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Table 2
Lines contributing to the meteor spectrum in the range of 3800 Å−8700 Å.
λ | Chemical species | Multiplet |
(Å) | ||
|
||
Low-temperature lines | ||
3831 | Mg I | 3 |
3859, 3885, 3926 | Fe I | 4 |
4045, 4066, 4143 | Fe I | 43 |
4201, 4273, 4308, 4326 | Fe I | 42 |
4226 | Ca I | 2 |
4255 | Cr I | 1 |
4384, 4405 | Fe I | 41 |
4703 | Mg I | 11 |
4872, 4891, 4920, 4957, 5008 | Fe I | 318 |
5182 | Mg I | 2 |
5269, 5328, 5371, 5404, 5431, 5449 | Fe I | 15 |
5892 | Na I | 1 |
High-temperature lines | ||
3934, 3969 | Ca II | 1 |
4481 | Mg II | 4 |
6347, 6371 | Si II | 2 |
Wake lines | ||
4376, 4427, 4462, 4482 | Fe I | 2 |
4571 | Mg I | 1 |
5169, 5205 | Fe I | 1 |
Atmospheric lines and bands | ||
5330 | OI | 12 |
5700−6000 | N2 1st. positive | Δν = 4 |
6200−6800 | N2 1st. positive | Δν = 3 |
7000−7500 | N2 1st. positive | Δν = 2 |
6157 | O I | 10 |
6455 | O I | 9 |
6484 | N I | 21 |
7424, 7442, 7468 | N I | 3 |
7774 | O I | 1 |
8186, 8218, 8143 | N I | 2 |
8446 | O I | 4 |
8682 | N I | 1 |
Train lines | ||
5577 | [O I] | 3F |
Notes. The lines are only given individually within the multiplet when they are well enough separated to be resolved in the video spectra. The multiplet numbers are given according to Moore (1945).
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