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Table A.7.
Nickel lines observed in EBIT-I within the wavelength band λ320–λ350.
| Spectrum | Transition type | Line intensity | λ(Å) This work | Unc. (mÅ) | λ(Å) CHIANTIa | λ(Å) NISTb |
|---|---|---|---|---|---|---|
| Known lines | ||||||
| X | 3p–3d | Blended | <320.0 | … | … | 159.977 (II) |
| XVIII | 3s–3p | 9.5 | 320.4 | 100 | 320.5580 | 320.558 |
| XVI | 3s–3p | 4.5 | 321.1 | 100 | 321.0370 | … |
| XII | 3p–3d | Blended | 321.1 | 100 | 160.5550 (II) | 160.556 (II) |
| XIII | 3s–3p | 0.9 | 321.90 | 50 | 321.8820 | 321.881 |
| XVII | 3s–3p | … | … | … | 322.0203 | … |
| XIII | 3p–3d | Blended | 323.1 | … | 161.5600 (II) | 161.547 (II) |
| XIII | 3p–3d | Blended | 323.5 | … | 161.7830 (II) | 161.752 (II) |
| XV | 3s–3p | 1.0 | 324.4 | 100 | 324.3540 | 324.354 |
| XV | 3s–3p | Blended | … | … | 324.6510 | 324.651 |
| XIV | 3s–3p | … | … | … | 325.7427 | … |
| XIV | 3s–3p | 0.3 | 325.9 | 200 | … | 325.957 |
| XIII | 3p–3d | 10 | 328.2 | 100 | 164.1460 (II) | 164.172 (II) |
| XXII | 3s–3p | 1.4 | 330.7 | 100 | 330.5290 | 330.58 |
| XIV | 3p–3d | 0.7 | 332.5 | 150 | 166.2799 (II) | … |
| XIV | 3s–3p | … | … | … | 334.4093 | 334.519 |
| XIV | 3p–3d | 1.5 | 336.7 | 100 | 168.1203 (II) | 168.12 (II) |
| XIV | 3p–3d | Blended | … | … | 168.3703 (II) | 168.37 (II) |
| XIV | 3s–3p | … | … | … | … | 338.655 |
| XIII | 3p–3d | 2.5 | 339.2 | 100 | 169.5900 (II) | 169.59 (II) |
| XIV | 3p–3d | 2.2 | 339.5 | 100 | 169.6903 (II) | 169.69 (II) |
| XIV | 3p–3d | 2.2 | 339.5 | 100 | 169.6903 (II) | 169.69 (II) |
| XIV | 3p–3d | Blended | Blended | Blended | 169.8742 (II) | … |
| XIV | 3p–3d | 1.0 | 341.1 | 100 | 170.5003 (II) | 170.50 (II) |
| XIV | 3p–3d | 2.9 | 342.7 | 100 | 171.3703 (II) | 171.37 (II) |
| XIV | 3p–3d | 1.4 | 344.3 | 100 | 172.1603 | 172.16 (II) |
| XV | 3p–3d | 1.9 | 347.3 | 100 | 173.7240 | 173.724 (II) |
| XIV | 3p–3d | 1.8 | 347.7 | 100 | … | 173.737 (II) |
| Unidentified lines | ||||||
| XI | … | 9.5 | 320.4 | 100 | … | … |
| XI | … | 7.3 | 320.7 | 100 | … | … |
| XI | … | 1.5 | 323.1 | 100 | … | … |
| XI | … | 0.9 | 327.6 | 100 | … | … |
| XVIII | … | 5.0 | 328.5 | 100 | … | … |
| XI | … | 0.3 | 329.4 | 200 | … | … |
| XI | … | 0.5 | 331.0 | 100 | … | … |
| XI | … | 0.3 | 331.6 | 200 | … | … |
| XI | … | 0.8 | 333.7 | 100 | … | … |
| XI | … | 1.6 | 336.3 | 100 | … | … |
| XI | … | 0.5 | 337.9 | 150 | … | … |
| XI | … | 2.2 | 343.0 | 100 | … | … |
| XIX | … | 0.7 | 345.9 | 100 | … | … |
| XVIII | … | 0.7 | 346.3 | 100 | … | … |
| XVIII | … | 2.1 | 347.3 | 100 | … | … |
| XVIII | … | 0.1 | 348.3 | 200 | … | … |
| XVIII | … | 0.4 | 349.4 | 150 | … | … |
Notes. The unknown Ni lines can technically originate in spectra up to Ni XI.
References.
(a)
From the CHIANTI database v.8 (Del Zanna et al. 2015);
(b)
from the online database at NIST (Kramida et al. 2015).
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