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Table 4:

List of the Fe XVII strongest lines in the 200-450 Å range.
i-j Transition Int Int(B84) $\lambda_{\rm exp.}$ $\lambda_{\rm CC}$ $\lambda_{\rm NIST}$ $\lambda_{\rm MR-MP}$
3-15 2s22p53s 1P1-2s22p53p 1S0 1.0 1 204.668 196.38 204.650 205.34
5-15 2s22p53s 3P1-2s22p53p 1S0 1.1 1.1 254.885 243.47 254.751 255.93
2-8 2s22p53s 3P2-2s22p53p 3D3 1.2 0.54 350.478 348.22 350.582 350.30
5-14 2s22p53s 3P1-2s22p53p 1D2 0.78 0.28 347.816 345.98 347.959 347.69
2-6 2s22p53s 3P2-2s22p53p 3S1 0.77 0.4 409.705 408.70 409.903 409.30
8-19 2s22p53p 3D3-2s22p53d 3F4 0.42 0.27 283.942 282.86 284.010 283.97
2-10 2s22p53s 3P2-2s22p53p 3P2 0.47 0.17 323.572 321.97 323.646 323.50
3-9 2s22p53s 1P1-2s22p53p 1P1 0.48 0.16 358.247 356.33 358.320 358.05
7-20 2s22p53p 3D2-2s22p53d 3F3 0.35 0.16 269.420 267.82 269.295 269.44
14-26 2s22p53p 1D2-2s22p53d 1F3 0.37 0.14 280.160 278.64 280.198 280.24
2-7 2s22p53s 3P2-2s22p53p 3D2 0.44 0.18 367.288 365.48 367.377 367.16
3-7 2s22p53s 1P1-2s22p53p 3D2 0.43 0.17 389.111 387.50 389.226 388.93
10-22 2s22p53p 3P2-2s22p53d 3D3 0.29 0.092 280.160 278.32 280.206 280.17
3-10 2s22p53s 1P1-2s22p53p 3P2 0.34 0.14 340.391 338.93 340.483 340.28
4-13 2s22p53s 3P0-2s22p53p 3P1 0.34 0.13 340.122 338.42 340.136 339.97
3-11 2s22p53s 1P1-2s22p53p 3P0 0.27 0.1 295.981 293.43 296.314 295.77
13-25 2s22p53p 3P1-2s22p53d 3D2 0.24 0.14 281.120 279.65 281.104 281.16
12-24 2s22p53p 3D1-2s22p53d 3F2 0.21 0.11 266.417 265.20 266.432 266.45
6-18 2s22p53p 3S1-2s22p53d 3P2 0.20 0.13 254.536 253.32 254.485 254.60
5-12 2s22p53s 3P1-2s22p53p 3D1 0.29 0.11 387.231 385.26 387.357 387.02
9-21 2s22p53p 1P1-2s22p53d 1D2 0.17 0.067 275.550 274.28 275.596 275.60
4-12 2s22p53s 3P0-2s22p53p 3D1 0.22 0.084 373.430 370.93 373.385 373.25
5-13 2s22p53s 3P1-2s22p53p 3P1 0.19 0.074 351.533 350.31 351.692 351.36
10-18 2s22p53p 3P2-2s22p53d 3P2 0.13 0.098 304.971 304.09 304.943 304.91
7-21 2s22p53p 3D2-2s22p53d 1D2 0.10 0.039 259.705 258.29 259.734 259.72
6-16 2s22p53p 3S1-2s22p53d 3P0 $9.6 \times 10^{-2}$ 0.072 269.886 269.62 269.884 269.98
8-22 2s22p53p 3D3-2s22p53d 3D3 $7.8 \times 10^{-2}$ - 262.699 261.29 262.729 262.76
2-13 2s22p53s 3P2-2s22p53p 3P1 $7.2 \times 10^{-2}$ - 252.525 250.31 252.704 252.44
8-20 2s22p53p 3D3-2s22p53d 3F3 $5.8\times 10^{-2}$ - 279.245 277.91 279.096 279.31
33-37 2p63p 1P1-2p63d 1D2 $4.9 \times 10^{-2}$ - 273.347 271.73 - 273.52
9-18 2s22p53p 1P1-2s22p53d 3P2 $3.6 \times 10^{-2}$ - 291.934 291.33 291.928 291.93
7-18 2s22p53p 3D2-2s22p53d 3P2 $3.3 \times 10^{-2}$ - 274.210 273.35 274.190 274.18
6-17 2s22p53p 3S1-2s22p53d 3P1 $2.8 \times 10^{-2}$ - 264.785 263.63 264.306 264.47
14-25 2s22p53p 1D2-2s22p53d 3D2 $3.0\times 10^{-2}$ - 283.543 282.48 283.535 283.56
5-11 2s22p53s 3P1-2s22p53p 3P0 $4.0 \times 10^{-2}$ - 413.911 412.69 414.285 413.52
14-24 2s22p53p 1D2-2s22p53d 3F2 $2.5\times 10^{-2}$ - 288.945 287.69 288.934 288.95
2-9 2s22p53s 3P2-2s22p53p 1P1 $2.8 \times 10^{-2}$ - 339.666 337.62 339.720 339.51
10-25 2s22p53p 3P2-2s22p53d 3D2 $1.6\times 10^{-2}$ - 225.902 223.97 225.999 225.90
3-6 2s22p53s 1P1-2s22p53p 3S1 $2.6\times 10^{-2}$ - 437.048 436.43 437.292 436.55
2-14 2s22p53s 3P2-2s22p53p 1D2 $1.3 \times 10^{-2}$ - 250.601 248.09 250.771 250.54
8-18 2s22p53p 3D3-2s22p53d 3P2 $1.2 \times 10^{-2}$ - 284.394 283.87 284.357 284.40
32-36 2p63p 3P2-2p63d 3D3 $1.1\times 10^{-2}$ - - 291.82 - 291.71
3-14 2s22p53s 1P1-2s22p53p 1D2 $1.0 \times 10^{-2}$ - 260.573 258.05 260.763 260.49
6-21 2s22p53p 3S1-2s22p53d 1D2 $7.3\times 10^{-3}$ - 241.990 240.33 241.984 242.09
31-35 2p63p 3P1-2p63d 3D2 $6.9 \times 10^{-3}$ - - 278.22 - 278.19
7-25 2s22p53p 3D2-2s22p53d 3D2 $5.1\times 10^{-3}$ - 208.571 206.84 208.655 208.58
31-37 2p63p 3P1-2p63d 1D2 $6.1\times 10^{-3}$ - 250.198 248.34 - 250.01
13-24 2s22p53p 3P1-2s22p53d 3F2 $5.1\times 10^{-3}$ - 286.429 284.76 286.410 286.47
28-32 2p63s 3S1-2p63p 3P2 $5.4\times 10^{-3}$ - - 346.41 - 348.84

Notes: For a description of the columns see Table 3. The relative intensities (photons) $Int=N_{j} A_{ji}/N_{\rm e}$were calculated at an electron density of 1011 cm-3. The fourth column provides the relative intensities calculated by Bhatia et al. (1985) as reported in Feldman et al. (1985).

Source LaTeX | All tables | In the text

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