Infrared Glow of Nitric Oxide in Earth’s Middle Atmosphere during GLE Events of the 23rd Solar Cycle

A. S. Kirillov; Кириллов А. С.; V. B. Belakhovsky; Белаховский В. Б.; E. A. Maurchev; Маурчев Е. А.; Yu. V. Balabin; Балабин Ю. В.; A. V. Germanenko; Германенко А. В.; B. B. Gvozdevsky; Гвоздевский Б. Б.

doi:10.31857/S0016794023600643

Infrared Glow of Nitric Oxide in Earth’s Middle Atmosphere during GLE Events of the 23rd Solar Cycle

作者: Kirillov A.S.¹, Belakhovsky V.B.¹, Maurchev E.A.¹^,2, Balabin Y.V.¹, Germanenko A.V.¹, Gvozdevsky B.B.¹
隶属关系:
1. Polar Geophysical Institute
2. Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
期: 卷 63, 编号 6 (2023)
页面: 822-831
栏目: Articles
URL: https://bakhtiniada.ru/0016-7940/article/view/232924
DOI: https://doi.org/10.31857/S0016794023600643
EDN: https://elibrary.ru/PTBOZU
ID: 232924

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详细

The article considers the production kinetics of vibrationally excited NO(X2Π, > 0) molecules at heights of Earth’s middle atmosphere during the precipitation of high-energy protons. The intensity profiles of the luminescence of the infrared bands of nitric oxide at 5.3 and 2.7 μm were calculated for precipitation of high-energy protons into Earth’s atmosphere during the events GLE65, GLE67, GLE69, and GLE70 of the 23rd solar cycle. Calculations have shown that the highest integral luminescence intensity values of the 5.3 and 2.7 μm bands were obtained for GLE69: 5.7 and 0.18 kR (kilorayleighs), respectively. Comparison of the calculation results for the 5.3 µm band during the GLE69 event with experimental data obtained from the TIMED spacecraft on January 20, 2005, showed that the calculation results were overestimated by a factor of 2.

参考

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