S (Z=16)
* Here "He-like" represents the final ionic state,
i.e., satellite lines due to dielectronic
recombination from H-like ion to He-like ion.
He-like S (SXV)
-
L.A. Vainshtein and U.I.Safronova, 1978, ADNDT 21, 49
"Wavelenvths and Transition Probabilities of Satellites to Resonance
Lines of H- and He-like Ions"
Table text file (1.7kbyte)
-
L.A. Vainshtein and U.I.Safronova, 1978, ADNDT 25, 311
"Dielectronic Satellite Spectra for Highly Charged H-like Ions
(2l'3l"-1s2l, 2l'3l"01s3l) and He-like Ions
(1s2l'3l"-1s22l, 1s2l'3l"-1s23l) with Z=6-33"
Table text file (5.9kbyte)
Li-like S (SXIV)
-
L.A. Vainshtein and U.I.Safronova, 1978, ADNDT 21, 49
"Wavelenvths and Transition Probabilities of Satellites to Resonance
Lines of H- and He-like Ions"
Table text file (2.3kbyte)
-
L.A. Vainshtein and U.I.Safronova, 1978, ADNDT 25, 311
"Dielectronic Satellite Spectra for Highly Charged H-like Ions
(2l'3l"-1s2l, 2l'3l"01s3l) and He-like Ions
(1s2l'3l"-1s22l, 1s2l'3l"-1s23l) with Z=6-33"
Table text file (8.1kbyte)
-
T. Kato, U.I. Safronova, A.S. Shlyaptseva, M. Cornille, J. Dubau and J. Nilsen 1997, ADNDT 67, 225
"COMPARISON OF SATELLITE SPECTRA FOR H-LIKE Fe AND He-LIKE Fe, Ca, AND S CALCULA
TED BY THREE DIFFERENT METHODS"
Calculated by Safronova (MZ code):
Text file (25kbyte)
Calculated by Cornille and Dubau (AUTOLSJ code):
Text file (10kbyte)
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