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Table A.4.
Neon 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 | ||||||
| III | 2p–3s | … | … | … | 322.6600 | 322.7045 |
| III | 2p–3s | … | … | … | 323.3300 | … |
| II | 2p–4s | 1.4 | 324.3 | 150 | 324.5690 | 324.57 |
| II | 2p–4s | … | … | … | 325.3920 | … |
| II | 2p–3d | 1.4 | 326.6 | 100 | 326.5170−326.5380 | 326.54 |
| II | 2p–3d | 3.0 | 327.2 | 100 | 327.3510 | 327.355 |
| II | 2p–3d | 4.4 | 328.0 | 100 | 327.6210−328.0990 | 327.626−328.090 |
| VI | 2p–3s | 7.0 | 328.3 | 100 | 164.0340 (II) | 164.027−164.296 (II) |
| IV | 2p–4d | 2.6 | 329.7 | 100 | … | 164.685−164.9085 (II) |
| II | 2p–4d Blended | … | … | 330.6250−330.7890 | 330.626; | 330.790 |
| V | 2p–3s | 2.2 | 330.8 | 100 | … | 165.224−165.527 (II) |
| II | 2p–4d | 2.2 | 331.2 | 100 | 331.0700 | 331.07 |
| II | 2p–4d | 1.5 | 331.7 | 150 | 331.5150 | 331.515 |
| IV | 2p–4s | … | … | … | … | 166.1314−166.1336 (II) |
| V | 2p–3s | 5.6 | 335.3 | 100 | 167.4740−167.9220 (II) | 167.475−167.924 (II) |
| VI | 2s 2p2–2s2 3p | 3.1 | 337.6 | 100 | 168.7650 (II) | … |
| IV | 2p–3d | 10 | 345.0 | 100 | … | 172.4894−172.6137 (II) |
| IV | 2p–3d | 2.4 | 346.3 | 100 | … | 173.2636−173.5343 (II) |
| V | 2p–3s | 2.1 | 347.8 | 100 | 173.9320 (II) | 173.928 (II) |
| Unidentified lines | ||||||
| … | … | 2.6 | 320.5 | 100 | … | … |
| … | … | 1.6 | 321.1 | 150 | … | … |
| … | … | 1.0 | 323.3 | 150 | … | … |
| … | … | 2.6 | 333.0 | 100 | … | … |
| … | … | 2.8 | 333.5 | 100 | … | … |
| … | … | 2.9 | 335.8 | 100 | … | … |
| … | … | 2.0 | 337.3 | 150 | … | … |
| … | … | 1.8 | 339.1 | 100 | … | … |
| … | … | 1.2 | 339.4 | 150 | … | … |
| … | … | 0.7 | 341.1 | 200 | … | … |
| … | … | 0.5 | 341.5 | 200 | … | … |
| … | … | 1.2 | 342.1 | 150 | … | … |
| … | … | 2.9 | 342.6 | 100 | … | … |
| … | … | 1.4 | 343.0 | 150 | … | … |
| … | … | 1.2 | 344.5 | 150 | … | … |
| … | … | 3.5 | 345.4 | 100 | … | … |
| … | … | 1.7 | 347.4 | 150 | … | … |
Notes. The unknown Ne lines may technically belong to spectra up to Ne IX, but are not likely to belong to spectra Ne vi or higher.
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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