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



 B-like ion: Z=26
   Table IVB    calculated by Cornille and Dubau (AUTOLSJ code)

lower level        upper level          lambda(A) Qd(1/s)     Ar(1/s)   SumAa(1/s) Br

1s2s2s2p2p 4P 0.5 1s1s2s2s2p 2P 0.5	  1.8883  1.510E+12  2.780E+13  2.192E+14  0.110
1s2s2s2p2p 4P 2.5 1s1s2s2s2p 2P 1.5	  1.8880  9.290E+12  2.550E+13  2.312E+14  0.098
1s2s2s2p2p 4P 2.5 1s1s2p2p2p 4S 1.5	  1.9293  1.420E+12  3.890E+12  2.312E+14  0.015
1s2s2s2p2p 2D 1.5 1s1s2s2s2p 2P 0.5	  1.8787  1.995E+14  2.889E+14  2.878E+14  0.470
1s2s2s2p2p 2D 1.5 1s1s2s2s2p 2P 1.5	  1.8830  2.115E+13  3.063E+13  2.878E+14  0.050
1s2s2s2p2p 2D 1.5 1s1s2p2p2p 2D 1.5	  1.9297  1.630E+12  2.360E+12  2.878E+14  0.004
1s2s2s2p2p 2D 1.5 1s1s2p2p2p 2D 2.5	  1.9312  2.230E+12  3.230E+12  2.878E+14  0.005
1s2s2s2p2p 2P 0.5 1s1s2s2s2p 2P 0.5	  1.8786  1.370E+13  5.070E+14  1.520E+14  0.666
1s2s2s2p2p 2P 0.5 1s1s2s2s2p 2P 1.5	  1.8829  2.470E+12  9.140E+13  1.520E+14  0.120
1s2s2s2p2p 2D 2.5 1s1s2s2s2p 2P 1.5	  1.8812  2.678E+14  1.953E+14  3.184E+14  0.375
1s2s2s2p2p 2D 2.5 1s1s2p2p2p 2D 1.5	  1.9278  2.020E+12  1.470E+12  3.184E+14  0.003
1s2s2s2p2p 2D 2.5 1s1s2p2p2p 2D 2.5	  1.9293  6.660E+12  4.860E+12  3.184E+14  0.009
1s2s2s2p2p 2P 1.5 1s1s2s2s2p 2P 0.5	  1.8736  1.540E+12  1.070E+13  1.766E+14  0.014
1s2s2s2p2p 2P 1.5 1s1s2s2s2p 2P 1.5	  1.8778  8.207E+13  5.691E+14  1.766E+14  0.741
1s2s2s2p2p 2S 0.5 1s1s2s2s2p 2P 1.5	  1.8763  8.036E+13  2.930E+14  2.543E+14  0.527
1s2s2s2p2p 2S 0.5 1s1s2p2p2p 2P 0.5	  1.9295  1.320E+12  4.820E+12  2.543E+14  0.009
1s2s2p2p2p 2P 0.5 1s1s2s2p2p 2P 0.5	  1.8785  1.620E+12  2.500E+14  2.726E+14  0.355
1s2s2p2p2p 2P 1.5 1s1s2s2p2p 2P 1.5	  1.8810  3.820E+12  2.005E+14  3.309E+14  0.358
1s2s2p2p2p 2S 0.5 1s1s2s2p2p 2P 1.5	  1.8794  1.280E+12  6.065E+14  1.540E+14  0.699