Table 3
List of the strongest Ni xi lines.
i–j | Levels | I | I | gf | Aji(s-1) | Aji(s-1) | λexp(Å) | λth(Å) | |
|
|||||||||
CHIANTI | BL11 | ||||||||
|
|||||||||
1–13 | 3s23p6 1S0–3s23p53d 1P1 | 1.0 | 1.0 | 2.72 | 2.7 × 1011 | 2.8 × 1011 | 148.377 | 144.66 (–3.7) | |
5–95 | 3s23p53d 3F4–3s23p43d2 3G5 | 5.1 × 10-2 | 4.7 × 10-2 | 5.12 | 1.2 × 1011 | 1.3 × 1011 | – | 152.54 | |
5–106 | 3s23p53d 3F4–3s23p43d2 3D3 | 3.8 × 10-2 | 3.7 × 10-2 | 5.05 | 2.0 × 1011 | 2.3 × 1011 | – | 143.87 | |
5–114 | 3s23p53d 3F4–3s23p43d2 3F4 | 3.5 × 10-2 | 3.3 × 10-2 | 5.92 | 2.0 × 1011 | 2.2 × 1011 | – | 137.72 | |
6–93 | 3s23p53d 3F3–3s23p43d2 3G4 | 3.2 × 10-2 | 2.9 × 10-2 | 3.85 | 1.1 × 1011 | 1.2 × 1011 | – | 153.95 | |
6–107 | 3s23p53d 3F3–3s23p43d2 3D2 | 1.9 × 10-2 | 1.7 × 10-2 | 3.30 | 1.9 × 1011 | 2.1 × 1011 | – | 144.40 | |
1–4 | 3s23p6 1S0–3s23p53d 3P2 | 0.19 | 0.12 | – | 1.4 × 102 | 1.4 × 102 | 207.922 | 205.01 (–2.9) | |
1–3 | 3s23p6 1S0–3s23p53d 3P1 | 9.1 × 10-2 | 5.0 × 10-2 | 3.8 × 10-4 | 1.9 × 107 | 2.3 × 107 | 211.430 | 208.58 (–2.8) | |
1–10 | 3s23p6 1S0–3s23p53d 3D1 | 4.4 × 10-2 | 2.3 × 10-2 | 8.2 × 10-3 | 5.1 × 108 | 5.7 × 108 | 186.975 | 183.60 (–3.4) | (bl) |
1–7 | 3s23p6 1S0–3s23p53d 3F2 | 2.2 × 10-2 | 1.3 × 10-2 | – | 5.9 | 5.6 | 198.42 | 195.01 (–3.4) | R (bl) |
1–9 | 3s23p6 1S0–3s23p53d 1D2 | 1.6 × 10-2 | 9.6 × 10-3 | – | 49. | 51 | 188.435 | 184.87 (–3.6) | R |
5–16 | 3s23p53d 3F4–3s3p63d 3D3 | 1.3 × 10-2 | 2.0 × 10-2 | 0.38 | 4.2 × 109 | 4.4 × 109 | 288.41 | 276.51 | TN (bl) |
1–139 | 3s23p6 1S0–3s23p54s 1P1 | 2.3 × 10-2 | 4.9 × 10-3 | 0.20 | 7.1 × 1010 | 7.3 × 1010 | 77.393 | 74.41 (–3.0) | |
1–133 | 3s23p6 1S0–3s23p54s 3P1 | 1.4 × 10-2 | 4.1 × 10-3 | 0.13 | 4.6 × 1010 | 5.0 × 1010 | 78.744 | 75.63 (–3.1) | (bl) |
13–440 | 3s23p53d 1P1–3s3p64s 1S0 | 1.1 × 10-2 | 5.6 × 10-3 | 2.5 × 10-2 | 1.5 × 1010 | 7.9 × 109 | 104.67 | 100.25 | TN |
5–540 | 3s23p53d 3F4–3s23p54f 3G5 | 6.7 × 10-3 | 5.5 × 10-3 | 5.66 | 4.8 × 1011 | 4.6 × 1011 | 82.416 | 78.96 (–3.5) | |
13–599 | 3s23p53d 1P1–3s23p54f 1D2 | 5.5 × 10-3 | 2.8 × 10-3 | 1.93 | 3.4 × 1011 | 2.0 × 1011 | 93.849 | 89.49 (–4.4) | |
1–357 | 3s23p6 1S0–3s23p54d 1P1 | 4.0 × 10-3 | 3.7 × 10-4 | 0.58 | 3.1 × 1011 | 7.7 × 1010 | 62.730 | 61.40 (–1.3) | ? |
6–545 | 3s23p53d 3F3–3s23p54f 3G4 | 3.8 × 10-3 | 2.9 × 10-3 | 3.89 | 4.1 × 1011 | 3.8 × 1011 | 82.530 | 79.04 (–3.5) | |
5–187 | 3s23p53d 3F4–3s23p54p 3D3 | 3.5 × 10-3 | 2.9 × 10-3 | 0.30 | 2.2 × 1010 | 2.2 × 1010 | – | 106.60 | |
10–577 | 3s23p53d 3D1–3s23p54f 3F2 | 2.5 × 10-3 | 2.5 × 10-3 | 1.51 | 2.7 × 1011 | 2.3 × 1011 | – | 80.43 | |
6–186 | 3s23p53d 3F3–3s23p54p 3D2 | 2.4 × 10-3 | 2.2 × 10-3 | 0.17 | 1.8 × 1010 | 1.8 × 1010 | – | 107.49 | |
10–599 | 3s23p53d 3D1–3s23p54f 1D2 | 1.9 × 10-3 | 1.3 × 10-3 | 0.52 | 1.1 × 1011 | 9.2 × 1010 | 83.010 | 79.11 (–3.9) | |
5–12 | 3s23p53d 3F4–3s23p53d 1F3 | 6.7 × 10-2 | 4.4 × 10-2 | – | 2.7 × 102 | 2.8 × 102 | 2001.20 | 1959.12 (–42) | |
4–8 | 3s23p53d 3P2–3s23p53d 3D3 | 5.5 × 10-2 | 3.8 × 10-2 | – | 34 | 37 | 2157.08 | 2021.38 (–136) | R |
4–11 | 3s23p53d 3P2–3s23p53d 3D2 | 4.2 × 10-2 | 2.6 × 10-2 | – | 1.7 × 102 | 1.9 × 102 | 1717.33 | 1627.83 (–89.5) | |
6–8 | 3s23p53d 3F3–3s23p53d 3D3 | 3.1 × 10-2 | 2.1 × 10-2 | – | 19 | 21 | 3339.46 | 3218.54 (–121) | R |
6–9 | 3s23p53d 3F3–3s23p53d 1D2 | 2.9 × 10-2 | 1.8 × 10-2 | – | 86 | 95 | 3000.93 | 2878.03 (–123) | R |
7–9 | 3s23p53d 3F2–3s23p53d 1D2 | 1.8 × 10-2 | 1.1 × 10-2 | – | 54 | 59 | 3743.07 | 3553.69 (–189) | R |
Notes. The first column lists the indices of the levels, as from Table 2. The second the spectroscopic notation. Columns 3 and 4 show the intensities (photons) of the strongest lines, relative to the resonance transition, calculated at log Ne [cm-3] = 9 and log Te [K] = 6.1, using the present and the CHIANTI ion models. The CHIANTI model uses the Aggarwal & Keenan (2007) collision strengths for the first 17 levels and for the rest those of Bhatia & Landi (2011). Column 5 lists the weighted oscillator strength gf and Col. 6 the A-values from our calculation. Column 7 lists the Bhatia & Landi (2011) A-values as given in the CHIANTI v.7.1 database. TN is a tentative new identification, R a revised wavelength (compared to NIST), bl a blend. All wavelengths are in vacuum.
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