00D-30 20 3 5.15D+04 1.00D-30 20 4 2.19D+03 1.00D-30 20 5 2.21D+10 1.85D+09 ------------------------------------------------------------------------------- Comments from target file --------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program From IFG file : JETXPQ.IFG#BE.ARCHIVE(N3#A) M O'Mullane 15:32 6/10/1998 SCF method used : HR Scale factors for Slater Parameters : 85 99 75 80 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 492 589 903 initially 492 589 903 reduced --------------------------------------------------------------------------------- Update: 02/10/98 HP Summers Adjusted energy levels from NIST (DAS) data 2s5p (3P) missing from NIST - estimate from qd. --------------------------------------------------------------------------------- Comments from supplementary file ----------------------------------------------------------------------- Energy Levels The results from NSRDS NBS3 SECT 4 were used. These were within 2 wavenumbers of the results of Edlen (Phys. Scr 32, 86, 1985 and 28, 51, 1983) who only considered n=2 levels. The NSRDS values are also those of Moore and Gallacher "Tables of Spectra of hydrogen, carbon, nitrogen and oxygen atoms and ions" CRC press 1993. Ionisation Potential As energy levels. A Values For transitions between n = 2 levels the results of the compilation by Allard et al (Astron Astrophys Suppl Ser 84, 563, 1990) were used and for values not given by them the results of Nussbaumer and Storey (Astron Astrophys 74, 244, 1979) were used. The Nusssbaumer and Storey results were adopted for forbidden transitions by Allard et al. For the 2-3 and 3-4 transitions the results of Idrees and Das (J Phys B 22, 3609, 1989 were used. For transitions involving n = 3 levels again the results of Allard et al were adopted. Collision Data The results of Ramsbottom et al (Phys Scr 50, 246-253 1994) were adopted. These results were obtained from a 12 eigenstate R-matrix calculation. The 12 states correpond to the 20 lowest finestructure levels. The partial wave expansion was for total angular momentum l <= 12 for both odd and even parities and doublet and quartet spin states. For allowed transitions the partial wave analysis was extended beyond 12. The transformation from LS to JJ coupling was by a program from Saraph (Comp Phys Comm 15, 247, 1978) which ignores term coupling and included the higher partial waves. In processing these data through ADAS 102 some obvious misprints in the paper were found. In Table VI transition 65 should have upper level 2s3p 1P not 2P. In Table VII transition 8 the second last temperature value should be to power -1 and transition 50 the last 3 temperature values should be to power +1 not -1. For the allowed transition 27, the effective collision strength falls with temperature although others rise. Similarly with transition 53. The allowed behaviour was forced by ADAS 101. The allowed members of the 2p2 3P - 2s3p 3P transition all have effective collision strengths which fall with increasing temperature. The allowed behaviour was forced by ADAS 101, making a difference of eg 6.36 10-3 to 6.67 10-3 at the highest temperature in this file for the 0-1 transition. Note that Ramsbottom et al did not give A values for this transition. In CIII and O V in similar calculations this double electron jump transition was presented in the same way. Also the type 1 behaviour was forced for transition 94. For allowed transitions between n=3 levels IPProg was used to generate the collision strengths using the enery levels and A values adopted here. J LANG May 1995. The energy levels adopted are also those given in the NIST Standard Ref Database 61, NIST Database for Atomic Spectrocopy Version 1.0 The A values have also been updated. Since the file was created, the assessed data from Wiese, Fuhr and Deters 'Atomic Transition Probabilities of Carbon, Nitrogen and Oxygen, A Critical Data Compilation' J Phys Chem Ref Data Mono 7, 1996 have been published. This is used for all A values except as given below. They use unpublished data of Weiss and results from the Opcity Project (for Be sequence Tully, Seaton and Berrington J Phys B 23, 381 1991). The Opacity Project wrok was in LS coupling and they justify spliitng the data by LS rules by comparison with published work. They say that the earlier review by Allard et al (see above) also used Opacity Project data as well as earlier work. The 1996 compilation gives a zero weight to the earlier work while Allard et al gave it a weight of 1 and Opacity results a weight of 5. There is only a slight difference from the 1996 work and Allard et al. Since the critical compilation was done there have been some further results published. Fleming et al Ap J 455,758, 1995 have published results from CIV3 and MCHF calculations. They agree closely with the compilation apart from 2 cases, the 2s2p 3P1 2p2 1S rate is 9.20+3 s-1 (CIV3) and 9.03+3 s-1 (MCHF) while the compilation gives 5.81+2 s-1 (from unpublished Wiess calculation) and above 8.84+2 s-1 is used. We adopt the Fleming et al result. The other case where there is a difference is in the 2s2 1S - 2s2p 3P1 intercombination rate. Fleming et al give 580 s-1 while the compilation gives 595 s-1. There are other recent calculations of this rate: Ralchenko and Vainstein (RV)(Phys Rev A 52, 2449, 1995) get 653 s-1 which is thought to be high (1/z expansion), Ynnerman and Froese Fischer (Phys Rev A 51 2020, 1995) give 564 s-1 and Jonsson, Froese Fischer and Trabert (J Phys B 31, 3497, 1998) give 559 and 562 s-1 in a MCDF calculation which they say gives a lower bound. We adopt the Fleming value. The latter authors other values agree with the compilation. Zhu and Chung (Phys Scr 52, 564, 1995) have published results for transitions involving 2s2p and 2s3p terms and 2p2 terms. Their results are close to the critical compilation apart from 2p2 1D -2s3p1P and 2p2 3P - 2s3p 3P (~6% different) and 2p2 1S to 2s3p 1P where they get 4.86 s-1 cf 6.67 +7 s-1. We adopt the compilation value. The 2s2 1S -2s3p 1P and 3P1 transitions also have been studied post compilation. For the allowed transition the compilation value of 1.19+10 s-1 should be compared to those of Fritsche and Grant (FG) (Phys Scr 50, 473, 1994) MCDF values of 1.12 +10 and 1.13+10 s-1 and the Frose Fischer, Godefeid and Olsen (J Phy B 30, 1163, 1997) value of 1.21+10 s-1. The compilation value is adopted. For the 2s2 1S - 2s3p3P1 rate FG get 1.33+6 and 1.40+6 s-1, RV get 4.96+6, and Froese Fischer, Gaigalas and Godefried (J Phys B 30, 3333, 1997) get 3.21+6 s-1 cf compilation value of 3.08+6 s-1. The compilation value appears a good compromise. The 3-3 effective collison strengths were estimated using the adopted energies and the A values of copjl#be_jl#n3j.dat. However, the energies remain the same and the A values change at most 3% so any difference in rates using new A values is very small. J Lang Sept 98 ----------------------------------------------------------------------- --------------------------------------------------------------------------------- ---------------------------------------------------------------------------------