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 CALCULATED BY THREE DIFFERENT METHODS A=1s 2s2 2p3, S=1s2 2s2 2p2 , Numbers following the letter mean (2S+1)(2L+1)(2J+1) Aa2 is the autoionizing rate to 1s2 2s2 2p 2P3/2 C-like ion: Z=26 Table VA calculated by Safranova (MZ code) Transition lambda(A) Qd1(1/s) Ar(1/s) Aa2(1/s) SumAa(1/s) Br A 155-S 335 1.8896 5.24E+12 4.70E+12 2.29E+14 5.20E+14 4.57E-03 A 313-S 331 1.8908 5.11E+12 2.35E+13 7.31E+13 3.24E+14 2.33E-02 A 133-S 155 1.8908 1.77E+14 3.91E+14 1.67E+14 4.50E+14 3.52E-01 A 335-S 333 1.8916 4.67E+12 4.79E+12 1.81E+14 5.34E+14 5.16E-03 A 331-S 333 1.8921 4.31E+13 2.14E+14 1.52E+14 5.23E+14 2.82E-01 A 333-S 335 1.8925 1.52E+14 3.27E+14 1.35E+14 4.80E+14 3.76E-01 A 335-S 335 1.8932 3.02E+14 3.09E+14 1.81E+14 5.34E+14 3.33E-01 A 313-S 333 1.8933 9.88E+13 4.53E+14 7.31E+13 3.24E+14 4.49E-01 A 155-S 155 1.8941 5.40E+14 4.86E+14 2.29E+14 5.20E+14 4.73E-01 A 353-S 331 1.8944 4.01E+13 2.78E+14 4.17E+13 5.19E+14 3.19E-01 A 313-S 335 1.8949 3.60E+13 1.65E+14 7.31E+13 3.24E+14 1.64E-01 A 133-S 111 1.8957 1.18E+14 2.61E+14 1.67E+14 4.50E+14 2.35E-01 A 355-S 333 1.8965 9.21E+13 2.09E+14 7.01E+13 5.62E+14 2.62E-01 A 357-S 335 1.8969 3.27E+14 1.75E+14 2.18E+14 5.85E+14 2.14E-01 A 335-S 155 1.8977 6.73E+13 6.89E+13 1.81E+14 5.34E+14 7.43E-02 A 355-S 335 1.8981 1.52E+12 3.45E+12 7.01E+13 5.62E+14 4.33E-03 A 353-S 335 1.8986 8.82E+12 6.13E+13 4.17E+13 5.19E+14 7.03E-02 A 313-S 155 1.8994 7.61E+12 3.50E+13 7.31E+13 3.24E+14 3.47E-02 A 357-S 155 1.9014 9.89E+13 5.29E+13 2.18E+14 5.85E+14 6.50E-02 A 333-S 111 1.9019 1.88E+13 4.04E+13 1.35E+14 4.80E+14 4.64E-02 A 355-S 155 1.9026 7.29E+12 1.66E+13 7.01E+13 5.62E+14 2.08E-02 A 353-S 155 1.9031 9.29E+11 6.47E+12 4.17E+13 5.19E+14 7.41E-03 A 515-S 333 1.9044 5.72E+11 7.72E+12 5.58E+12 3.58E+14 2.05E-02 A 515-S 335 1.9060 6.43E+11 8.68E+12 5.58E+12 3.58E+14 2.31E-02