chv6_ic#ca18.dat
Resolved Specific Ion Data Collections
- Ion
- Ca18+
- Temperature Range
- 15.51 eV → 1.551 x 104 eV
ADF04
- Filename
- chv6_ic#ca18.dat
- Full Path
- adf04/copch#20/chv6_ic#ca18.dat
Download data
- Spontaneous Emission: Ca+18(i) → Ca+18(j) + hv
- Electron Impact Excitation: Ca+18(i) + e → Ca+18(j) + e
| 1s2 1s0 1S0.0 | 0.0 cm-1 |
| 1s.2s 3s1 3S1.0 | 31165400.0 cm-1 |
| 1s.2p 3p0 3P0.0 | 31327800.0 cm-1 |
| 1s.2p 3p1 3P1.0 | 31345400.0 cm-1 |
| 1s.2s 1s0 1S0.0 | 31354100.0 cm-1 |
| 1s.2p 3p2 3P2.0 | 31389300.0 cm-1 |
| 1s.2p 1p1 1P1.0 | 31520900.0 cm-1 |
| 1s.3s 3s1 3S1.0 | 36893700.0 cm-1 |
| 1s.3s 1s0 1S0.0 | 36942000.0 cm-1 |
| 1s.3p 3p0 3P0.0 | 36942000.0 cm-1 |
| 1s.3p 3p1 3P1.0 | 36946400.0 cm-1 |
| 1s.3p 3p2 3P2.0 | 36955100.0 cm-1 |
| 1s.3d 3d1 3D1.0 | 36985900.0 cm-1 |
| 1s.3d 3d2 3D2.0 | 36985900.0 cm-1 |
| 1s.3d 3d3 3D3.0 | 36990300.0 cm-1 |
| 1s.3p 1p1 1P1.0 | 36994600.0 cm-1 |
| 1s.3d 1d2 1D2.0 | 36994600.0 cm-1 |
| 1s.4s 3s1 3S1.0 | 38873300.0 cm-1 |
| 1s.4p 3p0 3P0.0 | 38890900.0 cm-1 |
| 1s.4s 1s0 1S0.0 | 38895300.0 cm-1 |
| 1s.4p 3p1 3P1.0 | 38895300.0 cm-1 |
| 1s.4p 3p2 3P2.0 | 38899700.0 cm-1 |
| 1s.4p 1p1 1P1.0 | 38912900.0 cm-1 |
| 1s.4d 3d1 3D1.0 | 38912900.0 cm-1 |
| 1s.4d 3d2 3D2.0 | 38912900.0 cm-1 |
| 1s.4d 3d3 3D3.0 | 38912900.0 cm-1 |
| 1s.4d 1d2 1D2.0 | 38912900.0 cm-1 |
| 1s.4f 3f2 3F2.0 | 38912900.0 cm-1 |
| 1s.4f 3f3 3F3.0 | 38912900.0 cm-1 |
| 1s.4f 3f4 3F4.0 | 38917200.0 cm-1 |
| 1s.4f 1f3 1F3.0 | 38917200.0 cm-1 |
Contributors
- CHIANTI
- Douglas Sampson
- K P Dere
- Martin O'Mullane
A+18 20 19 39733116.0 ---------------------------------------------------------------------------- Data generated from CHIANTI version 6.0 http://www.chianti.rl.ac.uk/ CHIANTI references ------------------ Energy levels : %observed energy levels: Martin,W.C., Sugar,J., Musgrove,A., Dalton,G.R., 1995, NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61 %observed energy levels (2s2p 3P): Chen, M.H., Cheng, K.T., Johnson, W.R., 1993, Ph.Rev.A, 47, 3692 %theoretical energy levels: Sampson, D.H., Goett, S.J., Clark, R.E.H., 1983, ADNDT, 29, 467 %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration CHIANTI % % K.P.Dere and E.Landi 2000 A-values levels : %filename: ca_19.wgfa %observed energy levels: Martin,W.C., Sugar,J., Musgrove,A., Dalton,G.R., 1995, NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61. %observed energy levels (2s2p 3P): Chen, M.H., Cheng, K.T., Johnson, W.R., 1993, Ph.Rev.A, 47, 3692 %theoretical energy levels: Sampson, D.H., Goett, S.J., Clark, R.E.H., 1983, ADNDT, 29, 467 %A values (1-2,5,6; 2-4,5,6): Lin, C.D., Johnson, W.R., Dalgarno, A., Phys Rev A, 1977, 15, 154 %A values (1-3 2 phot transition): Drake, G.W.F., Phys Rev A, 1986, 34, 2871 %oscillator strengths involving the 1s2 and 1s.2s configuration: Sampson, D.H., Goett, S.J., Clark, R.E.H., 1983, ADNDT, 29, 467, Hydrogenic values %oscillator strengths: Wiese, W.L., Smith, M.W., Glennon, B.M., 1966, Atomic Transition Probabilities, NSRDS-NBS-4 %comment: Wiese's oscillator strengths are hydrogenic %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % K.P.Dere and E.Landi - Jan 2005 Collision strengths : %filename: ca_19.splups %oscillator strengths (levels up to 17): Kimura et al. 2000, J. Phys. B, 33, 3449 %oscillator strengths involving the 1s2 and 1s.2s configuration to levels 18-49: Sampson, D.H., Goett, S.J., Clark, R.E.H., 1983, ADNDT, 29, 467, Hydrogenic values %oscillator strengths: Wiese, W.L., Smith, M.W., Glennon, B.M., 1966, Atomic Transition Probabilities, NSRDS-NBS-4 %effective collision strengths (levels up to 17): Kimura et al. 2000, J. Phys. B, 33, 3449 %collison strengths involving the 1s2 and 1s.2s configuration: Sampson, D.H., Goett, S.J., Clark, R.E.H. 1983, ADNDT, 29, 467, Hydrogenic values %comment: effective collision strengths from Kimura et al. were provided in the temperature range 6.4 < log T < 8.0 %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % G. Del Zanna - Nov 2007 Added to ADAS by ---------------- Author : Martin O'Mullane Date : 28/10/10 ---------------------------------------------------------------------------- The following levels were above the ionisation potential : 39733116.0 32 1s.5s 3S1 (3)0( 1.0) 39781970.4 33 1s.5s 1S0 (1)0( 0.0) 39790751.2 34 1s.5p 3P0 (3)1( 0.0) 39790751.2 35 1s.5p 3P1 (3)1( 1.0) 39795141.6 36 1s.5p 3P2 (3)1( 2.0) 39795141.6 37 1s.5p 1P1 (1)1( 1.0) 39803919.2 38 1s.5d 3D1 (3)2( 1.0) 39803919.2 39 1s.5d 3D2 (3)2( 2.0) 39803919.2 40 1s.5d 3D3 (3)2( 3.0) 39803919.2 41 1s.5d 1D2 (1)2( 2.0) 39803919.2 42 1s.5f 3F2 (3)3( 2.0) 39803919.2 43 1s.5f 3F3 (3)3( 3.0) 39803919.2 44 1s.5f 3F4 (3)3( 4.0) 39803919.2 45 1s.5f 1F3 (1)3( 3.0) 39803919.2 46 1s.5g 3G3 (3)4( 3.0) 39803919.2 47 1s.5g 3G4 (3)4( 4.0) 39803919.2 48 1s.5g 3G5 (3)4( 5.0) 39803919.2 49 1s.5g 1G4 (1)4( 4.0) 39803919.2 ------------------------------------------------------------------------------- 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 Original level order : 1 2 4 5 3 6 7 8 9 10 11 12 14 15 16 13 17 18 20 19 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 ------------------------------------------------------------------------------- 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 : ADAS utility program, filter04 Date : 28-10-2010 Producer : Martin O'Mullane ------------------------------------------------------------------------------- Regenerated to use the standard ADAS temperature set. Add the transitions in the CHIANTI source which have a transition probability but no accompanying effective collision strength and set these upsilons to zero. Update : Martin O'Mullane Date : 28-10-2010 -------------------------------------------------------------------------------