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 Be-like ion: Z=26 Table IIIB calculated by Cornille and Dubau (AUTOLSJ code) lower level upper level lambda(A) Qd(1/s) Ar(1/s) SumAa(1/s) Br 1s2s2s2p 3P 0 1s1s2p2p 3P 1 1.9135 2.760E+12 7.970E+12 1.770E+14 0.043 1s2s2s2p 3P 1 1s1s2s2s 1S 0 1.8756 2.652E+13 3.203E+13 1.746E+14 0.148 1s2s2s2p 3P 1 1s1s2p2p 3P 0 1.9095 3.140E+12 3.790E+12 1.746E+14 0.018 1s2s2s2p 3P 1 1s1s2p2p 3P 2 1.9144 2.890E+12 3.500E+12 1.746E+14 0.016 1s2s2s2p 3P 2 1s1s2p2p 3P 1 1.9085 5.540E+12 3.330E+12 1.801E+14 0.017 1s2s2s2p 3P 2 1s1s2p2p 3P 2 1.9105 9.670E+12 5.810E+12 1.801E+14 0.030 1s2s2s2p 3P 2 1s1s2p2p 1D 2 1.9159 2.180E+12 1.310E+12 1.801E+14 0.007 1s2s2p2p 5P 1 1s1s2s2p 3P 1 1.8847 2.980E+12 7.260E+12 2.610E+12 0.538 1s2s2p2p 5P 2 1s1s2s2p 3P 2 1.8863 3.450E+12 4.150E+12 1.080E+12 0.791 1s2s2p2p 5P 3 1s1s2s2p 3P 2 1.8841 2.450E+13 9.160E+12 7.120E+12 0.563 1s2s2s2p 1P 1 1s1s2s2s 1S 0 1.8668 1.255E+13 4.356E+14 1.328E+14 0.744 1s2s2p2p 3P 0 1s1s2s2p 3P 1 1.8717 3.100E+12 5.959E+14 4.842E+13 0.924 1s2s2p2p 3P 1 1s1s2s2p 3P 0 1.8693 8.494E+13 3.840E+14 5.844E+13 0.629 1s2s2p2p 3P 1 1s1s2s2p 3P 1 1.8705 1.236E+13 5.587E+13 5.844E+13 0.092 1s2s2p2p 3P 1 1s1s2s2p 3P 2 1.8742 2.480E+13 1.121E+14 5.844E+13 0.184 1s2s2p2p 3D 2 1s1s2s2p 3P 1 1.8698 3.816E+14 3.235E+14 1.316E+14 0.667 1s2s2p2p 3D 2 1s1s2s2p 3P 2 1.8735 3.074E+13 2.606E+13 1.316E+14 0.054 1s2s2p2p 3D 2 1s1s2s2p 1P 1 1.8838 4.880E+12 4.130E+12 1.316E+14 0.009 1s2s2p2p 3D 1 1s1s2s2p 3P 1 1.8686 1.757E+14 2.603E+14 1.361E+14 0.545 1s2s2p2p 3D 1 1s1s2s2p 3P 2 1.8724 5.132E+13 7.602E+13 1.361E+14 0.159 1s2s2p2p 3D 3 1s1s2s2p 3P 2 1.8721 5.862E+14 2.215E+14 1.687E+14 0.568 1s2s2p2p 3P 2 1s1s2s2p 3P 1 1.8666 9.580E+12 2.520E+13 8.517E+13 0.042 1s2s2p2p 3P 2 1s1s2s2p 3P 2 1.8703 1.802E+14 4.741E+14 8.517E+13 0.795 1s2s2p2p 3P 2 1s1s2s2p 1P 1 1.8805 4.400E+12 1.157E+13 8.517E+13 0.019 1s2s2p2p 3S 1 1s1s2s2p 3P 1 1.8641 1.355E+13 4.227E+13 1.272E+14 0.155 1s2s2p2p 3S 1 1s1s2s2p 3P 2 1.8678 2.548E+13 7.950E+13 1.272E+14 0.292 1s2s2p2p 3S 1 1s1s2s2p 1P 1 1.8780 6.330E+12 1.976E+13 1.272E+14 0.072 1s2s2p2p 1D 2 1s1s2s2p 3P 2 1.8650 9.414E+13 8.739E+13 2.189E+14 0.190 1s2s2p2p 1D 2 1s1s2s2p 1P 1 1.8751 1.644E+14 1.526E+14 2.189E+14 0.332 1s2s2p2p 3P 1 1s1s2s2p 3P 2 1.8636 5.094E+13 1.697E+14 1.120E+14 0.592 1s2s2p2p 3P 2 1s1s2s2p 3P 2 1.8617 2.790E+12 3.360E+12 2.087E+14 0.012 1s2s2p2p 3P 2 1s1s2s2p 1P 1 1.8718 5.802E+13 6.997E+13 2.087E+14 0.248 1s2s2p2p 1P 1 1s1s2s2p 1P 1 1.8684 1.074E+13 6.747E+14 6.992E+13 0.904 1s2s2p2p 1S 0 1s1s2s2p 1P 1 1.8671 3.052E+13 2.254E+14 1.975E+14 0.533 1s2p2p2p 3P 1 1s1s2p2p 3P 2 1.8683 2.820E+12 2.669E+14 1.384E+14 0.576 1s2p2p2p 3P 2 1s1s2p2p 1D 2 1.8710 4.110E+12 3.842E+14 1.806E+14 0.670