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 Aa1 is the autoionizing rate to 1s2 2s2 2p 2P1/2 C-like ion: Z=26 Table VB calculated by Cornille and Dubau (AUTOLSJ code) lower level upper level lambda(A) Qd(1/s) Ar(1/s) Aa1(1/s) SumAa(1/s) Br 1s2s2 2p3 3D 1 1s2 2s2 2p2 3P 0 1.8905 1.472E+14 2.644E+14 1.309E+14 3.843E+14 0.375 1s2s2 2p3 3D 1 1s2 2s2 2p2 3P 2 1.8948 2.466E+13 4.430E+13 1.309E+14 3.843E+14 0.063 1s2s2 2p3 3D 1 1s2 2s2 2p2 1D 2 1.8995 4.340E+12 7.800E+12 1.309E+14 3.843E+14 0.011 1s2s2 2p3 3D 2 1s2 2s2 2p2 3P 1 1.8925 1.987E+14 2.010E+14 1.239E+14 4.098E+14 0.321 1s2s2 2p3 3D 2 1s2 2s2 2p2 3P 2 1.8941 3.140E+12 3.180E+12 1.239E+14 4.098E+14 0.005 1s2s2 2p3 3D 2 1s2 2s2 2p2 1D 2 1.8988 1.020E+13 1.032E+13 1.239E+14 4.098E+14 0.016 1s2s2 2p3 3D 3 1s2 2s2 2p2 3P 2 1.8926 7.576E+13 1.633E+14 4.243E+13 4.260E+14 0.255 1s2s2 2p3 3D 3 1s2 2s2 2p2 1D 2 1.8973 2.242E+13 4.834E+13 4.243E+13 4.260E+14 0.075 1s2s2 2p3 3S 1 1s2 2s2 2p2 3P 1 1.8893 2.066E+13 4.336E+14 1.391E+13 2.558E+14 0.495 1s2s2 2p3 3S 1 1s2 2s2 2p2 3P 2 1.8909 6.340E+12 1.330E+14 1.391E+13 2.558E+14 0.152 1s2s2 2p3 3P 0 1s2 2s2 2p2 3P 1 1.8884 2.008E+13 2.232E+14 5.559E+13 3.917E+14 0.361 1s2s2 2p3 3P 2 1s2 2s2 2p2 3P 2 1.8892 9.112E+13 3.045E+14 4.549E+13 3.906E+14 0.401 1s2s2 2p3 3P 2 1s2 2s2 2p2 1D 2 1.8939 1.743E+13 5.823E+13 4.549E+13 3.906E+14 0.077 1s2s2 2p3 3P 1 1s2 2s2 2p2 3P 2 1.8886 6.076E+13 3.637E+14 4.173E+13 3.385E+14 0.485 1s2s2 2p3 3P 1 1s2 2s2 2p2 1S 0 1.8976 5.810E+12 3.480E+13 4.173E+13 3.385E+14 0.046 1s2s2 2p3 1D 2 1s2 2s2 2p2 1D 2 1.8900 4.246E+13 4.847E+14 1.538E+13 3.807E+14 0.552 1s2s2 2p3 1P 1 1s2 2s2 2p2 1D 2 1.8872 2.330E+13 3.931E+14 1.938E+13 3.268E+14 0.401 1s2s2 2p3 1P 1 1s2 2s2 2p2 1S 0 1.8915 1.477E+13 2.493E+14 1.938E+13 3.268E+14 0.254