Table 3
A selection of the strongest Ni xii lines.
i–j | Levels | Int | gf | Aji (s-1) | λexp (Å) | λth (Å) | ||||
|
||||||||||
1–29 | 3s2 3p52P3/2–3s2 3p4 3d 2D5/2 | 1.0 | 4.35 | 2.1×1011 | 152.151 | 152.32 | ||||
1–28 | 3s2 3p52P3/2–3s2 3p4 3d 2P3/2 | 0.58 (0.49) | 2.50 | 1.8×1011 | 154.171 | 154.14 | ||||
1–27 | 3s2 3p52P3/2–3s2 3p4 3d 2S1/2 | 0.25 (0.21) | 1.17 | 1.5×1011 | 160.556 | 160.54 | ||||
1–5 | 3s2 3p52P3/2–3s2 3p4 3d 4D7/2 | 0.20 (0.06) | – | 91. | 220.247 | 221.87 | T | |||
1–3 | 3s2 3p52P3/2–3s 3p62S1/2 | 0.14 (0.09) | 0.13 | 5.1×109 | 295.321 | 295.10 | ||||
1–4 | 3s2 3p52P3/2–3s2 3p4 3d 4D5/2 | 6.6 (2.4)×10-2 | 3.7×10-4 | 8.3×106 | 220.870 | 222.40 | T | |||
2–27 | 3s2 3p52P1/2–3s2 3p4 3d 2S1/2 | 6.2 (6.0)×10-2 | 0.31 | 3.7×1010 | 166.887 | 167.09 | ||||
2–30 | 3s2 3p52P1/2–3s2 3p4 3d 2P1/2 | 5.6 (8.2)×10-2 | 1.00 | 1.3×1011 | 157.796 | 157.65 | ||||
1–19 | 3s2 3p52P3/2–3s2 3p4 3d 2D5/2 | 4.8 (1.3)×10-2 | 6.1×10-3 | 1.8×108 | – | 194.73 | ||||
1–17 | 3s2 3p52P3/2–3s2 3p4 3d 4P5/2 | 4.3 (0.6)×10-2 | 4.6×10-3 | 1.3×108 | – | 196.56 | ||||
1–22 | 3s2 3p52P3/2–3s2 3p4 3d 2F5/2 | 3.9 (0.7)×10-2 | 9.5×10-4 | 3.0×107 | – | 189.02 | ||||
2–31 | 3s2 3p52P1/2–3s2 3p4 3d 2D3/2 | 4.0 (13)×10-2 | 2.79 | 2.0×1011 | 152.697 | 152.92 | T | |||
2–3 | 3s2 3p52P1/2–3s 3p62S1/2 | 6.1 (4.0)×10-2 | 6.5×10-2 | 2.2×109 | 317.474 | 318.04 | ||||
1–2 | 3s2 3p52P3/2–3s2 3p52P1/2 | 0.57 (0.65) | – | 2.6×102 | 4232.09 | 4091.00 | ||||
5–9 | 3s2 3p4 3d 4D7/2–3s2 3p4 3d 4F9/2 | 9.4 (3.4)×10-2 | – | 28. | 3171.18 | 3014.08 | ||||
9–21 | 3s2 3p4 3d 4F9/2–3s2 3p4 3d 2G9/2 | 3.8 (1.4)×10-2 | – | 2.0×102 | 2398.08 | 2258.57 | ||||
5–18 | 3s2 3p4 3d 4D7/2–3s2 3p4 3d 2F7/2 | 2.5 (0.47)×10-2 | – | 90. | 1686.74 | 1661.20 | ||||
5–10 | 3s2 3p4 3d 4D7/2–3s2 3p4 3d 4F7/2 | 1.9 (0.66)×10-2 | – | 18. | 2580.38 | 2492.77 | ||||
9–18 | 3s2 3p4 3d 4F9/2–3s2 3p4 3d 2F7/2 | 1.8 (0.30)×10-2 | – | 57. | 3603.34 | 3701.00 | ||||
10–20 | 3s2 3p4 3d 4F7/2–3s2 3p4 3d 2G7/2 | 1.3 (0.28)×10-2 | – | 84. | 2923.12 | 2783.65 | ||||
9–24 | 3s2 3p4 3d 4F9/2–3s2 3p4 3d 2F7/2 | 1.1 (0.37)×10-2 | – | 2.3×102 | 1225.05 | 1235.02 | ||||
3–462 | 3s 3p62S1/2–3s 3p5 4s 2P3/2 | 1.9×10-2 | 0.25 | 8.0×1010 | – | 72.52 | ||||
1–282 | 3s2 3p52P3/2–3s2 3p4 4s 2D5/2 | 1.2×10-2 | 0.30 | 6.7×1010 | 71.378 | 71.39 | ||||
1–262 | 3s2 3p52P3/2–3s2 3p4 4s 2P3/2 | 1.1×10-2 | 0.45 | 1.4×1011 | 72.770 | 72.87 | ||||
1–435 | 3s2 3p52P3/2–3s2 3p4 4d 2D5/2 | 5.8×10-3 | 1.00 | 3.1×1011 | 60.020 | 60.07 | ||||
1–246 | 3s2 3p52P3/2–3s2 3p4 4s 4P3/2 | 4.5×10-3 | 0.10 | 3.0×1010 | – | 73.93 | ||||
1–242 | 3s2 3p52P3/2–3s2 3p4 4s 4P5/2 | 3.7×10-3 | 1.5×10-2 | 2.9×109 | – | 74.60 | ||||
22–526 | 3s2 3p4 3d 2F5/2–3s2 3p4 4f 2G7/2 | 3.1×10-3 | 2.33 | 3.3×1011 | – | 76.38 | ||||
2–283 | 3s2 3p52P1/2–3s2 3p4 4s 2D3/2 | 2.4×10-3 | 0.27 | 8.6×1010 | 72.570 | 72.57 | ||||
2–273 | 3s2 3p52P1/2–3s2 3p4 4s 2P1/2 | 2.4×10-3 | 0.17 | 1.0×1011 | 73.423 | 73.45 | ||||
9–483 | 3s2 3p4 3d 4F9/2–3s2 3p4 4f 4G11/2 | 2.3×10-3 | 6.47 | 6.3×1011 | 75.618 | 75.73 | ||||
1–273 | 3s2 3p52P3/2–3s2 3p4 4s 2P1/2 | 2.1×10-3 | 0.15 | 9.3×1010 | 72.171 | 72.15 | ||||
14–498 | 3s2 3p4 3d 4F5/2–3s2 3p4 4f 4G7/2 | 2.1×10-3 | 2.33 | 3.4×1011 | – | 75.78 | ||||
5–477 | 3s2 3p4 3d 4D7/2–3s2 3p4 4f 4F9/2 | 1.9×10-3 | 4.44 | 5.4×1011 | 74.440 | 74.35 |
Notes. Column 3 shows the relative intensities (photons) I = NjAji/Ne of the strongest lines, relative to the main transition. The intensities were calculated at an electron density of 109 cm-3 and log T [K] = 6.25, the temperature of peak ion abundance in equilibrium. Values in brackets are those calculated with the CHIANTI database. Columns 4 and 5 show the gf and A values calculated in this work with TECs. The λexp (Å) are our experimental wavelengths (in vacuum), while the λth (Å) values are our theoretical values obtained with the TECs. A “T” in the last column indicates a tentative new experimental wavelength.
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