Abstract
Oscillator strengths are calculated for resonance lines of some silicon and sulfur ions, which are present in the solar spectrum from about 160 Å to 380 Å. Spin-spin and spin-other orbit interactions are included. A comparison is made with Garstang's results for Six; agreement is good.
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References
Froese, C.: 1963, Can. J. Phys. 41, 1895.
Garstang, R. H.: 1962, Ann. Astrophys. 25, 109.
Jordan, C. J.: 1966, Mon. Not. Roy. Astron. Soc. 132, 463.
Moore, C. E.: 1949, Atomic Energy Levels, NBS Circ. 467.
Obi, S. and Yanagawa, S.: 1955, Pub. Astron. Soc. Japan 7, 125.
Pottasch, S. R.: 1963, Astrophys. J. 137, 945.
Shore, B. W. and Menzel, D. H.: 1965, Astrophys. J. Supplement 12, No. 106, 187.
Varsavsky, C.: 1961, Astrophys. J. Supplement 6, No. 53, 75.
Widing, K. G. and Porter, J. R.: 1964, I.A.U. Symposium (Liège) 23, 115.
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Kastner, S.O. Oscillator strengths for resonance lines of some silicon and sulfur ions. Sol Phys 2, 196–201 (1967). https://doi.org/10.1007/BF00155920
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DOI: https://doi.org/10.1007/BF00155920