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J/A+AS/102/435 Transitions of SI in visible and infra-red (Biemont+ 1993)
Delta(n) ≤ 2 allowed transitions of neutral sulphur within the visible and infrared spectral ranges BIEMONT E., QUINET P., ZEIPPEN C.J. <Astron. Astrophys. Suppl. Ser. 102, 435 (1993)> =1993A&AS..102..435B
ADC_Keywords: Atomic physics; Abundances Keywords: atomic data - atomic processes - sun: abundances File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 27 26 Configurations selected for the present SST and HFR calculations in S I table2 32 36 HFR fitted parameters (even configurations) table3 32 37 HFR fitted parameters (odd configurations) table4 58 133 Excitation energies and fine-structure splittings table5 73 33 Calculated HFR energy level (even configuration table6 73 40 Calculated HFR energy level (odd configuration) table7 93 114 Calculated oscillator strengths (3p3(4S)nl - 3p3(4S)n'l') table8 93 16 Calculated oscillator strengths (3p3 (2D)nl - 3p3(2D)n'l') table9 63 30 S I lines and corresponding gf values
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
1- 3 A3 --- Mode Calculation mode (SST or HFR) 7- 14 A8 --- EP Even parity configuration 20- 27 A8 --- OP Odd parity configuration
Byte-by-byte Description of file: table2 table3
Bytes Format Units Label Explanations
1- 10 A10 --- Conf. Configuration 12- 20 A9 --- Param. Parameter 22- 26 I5 cm-1 Fit ? Fitted value 28- 31 F4.2 --- Fit/HFR ? Fitted-HFR ratio 32 A1 --- n_Fit/HFR [ f] When f, fixed value
Byte-by-byte Description of file: table4
Bytes Format Units Label Explanations
1- 9 A9 --- Config Configuration 12- 16 A5 --- Level Level designation 21- 27 F7.1 cm-1 E(obs) ? Observed excitation energy 32- 36 F5.1 cm-1 DeltaE(obs) ? Observed fine-structure splitting 42- 47 F6.1 cm-1 DeltaE(cal) ? Calculed present fine-structure splitting 51- 58 F8.1 cm-1 TEC ? Semi-empirical corrections to calculated non-relativistic energies
Byte-by-byte Description of file: table5 table6
Bytes Format Units Label Explanations
1- 8 A8 --- Conf Configuration 10- 18 A9 --- Level Level designation 22- 27 F6.0 cm-1 E(calc) HFR energy level 32- 36 F5.0 cm-1 Delta ? E(obs) - E(calc) 44- 73 A30 % Comp LS coupling composition: contributions ≥ 5% only are given
Byte-by-byte Description of file: table7 table8
Bytes Format Units Label Explanations
1- 15 A15 --- Transition 18- 26 F9.3 0.1nm Lambda Wavelength calculated with the levels of Martin et al. (1990) 29- 33 F5.2 --- HFR Calculated oscillator strength (log gf) obtained with HFR method 34 A1 --- n_HFR [ *] Cancellation factor (CF) *, as defined by Cowan (1981) (1) 36- 40 F5.2 --- SST Calculated oscillator strength (log gf) obtained with SST method 41 A1 --- n_SST [ +] When +, the length and velocity results differ by more than a factor of two 43- 47 F5.2 --- lg1 Oscillator strength (log gf) from other work 48- 49 A2 --- r_lg1 Reference to result lg1 (2) 51- 55 F5.2 --- lg2 ? Oscillator strength (log gf) from other work 56- 59 A4 --- r_lg2 Reference to result lg2 (2) 61- 65 F5.2 --- lg3 ? Oscillator strength (log gf) from other work 66- 67 A2 --- r_lg3 Reference to result lg3 (2) 70- 74 F5.2 --- lg4 ? Oscillator strength (log gf) from other work 75- 76 A2 --- r_lg4 Reference to result lg4 (2) 81- 85 F5.2 --- lg5 ? Oscillator strength (log gf) from other work 86 A1 --- r_lg5 Reference to result lg5 (2) 88- 92 F5.2 --- lg6 ? Oscillator strength (log gf) from other work 93 A1 --- r_lg6 Reference to result lg6 (2)
Note (1): A small value indicates strong cancellation effect. The starred transitions are those for which CF≤0.02 Note (2): a: Kurucz R.L. & Peytremann E., Smith. Astron. Obs. Spec. Report 362 (1975) b: Lambert D.L. & Warner B., MNRAS 138, 181 (1968) c: Biemont E. & Grevesse N., ADNDT 12, 217 (1973) d: Lambert D.L. & Luck R.E., MNRAS 183, 79 (1978) e: Aymar M., NIM 110, 211 (1973) f: Aymar M., Physica 66, 364 (1973) g: Wiese W. L. et al., (1969) h: Foster E.W., Proc. Phys. Soc. London 90, 275 (1967) i: Bridges J.M. & Wiese W.L., Phys. Rev. A159, 31 (1967) k: Miller M.H., Wilkerson T.D., Roig R.A. & Bengston R.D., Phys. Rev. A9, 2312 (1974)
Byte-by-byte Description of file: table9
Bytes Format Units Label Explanations
1- 9 F9.3 0.1nm Lambda(lab) Laboratory wavelength 13- 32 A20 --- Transition 34- 38 F5.2 --- log(gf) HFR oscillator strength 42- 46 F5.1 0.1pm Wlambda Equivalent width 51- 54 F4.2 eV Einf 59- 62 F4.2 --- A Abundance in the logarithmic scale calculated with the Holweger & Muller (1974) solar model 63 A1 --- u_A When :, the value was not retained in the final sample as explained in the text
(End) Patricia Bauer [CDS] 20-Oct-1993
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