| Автор | Slanger, T. G. |
| Автор | Huestis, D. L. |
| Дата выпуска | 1981 |
| dc.description | Synthetic spectra have been calculated incorporating three O<sub>2</sub> emission systems, A³Σ<sub>u</sub><sup>+</sup> → X³Σ<sub>g</sub><sup>−</sup>, A′³Δ<sub>u</sub> → a¹Δ<sub>g</sub>, and c¹Σ<sub>u</sub><sup>−</sup> → X³Σ<sub>g</sub><sup>−</sup>, and matched to the 3100‐ to 4500‐Å nightglow spectrum of Broadfoot and Kendall (1968). The synthesis necessitated the inclusion of the c¹Σ<sub>u</sub><sup>−</sup> → X³Σ<sub>g</sub><sup>−</sup> system, which has never been previously identified in the airglow, although it is a dominant system in the Venusian nightglow. The emissions from the extremely metastable A′³Δ<sub>u</sub> and c¹Σ<sub>u</sub><sup>−</sup> states account for half the radiation in the 3100‐ to 4500‐Å region, from which it may be deduced that the mesospheric concentrations of O<sub>2</sub>(A′³Δ<sub>u</sub>) and O<sub>2</sub>(c¹Σ<sub>u</sub><sup>−</sup>) are much higher than that of O<sub>2</sub>(A³Σ<sub>u</sub><sup>+</sup>). The vibrational distributions are quite unrelaxed for all three states. |
| Формат | application.pdf |
| Копирайт | Copyright © 1981 by the American Geophysical Union. |
| Тема | IONOSPHERE |
| Тема | Particles and Fields—Ionosphere: Airglow |
| Тема | PLANETARY SCIENCES: SOLID SURFACE PLANETS |
| Тема | Planetology: Atmospheres of planets |
| Название | O<sub>2</sub> (c¹Σ<sub> u </sub> <sup>−</sup> → X³Σ<sub> g </sub> <sup>−</sup>) emission in the terrestrial nightglow |
| Тип | article |
| DOI | 10.1029/JA086iA05p03551 |
| Electronic ISSN | 2156-2202 |
| Print ISSN | 0148-0227 |
| Журнал | Journal of Geophysical Research: Space Physics |
| Том | 86 |
| Первая страница | 3551 |
| Последняя страница | 3554 |
| Выпуск | A5 |
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