| 2s2.2p3 4s3/2 4S1.5 | 0.0 cm-1 |
| 2s2.2p3 2d3/2 2D1.5 | 72146.2 cm-1 |
| 2s2.2p3 2d5/2 2D2.5 | 72493.1 cm-1 |
| 2s2.2p3 2p1/2 2P0.5 | 104207.0 cm-1 |
| 2s2.2p3 2p3/2 2P1.5 | 104852.0 cm-1 |
| 2s.2p4 4p5/2 4P2.5 | 311572.0 cm-1 |
| 2s.2p4 4p3/2 4P1.5 | 315121.0 cm-1 |
| 2s.2p4 4p1/2 4P0.5 | 316976.0 cm-1 |
| 2s.2p4 2d3/2 2D1.5 | 440862.0 cm-1 |
| 2s.2p4 2d5/2 2D2.5 | 440862.0 cm-1 |
| 2s.2p4 2s1/2 2S0.5 | 513533.0 cm-1 |
| 2s.2p4 2p3/2 2P1.5 | 548779.0 cm-1 |
| 2s.2p4 2p1/2 2P0.5 | 553054.0 cm-1 |
| 2p5 2p3/2 2P1.5 | 847769.0 cm-1 |
| 2p5 2p1/2 2P0.5 | 853415.0 cm-1 |
| 2s2.2p2(3p)3s 4p1/2 4P0.5 | 1436060.0 cm-1 |
| 2s2.2p2(3p)3s 4p3/2 4P1.5 | 1438320.0 cm-1 |
| 2s2.2p2(3p)3s 4p5/2 4P2.5 | 1441650.0 cm-1 |
| 2s2.2p2(3p)3s 2p1/2 2P0.5 | 1456560.0 cm-1 |
| 2s2.2p2(3p)3s 2p3/2 2P1.5 | 1460590.0 cm-1 |
| 2s2.2p2(1d)3s 2d5/2 2D2.5 | 1495610.0 cm-1 |
| 2s2.2p2(1d)3s 2d3/2 2D1.5 | 1495720.0 cm-1 |
| 2s2.2p2(3p)3p 2s1/2 2S0.5 | 1512720.0 cm-1 |
| 2s2.2p2(3p)3p 4d1/2 4D0.5 | 1518730.0 cm-1 |
| 2s2.2p2(3p)3p 4d3/2 4D1.5 | 1520000.0 cm-1 |
| 2s2.2p2(3p)3p 4d5/2 4D2.5 | 1522170.0 cm-1 |
| 2s2.2p2(3p)3p 4d7/2 4D3.5 | 1525110.0 cm-1 |
| 2s2.2p2(3p)3p 4p1/2 4P0.5 | 1527330.0 cm-1 |
| 2s2.2p2(3p)3p 4p3/2 4P1.5 | 1528120.0 cm-1 |
| 2s2.2p2(3p)3p 4p5/2 4P2.5 | 1530110.0 cm-1 |
| 2s2.2p2(3p)3p 2d3/2 2D1.5 | 1539940.0 cm-1 |
| 2s2.2p2(3p)3p 2d5/2 2D2.5 | 1544100.0 cm-1 |
| 2s2.2p2(3p)3p 2p3/2 2P1.5 | 1554660.0 cm-1 |
| 2s2.2p2(3p)3p 2p1/2 2P0.5 | 1554880.0 cm-1 |
| 2s2.2p2(3p)3p 4s3/2 4S1.5 | 1559360.0 cm-1 |
| 2s2.2p2(1s)3s 2s1/2 2S0.5 | 1569530.0 cm-1 |
| 2s2.2p2(1d)3p 2f5/2 2F2.5 | 1579980.0 cm-1 |
| 2s2.2p2(1d)3p 2f7/2 2F3.5 | 1580980.0 cm-1 |
| 2s2.2p2(1d)3p 2d5/2 2D2.5 | 1605260.0 cm-1 |
| 2s2.2p2(1d)3p 2d3/2 2D1.5 | 1605450.0 cm-1 |
| 2s2.2p2(1d)3p 2p1/2 2P0.5 | 1613690.0 cm-1 |
| 2s2.2p2(1d)3p 2p3/2 2P1.5 | 1616530.0 cm-1 |
| 2s2.2p2(3p)3d 4f3/2 4F1.5 | 1619900.0 cm-1 |
| 2s2.2p2(3p)3d 4f5/2 4F2.5 | 1621050.0 cm-1 |
| 2s2.2p2(3p)3d 4f7/2 4F3.5 | 1622760.0 cm-1 |
| 2s2.2p2(3p)3d 4f9/2 4F4.5 | 1625060.0 cm-1 |
| 2s2.2p2(3p)3d 4d3/2 4D1.5 | 1630250.0 cm-1 |
| 2s2.2p2(3p)3d 4d1/2 4D0.5 | 1630450.0 cm-1 |
| 2s2.2p2(3p)3d 4d5/2 4D2.5 | 1631690.0 cm-1 |
| 2s2.2p2(3p)3d 4d7/2 4D3.5 | 1632810.0 cm-1 |
| 2s2.2p2(3p)3d 2p3/2 2P1.5 | 1632900.0 cm-1 |
| 2s2.2p2(3p)3d 2p1/2 2P0.5 | 1635920.0 cm-1 |
| 2s2.2p2(3p)3d 2f5/2 2F2.5 | 1640560.0 cm-1 |
| 2s2.2p2(3p)3d 4p5/2 4P2.5 | 1643490.0 cm-1 |
| 2s2.2p2(3p)3d 2f7/2 2F3.5 | 1644910.0 cm-1 |
| 2s2.2p2(3p)3d 4p3/2 4P1.5 | 1645010.0 cm-1 |
| 2s2.2p2(3p)3d 4p1/2 4P0.5 | 1645810.0 cm-1 |
| 2s2.2p2(1s)3p 2p1/2 2P0.5 | 1664770.0 cm-1 |
| 2s2.2p2(1s)3p 2p3/2 2P1.5 | 1664770.0 cm-1 |
| 2s2.2p2(3p)3d 2d3/2 2D1.5 | 1668580.0 cm-1 |
| 2s2.2p2(3p)3d 2d5/2 2D2.5 | 1669500.0 cm-1 |
| 2s2.2p2(1d)3d 2g7/2 2G3.5 | 1683560.0 cm-1 |
| 2s2.2p2(1d)3d 2g9/2 2G4.5 | 1683900.0 cm-1 |
| 2s2.2p2(1d)3d 2d3/2 2D1.5 | 1694130.0 cm-1 |
| 2s2.2p2(1d)3d 2f5/2 2F2.5 | 1694270.0 cm-1 |
| 2s2.2p2(1d)3d 2f7/2 2F3.5 | 1694530.0 cm-1 |
| 2s2.2p2(1d)3d 2d5/2 2D2.5 | 1696400.0 cm-1 |
| 2s2.2p2(1d)3d 2p1/2 2P0.5 | 1704010.0 cm-1 |
| 2s2.2p2(1d)3d 2p3/2 2P1.5 | 1705280.0 cm-1 |
| 2s2.2p2(1d)3d 2s1/2 2S0.5 | 1712190.0 cm-1 |
| 2s2.2p2(1s)3d 2d5/2 2D2.5 | 1764900.0 cm-1 |
| 2s2.2p2(1s)3d 2d3/2 2D1.5 | 1765740.0 cm-1 |
---------------------------------------------------------------------------- Data generated from CHIANTI version 6.0 http://www.chianti.rl.ac.uk/ CHIANTI references ------------------ Energy levels : %Observed energy levels (1-15): Edlen, 1984, Phys.Scripta, 30, 135 %Observed energy levels (16-72): Fuhr, J.R., Kelleher, D.E., Martin, W.C., Musgrove, A., Sugar, J., Wiese, W.L., Dalton, G.R., Dragoset, R.A., Mohr, P.J., Olsen, K., Reader, J., Saloman, E.B., Sansonetti, C.J., Wiersma, G., "NIST Atomic Spectra Database" Ver. 2.0, March 1999, NIST Physical Reference Data %Observed energy levels (24-27; 43-46 -> 2s2.2p2(3P)3p 4D and 2s2.2p2(3P)3d 4F): Kink, I., Engstroem, L., Feldman, U., 1999, ApJ, 512, 496 %Theoretical energy levels (1-15): Zhang, Sampson, ADNDT, 1999, 72, 153 %Theoretical energy levels (16-72): Bhatia & Landi, 2003, ADNDT, 85, 317 %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E. Landi and G. Del Zanna, 2001 A-values levels : %filename: si_8.wgfa %Observed energy levels (1- 15): Edlen, 1984, Phys.Scripta, 30, 135 %Observed energy levels (16-72): Fuhr, J.R., et al., "NIST Atomic Spectra Database" Ver. 2.0, March 1999, NIST Physical Reference Data %Observed energy levels (24-27; 43-46 -> 2s2.2p2(3P)3p 4D and 2s2.2p2(3P)3d 4F): Kink, I., Engstroem, L., Feldman, U., 1999, ApJ, 512, 496 % A values for transitions within the ground configuration: Merkelis et al., 1999, Physica Scripta 59,122 % gf values for transitions between the (1- 15) levels: Zhang, Sampson, ADNDT, 1999, 72, 153 % A values for transitions with 2s.2p4 and 2p5 levels: Zhang, Sampson, ADNDT, 1999, 72, 153 % A values for forbidden transitions with n=2 configurations: Merkelis et al., 1999, Physica Scripta 59,122 % Oscillator strengths and A values levels 16-72: Bhatia & Landi, 2003, ADNDT, 85, 317 %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E. Landi and G. Del Zanna 2001 Collision strengths : %filename: si_8.splups %oscillator strengths (1 - 15): Zhang, Sampson, 1999, ADNDT, 72, 153 %oscillator strengths (16 - 72): Bhatia & Landi, 2003, ADNDT, 85, 317 %effective collision strengths within the ground configuration: Bell, Matthews and Ramsbottom, 2001, MNRAS 322, 779 %collision strengths all other transitions within levels 1 - 15: Zhang, Sampson, 1999, ADNDT, 72, 153 %collision strengths (16 - 72): Bhatia & Landi, 2003, ADNDT, 85, 317 %comment: transition energies within the ground configuration: Edlen, 1984, Phys.Scripta, 30, 135 %comment: effective collision strengths were provided in the temperature range 3.3 < Log T < 6.5 %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E. Landi and G. Del Zanna, Dec 2001 Added to ADAS by ---------------- Author : Martin O'Mullane Date : 12/03/13 ---------------------------------------------------------------------------- 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 : 12-03-2013 Producer : Martin O'Mullane -------------------------------------------------------------------------------