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J/A+AS/102/435 Transitions of SI in visible and infra-red (Biemont+ 1993)
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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
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ADC_Keywords: Atomic physics; Abundances
Keywords: atomic data - atomic processes - sun: abundances
File Summary:
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FileName Lrecl Records Explanations
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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 59 33 Calculated HFR energy level (even configuration
table6 72 40 Calculated HFR energy level (odd configuration)
table7 93 114 Calculated oscillator strengths
(3p3(4S)nl - 3p3(4S)n'l')
table8 75 16 Calculated oscillator strengths
(3p3 (2D)nl - 3p3(2D)n'l')
table9 63 30 S I lines and corresponding gf values
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Byte-by-byte Description of file: table1
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Bytes Format Units Label Explanations
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1- 3 A3 --- Mode Calculation mode (SST or HFR)
7- 14 A8 --- EP Even parity configuration
20- 27 A8 --- OP Odd parity configuration
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Byte-by-byte Description of file: table2 table3
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Bytes Format Units Label Explanations
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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
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Byte-by-byte Description of file: table4
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Bytes Format Units Label Explanations
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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
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Byte-by-byte Description of file: table5 table6
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Bytes Format Units Label Explanations
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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
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Byte-by-byte Description of file: table7 table8
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Bytes Format Units Label Explanations
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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)
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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
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Bytes Format Units Label Explanations
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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
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(End) Patricia Bauer [CDS] 20-Oct-1993