cop98#8_ic#o3.dat
Resolved Specific Ion Data Collections
- Ion
- O3+
- Temperature Range
- 0.689 eV → 1379 eV
ADF04
- Filename
- cop98#8_ic#o3.dat
- Full Path
- adf04/adas#8/cop98#8_ic#o3.dat
Download data
- Spontaneous Emission: O+3(i) → O+3(j) + hv
- Electron Impact Excitation: O+3(i) + e → O+3(j) + e
| 2s2 2p1 2P0.5 | 0.0 cm-1 |
| 2s2 2p1 2P1.5 | 385.9 cm-1 |
| 2s1 2p2 4P0.5 | 71439.8 cm-1 |
| 2s1 2p2 4P1.5 | 71570.1 cm-1 |
| 2s1 2p2 4P2.5 | 71755.5 cm-1 |
| 2s1 2p2 2D1.5 | 126950.0 cm-1 |
| 2s1 2p2 2D2.5 | 126936.0 cm-1 |
| 2s1 2p2 2S0.5 | 164366.0 cm-1 |
| 2s1 2p2 2P0.5 | 180481.0 cm-1 |
| 2s1 2p2 2P1.5 | 180724.0 cm-1 |
| 2p3 4S1.5 | 231538.0 cm-1 |
| 2p3 2D1.5 | 255185.0 cm-1 |
| 2p3 2D2.5 | 255156.0 cm-1 |
| 2p3 2P0.5 | 289015.0 cm-1 |
| 2p3 2P1.5 | 289024.0 cm-1 |
| 2s2 3s1 2S0.5 | 357614.0 cm-1 |
| 2s2 3p1 2P0.5 | 390161.0 cm-1 |
| 2s2 3p1 2P1.5 | 390248.0 cm-1 |
| 2s2 3d1 2D1.5 | 419534.0 cm-1 |
| 2s2 3d1 2D2.5 | 419551.0 cm-1 |
| 2s1 2p1 3s1 4P0.5 | 438849.0 cm-1 |
| 2s1 2p1 3s1 4P1.5 | 438984.0 cm-1 |
| 2s1 2p1 3s1 4P2.5 | 439231.0 cm-1 |
| 2s1 2p1 3s1 2P0.5 | 452807.0 cm-1 |
| 2s1 2p1 3s1 2P1.5 | 453072.0 cm-1 |
| 2s1 2p1 3p1 2P0.5 | 467229.0 cm-1 |
| 2s1 2p1 3p1 2P1.5 | 467345.0 cm-1 |
| 2s1 2p1 3p1 4D0.5 | 468337.0 cm-1 |
| 2s1 2p1 3p1 4D1.5 | 468415.0 cm-1 |
| 2s1 2p1 3p1 4D2.5 | 468551.0 cm-1 |
| 2s1 2p1 3p1 4D3.5 | 468760.0 cm-1 |
| 2s1 2p1 3p1 4S1.5 | 474478.0 cm-1 |
| 2s1 2p1 3p1 4P0.5 | 478849.0 cm-1 |
| 2s1 2p1 3p1 4P1.5 | 478943.0 cm-1 |
| 2s1 2p1 3p1 4P2.5 | 479072.0 cm-1 |
| 2s1 2p1 3p1 2D1.5 | 482666.0 cm-1 |
| 2s1 2p1 3p1 2D2.5 | 482922.0 cm-1 |
| 2s1 2p1 3d1 4F1.5 | 495169.0 cm-1 |
| 2s1 2p1 3d1 4F2.5 | 495246.0 cm-1 |
| 2s1 2p1 3d1 4F3.5 | 495360.0 cm-1 |
| 2s1 2p1 3d1 4F4.5 | 495513.0 cm-1 |
| 2s1 2p1 3p1 2S0.5 | 492890.0 cm-1 |
| 2s1 2p1 3d1 4D0.5 | 499767.0 cm-1 |
| 2s1 2p1 3d1 4D1.5 | 499796.0 cm-1 |
| 2s1 2p1 3d1 4D2.5 | 499843.0 cm-1 |
| 2s1 2p1 3d1 4D3.5 | 499907.0 cm-1 |
| 2s1 2p1 3d1 2D1.5 | 501509.0 cm-1 |
| 2s1 2p1 3d1 2D2.5 | 501564.0 cm-1 |
| 2s1 2p1 3d1 4P2.5 | 504096.0 cm-1 |
| 2s1 2p1 3d1 4P1.5 | 504209.0 cm-1 |
| 2s1 2p1 3d1 4P0.5 | 504282.0 cm-1 |
| 2s1 2p1 3d1 2F2.5 | 510745.0 cm-1 |
| 2s1 2p1 3d1 2F3.5 | 510977.0 cm-1 |
| 2s1 2p1 3d1 2P1.5 | 514220.0 cm-1 |
| 2s1 2p1 3d1 2P0.5 | 514371.0 cm-1 |
| 2s1 2p1 3s1 2P0.5 | 518699.0 cm-1 |
| 2s1 2p1 3s1 2P1.5 | 518709.0 cm-1 |
| 2s1 2p1 3p1 2D1.5 | 547326.0 cm-1 |
| 2s1 2p1 3p1 2D2.5 | 547355.0 cm-1 |
| 2s1 2p1 3p1 2P0.5 | 549792.0 cm-1 |
| 2s1 2p1 3p1 2P1.5 | 549855.0 cm-1 |
| 2s1 2p1 3p1 2S0.5 | 554461.0 cm-1 |
| 2p2 3s1 4P0.5 | 576854.0 cm-1 |
| 2p2 3s1 4P1.5 | 576998.0 cm-1 |
| 2p2 3s1 4P2.5 | 577210.0 cm-1 |
| 2s1 2p1 3d1 2F3.5 | 570791.0 cm-1 |
| 2s1 2p1 3d1 2F2.5 | 570791.0 cm-1 |
| 2s1 2p1 3d1 2D1.5 | 575819.0 cm-1 |
| 2s1 2p1 3d1 2D2.5 | 575853.0 cm-1 |
| 2s1 2p1 3d1 2P0.5 | 581721.0 cm-1 |
| 2s1 2p1 3d1 2P1.5 | 581743.0 cm-1 |
| 2p2 3p1 2S0.5 | 597254.0 cm-1 |
| 2p2 3s1 2P0.5 | 594340.0 cm-1 |
| 2p2 3s1 2P1.5 | 594538.0 cm-1 |
| 2p2 3p1 4D0.5 | 593602.0 cm-1 |
| 2p2 3p1 4D1.5 | 602962.0 cm-1 |
| 2p2 3p1 4D2.5 | 603077.0 cm-1 |
| 2p2 3p1 4D3.5 | 603227.0 cm-1 |
| 2p2 3p1 4P0.5 | 606530.0 cm-1 |
| 2p2 3p1 4P1.5 | 606578.0 cm-1 |
| 2p2 3p1 4P2.5 | 606694.0 cm-1 |
| 2p2 3s1 2D1.5 | 600092.0 cm-1 |
| 2p2 3s1 2D2.5 | 600106.0 cm-1 |
| 2p2 3p1 2D1.5 | 615431.0 cm-1 |
| 2p2 3p1 2D2.5 | 615460.0 cm-1 |
| 2p2 3p1 2P1.5 | 605788.0 cm-1 |
| 2p2 3p1 2P0.5 | 609570.0 cm-1 |
| 2p2 3p1 4S1.5 | 616881.0 cm-1 |
| 2p2 3d1 4F1.5 | 618354.0 cm-1 |
| 2p2 3d1 4F2.5 | 618468.0 cm-1 |
| 2p2 3d1 4F3.5 | 618627.0 cm-1 |
| 2p2 3d1 4F4.5 | 618829.0 cm-1 |
| 2p2 3d1 4D0.5 | 622892.0 cm-1 |
| 2p2 3d1 4D1.5 | 622684.0 cm-1 |
| 2p2 3p1 2F2.5 | 624882.0 cm-1 |
| 2p2 3d1 4D2.5 | 623872.0 cm-1 |
| 2p2 3d1 4D3.5 | 623972.0 cm-1 |
| 2p2 3p1 2F3.5 | 624882.0 cm-1 |
| 2p2 3d1 2P1.5 | 632426.0 cm-1 |
| 2p2 3d1 2P0.5 | 632597.0 cm-1 |
| 2p2 3d1 2F2.5 | 630095.0 cm-1 |
| 2p2 3d1 2F3.5 | 630095.0 cm-1 |
| 2p2 3d1 4P2.5 | 637114.0 cm-1 |
| 2p2 3d1 4P1.5 | 637213.0 cm-1 |
| 2p2 3d1 4P0.5 | 637275.0 cm-1 |
| 2p2 3p1 2D2.5 | 631913.0 cm-1 |
| 2p2 3p1 2D1.5 | 631913.0 cm-1 |
| 2p2 3p1 2P0.5 | 639123.0 cm-1 |
| 2p2 3d1 2D1.5 | 646859.0 cm-1 |
| 2p2 3d1 2D2.5 | 646859.0 cm-1 |
| 2p2 3p1 2P1.5 | 639344.0 cm-1 |
| 2p2 3d1 2G3.5 | 649778.0 cm-1 |
| 2p2 3d1 2G4.5 | 649847.0 cm-1 |
| 2p2 3s1 2S0.5 | 651465.0 cm-1 |
| 2p2 3d1 2D1.5 | 653328.0 cm-1 |
| 2p2 3d1 2D2.5 | 653411.0 cm-1 |
| 2p2 3d1 2F3.5 | 651098.0 cm-1 |
| 2p2 3d1 2F2.5 | 651117.0 cm-1 |
| 2p2 3d1 2P0.5 | 659998.0 cm-1 |
| 2p2 3d1 2P1.5 | 659998.0 cm-1 |
| 2p2 3d1 2S0.5 | 671701.0 cm-1 |
| 2p2 3p1 2P0.5 | 687844.0 cm-1 |
| 2p2 3p1 2P1.5 | 687863.0 cm-1 |
| 2p2 3d1 2D2.5 | 706333.0 cm-1 |
| 2p2 3d1 2D1.5 | 706333.0 cm-1 |
Predecessors
Contributors
- David Brooks
- Martin O'Mullane
- Douglas Sampson
------------------------------------------------------------------------------- Combined two specific ion files Target : /home/brooks/adas/adf04/cop98#8/copsm#b_sm#o3j.dat Supplementary : /home/brooks/adas/adf04/cop98#8/copjl#b_ic#o3.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 Code : /home/omullane/merge_adf04/merge_adf04 Date : 25-Nov-98 Producer : David Brooks ------------------------------------------------------------------------------- A value differences were detected for the following transitions and the target values are used. Tran. Target Supp 5 1 0.00D+00 1.00D-30 7 1 0.00D+00 1.00D-30 11 1 0.00D+00 1.00D-30 12 1 0.00D+00 1.00D-30 13 1 0.00D+00 1.00D-30 14 1 0.00D+00 1.00D-30 15 1 0.00D+00 1.00D-30 11 2 0.00D+00 1.00D-30 12 2 0.00D+00 1.00D-30 13 2 0.00D+00 1.00D-30 14 2 0.00D+00 1.00D-30 15 2 0.00D+00 1.00D-30 4 3 0.00D+00 1.00D-30 5 3 0.00D+00 1.00D-30 6 3 0.00D+00 1.00D-30 7 3 0.00D+00 1.00D-30 8 3 0.00D+00 1.00D-30 9 3 0.00D+00 1.00D-30 10 3 0.00D+00 1.00D-30 13 3 0.00D+00 1.00D-30 5 4 0.00D+00 1.00D-30 6 4 0.00D+00 1.00D-30 7 4 0.00D+00 1.00D-30 8 4 0.00D+00 1.00D-30 9 4 0.00D+00 1.00D-30 10 4 0.00D+00 1.00D-30 6 5 0.00D+00 1.00D-30 7 5 0.00D+00 1.00D-30 8 5 0.00D+00 1.00D-30 9 5 0.00D+00 1.00D-30 10 5 0.00D+00 1.00D-30 14 5 0.00D+00 1.00D-30 7 6 0.00D+00 1.00D-30 8 6 0.00D+00 1.00D-30 9 6 0.00D+00 1.00D-30 10 6 0.00D+00 1.00D-30 8 7 0.00D+00 1.00D-30 9 7 0.00D+00 1.00D-30 10 7 0.00D+00 1.00D-30 14 7 0.00D+00 1.00D-30 9 8 0.00D+00 1.00D-30 10 8 0.00D+00 1.00D-30 13 8 0.00D+00 1.00D-30 10 9 0.00D+00 1.00D-30 13 9 0.00D+00 1.00D-30 12 11 0.00D+00 1.00D-30 13 11 0.00D+00 1.00D-30 14 11 0.00D+00 1.00D-30 15 11 0.00D+00 1.00D-30 14 12 0.00D+00 1.00D-30 15 12 0.00D+00 1.00D-30 13 12 0.00D+00 1.00D-30 14 13 0.00D+00 1.00D-30 15 13 0.00D+00 1.00D-30 15 14 0.00D+00 1.00D-30 Choice of A values for the following transitions has been made 5 1, 7 1, 11 1, 12 1, 13 1, 14 1, 15 1, 11 2 12 2, 13 2, 14 2, 15 2, 4 3, 5 3, 6 3, 7 3 8 3, 9 3, 10 3, 13 3, 5 4, 6 4, 7 4, 8 4 9 4, 10 4, 6 5, 7 5, 8 5, 9 5, 10 5, 14 5 7 6, 8 6, 9 6, 10 6, 8 7, 9 7, 10 7, 14 7 9 8, 10 8, 13 8, 10 9, 13 9, 12 11, 13 11, 14 11 15 11, 14 12, 15 12, 13 12, 14 13, 15 13, 15 14 ------------------------------------------------------------------------------- For the following transitions supplement A values have been used, Check supplement values! Tran. Target Supp 2 1 0.00D+00 4.92D-04 4 2 2.83D+00 2.76D+02 12 3 3.16D+03 1.35D+01 13 4 5.17D+03 3.29D+02 11 6 1.93D+01 1.16D+00 11 7 2.50D+01 1.30D+03 11 9 5.13D+01 6.24D+02 11 10 1.81D+02 2.15D+03 ------------------------------------------------------------------------------- Comments from target file ----------------------------------------------------------------------------- Description of the Sampson source data set:- This data set gives relativistic distorted wave collision strengths and oscillator strengths for the 22 B-like ions with 6 <= Z <= 27 obtained by Zhang and Sampson (to appearin Vol. ?? of Atomic Data Nuclear Data Tables, ) Source file :- /JETSHP.RBDATA.TEXT The values of the ionization potential were taken from: Boron-like ionisation potential from Kelly Program :- JETSHP.STRIPSAM.FORT(STRIPSAM) Author :- R.W.P.McWhirter Data set produced :- 23/04/96 ----------------------------------------------------------------------------- The Sampson source data has been extended with impact parameter data for transitions between higher levels. Source data set :- /JETSHP.COPSS#B.DATA(SS#O3J) ----------------------------------------------------------------------------- NIST data added except for levels 75, 86, 87, 89, 90, 91, 92, 93, 94 96, 97, 108, 111, 112, 113, 114, 121, 122 and 123 where non was available. These levels retain the Cowan energies. David H. Brooks, 25th November 1998 ----------------------------------------------------------------------------- Comments from supplementary file ------------------------------------------------------------------------ ENERGY LEVELS AND IONISATION POTENTIAL The ionisation potential and energy levels are from 'Tables of Spectra of Hydrogen, Carbon, Nitrogen and Oxygen Atoms and Ions' by C E Moore, edited by J W Gallacher (CRC Press). The ionisation potential adopted is 1.8 cm-1 less than that given by Kelly (J Chem Ref Data 1, 1987). The ordering of the levels is as given in the work used for the effective collision strengths. The energies differ by at most 2.2 cm-1 from those given by Edlen (Phys Scripta 28, 483, 1983). TRANSITION PROBABILITIES For the transition between the 1/2 and 3/2 levels of the ground term the multiconfiguration Hartree-Fock Breit-Pauli result of C Froese Fischer (J Phys B 16, 157 1983) is used (4.92-04 s-1). Other values include 1.39-3 s-1 from the multiconfiguration Dirac-Fock calculations of Cheng, Kim and Desclaux (ADNDT 24, 111, 1979), and 5.17-4 s-1 from the Superstructure calculations done by Nussbaumer and Storey (Astron Astrophys 115, 205, 1982) who used a 60 configuration basis. The results of Dankwort and Trefftz (Astron Astrophys 65, 93, 1978) have been adopted for the majority of transitions. Their calculation used the multiconfiguration Hartree-Fock ansatz with Breit-Pauli corrections. For transitions 3-12, 3-14, 3-15, 4-12, 4-13, 4-14, 4-15, 5-12, 5-13, 5-15, 6-11, 7-11, 8-11, 8-12, 9-11 and 10-11 Dankwort and Trefftz did not give results. Accordingly the results of Merkelis, Vilkas, Gaigalas and Kisielius were used (Phys Scripta 51, 233, 1995). Their calculation employed the stationary second order many-body perturbation theory, the relativistic corrections being included using the Breit-Pauli approximation. EFFECTIVE COLLISION STRENGTHS In their assessment of effective collision strengths for the B-like sequence Sampson, Zhang and Fontes (ADNDT 57, 98, 1994) review the available results. The results of Blum and Pradhan (Ap J SS 80, 425, 1992) from a close-coupling R-matrix calculation involving all fine structure calculations among and within the 2s2 2p, 2s 2p2 and 2p3 configurations were discussed. There was no consensus if these results were more accurate than earlier close-coupling calculations. However, there was no reason to think they were less accurate. It was suggested that the Blum and Pradhan results be extended to higher temperatures. This has been done and the results published by Zhang, Graziani and Pradhan (Astron Astrophys 283, 319, 1994). The Zhang et al results were obtained electronically and processed into ADF04 format. Sampson et al pointed out that effective collision strength for the 1-2 transition appears to rise spuriously with temperature. In the newer results this does not occur. J Lang A Lanzafame May 1996 ----------------------------------------------------------------------------- File generated by altering the temperature set of an ADF04 file Comments from source file inserted above. Program: ADAS215 Source file: /u/hps/adas/adf04/cop98#8/blike_jl96#o3j.dat Producer: hps Date: 15/11/98 ------------------------------------------------------------------------------- --------------------------------------------------------------------------------- ---------------------------------------------------------------------------------