Email this article Spatial and temporal variations in infrared emissions of the upper atmosphere. 1. Atomic oxygen (λ 63 μm) emission
- Authors: Semenov A.I.1, Medvedeva I.V.2, Perminov V.I.1, Khomich V.Y.3
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Affiliations:
- Obukhov Institute of Atmospheric Physics
- Institute of Solar–Terrestrial Physics, Siberian Division
- Institute of Electrophysics and Electroenergetics
- Issue: Vol 56, No 5 (2016)
- Pages: 616-620
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/155786
- DOI: https://doi.org/10.1134/S0016793216050121
- ID: 155786
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Abstract
Rocket and balloon measurement data on atomic-oxygen (λ 63 µm) emission in the upper atmosphere are presented. The data from the longest (1989–2003) period of measurements of the atomic-oxygen (λ 63 µm) emission intensity obtained by spectral instruments on sounding balloons at an altitude of 38 km at midlatitudes have been systematized and analyzed. Regularities in diurnal and seasonal variations in the intensity of this emission, as well as in its relation with solar activity, have been revealed.
About the authors
A. I. Semenov
Obukhov Institute of Atmospheric Physics
Author for correspondence.
Email: anasemenov@yandex.ru
Russian Federation, Moscow, 119017
I. V. Medvedeva
Institute of Solar–Terrestrial Physics, Siberian Division
Email: anasemenov@yandex.ru
Russian Federation, Irkutsk, 664033
V. I. Perminov
Obukhov Institute of Atmospheric Physics
Email: anasemenov@yandex.ru
Russian Federation, Moscow, 119017
V. Yu. Khomich
Institute of Electrophysics and Electroenergetics
Email: anasemenov@yandex.ru
Russian Federation, St. Petersburg, 191186
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